Science.gov

Sample records for bibliothque scientifique nationale

  1. Nationale Roadmap Embedded Systems

    NASA Astrophysics Data System (ADS)

    Damm, Werner; Achatz, Reinhold; Beetz, Klaus; Broy, Manfred; Daembkes, Heinrich; Grimm, Klaus; Liggesmeyer, Peter

    Eingebettete Systeme" sind in ihrem Softwareanteil nicht sichtbar und doch hoch relevant für den Wirtschaftsstandort Deutschland. Ihre Bedeutung fasst die vorliegende Nationale Roadmap Embedded Systems in den folgenden 10 Thesen zusammen: These 1 Die zentralen ökonomischen und gesellschaftlichen Herausforderungen in Deutschland lassen sich ohne die Querschnittstechnologie Embedded Systems nicht lösen1.

  2. Café Scientifique.

    PubMed

    Grand, Ann

    2014-01-01

    Every month, in 700 or so bars, cafés, pubs, teahouses, shopping centres, community halls, art galleries, libraries, theatres, museums, bookshops ... and a blood donation centre, 40 or so people meet to have a conversation. A conversation that happens to be about science and technology, rather than soap operas or football; this is Café Scientifique. PMID:25549411

  3. A Cafe Scientifique for Teens

    NASA Astrophysics Data System (ADS)

    Hall, M.; Mayhew, M.

    2008-12-01

    It is well-known to those pursuing the quest to connect scientists to the public that an exceedingly hard-to- reach demographic is people of high school age. Typically, kids may tag along with their parents to museums until they reach adolescence, and then don't again appear in museums until they themselves have children. We have addressed this demographic challenge for free-choice-learning by developing a Cafe Scientifique program specifically for high school students. The Cafe Scientifique model for adults was developed in England and France, and has now spread like wildfire across the U.S. Typically, people come to a informal setting like a cafe, socialize and have food and drink, and then hear a short presentation by a scientist on a hot science topic in the news. This is followed by a period of lively discussion. We have followed this model for high school age students in four towns in northern New Mexico--Los Alamos, Santa Fe, Espanola, and Albuquerque--which represent a highly diverse demographic. We started this novel project with some trepidation, i.e. what if we build it and they don't come. But the program has proven popular beyond our expectations in all four towns. A part of the secret of success is the social setting, and-especially for this age group-the food provided. But we have also found that the kids are genuinely interested in the science topics, directing their own program, and interacting with scientists. We have often heard statements like, "I think it is important to be well-informed citizens". One of the most important aspects of the Cafes for the kids is to be able to discuss and argue about issues related to the science topic with the presenter and each other. It is an important part of the popularity that the Cafes do not involve school or parents, but also that we have strived to give the kids ownership of the program. Each town has a Youth Leadership Team-open to any teen-that discusses and prioritizes potential topics, conducts

  4. La Section 17 du Comité National de la Recherche Scientifique

    NASA Astrophysics Data System (ADS)

    Marcelin, M.

    2015-12-01

    This contribution presents the section 17 of the ``Comité National de la Recherche Scientifique" and its activity. Since it concerns mostly French researchers and researchers from French institutes, the rest of the contribution is provided in French language.

  5. The game of science: A grounded theory of the Cafe Scientifique experience

    NASA Astrophysics Data System (ADS)

    Rabe, Lisa A.

    Science Cafes are independent groups organized throughout the world for discussion of scientific topics. Little is known about the nature of this informal learning environment. A grounded-theory study was conducted to determine what attendees perceived as the essential qualities of the Cafe Scientifique experience in one science Cafe in the Western United States. Interviews with 12 attendees were transcribed and analyzed using ATLAS-ti. Concept maps and a grounded theory describing the essential characteristics were created. Member checking was used during theory generation. Findings are described in the context of a game metaphor, whereby scientific discussion at the Cafe is viewed as an intellectual game. The grounded theory describes the game of science being played at Cafe Scientifique involving attendees as players, social norms as rules for the game, an expert as the steward of truth, topics as the content for game play, interaction as playing of the game, and intellectual stimulation as the prize for playing. During the game, ideas were identified through a short presentation followed by a question-and-answer session. During this exchange, attendees heard about, analyzed, synthesized, and applied new information. As a result of the game play, players won a prize---intellectual stimulation. The Cafe Scientifique phenomenon provides insight into informal adult education. This study suggests the need for additional study of intellectual play in adult education, the role of curiosity and desire to explore new ways of thinking, and the developmental drive in adults to seek intellectual stimulation. The essential characteristics of Cafe Scientifique may be transferable to other informal adult-education settings.

  6. Engaging High School Students and Scientists in a Café Scientifique Program

    NASA Astrophysics Data System (ADS)

    Mayhew, M. A.; Hall, M. K.; Foutz, S.

    2010-12-01

    We have created an informal science program that engages high school age youth in exploring science relevant to their lives with researchers working at the cutting edge of science. The program provides scientists a challenging new audience to share their research and enthusiasm for science and science careers. It gives the youth an opportunity to discover how the often-mundane science they are learning in school is used to push the frontiers in science, with exciting applications in the real world. Our program, a youth-led Café Scientifique (cafenm.org), now in its fourth year, has been successful in attracting and retaining youth as well as attracting scientist-presenters. Modeled after the international Café Scientifique program for adults, we combine a social atmosphere with discussion of controversial or current topics to challenge youth to think about how science affects their lives. We feature short presentations with a high degree of interactivity and discussion during which the scientist expert communicates a single important idea or scientific principle. A good speaker will leave the audience with a dilemma or controversy to discuss, and with further opportunities to learn. Encouraging the presenters to interact frequently with the audience allows them to gauge the audience's engagement and knowledge. Alternatively we also host Cafés that offer more hands-on learning experiences, including extracting DNA from plants, building model fuel cell cars, using Google Earth to spy, and deciphering age, gender, ethnicity, and cause of death from human skeletons. Controversial topics are often presented within a scientific, economic, and social or political framework, because science is only part of the solution. A key element of success is in preparing the presenters for the youth audience. Presenters submit their presentation to the program directors for initial review and receive feedback on length, mechanisms for involving the audience, and clarifying or

  7. Effets potentiels d’un modèle rationnel de prescription sur les dépenses nationales en santé

    PubMed Central

    Littman, Jordan; Halil, Roland

    2016-01-01

    Résumé Objectif Estimer les économies que pourrait engendrer la mise en œuvre d’un modèle rationnel de prescription pour des classes de médicaments équivalents sur les plans de l’efficacité, de la toxicité et de la commodité. Conception L’Institut canadien d’information sur la santé a fourni des renseignements sur les 10 principales classes de médicaments en fonction des dépenses annuelles qui leur sont attribuables. Ces classes ont été examinées en vue de leur inclusion potentielle dans l’étude selon qu’il était possible de comparer les médicaments à l’intérieur d’une même classe. Lorsqu’à la suite d’une recherche documentaire, une équivalence a été établie en fonction de l’efficacité, de la toxicité et de la commodité des médicaments, les données annuelles sur les prescriptions ont été recueillies à partir de la base de données du Système national d’information sur l’utilisation des médicaments prescrits. Les économies potentielles de coûts ont ensuite été calculées en comparant les parts de marché actuelles avec les parts potentielles futures de ce marché. Contexte Le Canada. Principaux paramètres à l’étude Les différences estimées dans les dépenses que produirait un modèle rationnel de prescription. Résultats Une équivalence a été établie sur les plans de l’efficacité, de la toxicité et de la commodité dans les classes de statines, d’inhibiteurs de la pompe à protons, d’inhibiteurs de l’enzyme de conversion de l’angiotensine et d’inhibiteurs sélectifs du recaptage de l’angiotensine. Les dépenses annuelles totales dans ces classes se situent à 856 millions $ dans les programmes publics de médicaments et à 1,97 milliard $ environ à l’échelle nationale. Grâce à des prescriptions rationnelles, on estime que les économies annuelles pourraient atteindre 222 millions $ pour les programmes publics et 521 millions $ à l’échelle nationale. Conclusion La

  8. NATO granulite conference

    NASA Astrophysics Data System (ADS)

    Vielzeuf, D.; Vidal, Ph.

    On September 5-9, 1988, 83 participants from 20 different countries gathered in Clermont- Ferrand, France, for the workshop Petrology and Geochemistry of Granulites a nd Related Rocks. All geoscience disciplines were represented. The workshop was cosponsored by Universite Blaise Pascal, UFR Scientifique et Technique, Centre National de la Recherche Scientifique, International Lithosphere Program (working Group 2c), IGCP Project 235, Societe Francaise d e Mineralogie, Ministere de l'Education Nationale (DAGIC), Ministere des Affaires Etrangeres (DGSTD), Conseil Regional d Auvergne , Conseil General du Puy de Dome, Mairie de Clermont-Ferrand.

  9. Analyse de la prise en charge du nouveau-né dans le cadre de la stratégie nationale de subvention des accouchements et des soins obstétricaux et néonatals d'urgence au Centre Hospitalier Universitaire Pédiatrique Charles de Gaulle, Ouagadougou (Burkina Faso)

    PubMed Central

    Ouédraogo, Solange Odile Yugbaré; Yougbaré, Nestor; Kouéta, Fla; Dao; Ouédraogo, Moussa; Lougué, Claudine; Ludovic, Kam; Traoré, Ramata Ouédraogo; Yé, Diarra

    2015-01-01

    Introduction Il s'agit d'analyser la prise en charge du nouveau-né dans le cadre de la stratégie na-tionale de subvention des accouchements et des soins obstétricaux et néonatals d'urgence mis en place par le gouvernement du Burkina Faso en 2006. Méthodes Nous avons menée une étude à visée descriptive et analytique comportant un volet ré-trospectif du 01 janvier 2006 au 31 décembre 2010 portant sur les paramètres épidémiologiques, cliniques des nouveau-nés hospitalisés et un volet prospectif du 3 octobre 2011 au 29 février 2012 par une entrevue des accompagnateurs des nouveau-nés et des prestataires des services de santé. Résultats Les hospitalisations ont augmenté de 43,65% entre 2006 à 2010 Le taux de mortalité néo-natale hospitalière qui était de 11,04% a connu une réduction moyenne annuelle de 3,95%. L'entrevue a porté sur 110 accompagnateurs et 76 prestataires. La majorité des prestataires (97,44%) et des ac-compagnateurs (88,18%) étaient informés de la stratégie mais n'avait pas une connaissance exacte de sa définition. Les prestataires (94,74%) ont signalé des ruptures de médicaments, consommables médicaux et des pannes d’ appareils de laboratoire et d'imagerie. Parmi les accompagnateurs (89%) disaient être satisfaits des services offerts et (72,89%) trouvaient les coûts abordables mais évoquaient les difficultés du transport. Conclusion: La subvention a amélioré la prise en charge du nou-veau-né mais son optimisation nécessiterait une meilleur information et implication de tous les acteurs. Conclusion La subvention a amélioré la prise en charge du nouveau-né mais son optimisation nécessiterait une meilleur information et implication de tous les acteurs. PMID:26161166

  10. Etude RICH Nursing. Plus de connaissances et de preuves scientifiques

    PubMed Central

    SCHUBERT, MARIA

    2009-01-01

    L’importance et la validité des résultats de l’étude RICH-Nursing* ont été récemment mises en cause par certains milieux, ce qui a provoqué certaines incertitudes chez les infirmières. Les auteurs reviennent sur l’impact actuel de cette étude et évoquent les perspectives d’avenir. PMID:25221376

  11. Une approche des textes scientifiques: le "par-coeur" (An Approach to Scientific Texts: "By Heart").

    ERIC Educational Resources Information Center

    Descamps, Jean-Luc

    1980-01-01

    A method is provided for teaching reading comprehension of scientific or technical texts in a foreign language. The method involves analyzing language patterns and using some memorization for terminology. (MSE)

  12. L'appropriation du domaine scientifique chez l'eleve togolais

    NASA Astrophysics Data System (ADS)

    Lalancette, Lucie

    1998-12-01

    Science and technology are essential to sustainable development. They must be endogenous in nature to reduce the dependency and vulnerability of developing countries. Hence we seek to determine how Togolese students appropriate the field of science. Science education should answer fundamental educational needs by aiming for autonomy and individualization, that is, the skills and attitudes necessary to the resolution of, problems (and thus necessary to creativity), the concept of which includes the production of new ideas and adaptation to change. This basic scientific culture allows citizens to understand socioeconomic and environmental imperatives related to science and technology. This study answers the following questions: (1) How is the appropriation of knowledge by Togolese students favored? (2) What are the representations acquired by Togolese students in the science classroom regarding key research concepts, namely education, culture, science, knowledge and development? The objective of this research is to partially describe the context of science learning in the first cycle of the Second Degree in Togo, a French-language developing country of Africa, and particularly to understand the influence of the sociocultural setting on pedagogy and development. We first present our conception of science teaching, followed by the construction of knowledge in context. This research permits clearer propositions in terms of plausible explanations for the observed relationships among the categories of data. Indeed, the framework of the transmission of knowledge considerably influences the appropriation of the field of science by Togolese students. Science is a mythical and mystical field, still perceived as the "white mans's thing", in spite of favorable attitudes developed by students concerning the application of science and technology in their environment. By way of the favored learning methods (which also represent those of the traditional environment) and curricula (which are exogenous in nature), students formally appropriate scientific knowledge without actually transferring that knowledge outside the school setting. For this study, the validity of the propositions is dependent upon the perceptions of the key research concepts by the subjects. That is why the propositions are supported by the analysis of the Togolese student's answers during interviews, as well as by lectures given by African essayists. This is an a priori exploratory research, characterized by a qualitative methodology. The research concentrates on preliminary description and comprehension. Specifically, the method is based on an interpretive approach, while also being reflexive in nature. Observation data were gathered through documentation, field observations, a group discussion and a questionnaire. The pertinence of this study's results lies in a better understanding of the construction of knowledge in context.

  13. Le Francais des Professions Scientifiques et Techniques (French for the Scientific and Technical Professions).

    ERIC Educational Resources Information Center

    Muller, Brigitte

    Two sequential courses in scientific and technical French developed as a supplement to third- and fourth-year college French, in response to expressed student and industry demand, had as their objectives to develop a general familiarity with products of the large French industrial companies and their United States affiliates and to develop means…

  14. Discours didactique scientifique et competence de communication (Didactic Scientific Discourse and Communicative Competence).

    ERIC Educational Resources Information Center

    Cabut, Helene; And Others

    The situation of foreign students arriving in Paris with no knowledge of French 3 months prior to their enrollment in science and engineering courses gave the impetus for the development of a set of exercises designed to train these students in the listening and writing skills they would need for their courses. Exercises were devised based on…

  15. L'Harmonisation des langues maliennes: entre l'Integration nationale et régionale

    NASA Astrophysics Data System (ADS)

    Ouane, Adama

    1991-03-01

    The standardization of Malian languages, which began in the period after independence, has been an educational reform guided more by linguists than by any institutional framework laid down by the political authorities of the country. This situation has permitted the technical application of a scientific strategy, but it has not led to widespread and general acceptance of the formulas which have been worked out. The consequent opposition between technical and political considerations, which have admittedly not always been in conflict, has been complicated by a set of additional factors which have made it difficult to reconcile internal (national) harmonization, dictated by local tendencies and balances between languages, and the need to respect the (regional) ecolinguistics of the country, whose linguistic and sociocultural divisions frequently extend well into other countries of the sub-region. This conflict is illustrated by the example of Malian languages with a wide regional distribution — Bamanan (Bambara) and Fulfulde (Fulani) — and by that of languages with a narrower distribution such as Bomu and Syenara-Mamara. The standardization of orthography and the creation of terminology in the MAPE (Mandingo-Peul) Project are the manifestation of a general acceptance of regionalism, while the choice of central, standard languages has often been made without regard for regional factors.

  16. The Future of the National Library of Canada. L'Avenia de la Bibliotheque Nationale du Canada.

    ERIC Educational Resources Information Center

    National Library of Canada, Ottawa (Ontario).

    Initially undertaken as a review of the achievements of the National Library of Canada during its first 25 years of existence, this study submitted to the Canadian government by the National Librarian includes a set of 11 recommendations for the future development of National Library functions, resources, and services. A brief description of the…

  17. BOOK REVIEW: Astronomie von Olbers bis Schwarzschild. Nationale Entwicklungen und internationale Beziehungen im 19. Jahrhundert (Acta Historica Astronomiae Vol. 16)

    NASA Astrophysics Data System (ADS)

    Sterken, C.; Dick, W. R.; Hamel, J.

    2002-12-01

    The 14th volume of the Acta Historica Astronomiae is the Proceedings of a Colloquium International Relationships in Astronomy (in German) organised by the History of Astronomy Section of the Astronomische Gesellschaft held on September 18 in Lilienthal, Germany. The book contains 13 articles on astronomical topics covering the 19th and 20th centuries. The first paper is by Guenther Oestmann and deals with contemporary assessments of Johann Hieronymus Schroeter's (1745-1816) astronomical works and with later judgements of the scientific importance and significance of his observations as seen by astronomers and historians. This report is complemented by a second article on Schroeter's 25-ft reflector in Lilienthal near Bremen. To this end, author Felix Luehning has constructed a scale model of the telescope, and shows how the building of a model brings a deeper understanding of function and handling of this instrument. This brings us to a third paper on telescope building in Lilienthal: Hans-Joachim Leue describes the cooperation of Johann Hieronymus Schroeter and Johann Gottlieb Schrader in developing a white reflecting metal alloy for use as telescope mirror. The fourth article, by Klaus Schillinger, describes on the basis of archival documents the aquisition history of the Herschel telescopes, including telescope quality check, repair and building. Memorial sites referring to Wilhelm Olbers, Johann Hieronymus Schroeter, Friedrich Wilhelm Bessel and Carl Friedrich Gauss are described by Arno Langkavel in two walks outlined in the very last paper of this book. Peter Brosche, in the fifth paper, discusses the rediscovery of Ceres in December1801, a discovery that was the result of the combined efforts of a theoretician (Gauss) and an observer (Zach). Juergen Hamel's paper is based on previously unused archival sources and discusses the outstanding role played by H. C. Schumacher (1780-1850, editor of the Astronomische Nachrichten) in the communication between astronomers in his days, when his working place at Altona still belonged to the kingdom of Denmark. This paper is followed by a second one by the same author and deals with the correspondence of H. C. Schumacher and H C. Oersted (1777-1851) and shows how intense and diverse their cooperation was. In a subsequent paper, Wolfgang Kokott describes the role of the Astronomisches Jahrbuch (published from 1776 by the Royal Academy of Sciences at Berlin), a ranking international publication, with Bode's modest Berlin Observatory serving as a clearinghouse of information originating from virtually all European countries. "Karl Schwarzschild and the professionalisation of Astrophysics" is the title of Theodor Schmidt-Kaler's contribution and presents Schwarzschild's contributions to professionalization of astronomy: establishment of course lectures and a permanent astrophysical laboratory, a tight connection between teaching and research, stimulations and suggestions for astronomy at high school and for the formation of high school teachers, international organisation, and the planning of a southern observatory. Peter Habison describes the contribution of Leo de Ball (1853-1916, Director of the Kuffner Observatory in Vienna) to international astronomy. Internationalization in astronomy is also discussed in a following paper by Gudrun Wolfschmidt on the establishment of the Vereinigte Astronomische Gesellschaft, the international Astronomische Gesellschaft in 1863 and finally the International Astronomical Union in 1919. In the second but last paper of the book, Hilmar Duerbeck describes the history of the Chilean National Observatory, beginning with its origins out of Gilliss' US Naval Expedition to the Southern Hemisphere in 1849, over its directors Moesta, Vergara, Obrecht and Ristenpart, to the middle of the 20th century. The paper also includes the astronomical development at the Universidad Catolica and various international expeditions, which aimed at the observations of solar eclipses, the Venus transit of 1882, and the Mars opposition of 1907. An overview of the evolution and the actual state of the international observatories Cerro Tololo, La Silla and Paranal, as well as Las Campanas is also given.

  18. Results of screening activities in salt states prior to the enactment of the Nationall Waste Policy Act

    SciTech Connect

    Carbiener, W.A.

    1983-01-01

    The identification of potential sites for a nuclear waste repository through screening procedures in the salt states is a well-established, deliberate process. This screening process has made it possible to carry out detailed studies of many of the most promising potential sites, and general studies of all the sites, in anticipation of the siting guidelines specified in the Nuclear Waste Policy Act. The screening work completed prior to the passage of the Act allowed the Secretary of Energy to identify seven salt sites as potentially acceptable under the provisions of Section 116(a) of the Act. These sites were formally identified by letters from Secretary Hodel to the states of Texas, Utah, Mississippi, and Louisiana on February 2, 1983. The potentially acceptable salt sites were in Deaf Smith and Swisher Counties in Texas; Davis and Lavender Canyons in the Gibson Dome location in Utah; Richton and Cypress Creek Domes in Mississippi; and Vacherie Dome in Louisiana. Further screening will include comparison of each potentially acceptable site against disqualification factors and selection of a preferred site in each of the three geohydrologic settings from those remaining, in accordance with the siting guidelines. These steps will be documented in statutory Environmental Assessments prepared for each site to be nominated for detailed characterization. 9 references.

  19. SiO Chimneys and Supershells in M82

    NASA Astrophysics Data System (ADS)

    García-Burillo, S.; Martín-Pintado, J.; Fuente, A.; Neri, R.

    2001-12-01

    In this Letter we present the first images of the emission of SiO and H13CO+ in the nucleus of the starburst galaxy M82. Contrary to other molecular species that mainly trace the distribution of the star-forming molecular gas within the disk, the SiO emission extends noticeably out of the galaxy plane. The bulk of the SiO emission is restricted to two major features. The first feature, referred to as the SiO supershell, is an open shell of 150 pc diameter, located 120 pc west from the galaxy center. The SiO supershell represents the inner front of a molecular shell expanding at ~40 km s-1, produced by mass ejection around a supercluster of young stars containing supernova remnant SNR 41.95+57.5. The second feature is a vertical filament, referred to as the SiO chimney, emanating from the disk at 200 pc east from the galaxy center. The SiO chimney reaches a 500 pc vertical height, and it is associated with the most prominent chimney identified in radio continuum maps. The kinematics, morphology, and fractional abundances of the SiO gas features in M82 can be explained in the framework of shocked chemistry driven by local episodes of gas ejection from the starburst disk. The SiO emission stands out as a privileged tracer of the disk-halo interface in M82. We speculate that the chimney and the supershell, each injecting ~107 Msolar of molecular gas, are two different evolutionary stages in the outflow phenomenon building up the gaseous halo. Based on observations carried out with the Institut de Radioastronomie Millimétrique (IRAM) Plateau de Bure Interferometer. IRAM is supported by the Institut Nationale des Sciences de l'Univers/Centre Nationale de la Recherche Scientifique (France), Max-Planck-Gesellschaft (Germany), and Instituto Geografico Nacional (Spain).

  20. L'apprentissage de la lecture du francais scientifique et la langue maternelle (The Relationship between a Speaker's Native Language and Learning to Read Technical French).

    ERIC Educational Resources Information Center

    Ulijn, Jan

    Two questions arise from attempts to develop reading comprehension in scientific French: (1) should the concentration be mainly on vocabulary, or on grammar as well, and if so, what aspect of grammar; and (2) should the students' native language be taken into account, and if so, in what way: by translating, or through a systematic comparison of…

  1. Interpretation d'une Controverse Scientifique: Strategies Argumentatives d'Adolescentes et d'Adolescents Quebecois (Interpretation of a Scientific Controversy: Argument Strategies of Adolescents and Quebecois Adolescents).

    ERIC Educational Resources Information Center

    Bader, Barbara

    2003-01-01

    Sketches out the argumentative strategies used by three 17-year-old boys to interpret the disagreement presented to them. Shows that they were inclined to adduce current ideas about science--framed according to a realist, empiricist epistemology--but that there are grounds for thinking that high school students would be capable of actualizing…

  2. Opportunities for Tomorrow: National Learning Needs Assessment Summary Report = Des Possibilities pour L'Avenir: Rapport Sommaire sur L'Evaluation Nationale des Besoins en Apprentisage.

    ERIC Educational Resources Information Center

    Communications, Energy & Paperworkers Union of Canada, Ottawa (Ontario).

    The Communications, Energy, and Paperworkers Union of Canada assessed literacy learning needs. In focus group discussions, members were asked their perception of such needs in the face of changes in the workplace and society; local union officers (LUOs) were asked how they saw the role of unions in supporting members' literacy learning; employers…

  3. Support for a special symposium to highlight the research of early career women physical chemists at the 2011 fall ACS nationall meeting, Aug 28-Sept

    SciTech Connect

    Geraldine Richmond

    2012-12-19

    The symposium was well attended during the 4-day symposium. The invited speakers were primarily women in early career stage (~4-8 years) with a few senior women and men as invited speakers or session chairs. Included in each day was a Poster Session for graduate students and a lunch in which the turn out was strong and the posters presented encouraged much of dialogue with the invited speakers, guests and others attending the ACS meeting and wanted to discuss the student’s research and meet with the speakers. Most all speakers and participants were very positive about the sessions and expressed that the funding to cover some expenses made it possible for them to attend the conference and the poster session luncheon. There was a total of 51 presenters, below are the speakers and their abstracts, in order presented:

  4. Local network interconnection through a satellite point-to-multipoint link. Ph.D. Thesis - Ecole Nationale Superieure des Telecommunications, 6 Jul. 1985

    NASA Technical Reports Server (NTRS)

    Duarte, O. Muniz Bandeira

    1986-01-01

    Four architectures to implement a point to multipoint satellite link protocol for communication services offered by the Telecom 1 satellite network are presented. A safe communication service with error correction and flow control facilities is described. It is shown that a time transparent communication system combines simplicity and cost advantages.

  5. The IC1396N proto-cluster at a scale of ~250 AU

    NASA Astrophysics Data System (ADS)

    Neri, R.; Fuente, A.; Ceccarelli, C.; Caselli, P.; Johnstone, D.; van Dishoeck, E. F.; Wyrowski, F.; Tafalla, M.; Lefloch, B.; Plume, R.

    2007-06-01

    Aims:We investigate the mm-morphology of IC 1396 N with unprecedented spatial resolution to analyze its dust and molecular gas properties, and draw comparisons with objects of similar mass. Methods: We have carried out sensitive observations in the most extended configurations of the IRAM Plateau de Bure interferometer, to map the thermal dust emission at 3.3 and 1.3 mm, and the emission from the J=13_k→ 12k hyperfine transitions of methyl cyanide (CH3CN). Results: We unveil the existence of a sub-cluster of hot cores in IC 1396 N, distributed in a direction perpendicular to the emanating outflow. The cores are embedded in a common envelope of extended and diffuse dust emission. We find striking differences in the dust properties of the cores (β≃ 0) and the surrounding envelope (β≃ 1), very likely testifying to differences in the formation and processing of dust material. The CH3CN emission peaks towards the most massive hot core and is marginally extended in the outflow direction. Based on observations obtained at the IRAM Plateau de Bure Interferometer (PdBI). IRAM is funded by the Centre Nationale de la Recherche Scientifique (France), the Max-Planck Gesellschaft (Germany), and the Instituto Geográfico Nacional (Spain).

  6. Invatamantul cu Predarea in Limbile Minoritatilor Nationale din Romania. In Anul Scolar 1992/1993 = The Education System in Romania: Tuition in the Languages of Ethnic Minorities. The School Year 1992/1993 = L'enseignement dispense dans les langues des minorites nationales de Roumanie. L'annee scolaire 1992/1993.

    ERIC Educational Resources Information Center

    Council for National Minorities, Bucharest (Romania).

    Documentation of the Romanian system of language instruction in ethnic minority languages is presented in Romanian, French, and English. It consists of: relevant provisions from the national constitution concerning the rights of ethnic minority members; organization and functioning of the educational system at the elementary, middle, and secondary…

  7. The International System of Units (SI) in Oceanography. Report of IAPSO Working Group on Symbols, Units and Nomenclature in Physical Oceanography (SUN). Unesco Technical Papers in Marine Science 45. IAPSO Publication Scientifique No. 32.

    ERIC Educational Resources Information Center

    United Nations Educational, Scientific, and Cultural Organization, Paris (France). Div. of Marine Sciences.

    This report introduces oceanographers to the International System of Units (SI) in physical oceanography. The SI constitutes a universal language, designed to be understood by all scientists. It facilitates their mutual comprehension and exchange of views and results of their work. The first part of the report is devoted to physical quantities,…

  8. The International Development Research Centre: A Guide for the Canadian University Research Community = Le Centre de recherches pour le developpement international: guide a l'intention des scientifiques des universites Canadiennes.

    ERIC Educational Resources Information Center

    Tillman, George; Wasilewski, Ania, Ed.

    Written in both English and French this is a manual for the Canadian research community. It describes the International Development Research Centre (IDRC) and its operations. The main objective of the IDRC is to assist scientists in developing countries to identify and conduct research into long term practical solutions to development problems.…

  9. Biosimilars: from technical to pharmacoeconomic considerations. 30th Rencontres Nationales de Pharmacologie et Recherche clinique pour l'Innovation et l'Evaluation des Technologies de Santé. Tables rondes.

    PubMed

    Girault, Danièle; Trouvin, Jean-Hugues; Blachier-Poisson, Corinne; Gary, François; Laloye, Didier; Bergmann, Jean-François; Casadevall, Nicole; Delval, Cécile; De Sahb Berkovitch, Rima; Fagon, Jean-Yves; Gersberg, Marta; Lassale, Catherine; Lechat, Philippe; Le Jeunne, Claire; Montastruc, Jean-Louis; Prugnaud, Jean-Louis; Ratignier-Carbonneil, Christelle; Rey-Coquais, Cécile

    2015-01-01

    A biosimilar is a biological medicinal product claimed to be similar to a reference biological medicinal product. Its development plan includes studies comparing it with the reference product in order to confirm its similarity in terms of quality, preclinical safety, clinical efficacy, and clinical safety, including immunogenicity. Biosimilars differ from generics both in their molecular complexity and in the specific requirements that apply to them. Since patents on many biological medicinal products will expire within the next 5 years in major therapeutic areas such as oncology, rheumatology and gastroenterology and as those products are so costly to the French national health insurance system, the availability of biosimilars would have a considerable economic impact. The round table has issued a number of recommendations intended to ensure that the upcoming arrival of biosimilars on the market is a success, in which prescribing physicians would have a central role in informing and reassuring patients, an efficient monitoring of the patients treated with biologicals would be set up and time to market for biosimilars would be speeded up. PMID:25679193

  10. Resultats de l'enquete nationale sur les programmes de formation des enseignants de francais langue seconde au Canada (Results of the National Study for Teacher Education Programs for French Second Language Teachers in Canada).

    ERIC Educational Resources Information Center

    Boutin, France; Chinien, Christian; Boutin, Jean-Luc

    The implications of Canada's national study of core French instruction for second language (L2) teacher education in that country are examined. Literature on the study's impact on language teaching philosophy and policy and on French immersion instruction is reviewed, and a survey of 36 Canadian schools of education is reported. The questionnaire…

  11. Role of uncontrolled HIV RNA level and immunodeficiency in the occurrence of malignancy in HIV-infected patients during the combination antiretroviral therapy era: Agence Nationale de Recherche sur le Sida (ANRS) CO3 Aquitaine Cohort

    PubMed Central

    Bruyand, Mathias; Thiébaut, Rodolphe; Lawson-Ayayi, Sylvie; Joly, Pierre; Sasco, Annie-Jeanne; Mercié, Patrick; Luc Pellegrin, Jean; Neau, Didier; Dabis, François; Morlat, Philippe; Chêne, Geneviève; Bonnet, Fabrice

    2009-01-01

    Background HIV-infected patients are at higher risk of malignancies. Besides traditional determinants, a specific deleterious effect of HIV and immunodeficiency is speculated. We aimed at studying the association between immunological and virological characteristics of HIV-infected patients in care and the risk of AIDS-defining and non-AIDS-defining malignancies. Methods Patients consecutively enrolled in the hospital based ANRS CO3 Aquitaine Cohort were included if their follow-up was >3 months between 1998 and 2006. Multivariate modelling used an extended Cox proportional hazards models for time-dependent covariates and delayed entry. Results The 4,194 patients included developed 251 first malignancies during 22,389 person-years. A higher incidence of AIDS-defining malignancies (107 cases) was independently associated with: (i) both longer and current exposures to plasma HIV RNA >500 copies/ml: Hazard ratio [HR]=1.27 per year; p<0.001 and HR=3.30; p<0.001, respectively, and (ii) both longer and current exposure to CD4+ count<200/mm3: HR=1.36 per year; p<0.001 and HR=6.33; p<0.001, respectively. A higher incidence of non-AIDS-defining malignancies (144 cases) was independently associated with longer and current exposure to CD4+ count<500/mm3 (HR=1.13 per year; p=0.01 and HR=2.07; p<0.001, respectively), and male gender (HR=1.69; p=0.02) but not plasma HIV RNA (p=0.49 and p=0.10 for cumulative and current exposures). Conclusions Uncontrolled plasma HIV RNA was independently associated with a higher likelihood of developing AIDS-defining malignancies, while immunosuppression was associated with a higher risk of developing any types of malignancies. Antiretroviral treatment should aim at reaching and maintaining a CD4+ count >500/mm3 to prevent the occurrence of malignancy, this should be integrated to malignancy prevention policies. PMID:19705973

  12. Recherche universitaire et priorites nationales: l'effet du financement public sur la recherche energie solaire au Canada (University Research and National Priorities: The Effect of Public Financing on Solar Energy Research in Canada).

    ERIC Educational Resources Information Center

    Dalpe, Robert; Gingras, Yves

    1990-01-01

    The role of two main sources of university research financing in solar energy is examined to assess whether they oriented research in the direction of government programs. The strongest relationship appears to be in journal publication patterns. This scientific community has acquired the capacity to tap varying sources. (Author/MSE)

  13. Collaborateurs aux lignes directrices en soins primaires

    PubMed Central

    Allan, G. Michael; Kraut, Roni; Crawshay, Aven; Korownyk, Christina; Vandermeer, Ben; Kolber, Michael R.

    2015-01-01

    Résumé Objectif Déterminer la profession des collaborateurs scientifiques aux lignes directrices, les variables associées aux différences de participation des collaborateurs et si oui ou non les lignes directrices en soins primaires fournissent un énoncé sur les conflits d’intérêts. Type d’étude Analyse rétrospective des lignes directrices en soins primaires affichées sur le site web de l’Association médicale canadienne. Deux extracteurs de données indépendants ont examiné les lignes directrices et ont extrait les données pertinentes. Contexte Canada Principaux paramètres à l’étude Commanditaires des lignes directrices, territoire (national ou provincial) visé par les lignes directrices, profession des collaborateurs scientifiques aux lignes directrices et énoncés de conflits d’intérêts rapportés dans les lignes directrices. Résultats Sur les 296 lignes directrices de pratique clinique trouvées dans la section de la médecine familiale de l’Infobanque AMC, 65 apparaissaient en double et 35 se rapportaient de façon limitée à la médecine familiale. Vingt ne fournissaient aucune information sur les collaborateurs scientifiques, ce qui laissait 176 lignes directrices propices à l’analyse. Au total, il y avait 2495 collaborateurs (auteurs et membres de comité) : 1343 (53,8 %) spécialistes autres que des médecins de famille, 423 (17,0 %) médecins de famille, 141 (5,7 %) infirmières, 75 (3,0 %) pharmaciens, 269 (10,8 %) autres cliniciens, 203 (8,1 %) scientifiques non cliniciens et 41 (1,6 %) collaborateurs de profession inconnue. La proportion des collaborateurs de ces professions différait significativement entre les lignes directrices nationales et provinciales, de même qu’entre les lignes directrices financées par l’industrie et celles qui ne l’étaient pas (p < 0,001 dans les 2 cas). Dans le cas des lignes directrices de pratique clinique provinciales, 30,8 % des collaborateurs étaient des médecins de

  14. Préface

    NASA Astrophysics Data System (ADS)

    Aspect, Alain

    2004-11-01

    COLOQ est une conférence regroupant, tous les deux ans, la communauté scientifique et industrielle nationale travaillant dans les domaines des lasers, de l'optique non-linéaire et de l'optique quantique. Elle s'est tenue pour sa huitième édition à Toulouse, du 3 au 5 septembre 2004, sur le campus de I'INSA. Comme il est de tradition tous les quatre ans, COLOQ était couplé avec Horizons de l'optique, avec en particulier une journée commune dont le programme avait été préparé en concertation par les deux comités scientifiques. Depuis sa création, COLOQ a pour but de favoriser les rencontres entre les chercheurs des différents laboratoires nationaux publics ou privés travaillant sur les lasers et l'optique quantique au sens large. C'est un moyen privilégié de resserrer les liens de cette communauté et d'y intégrer les jeunes chercheurs. Ces derniers y trouvent l'occasion de se connaître, de se faire connaître, de découvrir la communauté à laquelle ils appartiennent et d'élargir leurs connaissances des thèmes qui la structurent. La participation de 230 chercheurs et d'une vingtaine d'exposants de matériels spécialisés dans les lasers et l'optoélectronique témoigne de la vitalité de COLOQ et de son audience dans les laboratoires et chez les industriels de l'optique. Le programme de COLOQ 8 comportait d'une vingtaine de conférences générales données par des chercheurs de renom international, et des séances de communications par affiches, occasions privilégiées de rencontres et d'échanges. Les exposés ont porté sur des sujets particulièrement actifs au niveau national et international, avec un accent sur des thèmes importants pour la région toulousaine : contrôle cohérent, optique et nanosciences, optique et astronomie, sans oublier la traditionnelle rubrique phénomènes fondamentaux, éclectique pour ne pas dire hétéroclite, mais si représentative d'une des ambitions de COLOQ qui est d'offrir à ses participants une

  15. EGS Richardson AGU Chapman NVAG3 Conference: Nonlinear Variability in Geophysics: scaling and multifractal processes

    NASA Astrophysics Data System (ADS)

    Schertzer, D.; Lovejoy, S.

    was followed by five days with 8 oral sessions and one poster session. Overall, there were 65 papers involving 74 authors. In general, the main topics covered are reflected in this special issue: geophysical turbulence, clouds and climate, hydrology and solid earth geophysics. In addition to AGU and EGS, the conference was supported by the International Science Foundation, the Centre Nationale de Recherche Scientifique, Meteo-France, the Department of Energy (US), the Commission of European Communities (DG XII), the Comite National Francais pour le Programme Hydrologique International, the Ministere de l'Enseignement Superieur et de la Recherche (France). We thank P. Hubert, Y. Kagan, Ph. Ladoy, A. Lazarev, S.S. Moiseev, R. Pierrehumbert, F. Schmitt and Y. Tessier, for help with the organization of the conference. However special thanks goes to A. Richter and the EGS office, B. Weaver and the AGU without whom this would have been impossible. We also thank the Institut d' Etudes Scientifiques de Cargese whose beautiful site was much appreciated, as well as the Bar des Amis whose ambiance stimulated so many discussions. 2. Tribute to L.F. Richardson With NVAG3, the European geophysical community paid tribute to Lewis Fry Richardson (1881-1953) on the 40th anniversary of his death. Richardson was one of the founding fathers of the idea of scaling and fractality, and his life reflects the European geophysical community and its history in many ways. Although many of Richardson's numerous, outstanding scientific contributions to geophysics have been recognized, perhaps his main contribution concerning the importance of scaling and cascades has still not received the attention it deserves. Richardson was the first not only to suggest numerical integration of the equations of motion of the atmosphere, but also to attempt to do so by hand, during the First World War. This work, as well as a presentation of a broad vision of future developments in the field, appeared in his

  16. Préface

    NASA Astrophysics Data System (ADS)

    Chardonnet, Christian; Millot, Guy

    2006-10-01

    COLOQ, réunion nationale biennale initiée en 1988 par la communauté française des lasers, de l'optique non linéaire et de l'optique quantique atteint sa neuvième édition. Depuis sa création, les objectifs poursuivis sont les suivants : - réunir la communauté française des lasers, de l'optique non linéaire et de l'optique quantique, en dépassant les clivages fondamental/appliqué, recherche publique/industrielle, - faire le point sur les avancées récentes, - permettre aux jeunes chercheurs de se rencontrer, de s'exprimer et de s'aguerrir au plan national. Le but est que tout thésard du domaine de l'optique puisse participer à COLOQ une fois durant sa thèse, présenter son travail et de se confronter à la communauté de l'optique. COLOQ9 s'est tenu, pour sa 9e édition, sur le campus universitaire de Dijon, du 7 au 9 septembre 2005. Il a été une grande réussite : nombre de participants (255) et de présentations scientifiques record (148 affiches), forte représentation des industriels (15) et participation d'environ 200 lycéens aux conférences grand public. Le nombre plus élevé que prévu d'affiches a rendu un peu serrée leur présentation : une attention particulière sera portée à cet aspect lors des prochaines éditions. Ces journées ont été consacrées à des conférences invitées données par des scientifiques de haut niveau et à des présentations sous forme d'affiches. Une plage de temps importante a été réservée pour des discussions autour des affiches. À proximité immédiate de la salle de conférence, l'exposition de matériels spécialisés pour les lasers, l'optique et l'optoélectronique a été une occasion pour les jeunes participants de découvrir et contacter les industriels et les autres grands acteurs de l'optique. L'année 2005 ayant été l'année mondiale de la physique, COLOQ9 a retenu comme thème central ”1905-2005 : à propos d'Einstein". Plusieurs grandes conférences ont été dédiées à ce th

  17. ESMC

    ScienceCinema

    None

    2011-04-25

    Workshops de 2 jours au Cern: 1.partie: communication scientifique: plusieurs discours suivis de questions et intenses discussions: 1.François de Closet "le progrès scientifique" 2.Gerhard Moosleiter(?) exposé avec dias et questions 3.H.Meyers "comment créer de meilleures conditions en communication scientifique 2.partie: science et communication :présentation des dias et questions. Une Russe de Moscou parle entre autre de la situation actuelle de la presse scientifique en Russie 3.partie: conclusions et rapports de la veille de differents groupes de travail 4.partie:questions avec C.Rubbia et N.Calder et remerciements

  18. ESMC

    SciTech Connect

    2007-10-31

    Workshops de 2 jours au Cern: 1.partie: communication scientifique: plusieurs discours suivis de questions et intenses discussions: 1.François de Closet "le progrès scientifique" 2.Gerhard Moosleiter(?) exposé avec dias et questions 3.H.Meyers "comment créer de meilleures conditions en communication scientifique 2.partie: science et communication :présentation des dias et questions. Une Russe de Moscou parle entre autre de la situation actuelle de la presse scientifique en Russie 3.partie: conclusions et rapports de la veille de differents groupes de travail 4.partie:questions avec C.Rubbia et N.Calder et remerciements

  19. Preface

    NASA Astrophysics Data System (ADS)

    Aspect, Alain

    2002-06-01

    COLOQ est une conférence regroupant, tous les deux ans, la communauté scientifique et industrielle nationale travaillant dans les domaines des lasers, de l'optique non-linéaire et de l'optique quantique. Elle s'est tenue pour sa septième édition à Rennes, du 5 au 7 septembre 2001, sur le campus de Beaulieu de l'Université de Rennes I. Cette réunion a pour but de favoriser les rencontres entre les membres des différents laboratoires nationaux publics ou privés travaillant sur ces sujets. C'est donc un moyen privilégié de resserrer les liens de cette communauté et d'y intégrer les jeunes chercheurs. Une dimension importante de COLOQ est de permettre aux jeunes chercheurs de se connaître, de se faire connaître, de découvrir la communauté à laquelle ils appartiennent et d'élargir leurs connaissances des thèmes qui la structurent. La participation de 200 chercheurs et de 18 exposants de matériels spécialisés dans les lasers et l'optoélectronique témoigne de la vitalité de COLOQ. Le programme de COLOQ 7 a comporté des conférences générales données par des chercheurs de renom international et des séances de communications par voie d'affiches. Les exposés ont porté sur des sujets d'optique particulièrement actifs au niveau national et international : les télécoms, thème cher à la région Bretagne en particulier, les phénomènes fondamentaux, les nouvelles percées de l'optique en métrologie et mesures ultra-sensibles, sujets privilégiés du laboratoire organisateur, les sources de l'extrême (incluant X et V-UV). Parallèlement à 20 conférences invitées, 130 communications par affiches ont présenté, tout au long du colloque, les plus récents résultats concernant les atomes froids et la métrologie, les télécoms optiques, l'optique non-linéaire et les nouveaux matériaux, les nanostructures et l'optique de champ proche, la physique des lasers, etc. Ce volume spécial du Journal de Physique IV regroupe la presque totalit

  20. Quel avenir pour les combustibles fossiles ? Les avancées scientifiques et technologiques permettront-elles la poursuite d'un développement soutenable avec les énergies carbonées ?What a future for fossil fuels? Will scientific and technological progresses warrant growth of use in carbon-based fuels?

    NASA Astrophysics Data System (ADS)

    Tissot, Bernard

    2001-12-01

    The world demand for primary energy keeps increasing and has little chance to decrease over the next decades, when considering the desirable and necessary development of the less wealthy countries. The two weightiest questions are to provide electricity to megalopolis, and fuels for transportation. In the present situation, fossil fuels (crude oil, natural gas and coal) provide 90 % of primary energy. Furthermore, hydrocarbons (crude oil and gas) are considered as closing energies to balance the level of demand. However, the link between fossil fuel consumption for one and a half century and climate change is now considered as highly probable. Crude oil and natural gas reserves are substantial, but limited. One half of the proven reserves of crude oil, and one third of gas reserves will be already used in year 2020. Gas reserves will be sufficient to reach 2050, but proven reserves of crude oil will not last until that year. Coal only, which is the largest source of CO 2 and pollutants, provides enough reserves for several centuries. A considerable effort of scientific and technological research is the only way to reach the end of the century using oil and gas, plus a drastic effort for saving energy. This effort in research is discussed in the paper, but it does not provide until now an answer to the climate problem.

  1. Communique: Special Issue on the International Scientific Conference and Exhibit and the 7th Session of the International Co-Ordinating Council for MAB (Paris, Sept. 22-Oct. 2, 1981) = Numero special sur la Conference Scientifique Internationale et Exposition et al 7e session du Counseil International de Coordination du MAB (Paris, du 22 Sept. au 2 Oct. 1981).

    ERIC Educational Resources Information Center

    Communique, 1982

    1982-01-01

    Presented are summaries of two separate but closely-related conferences. The International Scientific Conference and Exhibit, organized to mark the 10th anniversary of the Man and the Biosphere Program (MAB), was based on the theme "ecology in practice: establishing a scientific basis for land management." This summary includes: a 10 year…

  2. Presentation by the scientific and technical commission on the analysis of the events relating to the unexpected ice storm of 5 to 9 January. Presentation a la commission scientifique et technique chargee d'analyser les evenements relatifs (a) la tempete de verglas survenue du 5 au 9 janvier 1998

    SciTech Connect

    Not Available

    1998-01-01

    The first part of this report contains three presentations in French by directors of Hydro-Quebec regarding the utility's actions during the January 1998 ice storm and initiatives to reinforce and maintain the power network to avoid ice storm problems in the future. The second part is in a question and answer format and covers the utility's response to ice storm threats in the following areas: Climate (forecasting of ice storm periods, line design criteria, impact of climatic changes and El Nino, ice data interpretation and measurement, research); structural aspects, including failures of components, towers, and lines; electrical aspects, including consolidation of the transmission system, power system security, burying of installations, conductor de-icing, strategic lines, and manpower use; economic aspects (network improvement, reliability, continuity and maintenance expenditures, interconnections, internal communications, service enhancement programs, work force reduction, strategic plans); and the management of emergency measures, including planning, service restoration priorities, human and material resources management, coordination, communications, and risk analysis.

  3. Presentation by the scientific and technical commission on the analysis of the events relating to the unexpected ice storm of 5 to 9 January; Presentation a la commission scientifique et technique chargee d`analyser les evenements relatifs (a) la tempete de verglas survenue du 5 au 9 janvier 1998

    SciTech Connect

    1998-12-31

    The first part of this report contains three presentations in French by directors of Hydro-Quebec regarding the utility`s actions during the January 1998 ice storm and initiatives to reinforce and maintain the power network to avoid ice storm problems in the future. The second part is in a question and answer format and covers the utility`s response to ice storm threats in the following areas: Climate (forecasting of ice storm periods, line design criteria, impact of climatic changes and El Nino, ice data interpretation and measurement, research); structural aspects, including failures of components, towers, and lines; electrical aspects, including consolidation of the transmission system, power system security, burying of installations, conductor de-icing, strategic lines, and manpower use; economic aspects (network improvement, reliability, continuity and maintenance expenditures, interconnections, internal communications, service enhancement programs, work force reduction, strategic plans); and the management of emergency measures, including planning, service restoration priorities, human and material resources management, coordination, communications, and risk analysis.

  4. Communique: Special Issue on the International Network for Cooperation in Northern Science Created at a Meeting held in Edmonton, Alberta (October 12-15, 1982). Summary of Discussions and Agreements Reached = Numero special sur le Reseau Scientifique Internationale pour le Nord cree a la reunion tenue a Edmonton, Alberta (du 12 au 15 octobre 1982). Resume des discussions et accords conclus.

    ERIC Educational Resources Information Center

    Communique, 1983

    1983-01-01

    Delegations from Canada, Finland, Greenland, Norway, Sweden, and the United States agreed to the establishment of a network for cooperation among individuals engaged in problems peculiar to the circumpolar North. The Northern Science Network, established within the Unesco Man and the Biosphere Program, consists of three themes: studies on the…

  5. Factors associated with mortality in human immunodeficiency virus type 1-infected adults initiating protease inhibitor-containing therapy: role of education level and of early transaminase level elevation (APROCO-ANRS EP11 study). The Antiprotéases Cohorte Agence Nationale de Recherches sur le SIDA EP 11 study.

    PubMed

    Lewden, Charlotte; Raffi, François; Cuzin, Lise; Cailleton, Valérie; Vildé, Jean-Louis; Chêne, Geneviève; Allavena, Clotilde; Salamon, Roger; Leport, Catherine

    2002-09-01

    This study attempted to identify factors associated with mortality among human immunodeficiency virus (HIV)-infected adults starting a protease inhibitor (PI)-containing therapy. Among 1155 patients consecutively enrolled in the APROCO study between May 1997 and June 1998, clinical characteristics were as follows: median age, 36 years; median baseline CD4 cell count, 288 cells/mm(3); and median baseline plasma HIV RNA load, 4.4 log(10) copies/mL. After a median follow-up of 27 months, 48 deaths had occurred, of which 44% were related to acquired immune deficiency syndrome. The mortality rate was 2.9% at 12 months. When both data at baseline and data at 4 months after the start of PI therapy were considered, factors independently associated with mortality were (Cox model) low baseline plasma creatinine level, low school education level, low CD4 cell count at 4 months, low hemoglobin level, and elevated hepatic transaminase levels. Thus, social context plus clinical and biologic data, including the 4-month response to treatment, must be considered in treatment of HIV-infected patients. PMID:12195361

  6. Optical Disk Technology and the Library. Part 1: The Technology and Its Applications. Part 2: The National Library Videodisc Demonstration Project. Canadian Network Papers Number 9 = Technologie du Videodisque et la Bibliotheque. Premiere partie: La Technologie et ses Applications. Deuxieme partie: Projet de Demonstration du Videodisque a la Bibliotheque Nationale. Documents sur les Reseaux Canadiens Numero 9.

    ERIC Educational Resources Information Center

    Duchesne, Roddy; Sonnemann, Sabine S.

    This report is intended to assist Canadian libraries in assessing potential library applications of optical disk technology. Part 1 provides a general outline of the technology and describes a number of library applications and projects. Descriptions are purposely general and illustrative in nature since the technology and its applications are…

  7. Attitude of pregnant women towards HIV testing in Abidjan, Côte d'Ivoire and Bobo-Dioulasso, Burkina Faso. DITRAME Study Group (ANRS 049 Clinical Trial). Diminution de la Transmission Mère Enfant du VIH. Agence Nationale de Recherches sur le SIDA

    PubMed Central

    Cartoux, Michel; Msellati, Philippe; Meda, Nicolas; Welffens-Ekra, Christiane; Mandelbrot, Laurent; Leroy, Valériane; Van De Perre, Philippe; Dabis, François

    1998-01-01

    Objective To evaluate the attitude of pregnant women towards HIV testing in two cities of West Africa: Abidjan, Côte d’Ivoire and Bobo-Dioulasso, Burkina Faso. Methods In the context of a clinical trial to prevent HIV vertical transmission, HIV counselling and testing was offered systematically to women attending antenatal clinics. Informed consent was obtained and test results were given anonymously. Multiple logistic regression was performed to identify factors associated with refusal for testing and failure to return for test results. Results A total of 9724 pregnant women were interviewed from January 1995 to September 1996. In Abidjan (n = 5766) and Bobo-Dioulasso (n = 3958), 78 and 92.4% of the women consented to HIV testing, respectively, and 58.4 and 81.8% of them returned for the test results disclosure, respectively. In the two sites, the counsellors themselves and high educational level of the women appeared to be related to refusal of the test, whereas last trimester gestation was associated with failure to return for test results. In Abidjan, foreigners and employees were more likely to refuse testing, and HIV-infected women were three times less likely to return for results than uninfected women. Conclusion Future implementation of interventions to reduce vertical transmission of HIV that require antenatal HIV testing and counselling will have to solve issue of acceptability of HIV testing by pregnant women. PMID:9863877

  8. Problem of Questioning

    ScienceCinema

    None

    2011-04-25

    Le Prof.Leprince-Ringuet, chercheur sur le plan scientifique, artistique et humain, parle de la remise en question des hommes et la remise en question scientifique fondamentale ou exemplaire- plusieurs personnes prennent la parole p.ex Jeanmairet, Adam, Gregory. Le Prof.Gregory clot la soirée en remerciant le Prof.Leprince-Ringuet

  9. Regelungen im Verkehr mit Lebensmitteln und Bedarfsgegenständen in Deutschland

    NASA Astrophysics Data System (ADS)

    Thomas, Gundula; Freund, Astrid; Gründig, Friedrich

    Im Zuge der Globalisierung von Produktion und Handel ändert sich auch der Charakter der Vorschriften im Lebensmittelrecht. Zunehmend treten internationale Rechtsbestimmungen, Abkommen, Standards und andere Normen an die Stelle nationaler Regelungen.

  10. The Computerization of the National Library in Paris.

    ERIC Educational Resources Information Center

    Lerin, Christian; Bernard, Annick

    1986-01-01

    Describes the organization and automation plan of the Bibliotheque Nationale (Paris, France) that was begun in 1981. Highlights include the method of moving toward computerization; technical choices; the choosing procedure (pre-qualification, bench-mark test); short term and pilot operations; and preparation for the implementation of the…

  11. Cultural Dimensions of Digital Library Development, Part II: The Cultures of Innovation in Five European National Libraries (Narratives of Development)

    ERIC Educational Resources Information Center

    Dalbello, Marija

    2009-01-01

    This article presents the narrative accounts of the beginnings of digital library programs in five European national libraries: Biblioteca nacional de Portugal, Bibliotheque nationale de France, Die Deutsche Bibliothek, the National Library of Scotland, and the British Library. Based on interviews with policy makers and developers of digital…

  12. 21 CFR Appendix B to Subpart A of... - List of Authorities

    Code of Federal Regulations, 2013 CFR

    2013-04-01

    ... Control Farmacéutico. For medicinal products for veterinary use: Ministerio de Agricultura, Pesca y...: Agence du Médicament. For veterinary medicinal products: Agence Nationale du Médicament Vétérinaire..., Dipartimento Farmaci e Farmacovigilanza. For medicinal products for veterinary use: Ministero della...

  13. 21 CFR Appendix B to Subpart A of... - List of Authorities

    Code of Federal Regulations, 2012 CFR

    2012-04-01

    ... Control Farmacéutico. For medicinal products for veterinary use: Ministerio de Agricultura, Pesca y...: Agence du Médicament. For veterinary medicinal products: Agence Nationale du Médicament Vétérinaire..., Dipartimento Farmaci e Farmacovigilanza. For medicinal products for veterinary use: Ministero della...

  14. 21 CFR Appendix B to Subpart A of... - List of Authorities

    Code of Federal Regulations, 2014 CFR

    2014-04-01

    ... Control Farmacéutico. For medicinal products for veterinary use: Ministerio de Agricultura, Pesca y...: Agence du Médicament. For veterinary medicinal products: Agence Nationale du Médicament Vétérinaire..., Dipartimento Farmaci e Farmacovigilanza. For medicinal products for veterinary use: Ministero della...

  15. Unpublished manuscripts of Sophie Germain and a revaluation of her work on Fermat's Last Theorem

    NASA Astrophysics Data System (ADS)

    Del Centina, Andrea

    2008-07-01

    Published, and discussed, are some manuscripts and a letter of Sophie Germain concerning her work on Fermat's Last Theorem. These autographs, held at Bibliothèque Nationale, Paris, at the Moreniana Library, Florence, and at the University Library, Göttingen, contribute to a substantial revaluation of her work on this subject.

  16. Teacher Unionism as Mission and Battle; Success and Crisis in French Teacher Unions.

    ERIC Educational Resources Information Center

    Fowler, Frances C.

    In France, the National Education Federation (Federation d'Education Nationale (FEN)) and its major constituent union, the National Union of Elementary and Middle School Teachers (Syndicat National des Instituteurs et des Professeurs d'Enseignment General de College (SNI-PEGC)), are examples of "intelligent trade unions," i.e., unions that hold a…

  17. Teacher and Administrator Evaluation. Bibliographies in Education. No. 74.

    ERIC Educational Resources Information Center

    Moll, Marita

    This annotated bibliography contains 602 references on teacher and administrator evaluation appearing, between May 1975 and September 1981, in: (1) Bibliographie du Quebec (Bibliotheque nationale du Quebec); (2) British Education Index (British Library); (3) Canadian Books in Print (University of Toronto Press); (4) Canadian Education Index; (5)…

  18. Cultural Dimensions of Digital Library Development, Part I: Theory and Methodological Framework for a Comparative Study of the Cultures of Innovation in Five European National Libraries

    ERIC Educational Resources Information Center

    Dalbello, Marija

    2008-01-01

    This study examines the influence of culture on digital libraries of the first wave. The local cultures of innovation of five European national libraries (Biblioteca nacional de Portugal, Bibliotheque nationale de France, Die Deutsche Bibliothek, the National Library of Scotland, and the British Library) are reconstructed in case histories from…

  19. Computation of low Fronde number turbulent diffusion flames

    NASA Astrophysics Data System (ADS)

    Garreton, D.; Mechitoua, N.; Viollet, P. L.

    This study is related to the development of a model for the computation of pool fires of liquefied natural gas -sponsered by GAZ de FRANCE and SOCIETE NATIONALE d'EXPLORATION d'AQUITAINE-PRODUCTION. -As a first step, low Froude number flames which are similar to pool fires, are simulated.

  20. Langues et education en Afrique noire (Language and Education in Black Africa).

    ERIC Educational Resources Information Center

    Bearth, Thomas, Ed.

    1997-01-01

    Papers on language and education in Black Africa include: "L'enseignement des et en langues nationales au Zaire. Bilan d'une experience" ("The Teaching of and in National Languages in Zaire. Results of an Experiment") (Andre Mbula Paluku); "Langues et education au Rwanda" ("Languages and Education in Rwanda") (Melchior Kanyamibwa); "Un modele…

  1. Teachers' Organizations and Educational Policy: The Case of France

    ERIC Educational Resources Information Center

    Wanner, Raymond E.

    1978-01-01

    Characterizes membership and policy-making role of the largest teachers' organization in France, the Federation de l'Education Nationale. It represents 44 specialized educational unions. It supports the socialist party but has identified itself with the traditional way of administering education in France. (Author/AV)

  2. [Moyse Charas, an apothecary, a physician, as well as the author of "Pharmacopée royale galénique et chymique". The study of his dynasty].

    PubMed

    Warolin, Christian

    2005-01-01

    New research works conducted at the Archives nationales led to the discovery of numerous documents related to Moyse Charas's progeny and made it possible to complete former studies. Presently the filiation of this famous family of Parisians apothecaries of the seventeenth and eighteenth centuries is well established. A family tree has been drawn up. PMID:16217892

  3. International Meeting on Business Start-up (Lille, France, November 26-28, 1992).

    ERIC Educational Resources Information Center

    Melis, Africa, Ed.; Peigne, Florence, Ed.

    1992-01-01

    An international meeting explored work on business start-up undertaken jointly by CEDEFOP (European Centre for the Development of Vocational Training) and France's Agence Nationale pour la creation d'entreprise. One opening presentation (Melis) addressed the basic idea underlying the research: to identify and highlight the role of training and…

  4. IFLA General Conference, 1985. Papers on Bibliographic Control.

    ERIC Educational Resources Information Center

    International Federation of Library Associations, The Hague (Netherlands).

    Papers on bibliographic control which were presented at the 1985 conference of the International Federation of Library Associations (IFLA) include: (1) "Retrospective Bibliographic Control: A Program of Action for UAP (Universal Availability of Publications)" (Marcelle Beaudiquez, Bibliotheque Nationale, France); (2) "The National Union Catalog…

  5. Perrotin et la meilleure mesure française de la vitesse de la lumière

    NASA Astrophysics Data System (ADS)

    Bogaert, G.; Blanc, W.

    2012-12-01

    à la fin du 19ème siècle, la détermination de la vitesse de la lumière a fait l'objet d'une controverse scientifique impliquant d'éminents scientifiques français et américains : Alfred Cornu et Hippolyte Fizeau, d'un côté, Simon Newcomb et Albert Michelson de l'autre. Cette controverse prendra fin de façon inattendue avec les deux mesures réalisées en 1898 et 1902 par Henri Perrotin, le directeur de l'Observatoire de Nice.

  6. Eco-hydrology: Groundwater flow and site factors in plant ecology

    NASA Astrophysics Data System (ADS)

    Klijn, Frans; Witte, Jan-Philip M.

    Résumé En écologie végétale, le site est un concept central. Un site, c'est l'endroit où une espèce végétale ou une communauté de plantes se développe le site assure un ensemble de conditions dans lesquelles elles vivent. Dans un matériau homogène à l'origine, l'écoulement gravitaire d'une nappe influence les conditions du site par l'intermédiaire de la distribution spatiale des nutriments et d'autres composés chimiques associés. Les remontées d'eau peuvent tout spécialement produire et maintenir les conditions du site essentielles pour différentes espèces et communautés de plantes relativement rares. Les écologues ont porté une attention accrue à ces remontées d'eau, en sorte qu'une coopération avec les hydrologues en a résulté, avec l'émergence d'une discipline propre, l'éco-hydrologie, à la limite des deux domaines scientifiques et liée au concept de site. Aux Pays-Bas, une classification des types d'eau, basée sur l'histoire de l'eau souterraine à proximité de la surface, a été mise en oeuvre pour constituer une base nationale de données géographiques sur les remontées d'eau d'intérêt écologique. Des analyses des correspondances des données de cette base, portant sur l'existence de certaines espèces de plantes, montrent que dans les sols sableux pauvres du Pléistocène la remontée d'eau explique très bien la présence de certaines espèces et communautés, alors que, dans les plaines fluviales et les régions de polders à sols argileux riches, l'influence de la remontée d'eau est masquée par l'importance des caractéristiques des sols. En conclusion donc, certaines espèces de plantes peuvent être utilisées comme des indicateurs de la remontée d'eau dans des diagnostiques et des levés de terrain rapides, mais à condition de prendre en permanence des précautions sur les limites de l'approche. Resumen En ecología botánica un concepto de gran importancia es el de emplazamiento, definido como el lugar que

  7. FOREWORD: The 5th International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas

    NASA Astrophysics Data System (ADS)

    Tchang-Brillet, Wad Lydia; Wyart, Jean-François; Zeippen, Claude

    1996-01-01

    and astronomy have a long common history. Indeed, we are reminded that a century ago, terrestrial and solar helium were identified with one another through spectral lines, while recent studies of nebulae and the interstellar medium provide nice examples of the continuing interplay between spectroscopy and astrophysical models. During the Amsterdam meeting, some astrophysicists deplored that the so-called "traditional term analysis" was disappearing. They should be reassured about the near future owing to three invited papers and a great number of posters on this type of work. We are grateful to the members of the Scientific Committee who helped us to set up the scientific programme and to all the referees who reviewed the manuscripts published in this volume. We thank the Observatoire de Paris-Meudon, the Centre National de la Recherche Scientifique and the Centre National d'Etudes Spatiales for financial support. We also thank the Ministère de l'Education Nationale, de l'Enseignement Supérieur, de la Recherche et de l'Insertion Professionnelle, the National Aeronautics and Space Administration and the Laboratoire Aimé Cotton for providing travel grants, Further support from SUN Microsystems, Alcatel and Crédit Lyonnais is gratefully acknowledged. The colloquium greatly benefited from the infrastructure of the Observatoire de Paris-Meudon and the cooperation of its staff, especially members of the Département Atomes, Molécules en Astrophysique (DAMAp). The 6th International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas is scheduled to be held in Victoria, Canada in 1998.

  8. MONA, LISA and VINCI Soon Ready to Travel to Paranal

    NASA Astrophysics Data System (ADS)

    2000-11-01

    of this very complex system. Subsequently, it will serve to tune this key research facility to the highest possible performance. The VLTI is based on the combination of light (beams) from the telescopes at Paranal. Of these, the four 8.2-m Unit Telescopes are already in operation - they will soon be joined by three 1.8-m telescopes that can be relocated on rails, cf. PR Photo 43b/99. By means of a system of mirrors, the light from two or more of these telescopes will be guided to the central Interferometric Laboratory , at the center of the observing platform on Paranal. Information about the heart of this complex system, the Delay Lines that are located in the underground Interferometric Tunnel, is available with the recent ESO PR Photos 26a-e/00. The VLTI will later receive other front-line instruments, e.g. AMBER , MIDI and PRIMA. When fully ready some years from now, the VLTI will produce extremely sharp images. This will have a major impact on different types of exciting astronomical observations, e.g.: * the direct discovery and imaging of extra-solar planets comparable to Jupiter, * the discovery and imaging of low-mass stars such as brown dwarfs, * observations of star-forming regions and to better understand the physical processes that give birth to stars, * spectral analysis of the atmospheres of nearby stars, and * imaging the objects of the very core of our Galaxy and the detection of black holes in active nuclei of galaxies. The VINCI test instrument The new instrument, VINCI , will soon be delivered to Paranal by the Département de Recherche Spatiale (Department for Space Research), a joint unit of the Centre Nationale de la Recherche Scientifique (French National Centre for Scientific Research) and the Paris Observatory. VINCI is a functional copy of the FLUOR instrument - now at the IOTA (Infrared Optical Telescope Array) interferometer - that has been upgraded and adapted to the needs of the VLTI. FLUOR was developed by the Département de Recherche

  9. Relevé postnatal Rourke 2014

    PubMed Central

    Riverin, Bruno; Li, Patricia; Rourke, Leslie; Leduc, Denis; Rourke, James

    2015-01-01

    Résumé Objectif Mettre à jour la version de 2011 du Relevé postnatal Rourke (RPR) à la suite d’une révision des meilleures données probantes récentes sur le suivi de la santé des nourrissons et des enfants de la naissance jusqu’à l’âge de 5 ans. Qualité des données La qualité des données a été cotée en fonction de l’ancien système de classification du Groupe d’étude canadien sur les soins de santé préventifs (jusqu’à 2006) et l’approche de détermination, d’élaboration et d’évaluation des recommandations (GRADE). Message principal De nouveaux faits scientifiques ont été pris en compte dans les recommandations du RPR 2014 en ce qui a trait au suivi de la croissance, à la nutrition, à l’éducation et aux conseils, au développement, à l’examen physique et à l’immunisation. La croissance est surveillée à l’aide des courbes de l’Organisation mondiale de la Santé qui ont été révisées en 2014. On devrait introduire les aliments solides en fonction de l’état de préparation du nourrisson et ces produits devraient contenir du fer. Il n’est actuellement plus recommandé de retarder l’introduction des allergènes alimentaires courants pour prévenir les allergies. Il faut promouvoir l’utilisation d’une tasse sans couvercle au lieu d’une tasse à bec dès l’âge de 12 mois. La section sur l’éducation et les conseils porte sur les blessures causées par du mobilier instable, ainsi que l’utilisation d’un siège d’auto orienté vers l’arrière jusqu’à 2 ans. Elle comporte aussi de l’information sur les saines habitudes de sommeil, la prévention de la maltraitance des enfants, la vie saine et active et la sédentarité de la famille, de même que l’hygiène buccale. On a aussi ajouté à cette section une nouvelle catégorie consacrée à la santé environnementale pour tenir compte des effets des dangers environnementaux sur la santé des enfants. Le RPR a recours à une

  10. The new role of scientists

    ScienceCinema

    None

    2011-04-25

    Le D.G. Jentschke fait l'introduction et présente le Prof.Kowarsky, spécialiste en microbiologie, physique nucléaire et une des fondateurs du Cern. Il parle entre autre de l'énergie nucléaire (pacifique)et de remise en questions des valeurs scientifiques et techniques

  11. Fleischmann seminar (fusion)

    ScienceCinema

    None

    2011-04-25

    "pictures, television out, no flash and camera, there will be a press section later on in the council room if Prof. Fleischmann will accept"..le DG C.Rubbia insiste pour cette discussion scientifique de ne pas filmer, autrement de bien quitter la salle, ce qui provoque un petit remue-ménage...

  12. Post-Secondary Students' Relationship to People They Consider to Be Scientific Experts

    ERIC Educational Resources Information Center

    Pouliot, Chantal

    2011-01-01

    This article is situated in contemporary debates about the ways to achieve a scientific literacy that encourages a greater lay participation in public debates and political decision making. Drawing on the notion of "relationship to scientific experts" (in French, "rapport aux experts scientifiques"), I explore the ways in which a group of 3 Quebec…

  13. Science anc Society

    ScienceCinema

    None

    2011-04-25

    S.P.Worden, membre technique de l'U.S.délégation à Genève pour les négociations sur les armes nucléaires, est physicien, astronome, scientifique et officier de l'armée de l'air. Il parlera des technologies de défense stratégique

  14. Passion Research: A Joint Venture To Interest High School Students in Chemistry.

    ERIC Educational Resources Information Center

    Carriere, Francois J.; Abouaf, Madeleine

    1997-01-01

    Describes a joint venture between the Centre National de la Recherche Scientifique (CNRS) and the Department of Education in France that was created to allow students to do practical scientific work with the help of a CNRS researcher. Presents two practical projects done by students on organic polymers and on color. Concludes that this increases…

  15. Memorial I.Rabi

    ScienceCinema

    None

    2011-04-25

    Le DG H.Schopper ainsi que Norman Ramsey et le DG de l'Unesco rendent hommage à Isidor Rabi, grand scientifique et humaniste (1929-1988).Cette rencontre est organisée ensemble avec le Cern et l'Unesco.

  16. Centenarian Einstein

    ScienceCinema

    None

    2011-04-25

    Commémoration de A.Einstein avec 4 orateurs pour honnorer sa mémoire: le prof.Weisskopf parlera de l'homme de science engagé, Daniel Amati du climat de la physique aux années 1920, Sergio Fubini de l'heure scientifique d'A.Einstein et le prof.Berob(?)

  17. The Economic Aspect of the Exchange of Duplicates. Time Studies on Books. A Case Study.

    ERIC Educational Resources Information Center

    Ejlersen, Rita

    This report of a 10-month study performed at the Institut Danois des Echanges Internationaux de Publications Scientifiques et Litteraires (IDE) on its exchange program for duplicate monographs provides an analysis of the working methods and time spent on the various phases, i.e., acquisition, processing, and distribution. The major function of the…

  18. Colloquy to Paul Musset

    ScienceCinema

    None

    2011-04-25

    En honneur de Paul Musset il a été décidé de faire plutôt un colloque scientifique à la place d'une cérémonie. Plusieurs personnes temoignent de leurs estime et amitié pour ce physicien et ses activités

  19. Memorial I.Rabi

    SciTech Connect

    2006-11-01

    Le DG H.Schopper ainsi que Norman Ramsey et le DG de l'Unesco rendent hommage à Isidor Rabi, grand scientifique et humaniste (1929-1988).Cette rencontre est organisée ensemble avec le Cern et l'Unesco.

  20. Proceedings of the Annual Conference of the International Group for the Psychology of Mathematics Education (13th, Paris, France, July 9-13, 1989), Volume 1.

    ERIC Educational Resources Information Center

    International Group for the Psychology of Mathematics Education.

    This proceedings of the annual conference of the International Group for the Psychology of Mathematics Education (PME) includes the following papers: "Transformations Accelerees de l'Education Scientifique Pendant la Revolution Francaise" (Jean Dhombres); "Building on the Knowledge of Students and Teachers" (Thomas P. Carpenter & Elizabeth…

  1. Documenting and Researching Endangered Languages: The Pangloss Collection

    ERIC Educational Resources Information Center

    Michailovsky, Boyd; Mazaudon, Martine; Michaud, Alexis; Guillaume, Séverine; François, Alexandre; Adamou, Evangelia

    2014-01-01

    The Pangloss Collection is a language archive developed since 1994 at the Langues et Civilisations à Tradition Orale (LACITO) research group of the French Centre National de la Recherche Scientifique (CNRS). It contributes to the documentation and study of the world's languages by providing free access to documents of connected, spontaneous…

  2. Indexation Rules for Metallurgy in PASCAL. Original Title: Regles d'Indexation de la Metallurgie'--Technical Note Issued by Informascience--January 1980. Translated by Marie Wallin.

    ERIC Educational Resources Information Center

    Royal Inst. of Tech., Stockholm (Sweden). Library.

    The indexing rules presented are designed for use with a new French-German database on metallurgy being developed under an agreement by CNRS (Centre National de la Recherche Scientifique, Paris) and BAM (Bundesanstalt fur Materialprufung, Berlin). The new database, which will feature multilingual titles and index terms (French-German-English-) and…

  3. Science on the Fairgrounds: From Black to White Magic

    ERIC Educational Resources Information Center

    Daniel, Raichvarg

    2007-01-01

    During the 18th and 19th centuries, numerous "entrepreneurs de spectacles scientifiques"--a new category of "stall-keepers"--travelled around France, displaying their scientific shows to the public. They turned out to be physics demonstrators, magicians, mechanical engineers or curators of museums of anatomy. A general survey…

  4. Science anc Society

    SciTech Connect

    2006-09-12

    S.P.Worden, membre technique de l'U.S.délégation à Genève pour les négociations sur les armes nucléaires, est physicien, astronome, scientifique et officier de l'armée de l'air. Il parlera des technologies de défense stratégique

  5. Privacy Laws and Biobanking in Germany.

    PubMed

    Hoppe, Nils

    2016-03-01

    While the possibility of enacting a sui generis Biobank Act has been debated in Germany at great length, as of yet the country has not implemented any biobankspecific legislation. Instead, oversight is available via a network of research and privacy laws, including those of the European Union. The Nationale Kohorte, Germany's large-scale, population-based epidemiological research biobank, is funded by the Federal Ministry of Education and Research, and there are currently 108 registered bio-banks throughout Germany. The current system, including the structure and study design of the Nationale Kohorte, privileges the protection of personal information even at the cost of socially desirable research; it remains to be seen if forthcoming legislation will shift this balance. PMID:27256122

  6. [About two unpublished autographs of Louis Pasteur belonging to the Academie national de pharmacie].

    PubMed

    Storck, J

    1997-01-01

    Two unpublished autographs of Louis Pasteur, dated respectively november 26th 1853 and december 22nd 1853 in Strasbourg, were found in unclassified archives of the Academie nationale de pharmacie - Paris. They are described in the paper. They are related to the prize of F 1500 given to him by the Societe de pharmacie, the previous name of the Academy. This award concerned his famous studies on the racemic or paratartric acid. PMID:11625114

  7. Une Exception Francaise: Les Grandes Ecoles (A French Exception: The Great Schools).

    ERIC Educational Resources Information Center

    Kimmel, Alain

    1996-01-01

    Examines the role of exceptional schools in France that have produced famous personages such as Charles de Gaulle and Jean-Paul Sartre. The schools reviewed include L'Ecole Nationale d'Administration, L'Ecole Polytechnique, L'Ecole Normale Superieure, L'Ecole des Hautes Etudes Commerciales, Saint-Cyr, and L'Institut d'Etudes Politiques de Paris.…

  8. Exploratory simulations of multiphase effects in gas injection and ventilation tests in an underground rock laboratory

    SciTech Connect

    Finsterle, S. . Versuchsanstalt fuer Wasserbau, Hydrologie und Glaciologie); Schlueter, E.; Pruess, K. )

    1990-06-01

    This report is one of a series documenting the results of the Nagra-DOE Cooperative (NDC-I) research program in which the cooperating scientists explore the geological, geophysical, hydrological, geochemical, and structural effects was sponsored by the US Department of Energy (DOE) through the Lawrence Berkeley Laboratory (LBL) and the Swiss Nationale Genossenschaft fuer die Lagerung radioaktiver Abfaella (Nagra) and concluded in September 1989. 16 refs., 29 figs., 4 tabs.

  9. Le changement comme tradition dans la recherche et la formation a la recherche en biotechnologie et en peripherie Etude de cas en sciences de la sante, sciences naturelles et genie

    NASA Astrophysics Data System (ADS)

    Bourque, Claude Julie

    Le champ de la recherche scientifique et de la formation a la recherche est traverse depuis quelques dizaines d'annees par plusieurs courants et discours associes au changement, mais peu de travaux empiriques permettent de comprendre ce qui change concretement. C'est la contribution originale de cette these au champ de l'education, plus specifiquement a l'etude sociologique de l'enseignement superieur ou sont concentrees les activites liees a la triade thematique du programme doctoral dans lequel elle a ete produite : recherche, formation et pratique. L'enquete-terrain a ete realisee en 2009 et 2010 aupres de 808 repondants affilies a 60 etablissements au Quebec et a produit un vaste materiau de nature mixte (donnees quantitatives et qualitatives). Un portrait de la nebuleuse biotechnologique qui touche les secteurs des sciences de la sante, des sciences naturelles et du genie a ete realise. Ce domaine concerne des dizaines de disciplines et se revele de nature transdisciplinaire, mais les pratiques n'y sont pas davantage marquees par le changement que celles d'autres domaines connexes. Les dynamiques sociales ont fait l'objet d'analyses comparatives dans quatre contextes: le choix des programmes, des objets et des methodes, le financement, la diffusion et la planification de la carriere. Les resultats indiquent que les echanges entre les agents traditionnellement situes au coeur des activites de recherche dominent ces dynamiques dans tous les contextes etudies. L'etude des representations au fondement des pratiques a revele l'existence de trois ecoles de pensee qui coexistent dans le champ scientifique: academique, pragmatique et economiste. Ces ecoles permettent de categoriser les agents en fonction des zones de fractures qui marquent leurs oppositions tout en identifiant ce qu'ils ont en commun. Les representations et les pratiques liees a la formation temoignent d'un habitus plutot homogene, alors que les contradictions semblent plus souvent ancrees dans des

  10. SIRIUS FEL project

    NASA Astrophysics Data System (ADS)

    Roche, Michel; Moret-Bailly, Jacques

    1991-07-01

    This article presents a 6 MV electrostatic accelerator-driven free electron laser project, with a wavelength range of 80 to 1000 μm. The study of this facility, called SIRIUS (source intense de rayonnement infra-rouge pour utilisations scientifiques), is based on the facility realized by Elias at the University of California, Santa Barbara. We plan to improve some important technological features.

  11. Geoffrey Burbidge : L'art de la critique

    NASA Astrophysics Data System (ADS)

    Bonnet-Bidaud, J. M.

    1997-06-01

    Avec pres de cinquante ans de carriere derriere lui, Geoffrey Burbidge n'a rien perdu de son gout du débat et de la controverse. Mondialement reconnu pour ses travaux sur les quasars, il en agace aujourd'hui plus d'un en venant deranger le bel ordonnancement de la cosmologie. Il porte sur le monde scientifique un regard tres critique, condamnant notamment ces chercheurs qui acceptent trop volontiers d'emprunter les chemins tout traces.

  12. Partager : des technologies de pointe au service de la société

    ScienceCinema

    None

    2011-10-06

    Médecine, climatologie, métrologie et informatique, les techniques utilisées par le LHC trouvent déjà des répercussions dans d?autres domaines scientifiques. Utilisant des techniques inédites, la physique des particules en fait bénéficier la société toute entière.

  13. Torleif Ericson 60th Birthday

    SciTech Connect

    2008-04-09

    Plusieurs discours à l'occasion du 60me anniversaire de Torleif Ericson, physicien né à Lund (Suède), et remerciements pour son travail et son effort de relier la physique des particules à la physique nucléaire. A la fin de la cérémonie un document scientifique de 400 pages "die Festschrift" lui est remis comme cadeau d'anniversaire avec un grand nombre de contributions d'amis etc...

  14. Torleif Ericson 60th Birthday

    ScienceCinema

    None

    2011-04-25

    Plusieurs discours à l'occasion du 60me anniversaire de Torleif Ericson, physicien né à Lund (Suède), et remerciements pour son travail et son effort de relier la physique des particules à la physique nucléaire. A la fin de la cérémonie un document scientifique de 400 pages "die Festschrift" lui est remis comme cadeau d'anniversaire avec un grand nombre de contributions d'amis etc...

  15. Optimierung und Charakterisierung einer transportablen optischen Gitteruhr mit Ytterbium

    NASA Astrophysics Data System (ADS)

    Mura, Gregor

    2015-08-01

    This thesis deals with the improvement and the characterization of a transportable optical lattice clock with ytterbium. Building on results of former theses from T. Franzen [1] and C. Abou Jadoudeh [2] numerous improvements were needed to increase the overall stability of the whole apparatus. The improved stability should lead to a more accurate characterization of the system and a better mobility. Finally, the apparatus should be transported to the Instituto Nationale di Ricerca Metrologica (INRIM) in Torino (Italy) in the course of the Space Optical Clocks 2 (SOC2) project.(Abridged)

  16. EGS Richardson AGU Chapman NVAG3 Conference: Nonlinear Variability in Geophysics: scaling and multifractal processes

    NASA Astrophysics Data System (ADS)

    Schertzer, D.; Lovejoy, S.

    was followed by five days with 8 oral sessions and one poster session. Overall, there were 65 papers involving 74 authors. In general, the main topics covered are reflected in this special issue: geophysical turbulence, clouds and climate, hydrology and solid earth geophysics. In addition to AGU and EGS, the conference was supported by the International Science Foundation, the Centre Nationale de Recherche Scientifique, Meteo-France, the Department of Energy (US), the Commission of European Communities (DG XII), the Comite National Francais pour le Programme Hydrologique International, the Ministere de l'Enseignement Superieur et de la Recherche (France). We thank P. Hubert, Y. Kagan, Ph. Ladoy, A. Lazarev, S.S. Moiseev, R. Pierrehumbert, F. Schmitt and Y. Tessier, for help with the organization of the conference. However special thanks goes to A. Richter and the EGS office, B. Weaver and the AGU without whom this would have been impossible. We also thank the Institut d' Etudes Scientifiques de Cargese whose beautiful site was much appreciated, as well as the Bar des Amis whose ambiance stimulated so many discussions. 2. Tribute to L.F. Richardson With NVAG3, the European geophysical community paid tribute to Lewis Fry Richardson (1881-1953) on the 40th anniversary of his death. Richardson was one of the founding fathers of the idea of scaling and fractality, and his life reflects the European geophysical community and its history in many ways. Although many of Richardson's numerous, outstanding scientific contributions to geophysics have been recognized, perhaps his main contribution concerning the importance of scaling and cascades has still not received the attention it deserves. Richardson was the first not only to suggest numerical integration of the equations of motion of the atmosphere, but also to attempt to do so by hand, during the First World War. This work, as well as a presentation of a broad vision of future developments in the field, appeared in his

  17. Integration des sciences et de la langue: Creation et experimentation d'un modele pedagogique pour ameliorer l'apprentissage des sciences en milieu francophone minoritaire

    NASA Astrophysics Data System (ADS)

    Cormier, Marianne

    Les faibles resultats en sciences des eleves du milieu francophone minoritaire, lors d'epreuves au plan national et international, ont interpelle la recherche de solutions. Cette these avait pour but de creer et d'experimenter un modele pedagogique pour l'enseignement des sciences en milieu linguistique minoritaire. En raison de la presence de divers degres de francite chez la clientele scolaire de ce milieu, plusieurs elements langagiers (l'ecriture, la discussion et la lecture) ont ete integres a l'apprentissage scientifique. Nous avions recommande de commencer le processus d'apprentissage avec des elements langagiers plutot informels (redaction dans un journal, discussions en dyades...) pour progresser vers des activites langagieres plus formelles (redaction de rapports ou d'explications scientifiques). En ce qui a trait a l'apprentissage scientifique, le modele preconisait une demarche d'evolution conceptuelle d'inspiration socio-constructiviste tout en s'appuyant fortement sur l'apprentissage experientiel. Lors de l'experimentation du modele, nous voulions savoir si celui-ci provoquait une evolution conceptuelle chez les eleves, et si, simultanement, le vocabulaire scientifique de ces derniers s'enrichissait. Par ailleurs, nous cherchions a comprendre comment les eleves vivaient leurs apprentissages dans le cadre de ce modele pedagogique. Une classe de cinquieme annee de l'ecole de Grande-Digue, dans le Sud-est du Nouveau-Brunswick, a participe a la mise a l'essai du modele en etudiant les marais sales locaux. Lors d'entrevues initiales, nous avons remarque que les connaissances des eleves au sujet des marais sales etaient limitees. En effet, s'ils etaient conscients que les marais etaient des lieux naturels, ils ne pouvaient pas necessairement les decrire avec precision. Nous avons egalement constate que les eleves utilisaient surtout des mots communs (plantes, oiseaux, insectes) pour decrire le marais. Les resultats obtenus indiquent que les eleves ont

  18. Engaging the Public to Identify Opportunities to Improve Critical Care: A Qualitative Analysis of an Open Community Forum

    PubMed Central

    Potestio, Melissa L.; Boyd, Jamie M.; Bagshaw, Sean M.; Heyland, Daren; Oxland, Peter; Doig, Christopher J.; Zygun, Dave; Stelfox, Henry T.

    2015-01-01

    Objective To engage the public to understand how to improve the care of critically ill patients. Design A qualitative content analysis of an open community forum (Café Scientifique). Setting Public venue in Calgary, Alberta, Canada. Participants Members of the general public including patients, families of patients, health care providers, and members of the community at large. Methods A panel of researchers, decision-makers, and a family member led a Café Scientifique, an informal dialogue between the populace and experts, over three-hours to engage the public to understand how to improve the care of critically ill patients. Conventional qualitative content analysis was used to analyze the data. The inductive analysis occurred in three phases: coding, categorizing, and developing themes. Results Thirty-eight members of the public (former ICU patients, family members of patients, providers, community members) attended. Participants focused the discussion and provided concrete suggestions for improvement around communication (family as surrogate voice, timing of conversations, decision tools) and provider well-being and engagement, as opposed to medical interventions in critical care. Conclusions Café participants believe patient and family centered care is important to ensure high-quality care in the ICU. A Café Scientifique is a valuable forum to engage the public to contribute to priority setting areas for research in critical care, as well as a platform to share lived experience. Research stakeholders including health care organizations, governments, and funding organizations should provide more opportunities for the public to engage in meaningful conversations about how to best improve healthcare. PMID:26580406

  19. Pierre Ambroise-Thomas: a loyal friend and a strong supporter of tropical medicine in Brazil.

    PubMed

    Daniel-Ribeiro, Cláudio Tadeu

    2016-01-01

    Our colleagues at the Sociedade Brasileira de Medicina Tropical have been informed of the demise of Professor Pierre Ambroise-Thomas (1937-2014). However, considering that the tribute we paid to him in 2015 - at the 20th anniversary of the Seminário Laveran & Deane sobre Malária - is equally true today, it is worth sharing it with the readers of the RSBMT, in recognition of his many virtues. Pierre Ambroise-Thomas (MD in 1963 and DSc in 1969) was Honorary Professor of Parasitology and Tropical Medicine at the Faculté de Médecine de Grenoble (France), Honorary President of the Académie Nationale de Médecine, member of the Académie Nationale de Pharmacie and Officier dans l'Ordre de La Légion d'Honneur. In addition to his important contributions to tropical medicine and parasitology, working in France during his long and productive career (50 years and 300 publications), Ambroise-Thomas became an admirer and supporter of Brazilian activities related to research, teaching and information in Tropical Medicine. PMID:27598625

  20. Seminar Andrej Sacharov

    ScienceCinema

    None

    2011-04-25

    A l'occasion de son 63me anniversaire 2 orateurs rendent hommage à A.Sacharov, physicien russe et né à Moscou, pour ses accomplissements scientifiques et son courage. A.Sacharov a dénoncé les dangers de la radioactivité et a tenté de persuader les autorités soviétiques de supprimer une série de test après le developpement de la bombe atomique en 1949 et la bombe à hydrogène en 1953 par un groupe de chercheurs soviétiques. Il a obtenu le prix Nobel en 1975.

  1. Memorial V.J.Glaser

    ScienceCinema

    None

    2011-04-25

    Plusieurs orateurs rendent hommage au grand physicien et scientifique Vladimir Jurko Glaser (1924 - 1984) qui travaillait au Ruder Boscovic Institut à Zagreb avant de venir au Cern en 1957 où il trouvait un poste permanent au département de physique théorique. Walter Tearing, Harry Lehmann,Henry Epstein, Jacques Bros et André Martin font des résumés biographiques de leurs collègue et ami en honorant ses grands qualités d'homme et ses remarquables conquêtes de la science et leurs accomplissement.

  2. What would researchers like to improve in communication initiatives?

    NASA Astrophysics Data System (ADS)

    Russo, Pedro

    2015-08-01

    One of the most important current trends in astronomy communication has been “change”. The field of astronomy communication has rapidly evolved in just the past few years, as new techniques and technologies have been adopted. Research astronomy has also visibly changed, as automation of survey systems and the launch of new telescopes has produced a tsunami of big data sets. Today, scientists and communicators must work together to navigate the raging waters of this data flood as they strive to keep our tech-savvy society informed. This invited talk will be given by Alain Doressoundiram (Observatoire de Paris, Centre National de la Recherche Scientifique, France) TBC

  3. Identification of complex flows in Taylor-Couette counter-rotating cavities

    NASA Technical Reports Server (NTRS)

    Czarny, O.; Serre, E.; Bontoux, P.; Lueptow, R. M.

    2001-01-01

    The transition in confined rotating flows is a topical problem with many industrial and fundamental applications. The purpose of this study is to investigate the Taylor-Couette flow in a finite-length cavity with counter-rotating walls, for two aspect ratios L=5 or L=6. Two complex regimes of wavy vortex and spirals are emphasized for the first time via direct numerical simulation, by using a three-dimensional spectral method. The spatio-temporal behavior of the solutions is analyzed and compared to the few data actually available. c2001 Academie des sciences/Editions scientifiques et medicales Elsevier SAS.

  4. The entropy and stability of the universe

    NASA Astrophysics Data System (ADS)

    Gibbons, G. W.

    It is shown that among all universes admitting a moment of time symmetry, the Einstein static universe is an extremum (the only homogeneous one) and that this extremum is a local maximum against conformal changes if and only if the solution is stable against the Jeans instability or equivalently if the sound speed exceeds √1/5. Laboratoire Propre du Centre National de Recherche Scientifique, associé à l'Ecole Normale Supérieure et à l'Université de Paris-Sud.

  5. Toxoplasmose oculaire atypique chez une femme congolaise de 72 ans: à propos d'une observation

    PubMed Central

    Bienvenu, Yogolelo Asani; Angel, Musau Nkola; Eric, Kasamba Ilunga; Socrate, Kapalu Mwangala; Sebastien, Mbuyi Musanzayi; Philippe, Cilundika Mulenga; Leon, Kabamba Ngombe; Bruno, Iye Ombamba Kayimba; Gaby, Chenge Borasisi

    2015-01-01

    Les auteurs rapportent un cas de toxoplasmose oculaire binoculaire, rarement décrit dans la littérature, chez une personne âgée de 72 ans, de sexe féminin, à laquelle s'associe une rétinite pigmentaire unilatérale. Cette observation permet d'attirer l'attention de la communauté scientifique sur les autres formes ou variétés de présentation moins courantes, « atypiques », pouvant être rencontrées ou associées à la toxoplasmose oculaire. PMID:26958130

  6. Strong wind structure near a sea-land roughness discontinuity

    NASA Astrophysics Data System (ADS)

    Sacré, C.

    1981-08-01

    During the winters of 1977 and 1978, the Centre Scientifique et Technique du Bâtiment (CSTB) carried out a study on the Atlantic littoral in order to determine the modifications to which an air flow is subjected in the surface boundary layer, as it crosses a sea-land discontinuity. The study shows that, in the zone directly leeward of the shore, the structure of the flow is strongly influenced by the acceleration effect of the dune and by the magnitude of the land roughness. In particular, there is a significant disturbance of the ‘logarithmic’ equilibrium of the air flow.

  7. Multiplicity distributions up to √s = 540 GeV in the dual parton model

    NASA Astrophysics Data System (ADS)

    Capella, A.; Tran Thanh van, J.

    1982-08-01

    We compute the average charge multiplicities and dispersions in proton-proton and antiproton-proton interactions up to SPS collider energies in the framework of a multi-chain dual parton model. The corresponding data for deep inelastic lepton-proton and e+e- reactions are used as the sole input. The height of the central plateau is also computed. Laboratoire associé au Centre National de la Recherche Scientifique. Postal address: Bâtiment 211, Université Paris-Sud 91405 Orsay, France.

  8. Seminar Andrej Sacharov

    SciTech Connect

    2006-08-23

    A l'occasion de son 63me anniversaire 2 orateurs rendent hommage à A.Sacharov, physicien russe et né à Moscou, pour ses accomplissements scientifiques et son courage. A.Sacharov a dénoncé les dangers de la radioactivité et a tenté de persuader les autorités soviétiques de supprimer une série de test après le developpement de la bombe atomique en 1949 et la bombe à hydrogène en 1953 par un groupe de chercheurs soviétiques. Il a obtenu le prix Nobel en 1975.

  9. Hans Bethe : Des etoiles a la bombe

    NASA Astrophysics Data System (ADS)

    Bonnet-Bidaud, J. M.

    1996-06-01

    Il comprit le premier comment brillent les etoiles. Il fut aussi de cette poignee de scientifiques qui, dans le secret de Los Alamos, mirent au point la tristement celebre bombe atomique. Hans Bethe est l'un des derniers geants qui auront marque la physique de ce siecle d'une empreinte indelebile. C'est dans le bureau 01 du prestigieux laboratoire Kellog de l'institut Caltech qu'il a bien voulu retracer pour nous son impressionnante carriere, et revenir sur les motivations qui ont guide ses pas.

  10. CASSIS: Interactive spectrum analyzer

    NASA Astrophysics Data System (ADS)

    Cassis Team At Cesr/Irap

    2014-02-01

    CASSIS (Centre d'Analyse Scientifique de Spectres Infrarouges et Submillimetriques), written in Java, is suited for broad-band spectral surveys to speed up the scientific analysis of high spectral resolution observations. It uses a local spectroscopic database made of the two molecular spectroscopic databases JPL and CDMS, as well as the atomic spectroscopic database NIST. Its tools include a LTE model and the RADEX model connected to the LAMDA molecular collisional database. CASSIS can build a line list fitting the various transitions of a given species and to directly produce rotational diagrams from these lists. CASSIS is fully integrated into HIPE, the Herschel Interactive Processing Environment, as a plug-in.

  11. [SIGAPS: a software package for the evaluation of medical publications].

    PubMed

    Derancourt, C; Devos, P; Moore, N; Rouvillain, J-L

    2014-01-01

    The "système d'interrogation, de gestion et d'analyse des publications scientifiques" (System for Identification, Management and Analysis of Scientific Publications), or SIGAPS, is an innovative tool of French design that enables the identification and analysis of bibliographic references produced by a given researcher or unit using the Medline database (PubMed). This evaluation takes into account the author's rank of signature and the impact factor of the journal of publication within the discipline in question. The limits are those of the impact factor. Analyses produced by SIGAPS enable financial assessment to be made by hospitals. PMID:25209819

  12. Electric-field control of spin waves in multiferroic BiFeO3: Theory

    NASA Astrophysics Data System (ADS)

    de Sousa, Rogério; Rovillain, P.; Gallais, Y.; Sacuto, A.; Méasson, M. A.; Colson, D.; Forget, A.; Bibes, M.; Barthélémy, A.; Cazayous, M.

    2011-03-01

    Our recent experiment demonstrated gigantic (30%) electric-field tuning of magnon frequencies in multiferroic BiFeO3. We demonstrate that the origin of this effect is related to two linear magnetoelectric interactions that couple the component of electric field perpendicular to the ferroelectric vector to a quadratic form of the Néel vector. We calculate the magnon spectra due to each of these interactions and show that only one of them is consistent with experimental data. At high electric fields, this interaction induces a phase transition to a homogeneous state, and the multi-magnon spectra will fuse into two magnon frequencies. We discuss the possible microscopic mechanisms responsible for this novel interaction and the prospect for applications in magnonics. We acknowledge support from NSERC-Discovery (Canada) and the Agence Nationale pour la Recherche (France).

  13. Liquid catalyst efficiently removes H/sub 2/S from liquid sulfur

    SciTech Connect

    Nougayrede, J.; Voirin, R. )

    1989-07-17

    Efficient removal of H/sub 2/S from liquid sulfur can be accomplished by the use of a new liquid catalyst developed by Societe Nationale Elf Aquitaine (Production). Designated Aquisulf, the catalyst is used in the sulfur-degassing process the same way ammonia was previously used. H/sub 2/S can, of course, be deadly and the safe handling and shipping of elemental sulfur containing it is a challenge. Before degassing, elemental sulfur, for which the 1987 worldwide demand was about 20 million metric tons, can contain up to 100 ppm H/sub 2/S in Frasch-mined sulfur, and up to 550 ppm in sulfur produced by Claus sulfur recovery processes in refineries and gas processing plants. Lower catalyst quantities needed to achieve specified maximum H/sub 2/S levels in the liquid sulfur product, better sulfur quality, and lower system maintenance costs are the primary advantages provided by the new catalyst.

  14. The European "clinical trial" regulation; relationship with the Jardé Act: a Giens workshop.

    PubMed

    Lemaire, François; Marchenay, Brigitte; Chassany, Olivier; Barthélémy, Philippe; Bouzzagou, Mohamed; Comet, Denis; Delval, Cécile; Dubray, Claude; Fouret, Cécile; Frija-Orvoen, Elisabeth; Gambotti, Laetitia; Lamarque, Véronique; d'Orsay, Geneviève; Plattner, Valérie; Sibenaler, Claire; Roux, Jacques; Thoby, Frédérique

    2015-01-01

    In May 2014, the European Union Parliament and Council published a new regulation on clinical trials on medicinal products for human use, which is designed to replace Directive 2001/20/EC. It will not come into effect until 2016. Nevertheless, it is essential to examine its relationship with national legislation, i.e. the Jardé Act, whose implementation has been delayed pending publication of the European regulation. The Giens workshop identified and examined the various issues that this relationship is bound to raise. In particular, it looked at trial methodology assessment procedures, the working relationship between the French National Agency of Drug Safety and Health Products (Agence Nationale de Sécurité du Médicament et des Produits de Santé, ANSM) and ethics committees during the authorization application evaluation phase, review of post-authorization/registration studies on medicinal products and medical devices, and data transparency. PMID:25679191

  15. Shielding ultracold dipolar molecular collisions with electric fields

    NASA Astrophysics Data System (ADS)

    Quéméner, Goulven; Bohn, John

    2016-05-01

    The prospect for shielding ultracold dipolar molecules from inelastic and reactive collisions is investigated. Molecules placed in their first rotationally excited states are found to exhibit effective long-range repulsion for applied electric fields above a certain critical value. This repulsion can safely allow the molecules to scatter while reducing the risk of inelastic or chemically reactive collisions. Several molecular species of molecules of experimental interest such as NaRb, NaK, RbSr, SrF, BaF, and YO, are considered and all are shown to exhibit orders of magnitude suppression in quenching rates in a sufficiently strong laboratory electric field. We acknowledge the financial support of the COPOMOL project (ANR-13-IS04-0004) from Agence Nationale de la Recherche and the ARO MURI Grant No. W911NF-12-1-0476.

  16. Investigation of the mobile granular layer in bed-load transport

    NASA Astrophysics Data System (ADS)

    Guazzelli, Elisabeth; Aussillous, Pascale; Chauchat, Julien; Pailha, Mickael; Medale, Marc; Aix Marseille Université, Cnrs, Iusti Umr 7343 Team; Legi, Ujf/Inpg/Cnrs Team; Locie, Cnrs-Université de Savoie Team

    2012-11-01

    The mobile layer of a granular bed composed of spherical particles is experimentally investigated in a laminar rectangular-channel flow. Both particle and fluid velocity profiles are obtained using particle image velocimetry for different index-matched combinations of particles and fluid. While the Shields number controls incipient motion, it is not the most appropriate parameter for describing bed-load transport. The experimental observations suggest that the appropriate length-scale is the fluid height and that the proper control parameter is the dimensionless fluid flow-rate. A two-phase continuum model having a frictional rheology to describe particle-particle interactions can capture most of the experimental observations. Rheological constitutive laws having increasing degree of sophistication are discussed. Funding from Agence Nationale de la Recherche (Project Dunes ANR-07-3 18-3892) is gratefully acknowledged.

  17. The UT 8 February 2013 Sila-Nunam Mutual Event & Future Predictions

    NASA Astrophysics Data System (ADS)

    Benecchi, Susan D.; Noll, K.; Thirouin, A.; Ryan, E.; Grundy, W.; Verbiscer, A.; Doressoundiram, A.; Hestroffer, D.; Beaton, R.; Rabinowitz, D.; Chanover, N.

    2013-10-01

    A mutual event of the Kuiper Belt binary system (79360) Sila-Nunam was observed over 15.47 hours on UT 8 February 2013 by a coordinated effort at four telescopes: Telescopio Nationale Galileo in the Canary Islands, the du Pont telescope at Las Campanas Observatory, ARC at Apache Point Observatory and the IRTF on Mauna Kea. It is the first full event observed from start to finish for this binary system. The lightcurve is consistent with two objects of similar, but perhaps not identical, size and albedo. We will present the results from this event and predictions for future events which have been refined by this and other mutual event observations obtained since the events began.

  18. Ultracold two-body dynamics in optical lattices with topological singularities

    NASA Astrophysics Data System (ADS)

    Aghamalyan, Davit; Simoni, Andrea; Launay, Jean-Michel

    2016-05-01

    We study bound levels of two particles trapped in a 2D optical lattice. We use a short-range potential tuned to reproduce typical experimental conditions. Near-threshold bound states are computed using a spectral element discretization approach that guarantees exponential precision in the numerical results. High computational efficiency is attained due to the very sparse nature of the Hamiltonian in this representation. The calculated wavefunction is analyzed both in real and in momentum space. We perform calculations both for standard separable optical potentials and for lattice with topological singularities (Dirac cones) in the band structure. Extension to the calculation of scattering states will be addressed. This work was supported by the Agence Nationale de la Recherche (Contract No. ANR-12-BS04-0020-01).

  19. [National ethics committees and representative democracy: is the new German ethics committee more "democratic"?].

    PubMed

    Dagron, Stéphanie

    2007-01-01

    The bill passed in April 2007 by the German parliament aims to confer democratic legitimacy on the German Ethics Committee (deutscher Ethikrat) which has replaced the former National Ethics Committee (nationaler Ethikrat) set up in 2001. This law results from a wide debate which began in 2005 within the political parties about the role in democracy of the bodies charged with advising the people's representatives in the areas of biotechnology and modern medicine. In this article, the author explains why it was necessary to confer a certain democratic legitimacy on the new Ethics Committee and analyses the relation that exists between the democratic principle, the work of this type of committee and the national institutional structure retained to stimulate the debate and advise the political decision-makers, and even to prepare legislation concerning bioethics. PMID:17902580

  20. Remote system for subsea wells tested

    SciTech Connect

    Vielvoye, R.

    1981-05-04

    At its experimental submarine station in the Grondin field offshore the West African state of Gabon, Societe Nationale Elf-Aquitaine has run a series of inspection, repair, and maintenance tests on two producing wells using a robot controlled from the surface. Designed for water depths beyond the range of divers, the TIM robot has a pair of manipulator arms and a rotating telescopic crane installed on a 14 by 7.6 ft carriage. Five television cameras fitted at various spots on the robot allow surface operators to direct TIM in such tasks as (1) installing a jumper pipe between a Christmas tree and the manifold, (2) connecting a jumper electric cable and hydraulic hose, (3) locally operating a safety valve, and (4) removing a guide line. During 104 hr of seabed experience, TIM outperformed divers, particularly in jobs requiring great strength.

  1. [Grading of soft tissue and bone sarcomas].

    PubMed

    Petersen, I; Wardelmann, E

    2016-07-01

    Malignancy grading is an essential element in the classification of sarcomas. It correlates with the prognosis of the disease and the risk of metastasis. This article presents the grading schemes for soft tissue, bone and pediatric sarcomas. It summarizes the histological criteria of the Federation Nationale des Centres de Lutte Contre le Cancer (FNCLCC) system and the Pediatric Oncology Group as well as the grading of bone tumors by the College of American Pathologists (CAP). Furthermore, the potential relevance of gene expression signatures, the complexity index in sarcoma (CINSARC) and single genetic alterations (p53, MDM2, p16, SWI/SNF, EWSR1 fusions and PAX3/PAX7-FOXO1 fusions) for the prognosis of sarcomas are discussed. PMID:27384333

  2. Guidelines for the treatment of hemorrhoids (short report).

    PubMed

    Higuero, T; Abramowitz, L; Castinel, A; Fathallah, N; Hemery, P; Laclotte Duhoux, C; Pigot, F; Pillant-Le Moult, H; Senéjoux, A; Siproudhis, L; Staumont, G; Suduca, J M; Vinson-Bonnet, B

    2016-06-01

    Hemorrhoids are a common medical problem that is often considered as benign. The French Society of Colo-Proctology (Société nationale française de colo-proctologie [SNFCP]) recently revised its recommendations for the management of hemorrhoids (last issued in 2001), based on the literature and consensual expert opinion. We present a short report of these recommendations. Briefly, medical treatment, including dietary fiber, should always be proposed in first intention and instrumental treatment only if medical treatment fails, except in grade ≥III prolapse. Surgery should be the last resort, and the patient well informed of the surgical alternatives, including the possibility of elective ambulatory surgery, if appropriate. Postoperative pain should be prevented by the systematic implementation of a pudendal block and multimodal use of analgesics. PMID:27209079

  3. The Nagra-DOE Cooperative Project

    SciTech Connect

    Long, J.C.S.; Levitch, R.A.; Zuidema, P.

    1993-04-01

    The Nagra-DOE Cooperative (NDC-I) research program was sponsored by the US Department of Energy (DOE) through the Lawrence Berkeley Laboratory (LBL), and the Swiss Nationale Genossenschaft fuer die Lagerung radioaktiver Abfaella (Nagra). Scientists participating in this project explored the geological, geophysical, hydrological, geochemical, and structural effects anticipated from the use of a rock mass as a geologic repository for nuclear waste. Six joint tasks were defined and are described briefly below. Tasks 1, 2, 3 and 5 were concerned with the characterization of fractured rock. Task 5 in particular was focused on investigations at the Grimsel Underground Laboratory in the Swiss Alps. Tasks 2 and 6 focused on the phenomenology associated with storing radioactive waste underground.

  4. Spontaneous actin dynamics in contractile rings

    NASA Astrophysics Data System (ADS)

    Kruse, Karsten; Wollrab, Viktoria; Thiagarajan, Raghavan; Wald, Anne; Riveline, Daniel

    Networks of polymerizing actin filaments are known to be capable to self-organize into a variety of structures. For example, spontaneous actin polymerization waves have been observed in living cells in a number of circumstances, notably, in crawling neutrophils and slime molds. During later stages of cell division, they can also spontaneously form a contractile ring that will eventually cleave the cell into two daughter cells. We present a framework for describing networks of polymerizing actin filaments, where assembly is regulated by various proteins. It can also include the effects of molecular motors. We show that the molecular processes driven by these proteins can generate various structures that have been observed in contractile rings of fission yeast and mammalian cells. We discuss a possible functional role of each of these patterns. The work was supported by Agence Nationale de la Recherche, France, (ANR-10-LABX-0030-INRT) and by Deutsche Forschungsgemeinschaft through SFB1027.

  5. From dipolar to multipolar interactions between ultracold Feshbach molecules

    NASA Astrophysics Data System (ADS)

    Quéméner, Goulven; Lepers, Maxence; Luc-Koenig, Eliane; Dulieu, Olivier

    2016-05-01

    Using the multipolar expansion of electrostatic and magnetostatic potential energies, we characterize the long-range interactions between two weakly-bound diatomic molecules, taking as an example the paramagnetic Er2 Feshbach molecules which were produced recently. The interaction between atomic magnetic dipoles gives rise to the usual R-3 leading term of the multipolar expansion, where R is the intermolecular distance. We show that additional terms scaling as R-5, R-7 and so on also appear, which are strongly anisotropic with respect to the orientation of the molecules. These terms can be seen as effective molecular multipole moments reflecting the spatial extension of the molecules which is non-negligible compared to R. We acknowledge the financial support of the COPOMOL project (ANR-13-IS04-0004) from Agence Nationale de la Recherche.

  6. Elf's 20-year experience confirms effectiveness of smart pigs

    SciTech Connect

    Roche, M.; Samaran, J.P. )

    1992-11-30

    Societe Nationale Elf Aquitaine has acquired more than 20 years' experience with in-line inspection of pipelines, using tools from seven service companies. The first in-line inspection operation carried out by one of the companies affiliated with Elf Aquitaine occurred in 1971 and used a Linalog tool. This inspection was to evaluate the extent of external corrosion attacks at the bottom of a 24-in. OD, 69-km uncoated pipeline laid directly on the ground in a desert area. Later periodic inspections, performed in 1980 and 1987 on the main pipeline, detected important external corrosions in some salty areas. These attacks occurred beneath disbondments of the over the ditch-applied bituminous enamel coating. Inspections also detected internal corrosion produced by accumulation of water at low points as a result of intermittent reductions of flow velocity and even to some flow stoppages. This paper reports on service inspection in the use of pigs.

  7. Molecular spectroscopy for producing ultracold ground-state NaRb molecules

    NASA Astrophysics Data System (ADS)

    Wang, Dajun; Guo, Mingyang; Zhu, Bing; Lu, Bo; Ye, Xin; Wang, Fudong; Vexiau, Romain; Bouloufa-Maafa, Nadia; Quéméner, Goulven; Dulieu, Olivier

    2016-05-01

    Recently, we have successfully created an ultracold sample of absolute ground-state NaRb molecules by two-photon Raman transfer of weakly bound Feshbach molecules. Here we will present the detailed spectroscopic investigations on both the excited and the rovibrational ground states for finding the two-photon path. For the excited state, we focus on the A1Σ+ /b3 Π singlet and triplet admixture. We discovered an anomalously strong coupling between the Ω =0+ and 0- components which renders efficient population transfer possible. In the ground state, the pure nuclear hyperfine levels have been clearly resolved, which allows us to create molecules in the absolute ground state directly with Raman transfer. This work is jointly supported by Agence Nationale de la Recherche (#ANR-13- IS04-0004-01) and Hong Kong Research Grant Council (#A-CUHK403/13) through the COPOMOL project.

  8. How was the UNAIDS drug access initiative implemented in Chile?

    PubMed Central

    Brousselle, Astrid; Champagne, François

    2012-01-01

    In 1997, UNAIDS decided to implement Drug Access Initiatives (DAI) in four different pilot-countries. We studied the implementation of the DAI in Chile as part of the evaluation program conducted by the ‘Agence Nationale de Recherche sur le SIDA’ (ANRS/France). The objective was to understand how the politico-organizational dynamic influenced the implementation process of the DAI. Approximately 50 semi-directed interviews and observation activities were conducted with the actors who participated in the implementation of the DAI or who played a role in the HIV/AIDS context. The program theory models were established and their evolution analyzed. This article offers an original analysis of an international HIV/AIDS drug access program that was put in place at a time when such programs were seen as a priority by international and governmental institutions. It also offers some insights for the creation of international projects that will be locally implemented. PMID:23230344

  9. Role of Van der Waals interactions in determining the structure of liquid tellurides

    NASA Astrophysics Data System (ADS)

    Micoulaut, Matthieu; Flores-Ruiz, Hugo; Coulet, Vanessa; Piarristeguy, Andrea; Johnson, Mark; Cuello, Gabriel; Pradel, Annie

    The simulation of tellurides using standard density functional (DFT) theory based molecular dynamics usually leads to an overestimation of the bond distances and a noticeable mismatch between theory and experiments when e.g. structure functions are being directly compared. Here, the structural properties of several compositions of Ge-Te and Ge-Sb-Te liquids are studied from a combination of neutron diffraction and DFT-based molecular dynamics. Importantly, we find an excellent agreement in the reproduction of the structure in real and reciprocal spaces, resulting from the incorporation of dispersion forces in the simulation. We then investigate structural properties including structure factors, pair distribution functions, angular distributions, coordination numbers, neighbor distributions, and compare our results with experimental findings. References:Physical Review B 92, 134205 (2015)Physical Review B 89, 174205 (2014)Physical Review B 90, 094207 (2014) Support from Agence Nationale de la Recherche (ANR) (Grant No. ANR-11-BS08-0012) is gratefully acknowledged.

  10. La supraconductivité a 100 ans !

    ScienceCinema

    None

    2011-10-06

    Il y a 100 ans, le 8 avril 1911, une découverte majeure était réalisée : celle de la supraconductivité. La supraconductivité est la caractéristique qu?ont certains métaux et alliages de perdre toute résistance électrique en dessous d?une température donnée. Cette renversante découverte, réalisée de manière presque fortuite par Kammerlingh Onnes de l?Université de Leyde (Pays-Bas) et son étudiant Gilles Holst, a ouvert un nouveau champ de recherche en physique et de fabuleuses perspectives d?applications technologiques. Du point de vue scientifique, la supraconductivité est en effet l?une des rares manifestations de la physique quantique à l?échelle macroscopique.  Du point de vue des retombées techniques, elle est porteuse d?applications majeures dans le domaine de la santé, des communications et de l?énergie. 100 ans après, les physiciens n?ont toujours pas fini d?explorer ce phénomène et ses applications. Le CERN abrite des applications de la supraconductivité à des échelles inédites. L?accélérateur de particules LHC, avec ses milliers d?aimants supraconducteurs répartis sur 27 kilomètres de circonférence, est en effet la plus grande application mondiale de la supraconductivité. Il ne pourrait exister sans elle.  Le CERN fête donc la découverte de la supraconductivité avec une conférence exceptionnelle donnée par Philippe Lebrun. Au cours de cette conférence, l?expérience historique de Kammerlingh Onnes sera reproduite. Philippe Lebrun racontera l?histoire de cette étonnante découverte, en la replaçant dans le contexte scientifique de l?époque. Il racontera les développements scientifiques et les applications du premier siècle de la supraconductivité. Conférence en français Merci de bien vouloir vous inscrire au : +41 22 767 76 76 ou cern.reception@cern.ch

  11. The new powder diffractometer D1B of the Institut Laue Langevin

    NASA Astrophysics Data System (ADS)

    Puente Orench, I.; Clergeau, J. F.; Martínez, S.; Olmos, M.; Fabelo, O.; Campo, J.

    2014-11-01

    D1B is a medium resolution high flux powder diffractometer located at the Institut Laue Langevin, ILL. D1B a suitable instrument for studying a large variety of polycrystalline materials. D1B runs since 1998 as a CRG (collaborating research group) instrument, being exploited by the CNRS (Centre National de la Recherche Scientifique, France) and CSIC (Consejo Superior de Investigaciones Cientificas, Spain). In 2008 the Spanish CRG started an updating program which included a new detector and a radial oscillating collimator (ROC). The detector, which has a sensitive height of 100mm, covers an angular range of 128°. Its 1280 gold wires provide a neutron detection point every 0.1°. The ROC is made of 198 gadolinium- based absorbing collimation blades, regular placed every 0.67°. Here the present characteristics of D1B are reviewed and the different experimental performances will be presented.

  12. Development of the APEX experiment, preparatory activities for an airborne system supporting future space-borne imaging spectrometers in Europe

    NASA Astrophysics Data System (ADS)

    Schaepman, M.

    2002-06-01

    APEX is an airborne imaging spectrometer built in the framework of ESA PRODEX (Programme développement d'expériences scientifiques) with the support of ESA EO-EP. It is based on a Swiss/Belgian initiative and designed to be an airborne simulator for the support and development of future spaceborne systems for the study of land surface processes. It will be able to contribute to the simulation, calibration, and validation of planned ESA imaging spectrometer missions (e.g., MERIS/ENVISAT, SPECTRA, etc.) in the 400 - 2500 nm region of the spectrum. APEX will foster the use of imaging spectrometer data in Europe and will support the application development for imaging spectroscopy products. The industrial consortium building the instrument is composed out of joint Swiss/Belgian industries with the support of ESA EO-EP (e.g., detectors, calibration, technical management).

  13. SO(4)-->SU(2)R global symmetry properties of six-dimensional grand-unified theories

    NASA Astrophysics Data System (ADS)

    Fayet, P.

    1987-07-01

    We exhibit a global SU(2)×SU(2)'~SO(4) invariance of six-dimensional supersymmetric GUTs. After the elctroweak breaking, this invariance gets reduced to an SU(2)R subgroup which extends the U(1) R-invariance of 6D theories and acts on the single 6D Weyl supersymmetry generator. Gauge bosons, leptons and quarks are SU(2)R isosinglets; inos, sleptons and squarks isodoublets; and Higgs bosons, generally isotriplets. The W+/- and Z masses appear, in six dimensions, as an effect of the breaking of this global SO(4) symmetry. This may provide a reason for the extremely small value of the ration mw/mGUT. The residual SU(2)R symmetry may then be used to trigger the supersymmetry breaking in four dimensions. Laboratoire Propre du Centre National de la Recherche Scientifique, associé à l'Ecole Normale Supériure et à l'Université de Paris Sud.

  14. Astronomie et chronoligie chez Newton - arguments astronomiques à l'appui de la chronologie de Newton (Astronomical arguments in Newton's Chronology)

    NASA Astrophysics Data System (ADS)

    Nazé, Yaël

    2012-12-01

    In his Chronology, Newton uses astronomical "evidence" to support its extreme rejuvenation of ancient times. These elements, having a scientific varnish, provide some credibility to the work. They have been fiercely debated for a century, with a gradual undermining of Newton's assumptions. However, this has not dented the prestige of the English scientist. Dans sa Chronologie, Newton utilise des "preuves" astronomiques pour appuyer son rajeunissement extreme des epoques anciennes. Ces elements, au vernis scientifique, donnent une credibilite certaine a l'ensemble. Ils ont donc ete aprement discutes, les debats sapant petit a petit les hypotheses du savant anglais pour finalement porter un coup mortel a l'ensemble. Cela n'a toutefois pas entame le prestige du savant anglais.

  15. Georges Lemaître and Stigler's Law of Eponymy

    NASA Astrophysics Data System (ADS)

    Block, David L.

    One of the greatest discoveries of modern times is that of the expanding Universe, almost invariably attributed to Hubble (Proceedings of the National Academy of Sciences of the United States of America 15:168, 1929). What is not widely known is that the original treatise by Lemaître (Annales de la Société Scientifique de Bruxelles, Sèrie A 47:49, 1927) contained a rich fusion of both theory and of observation. The French paper was meticulously censored when published in English: all discussions of radial velocities and distances, and the very first empirical determination of H 0 , were suppressed. Stigler's law of eponymy is yet again affirmed: no scientific discovery is named after its original discoverer (Merton, American Sociological Review 22(6):635, 1957). An appeal is made for a Lemaître Telescope naming opportunity, to honour the discoverer of the expanding universe.

  16. A maximally symmetric no-scale inflationary universe

    NASA Astrophysics Data System (ADS)

    Kounnas, C.; Quiros, M.

    1985-02-01

    We present an inflationary model, based on maximally symmetric no-scale supergravity models, where the gravitino and inflation scale cosmological problems are solved simultaneously by means of a heavy - but weakly coupled to ordinary matter - gravitino. The gravitino mass is essentially given by the Hubble constant at the inflationary epoch, H≅1012 GeV. The reheating temperature of the universe after inflation is TR≅(1010-1011) GeV and so gravitinos are no longer regenerated. The grand unified theory suffers a rapid phase transition into the SU(3)×SU(2)×U(1) phase, during - or at the end of - inflation with dilution of magnetic monopoles. The dynamical determination of the electroweak scale predicts top quark masses between 40 and 50 GeV. Laboratoire Propre du Centre National de la Recherche Scientifique, associé à l'Ecole Normale Supérieure et à l'Université de Paris-Sud.

  17. Flux limits for high energy cosmic photinos from underground experiments

    NASA Astrophysics Data System (ADS)

    Fayet, P.

    1989-03-01

    Underground experiments, which detect the interactions of atmospheric neutrinos, could also be sensitive to photinos. Using data from the Fréjus and Kamiokande detectors we give upper limits on the possible flux of high-energy relativistic photinos incident on the Earth, as functions of the squark or selectron masses. These limits improve considerably the existing ones, by four to nine orders of magnitude or more, especially for very energetic photinos. Although not yet very constraining, they may be used to eliminate the possibility that high-energy cosmic photinos could contribute significantly to the energy density of the Universe. Laboratoire Propre du Centre National de la Recherche Scientifique, associé à l'École Normale Supérieure et à l'Université de Paris-Sud.

  18. Challenges to reestablishment of free-ranging populations of black-footed ferrets

    USGS Publications Warehouse

    Biggins, D.E.; Godbey, J.L.

    2003-01-01

    The black-footed ferret (Mustela nigripes) of North America is critically endangered due in part to its extreme specialization on formerly stable and abundant prairie dogs (Cynomys). Its close relative, the Siberian polecat (M. eversmannii) seems to have been subjected to a varying environment that was not conducive to specialization. One source of environmental variation in Asian steppes was plague (caused by Yersina pestis), which was absent from North America. Introduction of plague to North America presents serious challenges to ferret recovery. Partial solutions to other biological and political problems have been found, resulting in improved production in captivity, increased survival post-release, and thriving populations in plague-free South Dakota. ?? 2003 Acade??mie des sciences. Published by E??ditions scientifiques et me??dicales Elsevier SAS. All rights reserved.

  19. Snow fences on slopes at high wind speed: physical modelling in the CSTB cold wind tunnel

    NASA Astrophysics Data System (ADS)

    Naaim-Bouvet, F.; Naaim, M.; Michaux, J.-L.

    In order to determine the effect of steep slopes on snowdrift generated by snow fences, we have conducted physical modeling experiments in the CSTB (Centre Scientifique et Technique du Bâtiment) cold wind tunnel as part of the European project "Access to Large Facilities". After an overview of previous studies and an accurate description of the drifting snow process inside the experimental chamber, we present the main results obtained. (1) On flat areas, even for high wind speed, the acknowledged results for moderate wind are still valid: the porous snow fence (50%) is the most efficacious and the bottom gap increases the efficacy of the dense snow fence. (2) The steeper the slope is, the less effective all tested snow fences are. Their effectiveness decreases considerably: the snow catch is approximately divided by two for a slope of 10°. (3) Contrary to flat areas, on steep slopes, the "efficacy" is greater for a dense snow fence.

  20. The career paths of women (and men) in French research.

    PubMed

    de Cheveigné, Suzanne

    2009-02-01

    This paper presents results from a qualitative study of perceptions of science careers in the Centre National de la Recherche Scientifique (CNRS), the main research institution in France. Its aim is to understand the 'glass ceiling' effect, which reduces the proportion of women at the higher levels of the career hierarchy. Long interviews were carried out with men, as well as women, support staff and researchers. Factors such as tension between individual and collective dimensions of research activity, and long-term time-management problems, were identified: these affect both men and women but in different ways. Organizations bear an important responsibility through the way they reinforce or alleviate difficulties that women and men face in contributing to scientific research at all levels. PMID:19569427

  1. Allergie respiratoire et “sunko”: une association rare, à propos d'une observation

    PubMed Central

    Ngombe, Léon Kabamba; Kangulu, Ignace Bwana; Nzaji, Michel Kabamba

    2014-01-01

    Il est rapporté dans ce texte un cas d'allergie respiratoire ayant fait probablement suite à une consommation d'un tabac sans fumé couramment utilisé en République Démocratique du Congo, le « Sunko ». Une rhinite et un asthme allergiques sont les cas. Cette observation permet d'attirer l'attention du monde scientifique à mettre sur pieds des études concernant la composition et les effets du Sunko pour appréhender cette association, puis d'informer l'opinion sur les dangers que courent les consommateurs de ce type de tabac et de faire la revue de la littérature. PMID:25426218

  2. A la recherches d'autres mondes - les exoplanètes

    NASA Astrophysics Data System (ADS)

    Nazé, Yaël

    2013-10-01

    Habiter ailleurs que sur Terre, en dehors du système solaire, est-ce vraiment possible ? Est-ce que la vie existe en dehors du Système solaire et comment la chercher ? Ces questions sont celles que les hommes et les femmes se posent et celles qu'ils se sont posées de tout temps. Les scientifiques n'échappent pas à cette règle et nous vivons à une époque fascinante où cette recherche évolue extrêmement vite : ils ont découvert d'autres lieux potentiellement habitables ou habités, les exoplanètes, des planètes tournant autour d'autres soleils dans l'univers. À ce jour, plus de 900 exoplanètes ont ainsi été détectées

  3. André Saint-Marc 1944-1988

    NASA Astrophysics Data System (ADS)

    Reme, H.; Anderson, K. A.

    Andr Śaint-Marc, professor at the Institute of Technology of the Universite Paul Sabatier (IUT), in Toulouse, France, died suddenly and unexpectedly February 17, 1988, a few months before his 44th birthday.Saint-Marc carried out a research career in cosmic rays and space plasma physics beginning in 1969 at the Centre d'Etude Spatiale des Rayonnements (CESR), a laboratory of the Centre National de la Recherche Scientifique (CNRS) and the Université Paul Sabatier. He was born in Condegaygues, France (Lotet-Garonne). His four university degrees were awarded by the Universite Paul Sabatier. His Thèse de Docteur de Specialité was earned in 1973 for work on propagation of auroral X rays in Earth's atmosphere. The highest degree, the Doctorat d'Etat, came in 1979 for his studies of beam-plasma interactions in the ionosphere.

  4. A model for the construction of elementary concepts

    NASA Astrophysics Data System (ADS)

    von Glasersfeld, Ernst

    1999-03-01

    In his paper Les épistémologies constructivistes: Un nouveau commencement (Sciences de la Société, n°40, 1997), Jean-Louis Le Moigne poses the question: "Le rêve d'une connaissance autoréférentielle se fondant sur elle-même, est sans doute fascinant … Mais est-il scientifiquement raisonnable?". Building on the work of Jean Piaget, I shall try to show through a developmental analysis of elementary, scientifically relevant concepts, such as `change', `object permanence', `space', and `time', that the notion of the thinking subject's construction of knowledge constitutes a more reasonable foundation for science than the traditional belief in the representation of objective reality.

  5. Design considerations for solar furnace focal zone apparatus

    SciTech Connect

    Sievers, R.H. Jr.; Knasel, T.M.; McDonnell, M.; Gordon, B.; Woods, S.; Malinowski, R.

    1981-01-01

    Science Applications, Inc. has used the principal solar furnaces in conjunction with its study of the effect of high thermal fluxes and fluences on soil surfaces for the Defense Nuclear Agency. Apparatus to perform these tests has evolved from tests on the furnaces at the White Sands Missile Range, Georgia Institute of Technology in Atlanta; Centre National de Recherche Scientifique in Font Romeu, France; and Kirtland AFB, NM over the past 6 years. The apparatus is still evolving as it is adapted to additional furnaces and to obtain a greater variety of data. The evolution of the apparatus is traced to illustrate the interaction of experiment objectives; furnace capabilities, configuration, and support; apparatus design; data collection; and response to lessons learned.

  6. Master equation with quantized atomic motion including dipole-dipole interactions

    NASA Astrophysics Data System (ADS)

    Damanet, François; Braun, Daniel; Martin, John

    2016-05-01

    We derive a markovian master equation for the internal dynamics of an ensemble of two-level atoms including all effects related to the quantization of their motion. Our equation provides a unifying picture of the consequences of recoil and indistinguishability of atoms beyond the Lamb-Dicke regime on both their dissipative and conservative dynamics, and is relevant for experiments with ultracold trapped atoms. We give general expressions for the decay rates and the dipole-dipole shifts for any motional states, and we find analytical formulas for a number of relevant states (Gaussian states, Fock states and thermal states). In particular, we show that the dipole-dipole interactions and cooperative photon emission can be modulated through the external state of motion. The effects predicted should be experimentally observable with Rydberg atoms. FD would like to thank the F.R.S.-FNRS for financial support. FD is a FRIA Grant holder of the Fonds de la Recherche Scientifique-FNRS.

  7. 25th Birthday Cern- Restaurant

    ScienceCinema

    None

    2011-04-25

    Cérémonie du 25ème anniversaire du Cern avec plusieurs orateurs et la présence de nombreux autorités cantonales et communales genevoises et personnalités, directeurs généraux, ministres, chercheurs.... Le conseiller féderal et chef du département des affaires étrangères de la confédération Monsieur Pierre Aubert prend la parole pour célébrer à la fois les résultats très remarquables de la coopération internationale en matière scientifique, mais aussi la volonté politique des états européens de mettre en commun leurs ressources pour faire oeuvre d'avenir. Un grand hommage est aussi donné aux deux directeurs disparus, les prof.Bakker et Gregory.

  8. Hα kinematics of the Spitzer Infrared Nearby Galaxies Survey - II

    NASA Astrophysics Data System (ADS)

    Dicaire, I.; Carignan, C.; Amram, P.; Hernandez, O.; Chemin, L.; Daigle, O.; de Denus-Baillargeon, M.-M.; Balkowski, C.; Boselli, A.; Fathi, K.; Kennicutt, R. C.

    2008-04-01

    This is the second part of an Hα kinematics follow-up survey of the Spitzer Infrared Nearby Galaxies Survey (SINGS) sample. The aim of this paper is to shed new light on the role of baryons and their kinematics and on the dark/luminous matter relation in the star-forming regions of galaxies, in relation with studies at other wavelengths. The data for 37 galaxies are presented. The observations were made using Fabry-Perot interferometry with the photon-counting camera FaNTOmM on four different telescopes, namely the Canada-France-Hawaii 3.6-m, the ESO La Silla 3.6-m, the William Herschel 4.2-m and the Observatoire du mont Mégantic 1.6-m telescopes. The velocity fields are computed using custom IDL routines designed for an optimal use of the data. The kinematical parameters and rotation curves are derived using the GIPSY software. It is shown that non-circular motions associated with galactic bars affect the kinematical parameters fitting and the velocity gradient of the rotation curves. This leads to incorrect determinations of the baryonic and dark matter distributions in the mass models derived from those rotation curves. Based on observations made with the ESO 3.60-m telescope at La Silla Observatories under programme ID 076.B-0859 and on observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France and the University of Hawaii. E-mail: isabelle@astro.umontreal.ca (ID);claude.carignan@umontreal.ca (CC) ‡ Visiting Astronomer, Canada-France-Hawaii Telescope, operated by the National Research Council of Canada, the Centre National de la Recherche Scientifique de France and the University of Hawaii.

  9. Morocco, Kingdom of the young geologist!

    NASA Astrophysics Data System (ADS)

    Bouttemy, Franck

    2015-04-01

    The Kingdom of Morocco is a country of 33 million people where about thirty French schools enroll 32,000 students including a majority of Moroccans. The Rabat Center includes several institutions enrolling 5,700 students aged 10 to 18 years old whose High School René Descartes is directed by the A.E.F.E, "Agency for French Teaching Abroad". Sixteen professors teach S.V.T. "Sciences de la Vie et de la Terre" that focuses on biology and geology. The programs involved are French but the biology-geology colleagues seek to place the teaching of geology in the context of Morocco through the choice of Moroccan examples. (https://sites.google.com/site/aefesvtmaroc/) Morocco's geology lends itself to this approach! The laboratory is equipped with a seismometer in the network "Sismos to School" (https://sites.google.com/a/lycee-descartes.ma/rabt_sismo/home) and we have the equipment necessary for making thin sections of the Moroccan rocks for practical work on a polarizing microscope. We organize several field trips: On a half-day in the region of Rabat, 12-year old pupils of "5ème", learn about reading the landscape and studying sedimentary rocks such as marls and sandstones. On a 3-day excursion in the region of Azrou, the16-year old pupils of "première scientifique" study the tectonic context of formation of mineral resources. A 2-day trip in the region of Oulmès, the17-year old pupils of "terminale scientifique" (the last year in the French system finishing with the "baccalaureate") study continental crust, tectonics and geothermal energy. These field trips will be presented in this poster. Students make field studies: observation, testing, photography, drawing and taking notes. Some works are evaluated during the field trip, others are the subject of home work: preparing a slide show, an audio recording work...

  10. CONFERENCE NOTE: Conference on Precision Electromagnetic Measurements

    NASA Astrophysics Data System (ADS)

    1991-01-01

    The next Conference on Precision Electromagnetic Measurements (CPEM), will be held from 9 to 12 June 1992 at the Centre des Nouvelles Industries et Technologies (CNIT), La Défense, Paris, France. This conference, which is held every two years and whose importance and high level, confirmed by thirty years' experience, are recognized throughout the world, can be considered as a forum in which scientists, metrologists and professionals will have the opportunity to present and compare their research results on fundamental constants, standards and new techniques of precision measurement in the electromagnetic domain. Topics The following topics are regarded as the most appropriate for this conference: realization of units and fundamental constants d.c. a.c. and high voltage time and frequency radio-frequency and microwaves dielectrics, antennas, fields lasers, fibre optics advanced instrumentation, cryoelectronics. There will also be a session on international cooperation. Conference Language The conference language will be English. No translation will be provided. Organizers Société des Electriciens et des Electroniciens (SEE). Bureau National de Métrologie (BNM) Sponsors Institute of Electrical and Electronics Engineers (IEEE) Instrumentation & Measurement Society Union Radio Scientifique Internationale United States National Institute of Standards and Technology Centre National d'Etudes des Télécommunications Mouvement Français pour la Qualité, Section Métrologie Comité National Français de Radioélectricité Scientifique Contact Jean Zara, CPEM 92 publicity, Bureau National de Métrologie, 22, rue Monge, 75005 Paris Tel.: (33) 1 46 34 48 16, Fax: (33) 1 46 34 48 63

  11. Magnetic field, chemical composition and line profile variability of the peculiar eclipsing binary star AR Aur

    NASA Astrophysics Data System (ADS)

    Folsom, C. P.; Kochukhov, O.; Wade, G. A.; Silvester, J.; Bagnulo, S.

    2010-10-01

    AR Aur is the only eclipsing binary known to contain a HgMn star, making it an ideal case for a detailed study of the HgMn phenomenon. HgMn stars are a poorly understood class of chemically peculiar stars, which have traditionally been thought not to possess significant magnetic fields. However, the recent discovery of line profile variability in some HgMn stars, apparently attributable to surface abundance patches, has brought this belief into question. In this paper we investigate the chemical abundances, line profile variability, and magnetic field of the primary and secondary of the AR Aur system, using a series of high-resolution spectropolarimetric observations. We find the primary is indeed a HgMn star, and present the most precise abundances yet determined for this star. We find the secondary is a weak Am star, and is possibly still on the pre-main sequence. Line profile variability was observed in a range of lines in the primary, and is attributed to inhomogeneous surface distributions of some elements. No magnetic field was detected in any observation of either stars, with an upper limit on the longitudinal magnetic field in both stars of 100 G. Modelling of the phase-resolve longitudinal field measurements leads to a 3σ upper limit on any dipole surface magnetic field of about 400 G. Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France and the University of Hawaii. Also based on observations obtained at the Bernard Lyot Telescope (TBL, Pic du Midi, France) of the Midi-Pyrénées Observatory, which is operated by the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France. E-mail: cpf@arm.ac.uk

  12. Celestial Treasury

    NASA Astrophysics Data System (ADS)

    Lachièze-Rey, Marc; Luminet, Jean-Pierre

    2001-07-01

    Throughout history, the mysterious dark skies have inspired our imaginations in countless ways, influencing our endeavors in science and philosophy, religion, literature, and art. Filled with 380 full-color illustrations, Celestial Treasury shows the influence of astronomical theories and the richness of illustrations in Western civilization through the ages. The authors explore the evolution of our understanding of astronomy and weave together ancient and modern theories in a fascinating narrative. They incorporate a wealth of detail from Greek verse, medieval manuscripts and Victorian poetry with contemporary spacecraft photographs and computer-generated star charts. Celestial Treasury is more than a beautiful book: it answers a variety of questions that have intrigued scientists and laymen for centuries. -- How did philosophers and scientists try to explain the order that governs celestial motion? -- How did geometers and artists measure and map the skies? -- How many different answers have been proposed for the most fundamental of all questions: When and how did Earth come about? -- Who inhabits the heavens--gods, angels or extraterrestrials? No other book recounts humankind's fascination with the heavens as compellingly as Celestial Treasury. Marc Lachièze-Rey is a director of research at the Centre National pour la Récherche Scientifique and astrophysicist at the Centre d'Etudes de Saclay. He is the author of The Cosmic Background Radiation (Cambridge, 1999), and and The Quest for Unity, (Oxford, 1999 ), as well as many books in French. Jean-Pierre Luminet is a research director of the Centre National pour la Rechérche Scientifique, based at the Paris-Meudon observatory. He is the author of Black Holes, (Cambridge 1992), as well as science documentaries for television.

  13. Organizational Strategies for Critical Transportation Infrastructure: Characteristics of Urban Resilience. The Case of Montreal.

    NASA Astrophysics Data System (ADS)

    Beauregard, Stéphane; Therrien, Marie-Christine; Normandin, Julie-Maude

    2010-05-01

    Organizational Strategies for Critical Transportation Infrastructure: Characteristics of Urban Resilience. The Case of Montreal. Stéphane Beauregard M.Sc. Candidate École nationale d'administration publique Julie-Maude Normandin Ph.D. Candidate École nationale d'administration publique Marie-Christine Therrien Professor École nationale d'administration publique The proposed paper presents preliminary results on the resilience of organizations managing critical infrastructure in the Metropolitan Montreal area (Canada). A resilient city is characterized by a network of infrastructures and individuals capable of maintaining their activities in spite of a disturbance (Godschalk, 2002). Critical infrastructures provide essential services for the functioning of society. In a crisis situation, the interruption or a decrease in performance of critical infrastructures could have important impacts on the population. They are also vulnerable to accidents and cascading effects because on their complexity and tight interdependence (Perrow, 1984). For these reasons, protection and security of the essential assets and networks are one of the objectives of organizations and governments. But prevention and recovery are two endpoints of a continuum which include also intermediate concerns: ensuring organizational robustness or failing with elegance rather than catastrophically. This continuum also includes organizational resilience (or system), or the ability to recover quickly after an interruption has occurred. Wildavsky (1988) proposes that anticipation strategies work better against known problems while resilience strategies focus on unknown problems. Anticipation policies can unnecessarily immobilize investments against risks, while resilience strategies include the potential for a certain sacrifice in the interests of a more long-term survival and adaptation to changing threats. In addition, a too large confidence in anticipation strategies can bring loss of capacity of an

  14. Modélisation et simulation en régime stationnaire d'ateliers d'évaporation de sucreries à l'aide de l'équation d'état de Peng-Robinson

    NASA Astrophysics Data System (ADS)

    Rabi, M.; Bounahmidi, T.

    1999-03-01

    In this work the Peng-Robinson equation of state, previously adapted in our laboratory to predict physical and vapor-liquid equilibrium properties of sugar juices caracterised by the pseudo-components: sugar, amino acid ,carboxylic acid and cinders in aquesus solution, was tested in the modeling and simulation of the steady-state behaviour of multiple effect evaporation plants in sugar factory. The results of simulation has been compared to the real average measurements in the SUNABEL(Sucrerie Nationale de Betterave de Loukkos,Maroc) sugar factory, and showed that the Peng-Robinson equation of state can be used to predict, with a sufficient precision, of the steady-state behaviour of multiple effect evaporation plants in sugar factory. The originality of the model in comparison with the published others models consist in takening account of purity and natural of impurity in the juice. The simultanious modular approach is used in steady state process simulation. Dans ce travail l'équation d'état de Peng-Robinson, adaptée antérieurement dans notre laboratoire aux jus sucrés industriels en caractérisant ces derniers à l'aide de pseudo-composés sucre, acide aminé, acide carboxylique et cendre en solution dans l'eau, a ?été? testée pour la modélisation en régime stationnaire d'ateliers d'évaporation de sucreries. La confrontation des résultats de simulation à l'aide de ce modèle, avec des mesures moyennes observées sur l'atelier d'évaporation de la Sucrerie Nationale de Betterave du Loukkos (SUNABEL) Ksar El Kébir, a montré? que cette ?équation permet de prédire, avec une précision suffisante, les performances de l'atelier en régime stationnaire. L'originalité? du modèle développé, par rapport aux modèles proposés dans la littérature, réside dans la prise en compte de la pureté? et de la nature des impuretés présentes dans le jus. La simulation de l'atelier d'évaporation à l'aide de ce modèle a été menée en utilisant l

  15. Préface

    NASA Astrophysics Data System (ADS)

    Mazière, D.

    2002-04-01

    Faisant suite aux deux précédents colloques "Matériaux pour les machines thermiques" et "Matériaux pour le nucléaire" , le colloque 2001 de l'INSTN intitulé "Matériaux pour les énergies propres" s'est focalisé sur les problèmes de matériaux encore à résoudre dans ce secteur industriel. Le colloque de métallurgie est traditionnellement organisé par des ense ignants du DEA Métallurgie et Matériaux et un comité scientifique choisi chaq ue année en liaison avec le thème traité. Les étudiants de ce DEA, qui est hab ilité entre Paris XI, Paris VI, l'Ecole des Mines de Paris, l'Ecole Centrale de Pari s et l'INSTN, sont invités à participer à ce colloque et aux débats scientifiques qui s'y déroulent. Des conférences invitées à caractère péda gogique permettent d'introduire les différents thèmes abordés qui sont ensuite développés dans des présentations plus novatrices. Cette manifestation a pour ambition de favoriser la rencontre de scientifiques d'horizons divers venant de milieux académiques ou industriels entre eux et avec les étudiants et thésards. Cette 44e édition, dont les comptes rendus sont publiés ici, a fait le point sur les problèmes de matériaux rencontrés lors de la production, du stockage et de la conversion des énergies dites propres en englobant lesprogrès constants des industriels de l'automobile. Ce colloque a réuni, du 26 au 28 juin 2001, 63 participants provenant d'universités ou grandes écoles (18), du CEA (17), du CNRS (10) et de l'industrie ou de centres de recherche associés. L'ensemble des problèmes de matériaux de ce secteur ont été examinés au cours des six sessions ci-dessous : dépollution des gaz d'échappement ; combustion catalytique en production thermique ; nouvelles batteries ; piles à combustibles ; production et stockage d'hydrogène ; production et stockage d'énergie solaire. Vingt huit communications dont vingt deux orales ont illustré les dével oppements en cours. Dix

  16. Paternité des articles et intérêts concurrents : une analyse des recommandations aux auteurs des journaux traitant de pratique pharmaceutique

    PubMed Central

    Courbon, Ève; Tanguay, Cynthia; Lebel, Denis; Bussières, Jean-François

    2014-01-01

    RÉSUMÉ Contexte : La présence d’auteurs honorifiques et fantômes ainsi que les intérêts concurrents représentent des difficultés bien documentées, liées à la publication d’articles scientifiques. Il existe des lignes directrices encadrant la rédaction et la publication de manuscrits scientifiques, notamment celles de l’International Committee of Medical Journal Editors (ICMJE). Objectifs : L’objectif principal de cette étude descriptive et transversale visait à recenser les instructions portant sur la paternité des articles et les intérêts concurrents provenant des recommandations aux auteurs des journaux traitant de pratique pharmaceutique. L’objectif secondaire visait à déterminer des mesures correctrices pour une paternité des articles plus transparente. Méthode : La recherche a débuté par l’identification des journaux traitant de pratique pharmaceutique. La consultation des instructions aux auteurs des journaux a permis ensuite de recenser les recommandations destinées à éviter les problèmes de paternité des articles et d’intérêts concurrents. Finalement, les membres de l’équipe de recherche se sont consultés afin de définir des mesures correctrices possibles à l’intention des chercheurs. Résultats : Des 232 journaux traitant de pharmacie, 33 ont été définis comme traitant de pratique pharmaceutique. Un total de 24 (73 %) journaux mentionnaient suivre la politique de l’ICMJE, 14 (42 %) demandaient aux auteurs de remplir un formulaire de déclaration d’intérêts concurrents au moment de la soumission de l’article, 17 (52 %) présentaient une définition de la qualité d’auteur et 5 (15 %) demandaient de détailler les contributions de chaque auteur. Une grille de 40 critères a été élaborée pour définir l’attribution du statut d’auteur. Conclusion : Moins de la moitié des journaux demandait aux auteurs de transmettre un formulaire de déclaration des intérêts concurrents au moment de la

  17. Démarche pour la mise à niveau d’un secteur de soins pharmaceutiques : le cas de l’hémato-oncologie pédiatrique

    PubMed Central

    Bussières, Jean-François; Robelet, Antoine; Therrien, Roxane; Touzin, Karine

    2010-01-01

    Contexte : Bien que le concept de pharmacie clinique ait été développé dans les années soixante, il existe une grande variété de programmes et une grande disparité entre les programmes en clinique externe et en hospitalisation, bénéficiant de la présence d’un pharmacien dans un secteur de soins. Objectif: Éprouver une méthode de mise à niveau des secteurs de soins pharmaceutiques en établissement de santé. Méthode : Il s’agit d’une étude descriptive se déroulant au Centre hospitalier universitaire Sainte-Justine, un établissement mère-enfant de 500 lits. Le secteur de soins pharmaceutiques ciblé pour illustrer la méthode de mise à niveau est l’hématologie-oncologie pédiatrique. La méthode comporte trois étapes, soit une revue de la documentation scientifique, un profil du secteur et une mise à jour du niveau de pratique selon un profil des activités pharmaceutiques dans le secteur avant et après la mise à niveau. Résultats : Au total, 108 articles ont été recensés et 22 ont été retenus à partir d’une recherche dans PubMed. Après une recherche manuelle complémentaire, 36 articles ont finalement été évalués. Parmi les articles retenus, on compte trois lignes directrices, 11 études de développement, une revue de la littérature scientifique, six études pré- et post-interventions et 15 études quasi expérimentales. Bien que les patients de ce secteur ne comptent que pour 5 % des admissions de l’hôpital, la complexité des cas est élevée tant sur le plan de la codification de l’épisode de soins que du potentiel d’intervention pharmaceutique par admission. Conclusion : Il existe peu de données illustrant une démarche de mise à niveau de la pratique dans un secteur de soins pharmaceutiques. Cette étude a éprouvé une méthode de mise à niveau dans un service d’hématologie-oncologie pédiatrique et comporte une revue de la documentation scientifique, un profil du secteur et une description des t

  18. Foreword

    NASA Astrophysics Data System (ADS)

    Boutron, Claude; Ferrari, Christophe

    2003-05-01

    It is our pleasure to host the “12th International Conference on Heavy Metals in the Environment” in the city of Grenoble (France), in the heart of the Alps. This is the latest in this successful and popular series of conferences, which previously took place in Toronto (1975), London (1979), Amsterdam (1981), Heidelberg (1983), Athens (1985), New Orleans (1987), Geneva (1989), Edinburgh (1991), Hamburg (1995) and Ann Arbor (2000). Grenoble is one of the major research centres in Europe, with a very large number of researchers in various fields, especially Physics and Chemistry, Mathematics and Computer Sciences, Biology and Medicine, and Earth and Universe Sciences. There are two internationally recognized scientific Universities: Université Joseph Fourier (UJF), and Institut National Polytechnique de Grenoble (INPG). There are also the main research laboratories of various French and European governmental organizations such as Commissariat à l'énergie Atomique (CEA), Centre National de la Recherche Scientifique (CNRS), Institut Laue Langevin (ILL), European Synchrotron Radiation Facility (ESRF) and Institut de Radio-Astronomie Millimètrique (IRAM). Finally, there are various hi-tech companies such as Hewlett Packard, ST Microelectronics, Schneider Electric and SGS-Thomson. There is a long tradition of research in the field of heavy metals in the environment, especially at the Laboratoire de Glaciologie et Géophysique de l'Environnement and at the Laboratoire de Géophysique Interne et Tectonophysique. These two volumes contain papers presented both in oral and poster sessions. The papers are not organised in order of presentation, but according to the alphabetical order of the family name of the first author of each paper. It is our pleasure to thank the authors for the excellent level of their submissions. We are also particularly grateful to Isabelle Houlbert and Laurence Castagné for editorial assistance. We would like to take this opportunity to

  19. Heat transfer enhancement by the Goertler vortices developed on a wall with a finite thermal conductivity

    NASA Astrophysics Data System (ADS)

    Mutabazi, Innocent; Yoshikawa, Harunori; Peixinho, Jorge; Kahouadji, Lyes

    2013-11-01

    Görtler vortices appear in a flow over a concave wall as a result of centrifugal instability [Saric, Annu. Rev. Fluid Mech. 26, 379 (1994)]. They may have a strong influence on heat transfer [Momayez et al., Int. J. heat Mass transfer 47, 3783 (2004)]. The purpose of this work is to model heat transfer by Görtler vortices using a weakly nonlinear analysis of Smith &-Haj- Hariri [Phys. Fluids A 5, 2815 (1993)]. We have investigated the coupling of the convective heat transfer by the stationary vortices with the heat conduction inside the solid wall. The finite thickness and thermal conductivity of the wall enter into the boundary conditions of the problem through the ratio δ of the wall thickness to the boundary layer thickness and through the ratio K of the thermal conductivities of the fluid and the wall. The parametric dependence Nu (δ , K) of the Nusselt number is performed and it is shown that found the heat transfer is quite well modified by these two parameters. The local thermal stress can be estimated in order to analyze the effects on ageing of the wall material. The authors acknowledge the financial support of the french Agence Nationale de la Recherche (ANR), through the program ``Investissements d'Avenir'' (ANR-10-LABX-09-01), LabEx EMC3.

  20. Commercial runs show TiO/sub 2/ Claus catalyst retains activity

    SciTech Connect

    Nougayrede, J.; Philippe, A.; Quesmerel, E.; Vermeersch, R.

    1987-08-10

    Commercial data are given for the CRS 31 Claus catalyst, jointly developed by Rhone Poulenc and Societe Nationale Elf Aquitane (Production) (SNEA). The data confirm laboratory results that show the catalyst's ability to deliver more complete hydrolysis in the first reactor of Claus sulfur recovery plants, and its ability to maintain activity in the second and third reactors. The most important losses in sulfur yields in Claus plants generally come from COS and CS/sub 2/ formed in the thermal steps of the process in the first reactor, and from the low Claus activity of alumina-based catalysts in the second and third reactors. In the first reactor, loaded with alumina-based catalyst, hydrolysis is only partial. Low Claus activity in second and third reactors is caused by the inevitable sulfation of the alumina. Catalytic-activity decrease of aluminas is caused particularly by the presence of oxygen, even in trace amounts, in the Claus gases. Therefore, in the first reactor, the CS/sub 2/ hydrolysis rate is lowered in the subsequent reactors, the H/sub 2/ + SO/sub 2/ conversion significantly drops. The chemical composition of CRS 31, TiO/sub 2/ only, in the same operating conditions, causes a significant improvement in activity because of its increased resistance to sulfation. The economics of the process are given.

  1. Color, light, and altruistic creation

    NASA Astrophysics Data System (ADS)

    Charnay, Yves

    2002-06-01

    It seems necessary to me to combine a certain technical inventivity with plastic creation, a particular poetry arises from this relation. The sources of inspiration for works, especially works in which color plays a pre-eminent role, do not only come from nature. The fantasy of the creators evolves and changes thanks to discoveries and technological inventions. My work as a painter has made me particularly sensitive to the diversity of the plastic writings in general and to the chromatic writings in particular. (1) Environmental creation imposes a renewal of the means of creation. Conducting experimental works, I study the particularities of light, mainly its incidence on materials (transmission, reflection, colors, textures, etc.) and its mobility. These works are a source of inspiration for my architectural works and nurture my lectures at the Ecole Nationale Superieure des Arts Decoratifs (National College of Decorative Arts). Environmental creation also imposes some qualities on the artist since he, whether he serves a social entity or a person, serves the whole collectivity. Environmental creation has to be envisaged as an altruistic approach.

  2. Terahertz Specroscopy of Methylamine

    NASA Astrophysics Data System (ADS)

    Motiyenko, R. A.; Margulès, L.; Ilyushin, V. V.; Alekseev, E. A.; Drouin, B.; Yu, S.; Cernicharo, J.; Tercero, B.

    2012-06-01

    Methylamine (CH_3NH_2) is a light molecule with an intense rotational spectrum that extends far beyond 1 THz even at temperatures characteristic for interstellar medium. This fact makes methylamine an interesting object of studies for THz radio telescopes like Herschel and SOFIA. In this context we present recent advances in global fitting of the rotational spectrum of parent isotopic species of CH_3NH_2 up to 2.6 THz. The Hamiltonian used in the analysis is based on the group-theoretical formalism developed by Ohashi and Hougen. It has been successfully applied for the analysis of mm-wave and far-IR spectrum of methylamine as well as for the analysis of sub-THz spectra of its 13C isotopologue. We will also present the latest results on searches for interstellar 13CH_3NH_2 as well as the results on the analysis of deuterated species of methylamine which is in progress now. This work is supported by Centre Nationale d'Etudes Spatiales (CNES), Action sur Projet Physico-Chimie du Milieu Interstellaire (PCMI-CNRS) and by the contract ANR-08-BLAN-0054. Ohashi, N. and Hougen, J. T. J. Mol. Spec. 121 (1987) 474. Ilyushin, V.V. et al. J. Mol. Spec. 229 (2005) 170. R.A. Motiyenko et al. FA08, 66th International Symposium on Molecular Spectroscopy (2011).

  3. Highlights of recent studies and future plans for the French human biomonitoring (HBM) programme.

    PubMed

    Fréry, Nadine; Vandentorren, Stéphanie; Etchevers, Anne; Fillol, Clémence

    2012-02-01

    This manuscript presents highlights of recent studies and perspectives from the French human biomonitoring (HBM) programme. Until recently, HBM studies focused on specific populations or pollutants to gain a better understanding of exposure to environmental chemicals, to help regulators reduce environmental exposure and to monitor existing policies on specific concerns. Highlights of recent multicentre biomonitoring studies with specific population or pollutant focus are given. These French HBM studies have been implemented to know: (1) the influence of living near an incinerator on serum dioxin and polychlorinated biphenyl (PCB) levels, (2) the influence of consuming river fish contaminated by PCBs on serum PCBs of fishermen, and (3) the evolution of blood lead levels in children from 1 to 6 years old since 1995. Special emphasis is placed on the use of an integrated (HBM coupled with nutrition and health studies), multipollutant approach. This approach has been initiated in France with a recent national population-based biomonitoring survey, the Etude Nationale Nutrition Santé (ENNS; French Nutrition and Health Survey). This survey will provide the first reference distribution for 42 biomarkers in the French population. The current national HBM strategy will build upon the ENNS and include a national survey of people aged between 6 and 74 years complemented for the neonatal period and childhood by the Etude Longitudinale Française depuis l'Enfance (ELFE; French longitudinal study of children). France also contributes to the harmonization of HBM activities in Europe through participation in European HBM projects. PMID:21940210

  4. The Gutenberg Bibles: analysis of the illuminations and inks using Raman spectroscopy.

    PubMed

    Chaplin, Tracey D; Clark, Robin J H; Jacobs, David; Jensen, Kristian; Smith, Gregory D

    2005-06-01

    The King George III copy of the Gutenberg Bible, held at the British Library, has been analyzed using Raman spectroscopy to determine the palette of pigments used in the illuminations on this work. The palette is found to comprise cinnabar/vermilion, lead tin yellow (type 1), carbon-based black, azurite, malachite, an organo-copper complex (a "verdigris"), calcium carbonate (chalk), gypsum, gold leaf, and basic lead carbonate ("lead white"). This is in agreement with contemporary descriptions of the pigments used for the illuminations. One pigment could not be identified, specifically the organic dark red/purple color used for the foliage. The palette of this copy of the Gutenberg Bible has been compared with those used for six other copies, held at Eton College and Lambeth Palace, England, the Bibliothèque Mazarine and the Bibliothèque nationale de France, and the Staatsbibliothek zu Berlin and the Niedersachsische Staats- und Universitatsbibliothek (SUB) Göttingen, Germany. The palettes are shown to be similar to one another, even though the styles of the primary illuminations differ. The two Gutenberg Bibles held in Germany, printed on vellum, have the more expensive palettes, which include lazurite. The SUB Göttingen copy has the most extensive palette with 16 pigment-related materials having been identified. PMID:15924396

  5. Effect of the band structure in a rigorous two-body model with long-range interactions in 1D optical lattices

    NASA Astrophysics Data System (ADS)

    Kristensen, Tom; Simoni, Andrea; Launay, Jean-Michel

    2016-05-01

    We compute scattering and bound state properties for two ultracold molecules in a pure 1D optical lattice. We introduce reference functions with complex quasi-momentum that naturally account for the effect of excited energy bands. Our exact results for a short-range interaction are first compared with the simplest version of the standard Bose-Hubbard (BH) model. Such comparison allows us to highlight the effect of the excited bands, of the non-on-site interaction and of tunneling with distant neighbor, that are not taken into account in the BH model. The effective interaction can depend strongly on the particle quasi-momenta and can present a resonant behavior even in a deep lattice. As a second step, we study scattering of two polar particles in the optical lattice. Peculiar Wigner threshold laws stem from the interplay of the long range dipolar interaction and the presence of the energy bands. We finally assess the validity of an extended Bose-Hubbard model for dipolar gases based on our exact two-body calculations. This work was supported by the Agence Nationale de la Recherche (Contract No. ANR-12-BS04-0020-01).

  6. Quantitation of HIV-1 RNA in dried blood and plasma spots.

    PubMed

    Reigadas, S; Schrive, M H; Aurillac-Lavignolle, V; Fleury, H J

    2009-10-01

    Dried blood spots (DBSs) and dried plasma spots (DPSs) are an attractive method for serological and molecular diagnosis of HIV infection. Recently, Youngpairoj et al. [Youngpairoj, A.S., Masciotra, S., Garrido, C., Zahonero, N., de Mendoza, C., Garcia-Lerma, J.G., 2008. HIV-1 drug resistance genotyping from dried blood spots stored for 1 year at 4 degrees C. J. Antimicrob. Chemother. 61, 1217-1220] showed that HIV-1 can be genotyped efficiently from DBS specimens stored at 4 degrees C for 1 year. The viral load obtained from DBS and DPS samples was compared with that obtained from plasma samples. A total of 86 samples was prepared from people infected with HIV subtype B or non-B and spotted on 903 filter papers stored with desiccant at 4 degrees C. RNA was extracted using the QIAamp Viral RNA mini kit (Qiagen, Courtaboeuf, France). RNA from DBS or DPS samples was quantified in accordance with the Agence Nationale de Recherche sur le SIDA (ANRS, AC11, Paris, France) assay for HIV-1 quantitation. When the mean viral load of plasma samples and DPS samples or plasma samples and DBS samples were compared, there were no significant differences. The overall data showed that although the sensitivity threshold of the assays was different, there was a correlation between the three specimen types and that DBS and DPS samples can be routinely used for viral load quantification particularly in resource-limited settings. PMID:19523984

  7. Spatial organization of cilia tufts governs airways mucus transport: Application to severe asthma

    NASA Astrophysics Data System (ADS)

    Khelloufi, Mustapha Kamel; Gras, Delphine; Chanez, Pascal; Viallat, Annie

    2014-11-01

    We study the coupling between both density and spatial repartition of beating cilia tufts, and the coordinated transport of mucus in an in-vitro epithelial model. We use a fully differentiated model epithelium in air liquid interface (ALI) obtained from endo-bronchial biopsies from healthy subjects and patients with asthma. The asthma phenotype is known to persist in the model. Mucus transport is characterized by the trajectories and velocities of microscopic beads incorporated in the mucus layer. When the beating cilia tufts density is higher than dc = 11/100 × 100 μm2 a spherical spiral coordinated mucus transport is observed over the whole ALI chamber (radius = 6 mm). Below dc, local mucus coordinated transport is observed on small circular domains on the epithelium surface. We reveal that the radii of these domains scale with the beating cilia tufts density with a power 3.7. Surprisingly, this power law is independent on cilia beat frequency, concentration and rheological properties of mucus for healthy subject and patient with asthma. The rotating or linear mucus transport is related to dispersion of the cilia tufts on the epithelium surface. We show that impaired mucus transport observed in severe asthma model epithelia is due to a drastic lack and dysfunction of cilia tufts. The author acknowledges the support of the French Agence Nationale de la Recherche (ANR) under reference ANR-13-BSV5-0015-01.

  8. Forensic entomology: implementing quality assurance for expertise work.

    PubMed

    Gaudry, Emmanuel; Dourel, Laurent

    2013-09-01

    The Department of Forensic Entomology (Institut de Recherche Criminelle de la Gendarmerie Nationale, France) was accredited by the French Committee of Accreditation (Cofrac's Healthcare section) in October 2007 on the basis of NF EN ISO/CEI 17025 standard. It was the first accreditation in this specific field of forensic sciences in France and in Europe. The present paper introduces the accreditation process in forensic entomology (FE) through the experience of the Department of Forensic Entomology. Based upon the identification of necrophagous insects and the study of their biology, FE must, as any other expertise work in forensic sciences, demonstrate integrity and good working practice to satisfy both the courts and the scientific community. FE does not, strictly speaking, follow an analytical method. This could explain why, to make up for a lack of appropriate quality reference, a specific documentation was drafted and written by the staff of the Department of Forensic Entomology in order to define working methods complying with quality standards (testing methods). A quality assurance system is laborious to set up and maintain and can be perceived as complex, time-consuming and never-ending. However, a survey performed in 2011 revealed that the accreditation process in the frame of expertise work has led to new well-defined working habits, based on an effort at transparency. It also requires constant questioning and a proactive approach, both profitable for customers (magistrates, investigators) and analysts (forensic entomologists). PMID:23842668

  9. [Gastroentérologie Clinique et Biologique: a century's history of digestive system diseases].

    PubMed

    Hecketsweiler, P; Frexinos, J

    2009-01-01

    The journal Gastroentérologie clinique et biologique succeded to Archives des maladies de l'appareil digestif published since 1907 and is one of the world's oldest journals in gastroenterology. Gastroentérologie Clinique et Biologique was created as the discipline was emerging, benefiting from new techniques such as nasogastric intubation, coprologic examinations, the first images from gastrointestinal radiology, as well as the enormous progress made in gastrointestinal surgery. The journal was founded by Albert Mathieu, a remarkable chef d'école at Paris's Saint-Antoine Hospital. The journal showed rapid success, becoming the official organ of several learned societies, in particular the French National Society of Gastroenterology (Société nationale française de gastroentérologie [SNFGE]). Thoroughly updated in the 1970s, Gastroentérologie clinique et biologique has never ceased to evolve, adapting to technical and scientific upheavals, the globalization of knowledge, and the domination of the English language. PMID:19717255

  10. Inverse turbulent cascade in swarming sperm

    NASA Astrophysics Data System (ADS)

    Creppy, Adama; Praud, Olivier; Druart, Xavier; Kohnke, Philippa; Plouraboue, Franck; Inra, Cnrs, Umr, F-37380 Nouzilly, France Team; Université de Toulouse, Inpt, Ups, Imft, Umr 5502, France Team

    2014-11-01

    Collective motion of self-sustained swarming flows has recently provided examples of small scale turbulence arising where viscosity effects are dominant. We report the first observation of an universal inverse enstrophy cascade in concentrated swarming sperm consistent with a body of evidence built from various independent measurements. We found a well-defined k-3 power-law decay of velocity field power-spectrum and relative dispersion of small beads consistent with theoretical predictions in two-dimensional turbulence. Concentrated living sperm displays long-range, correlated whirlpool structures the size of which provides turbulence's integral scale. We propose a consistent explanation for this quasi-two-dimensional turbulence based on self-structured laminated flow forced by steric interaction and alignment, a state of active matter that we call ``swarming liquid crystal.'' We develop scaling arguments consistent with this interpretation. The implication of multi-scale collective dynamics of sperm's collective motility for fertility assessment is discussed. This work has been supported by the French Agence Nationale pour la Recherche (ANR) in the frame of the Contract MOTIMO (ANR-11-MONU-009-01). We thank Pierre Degond, Eric Climent, Laurent Lacaze and Frédéric Moulin for interesting discussions.

  11. [Molecular biology methods in immunohematology].

    PubMed

    Tournamille, C

    2013-05-01

    The molecular basis of almost all antigens of the 33 blood group systems are known. These knowledge and the advent of the PCR technology have allowed the DNA-based genotyping in order to predict the presence or absence of a blood group antigen on the cell membrane of red blood cells. DNA genotyping is required in cases where red blood cells patient cannot be used for serological typing either after a recent transfusion or because of the presence of autoantibodies on the red blood cells. Numerous DNA assays are available to detect any nucleotide polymorphism on the genes encoding blood group antigens. The technologies have improved to answer quickly to any case of transfusion emergency and to limit the risk of DNA contamination in a molecular diagnostic laboratory. Some technologies are ready for high-throughput blood group genotyping. They will be used in the future to obtain a fully typed blood group card of each donor but also to detect blood donors with rare phenotypes to register them to the Banque Nationale de Sang de Phénotype Rare (BNSPR). PMID:23587623

  12. Factors related to lipodystrophy and metabolic alterations in patients with human immunodeficiency virus infection receiving highly active antiretroviral therapy.

    PubMed

    Savès, Marianne; Raffi, François; Capeau, Jacqueline; Rozenbaum, Willy; Ragnaud, Jean-Marie; Perronne, Christian; Basdevant, Arnaud; Leport, Catherine; Chêne, Geneviève

    2002-05-15

    Morphologic and metabolic changes associated with protease inhibitor (PI) therapy have been reported since the introduction of PIs for treatment of human immunodeficiency virus infection. These changes were measured 12-20 months after initiation of PI therapy in a cross-sectional study involving 614 patients from the Antiprotéases Cohorte (APROCO) Study (Agence Nationale de Recherches sur le Sida-EP11). The prevalence was 21% for isolated peripheral atrophy, 17% for isolated fat accumulation, 24% for mixed syndrome, 23% for glucose metabolism alterations, 28% for hypertriglyceridemia (triglyceride level, > or =2.2 mM), and 57% for hypercholesterolemia (cholesterol level, > or =5.5 mM). Age was significantly associated with different phenotypes of lipodystrophy and metabolic alterations, but body-mass index, CD4(+) cell count, and type of nucleoside reverse-transcriptase inhibitor or PI received were not constantly associated with these changes. Furthermore, in all models tested, exposure to stavudine was associated with lipoatrophy and exposure of ritonavir was associated with hypertriglyceridemia. Detection and management of these disorders should be implemented to prevent further complications. PMID:11981737

  13. Long-term association of food and nutrient intakes with cognitive and functional decline: a 13-year follow-up study of elderly French women.

    PubMed

    Vercambre, Marie-Noël; Boutron-Ruault, Marie-Christine; Ritchie, Karen; Clavel-Chapelon, Françoise; Berr, Claudine

    2009-08-01

    The objective of the present study was to determine the potential long-term impact of dietary habits on age-related decline among 4809 elderly women (born between 1925 and 1930) in the 'Etude Epidémiologique de Femmes de la Mutuelle Générale de l'Education Nationale' (E3N) study, a French epidemiological cohort. In 1993, an extensive diet history self-administered questionnaire was sent to all participants, and in 2006 another questionnaire on instrumental activities of daily living (IADL) and recent cognitive change was sent to a close relative or friend of each woman. Logistic models adjusted for socio-demographic, lifestyle and health factors were performed to evaluate associations between habitual dietary intakes and two outcomes of interest based on the informant response: recent cognitive decline and IADL impairment. Recent cognitive decline was associated with lower intakes of poultry, fish, and animal fats, as well as higher intakes of dairy desserts and ice-cream. IADL impairment was associated with a lower intake of vegetables. The odds of recent cognitive decline increased significantly with decreasing intake of soluble dietary fibre and n-3 fatty acids but with increasing intake of retinol. The odds of IADL impairment increased significantly with decreasing intakes of vitamins B2, B6 and B12. These results are consistent with a possible long-term neuroprotective effect of dietary fibre, n-3 polyunsaturated fats and B-group vitamins, and support dietary intervention to prevent cognitive decline. PMID:19203415

  14. Representation-based user interfaces for the audiovisual library of the year 2000

    NASA Astrophysics Data System (ADS)

    Aigrain, Philippe; Joly, Philippe; Lepain, Philippe; Longueville, Veronique

    1995-03-01

    The audiovisual library of the future will be based on computerized access to digitized documents. In this communication, we address the user interface issues which will arise from this new situation. One cannot simply transfer a user interface designed for the piece by piece production of some audiovisual presentation and make it a tool for accessing full-length movies in an electronic library. One cannot take a digital sound editing tool and propose it as a means to listen to a musical recording. In our opinion, when computers are used as mediations to existing contents, document representation-based user interfaces are needed. With such user interfaces, a structured visual representation of the document contents is presented to the user, who can then manipulate it to control perception and analysis of these contents. In order to build such manipulable visual representations of audiovisual documents, one needs to automatically extract structural information from the documents contents. In this communication, we describe possible visual interfaces for various temporal media, and we propose methods for the economically feasible large scale processing of documents. The work presented is sponsored by the Bibliotheque Nationale de France: it is part of the program aiming at developing for image and sound documents an experimental counterpart to the digitized text reading workstation of this library.

  15. Comparison of the Explantation Rate of Poly Implant Prothèse, Allergan, and Pérouse Silicone Breast Implants within the First Four Years after Reconstructive Surgery before the Poly Implant Prothèse Alert by the French Regulatory Authority

    PubMed Central

    Leduey, Alexandre; Mazouni, Chafika; Leymarie, Nicolas; Alkhashnam, Heba; Sarfati, Benjamin; Garbay, Jean-Rémi; Gaudin, Amélie; Kolb, Frédéric; Rimareix, Françoise

    2015-01-01

    Background. In March 2010, ANSM (Agence Nationale de Sécurité du Medicament), the French Medical Regulatory Authority, withdrew Poly Implant Prothèse (PIP) breast implants from the market due to the use of non-medical-grade silicone gel. The aim of this study was to compare the removal rate (and reasons thereof) of breast implants produced by different manufacturers before the ANSM alert. Materials and Methods. From October 2006 to January 2010, 652 women received 944 implants after breast cancer surgery at the Gustave Roussy Comprehensive Cancer Center, Paris (France). The complications and removal rates of the different implant brands used (PIP, Allergan, and Pérouse) were evaluated and compared. Results. PIP implants represented 50.6% of the used implants, Allergan 33.4%, and Pérouse 16%. The main reasons for implant removal were patient dissatisfaction due to aesthetic problems (43.2%), infection (22.2%), and capsular contracture (13.6%). Two years after implantation, 82% of Pérouse implants, 79% of PIP, and 79% of Allergan were still in situ. There was no difference in removal rate among implant brands. Conclusion. Before the ANSM alert concerning the higher rupture rate of PIP breast implants, our implant removal rate did not predict PIP implant failure related to the use of nonapproved silicone gel. PMID:26543648

  16. Dioxin and dl-PCB exposure from food: the German LExUKon project.

    PubMed

    Schwarz, Markus A; Lindtner, Oliver; Blume, Katrin; Heinemeyer, Gerhard; Schneider, Klaus

    2014-04-01

    Polychlorinated dibenzo-p-dioxin and -furan (PCDD/F) and dioxin-like polychlorinated biphenyl (dl-PCB) exposure from food were estimated using new food consumption data from the recent German food consumption survey (Nationale Verzehrsstudie II - NVS II). Based on these comprehensive data, information on the consumption of 545 individual food items by the German population was derived. Concentrations of dioxin-like compounds in food were compiled from the German Food Monitoring Programme (GFMP), the German Dioxin Database, other German authority programmes, European countries' authority programmes and the published literature covering the years 2000-2010. By multiplication with consumption data, estimates of intake from food were determined. The main food groups contributing most to the intake of the general public are dairy products (including milk), meat and fish (including seafood), followed - due to high consumption - by the main group vegetables. The combined intake of PCDD/F and dl-PCB (as toxic equivalents - TEQ) from food was estimated to be 2.11/1.53 pg kg(-1) bw and day and 3.56/2.85 pg kg(-1) bw and day (upper/lower bound) for average and high-end consumers, respectively. The estimated intake of average consumers is close to a reference value derived by the Scientific Committee on Food in 2001. Uncertainties in these estimates pertain to the influence of values below the limit of quantification (upper/lower bound ratio) and some foods not considered due to the lack of contamination data. PMID:24405321

  17. Experimental results of an iodine plasma in PEGASES gridded thruster

    NASA Astrophysics Data System (ADS)

    Grondein, Pascaline; Aanesland, Ane

    2015-09-01

    In the electric gridded thruster PEGASES, both positive and negative ions are expelled after extraction from an ion-ion plasma. This ion-ion plasma is formed downstream a localized magnetic field placed a few centimeters from the ionization region, trapping and cooling down the electron to allow a better attachment to an electronegative gas. For this thruster concept, iodine has emerged as the most attractive option. Heavy, under diatomic form and therefore good for high thrust, its low ionization threshold and high electronegativity lead to high ion-ion densities and low RF power. After the proof-of-concept of PEGASES using SF6 as propellant, we present here experimental results of an iodine plasma studied inside PEGASES thruster. At solid state at standard temperature and pressure, iodine is heated to sublimate, then injected inside the chamber where the neutral gas is heated and ionized. The whole injection system is heated to avoid deposition on surfaces and a mass flow controller allows a fine control on the neutral gas mass flow. A 3D translation stage inside the vacuum chamber allows volumetric plasma studies using electrostatic probes. The results are also compared with the global model dedicated to iodine as propellant for electric gridded thrusters. This work has been done within the LABEX Plas@par project, and received financial state aid managed by the Agence Nationale de la Recherche, as part of the programme ``Investissements d'avenir.''

  18. What make differences in the outcome of adjuvant treatments for resected gastric cancer?

    PubMed Central

    Nakajima, Toshifusa; Fujii, Masashi

    2014-01-01

    After a long history of Dark Age of adjuvant chemotherapy for gastric cancer, definite evidences of survival benefit from adjuvant treatment have been reported since 2000s. These survival benefits are likely attributed to something new approach different from pervious studies. In 2001, South West Oncology Group INT0116 trial yielded survival benefit in curatively resected gastric cancer patients with postoperative chemoradiotherapy [5-fluorouracil (5-FU) + Leucovorin + radiotherapy], followed by positive result by MAGIC Trial, employing peri-operative(pre- and postoperative chemotherapy with Epirubicin, cisplatin (CDDP), 5-fluorouracil (ECF) regimen in patients with curative resection. A novel drug [S1: ACTS-GC (Adjuvant chemotherapy trial of TS-1 for gastric cancer) in 2007], or new drug combination chemotherapys [CDDP + 5-FU: FNCLCC/FFCD (Federation Nationale des Centres de Lutte contre le cancer/Federation Francophone de Cancerologie Digestive) in 2011, Capecitabine + Oxaliplatin: CLASSIC in 2012] also produced positive results in terms of improved prognosis. Neoadjuvant or perioperative chemotherapy, novel anti-cancer drugs, and chemoradiotherapy might be the key words to develop further improvement in the adjuvant treatment of resectable gastric cancer. Moreover, it is not new but still true to stress the importance of D2 surgery as the baseline treatment in order to minimize the amount of residual tumor after surgery. PMID:25206264

  19. Comparison of the Explantation Rate of Poly Implant Prothèse, Allergan, and Pérouse Silicone Breast Implants within the First Four Years after Reconstructive Surgery before the Poly Implant Prothèse Alert by the French Regulatory Authority.

    PubMed

    Leduey, Alexandre; Mazouni, Chafika; Leymarie, Nicolas; Alkhashnam, Heba; Sarfati, Benjamin; Garbay, Jean-Rémi; Gaudin, Amélie; Kolb, Frédéric; Rimareix, Françoise

    2015-01-01

    Background. In March 2010, ANSM (Agence Nationale de Sécurité du Medicament), the French Medical Regulatory Authority, withdrew Poly Implant Prothèse (PIP) breast implants from the market due to the use of non-medical-grade silicone gel. The aim of this study was to compare the removal rate (and reasons thereof) of breast implants produced by different manufacturers before the ANSM alert. Materials and Methods. From October 2006 to January 2010, 652 women received 944 implants after breast cancer surgery at the Gustave Roussy Comprehensive Cancer Center, Paris (France). The complications and removal rates of the different implant brands used (PIP, Allergan, and Pérouse) were evaluated and compared. Results. PIP implants represented 50.6% of the used implants, Allergan 33.4%, and Pérouse 16%. The main reasons for implant removal were patient dissatisfaction due to aesthetic problems (43.2%), infection (22.2%), and capsular contracture (13.6%). Two years after implantation, 82% of Pérouse implants, 79% of PIP, and 79% of Allergan were still in situ. There was no difference in removal rate among implant brands. Conclusion. Before the ANSM alert concerning the higher rupture rate of PIP breast implants, our implant removal rate did not predict PIP implant failure related to the use of nonapproved silicone gel. PMID:26543648

  20. Turbulent Flows Driven by the Mechanical Forcing of an Ellipsoidal Container

    NASA Astrophysics Data System (ADS)

    Favier, Benjamin; Le Bars, Michael; Grannan, Alexander; Ribeiro, Adolfo; Aurnou, Jonathan; Irphe Team; Spinlab Team

    2015-11-01

    We present a combination of laboratory experiments and numerical simulations modelling geophysically relevant mechanical forcings. Libration and tides correspond to the periodic perturbation of a body's rotation rate and shape, and are both due to gravitational interactions with orbiting companions. Such mechanical forcings can convey a fraction of the rotational energy available and generate intense turbulence in the fluid interior of satellites and planets. We investigate the fluid motions inside a librating or tidally deformed triaxial ellipsoidal container filled with an incompressible fluid. In both cases, the turbulent flow is driven by the elliptic instability which is a triadic resonance between two inertial modes and the base flow. We characterize the transition to turbulence as triadic resonances develop while also investigating both intermittent and sustained regimes. It is shown that the flow is largely independent of the properties of the mechanical forcing, hinting at a possible universal behaviour of the saturated elliptical instability. The existence of such intense flows may play an important role in understanding the thermal and magnetic evolution of celestial bodies. This work was funded by the French Agence Nationale pour la Recherche and the National Science Foundation Geophysics Program.

  1. The Aeroclipper: A new instrument for quasi-Lagrangian measurements at the air-sea interface

    NASA Astrophysics Data System (ADS)

    Duvel, J. P.; Reverdin, G.; Pichon, T.; Vargas, A.

    The Aeroclipper is a new balloon developed by CNES. The Aeroclipper is a balloon equipped with a cable extended by a guide-rope in contact with the surface of the ocean. The balloon is vertically stabilised at a given height (currently 40 to 60m above the sea surface) and move on quasi-Lagrangian trajectories depending on the surface wind. LMD (Laboratoire de Méteorologie Dynamique), LodyC (Laboratoire d'océanographie physique et de Climatologie) and ENSTA (Ecole Nationale Supérieure de Techniques Avancées) developed an instrumentation adapted to this new measurement system. This instrumentation is distributed on one atmospheric gondola and one oceanic gondola. The aim is to measure surface physical parameters (Air and sea surface temperatures, sea surface salinity, wind, pressure and humidity) and to derive turbulent fluxes of moisture, heat and momentum. The Aeroclippers will give legs of the different parameters at a relatively high spatial resolution and thus information on the perturbation of these parameters at mesoscale. A first test of the full system will be performed from Banyuls (France) during spring 2004. The first scientific use of the Aeroclipper is planned in February 2005 in the Indian Ocean South of the Equator in link with the pilot phase of the Vasco (Variability of the Atmosphere at the intra-Seasonal time scale and Coupling with the Ocean) experiment.

  2. The FRIPON and Vigie-Ciel networks

    NASA Astrophysics Data System (ADS)

    Colas, François; Zanda, Brigitte; Bouley, Sylvain; Vaubaillon, Jérémie; Vernazza, Pierre; Gattacceca, Jérôme; Marmo, Chiara; Audureau, Yoan; Kwon, Min Kyung; Maquet, Lucie; Rault, Jean-Louis; Birlan, Mirel; Egal, Auriane; Rotaru, Monica; Birnbaum, Cyril; Cochard, François; Thizy, Olivier

    2014-02-01

    FRIPON (Fireball Recovery and interplanetary Observation Network) is a French fireball network recently founded by ANR (Agence Nationale de la Recherche). His aim is to connect meteoritical science with asteroidal and cometary sciences in order to better understand the solar system formation and evolution. The main idea is to cover all the French territory in order to collect a large number of meteorites (one or two per year) with an accurate orbit computation allowing us to pinpoint the parent bodies of the meteorites. About 100 allsky cameras will be installed in 2015 to create a dense network with an average distance of 100 km between two stations. In order to maximize the accuracy of orbit determination, we will mix our optical data with radar data from the GRAVES beacon received by 25 stations (Rault, 2014). As the network installation and the creation of the research teams for meteorites need many persons, at least much more than our small team of professionals, we will develop in parallel a participative science network for amateurs called Vigie-Ciel. As FRIPON is an open project, anybody will be able to buy a "FRIPON like" camera to be within the network, using our FreeTure detection software (Audureau, 2014; Kwon, 2014). Vigie-Ciel will also be used by observers using other types of cameras and by teams of meteorite researchers. Finally we will use the public affinity with meteors and meteorites to develop scientific activities to popularize science.

  3. Observing interferences between past and future quantum states in resonance fluorescence

    NASA Astrophysics Data System (ADS)

    Huard, Benjamin

    2014-03-01

    In quantum physics, measurement results are random but their statistics can be predicted at any time assuming some knowledge about the system in the past. Additional knowledge from a future measurement deeply changes these statistics in the present and leads to purely quantum features. In particular conditioned average outcomes of a weak measurement, so-called weak values, were shown to go beyond the conventional range, give a way to directly measure complex values, and can be used to enhance the sensitivity of quantum meters. Recently, these concepts have been considered in the general case of open quantum systems where decoherence occurs. Then, what are the properties of weak values for the unavoidable measurement associated to decoherence, the one performed by the environment? Here, we answer this question in the simplest open quantum system: a quantum bit in presence of a relaxation channel. We continuously monitor the fluorescence emitted by a superconducting qubit driven at resonance. Conditioned on initial preparation and final single shot measurement outcome of the qubit state, we probe weak values displaying all the above properties. The fluorescence signal exhibits interferences between oscillations associated to past or future quantum states. The measured data are in excellent agreement with a recently developed formalism. This work was supported by the Agence Nationale pour la Recherche grants ANR-12-JCJC-TIQS and ANR-13-JCJCINCAL.

  4. FOREWORD: International Conference on Heavy Ion Collisions in the LHC Era

    NASA Astrophysics Data System (ADS)

    Arleo, Francois; Salgado, Carlos A.; Tran Thanh Van, Jean

    2013-03-01

    The International Conference on Heavy Ion Collisions in the LHC Era was held in Quy Nhon, Vietnam, on 16-20 July 2012. The series Rencontres du Vietnam, created by Jean Tran Thanh Van in 1993, consists of international meetings aimed to stimulate the development of advanced research in Vietnam and more generally in South East Asia, and to establish collaborative research networks with Western scientific communities. This conference, as the whole series, also supports the International Center for Interdisciplinary Science Education being built in Quy Nhon. The articles published in this volume present the latest results from the heavy-ion collision programs of RHIC and LHC as well as the corresponding theoretical interpretation and future perspectives. Lower energy nuclear programs were also reviewed, providing a rather complete picture of the state-of-the-art in the field. We wish to thank the sponsors of the Conference on Heavy Ion Collisions in the LHC Era: the European Research Council; Xunta de Galicia (Spain); EMMI (Germany) and Agence Nationale de la Recherche (France) François Arleo (Laboratoire d'Annecy-le-Vieux de Physique Théorique, France) Francois Arleo, Carlos A Salgado and Jean Tran Thanh Van Conference photograph

  5. Patentierung und Patentlage

    NASA Astrophysics Data System (ADS)

    Herrmann, Uwe

    Gewerbliche Schutzrechte nehmen in der nationalen Rechts- und Wirtschaftsordnung sowie auch auf internationaler Ebene stetig an Bedeutung zu. Sie dienen dem Schutz geistigen Eigentums und sind für jeden Gewerbetreibenden nicht nur im Hinblick darauf von Bedeutung, eigene Rechte zu sichern, sondern auch insofern von Relevanz, dass ein Verstoß gegen Rechte Dritter zu vermeiden ist. Zu den gewerblichen Schutzrechten gehören unter anderem Kennzeichenrechte, Geschmacksmusterrechte sowie die sogenannten technischen Schutzrechte in Form des Patents sowie des Gebrauchsmusters. Die folgenden Ausführungen befassen sich ausschließlich mit den technischen Schutzrechten und geben eine kurze Einführung in die Voraussetzungen, das Entstehen und den Wegfall sowie in die Wirkungen technischer Schutzrechte. Beleuchtet wird die Situation im Wesentlichen im Hinblick auf nationale technische Schutzrechte, d. h. auf Deutsche Patente und Gebrauchsmuster sowie auf Europäische Patente, die Schutz in Deutschland entfalten. Die Möglichkeit der Erlangung von Schutzrechten im außereuropäischen Ausland wird nur am Rande gestreift.

  6. Prognostic relevance of a novel proliferation marker, Ki-S11, for soft-tissue sarcoma. A multivariate study.

    PubMed Central

    Rudolph, P.; Kellner, U.; Chassevent, A.; Collin, F.; Bonichon, F.; Parwaresch, R.; Coindre, J. M.

    1997-01-01

    In 132 soft-tissue sarcomas and 52 benign soft-tissue tumors, cellular proliferation was examined by immunohistochemistry using monoclonal antibodies Ki-S11 (Ki-67 antigen) and Ki-S1 (topoisomerase II alpha) and by flow cytometric analysis of the S-phase fraction (SPF). Malignant tumors were graded histologically according to the Fédération Nationale des Centres de Lutte Contre le Cancer (FNCLCC) system. Patient age, sex, tumor location, histological type, and DNA ploidy were considered as additional prognostic variables. Consistent immunoreactivity was seen in approximately 95% of the cases, and determination of SPF was possible in approximately 60% Ki-S11 and Ki-S1 immunolabeling indices correlated in a linear manner. All proliferation parameters yielded significant differences between benign and malignant tumors. Ki-S11 and Ki-S1 immunoreactive scores also co-varied significantly with SPF, mitotic count, and histopathological grade. In univariate analysis, immunohistochemical proliferation indices, histopathological grade, mitotic count, and SPF were predictive of overall survival and the development of metastases. In multivariate analysis, immunolabeling scores of proliferation markers, grade, and SPF emerged as independent predictors of global survival and systemic progression. We conclude that the immunohistochemical assessment of proliferation, being more readily performable and more easily assessable than the equally relevant S phase fraction, may add appreciable information to the current prognostic models for soft-tissue sarcoma. Images Figure 1 Figure 2 Figure 3 PMID:9176393

  7. [Pica in tunisian children. Results of a survey performed in a polyclinic of the tunisian social security national administration].

    PubMed

    Karoui, A; Karoui, H

    1993-01-01

    During a 15 month-period, 63, 10 to 59 month-old children, with pica habits were collected in a day care centre of the Caisse nationale de sécurité sociale in Tunis. Anemia was the main alert sign. They were compared with 43 non pica children presenting with a similar degree of anemia. The male to female ratio was 1.42. A family history of pica was present in 57% of the cases. Most children ingested earth but 50% of the patients ingested multiple substances. The beginning of the eating disorder was observed between 12 and 18 months in 71% of the cases. 95% of pica patients were from low income parents and urban status. No differences were observed between the pica children and the anemic children without pica habits in term of anamnestic, clinical and biological data. Treatment with iron supplements led to cessation of pica in most patients. The physiopathological hypothesis were dominated by iron and zinc deficiency of which geophagia can be, at the same time, the cause and the consequence. From our study, pica appears to remain very frequent among Tunisian children. Its prevention requires information of parents and dietary prevention of early iron deficiency. PMID:8165119

  8. The PEGASES gridded ion-ion thruster physics, performance and predictions

    NASA Astrophysics Data System (ADS)

    Aanesland, Ane; Rafalskyi, Dmytro; Bredin, Jerome; Grondein, Pascaline; Oudini, Noureddine; Chabert, Pascal

    2013-09-01

    The PEGASES (Plasma propulsion with Electronegative gases) thruster is a gridded ion thruster that accelerates alternately positively and negatively charged ions to provide thrust. Over the last years various prototypes have been tested, adequate diagnostics have been developed and analytical models and simulations are made to better understand and control the physics involved. The plasma density in the region of the ion-ion plasma predicts that the performance of the PEGASES thruster can be comparable to existing thrusters on the market. We have recently provided the first experimental proof-of-concept, accelerating alternately positive and negative ions from an ion-ion plasma within a 10 kHz cycle. Here we present the state of the art in the PEGASES development and discuss the various physics involved and its possible future in space. This work is funded by EADS Astrium, ANR (Agence nationale de la recherche) under contract ANR-11-BS09-040 and FP7 under contract PIIF-GA-2012-326054.

  9. "Applied science": a phrase in search of a meaning.

    PubMed

    Bud, Robert

    2012-09-01

    The term "applied science," as it came to be popularly used in the 1870s, was a hybrid of three earlier concepts. The phrase "applied science" itself had been coined by Samuel Taylor Coleridge in 1817, translating the German Kantian term "angewandte Wissenschaft." It was popularized through the Encyclopaedia Metropolitana, which was structured on principles inherited from Coleridge and edited by men with sympathetic views. Their concept of empirical as opposed to a priori science was hybridized with an earlier English concept of "practical science" and with "science applied to the arts," adopted from the French. Charles Dupin had favored the latter concept and promoted it in the reconstruction of the Conservatoire Nationale des Arts et Métiers. The process of hybridization took place from the 1850s, in the wake of the Great Exhibition, as a new technocratic government favored scientific education. "Applied science" subsequently was used as the epistemic basis for technical education and the formation of new colleges in the 1870s. PMID:23286192

  10. A French-speaking speech-language pathology program in West Africa: transfer of training between Minority and Majority World countries.

    PubMed

    Topouzkhanian, Sylvia; Mijiyawa, Moustafa

    2013-02-01

    In West Africa, as in Majority World countries, people with a communication disability are generally cut-off from the normal development process. A long-term involvement of two partners (Orthophonistes du Monde and Handicap International) allowed the implementation in 2003 of the first speech-language pathology qualifying course in West Africa, within the Ecole Nationale des Auxiliaires Medicaux (ENAM, National School for Medical Auxiliaries) in Lome, Togo. It is a 3-year basic training (after the baccalaureate) in the only academic training centre for medical assistants in Togo. This department has a regional purpose and aims at training French-speaking African students. French speech-language pathology lecturers had to adapt their courses to the local realities they discovered in Togo. It was important to introduce and develop knowledge and skills in the students' system of reference. African speech-language pathologists have to face many challenges: creating an African speech and language therapy, introducing language disorders and their possible cure by means other than traditional therapies, and adapting all the evaluation tests and tools for speech-language pathology to each country, each culture, and each language. Creating an African speech-language pathology profession (according to its own standards) with a real influence in West Africa opens great opportunities for schooling and social and occupational integration of people with communication disabilities. PMID:23323818

  11. 3D Model of Surfactant Replacement Therapy

    NASA Astrophysics Data System (ADS)

    Grotberg, James; Tai, Cheng-Feng; Filoche, Marcel

    2015-11-01

    Surfactant Replacement Therapy (SRT) involves instillation of a liquid-surfactant mixture directly into the lung airway tree. Though successful in neonatal applications, its use in adults had early success followed by failure. We present the first mathematical model of 3D SRT where a liquid plug propagates through the tree from forced inspiration. In two separate modeling steps, the plug first deposits a coating film on the airway wall which subtracts from its volume, a ``coating cost''. Then the plug splits unevenly at the airway bifurcation due to gravity. The steps are repeated until a plug ruptures or reaches the tree endpoint alveoli/acinus. The model generates 3D images of the resulting acinar distribution and calculates two global indexes, efficiency and homogeneity. Simulating published literature, the earlier successful adult SRT studies show comparatively good index values, while the later failed studies do not. Those unsuccessful studies used smaller dose volumes with higher concentration mixtures, apparently assuming a well mixed compartment. The model shows that adult lungs are not well mixed in SRT due to the coating cost and gravity effects. Returning to the higher dose volume protocols could save many thousands of lives annually in the US. Supported by NIH Grants HL85156, HL84370 and Agence Nationale de la Recherche, ANR no. 2010-BLAN-1119-05.

  12. Illicit material detector based on gas sensors and neural networks

    NASA Astrophysics Data System (ADS)

    Grimaldi, Vincent; Politano, Jean-Luc

    1997-02-01

    In accordance with its missions, le Centre de Recherches et d'Etudes de la Logistique de la Police Nationale francaise (CREL) has been conducting research for the past few years targeted at detecting drugs and explosives. We have focused our approach of the underlying physical and chemical detection principles on solid state gas sensors, in the hope of developing a hand-held drugs and explosives detector. The CREL and Laboratory and Scientific Services Directorate are research partners for this project. Using generic hydrocarbon, industrially available, metal oxide sensors as illicit material detectors, requires usage precautions. Indeed, neither the product's concentrations, nor even the products themselves, belong to the intended usage specifications. Therefore, the CREL is currently investigating two major research topics: controlling the sensor's environment: with environmental control we improve the detection of small product concentration; determining detection thresholds: both drugs and explosives disseminate low gas concentration. We are attempting to quantify the minimal concentration which triggers detection. In the long run, we foresee a computer-based tool likely to detect a target gas in a noisy atmosphere. A neural network is the suitable tool for interpreting the response of heterogeneous sensor matrix. This information processing structure, alongside with proper sensor environment control, will lessen the repercussions of common MOS sensor sensitivity characteristic dispersion.

  13. Layering from anticyclonic vortices in a rotating stratified medium with combined salinity and temperature effects

    NASA Astrophysics Data System (ADS)

    Sommeria, Joel; Burin, Michael; Viboud, Samuel

    2015-11-01

    We generate anticyclonic vortices by a fluid source in a rotating and uniformly stratified medium, a laboratory model of long lived vortex lenses in the ocean. Experiments are performed in the large `Coriolis' rotating platform at Grenoble, 13 m in diameter, providing previously unaccessible turbulent regimes. The other novelty is to combine temperature and salinity effects, like in `meddies', vortices formed by intrusion in the Atlantic ocean of warm and salty water from the Mediterranean Sea. For both heated an unheated cases, we observe shear driven instability at the vortex periphery, leading to the emission of material filament from a large-scale m=2 instability. Heated vortices behave much the same way but with two key additions. One, prominent at early times, is that the vortex edge appears serrated around most of its circumference in the upper part of the lens. Two, clearer for later times, a staircase density profile develops above the eddy. We explain this small scale turbulence as thermal convection in the statically unstable density profile resulting from selective vertical diffusion of temperature (while salinity is less diffusive). The resulting turbulent mixing generates horizontal intrusions at the upper part of the vortex, unlike the double-diffusive instability. This work has been funded by Agence Nationale de la Recherche (ANR), project `OLA'.

  14. Elastic moduli of hard c-Zr3N4 and η-Ta2N3, a tough self-healing material, via laser ultrasonics and nanoindentation

    NASA Astrophysics Data System (ADS)

    Zerr, Andreas; Chigarev, Nikolay; Bourguille, Judith; Tetard, Florent; Brinza, Ovidiu; Nikitin, Sergey; Lomonosov, Alexey; Gusev, Vitalyi

    2013-06-01

    Bulk and shear moduli (B0 and G0) of the dense polycrystalline oxygen bearing c-Zr3N4 and η-Ta2N3 were determined from the laser ultrasonic (LU) measurements on highly porous samples having the volume fraction porosity of 0.23 and 0.18, respectively. Dense samples of these high-pressure (HP) materials are today not available due to their very high hardness and absence of a densification procedure. Combining the LU data with a numerical analysis of the sample porosity, the ``true'' isotropic moduli were determined to be B0 = 217(20) GPa and G0 = 163(9) GPa, for c-Zr3N4, and B0 = 281(15) GPa and G0 = 123(2) GPa, for η-Ta2N3. For both HP-nitrides the B0 values agree with those obtained earlier via the HP compression measurements in a diamond anvil cell. Also, the self-healing behavior of η-Ta2N3 by mechanical polishing was confirmed by two independent methods. Finally, the results obtained for η-Ta2N3 via the LU method were compared with our nanoindentation measurements. The high G0 value of c-Zr3N4 suggests that this material could vie with γ-Si3N4 for the rank of the third hardest material after diamond and c-BN. Supported by the Agence Nationale de la Recherche (France).

  15. Proposal for laser cooling of rare-earth ions

    NASA Astrophysics Data System (ADS)

    Dulieu, Olivier; Hong, Ye; Wyart, Jean-François; Lepers, Maxence

    2016-05-01

    The efficiency of laser cooling relies on the existence of an almost closed optical-transition cycle in the energy spectrum of the considered species. In this respect, rare-earth elements exhibit many transitions which are likely to induce noticeable leaks from the cooling cycle. In this work, to determine whether laser cooling of singly ionized erbium Er+ is feasible, we have performed accurate electronic-structure calculations of energies and spontaneous-emission Einstein coefficients of Er+, using a combination of ab initio and least-squares-fitting techniques. We identify five weak closed transitions suitable for laser cooling, the broadest of which is in the kilohertz range. For the strongest transitions, by simulating the cascade dynamics of spontaneous emission, we show that repumping is necessary, and we discuss possible repumping schemes.We expect our detailed study on Er+ to give good insight into the laser cooling of neighboring ions such as Dy+. Supported by ``Agence Nationale de la Recherche'' (ANR), under the project COPOMOL (Contract No. ANR-13-IS04-0004-01).

  16. HIV preventive vaccine research at the ANRS: the lipopeptide vaccine approach.

    PubMed

    Gahery, Hanne; Choppin, Jeannine; Bourgault, Isabelle; Fischer, Elizabeth; Maillère, Bernard; Guillet, Jean-Gèrard

    2005-01-01

    The HIV (human immunodeficiency virus)/AIDS epidemic is of unprecedented gravity and is spreading rapidly, notably in the most disadvantaged regions of the world. The search for a preventive vaccine is thus an absolute priority. For over 10 years the ANRS (Agence Nationale de Recherches sur le SIDA) has been committed to an original programme combining basic science and clinical research. The HIV preventive vaccine research programme includes upstream research for the definition of immunogens, animal models, and clinical research to evaluate candidate vaccines. In 2004, most researchers believed that it should be possible to obtain partial vaccine protection through the induction of a strong and multiepitopic cellular response. Since 1992, 15 phase I and II clinical trials have been established with the aim of evaluating the safety of candidate vaccines and their capacity to induce cellular immune responses. The candidate vaccines tested were recombinant canarypox viruses (ALVAC) containing sequences coding for certain viral proteins, utilised alone or combined with other immunogens (whole or truncated envelope proteins). An original strategy, based on the use of lipopeptides, is also under development. These vaccines comprise synthetic fragments of HIV proteins associated with lipids that facilitate the induction of a cellular immune response. These approaches have within a short time allowed the assessment of a prime-boost strategy combining a viral vector and lipopeptides. PMID:16128266

  17. FRIPON, the French fireball network

    NASA Astrophysics Data System (ADS)

    Colas, F.; Zanda, B.; Bouley, S.; Vaubaillon, J.; Marmo, C.; Audureau, Y.; Kwon, M. K.; Rault, J. L.; Caminade, S.; Vernazza, P.; Gattacceca, J.; Birlan, M.; Maquet, L.; Egal, A.; Rotaru, M.; Gruson-Daniel, Y.; Birnbaum, C.; Cochard, F.; Thizy, O.

    2015-10-01

    FRIPON (Fireball Recovery and InterPlanetary Observation Network) [4](Colas et al, 2014) was recently founded by ANR (Agence Nationale de la Recherche). Its aim is to connect meteoritical science with asteroidal and cometary science in order to better understand solar system formation and evolution. The main idea is to set up an observation network covering all the French territory to collect a large number of meteorites (one or two per year) with accurate orbits, allowing us to pinpoint possible parent bodies. 100 all-sky cameras will be installed at the end of 2015 forming a dense network with an average distance of 100km between stations. To maximize the accuracy of orbit determination, we will mix our optical data with radar data from the GRAVES beacon received by 25 stations [5](Rault et al, 2015). As both the setting up of the network and the creation of search teams for meteorites will need manpower beyond our small team of professionals, we are developing a citizen science network called Vigie-Ciel [6](Zanda et al, 2015). The public at large will thus be able to simply use our data, participate in search campaigns or even setup their own cameras.

  18. Costless Platform for High Resolution Stereoscopic Images of a High Gothic Facade

    NASA Astrophysics Data System (ADS)

    Héno, R.; Chandelier, L.; Schelstraete, D.

    2012-07-01

    In October 2011, the PPMD specialized master's degree students (Photogrammetry, Positionning and Deformation Measurement) of the French ENSG (IGN's School of Geomatics, the Ecole Nationale des Sciences Géographiques) were asked to come and survey the main facade of the cathedral of Amiens, which is very complex as far as size and decoration are concerned. Although it was first planned to use a lift truck for the image survey, budget considerations and taste for experimentation led the project to other perspectives: images shot from the ground level with a long focal camera will be combined to complementary images shot from what higher galleries are available on the main facade with a wide angle camera fixed on a horizontal 2.5 meter long pole. This heteroclite image survey is being processed by the PPMD master's degree students during this academic year. Among other type of products, 3D point clouds will be calculated on specific parts of the facade with both sources of images. If the proposed device and methodology to get full image coverage of the main facade happen to be fruitful, the image acquisition phase will be completed later by another team. This article focuses on the production of 3D point clouds with wide angle images on the rose of the main facade.

  19. Acute Ischemia of Extremity as a First Manifestation of Peripheral Artery Leiomyosarcoma: Report of a Case and Review of the Literature.

    PubMed

    Voulalas, Grigorios; Giannakakis, Sotirios; Maltezos, Chrisostomos

    2016-07-01

    Leiomyosarcoma is an aggressive soft tissue sarcoma derived from smooth muscle cells. Of all soft tissue sarcomas, approximately 5-10% are leiomyosarcomas. Vascular leiomyosarcoma constitutes about 2% of all leiomyosarcomas and involves veins 5 times more than arteries. When they arise from a major blood vessel, symptoms of vascular compromise or leg edema may be present. Because they are rare, definite diagnosis is often delayed. We present the case of an 88-year-old man who was admitted to our department with acute limb ischemia stage 4 according to Rutherford's criteria. His personal medical history included arterial hypertension under medication with nonspecific conduction disturbances showed in the electrocardiography. The duplex scan revealed the presence of thrombotic material to the distal superficial femoral and popliteal artery, whereas the presence of popliteal artery aneurysm was excluded. After the initial diagnostic approach, he underwent 2 unsuccessful embolectomy procedures. During the amputation procedure, a 6-cm mass was palpated in the popliteal fossa, and it was excised. The immunohistopathologic study revealed a grade 3 according to the French Federation Nationale des Centers de Lutte Contre le Cancer classification leiomyosarcoma. The patient was discharged 10 days later and referred to an oncologic center. He returned 6 months later with edema of the amputated limb and inguinal lymphadenopathy. Specimen of the inguinal lymph nodes was sent for histopathologic examination, which indicated the recurrence of the disease. Leiomyosarcomas should be taken into consideration in elderly patients presenting with acute limb ischemia. PMID:26923155

  20. Evaluation d'un scenario d'apprentissage favorisant la mobilisation des habiletes reliees au processus d'enquete

    NASA Astrophysics Data System (ADS)

    Blanchard, Samuel F. J.

    Les resultats au Programme international pour le suivi des acquis des eleves (PISA) demontrent que les jeunes neobrunswickois francophones se classent b un niveau significativement inferieur comparaiivement aux eleves anglophones du Nouveau-Brunswick, aux eleves des autres provinces canadiennes et se classent sous la moyenne internationale de tous les pays participants quant b la culture scientifique. L'evaluation de cette culture scientifique est basee sur une serie de savoirs, de savoir-faire et de savoir-etre reliee au processus d'enquete scolaire. Le processus d'enquete scolaire est une approche b l'apprentissage ou les eleves effectuent des recherches d'informations, discutent d'idees et entreprennent des investigations pour augmenter leur comprehension d'un probleme ou d'un sujet. Les recherches demontrent que le processus d'enquete scolaire est rarement une composante pedagogique importante de la salle de classe et les recherches portant sur l'implantation du processus d'enquete scolaire recommandent de rendre ce dernier plus accessible aux enseignantes et aux enseignants. Afin de rendre le processus d'enquete plus accessible aux enseignantes et aux enseignants, notre recherche porte sur l'evaluation de la valeur pedagogique d'un scenario d'apprentissage (PhaRoboS) concu specialement pour creer un environnement dans lequel les eleves auront plusieurs occasions a mobiliser les habiletes reliees au processus d'enquete. Les retombees de cette evaluation nous permettront d'offrir des pistes de remediations afin d'aider plus d'enseignantes et d'enseignants b creer un environnement dans lequel les eleves auront plusieurs occasions b mobiliser les habiletes reliees au processus d'enquete. Cette evaluation s'est faite a partir d'une methodologie inspiree de l'evaluation pour fin d'amelioration d'un objet pedagogique. L'analyse des donnees qualitatives recueillies aupres des eleves et de leur enseignante d'une ecole francophone du Nouveau-Brunswick semble montrer que

  1. Large-scale Periodic Variability of the Wind of the Wolf-Rayet Star WR 1 (HD 4004)

    NASA Astrophysics Data System (ADS)

    Chené, A.-N.; St-Louis, N.

    2010-06-01

    We present the results of an intensive photometric and spectroscopic monitoring campaign of the WN4 Wolf-Rayet (WR) star WR 1 = HD 4004. Our broadband V photometry covering a timespan of 91 days shows variability with a period of P = 16.9+0.6 -0.3 days. The same period is also found in our spectral data. The light curve is non-sinusoidal with hints of a gradual change in its shape as a function of time. The photometric variations nevertheless remain coherent over several cycles and we estimate that the coherence timescale of the light curve is of the order of 60 days. The spectroscopy shows large-scale line-profile variability which can be interpreted as excess emission peaks moving from one side of the profile to the other on a timescale of several days. Although we cannot unequivocally exclude the unlikely possibility that WR 1 is a binary, we propose that the nature of the variability we have found strongly suggests that it is due to the presence in the wind of the WR star of large-scale structures, most likely corotating interaction regions (CIRs), which are predicted to arise in inherently unstable radiatively driven winds when they are perturbed at their base. We also suggest that variability observed in WR 6, WR 134, and WR 137 is of the same nature. Finally, assuming that the period of CIRs is related to the rotational period, we estimate the rotation rate of the four stars for which sufficient monitoring has been carried out, i.e., v rot = 6.5, 40, 70, and 275 km s-1 for WR 1, WR 6, WR 134, and WR 137, respectively. Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de Recherche Scientifique of France, and the University of Hawaii. Also based on observations obtained at the Observatoire du Mont Mégantic with is operated by the Centre de Recherche en Astrophysique du Québec and the Observatoire de

  2. The MiMeS survey of magnetism in massive stars: CNO surface abundances of Galactic O stars

    NASA Astrophysics Data System (ADS)

    Martins, F.; Hervé, A.; Bouret, J.-C.; Marcolino, W.; Wade, G. A.; Neiner, C.; Alecian, E.; Grunhut, J.; Petit, V.

    2015-03-01

    Context. The evolution of massive stars is still partly unconstrained. Mass, metallicity, mass loss, and rotation are the main drivers of stellar evolution. Binarity and the magnetic field may also significantly affect the fate of massive stars. Aims: Our goal is to investigate the evolution of single O stars in the Galaxy. Methods: For that, we used a sample of 74 objects comprising all luminosity classes and spectral types from O4 to O9.7. We relied on optical spectroscopy obtained in the context of the MiMeS survey of massive stars. We performed spectral modelling with the code CMFGEN. We determined the surface properties of the sample stars, with special emphasis on abundances of carbon, nitrogen, and oxygen. Results: Most of our sample stars have initial masses in the range of 20 to 50 M⊙. We show that nitrogen is more enriched and carbon and oxygen are more depleted in supergiants than in dwarfs, with giants showing intermediate degrees of mixing. CNO abundances are observed in the range of values predicted by nucleosynthesis through the CNO cycle. More massive stars, within a given luminosity class, appear to be more chemically enriched than lower mass stars. We compare our results with predictions of three types of evolutionary models and show that for two sets of models, 80% of our sample can be explained by stellar evolution including rotation. The effect of magnetism on surface abundances is unconstrained. Conclusions: Our study indicates that in the 20-50 M⊙ mass range, the surface chemical abundances of most single O stars in the Galaxy are fairly well accounted for by stellar evolution of rotating stars. Based on observations obtained at 1) the Telescope Bernard Lyot (USR5026) operated by the Observatoire Midi-Pyrénées, Université de Toulouse (Paul Sabatier), Centre National de la Recherche Scientifique of France; 2) at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut

  3. Stokes IQUV magnetic Doppler imaging of Ap stars - I. ESPaDOnS and NARVAL observations

    NASA Astrophysics Data System (ADS)

    Silvester, J.; Wade, G. A.; Kochukhov, O.; Bagnulo, S.; Folsom, C. P.; Hanes, D.

    2012-10-01

    high-resolution spectropolarimeters during the period 2006-2010. Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France and the University of Hawaii. Also based on observations obtained at the Bernard Lyot Telescope (TBL, Pic du Midi, France) of the Midi-Pyrénées Observatory, which is operated by the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France.

  4. Sur la nature des absorbeurs dans l'interpretation transactionnelle de la mecanique quantique

    NASA Astrophysics Data System (ADS)

    Boisvert, Jean-Sebastien

    L'interpretation transactionnelle de la mecanique quantique est l'une des plus recentes propositions de description des phenomenes du microcosme. En accord avec les predictions de la mecanique quantique standard, l'interpretation transactionnelle propose une alternative a celle de Copenhague. Son principal avantage est qu'elle permet de visualiser les mecanismes sous-jacents a l'echange d'energie, de quantite de mouvement ou d'autres quantites quantiques entre un emetteur et un absorbeur. Ces echanges sont le resultat, a l'instar de la theorie de l'absorbeur de Wheeler et Feynman, de l'utilisation autant d'ondes avancees que retardees. Bien que l'interpretation transactionnelle n'ait pas attire la plus grande attention scientifique, plusieurs critiques lui ont ete adressees. Dans les annees 1990, differentes experiences a mesure sans interaction ont ete concues. Depuis, il a ete avance que la version originale de l'interpretation transactionnelle pouvait difficilement rendre compte de ce type d'experience et meme qu'elle n'est pas compatible avec le concept d'univers quadridimensionnel. La recherche de ce memoire par article consiste a montrer que lorsque l'on utilise systematiquement l'interpretation transactionnelle en considerant la configuration totale des absorbeurs (incluant l'absorbeur universel), il n'est pas necessaire de faire appel a une hierarchie de transactions comme certains l'ont propose.

  5. Post-Secondary Students' Relationship to People They Consider to Be Scientific Experts

    NASA Astrophysics Data System (ADS)

    Pouliot, Chantal

    2011-03-01

    This article is situated in contemporary debates about the ways to achieve a scientific literacy that encourages a greater lay participation in public debates and political decision making. Drawing on the notion of "relationship to scientific experts" (in French, "rapport aux experts scientifiques"), I explore the ways in which a group of 3 Quebec post-secondary students describe the relationships they hold toward people whom they consider to be scientific experts, as revealed during a project in which they investigated the controversy surrounding cellular telephone use. To this end, I scrutinize how the members of the group go about describing scientific experts and picture a prospective face-to-face discussion with a scientific expert. The data come from a case study (conducted over a 15-week period). The findings show that the group maintains a relationship of intimidation by scientific experts, in which the latter are depicted in terms of their knowledge and qualifications. Accordingly, the group was overawed not only by the accumulation of knowledge held and produced by scientific experts but also by the latter's research experience and the high social recognition they occasionally enjoyed. Similarly, the group describes a prospective face-to-face discussion with a doctor or a researcher in terms of an impersonal, intimidating encounter during which its members' learning and comprehension in relation to the controversy are assumed to be unequal to the task. The implications of the findings for future research are discussed.

  6. Autisme et douleur – analyse bibliographique

    PubMed Central

    Dubois, Amandine; Rattaz, Cécile; Pry, René; Baghdadli, Amaria

    2010-01-01

    La présente analyse bibliographique a pour objectif de réaliser un bilan des travaux publiés dans le champ de la douleur et de l’autisme. L’article aborde, dans un premier temps, les études publiées concernant les modes d’expression de la douleur observés dans cette population. Différentes hypothèses permettant d’expliquer les particularités expressives des personnes avec autisme sont ensuite passées en revue : excès d’endorphines, particularités dans le traitement sensoriel, déficit sociocommunicatif. Cette analyse bibliographique aborde, pour terminer, la question de l’évaluation et de la prise en compte de la douleur chez les personnes avec autisme. Les auteurs concluent à l’absence d’homogénéité des résultats des études publiées et au besoin de poursuivre les recherches afin de parvenir à des données consensuelles sur un domaine d’étude encore peu exploité au plan scientifique. Sur un plan clinique, l’approfondissement des connaissances dans ce domaine devrait permettre de mettre au point des outils d’évaluation de la douleur et d’ainsi en assurer une meilleure prise en charge au quotidien. PMID:20808970

  7. L'astronomie au féminin

    NASA Astrophysics Data System (ADS)

    Nazé, Yaël

    2006-03-01

    Qui détient le record des découvertes de comètes ? Une femme. Qui a permis de comprendre comment est organisée la population des étoiles ? Une femme. Qui a découvert la loi permettant d'arpenter l'Univers, a trouvé des phares dans l'espace, a compris le fonctionnement des forges stellaires et a bouleversé notre vision de l'Univers ? Encore et toujours une femme... Pourtant, quand on doit citer un astronome -- historique -- au hasard, on pense le plus souvent -- des hommes : Ptolémée, Galilée, Copernic ou, plus près de nous par exemple, Hubble. Certes, au cours des siècles, les femmes n'ont guère eu accès aux sciences en général et -- l'astronomie en particulier mais ce n'est pas une raison pour croire en l'absence totale de contributions dues au beau sexe ! C'est ce que dévoile ici l'auteur. Loin de toute forme de féminisme enragé, on suivra le parcours de quelques scientifiques importantes qui ont par hasard en commun une même particularité : leur sexe.

  8. A Precise Measurement of the Deuteron Elastic Structure Function A(A2)

    SciTech Connect

    Andrian Honegger

    1999-12-01

    During summer 1997 experiment 394-018 measured the deuteron tensor polarization in D(e,e'd) scattering in Hall C at Jefferson Laboratory. In a momentum transfer range between 0.66 and 1:8 (GeV=c){sup 2}, with slight changes in the experimental setup, the collaboration performed six precision measurements of the deuteron structure function A(Q{sup 2}) in elastic D(e,e'd) scattering . Scattered electrons and recoil deuterons were detected in coincidence in the High Momentum Spectrometer and the recoil polarimeter POLDER, respectively. At every kinematics H(e,e') data were taken to study systematic effects of the measurement. These new precise measurements resolve discrepancies between older data sets and put significant constraints on existing models of the deuteron electromagnetic structure. This work was supported by the Swiss National Science Foundation, the French Centre National de la Recherche Scientifique and the Commissariat 'a l'Energie Atomique, the U.S. Department of Energy and the National Science Foundation and the K.C. Wong Foundation.

  9. VizieR Online Data Catalog: IRAM Observation Logs (IRAM 1991-2015)

    NASA Astrophysics Data System (ADS)

    Dan, M.; Neri, R.; Sievers, A.

    2008-04-01

    The Institut de Radio Astronomie Millimetrique (IRAM) was founded in 1979 and is operated as a French-German-Spanish collaboration. Its partner institutes are the CNRS (Centre National de la Recherche Scientifique, France), the MPG (Max Planck Gesellschaft, Germany), and the IGN (Instituto Geografico Nacional, Spain). The principal activity of IRAM is the study of cold matter (molecular gas and dust) in the solar system, in our Galaxy, and out to cosmological distances in order to determine its composition, density, mass, temperature, and kinematics. IRAM operates two observatories at millimeter wavelengths which are open to the international astronomical community: The 30-m single-dish telescope on Pico Veleta (2850m), Spain, and the six-antenna interferometer on the Plateau de Bure (2550m) in France. Both sites are at high altitude to reduce the absorption by water vapor. The observatories are supported by the IRAM offices and laboratories in Granada and Grenoble. The observation log included here concerns the Plateau de Bure site, and summarizes the observations made there from December 1990. The observations log of the 30-m single-dish telescope covers a period starting in January 2009. This log was produced using a header archive, a collaborative effort between IRAM and IAA/CSIC. (4 data files).

  10. A comparison of weak-lensing masses and X-ray properties of galaxy clusters

    NASA Astrophysics Data System (ADS)

    Hoekstra, Henk

    2007-07-01

    We present measurements of the masses of 20 X-ray luminous clusters of galaxies at intermediate redshifts, determined from a weak-lensing analysis of deep archival R-band data obtained using the Canada-France-Hawaii Telescope. Compared to previous work, our analysis accounts for a number of effects that are typically ignored, but can lead to small biases, or incorrect error estimates. We derive masses that are essentially model-independent and find that they agree well with measurements of the velocity dispersion of cluster galaxies and with the results of X-ray studies. Assuming a power law between the lensing mass and the X-ray temperature, M2500 ~ Tα, we find a best-fitting slope of α = 1.34+0.30-0.28. This slope agrees with self-similar cluster models and studies based on X-ray data alone. For a cluster with a temperature of kT = 5 keV we obtain a mass M2500 = (1.4 +/- 0.2)×1014h-1Msolar in fair agreement with recent Chandra and XMM studies. Based on observations from the Canada-France-Hawaii Telescope, which is operated by the National Research Council of Canada, le Centre National de la Recherche Scientifique and the University of Hawaii. E-mail: hoekstra@uvic.ca

  11. Discovery of the first τ Sco analogues: HD 66665 and HD 63425

    NASA Astrophysics Data System (ADS)

    Petit, V.; Massa, D. L.; Marcolino, W. L. F.; Wade, G. A.; Ignace, R.; Mimes Collaboration

    2011-03-01

    The B0.2 V magnetic star τ Sco stands out from the larger population of massive OB stars due to its high X-ray activity, peculiar wind diagnostics and highly complex magnetic field. This Letter presents the discovery of the first two τ Sco analogues - HD 66665 and HD 63425, identified by the striking similarity of their ultraviolet (UV) spectra to that of τ Sco. ESPaDOnS spectropolarimetric observations were secured by the Magnetism in Massive Stars CFHT Large Program, in order to characterize the stellar and magnetic properties of these stars. CMFGEN modelling of optical ESPaDOnS spectra and archived IUE UV spectra showed that these stars have stellar parameters similar to those of τ Sco. A magnetic field of similar surface strength is found on both stars, reinforcing the connection between the presence of a magnetic field and wind peculiarities. However, additional phase-resolved observations will be required in order to assess the potential complexity of the magnetic fields and verify if the wind anomalies are linked to this property. Based on observations obtained at the Canada--France--Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France and the University of Hawaii.

  12. Identification of More Interstellar C60+ Bands

    NASA Astrophysics Data System (ADS)

    Walker, G. A. H.; Bohlender, D. A.; Maier, J. P.; Campbell, E. K.

    2015-10-01

    Based on gas-phase laboratory spectra at 6 K, Campbell et al. confirmed that the diffuse interstellar bands (DIBs) at 9632.7 and 9577.5 Å are due to absorption by the fullerene ion {{{C}}}60+. They also reported the detection of two other, weaker bands at 9428.5 and 9365.9 Å. These lie in spectral regions heavily contaminated by telluric water vapor lines. We acquired CFHT ESPaDOnS spectra of HD 183143 close to the zenith and chopped with a nearby standard to correct for the telluric line absorption which enabled us to detect a DIB at 9365.9 Å of relative width and strength comparable to the laboratory absorption. There is a DIB of similar strength and FWHM at 9362.5 Å. A stellar emission feature at 9429 Å prevented detection of the 9428.5 Å band. However, a CFHT archival spectrum of HD 169454, where emission is absent at 9429 Å, clearly shows the 9428.5 Å DIB with the expected strength and width. These results further confirm {{{C}}}60+ as a DIB carrier. Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT), which is operated by the National Research Council of Canada, the Institut National des Sciences de l’Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  13. Modelisation et analyse de la reflectance de couverts forestiers de resineux

    NASA Astrophysics Data System (ADS)

    Fournier, Richard A.

    Une analyse de la reflectance de couverts forestiers de resineux constitue l'essentiel de ce projet de recherche. L'objectif pricipal de la demarche scientifique choisie vise a apporter des explications sur l'influence de l'architecture de la foret et des processus d'interaction entre l'eclairement solaire incident et le couvert forestier pour decrire les patrons de reflectance, tel que vue par un capteur numerique. La strategie de recherche s'opere en quatre etapes, c'est-a-dire (1) l'etude des patron radiometriques de couronnes d'arbres, (2) la comprehension du regime de lumiere dans le couvert, (3) la mesure et l'intetgration de l'architecture du couvert de l'echelle regionale jusqu'a la description detaillee de l'arbre et (4) la simulation et la validation des images numeriques a fine resolution spatiale (autour de 50 cm). Ces travaux ont fait ressortir les parametres directeurs pour expliquer la reflectance des couverts forestiers de resineux, donc de fournir une clarification du probleme dans son ensemble.

  14. Plasma membrane NADH oxidase of maize roots responds to gravity and imposed centrifugal forces

    NASA Technical Reports Server (NTRS)

    Bacon, E.; Morre, D. J.

    2001-01-01

    NADH oxidase activities measured with excised roots of dark-grown maize (Zea mays) seedlings and with isolated plasma membrane vesicles from roots of dark-grown maize oscillated with a regular period length of 24 min and were inhibited by the synthetic auxin 2,4-dichlorophenoxyacetic [correction of dichorophenoxyacetic] acid. The activities also responded to orientation with respect to gravity and to imposed centrifugal forces. Turning the roots upside down resulted in stimulation of the activity with a lag of about 10 min. Returning the sections to the normal upright position resulted in a return to initial rates. The activity was stimulated reversibly to a maximum of about 2-fold with isolated plasma membrane vesicles, when subjected to centrifugal forces of 25 to 250 x g for 1 to 4 min duration. These findings are the first report of a gravity-responsive enzymatic activity of plant roots inhibited by auxin and potentially related to the gravity-induced growth response. c2001 Editions scientifiques et medicales Elsevier SAS.

  15. On the performance of updating Stochastic Dynamic Programming policy using Ensemble Streamflow Prediction in a snow-covered region

    NASA Astrophysics Data System (ADS)

    Martin, A.; Pascal, C.; Leconte, R.

    2014-12-01

    Stochastic Dynamic Programming (SDP) is known to be an effective technique to find the optimal operating policy of hydropower systems. In order to improve the performance of SDP, this project evaluates the impact of re-updating the policy at every time step by using Ensemble Streamflow Prediction (ESP). We present a case study of the Kemano's hydropower system on the Nechako River in British Columbia, Canada. Managed by Rio Tinto Alcan (RTA), this system is subject to large streamflow volumes in spring due to important amount of snow depth during the winter season. Therefore, the operating policy should not only maximize production but also minimize the risk of flooding. The hydrological behavior of the system is simulated with CEQUEAU, a distributed and deterministic hydrological model developed by the Institut national de la recherche scientifique - Eau, Terre et Environnement (INRS-ETE) in Quebec, Canada. On each decision time step, CEQUEAU is used to generate ESP scenarios based on historical meteorological sequences and the current state of the hydrological model. These scenarios are used into the SDP to optimize the new release policy for the next time steps. This routine is then repeated over the entire simulation period. Results are compared with those obtained by using SDP on historical inflow scenarios.

  16. Performance of Wielandt-Streckeisen STS-1 seismometers in the tidal domain—preliminary results

    NASA Astrophysics Data System (ADS)

    Pillet, R.; Florsch, N.; Hinderer, J.; Rouland, D.

    1994-07-01

    The aim of this work is to show that STS-1 seismometers are able to provide a signal with a very long period vertical component which can be used for Earth tide studies provided a number of recording conditions are improved. We use data from the GEOSCOPE network for BNG (Bangui, Central African Republic), MBO (M'bour, Senegal), CRZF (Crozet, TAAF (Terres Australes et Antarctiques FranDçaises), Indian Ocean), ECH (Echery, France) and PAF (Port-aux-FranDçais, Kerguelen, TAAF, Indian Ocean) stations operated by the Ecole et Observatoire de Physique du Globe de Strasbourg (EOPGS) and Institut FranDçais de Recherche Scientifique pour le Développement en Coopération (ORSTOM). These data are analysed with a least-squares adjustment method to fit the Earth tidal waves, and the results for these stations are compared. Special attention is paid to the comparison of results from ECH with those from the superconducting gravimeter of Strasbourg (J-9). For several stations used in this study (CRZF, MBO and ECH) the results are promising, but they are disappointing for others (PAF and BNG). We did not find any clear reason for such a difference in quality. We propose some improvements that will enable researchers to achieve a better recording of this long-period signal and obtain higher-quality data allowing gravimetric studies from global seismological networks.

  17. Decadal climate predictions with an high resolution coupled model

    NASA Astrophysics Data System (ADS)

    Monerie, P. A.; Valcke, S.; Moine, M. P.; Maisonnave, E.; Coquart, L.; Cassou, C.; Terray, L.

    2014-12-01

    We analyze the decadal prediction skill of sea surface temperature variability with a high resolution coupled Ocean-Atmosphere General Circulation Model (OAGCM). The HR CERFACS was developed at the CERFACS (Centre Européen de Recherche et de Formation Avancée en Calcul Scientifique) laboratory in the framework of the EU-FP7 SPECS (Seasonal-to-decadal climate Predictions for the improvement of European Climate Services) project in order to address the question of decadal predictability with the use of a high spatial resolution. The atmospheric model is ARPEGE/IFS with a T359 spectral truncature and the oceanic model is NEMO at 0.25° resolution including the LIM2 sea ice model. Each hindcasts consist of a 10-members ensemble integrated over a 10-years period. These hindcasts are full-field initialized every year from 1993 to 2009 and initial oceanic state is given by the GLORYS2V1 (0.25° resolution) sea-surface temperatures. Members of a given ensemble (one initialization date) are generated by perturbations of the atmospheric initial conditions. We study the predictability of the global sea-surface temperature focusing on the Atlantic Multidecadal Oscillation (AMO), the Pacific Decadal Oscillation (PDO), the North Atlantic Subpolar Gyre (SPG) and the El-Nino Southern Oscillation (ENSO). We also investigate the prediction skill of the Atlantic Meridional Overturning Circulation (AMOC).

  18. A new Raman-N2 lidar dedicated to air quality survey

    NASA Astrophysics Data System (ADS)

    Royer, P.; Chazette, P.; Lardier, M.; Raut, J.-C.; Sauvage, L.

    2010-05-01

    The Commissariat à l'Energie Atomique (CEA) and the Centre National de la Recherche Scientifique (CNRS) have developed the Lidar Aérosols UltraViolet Aéroporté (LAUVA). The new version of this prototype is now commercialized with success under license by the LEOSPHERE Company with the name EZ LIDAR®. This eye-safe lidar is based on a Nd:YAG laser giving pulses of 16 mJ at 355 nm with a frequency of 20 Hz. The CEA and LEOSPHERE have recently upgraded this instrument into a three detection channels lidar measuring the two elastic cross-polarizations and the Raman-N2 backscatter signal at 387 nm. It is able to retrieve aerosol optical properties (extinction, backscatter coefficients and depolarization ratio) and atmospheric structures (boundary layer height and clouds) with a resolution of 1.5 m along the line-of-sight in analog mode and 15 m in photon-counting mode. This new lidar is particularly well-adapted to air quality survey thanks to a full overlap reached at ~150 m. This compact (90x50x20 cm) and light (less than50 kg) instrument has been integrated into the Mobile Aerosol Station (MAS) onboard a small truck and enables mobile measurements. We will here present and analyze some results obtained around Paris area with this Raman-N2 lidar.

  19. CASSIS, a software package to analyse high spectral resolution observations

    NASA Astrophysics Data System (ADS)

    Caux, E.; Bottinelli, S.; Vastel, C.; Glorian, J. M.

    2011-05-01

    CASSIS (Centre d'Analyse Scientifique de Spectres Infrarouges et Submillimetriques) is a software package aimed to speed-up the scientific analysis of high spectral resolution observations, particularly suited for broad-band spectral surveys. CASSIS is written in Java and can be ran on any platform. It has been extensively tested on Mac OSX, Linux and Windows operating systems. CASSIS is regularly enhanced, and can be easily installed and updated on any modern laptop. It uses a fast Sql-lite access to a local spectroscopic database made of the two molecular spectroscopic databases JPL and CDMS, as well as the atomic spectroscopic database NIST. The tools available in the currently distributed version (2.6) include a LTE model and the RADEX model connected to the LAMDA molecular collisional database. A module allows to build a line list fitting the various transitions of a given species and to directly produce rotational diagrams from these lists. CASSIS has been recently fully integrated into HIPE, the Herschel Interactive Processing Environment, as a plug-in (from version 5.1).

  20. Facility for assessing spectral normal emittance of solid materials at high temperature.

    PubMed

    Mercatelli, Luca; Meucci, Marco; Sani, Elisa

    2015-10-10

    Spectral emittance is a key topic in the study of new compositions, depositions, and mechanical machining of materials for solar absorption and for renewable energies in general. The present work reports on the realization and testing of a new experimental facility for the measurement of directional spectral emittance in the range of 2.5-20 μm. Our setup provides emittance spectral information in a completely controlled environment at medium-high temperatures up to 1200 K. We describe the layout and first tests on the device, comparing the results obtained for hafnium carbide and tantalum diboride ultrarefractory ceramic samples to previous quasi-monochromatic measurements carried out in the PROMES-CNRS (PROcedes, Materiaux et Energie Solaire- Centre National de la Recherche Scientifique, France) solar furnace, obtaining a good agreement. Finally, to assess the reliability of the widely used approach of estimating the spectral emittance from room-temperature reflectance spectrum, we compared the calculation in the 2.5-17 μm spectral range to the experimental high-temperature spectral emittance, obtaining that the spectral trend of calculated and measured curves is similar but the calculated emittance underestimates the measured value. PMID:26479806

  1. Inversion of stellar fundamental parameters from ESPaDOnS and Narval high-resolution spectra

    NASA Astrophysics Data System (ADS)

    Paletou, F.; Böhm, T.; Watson, V.; Trouilhet, J.-F.

    2015-01-01

    The general context of this study is the inversion of stellar fundamental parameters from high-resolution Echelle spectra. We aim at developing a fast and reliable tool for the post-processing of spectra produced by ESPaDOnS and Narval spectropolarimeters. Our inversion tool relies on principal component analysis. It allows reducing dimensionality and defining a specific metric for the search of nearest neighbours between an observed spectrum and a set of observed spectra taken from the Elodie stellar library. Effective temperature, surface gravity, total metallicity, and projected rotational velocity are derived. Various tests presented in this study that were based solely on information coming from a spectral band centred on the Mg i b-triplet and had spectra from FGK stars are very promising. Based on observations obtained at the Télescope Bernard Lyot (TBL, Pic du Midi, France), which is operated by the Observatoire Midi-Pyrénées, Université de Toulouse, Centre National de la Recherche Scientifique (France) and the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, CNRS/INSU and the University of Hawaii (USA).

  2. The dramatic change of the fossil magnetic field of HD 190073: evidence of the birth of the convective core in a Herbig star?

    NASA Astrophysics Data System (ADS)

    Alecian, E.; Neiner, C.; Mathis, S.; Catala, C.; Kochukhov, O.; Landstreet, J.

    2013-01-01

    In the context of the ESPaDOnS and Narval spectropolarimetric surveys of Herbig Ae/Be stars, we discovered and then monitored the magnetic field of HD 190073 over more than four years, from 2004 to 2009. Our observations all displayed similar Zeeman signatures in the Stokes V spectra, indicating that HD 190073 hosted an aligned dipole, stable over many years, consistent with a fossil origin. We obtained new observations of the star in 2011 and 2012 and detected clear variations of the Zeeman signature on timescales of days to weeks, indicating that the configuration of its field has changed between 2009 and 2011. Such a sudden change of external structure of a fossil field has never previously been observed in any intermediate or high-mass star. HD 190073 is an almost entirely radiative pre-main sequence star, probably hosting a growing convective core. We propose that this dramatic change is the result of the interaction between the fossil field and the ignition of a dynamo field generated in the newly-born convective core. Based on observations collected at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers (INSU) of the Centre National de la Recherche Scientifique (CNRS) of France and the University of Hawaii, at the Observatoire du Pic du Midi (France), operated by INSU, and at the European Southern Observatory, Chile (Program ID 187.D-0917).

  3. GEOTRACES: Studying the global marine biogeochemistry of trace elements and isotopes

    NASA Astrophysics Data System (ADS)

    Frank, Martin; Jeandel, Catherine; Anderson, Robert F.; Henderson, Gideon; Francois, Roger; Sharma, Mukul

    There is a growing international interest among geochemists and oceanographers in building a coordinated global study of the marine biogeochemical cycles of selected trace elements and isotopic tracers. This is reflected by the increasing numbers of contributions to corresponding special sessions at meetings such as the 2001 AGU Fall Meeting, the 2002 Goldschmidt Meeting, and the 2003 European Geophysical Union Annual Meeting. With support from the U.S. National Science Foundation's Chemical Oceanography program, the Centre National de Recherche Scientifique in France, the University Paul Sabatier, and the Observatoire Midi-Pyrénées, an international planning workshop was recently held to define the scientific goals for such a global study.Eighty-five scientists from 15 nations representing fields as diverse as physical oceanography, dynamic and biogeochemical ocean modeling, ocean geochemistry, and paleoceanography attended the workshop. There was a broad consensus recognizing the need for a coordinated research effort in the spirit of the 1970s Geochemical Ocean Sections Study (GEOSECS) program, which led to fundamental advances in the understanding of ocean circulation and biogeochemical cycles. Dramatic advances have been made in a nalytical techniques, chemical sensors, and modeling since the days of GEOSECS, but progress in understanding the global biogeochemical cycles of trace elements and their isotopes has been limited by the lack of a large-scale coordinated effort. Workshop participants enthusiastically endorsed the development of such a program, for which the name GEOTRACES was adopted.

  4. L'astronomie dans le monde

    NASA Astrophysics Data System (ADS)

    Manfroid, J.

    2007-09-01

    Anions interstellaires; S Orionis; Altaîr; Courants stellaires; Etoiles jeunes; 2MASSW J1207334-393254; Alpha Andromède; Etoiles à neutrons (1); LH54-425; AGNs invisibles; Deux supernovae; Les GRBs seon Swift; Peser les trous noirs; Formation de trous noirs; Trou noir; ondes gravitationnelles : Virgo entre dans sa phase d'exploitation scientifique; Amas de galaxies actifs; Amas de galaxies; Galaxies actives d'amas; L'univers statique: le retour; Macho; Exoplanètes; Exoplanètes habitables?; Exoplanètes habitables? (suite); Une année d'un an; Une année de 31 heures; Valse des Jupiters; Disque de HD 15115; Impact majeur; Planètes isolées; Super-Jupiter; Impact et mini-extinction; L'effet Pioneer; Toungouska; Spéléo martienne; Autres lunes dactives; Encelade; Hypérion; Pluton dépassé; Satellites d'Uranus; Titan

  5. Frontiers of QCD with Precision nPDFs

    NASA Astrophysics Data System (ADS)

    Kusina, Aleksander; Lyonnet, Florian; Olness, Fredrick I.; Schienbein, Ingo

    2016-03-01

    Searches for new physics will increasingly depend on identifying deviations from precision Standard Model (SM) predictions. Quantum Chromodynamics (QCD) will necessarily play a central role in this endeavor as it provides the framework for the parton model. However, as we move to higher orders and into extreme kinematic regions, we begin to see the full complexities of the QCD theory. Recent theoretical developments improve our ability to analyze both proton and nuclear PDFs across the full kinematic range. These developments are incorporated into the new nCTEQ15 PDFs, and we review these developments with respect to future measurements, and identify areas where additional effort is required. Based on work in collaboration with D. B. Clark, E. Godat, T. Ježo, C. Keppel, K. Kovařík, J.G. Morfín, P. Nadolsky, J.F. Owens, & J.Y. Yu. This work is supported in part by the U.S. Department of Energy under grant DE-FG02-04ER41299, and by Projet international de cooperation scientifique PICS05854 between France and the U.S.

  6. Follow-up of a report of a potential linkage for schizophrenia on chromosome 22q12-q13.1: Part 2

    SciTech Connect

    Pulver, A.E.; Lasseter, V.K.; Wolyniec, P.

    1994-03-15

    A collaboration involving four groups of investigators (Johns Hopkins University/Massachusetts Institute of Technology; Medical College of Virginia/The Health Research Board, Dublin; Institute of Psychiatry, London/University of Wales, Cardiff; Centre National de la Recherche Scientifique, Paris) was organized to confirm results suggestive of a schizophrenia susceptibility locus on chromosome 22 identified by the JHU/MIT group after a random search of the genome. Diagnostic, laboratory, and analytical reliability exercises were conducted among the groups to ensure uniformity of procedures. Data from genotyping of 3 dinucleotide repeat polymorphisms (at the loci D22S268, IL2RB, D22S307) for a combined replication sample of 256 families, each having 2 or more affected individuals with DNA, were analysed using a complex autosomal dominant model. This study provided no evidence for linkage or heterogeneity for the region 22q12-q13 under this model. We conclude that if this region confers susceptibility to schizophrenia, it must be in only a small proportion of families. Collaborative efforts to obtain large samples must continue to play an important role in the genetic search for clues to complex psychiatric disorders such as schizophrenia. 32 refs., 3 tabs.

  7. The space instrument SOVAP of the PICARD mission

    NASA Astrophysics Data System (ADS)

    Dewitte, S.; Conscience, C.; Mefta, M.; Chevalier, A.; Crommelynck, D.

    2010-12-01

    PICARD is a scientific mission of the French space agency CNES. Its objectives are the study of the origin of the solar variability and the study of the relations between the Sun and the Earth's climate. The payload was launched on 15 june 2010 in a Sun Synchronous Orbit at 725 km altitude. The mission life time is two years, however to be extended to three years. The payload consists of two absolute radiometers measuring the TSI (Total Solar Irradiance) and an imaging telescope to determine the solar diameter, the limb shape and asphericity. SOVAP (SOlar VAriability PICARD) is an experiment developed by the STCE (Solar Terrestrial Center of Excellence) with a contribution of the CNRS (Centre National de Recherche Scientifique) composed of an absolute radiometer provided by the RMIB (Royal Meteorological Institute of Belgium) to measure the TSI and a bolometer provided by the ROB (Royal Observatory of Belgium) to measure both the solar and terrestrial outgoing radiation with 10 s sampling . The Sovap instrument aims at high quality metrology in the space environment. In this paper, we describe the SOVAP instrument and its technical performances.

  8. The space instrument SOVAP of the PICARD mission

    NASA Astrophysics Data System (ADS)

    Conscience, C.; Meftah, M.; Chevalier, A.; Dewitte, S.; Crommelynck, D.,

    2011-09-01

    PICARD is a Satellite dedicated to the simultaneous measurement of the absolute total and spectral solar irradiance, the diameter and solar shape and the Sun's interior probed by helioseismology method. Its objectives are the study of the origin of the solar variability and the study of the relations between the Sun and the Earth's climate. PICARD was launched on June 15, 2010. The Satellite was placed into the heliosynchronous orbit of 735 km with inclination of 98.28 degrees. The payload consists in two absolute radiometers measuring the TSI (Total Solar Irradiance) and an imaging telescope to determine the solar diameter, the limb shape and asphericity. SOVAP (SOlar VAriability Picard) is an experiment developed by the Belgian STCE (Solar Terrestrial Center of Excellence) with a contribution of the CNRS (Centre National de la Recherche Scientifique) composed of an absolute radiometer provided by the RMIB (Royal Meteorological Institute of Belgium) to measure the TSI and a bolometer provided by the ROB (Royal Observatory of Belgium). The continuous observation of the solar irradiance at the highest possible precision and accuracy is an important objective of the Earth climate change. This requires: high quality metrology in the space environment. In this article, we describe the SOVAP instrument, its performances and uncertainties on the measurements of the TSI.

  9. Redistribution of annexin in gravistimulated pea plumules

    NASA Technical Reports Server (NTRS)

    Clark, G. B.; Rafati, D. S.; Bolton, R. J.; Dauwalder, M.; Roux, S. J.

    2000-01-01

    We used immunocytochemistry to investigate the effects of gravistimulation on annexin localization in etiolated pea plumule shoots. In longitudinal sections, an asymmetric annexin immunostaining pattern was observed in a defined group of cells located just basipetal to apical meristems at the main shoot apex and at all of the axillary buds, an area classically referred to as the leaf gap. The pattern was observed using both protein-A-purified anti-annexin and affinity-purified anti-annexin antibodies for the immunostaining. A subset of the cells with the annexin staining also showed an unusually high level of periodic acid Schiff (PAS) staining in their cell walls. Prior to gravistimulation, the highest concentration of annexin was oriented toward the direction of gravity along the apical end of these immunostained cells. In contrast, both at 15 and 30 min after gravistimulation, the annexin immunostain became more evenly distributed all around the cell and more distinctly cell peripheral. The asymmetry along the lower wall of these cells was no longer evident. In accord with current models of annexin action, we interpret the results to indicate that annexin-mediated secretion in the leaf gap area is preferentially toward the apical meristem prior to gravistimulation, and that gravistimulation results in a redirection of this secretion. These data are to our knowledge the first to show a correlation between the vector of gravity and the distribution of annexins in the cells of flowering plants. c 2000 Editions scientifiques et medicales Elsevier SAS.

  10. Feeling the Pull: a Study of Natural Galactic Accelerometers. I. Photometry of the Delicate Stellar Stream of the Palomar 5 Globular Cluster

    NASA Astrophysics Data System (ADS)

    Ibata, Rodrigo A.; Lewis, Geraint F.; Martin, Nicolas F.

    2016-03-01

    We present an analysis of wide-field photometric surveys of the Palomar 5 globular cluster and its stellar stream, based on g- and r-band measures together with narrow-band DDO 51 photometry. In this first study, we use the deep (g, r) data to measure the incidence of gaps and peaks along the stream. Examining the star-counts profile of the stream plus contaminating populations, we find no evidence for significant underdensities, and find only a single significant overdensity. This is at odds with earlier studies based on matched-filter maps derived from shallower SDSS data if the contaminating population possesses plausible spatial properties. The lack of substantial substructure along the stream may be used in future dynamical simulations to examine the incidence of dark matter sub-halos in the Galactic halo. We also present a measurement of the relative distances along the stream, which we use to create the deepest wide-field map of this system to date. Based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institute National des Sciences de l’Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  11. Selecting and Scheduling Observations at the IRAM Observatories

    NASA Astrophysics Data System (ADS)

    Grewing, Michael

    2006-12-01

    After a brief characterization of the IRAM Observatories on Pico Veleta in Spain, and the Plateau de Bure in France, the process by which observing proposals are selected is described. The observatories have initially been created in response to the scientific interests of a relatively small group if scientists affiliated with the Centre National de la Recherche Scientifique (CNRS) in France, the Max-Planck-Gesellschaft (MPG) in Germany, and the Instituto Geográafico Nacional (IGN) in Spain. The CNRS, the MPG, and the IGN have paid for the initial investment and operations costs, and contribute at present 47%, 47%, and 6% to IRAMs budget, respectively. However, since the beginning IRAM has received observing time requests not only from scientists in France, Germany and Spain, but from all around the world. While this proves the strong interest in observations at millimeter wavelengths, and the important role that the IRAM Observatories are playing, it also leads to a number of questions in connection with future developments.

  12. International Heliophysical Year: European Activities

    NASA Astrophysics Data System (ADS)

    Briand, C.

    2007-08-01

    The First European General Assembly of the "International Heliophysical Year" (IHY) took place at the headquarters of the Centre Nationial de la Recherche Scientifique (CNRS) in Paris, France, 10-13 January 2006. There were 113 participants representing 27 nations. The science concerned with the International Heliophysical Year programme was first illustrated. Then, the status of current instruments as well as practical information on the campaign management policy was given. Twenty European National Coordinators described the progress of their IHY activities. Representatives from Egypt, Angola and the coordinator of the Balkan, Black and Caspian Sea Region also reported on the progress of IHY activities in their respective regions. People from the IHY Secretariat provided a summary of the global IHY efforts including the United Nations Basic Space Sciences Program. In the education and public outreach front, a variety of activities have been planned: TV and radio shows, board games on space weather, specific programmes for schools and universities, workshops for teachers are some of the actions that were presented by the delegates. Beyond of these national and individual initiatives, specific activities requiring European coordination were discussed. This paper provides an extended summary of the main talks and discussions that held during the meeting.

  13. Micromechanical Study of Metals

    NASA Technical Reports Server (NTRS)

    Velikov, P. A.; Stchapov, N. P.; Lorenz, W. F.

    1945-01-01

    The Institut Scientifique Experimental des Transports at Moscow established toward the end of 1925 had since its inception included in its program the study of the mechanism of plastic deformation and the problems associated with it with reference to the materials of the means of transport. Before the program thus determined upon could be carried out, it was necessary to adopt a method of research, or, more exactly, a system of such methods. Because of the modest equipment of the laboratory of the recently established institute, the choice of any particular method was determined not only by the advantages it offered but also by the resources available. As a result of a series of studies and investigations, a method was determined upon which in this paper will be denoted as the micromechanical method. The underlying basis of this method is already known. As will be seen from the description that follows, the micromechanical method is merely a combination of the micrographic study of plastic deformations with mechanical tests on small specimens. It is a well-known fact that a number of investigators have largely employed and still are employing these two procedures and have thereby obtained good results. The authors of the present paper have found it useful to combine the two methods, by making the two studies simultaneously on the sane specimen.

  14. L'Education relative a l'environnement: La representation sociale d'educatrices et d'educateurs

    NASA Astrophysics Data System (ADS)

    Rooney, Elizabeth

    Cette recherche, qui prend appui sur la theorie des representations sociales, a tente de comprendre le phenomene de l'Education relative a l'environnement (ERE) au Quebec. Pour ce faire, j'ai choisi de m'interesser aux points de vue sur le sujet de neuf enseignantes et enseignants d'ecologie oeuvrant dans des ecoles (contexte formel) et de dix animatrices et animateurs oeuvrant dans des centres d'interpretation (contexte non formel). L'analyse narrative de leurs discours recueillis lors d'entrevues individuelles semi-structurees a permis de montrer que la mise en forme et la mise en pratique de l'ERE tendent a s'inscrire dans le prolongement d'une conception essentiellement ecologique de l'environnement et d'une conception plutot mecaniste et sensualiste de l'education, c'est-a-dire comme une simple affaire de transmission de connaissances scientifiques et d'eveil d'acuite sensorielle. Cette analyse a egalement permis de montrer que les educatrices et les educateurs retravaillent ces conceptions pour composer avec les moments et les lieux singuliers de leurs pratiques. Ce faisant, ils innovent et soulevent des questions a propos de la teneur des conceptions ou definitions standardisees de l'ERE. Cette recherche permet ainsi d'eclairer l'aspect a la fois traditionnel et potentiellement innovateur de la representation sociale de l'ERE d'educatrices et d'educateurs de terrain.

  15. "De Cassini à l'an 2000": The Paris Observatory Library

    NASA Astrophysics Data System (ADS)

    Vallet, M.; Reymonet, N.

    Paris Observatory founded in 1667 by Louis XIV is one of the so called "Grand Etablissement" under of the aegis of the Ministry of higher education and research, and includes two other centres: Meudon Observatory and the Radioastronomy centre in Nancay, created respectively in 1876 and 1955. The decree which gave birth to the library itself was signed in 1785 by Louis XVI. In 1926 Meudon is joined to Paris. The total number of bound volumes, including journals, is 100.000. This comprises 2000 periodical titles (of which 1200 are current titles), monographs, photographs, incunabula and manuscripts from the 16th to the 20th century, microfilm versions of historical material. The collections of two libraries are complementary. Starting in 1981, the library became part of a national "Centre d'Acquisition et de Diffusion de l'Information Scientifique et Technique" (CADIST) for astronomy and astrophysics documents. The catalogue is available on national networks such as the Pancatalogue or CCN. It may also be accessed on the international OCLC network. Finally the library may be accessed on internet via WWW.

  16. Lessons learnt from the 15 years experience of the French case in the field of HLLL waste

    SciTech Connect

    Ouzounian, G.

    2007-07-01

    Year 2006 has been marked in France by the vote in the Parliament of the Planning Act of 28 June, 2006, concerning the sustainable management of radioactive materials and waste. This vote was the achievement of a 15 years research programme performed as required by the previous Research Law of 1991, also known as the Bataille Law, from the name of Christian Bataille, MP, who drafted it and monitored its enforcement as a member of the Parliamentary Office for Scientific and Technological Assessment (Office Parlementaire d'Evaluation des Choix Scientifiques et Techniques - OPECST). At that time a stepwise approach to siting was introduced in the process. It included the study of several alternatives to the geological disposal of long lived high level radioactive waste. Those alternatives have been thoroughly studied and assessed before the Government decided to submit the bill to the Parliament. Experience has been gained not only on the scientific and technical aspects, but also in the field of decision making process, also called now governance. However, not only the results of the research programme were decisive in preparing the bill, but also of major importance were the industrial experience of ANDRA and the rigorous programme management along all those years. Main lessons learnt from the experience are given in this paper. (authors)

  17. Vigie Ciel a collaborative project to study fireballs and organise meteorite recoveries

    NASA Astrophysics Data System (ADS)

    Colas, F.; Zanda, B.; Bouley, S.; Lewin, E.; Vaubaillon, J.; Marmo, C.; Rotaru, M.; Labenne, L.; Julien, J. F.; Linares, M.; Steinhausser, A.; Rault, J. L.; Vernazza, P.

    2015-10-01

    Research on fireballs and meteorites has always been of interest to the public, due to the beauty of shooting stars in the night sky and to the extraterrestrial origin of meteorites. A fireball observation network called FRIPON [1] (Colas et al, 2015) is currently being setup, funded by ANR (Agence Nationale pour la Recherche). It will cover France with 100 cameras and is expected to be operational for the end of 2015. FRIPON will detect fireballs and hence allow us to define meteorite strewn fields within 24h, so that meteorite searches can be launched very early on. Because of the need to search all over France, including in private land, it is important that the general public be aware of our project and be willing to help or participate. Indeed, as the main goal of FRIPON is to recover fresh meteorites (within a few days), our aim is to be able to organize a search with at least 50 persons to scan an area of a few km2 within a week. Help from the public would hence be most helpful but it is also important to have an operational and trained research team. This project thus appears as a unique occasion to involve the public in a scientific project while promoting informal scientific education. This prompted us to set up Vigie-Ciel, a citizen science network centered on meteorite recovery. FRIPON is an open network based on open-source software, it will accept citizenrun cameras. In addition to fireballs, it will allow scientists and Vigie-Ciel participants to study anything that can be observed by all-sky cameras: bird migrations, bats, clouds, lightning, etc. The data will be freely available to all.

  18. Atmospheric Measurements by Cavity Enhanced Absorption Spectroscopy

    NASA Astrophysics Data System (ADS)

    Yi, Hongming; Wu, Tao; Coeur-Tourneur, Cécile; Fertein, Eric; Gao, Xiaoming; Zhao, Weixiong; Zhang, Weijun; Chen, Weidong

    2015-04-01

    Since the last decade, atmospheric environmental monitoring has benefited from the development of novel spectroscopic measurement techniques owing to the significant breakthroughs in photonic technology from the UV to the infrared spectral domain [1]. In this presentation, we will overview our recent development and applications of cavity enhanced absorption spectroscopy techniques for in situ optical monitoring of chemically reactive atmospheric species (such as HONO, NO3, NO2, N2O5) in intensive campaigns [2] and/or in smog chamber studies [3]. These field deployments demonstrated that modern photonic technologies (newly emergent light sources combined with high sensitivity spectroscopic techniques) can provide a useful tool to improve our understanding of tropospheric chemical processes which affect climate, air quality, and the spread of pollution. Experimental detail and preliminary results will be presented. Acknowledgements. The financial support from the French Agence Nationale de la Recherche (ANR) under the NexCILAS (ANR-11-NS09-0002) and the CaPPA (ANR-10-LABX-005) contracts is acknowledged. References [1] X. Cui, C. Lengignon, T. Wu, W. Zhao, G. Wysocki, E. Fertein, C. Coeur, A. Cassez,L. Croisé, W. Chen, et al., "Photonic Sensing of the Atmosphere by absorption spectroscopy", J. Quant. Spectrosc. Rad. Transfer 113 (2012) 1300-1316 [2] T. Wu, Q. Zha, W. Chen, Z. XU, T. Wang, X. He, "Development and deployment of a cavity enhanced UV-LED spectrometer for measurements of atmospheric HONO and NO2 in Hong Kong", Atmos. Environ. 95 (2014) 544-551 [3] T. Wu, C. Coeur-Tourneur, G. Dhont,A. Cassez, E. Fertein, X. He, W. Chen,"Application of IBBCEAS to kinetic study of NO3 radical formation from O3 + NO2 reaction in an atmospheric simulation chamber", J. Quant. Spectrosc. Rad. Transfer 133 (2014)199-205

  19. The neutron channeling phenomenon.

    PubMed

    Khanouchi, A; Sabir, A; Boulkheir, M; Ichaoui, R; Ghassoun, J; Jehouani, A

    1997-01-01

    Shields, used for protection against radiation, are often pierced with vacuum channels for passing cables and other instruments for measurements. The neutron transmission through these shields is an unavoidable phenomenon. In this work we study and discuss the effect of channels on neutron transmission through shields. We consider an infinite homogeneous slab, with a fixed thickness (20 lambda, with lambda the mean free path of the neutron in the slab), which contains a vacuum channel. This slab is irradiated with an infinite source of neutrons on the left side and on the other side (right side) many detectors with windows equal to 2 lambda are placed in order to evaluate the neutron transmission probabilities (Khanouchi, A., Aboubekr, A., Ghassoun, J. and Jehouani, A. (1994) Rencontre Nationale des Jeunes Chercheurs en Physique. Casa Blanca Maroc; Khanouchi, A., Sabir, A., Ghassoun, J. and Jehouani, A. (1995) Premier Congré International des Intéractions Rayonnements Matière. Eljadida Maroc). The neutron history within the slab is simulated by the Monte Carlo method (Booth, T. E. and Hendricks, J. S. (1994) Nuclear Technology 5) and using the exponential biasing technique in order to improve the Monte Carlo calculation (Levitt, L. B. (1968) Nuclear Science and Engineering 31, 500-504; Jehouani, A., Ghassoun, J. and Aboubker, A. (1994) In Proceedings of the 6th International Symposium on Radiation Physics, Rabat, Morocco). Then different geometries of the vacuum channel have been studied. For each geometry we have determined the detector response and calculated the neutron transmission probability for different detector positions. This neutron transmission probability presents a peak for the detectors placed in front of the vacuum channel. This study allowed us to clearly identify the neutron channeling phenomenon. One application of our study is to detect vacuum defects in materials. PMID:9463884

  20. Lipid intake in children under 3 years of age in France. A position paper by the Committee on Nutrition of the French Society of Paediatrics.

    PubMed

    Briend, A; Legrand, P; Bocquet, A; Girardet, J-P; Bresson, J-L; Chouraqui, J-P; Darmaun, D; Dupont, C; Frelut, M L; Goulet, O; Hankard, R; Rieu, D; Simeoni, U; Turck, D; Vidailhet, M

    2014-04-01

    Lipids are an important source of energy for young children and play a major role in the development and functioning of nervous tissue. Essential fatty acids and their long-chain derivatives also fulfill multiple metabolic functions and play a role in the regulation of numerous genes. The Food and Agriculture Organization of the United Nations (FAO), the World Health Organization (WHO), and the French Agency for Food, Environmental and Occupational Health & Safety (Agence nationale de sécurité sanitaire de l'alimentation, de l'environnement et du travail [ANSES]) have recently recommended a minimum daily intake in preformed long-chain polyunsaturated fatty acids (LC-PUFAs): arachidonic acid (ARA), eicosapentaenoic acid (EPA), and docosahexaenoic acid (DHA). Mother's milk remains the only reference, but the large variability in its DHA content does not guarantee that breastfed children receive an optimal DHA intake if the mother's intake is insufficient. For children fed with infant formulas, ARA and DHA intake is often below the recommended intake because only one-third of infant formulas available on the market in France are enriched in LC-PUFAs. For all children, linoleic acid (LA) intake is on average higher than the minimal recommended values. The consequences of these differences between intake and recommended values are uncertain. A cautious attitude is to come close to the current recommendations and to advise sufficient consumption of DHA in breastfeeding women. For bottle-fed children, infant formulas enriched in LC-PUFAs and with moderate levels of LA should be preferred. LC-PUFA-rich fish should be consumed during breastfeeding, and adapted vegetable oils when complementary foods are introduced. PMID:24636590

  1. Rotational Spectroscopy of Isocyanic Molecules: Allyl Isocyanide and Diisocyanomethane

    NASA Astrophysics Data System (ADS)

    Motiyenko, R. A.; Margules, L.; Haykal, I.; Huet, T. R.; Cocinero, E. J.; Ecija, P.; Fernandez, J. A.; Castano, F.; Lesarri, A.; Guillemin, J.-C.

    2012-06-01

    Isocyanides are less stable isomers of nitriles and some of them have already been observed in the interstellar medium (HNC, CH_3NC, HCCNC). But still there exists a lack of experimental spectroscopic data on simple isocyanic molecules that can represent potential astrophysical interest. In this view we have performed high resolution studies of rotational spectra of allyl isocyanide (CH_2=CH--CH_2--NC) and diisocyanomethane (CN--CH_2--NC). The rotational spectra of allyl isocyanide have been measured in the frequency range 6 -- 18 GHz by means of FTMW spectrometer in Bilbao and in the frequency range 150 -- 945 GHz by means of classic absorption spectroscopy in Lille. Two stable confomers of allyl isocyanide have been observed in both series of measurements. In addition, all 13C-monosubstituted isotopologues and 15N isotopologues were detected in natural abundance. Due to much lower kinetic stability the rotational spectrum of diisocyanomethane has been measured only in absorption using the Lille spectrometer. The spectral assignments have been supported by high-level quantum chemical calculations. For both molecules accurate sets of rotational and centrifugal distortion constants (up to the octics) have been produced. As a result, reliable predictions of transitions frequencies suitable for astrophysical detection have been obtained for both molecules. Finally, the effective and substitution structures were determined for the two conformers of allyl isocyanide, comparing the result with ab initio data. This work is supported by Centre Nationale d'Etudes Spatiales (CNES), Action sur Projet Physico-Chimie du Milieu Interstellaire (PCMI-CNRS) and by the contract ANR-08-BLAN-0054. Spanish part acknowledges funding from the MICINN and the MINECO.

  2. Malignant Peripheral Nerve Sheath Tumor Is a Challenging Diagnosis: A Systematic Pathology Review, Immunohistochemistry, and Molecular Analysis in 160 Patients From the French Sarcoma Group Database.

    PubMed

    Le Guellec, Sophie; Decouvelaere, Anne-Valérie; Filleron, Thomas; Valo, Isabelle; Charon-Barra, Céline; Robin, Yves-Marie; Terrier, Philippe; Chevreau, Christine; Coindre, Jean-Michel

    2016-07-01

    An accurate histopathologic diagnosis is essential for an adequate treatment of soft tissue sarcomas. The diagnosis of malignant peripheral nerve sheath tumor (MPNST) can be complex, particularly outside the neurofibromatosis type 1 (NF1) context. MPNST is a rare malignancy, and due to the lack of specific histologic criteria, several differential diagnoses must be considered. A total of 350 patients diagnosed with MPNST (from 1990 to 2013) were retrieved from the French sarcoma network (RRePS) and the Conticabase (Connective Tissue Cancer Network database). Tumor samples were available for 160 cases (45.2%). Pathology review, immunohistochemistry (IHC), and molecular analysis (when dealing with a monomorphic sarcoma) were systematically performed. Patient, tumor, and treatment characteristics were evaluated to identify prognostic factors for the definitive primary MPNST (n=106) cohort. Twenty-nine tumors (18.1%) initially diagnosed as MPNST were reclassified on the basis of histologic review, IHC, and molecular analysis. Patients with NF1 disease comprised 64% of the remaining cohort. The 5-year overall survival for patients from the entire cohort was 47%, 34.8% for NF1 patients, and 68.5% for patients without NF1 disease, making NF1 syndrome an independent poor prognostic factor of survival. Positive margins and lack of radiation therapy were independent predictors of local recurrence. The Fédération Nationale des Centres de Lutte Contre le Cancer tumor grade was an independent prognostic indicator of metastasis. Given the therapeutic implications of a misdiagnosis, the systematic pathology review, IHC, and molecular analysis (when dealing with monomorphic sarcoma) strategy allowed reclassification of 20% of cases, mainly the sporadic MPNSTs. PMID:27158754

  3. Deep Dermatophytosis and Inherited CARD9 Deficiency

    PubMed Central

    Vincent, Quentin B.; Liu, Luyan; Cypowyj, Sophie; Prando, Carolina; Migaud, Mélanie; Taibi, Lynda; Ammar-Khodja, Aomar; Stambouli, Omar Boudghene; Guellil, Boumediene; Jacobs, Frederique; Goffard, Jean-Christophe; Schepers, Kinda; del Marmol, Véronique; Boussofara, Lobna; Denguezli, Mohamed; Larif, Molka; Bachelez, Hervé; Michel, Laurence; Lefranc, Gérard; Hay, Rod; Jouvion, Gregory; Chretien, Fabrice; Fraitag, Sylvie; Bougnoux, Marie-Elisabeth; Boudia, Merad

    2014-01-01

    BACKGROUND Deep dermatophytosis is a severe and sometimes life-threatening fungal infection caused by dermatophytes. It is characterized by extensive dermal and subcutaneous tissue invasion and by frequent dissemination to the lymph nodes and, occasionally, the central nervous system. The condition is different from common superficial dermatophyte infection and has been reported in patients with no known immunodeficiency. Patients are mostly from North African, consanguineous, multiplex families, which strongly suggests a mendelian genetic cause. METHODS We studied the clinical features of deep dermatophytosis in 17 patients with no known immunodeficiency from eight unrelated Tunisian, Algerian, and Moroccan families. Because CARD9 (caspase recruitment domain–containing protein 9) deficiency has been reported in an Iranian family with invasive fungal infections, we also sequenced CARD9 in the patients. RESULTS Four patients died, at 28, 29, 37, and 39 years of age, with clinically active deep dermatophytosis. No other severe infections, fungal or otherwise, were reported in the surviving patients, who ranged in age from 37 to 75 years. The 15 Algerian and Tunisian patients, from seven unrelated families, had a homozygous Q289X CARD9 allele, due to a founder effect. The 2 Moroccan siblings were homozygous for the R101C CARD9 allele. Both alleles are rare deleterious variants. The familial segregation of these alleles was consistent with autosomal recessive inheritance and complete clinical penetrance. CONCLUSIONS All the patients with deep dermatophytosis had autosomal recessive CARD9 deficiency. Deep dermatophytosis appears to be an important clinical manifestation of CARD9 deficiency. (Funded by Agence Nationale pour la Recherche and others.) PMID:24131138

  4. La Ferrassie 8 Neandertal child reloaded: New remains and re-assessment of the original collection.

    PubMed

    Gómez-Olivencia, Asier; Crevecoeur, Isabelle; Balzeau, Antoine

    2015-05-01

    The first evidence of the partial infant Neandertal skeleton La Ferrassie 8 (LF8) was discovered in 1970, although most of the remains were found in 1973 as part of the 1968-1973 work at the site by H. Delporte. This individual and the other Neandertal children from La Ferrassie were published in the early 1980s by J.-L. Heim, and since then LF8 has been regarded as coming from a poorly documented excavation. The recent rediscovery of the box that contained the hominin bones given by Delporte to Heim in the Muséum national d'Histoire naturelle (MNHN) collection provided new fossils and helped to locate LF8 in the site: level M2 in square 1. Two visits to the Musée d'Archéologie nationale et Domaine national de Saint-Germain-en-Laye (MAN) yielded additional fossil remains from both the 1970 and 1973 excavations and resulted in the discovery of all of the notes from the excavation of H. Delporte between 1968 and 1973. Here the new fossil remains (47 after performing all possible refits), representing significant portions of the cranium, mandible, and vertebral column together with fragmentary hand and costal remains, are described. Unsurprisingly, the morphology of the bony labyrinth and of a complete stapes from the nearly complete left temporal show clear Neandertal affinities. Additionally, a complete reassessment of the original LF8 collection has resulted in the identification of several errors in the anatomical determination. Despite the significant increase in the anatomical representation of LF8, the skeletal remains are still limited to the head, thorax, pelvis, and four hand phalanges, with some very fragile elements relatively well preserved. Different hypotheses are proposed to explain this anatomical representation, which can be tested during future fieldwork. PMID:25805043

  5. Algeria: country profile.

    PubMed

    Harding, J

    1987-12-01

    Data are presented on the economy, the people, the population's health, and the culture in this country profile of Algeria. The population numbers 21.7 million. The infant mortality rate, used as a health indicator, is 81/1000 live births. Algeria's gross national product per capita is $2410 (US$15,390). Its main imports are machinery, transport equipment, food, tobacco, and consumer goods. The primary exports include oil, petroleum products, liquified natural gas, wine, and tobacco. Algeria's traditional Berber culture has survived occupation by Phoenicians, Romans, Arabs, and Europeans. The country is made up of an assortment of different social groups and ethnicities, and modern Algeria realized its unitary identity from the anti-colonial struggle. Recent laws allow freedom of association, an indication of growing pluralism in a state where opposition traditionally has been proscribed. 1987 marks the 25th anniversary of Algeria's independence, obtained after a long and bitter war with France. The victory of the Front de Liberation Nationale (FLN) was a signal for French settlers to leave in droves, and much of the country's managerial and technical expertise left with them. Yet, the FLN inherited a sound infrastructure on which to build a modern post-colonial society. Additionally, the country also was to benefit from plentiful hydrocarbon reserves, which guaranteed good foreign exchange earnings. One of the country's goals is to feed itself by investing in a long-neglected agricultural sector, yet presently oil and gas revenues continue to be the driving force behind development. The plans for increasing food production include greater scope for private farmers. A widening gap exists between those who espouse the old values forged by the liberation struggle and a younger generation, for whom the FLN's founding precepts and the leadership's old authoritarian style mean considerably less. PMID:12315296

  6. Can shale safely host US nuclear waste?

    USGS Publications Warehouse

    Neuzil, C.E.

    2013-01-01

    "Even as cleanup efforts after Japan’s Fukushima disaster offer a stark reminder of the spent nuclear fuel (SNF) stored at nuclear plants worldwide, the decision in 2009 to scrap Yucca Mountain as a permanent disposal site has dimmed hope for a repository for SNF and other high-level nuclear waste (HLW) in the United States anytime soon. About 70,000 metric tons of SNF are now in pool or dry cask storage at 75 sites across the United States [Government Accountability Office, 2012], and uncertainty about its fate is hobbling future development of nuclear power, increasing costs for utilities, and creating a liability for American taxpayers [Blue Ribbon Commission on America’s Nuclear Future, 2012].However, abandoning Yucca Mountain could also result in broadening geologic options for hosting America’s nuclear waste. Shales and other argillaceous formations (mudrocks, clays, and similar clay-rich media) have been absent from the U.S. repository program. In contrast, France, Switzerland, and Belgium are now planning repositories in argillaceous formations after extensive research in underground laboratories on the safety and feasibility of such an approach [Blue Ribbon Commission on America’s Nuclear Future, 2012; Nationale Genossenschaft für die Lagerung radioaktiver Abfälle (NAGRA), 2010; Organisme national des déchets radioactifs et des matières fissiles enrichies, 2011]. Other nations, notably Japan, Canada, and the United Kingdom, are studying argillaceous formations or may consider them in their siting programs [Japan Atomic Energy Agency, 2012; Nuclear Waste Management Organization (NWMO), (2011a); Powell et al., 2010]."

  7. Hailstorm forecast from stability indexes in Southwestern France

    NASA Astrophysics Data System (ADS)

    Melcón, Pablo; Merino, Andrés; Sánchez, José Luis; Dessens, Jean; Gascón, Estíbaliz; Berthet, Claude; López, Laura; García-Ortega, Eduardo

    2016-04-01

    Forecasting hailstorms is a difficult task because of their small spatial and temporal scales. Over recent decades, stability indexes have been commonly used in operational forecasting to provide a simplified representation of different thermodynamic characteristics of the atmosphere, regarding the onset of convective events. However, they are estimated from vertical profiles obtained by radiosondes, which are usually available only twice a day and have limited spatial representativeness. Numerical models predictions can be used to overcome these drawbacks, providing vertical profiles with higher spatiotemporal resolution. The main objective of this study is to create a tool for hail prediction in the southwest of France, one of the European regions where hailstorms have a higher incidence. The Association Nationale d'Etude et de Lutte contre les Fleáux Atmosphériques (ANELFA) maintains there a dense hailpad network in continuous operation, which has created an extensive database of hail events, used in this study as ground truth. The new technique is aimed to classify the spatial distribution of different stability indexes on hail days. These indexes were calculated from vertical profiles at 1200 UTC provided by WRF numerical model, validated with radiosonde data from Bordeaux. Binary logistic regression is used to select those indexes that best represent thermodynamic conditions related to occurrence of hail in the zone. Then, they are combined in a single algorithm that surpassed the predictive power they have when used independently. Regression equation results in hail days are used in cluster analysis to identify different spatial patterns given by the probability algorithm. This new tool can be used in operational forecasting, in combination with synoptic and mesoscale techniques, to properly define hail probability and distribution. Acknowledgements The authors would like to thank the CEPA González Díez Foundation and the University of Leon for its

  8. Cadmium exposure from food: the German LExUKon project.

    PubMed

    Schwarz, Markus A; Lindtner, Oliver; Blume, Katrin; Heinemeyer, Gerhard; Schneider, Klaus

    2014-01-01

    Cadmium is a very toxic contaminant with food being the major source of exposure for the general public. The second German food consumption survey (Nationale Verzehrsstudie II - NVS II) with about 20 000 participants (15 371 for dietary history interviews used for this study) allowed for an updated exposure assessment for the German population. Based on these comprehensive data, information on the consumption of 545 individual food items by the German population was generated. Cadmium concentrations in food were compiled from the German food monitoring programme, European countries' authority programmes and the published literature, covering the years from 1993 to 2008, and were multiplied with consumption data to obtain estimates of cadmium intake from food. Consumption-weighted mean cadmium concentrations per main food group were highest for cereals, followed by oily seeds & fruits, and vegetables. Due to both high consumption and considerable occurrence of cadmium, cereals and vegetables contributed most to the intake of the general public, followed by the main groups beverages, fruits & nuts, and dairy products (including milk). Cadmium intake from food was estimated to be 1.46 and 2.35 µg kg(-1) bw week(-1) for average and high-end consumers, respectively. This corresponds to 58% for average and 95% for high-end consumers, respectively, of a reference value derived from a recent health risk evaluation performed by EFSA, using the benchmark approach. Uncertainties in these estimates pertain to the influence of values below the limit of quantification and some foods not considered due to lacking occurrence data. In conclusion, the estimated cadmium intake of the German population from food is still close to health-based reference values. Further efforts to reduce cadmium intake are required. PMID:24645975

  9. Douleurs et conflits : Approche comparative et implications pour la qualité des soins en fin de vie

    PubMed Central

    Mpinga, Emmanuel Kabengele; Verloo, Henk; Rapin, Charles-Henri; Chastonay, Philippe

    2009-01-01

    Le conflit serait-il à l’organisation ce que la douleur est à un organisme ? OBJECTIFS: Explorer les similitudes et les differences entre les douleurs et les conflits dans les contextes de soins de fin de vie. Mieux comprendre le rôle des conflits dans la qualité de ces soins. MÉTHODOLOGIE: Méthode comparative et réflexive autour des politiques de prise en charge des douleurs et des conflits dans les systèmes de soins. RÉSULTATS: Les conflits et les douleurs présentent de nombreuses similitudes de par leur identité, leur typologie, leur prévalence, leur fonction d’alerte, leurs coûts économiques et sociaux, le déni ou l’occultation qui les entourent et les obstacles à leur prise en charge adéquate. À l’inverse, des différences apparaissent dans la prise en charge des douleurs comparée à celle des conflits. Ces différences portent sur l’existence des programmes de prévention et de lutte sur les scènes nationale et internationale, la mise en œuvre des activités de recherche et de formation et la visibilité sociale. Pour les conflits, cette mise en œuvre n’existe pas encore. CONCLUSION: Les décideurs en clinique et en santé publique devraient intégrer les conflits comme un indicateur de la qualité des soins et élaborer des politiques pertinentes en matière de santé. PMID:19714268

  10. Extraction and anonymity protocol of medical file.

    PubMed Central

    Bouzelat, H.; Quantin, C.; Dusserre, L.

    1996-01-01

    To carry out the epidemiological study of patients suffering from a given cancer, the Department of Medical Informatics (DIM) has to link information coming from different hospitals and medical laboratories in the Burgundy region. Demands from the French department for computerized information security (Commission Nationale de l'Informatique et des Libertés: CNIL), in regard to abiding by the law of January 6, 1978, completed by the law of July 1st, 1994 on nominal data processing in the framework of medical research have to be taken into account. Notably, the CNIL advised to render anonymous patient identities before the extraction of each establishment file. This paper describes a recently implemented protocol, registered with the French department for computerized information security (Service Central de la Sécurité des Systèmes d'information : SCSSI) whose purpose is to render anonymous medical files in view of their extraction. Once rendered anonymous, these files will be exportable so as to be merged with other files and used in a framework of epidemiological studies. Therefore, this protocol uses the Standard Hash Algorithm (SHA) which allows the replacement of identities by their imprints while ensuring a minimal collision rate in order to allow a correct linkage of the different information concerning the same patient. A first evaluation of the extraction and anonymity software with regard to the purpose of an epidemiological survey is described here. In this paper, we also show how it would be possible to implement this system by means of the Internet communication network. PMID:8947681

  11. Development and validation of a quantitative competitive ELISA for potency testing of equine anti rabies sera with other potential use.

    PubMed

    Korimbocus, Jehanara; Dehay, Nicolas; Tordo, Noël; Cano, François; Morgeaux, Sylvie

    2016-06-14

    In case of a bite by a rabies infected animal, the World Health Organisation recommends a prophylactic treatment including the administration of Human Rabies Immunoglobulins (HRIGs) or highly purified F(ab')2 fragments produced from Equine Rabies Immunoglobulin (F(ab')2 - ERIGs). According to international regulation, quality control of F(ab')2 - ERIGs lots requires potency testing by the in vivo Mouse Neutralisation Test (MNT) prior marketing. However, the strategy of the 3Rs (Reduce, Refine, Replace) for animal testing required by the European Directive encourages the replacement of the in vivo potency test by an in vitro assay. In this context, a competitive ELISA method (c-ELISA) has been developed by the Agence Nationale de Sécurité du Médicament et des Produits de Santé where F(ab')2 - ERIGs are in competition with a monoclonal antibody recognizing the trimeric native form of the rabies glycoprotein. After a full validation study, the c-ELISA has been applied to commercial batches of F(ab')2 - ERIGs. A correlation study with the MNT demonstrated a similarity between the two methods (r=0.751). Moreover, the c-ELISA method which does not need any species specific reagent has been applied to HRIGs potency testing as an alternative method to Rapid Fluorescent Focus Inhibition Test (RFFIT), thus avoiding the handling of live rabies virus in BSL3 containment. In conclusion, the c-ELISA has shown its potential to replace MNT and possibly RFFIT for the quantification of rabies immunoglobulin. After optimisation it may be used for the quantification of rabies immunoglobulin in any animal species, notably for rabies immunogenicity assay in mice. PMID:27151880

  12. The FORCLIM Eco-Physiological Growth Model for Planktic Foraminifera: a new Tool to Reconstruct Ecological Niches, Abundance and Potential Depth and Season of Growth for Fossil Foraminifera Species in Ocean Sediment Records

    NASA Astrophysics Data System (ADS)

    Lombard, F.; Labeyrie, L.; Michel, E.; Lea, D.; Spero, H. J.; Forclim, M. O.

    2007-12-01

    Paleocean hydrological reconstructions derived from planktic foraminifera isotopic ratios (δ18O and δ13C) or trace element ratio (Mg/Ca) are poorly constrained, for lack of precise knowledge on seasonality and water depth of test formation. This is particularly limiting for reconstruction of the thermocline characteristics. Various calibrations have been published, based on statistical correlation with core tops fossil fauna, sediment traps or plankton net collection. We present here what we think is the first eco-physiological model reproducing the growth of different foraminifera species in function of environmental parameter. By reproducing the main physiological rates of foraminifera (nutrition, respiration, symbiotic photosynthesis), this model estimates their growth in function of temperature, light availability and food concentration. The model is now calibrated for the species Neogloboquadrina pachyderma (dextral and sinistral forms), Neogloboquadrina dutertrei, Globigerina bulloides, Globigerinoides ruber, Globigerinoides sacculifer, Globigerinella siphonifera and Orbulina universa. Most of the model parameters are derived from newly performed experimental observations or from published data and only the influence of food concentration (in a Chl a basis) was calibrated with field observations. Using satellite data, the model predict the seasonal distribution of dominant foraminifer species over 576 field observations worldwide with efficiency higher than 60%. Moreover, the growth rate estimated for each foraminifera species can be used as an abundance indicator which allows prediction of the season and water depth at which most of the population has developed. This offers larges perspectives for both actual understanding of foraminifera role in the carbon/carbonate ocean cycle and for better quantification of paleoceanographic proxies. Forclim is a program supported by the Agence Nationale pour la Recherche and Institut National des Sciences de l

  13. Protéger les nourrissons contre la coqueluche

    PubMed Central

    Gilley, Meghan; Goldman, Ran D.

    2014-01-01

    Résumé Question Compte tenu du taux à la hausse de la coqueluche chez les enfants, plusieurs familles m’ont demandé quels moyens prendre pour protéger leurs tout-petits de cette infection. Quelles devraient être mes recommandations à ces familles? Réponse La coqueluche est une maladie évitable qui est endémique dans le monde entier. Chez les adultes, la coqueluche cause une maladie bénigne semblable à un rhume, suivie d’une toux persistante. Chez les nourrissons, elle peut causer de l’apnée, des convulsions, une encéphalopathie, une bronchopneumonie et la mort. Les décès dus à la coqueluche se produisent dans 86 % des cas chez des nourrissons de moins de 4 mois. La stratégie du cocooning, c’est-à-dire la vaccination des adultes en étroit contact avec des nourrissons, est recommandée par de nombreuses agences mondiales et nationales, mais elle ne prévient probablement que 20 % des cas de coqueluche chez les nourrissons. La vaccination durant la grossesse est plus efficace, mais elle n’est pas encore approuvée au Canada. Il n’a pas été démontré que la vaccination à la naissance soit uniformément efficace et elle n’est donc pas recommandée à l’heure actuelle.

  14. New sensitive one-step real-time duplex PCR method for group A and B HIV-2 RNA load.

    PubMed

    Avettand-Fenoel, Véronique; Damond, Florence; Gueudin, Marie; Matheron, Sophie; Mélard, Adeline; Collin, Gilles; Descamps, Diane; Chaix, Marie-Laure; Rouzioux, Christine; Plantier, Jean-Christophe

    2014-08-01

    The Agence Nationale de Recherche sur le Sida et les hépatites virales (ANRS) previously developed a widely used method for HIV-1 RNA quantification (Biocentric). Here, we report the development of a new specific and sensitive method for HIV-2 RNA quantification, based on an adaptation of the existing HIV-1 protocol. The new test is based on TaqMan one-step reverse transcription-quantitative PCR (qRT-PCR) targeting two conserved consensus regions of HIV-2 (long terminal repeat [LTR] and gag). Analytic performances were determined in three laboratories. Clinical performances were evaluated on 100 plasma samples from HIV-2-infected patients (groups A, B, and H) by comparison with the assay currently used for the ANRS HIV-2 cohort. The specificity was 100%. Sensitivity was 50 copies/ml (cp/ml) and was optimized to 10 cp/ml. The within-run coefficients of variation in the three laboratories varied from 0.54% to 1.61% at 4 log10 copies/ml and from 7.24% to 14.32% at 2 log10 cp/ml. The between-run coefficients of variation varied from 2.28% to 6.43%. Of the 39 clinical samples below 2 log10 in the current assay, the new test improved the detection or quantification of 17 samples, including eight group B samples. For quantifiable samples, similar loads were obtained with the two assays for group A samples. The median difference between the two assays for group B samples was +0.18 but with greater heterogeneity than for group A. The HIV-2 group H sample had similar results with the two assays. This new assay is highly sensitive and accurately quantifies the most prevalent HIV-2 groups. This test will be useful for monitoring low viral loads in HIV-2-infected patients. PMID:24920771

  15. Protoplanetary disk formation and evolution models: DM Tau and GM Aur

    NASA Astrophysics Data System (ADS)

    Hueso, R.; Guillot, T.

    2002-09-01

    We study the formation and evolution of protoplanetary disks using an axisymmetric turbulent disk model. We compare model results with observational parameters derived for the DM Tau and GM Aur systems. These are relatively old T Tauri stars with large and massive protoplanetary disks. Early disk formation is studied in the standard scenario of slowly rotating isothermal collapsing spheres and is strongly dependent on the initial angular momentum and the collapse accretion rate. The viscous evolution of the disk is integrated in time using the classical Alpha prescription of turbulence. We follow the temporal evolution of the disks until their characteristics fit the observed characteristics of DM Tau and GM Aur. We therefore obtain the set of model parameters that are able to explain the present state of these disks. We also study the disk evolution under the Beta parameterization of turbulence, recently proposed for sheared flows on protoplanetary disks. Both parameterizations allow explaining the present state of both DM Tau and GM Aur. We infer a value of Alpha between 5x10-3 to 0.02 for DM Tau and one order of magnitude smaller for GM Aur. Values of the Beta parameter are in accordance with theoretical predictions of Beta around 2x10-5 but with a larger dispersion on other model parameters, which make us favor the Alpha parameterization of turbulence. Implications for planetary system development in these systems are presented. In particular, GM Aur is a massive and slowly evolving disk where conditions are very favorable for planetesimal growth. The large value of present disk mass and the relatively small observed accretion rate of this system may also be indicative of the presence of an inner gas giant planet. Acknowledgements: This work has been supported by Programme Nationale de Planetologie. R. Hueso acknowledges a post-doctoral fellowship from Gobierno Vasco.

  16. Monitoring of Climate Change in Germany - Data, products and services of Germany's National Climate Data Centre

    NASA Astrophysics Data System (ADS)

    Kaspar, F.; Penda, E.; Müller-Westermeier, G.; Zimmermann, K.; Mächel, H.

    2012-04-01

    Germany's meteorological service (Deutscher Wetterdienst, DWD) is responsible for monitoring climate change in Germany. The section "National Climate Monitoring" is responsible for operating the National Climate Data Centre (NCDC, "Nationales KlimaDatenZentrum NKDZ") and for provision of statistical data derived from these observations. The NCDC database mainly comprises 'conventional' in-situ observations that are observed within the station network of DWD, but also other categories of data, e.g. phenological observations. The main aim of the NCDC is the sustained development of a comprehensive data base of high quality, which provides basic information for climate research and applied climatology. A major focus of the activity is to guarantee a defined data quality by means of validation and correction of the data (or at least a description of errors), as well as a detailed description of the data base. The main focus of these quality assurance tasks has been shifted to the quality control of previously insufficiently verified historical data. The data base can be used to analyse the climate in Germany over a period of more than 100 years. DWD's National Climate Data Centre is thus the reference for climate data from stations in Germany and acts as data supplier especially for national climate research, but data and products are also used in international projects. In order to complete the data base for historic periods (esp. the first half of the 20th century), original paper documents are currently digitized and integrated into the data base. External customers may obtain data and products directly via Internet-based access tools. DWD currently starts to provide access to its climate data based on standards of the Open Geospatial Consortium (OGC), e.g. Web Mapping Services (WMS) to provide access to the derived gridded data products of NCDC.

  17. Using Remotely Piloted Aircraft System to Study the Evolution of the Boundary Layer Related to Fog Events

    NASA Astrophysics Data System (ADS)

    Roberts, G. C.; Cayez, G.; Ronflé-Nadaud, C.; Albrand, M.; Dralet, J. P.; Momboisse, G.; Nicoll, K.; Seity, Y.; Bronz, M.; Hattenberger, G.; Gorraz, M.; Bustico, A.

    2014-12-01

    Over the past decade, the scientific community has embraced the use of RPAS (remotely piloted aircraft system) as a tool to improve observations of the Earth's surface and atmospheric phenomena. The use of small RPAS (Remotely Piloted Aircraft System) in atmospheric research has increased because of their relative low-cost, compact size and ease of operation. Small RPAS are especially adapted for observing the atmospheric boundary layer processes at high vertical and temporal resolution. To this end, CNRM, ENAC, and ENM have developed the VOLTIGE (Vecteurs d'Observation de La Troposphere pour l'Investigation et la Gestion de l'Environnement) program to study the life cycle of fog with multiple, small RPAS. The instrumented RPAS flights have successfully observed the evolution of the boundary layer and dissipation of fog events. In addition, vertical profiles from the RPAS have been compared with Météo France forecast models, and the results suggest that forecast models may be improved using high resolution and frequent in-situ measurements. Within the VOLTIGE project, a flying-wing RPAS with four control surfaces was developed to separate elevator and aileron controls in order to reduce the pitch angle envelope and improve turbulence and albedo measurements. The result leads to a small RPAS with the capability of flying up to two hours with 150 grams of payload, while keeping the hand-launch capability as a constraint for regular atmospheric research missions. High frequency data logging has been integrated into the main autopilot in order to synchronize navigation and payload measurements, as well as allowing an efficient sensor-based navigation. The VOLTIGE program also encourages direct participation of students on the advancement of novel observing systems for atmospheric sciences, and provides a step towards deploying small RPAS in an operational network. VOLTIGE is funded by the Agence Nationale de Recherche (ANR-Blanc 2012) and supported by Aerospace

  18. Physicochemical characterization of the thermal aging of insulating paper in power transformers

    SciTech Connect

    Lessard, M.C.; Van Nifterik, L.; Masse, M.; Penneau, J.F.; Grob, R.

    1996-12-31

    Paper is a low-cost base material with outstanding mechanical and electrical properties, which is why it is still a key element in the insulation of electrical apparatus. Under the effect of a variety of factors including temperature, paper can substantially lose its properties, thus jeopardizing the service life of costly equipment. To remedy this situation, new so-called thermally upgraded papers are being made by certain manufacturers. A study carried out jointly by Hydro-Quebec, Electricite de France and the Ecole Nationale Superieure de Chimie de Toulouse has allowed researchers to qualify the thermal resistance of three different types of thermostable paper. These papers have been selected as being representative of what is available on the market today. The paper samples were subjected to a thermal aging test in the presence of mineral oil to represent normal conditions of operation (150 C). The thermal degradation of the paper insulation is characterized by various physicochemical methods including measurement of the degree of polymerization, determination of 2-furfural in mineral oil by HPLC as well as determination of various sugars (monosaccharides, polysaccharides and anhydrosugars) in the paper using ion chromatography. This last method allows the authors to verify the formation of cellobiose, which is the real repeat unit of cellulose, as well as that of levoglucosan, which is an anhydrosugar and a precursor of 2-furfural. The evolution of all of these parameters, measured as a function of time, has allowed them to compare the thermal resistance of various insulating papers. The results of this study seem to show that, compared to traditional kraft paper, certain paper types are more susceptible to being thermally upgraded than others. This study also allowed the authors to demonstrate that the use of an inhibitor in mineral oil (DBPC) does not seem to influence the thermal degradation of these papers.

  19. A Secular Variation Model for Igrf-12 Based on Swarm Data and Inverse Geodynamo Modelling

    NASA Astrophysics Data System (ADS)

    Fournier, A.; Aubert, J.; Erwan, T.

    2014-12-01

    We are proposing a secular variation candidate model for the 12th generation of the international geomagnetic reference field, spanning the years 2015-2020. The novelty of our approach stands in the initialization of a 5-yr long integration of a numerical model of Earth's dynamo by means of inverse geodynamo modelling, as introduced by Aubert (GJI, 2014). This inverse technique combines the information coming from the observations (in the form of an instantaneous estimate of the Gauss coefficients for the magnetic field and its secular variation) with that coming from the multivariate statistics of a free run of a numerical model of the geodynamo. The Gauss coefficients and their error covariance properties are determined from Swarm data along the lines detailed by Thébault et al. (EPS, 2010). The numerical model of the geodynamo is the so-called Coupled Earth Dynamo model (Aubert et al., Nature, 2013), whose variability possesses a strong level of similarity with that of the geomagnetic field. We illustrate and assess the potential of this methodology by applying it to recent time intervals, with an initialization based on CHAMP data, and conclude by presenting our SV candidate, whose initialization is based on the 1st year of Swarm data This work is supported by the French "Agence Nationale de la Recherche" under the grant ANR-11-BS56-011 (http://avsgeomag.ipgp.fr) and by the CNES. References: Aubert, J., Geophys. J. Int. 197, 1321-1334, 2014, doi: 10.1093/gji/ggu064 Aubert, J., Finlay, C., Fournier, F. Nature 502, 219-223, 2013, doi: 10.1038/nature12574 Thébault E. , A. Chulliat, S. Maus, G. Hulot, B. Langais, A. Chambodut and M. Menvielle, Earth Planets Space, Vol. 62 (No. 10), pp. 753-763, 2010.

  20. La prévention des blessures non intentionnelles chez les enfants et adolescents autochtones au Canada

    PubMed Central

    Banerji, Anna

    2012-01-01

    RÉSUMÉ Les blessures non intentionnelles sont la principale cause de décès chez les enfants et adolescents autochtones canadiens, à un taux de trois à quatre fois la moyenne nationale. Non seulement les décès et les blessures invalidantes dévastent les familles et les communautés, mais elles font également d’énormes ravages sur les ressources de santé. L’absence de statistiques, de surveillance continue ou de programmes de prévention des blessures à l’égard des enfants et adolescents autochtones exacerbe les coûts en matière de main-d’œuvre et de santé. Les communautés autochtones sont hétérogènes sur le plan culturel, qu’il s’agisse de l’accès aux ressources ou même des risques et des types de blessures. Pourtant, en général, ces communautés sont beaucoup plus susceptibles d’être pauvres, d’habiter dans un logement insalubre et d’éprouver de la difficulté à accéder aux soins de santé, des facteurs qui accroissent le risque et les conséquences des blessures. Il existe un besoin urgent de surveillance des blessures, de recherche, de renforcement des capacités, de diffusion des connaissances et de programmes de prévention des blessures qui sont axés sur les populations autochtones. Pour prévenir les blessures de manière efficace, il faut adopter des démarches multidisciplinaires, coopératives et durables, fondées sur des pratiques exemplaires, tout en étant spécifiques et sensibles sur le plan culturel et linguistique.

  1. Measuring IVDF through high-aspect holes in pulsed ICP plasma

    NASA Astrophysics Data System (ADS)

    Cunge, Gilles; Darnon, Maxime; Dubois, Jerome; Bezard, Philippe; Mourey, Odile; Petit-Etienne, Camille; Vallier, Laurent; Despiau-Pujo, Emilie; Joubert, Olivier; Sadeghi, Nader

    2015-09-01

    Plasma etching of high aspect-ratio (AR) structures is challenging. Several issues originate from the ion angular distribution: the feature sidewalls are bombarded by energetic ions and the ion flux at the bottom of the features is reduced. In ICP reactors at low pressure, this angular dispersion is due to two effects: the finite transverse velocity component of the ions when they enter the sheath region (i.e. the ion temperature Ti in plasma bulk) and charging effect of the feature sidewalls. To analyze those effects, we have measured the IVDF at the wafer surface in an industrial ICP reactor (AMAT) by using Semion multigrid ion energy analyzers. The plasma is operated in different chemistries (Ar, He, H2 and CF4) both in CW and pulsed mode. To analyze ion transport through high AR holes, we place 0.4 mm thick capillary plates with holes of AR 16, 8 and 4 in front of the RFA analyzer, which then probe IVDF at the exit of these holes. The results show that the ion flux drops dramatically when the AR is increased. By comparing the measured IVDF with an analytical model which calculates the transmission of a hole as a function of its AR and of Ti we concluded that Ti is about 3000 K. Charging effects are also observed and are shown to reduce significantly the ion energy at the feature bottom but with a ``minor'' effect on the ion flux and shape of the IVDF. We will discuss electropositive versus electronegative gases, pulsing and the role of ion mass on charging. This project is funded by the French Agence Nationale de la Recherche in the frame of the project clean GRAPH (ANR-13-BS09-0019).

  2. A passive brain-computer interface application for the mental workload assessment on professional air traffic controllers during realistic air traffic control tasks.

    PubMed

    Aricò, P; Borghini, G; Di Flumeri, G; Colosimo, A; Pozzi, S; Babiloni, F

    2016-01-01

    In the last decades, it has been a fast-growing concept in the neuroscience field. The passive brain-computer interface (p-BCI) systems allow to improve the human-machine interaction (HMI) in operational environments, by using the covert brain activity (eg, mental workload) of the operator. However, p-BCI technology could suffer from some practical issues when used outside the laboratories. In particular, one of the most important limitations is the necessity to recalibrate the p-BCI system each time before its use, to avoid a significant reduction of its reliability in the detection of the considered mental states. The objective of the proposed study was to provide an example of p-BCIs used to evaluate the users' mental workload in a real operational environment. For this purpose, through the facilities provided by the École Nationale de l'Aviation Civile of Toulouse (France), the cerebral activity of 12 professional air traffic control officers (ATCOs) has been recorded while performing high realistic air traffic management scenarios. By the analysis of the ATCOs' brain activity (electroencephalographic signal-EEG) and the subjective workload perception (instantaneous self-assessment) provided by both the examined ATCOs and external air traffic control experts, it has been possible to estimate and evaluate the variation of the mental workload under which the controllers were operating. The results showed (i) a high significant correlation between the neurophysiological and the subjective workload assessment, and (ii) a high reliability over time (up to a month) of the proposed algorithm that was also able to maintain high discrimination accuracies by using a low number of EEG electrodes (~3 EEG channels). In conclusion, the proposed methodology demonstrated the suitability of p-BCI systems in operational environments and the advantages of the neurophysiological measures with respect to the subjective ones. PMID:27590973

  3. Localized Resectable Genitourinary Sarcoma in Adult Korean Patients: Experiences at a Single Center

    PubMed Central

    Cho, Sung Yong; Moon, Kyung Chul; Cheong, Min Su; Kwak, Cheol; Kim, Hyeon Hoe

    2011-01-01

    Purpose To evaluate the clinicopathological characteristics and prognosis of localized resectable genitourinary sarcomas in adults. Materials and Methods Between September, 1996 and November, 2008, 18 consecutive cases of adults (12 men and 6 women; median age 48.8 years) who were treated for primary genitourinary sarcomas were identified. The following variables were analyzed: patient age, gender, body mass index, American Society of Anesthesiologists (ASA) score, primary organ, tumor histology, size, necrosis, Fédération Nationale des Centres de Lutte Contre le Cancer (FNCLCC) grade, and surgical margin positivity. Recurrence-free survival and disease-specific survival were the study end-points. Results The most common presenting symptom was a palpable mass (six cases, 33.3%), the most common site was the kidney (six cases, 33.3%), and the most common histological subtype was leiomyosarcoma (eight patients, 44.4%). Complete resection with negative surgical margins was achieved in 13 patients (72.2%). The median follow-up period was 49.9 months (range 6.4 to 147.6). The recurrence-free survival rates at 1, 3, and 5 years were 81.6%, 66.5%, and 66.5%, respectively. Recurrence-free survival only associated significantly with ASA score (p=0.018). The disease-specific survival rate at 1, 3, and 5 years was 88.9%, 76.2%, and 67.7%, respectively. Disease-specific survival was associated significantly only with FNCLCC grade (p=0.042). Conclusion Although genitourinary sarcomas in adults are a rare group of tumors with a poor prognosis, some patients may have a favorable prognosis. Our findings suggest that FNCLCC grade is the most important prognostic factor for these patients. PMID:21786440

  4. Reptiles with dermatological lesions: a retrospective study of 301 cases at two university veterinary teaching hospitals (1992-2008).

    PubMed

    White, Stephen D; Bourdeau, Patrick; Bruet, Vincent; Kass, Philip H; Tell, Lisa; Hawkins, Michelle G

    2011-04-01

    This retrospective study reviews the medical records of 301 reptiles with dermatological lesions that were examined at the Veterinary Medical Teaching Hospital, University of California at Davis (VMTH-UCD) and the Unité de Dermatologie-Parasitologie-Mycologie, Ecole Nationale Vétérinaire de Nantes (UDPM-ENVN) from 1 January 1992 to 1 July 2008. The most common reptile groups differed between the two hospitals, with lizards being the most common at the VMTH-UCD and chelonians at the UDPM-ENVN. At the VMTH-UCD, boa constrictors (Boa constrictor), ball pythons (Python regius) and other Python species were over-represented, and box turtles (Terrapene carolina) were under-represented in the dermatological lesion caseload. When institutional data were combined, 47% of all reptiles at both institutions with confirmed or suspected cases of sepsis had petechiae, with the highest association seen in chelonians at 82%. Dependent on institution and reptile group, from 29% to 64% of the cases had underlying husbandry issues. Sixty-two per cent of all cases were alive at final status. Veterinarians treating reptiles with skin disease should be aware of the following: (i) that boa constrictors and Python species may be predisposed to dermatological lesions; (ii) that client education is important for proper husbandry; and (iii) that there is a possible association between petechiae and sepsis, especially in chelonians. The conjectural association between certain skin lesions and sepsis remains to be confirmed by systematically derived data that demonstrate a causal relationship between the two. PMID:20887405

  5. Orbit determination support of the Ocean Topography Experiment (TOPEX)/Poseidon operational orbit

    NASA Technical Reports Server (NTRS)

    Schanzle, A. F.; Rovnak, J. E.; Bolvin, D. T.; Doll, C. E.

    1993-01-01

    The Ocean Topography Experiment (TOPEX/Poseidon) mission is designed to determine the topography of the Earth's sea surface over a 3-year period, beginning shortly after launch in July 1992. TOPEX/Poseidon is a joint venture between the United States National Aeronautics and Space Administration (NASA) and the French Centre Nationale d'Etudes Spatiales. The Jet Propulsion Laboratory is NASA's TOPEX/Poseidon project center. The Tracking and Data Relay Satellite System (TDRSS) will nominally be used to support the day-to-day orbit determination aspects of the mission. Due to its extensive experience with TDRSS tracking data, the NASA Goddard Space Flight Center (GSFC) Flight Dynamics Facility (FDF) will receive and process TDRSS observational data. To fulfill the scientific goals of the mission, it is necessary to achieve and maintain a very precise orbit. The most stringent accuracy requirements are associated with planning and evaluating orbit maneuvers, which will place the spacecraft in its mission orbit and maintain the required ground track. To determine if the FDF can meet the TOPEX/Poseidon maneuver accuracy requirements, covariance analysis was undertaken with the Orbit Determination Error Analysis System (ODEAS). The covariance analysis addressed many aspects of TOPEX/Poseidon orbit determination, including arc length, force models, and other processing options. The most recent analysis has focused on determining the size of the geopotential field necessary to meet the maneuver support requirements. Analysis was undertaken with the full 50 x 50 Goddard Earth Model (GEM) T3 field as well as smaller representations of this model.

  6. Materials vigilance and traceability.

    PubMed

    Tracol, P

    2016-02-01

    Patient safety requires speedy detection of any medical device malfunction; this is known as "materials vigilance". It entails the need to be able to trace back the life-long pathway of a device; this is "traceability". European regulations enact free circulation of medical devices throughout the European Union, with each member state being responsible for safety within its own territory. Medical devices are divided into 3 categories of increasing risk. CE marking mandatory for medical devices distributed within the EU, and count as market authorizations. They are delivered with 5-year validity by what is known as a "notified body". Health authorities are responsible for monitoring the market and any incidents. New regulations are presently being drawn up to improve efficiency and transparency. Materials vigilance is founded on mandatory declaration of medical device incidents. At local level, it comprises local reporters responsible for informing the National Health Products Safety Agency (Agence nationale de sécurité du médicament et des produits de santé [ANSM]) of any incidents and taking all necessary precautions. At national level, the ANSM assesses the safety, efficacy and quality of healthcare products; it centralizes and assesses materials vigilance reports and takes the requisite decisions. Materials vigilance is further organized at the European and international levels, to harmonize legislation regarding medical devices. Traceability is intended to rapidly identify medical device bearers in case of product recall. Each center is to organize the traceability of its devices; manufacturers' obligation of traceability ceases with the healthcare establishment or user. CE marking involves strict labeling rules to ensure safety of use. A change in the organization of traceability is presently underway, in the form of international Unique Device Identifiers, with harmonized label data, barcodes and standardized terminology. A European and later

  7. The Mysterious sdO X-ray Binary BD+37°442

    NASA Astrophysics Data System (ADS)

    Heber, U.; Geier, S.; Irrgang, A.; Schneider, D.; Barbu-Barna, I.; Mereghetti, S.; La Palombara, N.

    2014-04-01

    Pulsed X-ray emission in the luminous, helium-rich sdO BD +37°442 has recently been discovered (La Palombara et al. 2012). It was suggested that the sdO star has a neutron star or white dwarf companion with a spin period of 19.2 s. After HD 49798, which has a massive white dwarf companion spinning at 13.2 s in an 1.55 day orbit, this is only the second O-type subdwarf from which X-ray emission has been detected. We report preliminary results of our ongoing campaign to obtain time-resolved high-resolution spectroscopy using the CAFE instrument at Calar Alto observatory and SARG at the Telescopio Nationale Galileo. Atmospheric parameters were derived via a quantitative NLTE spectral analysis. The line fits hint at an unusually large projected rotation velocity. Therefore it seemed likely that BD +37°442 is a binary similar to HD 49798 and that the orbital period is also similar. The level of X-ray emission from BD +37°442 could be explained by accretion from the sdO wind by a neutron star orbiting at a period of less than ten days. Hence, we embarked on radial velocity monitoring in order to derive the binary parameters of the BD+37°442 system and obtained 41 spectra spread out over several month in 2012. Unlike for HD 49798, no radial velocity variations were found and, hence, there is no dynamical evidence for the existence of a compact companion yet. The origin of the pulsed X-ray emission remains as a mystery.

  8. Prototype pushing robot for emplacing vitrified waste canisters into horizontal disposal drifts

    SciTech Connect

    Londe, L.; Seidler, W.K.; Bosgiraud, J.M.; Guenin, J.J.; Devaux, P.

    2007-07-01

    Within the French Underground Disposal concept, as described in ANDRA's (Agence Nationale pour la Gestion des Dechets Radioactifs) Dossier 2005, the Pushing Robot is an application envisaged for the emplacement (and the potential retrieval) of 'Vitrified waste packages', also called 'C type packages'. ANDRA has developed a Prototype Pushing Robot within the framework of the ESDRED Project (Engineering Studies and Demonstration of Repository Design) which is co-funded by the European Commission as part of the sixth EURATOM Research and Training Framework Programme (FP6) on nuclear energy (2002 - 2006). The Rationale of the Pushing Robot technology comes from various considerations, including the need for (1) a simple and robust system, capable of moving (and potentially retrieving) on up to 40 metres (m), a 2 tonne C type package (mounted on ceramic sliding runners) inside the carbon steel sleeve constituting the liner (and rock support) of a horizontal disposal cell, (2) small annular clearances between the package and the liner, (3) compactness of the device to be transferred from surface to underground, jointly with the package, inside a shielding cask, and (4) remote controlled operations for the sake of radioprotection. The initial design, based on gripping supports, has been replaced by a 'technical variant' based on inflatable toric jacks. It was then possible, using a test bench, to check that the Pushing Robot worked properly. Steps as high as 7 mm were successfully cleared by a dummy package pushed by the Prototype.. Based on the lessons learned by ANDRA's regarding the Prototype Pushing Robot, a new Scope of Work is being written for the Contract concerning an Industrial Scale Demonstrator. The Industrial Scale Demonstration should be completed by the end of the second Quarter of 2008. (authors)

  9. Grading of Non-Rhabdomyosarcoma Soft Tissue Sarcoma in Children and Adolescents: A Comparison of Parameters Used for the FNCLCC and POG systems

    PubMed Central

    Khoury, Joseph D.; Coffin, Cheryl M.; Spunt, Sheri L.; Anderson, James R.; Meyer, William H.; Parham, David M.

    2010-01-01

    Two systems for grading soft tissue sarcoma are widely used currently: the National Cancer Institute (NCI) and the Fédération Nationale des Centers de Lutte Contre le Cancer (FNCLCC) systems. Both were developed using cohorts of predominantly adult patients. The Pediatric Oncology Group (POG) system, based on the NCI system, was adapted for grading pediatric non-rhabdomyosarcoma soft tissue sarcoma (NRSTS). The applicability and prognostic utility of the FNCLCC system in pediatric NRSTS has not been assessed or compared to the POG system. Tumors from 130 patients with malignant NRSTS enrolled on three completed multi-institutional clinical trials were assessed. Of 130 tumors, 102 (78%) were localized and 28 (22%) metastatic. Of the localized tumors, 55/102 (54%) were >5cm. The estimated 5-year EFS for the entire group was 47%. As expected, stage and tumor size were predictive of EFS (p<0.001). Both systems were predictive of 5-year event-free survival (EFS) (POG p=0.0095 and FNCLCC p=0.0075). Patients whose tumors received discrepant grades (POG-G3 vs. FNCLCC-G2/G1) (n=44) had an intermediate outcome between those with concordant (G3 (n=44) or G1/G2 (n=42)) grades on both systems (p=0.0018). By multivariate analysis, the mitotic index was predictive of EFS using a cutoff of 10 mitotic figures per 10 high power fields (p<0.001). In conclusion, both the FNCLCC and POG systems provide an adequate prognostic measure of outcome for pediatric NRSTS; albeit, a sizeable subset of cases with apparently intermediate prognosis was graded differently by the two systems. The mitotic index appears to be a key parameter in grading pediatric NRSTS. PMID:20166208

  10. Soins primaires des personnes victimes d’une lésion médullaire

    PubMed Central

    McColl, Mary Ann; Aiken, Alice; McColl, Alexander; Sakakibara, Brodie; Smith, Karen

    2012-01-01

    Résumé Objectif Effectuer une étude de la portée des données empiriques, entre 1980 et 2009, concernant les soins primaires aux adultes victimes d’une lésion médullaire (LME). Sources des données Une recension dans des revues révisées par des pairs de1980 à 2009 à l’aide de CINAHL, PubMed-MEDLINE, EMBASE, PsycINFO, Social Sciences Abstracts et Social Work Abstracts. Sélection des études La recherche électronique au moyen de mots-clés a permis de cerner 42 articles sur les soins primaires et les LME. Des critères d’inclusion ont servi à réduire la liste à un ensemble de 21 articles publiés en anglais qui portaient sur un échantillon de plus de 3 et présentaient une analyse empirique. Synthèse Environ 90 % des personnes atteintes d’une LME ont identifié leur médecin de famille comme étant leur docteur habituel; 63 % avaient un spécialiste des LME. Les personnes vivant à long terme avec une LME développent des rubriques complexes pour naviguer dans leurs systèmes de soins de santé personnels. Les données scientifiques ne sont pas unanimes quant à l’efficacité des programmes d’intervention directe pour le maintien de la santé et la prévention des complications à la suite d’une LME. Les données appuient cependant le suivi périodique par une équipe spécialisée et un bilan de santé annuel complet. La recherche fait valoir un fort degré d’uniformité dans l’identification des problèmes les plus courants soulevés par les personnes atteintes d’une LME en soins primaires, dont la plupart concernent l’incapacité, plus précisément les complications secondaires, comme la dysfonction intestinale ou vésicale et la douleur. Il existe aussi de bonnes données probantes à l’effet que de nombreux problèmes de santé généraux exigent de l’attention dans une telle population, comme les problèmes de la densité osseuse, la dépression et les questions entourant la santé sexuelle et la reproduction. Il y a

  11. La nutrition du nourrisson né à terme et en santé

    PubMed Central

    1998-01-01

    La nutrition du nourrisson né à terme et en santé constitue le nouvel énoncé national sur la nutrition du nourrisson, de la naissance à l’âge de 24 mois. Il s’agit d’un projet conjoint de la Société canadienne de pédiatrie, des Diététistes du Canada et de Santé Canada. Cet ouvrage est une synthèse de la documentation scientifique actuelle en matière de nutrition du nourrisson ; il contient des principes et recommandations afin d’aider les professionnels de la santé à promouvoir la prestation des meilleurs soins alimentaires possibles pour les nourrissons du Canada, compte tenu de l’état actuel de la recherche. La collaboration entre les trois principaux organismes qui s’intéressent à cette question a permis d’uniformisé le message que les professionnels transmettront au public. Le document aborde quatre grands sujets relatifs à la première année d’existence : l’allaitement, les laits de remplacement, les autres liquides dans le régime du nourrisson et la transition aux aliments solides. On y examine ensuite la question de la sécurité dans l’alimentation, puis celle de la nutrition durant la deuxième année. La dernière section couvre les autres questions liées à la nutrition du nourrisson ; on y traite de sujets tels que les allergies alimentaires, les coliques, la constipation, les matières grasses dans le régime alimentaire, la carie dentaire, la gastroentérite, le diabète, l’anémie ferriprive et les régimes végétariens. Le document contient également un répertoire complet de plus de 200 citations. Le sommaire des principes et recommandations paraîtra dans les revues officielles de la Société canadienne de pédiatrie (Paediatrics and Child Health, 1998) et des Diététistes du Canada (Revue canadienne de pratique et de recherche en diététique, juin 1998). On peut télécharger le document intégral à partir des sites Web respectifs des trois organismes associés ; on peut aussi obtenir la

  12. The Teen Science Café Network

    NASA Astrophysics Data System (ADS)

    Hall, M.; Mayhew, M. A.

    2013-12-01

    The 'Teen Cafè' phenomenon grew out of an NSF-funded experiment to bring the Cafè Scientifique model for engagement of the public with science and scientists to high school teenagers. Cafè Scientifique New Mexico (cafènm.org), now in its seventh year, has proven highly popular with high school teens for much the same reason as for adult Cafè programs: the blend of socializing in an attractive venue and interaction with a scientist on an interesting science topic. Teen Cafés also include exploration of the topic with hands-on activities. The success of the model has led to the creation of the national Teen Science Cafè Network (teensciencecafe.org. This first year of the new program, four 'Founding Members' of the Network-- in Florida, Colorado, North Carolina, and the St. Louis, Missouri region--started up Teen Cafè programs. Each applied the model with a unique flair appropriate to local institutions and demographics. Each Member in the Network runs Cafès in multiple local venues. We are now gearing up for our second year, and the Network is growing. Our Teen Cafè topics have covered a very wide range, from belly-button biodiversity to cyber-security to patterns of mega-earthquakes to a day in the life of a teen dolphin to corals on acid to emergency room medicine to alternative fuel cars. Presenters have come from a great variety of local institutions. Though they are popular with teens because they are fun and interesting, our evaluations have demonstrated that the programs are having a significant impact on participating teens' understanding of the nature of science, the work that scientists do, and the importance of science to their daily lives. We are also having success in training scientists to communicate effectively with this public audience. Presenters report strong satisfaction with their resulting quality of science communication. A surprising number have reported that their experience with the program has led them to think in a new way about

  13. Galactic abundance gradients from Cepheids. α and heavy elements in the outer disk

    NASA Astrophysics Data System (ADS)

    Lemasle, B.; François, P.; Genovali, K.; Kovtyukh, V. V.; Bono, G.; Inno, L.; Laney, C. D.; Kaper, L.; Bergemann, M.; Fabrizio, M.; Matsunaga, N.; Pedicelli, S.; Primas, F.; Romaniello, M.

    2013-10-01

    at the Canada-France-Hawaii Telescope (CFHT), which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. Based on observations collected with FEROS at the European Southern Observatory (La Silla, Chile) under proposal ID: 60.A-9120. Based on observations obtained at the Telescope Bernard Lyot (USR5026) operated by the Observatoire Midi-Pyrénées and the Institut National des Science de l'Univers of the Centre National de la Recherche Scientifique of France. The data of NARVAL were reduced using the data reduction software Libre-ESpRIT, written and provided by Donati from the LATT (Observatoire Midi-Pyrénées).Appendices are available in electronic form at http://www.aanda.org

  14. Magnetic field structure in single late-type giants: β Ceti in 2010-2012

    NASA Astrophysics Data System (ADS)

    Tsvetkova, S.; Petit, P.; Aurière, M.; Konstantinova-Antova, R.; Wade, G. A.; Charbonnel, C.; Decressin, T.; Bogdanovski, R.

    2013-08-01

    status of the star, we suggest that dynamo action alone may not be efficient enough to account for the high magnetic activity of β Ceti. As an alternate option, we propose that it is a descendant of an Ap star presently undergoing central helium-burning and still exhibiting a remnant of the Ap star magnetic field. Based on observations obtained at the Bernard Lyot Télescope (TBL, Pic du Midi, France) of the Midi-Pyrénées Observatory, which is operated by the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France and Université de Toulouse, and at the Canada-France-Hawaii Telescope (CFHT), which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.Table 1 is available in electronic form at http://www.aanda.org

  15. Préface

    NASA Astrophysics Data System (ADS)

    Hamieh, Tayssir

    2005-05-01

    Né simultanément à Mulhouse et à Beyrouth en 1996 dans le cadre d'une collaboraiion franco-libanaise sur une initiative personnelle de Monsieur Tayssir HAMIEH. le Colloque Franco-Libanais sur la Science des Matériaux (CSM), qui s'inscrit dans le cadre des relations étroites entre la France et le Liban, est très vite devenu une occasion très importante de rencontre entre scientifiques de haut niveau, non seulement, du contour méditerranéen mais également des pays européens, américains et arabes. La quatrieme édition CSM4 est une véritable réussite grâce à la participation des chercheurs confirmés dans tous les domaines des sciences de matériaux et venant de plusieurs pays tels que la France, I'Algérie, Le Liban, la Syrie, le Maroc, la Tunisie, l'Italie, l'Espagne, le Portugal, le Royaume Uni, les États-Unis, la Russie, l'Allemagne, le Japon et I'Inde ; pour présenter plus de 350 communications orales et par affiche et couvrant presque toutes les disciplines des systèmes des matériaux. Le choix des diffèrents thèmes du colloque sur la science des matériaux a été dicté par l'importance capitale de cette discipline dans notre civilisation moderne. En fait, les matériaux utilisés pour la fabrication artisanale ou industrielle d'objets, de produits et de systèmes ainsi que pour la réalisation de constructions et d'équipements ont de tout temps défini le niveau de notre civilisation technique. La réalisation des objectifs communs de notre monde en plein développement, pour ne pas dire en pleine mutation, est en grande partie tributaire de la mise au point de nouveaux matériaux et de procédés de transformation et d'assemblages nouveaux, présentant des performances et des qualités améliorées. Le colloque a illustré et traduit, de manière remarquables, l'excellente collaboration entre chercheurs libanais et français. Le partenariat est exemplaire par la qualité des laboratoires impliqués et par le niveau scientifique des r

  16. Assembly and test of MEDUSA, a multi-spectral instrument for stratospheric Earth observation

    NASA Astrophysics Data System (ADS)

    Delauré, B.; Van Achteren, T.; Everaerts, J.; Livens, S.; Beghuin, D.

    2008-10-01

    MEDUSA is a lightweight high resolution camera, designed to operate at stratospheric altitudes mounted on a solar-powered unmanned aerial vehicle (UAV). The MEDUSA instrument targets applications such as crisis monitoring and large scale mapping, requiring high resolution images with regional coverage, flexible flight patterns, high update rates and long mission lengths (weeks to months). The instrument is subject to severe constraints on mass (< 2,5 kg), volume, power consumption and survivability in the stratospheric environment. Operating temperatures within the payload vary over several tens of degrees Celsius over the day-night cycle. Nonetheless, the instrument will be able to provide panchromatic and color images of 30 cm ground resolution at an altitude of 18000 m and a wide swath of 3000m. This ESA-PRODEX (PROgramme de Développement d'Expériences scientifiques) funded project successfully passed the Critical Design Review in September 2007 and the assembly, integration and test (AIT) phase of the subsystems will be finalized by the end of 2008. Subsystem tests include an optical performance verification performed on optical compartment with a test-sensor assembly both at ambient and operational environmental conditions. The electronic subsystems and their interfaces are tested for functionality and performance in the operational temperature and pressure range. From early 2009 onwards, the MEDUSA system will be fully integrated including a custom designed wide swath MEDUSA CMOS frame sensor (10000x1200 pixels). The MEDUSA instrument will be ready for its first flight in spring of 2009. The detailed design of the optical instrument and its performances have been discussed in [1]. In this paper we will give an overview of the AIT status of the MEDUSA sensor and the optical system and an outlook on the system integration and test phase.

  17. On the global model for foF2 using neural networks

    NASA Astrophysics Data System (ADS)

    Oyeyemi, E. O.; Poole, A. W. V.; McKinnell, L. A.

    2005-12-01

    The use of neural networks (NNs) has been employed in this work to develop a global model of the ionospheric F2 region critical frequency, foF2. The main principle behind our approach has been to utilize parameters other than simple geographic coordinates, on which foF2 is known to depend, and to exploit the ability of NNs to establish and model this nonlinear relationship for predictive purposes. The foF2 data used in the training of the NNs were obtained from 59 ionospheric stations across the globe at various times from 1964 to 1986, on the basis of availability. To test the success of this approach, one NN (NN1) was trained without data from 13 stations, selected for their geographic remoteness, which could then be used to validate the predictions of the NN for those remote coordinates. These stations were subsequently included in our final NN (NN2). The input parameters consisted of day number (day of the year), universal time, solar activity, magnetic activity, geographic latitude, angle of meridian relative to subsolar point, magnetic dip angle, magnetic declination, and solar zenith angle. Comparisons between foF2 values determined using NNs and the International Reference Ionosphere (IRI) model (from Union Radio Scientifique Internationale (URSI) and International Radio Consultative Committee (CCIR) coefficients) with observed values are given with their root-mean-square (RMS) error differences for test stations. The results from NN2 are used to produce the global behavior of hourly values of foF2 and are compared with the IRI model using URSI and CCIR coefficients. The results obtained (i.e., RMS error differences), which compare favorably with the IRI models, justify this technique for global foF2 modeling.

  18. Le syndrome de Cri du Chat : A propos d’une observation

    PubMed Central

    Ouldim, Karim; Samri, Imane; Bouguenouch, Laila; Hamdaoui, Hasna; Otmani, Ihsan El; Hbibi, Mohamed; Chaouki, Sana; Hida, Moustapha

    2012-01-01

    Le syndrome du Cri du Chat (Cri du Chat syndrome, CdCS) est une anomalie chromosomique résultant d’une délétion de taille variable de l’extrémité du bras court du chromosome 5 (5p), incluant une région critique située en p15.2. Il représente une des délétions chromosomiques les plus fréquentes, son incidence dans la population générale est de 1/20 000 à 1/50 000. Les caractéristiques cliniques comprennent un cri monochromatique aigu, une microcéphalie, une dysmorphie cranio-faciale caractéristique évoluant avec l’âge et un retard mental et psychomoteur important. La taille de la délétion est variable, Le traitement est fonction des différents symptômes. Un remaniement chromosomique parental est retrouvé dans 12% des cas et la majorité des délétions responsables de la maladie du cri-du-chat surviennent de novo. Nous présentons une observation d’un syndrome du Cri du Chat, confirmé par caryotype métaphasique (46,XY,del(5)(p13) de novo). A travers cette observation nous mettrons à jour, les actualités scientifiques de ce rare syndrome, ainsi que la place des explorations cytogénétiques dans le diagnostic précis et le conseil génétique des syndromes dysmorphiques. PMID:22368747

  19. TRIDENT: An Infrared Differential Imaging Camera Optimized for the Detection of Methanated Substellar Companions

    NASA Astrophysics Data System (ADS)

    Marois, Christian; Doyon, René; Nadeau, Daniel; Racine, René; Riopel, Martin; Vallée, Philippe; Lafrenière, David

    2005-07-01

    We describe a near-infrared camera in use at the Canada-France-Hawaii Telescope (CFHT) and at the 1.6 m telescope of the Observatoire du mont Mégantic (OMM). The camera is based on a Hawaii-1 1024 × 1024 HgCdTe array detector. Its main feature is the acquisition of three simultaneous images at three wavelengths across the methane absorption bandhead at 1.6 μm, enabling, in theory, an accurate subtraction of the stellar point-spread function (PSF) and the detection of faint close, methanated companions. The instrument has no coronagraph and features fast data acquisition, yielding high observing efficiency on bright stars. The performance of the instrument is described, and it is illustrated by laboratory tests and CFHT observations of the nearby stars GL 526, υ And, and χ And. TRIDENT can detect (6 σ) a methanated companion with ΔH=9.5 at 0.5" separation from the star in 1 hr of observing time. Non-common-path aberrations and amplitude modulation differences between the three optical paths are likely to be the limiting factors preventing further PSF attenuation. Instrument rotation and reference-star subtraction improve the detection limit by a factor of 2 and 4, respectively. A PSF noise attenuation model is presented to estimate the non-common-path wave-front difference effect on PSF subtraction performance. Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT), which is operated by the National Research Council of Canada, the Institut National des Science de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  20. Discovery of a strong magnetic field in the rapidly rotating B2Vn star HR 7355

    NASA Astrophysics Data System (ADS)

    Oksala, M. E.; Wade, G. A.; Marcolino, W. L. F.; Grunhut, J.; Bohlender, D.; Manset, N.; Townsend, R. H. D.; Mimes Collaboration

    2010-06-01

    We report the detection of a strong, organized magnetic field in the He-variable early B-type star HR 7355 using spectropolarimetric data obtained with ESPaDOnS on the 3.6-m Canada-France-Hawaii Telescope within the context of the Magnetism in Massive Stars (MiMeS) Large Program. HR 7355 is both the most rapidly rotating known main-sequence magnetic star and the most rapidly rotating He-strong star, with v sin i = 300 +/- 15 km s-1 and a rotational period of 0.5214404+/-0.0000006 d. We have modelled our eight longitudinal magnetic field measurements assuming an oblique dipole magnetic field. Constraining the inclination of the rotation axis to be between 38° and 86°, we find the magnetic obliquity angle to be between 30° and 85°, and the polar strength of the magnetic field at the stellar surface to be between 13-17 kG. The photometric light curve constructed from HIPPARCOS archival data and new CTIO measurements shows two minima separated by 0.5 in rotational phase and occurring 0.25 cycles before/after the magnetic extrema. This photometric behaviour, coupled with previously reported variable emission of the Hα line (which we confirm), strongly supports the proposal that HR 7355 harbours a structured magnetosphere similar to that in the prototypical He-strong star, σ Ori E. Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France and the University of Hawaii.

  1. Measuring the surface magnetic fields of magnetic stars with unresolved Zeeman splitting

    NASA Astrophysics Data System (ADS)

    Bailey, J. D.

    2014-08-01

    Aims: High-dispersion, archival spectra of magnetic Ap stars with resolved Zeeman components in Stokes I are used to derive a simple relation that can be utilised to estimate the mean surface field strengths of stars with v sin i ≳ 10 km s-1. Methods: For each star, the mean surface field, as measured from the observed splitting in Fe ii at 6149 Å, is compared to the differential broadening of spectral lines with large and small Landé factors in order to produce a relation to estimate the field strengths of magnetic stars with unresolved Zeeman patterns. Results: The method is shown to be reliable for rotational velocities up to about 50 km s-1 for field strengths down to about 5 kG. Conclusions: These results should allow for better constraints to be placed on the mean surface magnetic fields of Ap stars where Zeeman patterns are unresolved. Based on observations made with the European Southern Observatory telescopes under ESO programmes 60.A-9036(A), 68.D-0254(A), 69.D-0378(A), 074.D-0392(A), 075.C-0234(A), 075.C-0234(B), 076.C-0073(A), 076.D-0169(A), 077.D-0477(A), 079.D-0118(A), 079.C-0170(A), 079.C-0170(B), 080.C-0032(A), 080.C-0032(B), 081.C-0034(A), 081.C-0034(B), 082.C-0218(A), 082.C-0308(A), 089.C-0207(A), 089.D-0383(A), 266.D-5655(A), obtained from the ESO/ST-ECF Science Archive Facility. Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Science de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. Based in part on observations available on the ELODIE archive.

  2. The end of the white dwarf cooling sequence in M 67

    NASA Astrophysics Data System (ADS)

    Bellini, A.; Bedin, L. R.; Piotto, G.; Salaris, M.; Anderson, J.; Brocato, E.; Ragazzoni, R.; Ortolani, S.; Bonanos, A. Z.; Platais, I.; Gilliland, R.; Raimondo, G.; Bragaglia, A.; Tosi, M.; Gallozzi, S.; Testa, V.; Kochanek, C. S.; Giallongo, E.; Baruffolo, A.; Farinato, J.; Diolaiti, E.; Speziali, R.; Carraro, G.; Yadav, R. K. S.

    2010-04-01

    In this paper, we present for the first time a proper-motion-selected white dwarf (WD) sample of the old Galactic open cluster M 67, down to the bottom of the WD cooling sequence (CS). The color-magnitude diagram is based on data collected with the LBC-Blue camera at the prime-focus of LBT. As first epoch data, we used CFHT-archive images collected 10 years before LBC data. We measured proper motions of all the identified sources. Proper motions are then used to separate foreground and background objects from the cluster stars, including WDs. Finally, the field-object cleaned WD CS in the V vs. B-I color-magnitude diagram is compared with the models. We confirm that the age derived from the location of the bottom of the WD CS is consistent with the turn off age. Based on data acquired using the Large Binocular Telescope (LBT) at Mt. Graham, Arizona, under the Commissioning of the Large Binocular Blue Camera. The LBT is an international collaboration among institutions in the United States, Italy and Germany. LBT Corporation partners are: The University of Arizona on behalf of the Arizona university system; Istituto Nazionale di Astrofisica, Italy; LBT Beteiligungsgesellschaft, Germany, representing the Max-Planck Society, the Astrophysical Institute Potsdam, and Heidelberg University; The Ohio State University, and The Research Corporation, on behalf of The University of Notre Dame, University of Minnesota and University of Virginia; and on observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.Visiting PhD Student at STScI under the “2008 graduate research assistantship” program.

  3. A Multi-wavelength Mass Analysis of RCS2 J232727.6-020437, A ˜3 × 1015 M⊙ Galaxy Cluster at z = 0.7

    NASA Astrophysics Data System (ADS)

    Sharon, K.; Gladders, M. D.; Marrone, D. P.; Hoekstra, H.; Rasia, E.; Bourdin, H.; Gifford, D.; Hicks, A. K.; Greer, C.; Mroczkowski, T.; Barrientos, L. F.; Bayliss, M.; Carlstrom, J. E.; Gilbank, D. G.; Gralla, M.; Hlavacek-Larrondo, J.; Leitch, E.; Mazzotta, P.; Miller, C.; Muchovej, S. J. C.; Schrabback, T.; Yee, H. K. C.; RCS-Team

    2015-11-01

    We present an initial study of the mass and evolutionary state of a massive and distant cluster, RCS2 J232727.6-020437. This cluster, at z = 0.6986, is the richest cluster discovered in the RCS2 project. The mass measurements presented in this paper are derived from all possible mass proxies: X-ray measurements, weak-lensing shear, strong lensing, Sunyaev-Zel’dovich effect decrement, the velocity distribution of cluster member galaxies, and galaxy richness. While each of these observables probe the mass of the cluster at a different radius, they all indicate that RCS2 J232727.6-020437 is among the most massive clusters at this redshift, with an estimated mass of {M}200˜ 3× {10}15{h}70-1 {M}⊙ . In this paper, we demonstrate that the various observables are all reasonably consistent with each other to within their uncertainties. RCS2 J232727.6-020437 appears to be well relaxed—with circular and concentric X-ray isophotes, with a cool core, and no indication of significant substructure in extensive galaxy velocity data. Based on observations obtained with : MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Science de l’Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii; the NASA/ESA Hubble Space Telescope (HST), obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-2655; the 6.5 m Magellan telescopes located at Las Campanas Observatory, Chile;

  4. The Globular Cluster System of M60 (NGC 4649). I. Canada-France-Hawaii Telescope MOS Spectroscopy and Database

    NASA Astrophysics Data System (ADS)

    Lee, Myung Gyoon; Hwang, Ho Seong; Park, Hong Soo; Park, Jang-Hyun; Kim, Sang Chul; Sohn, Young-Jong; Lee, Sang-Gak; Rey, Soo-Chang; Lee, Young-Wook; Kim, Ho-Il

    2008-02-01

    We present radial velocity measurements for globular clusters in M60, a giant elliptical galaxy in the Virgo Cluster. Target globular cluster candidates were selected using Washington photometry based on deep 16' × 16' images taken at the KPNO 4 m telescope and using VI photometry derived from Hubble Space Telescope WFPC2 archival images. The spectra of the target objects were obtained with the Multi-Object Spectrograph at the Canada-France-Hawaii Telescope. We have measured the radial velocities of 111 objects in the field of M60: 93 globular clusters (72 blue globular clusters with 1.0 <= C-T1 < 1.7, and 21 red globular clusters with 1.7 <= C-T1 < 2.4), 11 foreground stars, six small galaxies, and the nucleus of M60. The measured velocities of the 93 globular clusters range from ~500 to ~1600 km s-1, with a mean value of 1070+ 27-25 km s-1, which is in good agreement with the velocity of the nucleus of M60 (vgal = 1056 km s-1). Combining our results with data from the literature, we present a master catalog of radial velocities for 121 globular clusters in M60. The velocity dispersion of the clusters in the master catalog is found to be 234+ 13-14 km s-1 for the entire sample, 223+ 13-16 km s-1 for 83 blue globular clusters, and 258+ 21-31 km s-1 for 38 red globular clusters. Based on observations obtained at the Canada-France-Hawaii Telescope, which is operated by the National Research Council of Canada, the Institut National des Science de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. This work was organized by the Korea Astronomy and Space Science Institute.

  5. Testing the chemical tagging technique with open clusters

    NASA Astrophysics Data System (ADS)

    Blanco-Cuaresma, S.; Soubiran, C.; Heiter, U.; Asplund, M.; Carraro, G.; Costado, M. T.; Feltzing, S.; González-Hernández, J. I.; Jiménez-Esteban, F.; Korn, A. J.; Marino, A. F.; Montes, D.; San Roman, I.; Tabernero, H. M.; Tautvaišienė, G.

    2015-05-01

    Context. Stars are born together from giant molecular clouds and, if we assume that the priors were chemically homogeneous and well-mixed, we expect them to share the same chemical composition. Most of the stellar aggregates are disrupted while orbiting the Galaxy and most of the dynamic information is lost, thus the only possibility of reconstructing the stellar formation history is to analyze the chemical abundances that we observe today. Aims: The chemical tagging technique aims to recover disrupted stellar clusters based merely on their chemical composition. We evaluate the viability of this technique to recover co-natal stars that are no longer gravitationally bound. Methods: Open clusters are co-natal aggregates that have managed to survive together. We compiled stellar spectra from 31 old and intermediate-age open clusters, homogeneously derived atmospheric parameters, and 17 abundance species, and applied machine learning algorithms to group the stars based on their chemical composition. This approach allows us to evaluate the viability and efficiency of the chemical tagging technique. Results: We found that stars at different evolutionary stages have distinct chemical patterns that may be due to NLTE effects, atomic diffusion, mixing, and biases. When separating stars into dwarfs and giants, we observed that a few open clusters show distinct chemical signatures while the majority show a high degree of overlap. This limits the recovery of co-natal aggregates by applying the chemical tagging technique. Nevertheless, there is room for improvement if more elements are included and models are improved. Based on observations obtained at the Telescope Bernard Lyot (USR5026) operated by the Observatoire Midi-Pyrénées, Université de Toulouse (Paul Sabatier), Centre National de la Recherche Scientifique of France, and on public data obtained from the ESO Science Archive Facility under requests number 81252 and 81618.

  6. Near-Infrared Thermal Emission from the Hot Jupiter TrES-2b: Ground-based Detection of the Secondary Eclipse

    NASA Astrophysics Data System (ADS)

    Croll, Bryce; Albert, Loic; Lafreniere, David; Jayawardhana, Ray; Fortney, Jonathan J.

    2010-07-01

    We present near-infrared Ks-band photometry bracketing the secondary eclipse of the hot Jupiter TrES-2b using the Wide-field Infrared Camera on the Canada-France-Hawaii Telescope. We detect its thermal emission with an eclipse depth of 0.062+0.013 -0.011% (5σ). Our best-fit secondary eclipse is consistent with a circular orbit (a 3σ upper limit on the eccentricity, e, and argument or periastron, ω, of |e cos ω| < 0.0090), in agreement with mid-infrared detections of the secondary eclipse of this planet. A secondary eclipse of this depth corresponds to a dayside Ks-band brightness temperature of TB = 1636+79 -88 K. Our thermal emission measurement, when combined with the thermal emission measurements using Spitzer/IRAC from O'Donovan and collaborators, suggests that this planet exhibits relatively efficient dayside to nightside redistribution of heat and a near isothermal dayside atmospheric temperature structure, whose spectrum is well approximated by a blackbody. It is unclear if the atmosphere of TrES-2b requires a temperature inversion; if it does it is likely due to chemical species other than TiO/VO as the atmosphere of TrES-2b is too cool to allow TiO/VO to remain in gaseous form. Our secondary eclipse has the smallest depth of any detected from the ground, at around 2 μm, to date. Based on observations obtained with WIRCam, a joint project of Canada-France-Hawaii Telescope (CFHT), Taiwan, Korea, Canada, France, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institute National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  7. Art & Astronomie - impressions celestes

    NASA Astrophysics Data System (ADS)

    Nazé, Yaël

    2015-10-01

    Ce livre revisite l'histoire de l'art dans ce qu'elle a de plus universel : son rapport au ciel. De l'Orient à l'Occident, de l'Antiquité à l'époque contemporaine, du classique au plus inattendu, il crée un espace singulier où se mêlent art et science, un musée imaginaire croisant sensibilité intime et compréhension du Cosmos, un jeu sans cesse réinventé...; car il n'y a pas une seule manière de regarder les étoiles. Bien sûr, le ciel possède un énorme pouvoir évocateur, une force inspiratrice à nulle autre pareille, mais l'inspiration n'est pas la seule des relations entre l'art et l'astronomie. En effet, les artistes peuvent apporter leur grain de sel aux révolutions scientifiques, tandis que l'astronomie peut aider à comprendre certaines œuvres. Avec près de 600 illustrations, cet ouvrage n'a pas pour but d'égrener la liste exhaustive des représentations de ciel étoilé, clair de lune, ambiance crépusculaire ou soleil de midi, mais plutôt d'aborder les multiples relations entre l'art et la science. Il s'agit d'une invitation à un voyage aux frontières mouvantes et incertaines des plus belles réalisations de l'esprit humain.

  8. Calibration, Sensor Model Improvements and Uncertainty Budget of the Airborne Imaging Spectrometer APEX

    NASA Astrophysics Data System (ADS)

    Hueni, A.

    2015-12-01

    ESA's Airborne Imaging Spectrometer APEX (Airborne Prism Experiment) was developed under the PRODEX (PROgramme de Développement d'EXpériences scientifiques) program by a Swiss-Belgian consortium and entered its operational phase at the end of 2010 (Schaepman et al., 2015). Work on the sensor model has been carried out extensively within the framework of European Metrology Research Program as part of the Metrology for Earth Observation and Climate (MetEOC and MetEOC2). The focus has been to improve laboratory calibration procedures in order to reduce uncertainties, to establish a laboratory uncertainty budget and to upgrade the sensor model to compensate for sensor specific biases. The updated sensor model relies largely on data collected during dedicated characterisation experiments in the APEX calibration home base but includes airborne data as well where the simulation of environmental conditions in the given laboratory setup was not feasible. The additions to the model deal with artefacts caused by environmental changes and electronic features, namely the impact of ambient air pressure changes on the radiometry in combination with dichroic coatings, influences of external air temperatures and consequently instrument baffle temperatures on the radiometry, and electronic anomalies causing radiometric errors in the four shortwave infrared detector readout blocks. Many of these resolved issues might be expected to be present in other imaging spectrometers to some degree or in some variation. Consequently, the work clearly shows the difficulties of extending a laboratory-based uncertainty to data collected under in-flight conditions. The results are hence not only of interest to the calibration scientist but also to the spectroscopy end user, in particular when commercial sensor systems are used for data collection and relevant sensor characteristic information tends to be sparse. Schaepman, et al, 2015. Advanced radiometry measurements and Earth science

  9. Submillimeter Galaxies at z ~ 2: Evidence for Major Mergers and Constraints on Lifetimes, IMF, and CO-H2 Conversion Factor

    NASA Astrophysics Data System (ADS)

    Tacconi, L. J.; Genzel, R.; Smail, I.; Neri, R.; Chapman, S. C.; Ivison, R. J.; Blain, A.; Cox, P.; Omont, A.; Bertoldi, F.; Greve, T.; Förster Schreiber, N. M.; Genel, S.; Lutz, D.; Swinbank, A. M.; Shapley, A. E.; Erb, D. K.; Cimatti, A.; Daddi, E.; Baker, A. J.

    2008-06-01

    We report subarcsecond resolution IRAM PdBI millimeter CO interferometry of four z ~ 2 submillimeter galaxies (SMGs), and sensitive CO(3-2) flux limits toward three z ~ 2 UV/optically selected star-forming galaxies. The new data reveal for the first time spatially resolved CO gas kinematics in the observed SMGs. Two of the SMGs show double or multiple morphologies, with complex, disturbed gas motions. The other two SMGs exhibit CO velocity gradients of ~500 km s-1 across <=0.2'' (1.6 kpc) diameter regions, suggesting that the star-forming gas is in compact, rotating disks. Our data provide compelling evidence that these SMGs represent extreme, short-lived "maximum" star-forming events in highly dissipative mergers of gas-rich galaxies. The resulting high-mass surface and volume densities of SMGs are similar to those of compact quiescent galaxies in the same redshift range and much higher than those in local spheroids. From the ratio of the comoving volume densities of SMGs and quiescent galaxies in the same mass and redshift ranges, and from the comparison of gas exhaustion timescales and stellar ages, we estimate that the SMG phase duration is about 100 Myr. Our analysis of SMGs and optically/UV selected high-redshift star-forming galaxies supports a "universal" Chabrier IMF as being valid over the star-forming history of these galaxies. We find that the 12CO luminosity to total gas mass conversion factors at z ~ 2-3 are probably similar to those assumed at z ~ 0. The implied gas fractions in our sample galaxies range from 20% to 50%. Based on observations obtained at the IRAM Plateau de Bure Interferometer (PdBI). IRAM is funded by the Centre National de la Recherché Scientifique (France), the Max-Planck Gesellschaft (Germany), and the Instituto Geografico Nacional (Spain).

  10. Gas Phase Absorption Spectroscopy of C+60 and C+70 in a Cryogenic Ion Trap: Comparison with Astronomical Measurements

    NASA Astrophysics Data System (ADS)

    Campbell, E. K.; Holz, M.; Maier, J. P.; Gerlich, D.; Walker, G. A. H.; Bohlender, D.

    2016-05-01

    Recent low-temperature laboratory measurements and astronomical observations have proved that the fullerene cation {{{C}}}60+ is responsible for four diffuse interstellar bands (DIBs). These absorptions correspond to the strongest bands of the lowest electronic transition. The gas phase spectrum below 10 {{K}} is reported here for the full wavelength range encompassed by the electronic transition. The absorption spectrum of {{{C}}}70+, with its origin band at 7959.2 {{\\mathringA }}, has been obtained under similar laboratory conditions. Observations made toward the reddened star {HD} 183143 were used in a specific search for the absorption of these fullerene cations in diffuse clouds. In the case of {{{C}}}60+, one further band in the astronomical spectrum at 9348.5 \\mathringA is identified, increasing the total number of assigned DIBs to five. Numerous other {{{C}}}60+ absorptions in the laboratory spectrum are found to lie below the astronomical detection limit. Special emphasis is placed on the laboratory determination of absolute absorption cross-sections. For {{{C}}}60+ this directly yields a column density, N({{{C}}}60+), of 2× {10}13 {{{cm}}}-2 in diffuse clouds, without the need to rely on theoretical oscillator strengths. The intensity of the {{{C}}}70+ electronic transition in the range 7000–8000 Å is spread over many features of similar strength. Absorption cross-section measurements indicate that even for a similar column density, the individual absorption bands of {{{C}}}70+ will be too weak to be detected in the astronomical spectra, which is confirmed giving an upper limit of 2 {{m\\mathringA }} to the equivalent width. Based on observations obtained at the Canada‑France‑Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l’Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  11. PHENIX Collaboration

    NASA Astrophysics Data System (ADS)

    Adare, A.; Afanasiev, S.; Aidala, C.; Ajitanand, N. N.; Akiba, Y.; Akimoto, R.; Al-Bataineh, H.; Al-Ta'ani, H.; Alexander, J.; Alfred, M.; Andrews, K. R.; Angerami, A.; Aoki, K.; Apadula, N.; Aphecetche, L.; Appelt, E.; Aramaki, Y.; Armendariz, R.; Aronson, S. H.; Asai, J.; Asano, H.; Aschenauer, E. C.; Atomssa, E. T.; Averbeck, R.; Awes, T. C.; Azmoun, B.; Babintsev, V.; Bai, M.; Bai, X.; Baksay, G.; Baksay, L.; Baldisseri, A.; Bandara, N. S.; Bannier, B.; Barish, K. N.; Barnes, P. D.; Bassalleck, B.; Basye, A. T.; Bathe, S.; Batsouli, S.; Baublis, V.; Baumann, C.; Baumgart, S.; Bazilevsky, A.; Beaumier, M.; Beckman, S.; Belikov, S.; Belmont, R.; Ben-Benjamin, J.; Bennett, R.; Berdnikov, A.; Berdnikov, Y.; Bhom, J. H.; Bickley, A. A.; Bing, X.; Black, D.; Blau, D. S.; Boissevain, J. G.; Bok, J. S.; Borel, H.; Boyle, K.; Brooks, M. L.; Broxmeyer, D.; Bryslawskyj, J.; Buesching, H.; Bumazhnov, V.; Bunce, G.; Butsyk, S.; Camacho, C. M.; Campbell, S.; Caringi, A.; Castera, P.; Chang, B. S.; Chang, W. C.; Charvet, J.-L.; Chen, C.-H.; Chernichenko, S.; Chi, C. Y.; Chiba, J.; Chiu, M.; Choi, I. J.; Choi, J. B.; Choi, S.; Choudhury, R. K.; Christiansen, P.; Chujo, T.; Chung, P.; Churyn, A.; Chvala, O.; Cianciolo, V.; Citron, Z.; Cleven, C. R.; Cole, B. A.; Comets, M. P.; Conesa del Valle, Z.; Connors, M.; Constantin, P.; Cronin, N.; Crossette, N.; Csanád, M.; Csörgő, T.; Dahms, T.; Dairaku, S.; Danchev, I.; Das, K.; Datta, A.; Daugherity, M. S.; David, G.; Dayananda, M. K.; Deaton, M. B.; DeBlasio, K.; Dehmelt, K.; Delagrange, H.; Denisov, A.; d'Enterria, D.; Deshpande, A.; Desmond, E. J.; Dharmawardane, K. V.; Dietzsch, O.; Ding, L.; Dion, A.; Do, J. H.; Donadelli, M.; Drapier, O.; Drees, A.; Drees, K. A.; Dubey, A. K.; Durham, J. M.; Durum, A.; Dutta, D.; Dzhordzhadze, V.; D'Orazio, L.; Edwards, S.; Efremenko, Y. V.; Egdemir, J.; Ellinghaus, F.; Emam, W. S.; Engelmore, T.; Enokizono, A.; En'yo, H.; Esumi, S.; Eyser, K. O.; Fadem, B.; Feege, N.; Fields, D. E.; Finger, M.; Finger, M.; Fleuret, F.; Fokin, S. L.; Fraenkel, Z.; Frantz, J. E.; Franz, A.; Frawley, A. D.; Fujiwara, K.; Fukao, Y.; Fusayasu, T.; Gadrat, S.; Gainey, K.; Gal, C.; Gallus, P.; Garg, P.; Garishvili, A.; Garishvili, I.; Ge, H.; Giordano, F.; Glenn, A.; Gong, H.; Gong, X.; Gonin, M.; Gosset, J.; Goto, Y.; Granier de Cassagnac, R.; Grau, N.; Greene, S. V.; Grim, G.; Grosse Perdekamp, M.; Gu, Y.; Gunji, T.; Guo, L.; Guragain, H.; Gustafsson, H.-Å.; Hachiya, T.; Hadj Henni, A.; Haegemann, C.; Haggerty, J. S.; Hahn, K. I.; Hamagaki, H.; Hamblen, J.; Han, R.; Han, S. Y.; Hanks, J.; Harada, H.; Harper, C.; Hartouni, E. P.; Haruna, K.; Hasegawa, S.; Hashimoto, K.; Haslum, E.; Hayano, R.; Hayashi, S.; He, X.; Heffner, M.; Hemmick, T. K.; Hester, T.; Hiejima, H.; Hill, J. C.; Hobbs, R.; Hohlmann, M.; Hollis, R. S.; Holzmann, W.; Homma, K.; Hong, B.; Horaguchi, T.; Hori, Y.; Hornback, D.; Hoshino, T.; Huang, J.; Huang, S.; Ichihara, T.; Ichimiya, R.; Ide, J.; Iinuma, H.; Ikeda, Y.; Imai, K.; Imazu, Y.; Imrek, J.; Inaba, M.; Inoue, Y.; Iordanova, A.; Isenhower, D.; Isenhower, L.; Ishihara, M.; Isinhue, A.; Isobe, T.; Issah, M.; Isupov, A.; Ivanischev, D.; Ivanishchev, D.; Iwanaga, Y.; Jacak, B. V.; Javani, M.; Jeon, S. J.; Jezghani, M.; Jia, J.; Jiang, X.; Jin, J.; Jinnouchi, O.; John, D.; Johnson, B. M.; Jones, T.; Joo, E.; Joo, K. S.; Jouan, D.; Jumper, D. S.; Kajihara, F.; Kametani, S.; Kamihara, N.; Kamin, J.; Kanda, S.; Kaneta, M.; Kaneti, S.; Kang, B. H.; Kang, J. H.; Kang, J. S.; Kanou, H.; Kapustinsky, J.; Karatsu, K.; Kasai, M.; Kawall, D.; Kawashima, M.; Kazantsev, A. V.; Kempel, T.; Key, J. A.; Khachatryan, V.; Khandai, P. K.; Khanzadeev, A.; Kihara, K.; Kijima, K. M.; Kikuchi, J.; Kim, A.; Kim, B. I.; Kim, C.; Kim, D. H.; Kim, D. J.; Kim, E.; Kim, E.-J.; Kim, H.-J.; Kim, H. J.; Kim, K.-B.; Kim, M.; Kim, S. H.; Kim, Y.-J.; Kim, Y. K.; Kinney, E.; Kiriluk, K.; Kiss, Á.; Kistenev, E.; Kiyomichi, A.; Klatsky, J.; Klay, J.; Klein-Boesing, C.; Kleinjan, D.; Kline, P.; Koblesky, T.; Kochenda, L.; Kochetkov, V.; Kofarago, M.; Komatsu, Y.; Komkov, B.; Konno, M.; Koster, J.; Kotchetkov, D.; Kotov, D.; Kozlov, A.; Král, A.; Kravitz, A.; Krizek, F.; Kubart, J.; Kunde, G. J.; Kurihara, N.; Kurita, K.; Kurosawa, M.; Kweon, M. J.; Kwon, Y.; Kyle, G. S.; Lacey, R.; Lai, Y. S.; Lajoie, J. G.; Layton, D.; Lebedev, A.; Lee, B.; Lee, D. M.; Lee, G. H.; Lee, J.; Lee, K.; Lee, K. B.; Lee, K. S.; Lee, M. K.; Lee, S. H.; Lee, S. R.; Lee, T.; Leitch, M. J.; Leite, M. A. L.; Leitgab, M.; Leitner, E.; Lenzi, B.; Lewis, B.; Li, X.; Lichtenwalner, P.; Liebing, P.; Lim, S. H.; Linden Levy, L. A.; Liška, T.; Litvinenko, A.; Liu, H.; Liu, M. X.; Love, B.; Luechtenborg, R.; Lynch, D.; Maguire, C. F.; Makdisi, Y. I.; Ma, M.; Malakhov, A.; Malik, M. D.; Manion, A.; Manko, V. I.; Mannel, E.; Mao, Y.

    2014-12-01

    We thank the staff of the Collider-Accelerator and Physics Departments at Brookhaven National Laboratory and the staff of the other PHENIX participating institutions for their vital contributions. We acknowledge support from the Office of Nuclear Physics in the Office of Science of the Department of Energy, the National Science Foundation, a sponsored research grant from Renaissance Technologies LLC, Abilene Christian University Research Council, Research Foundation of SUNY, and Dean of the College of Arts and Sciences, Vanderbilt University (USA), Ministry of Education, Culture, Sports, Science, and Technology and the Japan Society for the Promotion of Science (Japan), Conselho Nacional de Desenvolvimento Científico e Tecnológico and Fundação de Amparo à Pesquisa do Estado de São Paulo (Brazil), Natural Science Foundation of China, (People's Republic of China), Ministry of Science, Education, and Sports (Croatia), Ministry of Education, Youth and Sports (Czech Republic), Centre National de la Recherche Scientifique, Commissariat à l'Énergie Atomique, and Institut National de Physique Nucléaire et de Physique des Particules (France), Bundesministerium für Bildung und Forschung, Deutscher Akademischer Austausch Dienst, and Alexander von Humboldt Stiftung (Germany), OTKA NK 101 428 grant and the Ch. Simonyi Fund (Hungary), Department of Atomic Energy and Department of Science and Technology (India), Israel Science Foundation (Israel), National Research Foundation and WCU program of the Ministry Education Science and Technology (Republic of Korea), Physics Department, Lahore University of Management Sciences (Pakistan), Ministry of Education and Science, Russian Academy of Sciences, Federal Agency of Atomic Energy (Russia), VR and Wallenberg Foundation (Sweden), the US Civilian Research and Development Foundation for the Independent States of the Former Soviet Union, and the US-Israel Binational Science Foundation.

  12. PHENIX Collaboration

    NASA Astrophysics Data System (ADS)

    Adare, A.; Afanasiev, S.; Aidala, C.; Ajitanand, N. N.; Akiba, Y.; Akimoto, R.; Al-Bataineh, H.; Al-Ta'ani, H.; Alexander, J.; Alfred, M.; Andrews, K. R.; Angerami, A.; Aoki, K.; Apadula, N.; Aphecetche, L.; Appelt, E.; Aramaki, Y.; Armendariz, R.; Aronson, S. H.; Asai, J.; Asano, H.; Aschenauer, E. C.; Atomssa, E. T.; Averbeck, R.; Awes, T. C.; Azmoun, B.; Babintsev, V.; Bai, M.; Bai, X.; Baksay, G.; Baksay, L.; Baldisseri, A.; Bandara, N. S.; Bannier, B.; Barish, K. N.; Barnes, P. D.; Barnes, P. D.; Bassalleck, B.; Basye, A. T.; Bathe, S.; Batsouli, S.; Baublis, V.; Baumann, C.; Baumgart, S.; Bazilevsky, A.; Beaumier, M.; Beckman, S.; Belikov, S.; Belmont, R.; Ben-Benjamin, J.; Bennett, R.; Berdnikov, A.; Berdnikov, Y.; Bhom, J. H.; Bickley, A. A.; Bing, X.; Black, D.; Blau, D. S.; Boissevain, J. G.; Bok, J.; Bok, J. S.; Borel, H.; Boyle, K.; Brooks, M. L.; Broxmeyer, D.; Bryslawskyj, J.; Buesching, H.; Bumazhnov, V.; Bunce, G.; Butsyk, S.; Camacho, C. M.; Campbell, S.; Caringi, A.; Castera, P.; Chang, B. S.; Chang, W. C.; Charvet, J.-L.; Chen, C.-H.; Chernichenko, S.; Chi, C. Y.; Chiba, J.; Chiu, M.; Choi, I. J.; Choi, J. B.; Choi, S.; Choudhury, R. K.; Christiansen, P.; Chujo, T.; Chung, P.; Churyn, A.; Chvala, O.; Cianciolo, V.; Citron, Z.; Cleven, C. R.; Cole, B. A.; Comets, M. P.; Conesa del Valle, Z.; Connors, M.; Constantin, P.; Cronin, N.; Crossette, N.; Csanád, M.; Csörgő, T.; Dahms, T.; Dairaku, S.; Danchev, I.; Das, K.; Datta, A.; Daugherity, M. S.; David, G.; Dayananda, M. K.; Deaton, M. B.; DeBlasio, K.; Dehmelt, K.; Delagrange, H.; Denisov, A.; d'Enterria, D.; Deshpande, A.; Desmond, E. J.; Dharmawardane, K. V.; Dietzsch, O.; Ding, L.; Dion, A.; Do, J. H.; Donadelli, M.; Drapier, O.; Drees, A.; Drees, K. A.; Dubey, A. K.; Durham, J. M.; Durum, A.; Dutta, D.; Dzhordzhadze, V.; D'Orazio, L.; Edwards, S.; Efremenko, Y. V.; Egdemir, J.; Ellinghaus, F.; Emam, W. S.; Engelmore, T.; Enokizono, A.; En'yo, H.; Esumi, S.; Eyser, K. O.; Fadem, B.; Feege, N.; Fields, D. E.; Finger, M.; Finger, M.; Fleuret, F.; Fokin, S. L.; Fraenkel, Z.; Frantz, J. E.; Franz, A.; Frawley, A. D.; Fujiwara, K.; Fukao, Y.; Fusayasu, T.; Gadrat, S.; Gainey, K.; Gal, C.; Gallus, P.; Garg, P.; Garishvili, A.; Garishvili, I.; Ge, H.; Giordano, F.; Glenn, A.; Gong, H.; Gong, X.; Gonin, M.; Gosset, J.; Goto, Y.; Granier de Cassagnac, R.; Grau, N.; Greene, S. V.; Grim, G.; Grosse Perdekamp, M.; Gu, Y.; Gunji, T.; Guo, L.; Guragain, H.; Gustafsson, H.-Å.; Hachiya, T.; Hadj Henni, A.; Haegemann, C.; Haggerty, J. S.; Hahn, K. I.; Hamagaki, H.; Hamblen, J.; Han, R.; Han, S. Y.; Hanks, J.; Harada, H.; Harper, C.; Hartouni, E. P.; Haruna, K.; Hasegawa, S.; Hashimoto, K.; Haslum, E.; Hayano, R.; Hayashi, S.; He, X.; Heffner, M.; Hemmick, T. K.; Hester, T.; Hiejima, H.; Hill, J. C.; Hobbs, R.; Hohlmann, M.; Hollis, R. S.; Holzmann, W.; Homma, K.; Hong, B.; Horaguchi, T.; Hori, Y.; Hornback, D.; Hoshino, T.; Huang, J.; Huang, S.; Ichihara, T.; Ichimiya, R.; Ide, J.; Iinuma, H.; Ikeda, Y.; Imai, K.; Imazu, Y.; Imrek, J.; Inaba, M.; Inoue, Y.; Iordanova, A.; Isenhower, D.; Isenhower, L.; Ishihara, M.; Isinhue, A.; Isobe, T.; Issah, M.; Isupov, A.; Ivanischev, D.; Ivanishchev, D.; Iwanaga, Y.; Jacak, B. V.; Javani, M.; Jeon, S. J.; Jezghani, M.; Jia, J.; Jiang, X.; Jin, J.; Jinnouchi, O.; John, D.; Johnson, B. M.; Jones, T.; Joo, E.; Joo, K. S.; Jouan, D.; Jumper, D. S.; Kajihara, F.; Kametani, S.; Kamihara, N.; Kamin, J.; Kanda, S.; Kaneta, M.; Kaneti, S.; Kang, B. H.; Kang, J. H.; Kang, J. S.; Kanou, H.; Kapustinsky, J.; Karatsu, K.; Kasai, M.; Kawall, D.; Kawashima, M.; Kazantsev, A. V.; Kempel, T.; Key, J. A.; Khachatryan, V.; Khandai, P. K.; Khanzadeev, A.; Kihara, K.; Kijima, K. M.; Kikuchi, J.; Kim, A.; Kim, B. I.; Kim, C.; Kim, D. H.; Kim, D. J.; Kim, E.; Kim, E.-J.; Kim, H.-J.; Kim, H. J.; Kim, K.-B.; Kim, M.; Kim, S. H.; Kim, Y.-J.; Kim, Y. K.; Kinney, E.; Kiriluk, K.; Kiss, Á.; Kistenev, E.; Kiyomichi, A.; Klatsky, J.; Klay, J.; Klein-Boesing, C.; Kleinjan, D.; Kline, P.; Koblesky, T.; Kochenda, L.; Kochetkov, V.; Kofarago, M.; Komatsu, Y.; Komkov, B.; Konno, M.; Koster, J.; Kotchetkov, D.; Kotov, D.; Kozlov, A.; Král, A.; Kravitz, A.; Krizek, F.; Kubart, J.; Kunde, G. J.; Kurihara, N.; Kurita, K.; Kurosawa, M.; Kweon, M. J.; Kwon, Y.; Kyle, G. S.; Lacey, R.; Lai, Y. S.; Lajoie, J. G.; Layton, D.; Lebedev, A.; Lee, B.; Lee, D. M.; Lee, G. H.; Lee, J.; Lee, K.; Lee, K. B.; Lee, K. S.; Lee, M. K.; Lee, S. H.; Lee, S. R.; Lee, T.; Leitch, M. J.; Leite, M. A. L.; Leitgab, M.; Leitner, E.; Lenzi, B.; Lewis, B.; Li, X.; Lichtenwalner, P.; Liebing, P.; Lim, S. H.; Linden Levy, L. A.; Liška, T.; Litvinenko, A.; Liu, H.; Liu, M. X.; Love, B.; Luechtenborg, R.; Lynch, D.; Maguire, C. F.; Makdisi, Y. I.; Maai, M.; Malakhov, A.; Malik, M. D.; Manion, A.; Manko, V. I.

    2014-11-01

    We thank the staff of the Collider-Accelerator and Physics Departments at Brookhaven National Laboratory and the staff of the other PHENIX participating institutions for their vital contributions. We acknowledge support from the Office of Nuclear Physics in the Office of Science of the Department of Energy, the National Science Foundation, a sponsored research grant from Renaissance Technologies LLC, Abilene Christian University Research Council, Research Foundation of SUNY, and Dean of the College of Arts and Sciences, Vanderbilt University (USA), Ministry of Education, Culture, Sports, Science, and Technology and the Japan Society for the Promotion of Science (Japan), Conselho Nacional de Desenvolvimento Científico e Tecnológico and Fundaç ao de Amparo à Pesquisa do Estado de São Paulo (Brazil), Natural Science Foundation of China (People's Republic of China), Ministry of Science, Education, and Sports (Croatia), Ministry of Education, Youth and Sports (Czech Republic), Centre National de la Recherche Scientifique, Commissariat à l'Énergie Atomique, and Institut National de Physique Nucléaire et de Physique des Particules (France), Bundesministerium für Bildung und Forschung, Deutscher Akademischer Austausch Dienst, and Alexander von Humboldt Stiftung (Germany), OTKA NK 101 428 grant and the Ch. Simonyi Fund (Hungary), Department of Atomic Energy and Department of Science and Technology (India), Israel Science Foundation (Israel), National Research Foundation and WCU program of the Ministry Education Science and Technology (Korea), Physics Department, Lahore University of Management Sciences (Pakistan), Ministry of Education and Science, Russian Academy of Sciences, Federal Agency of Atomic Energy (Russia), VR and Wallenberg Foundation (Sweden), the US Civilian Research and Development Foundation for the Independent States of the Former Soviet Union, and the US-Israel Binational Science Foundation.

  13. Vertical abundance stratification in the blue horizontal branch star HD 135485

    NASA Astrophysics Data System (ADS)

    Khalack, V. R.; Leblanc, F.; Bohlender, D.; Wade, G. A.; Behr, B. B.

    2007-05-01

    Context: It is commonly believed that the observed overabundances of many chemical species relative to the expected cluster metallicity in blue horizontal branch (BHB) stars appear as a result of atomic diffusion in the photosphere. The slow rotation of BHB stars (with T_eff > 11 500 K), typically v sin{i} < 10 km s-1, is consistent with this idea. Aims: In this work we search for observational evidence of vertical chemical stratification in the atmosphere of HD 135485. If this evidence exists, it will demonstrate the importance of atomic diffusion processes in the atmospheres of BHB stars. Methods: We undertake an extensive abundance stratification analysis of the atmosphere of HD 135485, based on recently acquired high resolution and S/N CFHT ESPaDOnS spectra and a McDonald-CE spectrum. Results: Our numerical simulations show that nitrogen and sulfur reveal signatures of vertical abundance stratification in the stellar atmosphere. It appears that the abundances of these elements increase toward the upper atmosphere. This fact cannot be explained by the influence of microturbulent velocity, because oxygen, carbon, neon, argon, titanium and chromium do not show similar behavior and their abundances remain constant throughout the atmosphere. It seems that the iron abundance may increase marginally toward the lower atmosphere. This is the first demonstration of vertical abundance stratification of metals in a BHB star. Based on observations made with ESPaDOnS at the Canada-France-Hawaii Telescope (CFHT) operated by the National Research Council (NRC) of Canada, the Institut des Sciences de l'Univers of the Centre National de la Recherche Scientifique (CNRS) and the University of Hawaii and on observations made with Echelle Spectrograph on the McDonald Observatory 2.1-m Otto Struve Telescope. Full Table 2 is only available in electronic form at http://www.aanda.org

  14. Entrevue avec le Dr Charley Zeanah

    PubMed Central

    2013-01-01

    Le Dr Charles Zeanah est titulaire de la chaire de psychiatrie Mary K. Sellars-Polchow, professeur de pédiatrie clinique et vice-président de la pédopsychiatrie au département de psychiatrie et des sciences du comportement de la faculté de médecine de l’Université Tulane, à la Nouvelle-Orléans. Il est également directeur général de l’institut de la santé mentale des nourrissons et des jeunes enfants de Tulane. Il est récipiendaire de nombreux prix, notamment le prix de prévention Irving Phillips (AACAP), la mention élogieuse présidentielle pour sa recherche et son leadership exceptionnels en santé mentale des nourrissons (American Orthopsychiatric Association), le prix d’excellence clinique Sarah Haley Memorial (International Society for Traumatic Stress Studies), le prix de recherche en pédopsychiatrie Blanche F. Ittelson (APA), et le prix Serge Lebovici Award soulignant les contributions internationales à la santé mentale des nourrissons (World Association for Infant Mental Health). Le Dr Zeanah est fellow distingué de l’AACAP, fellow distingué de l’APA et membre du conseil d’administration de Zero to Three. Il est l’éditeur scientifique de Handbook of Infant Mental Health (3e édition) qui est considéré comme étant le manuel de pointe et la référence de base du domaine de la santé mentale des nourrissons.

  15. Data Processing from the Chandra and XMM-Newton Space Missions

    NASA Astrophysics Data System (ADS)

    Willmore, P.

    2009-10-01

    The fourth in the series of COSPAR Capacity-Building Workshops was held in Durban in 2004. The availability of large archives of data from space missions via the internet provides an important research opportunity for scientists in developing countries. The aim of the COSPAR Capacity-Building Workshop programme is to ensure that this opportunity is taken up as widely as possible. The character of the workshops and the programme for the first five years are described. Evaluation of the longer-term results of the first workshop, which was held in Brazil in 2001, show that a good proportion of past participants have used archival data and have produced publishable results from it. Some comments are made about future development of the programme. L'agence internationale COSPAR a organisé à Durban en 2004, le quatrième d'une série d'ateliers dédiés au renforcement des capacités. La disponibilité actuelle de larges bases de données en ligne offre des possibilités de recherche pour les scientifiques des pays émergents. Le but de cet atelier est de rendre cette opportunité pleinement exploitable. La spécificité ainsi que le programme pour les cinq premières années est décrit ici. L'évaluation des retombées à long terme, consécutives au premier atelier tenu au Brésil en 2001, montre qu'une large proportion de participants ont déjà utilises lesdites.

  16. Modelisations des effets de surface sur les jets horizontaux subsoniques d'hydrogene et de methane

    NASA Astrophysics Data System (ADS)

    Gomez, Luis Fernando

    Le developpement des codes et de normes bases sur une methodologie scientifique requiert la capacite de predire l'etendue inflammable de deversements gazeux d'hydrogene sous differentes conditions. Des etudes anterieures ont deja etabli des modeles bases sur les lois de conservation de la mecanique des fluides basees sur des correlations experimentales qui permettent de predire la decroissance de la concentration et de la vitesse d'un gaz le long de l'axe d'un jet libre vertical. Cette etude s'interesse aux effets de proximite a une surface horizontale parallele sur un jet turbulent. Nous nous interessons a son impact sur l'etendue du champ de la concentration et sur l'enveloppe inflammable en particulier. Cette etude est comparative : l'hydrogene est compare au methane. Ceci permet de degager l'influence des effets de difference de la densite sur le comportement du jet, et de comparer le comportement de l'hydrogene aux correlations experimentales, qui ont ete essentiellement etablies pour le methane. Un modele decrivant l'evolution spatio-temporelle du champ de concentration du gaz dilue est propose, base sur la mecanique des fluides computationnelle. Cette approche permet de varier systematiquement les conditions aux frontieres (proximite du jet a la surface, par exemple) et de connaitre en detail les proprietes de l'ecoulement. Le modele est implemente dans le code de simulations par volumes finis de FLUENT. Les resultats des simulations sont compares avec les lois de similitudes decoulant de la theorie des jets d'ecoulements turbulents libres ainsi qu'avec les resultats experimentaux disponibles. L'effet de la difference des masses molaires des constituantes du jet et des constituantes du milieu de dispersion est egalement etudie dans le contexte du comportement d'echelle de la region developpee du jet.

  17. The magnetic field of ζ Orionis A

    NASA Astrophysics Data System (ADS)

    Blazère, A.; Neiner, C.; Tkachenko, A.; Bouret, J.-C.; Rivinius, Th.

    2015-10-01

    Context. ζ Ori A is a hot star claimed to host a weak magnetic field, but no clear magnetic detection was obtained so far. In addition, it was recently shown to be a binary system composed of a O9.5I supergiant and a B1IV star. Aims: We aim at verifying the presence of a magnetic field in ζ Ori A, identifying to which of the two binary components it belongs (or whether both stars are magnetic), and characterizing the field. Methods: Very high signal-to-noise spectropolarimetric data were obtained with Narval at the Bernard Lyot Telescope (TBL) in France. Archival HEROS, FEROS and UVES spectroscopic data were also used. The data were first disentangled to separate the two components. We then analyzed them with the least-squares deconvolution technique to extract the magnetic information. Results: We confirm that ζ Ori A is magnetic. We find that the supergiant component ζ Ori Aa is the magnetic component: Zeeman signatures are observed and rotational modulation of the longitudinal magnetic field is clearly detected with a period of 6.829 d. This is the only magnetic O supergiant known as of today. With an oblique dipole field model of the Stokes V profiles, we show that the polar field strength is ~140 G. Because the magnetic field is weak and the stellar wind is strong, ζ Ori Aa does not host a centrifugally supported magnetosphere. It may host a dynamical magnetosphere. Its companion ζ Ori Ab does not show any magnetic signature, with an upper limit on the undetected field of ~300 G. Based on observations obtained at the Télescope Bernard Lyot (USR5026) operated by the Observatoire Midi-Pyrénées, Université de Toulouse (Paul Sabatier), Centre National de la Recherche Scientifique of France.Appendix A is available in electronic form at http://www.aanda.org

  18. Homogeneous spectroscopic parameters for bright planet host stars from the northern hemisphere . The impact on stellar and planetary mass

    NASA Astrophysics Data System (ADS)

    Sousa, S. G.; Santos, N. C.; Mortier, A.; Tsantaki, M.; Adibekyan, V.; Delgado Mena, E.; Israelian, G.; Rojas-Ayala, B.; Neves, V.

    2015-04-01

    Aims: In this work we derive new precise and homogeneous parameters for 37 stars with planets. For this purpose, we analyze high resolution spectra obtained by the NARVAL spectrograph for a sample composed of bright planet host stars in the northern hemisphere. The new parameters are included in the SWEET-Cat online catalogue. Methods: To ensure that the catalogue is homogeneous, we use our standard spectroscopic analysis procedure, ARES+MOOG, to derive effective temperatures, surface gravities, and metallicities. These spectroscopic stellar parameters are then used as input to compute the stellar mass and radius, which are fundamental for the derivation of the planetary mass and radius. Results: We show that the spectroscopic parameters, masses, and radii are generally in good agreement with the values available in online databases of exoplanets. There are some exceptions, especially for the evolved stars. These are analyzed in detail focusing on the effect of the stellar mass on the derived planetary mass. Conclusions: We conclude that the stellar mass estimations for giant stars should be managed with extreme caution when using them to compute the planetary masses. We report examples within this sample where the differences in planetary mass can be as high as 100% in the most extreme cases. Based on observations obtained at the Telescope Bernard Lyot (USR5026) operated by the Observatoire Midi-Pyrénées and the Institut National des Science de l'Univers of the Centre National de la Recherche Scientifique of France (Run ID L131N11 - OPTICON_2013A_027).

  19. Search for magnetic fields in particle-accelerating colliding-wind binaries

    NASA Astrophysics Data System (ADS)

    Neiner, C.; Grunhut, J.; Leroy, B.; De Becker, M.; Rauw, G.

    2015-03-01

    Context. Some colliding-wind massive binaries, called particle-accelerating colliding-wind binaries (PACWB), exhibit synchrotron radio emission, which is assumed to be generated by a stellar magnetic field. However, no measurement of magnetic fields in these stars has ever been performed. Aims: We aim at quantifying the possible stellar magnetic fields present in PACWB to provide constraints for models. Methods: We gathered 21 high-resolution spectropolarimetric observations of 9 PACWB available in the ESPaDOnS, Narval and HarpsPol archives. We analysed these observations with the least squares deconvolution method. We separated the binary spectral components when possible. Results: No magnetic signature is detected in any of the 9 PACWB stars and all longitudinal field measurements are compatible with 0 G. We derived the upper field strength of a possible field that could have remained hidden in the noise of the data. While the data are not very constraining for some stars, for several stars we could derive an upper limit of the polar field strength of the order of 200 G. Conclusions: We can therefore exclude the presence of strong or moderate stellar magnetic fields in PACWB, typical of the ones present in magnetic massive stars. Weak magnetic fields could however be present in these objects. These observational results provide the first quantitative constraints for future models of PACWB. Based on archival observations obtained at the Télescope Bernard Lyot (USR5026) operated by the Observatoire Midi-Pyrénées, Université de Toulouse (Paul Sabatier), Centre National de la Recherche Scientifique (CNRS) of France, at the Canada-France-Hawaii Telescope (CFHT) operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the CNRS of France, and the University of Hawaii, and at the European Southern Observatory (ESO), Chile.

  20. Discovery of a magnetic field in the B pulsating system HD 1976

    NASA Astrophysics Data System (ADS)

    Neiner, C.; Tkachenko, A.; MiMeS Collaboration

    2014-03-01

    Aims: A magnetic field can have a strong impact on the evolution of a binary star. However, only a dozen magnetic OB binaries are known as of today and are available to study this effect, including some very few magnetic pulsating spectroscopic OB binaries. We checked for the presence of a magnetic field in the B5IV hierarchical triple system HD 1976 with spectropolarimetric data obtained with Narval at the Bernard Lyot Telescope (TBL). Methods: We used orbital parameters of HD 1976 available in the literature to disentangle the Narval intensity spectra. We computed Stokes V profiles with the least squares deconvolution technique to search for magnetic signatures. We then derived an estimate of the longitudinal magnetic field strength for each observation and for various line lists. Results: Our disentangling of the intensity spectra shows that HD 1976 is a double-lined spectroscopic (SB2) binary, the lines of the secondary component are about twice as broad as those of the primary component. We did not identify the third component. Moreover, we find clear magnetic signatures in the spectropolarimetric measurements of HD 1976 that seem to be associated with the primary component. We conclude that HD 1976 is a magnetic slowly pulsating double-lined spectroscopic binary star with an undetected third component. It is the second such example known (the other is HD 25558). Based on observations obtained at the Telescope Bernard Lyot (USR5026) operated by the Observatoire Midi-Pyrénées, Université de Toulouse (Paul Sabatier), Centre National de la Recherche Scientifique of France.

  1. The Rise Time of Type Ia Supernovae from the Supernova Legacy Survey

    NASA Astrophysics Data System (ADS)

    Conley, A.; Howell, D. A.; Howes, A.; Sullivan, M.; Astier, P.; Balam, D.; Basa, S.; Carlberg, R. G.; Fouchez, D.; Guy, J.; Hook, I.; Neill, J. D.; Pain, R.; Perrett, K.; Pritchet, C. J.; Regnault, N.; Rich, J.; Taillet, R.; Aubourg, E.; Bronder, J.; Ellis, R. S.; Fabbro, S.; Filiol, M.; Le Borgne, D.; Palanque-Delabrouille, N.; Perlmutter, S.; Ripoche, P.

    2006-10-01

    We compare the rise times of nearby and distant Type Ia supernovae (SNe Ia) as a test for evolution using 73 high-redshift spectroscopically confirmed SNe Ia from the first 2 years of the 5 year Supernova Legacy Survey (SNLS) and published observations of nearby SNe. Because of the ``rolling'' search nature of the SNLS, our measurement is approximately 6 times more precise than previous studies, allowing for a more sensitive test of evolution between nearby and distant SNe. Adopting a simple t2 early-time model (as in previous studies), we find that the rest-frame B rise times for a fiducial SN Ia at high and low redshift are consistent, with values 19.10+0.18-0.17(stat)+/-0.2(syst) and 19.58+0.22-0.19 days, respectively; the statistical significance of this difference is only 1.4 σ. The errors represent the uncertainty in the mean rather than any variation between individual SNe. We also compare subsets of our high-redshift data set based on decline rate, host galaxy star formation rate, and redshift, finding no substantive evidence for any subsample dependence. Based on observations obtained with MegaPrime/MegaCam, a joint project of the Canada-France-Hawaii Telescope (CFHT) and CEA/DAPNIA, at CFHT, which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. This work is based in part on data products produced at the Canadian Astronomy Data Centre as part of the CFHT Legacy Survey, a collaborative project of NRC and CNRS.

  2. The VIMOS Public Extragalactic Redshift Survey (VIPERS). On the recovery of the count-in-cell probability distribution function

    NASA Astrophysics Data System (ADS)

    Bel, J.; Branchini, E.; Di Porto, C.; Cucciati, O.; Granett, B. R.; Iovino, A.; de la Torre, S.; Marinoni, C.; Guzzo, L.; Moscardini, L.; Cappi, A.; Abbas, U.; Adami, C.; Arnouts, S.; Bolzonella, M.; Bottini, D.; Coupon, J.; Davidzon, I.; De Lucia, G.; Fritz, A.; Franzetti, P.; Fumana, M.; Garilli, B.; Ilbert, O.; Krywult, J.; Le Brun, V.; Le Fèvre, O.; Maccagni, D.; Małek, K.; Marulli, F.; McCracken, H. J.; Paioro, L.; Polletta, M.; Pollo, A.; Schlagenhaufer, H.; Scodeggio, M.; Tasca, L. A. M.; Tojeiro, R.; Vergani, D.; Zanichelli, A.; Burden, A.; Marchetti, A.; Mellier, Y.; Nichol, R. C.; Peacock, J. A.; Percival, W. J.; Phleps, S.; Wolk, M.

    2016-04-01

    We compare three methods to measure the count-in-cell probability density function of galaxies in a spectroscopic redshift survey. From this comparison we found that, when the sampling is low (the average number of object per cell is around unity), it is necessary to use a parametric method to model the galaxy distribution. We used a set of mock catalogues of VIPERS to verify if we were able to reconstruct the cell-count probability distribution once the observational strategy is applied. We find that, in the simulated catalogues, the probability distribution of galaxies is better represented by a Gamma expansion than a skewed log-normal distribution. Finally, we correct the cell-count probability distribution function from the angular selection effect of the VIMOS instrument and study the redshift and absolute magnitude dependency of the underlying galaxy density function in VIPERS from redshift 0.5 to 1.1. We found a very weak evolution of the probability density distribution function and that it is well approximated by a Gamma distribution, independently of the chosen tracers. Based on observations collected at the European Southern Observatory, Cerro Paranal, Chile, using the Very Large Telescope under programmes 182.A-0886 and partly 070.A-9007. Also based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT), which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. This work is based in part on data products produced at TERAPIX and the Canadian Astronomy Data Centre as part of the Canada-France-Hawaii Telescope Legacy Survey, a collaborative project of NRC and CNRS. The VIPERS web site is http://www.vipers.inaf.it/

  3. The size and structure of the spheroid of IC 1613

    NASA Astrophysics Data System (ADS)

    Battinelli, P.; Demers, S.; Artigau, É.

    2007-05-01

    Context: Nearby galaxies, spirals as well as irregulars, have been found to be much larger than previously believed. The structure of the huge spheroid surrounding dwarf galaxies could give clues to their past gravitational history. Thanks to wide field imagers, nearby galaxies with diameter of dozens of arcmin can be effectively surveyed. Aims: We obtain, from the CFHT archives, a series of i' and g' MegaCam images of IC 1613 in order to determine the stellar surface density of the field and determine the shape of its spheroid. Methods: From the colour magnitude diagram we select some 36 000 stars, in the first three magnitudes of the red giant branch. The spatial distribution of these stars is used to establish the structure of the spheroid. Results: The position angle of the major axis of the stellar spheroid is found to be ≈90°, some 30° from the major axis of the HI cloud surrounding IC 1613. The surface density profile of the spheroid is not exponential over all the length of the major axis. A King profile, with a core radius of 4.5' and a tidal radius of 24' fits the data. The tidal truncation of the spheroid suggests that IC 1613 is indeed a satellite of M 31. Based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institute National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  4. An attempt to detect the dust disk of VEGA by photopolarimetry, and constraints on the grain size

    NASA Astrophysics Data System (ADS)

    Mauron, N.; Dole, H.

    1998-09-01

    We report on a first attempt to detect Vega's disk through optical scattered light by using linear photopolarimetry. Polarization measurements on the aureole of Vega were carried out between 7'' and 30'' from the star with a 10'' diameter hole and down to polarization level of ~ 10(-4) . No signal reliably attributable to circumstellar dust was detected, and an upper limit to the polarized surface brightness of the disk is derived. This upper limit for Vega's disk is about 200 times lower than the polarized brightness observed around beta Pic, at an angular offset of 15'' from the stars. The upper limit is also compared to a simple model, in which one assumes a plausible total dust mass of 2 10(-8) Msun, and a pole-on oriented disk with a typical radius of ~ 20'' as favoured by far-infrared and submillimetric experiments. We also suppose that the grains are spherical (Mie) particles. Our analysis can exclude that a major part of dust mass would consist of grains of 0.01-0.3 mu m, as in the interstellar medium. If a single size is assumed, the observational upper limit favours radii of at least 5-10 mu m or larger. If a size distribution including large particles ( ~ 300 mu m) is assumed, the data suggests that only a very small fraction ( ~ 1/1000 ) of the dust mass is in 0.01-0.3 mu m grains. Based on observations made at the 2-m telescope of Pic-du-Midi, operated by Observatoire Midi Pyrénées (Centre National de la Recherche Scientifique \\& Université Paul Sabatier de Toulouse, France)

  5. The RISQ network as an R and D catalyst and test bench

    NASA Astrophysics Data System (ADS)

    Lauzon, Jocelyn

    2005-09-01

    The RISQ (Réseau d'Informations Scientifiques du Québec) research and education network has been a trail-blazer in the development of privately owned fiber networks, by implementing an optical fiber owner model. This model allows RISQ to have a gracefully upgradable network that is at the forefront of the large bandwidth optical communications technology. It also allows RISQ to offer a parallel network that can be used as a test equipment for the R&D community, in universities, research institutions or the industry; a real in-the-field fiber optic network test bench. RISQ is in a privileged situation to influence optical communications R&D work. It is aware of the real needs of the telecommunications industry. It is also aware of the technological needs of the next-generation networks. RISQ suggests that telecommunications R&D should be focused on increasing network reliability and decrease network operations and capital expanses, rather than on increasing their capacity. A key to decreasing expanses would be to avoid SONET network management on long-haul trunks, without affecting the transmission quality of service. IP over optics should thus be reinstalled as a priority in the telecom R&D world. RISQ thinks optical 3R might be the solution that will allow IP over optics. As for the next-generation networks: flexibility, reconfigurability, in order to offer lightpaths of adjustable bandwidth to the user; while wasting a minimum of the valuable network bandwidth, is where we believe efforts should be concentrated on.

  6. A 10-h period revealed in optical spectra of the highly variable WN8 Wolf-Rayet star WR 123

    NASA Astrophysics Data System (ADS)

    Chené, A.-N.; Foellmi, C.; Marchenko, S. V.; St-Louis, N.; Moffat, A. F. J.; Ballereau, D.; Chauville, J.; Zorec, J.; Poteet, C. A.

    2011-06-01

    Aims: What is the origin of the large-amplitude variability in Wolf-Rayet WN8 stars in general and WR123 in particular? A dedicated spectroscopic campaign targets the ten-hour period previously found in the high-precision photometric data obtained by the MOST satellite. Methods: In June-August 2003 we obtained a series of high signal-to-noise, mid-resolution spectra from several sites in the λλ 4000-6940 Å domain. We also followed the star with occasional broadband (Johnson V) photometry. The acquired spectroscopy allowed a detailed study of spectral variability on timescales from ~5 min to months. Results: We find that all observed spectral lines of a given chemical element tend to show similar variations and that there is a good correlation between the lines of different elements, without any significant time delays, save the strong absorption components of the Hei lines, which tend to vary differently from the emission parts. We find a single sustained periodicity, P ~ 9.8 h, which is likely related to the relatively stable pulsations found in MOST photometry obtained one year later. In addition, seemingly stochastic, large-amplitude variations are also seen in all spectral lines on timescales of several hours to several days. Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Concil of Canada, the Institut National des Sciences de l'Univers of the Centre National de Recherche Scientifique of France, and the University of Hawaii. Based also on observations made with ESO Telescopes at the La Silla Observatory, under programme ID 271.D-5025.Photometric data presented in Fig. 1 are only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/530/A151

  7. Linkage Relationships of Genes Controlling Isoleucine, Valine, and Leucine Biosynthesis in Bacillus subtilis

    PubMed Central

    Barat, M.; Anagnostopoulos, C.; Schneider, A.-M.

    1965-01-01

    Barat, M. (Centre National de la Recherche Scientifique, Gif-sur-Yvette, Seine et Oise, France), C. Anagnostopoulos, and A.-M. Schneider. Linkage relationships of genes controlling isoleucine, valine, and leucine biosynthesis in Bacillus subtilis. J. Bacteriol.90:357–369. 1965.—In Bacillus subtilis, the genetic loci controlling isoleucine and valine biosynthesis are not all clustered. Some of them were located on two distinct transforming deoxyribonucleic acid “molecules.” One of these molecules (the “ileilva2–4-met segment”) carries the threonine deaminase and the dihydroxy acid dehydrase loci linked to methionine markers. The other (the “ilva1–3-leu segment”) bears the reductoisomerase locus and one or more loci involved in leucine synthesis. A phenylalanine marker was also shown to be weakly linked to this latter group. In transduction mediated by phage PBS-1, these groups are transferred jointly with other gene clusters. The phage appears to convey chromosome fragments considerably longer than the transforming “molecules.” The genetic maps of both the above segments were extended by transduction. Some groups previously studied by transformation can be placed in the following linear order: the ile-ilva2–4-met segment, the cluster of loci involved in aromatic amino acid synthesis (try segment), and a lysine locus. An arginine locus is cotransduced with the phe-ilva1–2-leu segment. Recombination frequencies between linked markers are much lower in transduction by this phage than in transformation. PMID:14329448

  8. Spectroscopic confirmation of high-redshift supernovae with the ESO VLT.

    NASA Astrophysics Data System (ADS)

    Lidman, C.; Howell, D. A.; Folatelli, G.; Garavini, G.; Nobili, S.; Aldering, G.; Amanullah, R.; Antilogus, P.; Astier, P.; Blanc, G.; Burns, M. S.; Conley, A.; Deustua, S. E.; Doi, M.; Ellis, R.; Fabbro, S.; Fadeyev, V.; Gibbons, R.; Goldhaber, G.; Goobar, A.; Groom, D. E.; Hook, I.; Kashikawa, N.; Kim, A. G.; Knop, R. A.; Lee, B. C.; Mendez, J.; Morokuma, T.; Motohara, K.; Nugent, P. E.; Pain, R.; Perlmutter, S.; Prasad, V.; Quimby, R.; Raux, J.; Regnault, N.; Ruiz-Lapuente, P.; Sainton, G.; Schaefer, B. E.; Schahmaneche, K.; Smith, E.; Spadafora, A. L.; Stanishev, V.; Walton, N. A.; Wang, L.; Wood-Vasey, W. M.; Yasuda, N.; Supernova Cosmology Project

    2005-02-01

    We present VLT FORS1 and FORS2 spectra of 39 candidate high-redshift supernovae that were discovered as part of a cosmological study using type Ia supernovae (SNe Ia) over a wide range of redshifts. From the spectra alone, 20 candidates are spectrally classified as SNe Ia with redshifts ranging from z=0.212 to z=1.181. Of the remaining 19 candidates, 1 might be a type II supernova and 11 exhibit broad supernova-like spectral features and/or have supernova-like light curves. The candidates were discovered in 8 separate ground-based searches. In those searches in which SNe Ia at z ˜ 0.5 were targeted, over 80% of the observed candidates were spectrally classified as SNe Ia. In those searches in which SNe Ia with z > 1 were targeted, 4 candidates with z > 1 were spectrally classified as SNe Ia and later followed with ground and space based observatories. We present the spectra of all candidates, including those that could not be spectrally classified as supernova. Based on observations obtained at the European Southern Observatory using the ESO Very Large Telescope on Cerro Paranal (ESO programs 265.A-5721(A), 67.A-0361(A), 267.A-5688(A), 169.A-0382(A) and (B)). Based in part on data collected at the Subaru Telescope, which is operated by the National Astronomical Observatory of Japan. Based in part on data collected from the Canada-France-Hawaii Telescope Corporation, which is operated by the National Research Council of Canada, le Centre National de la Recherche Scientifique de France, and the University of Hawaii. Based in part on data collected at the Cerro Tololo Inter-American Observatory, which is operated by Association of Universities for Research in Astronomy, Inc. under a cooperative agreement with the National Science Foundation. Appendix A is only available in electronic form via http://www.edpsciences.org

  9. The Recent Stellar Archeology of M31—The Nearest Red Disk Galaxy

    NASA Astrophysics Data System (ADS)

    Davidge, T. J.; McConnachie, A. W.; Fardal, M. A.; Fliri, J.; Valls-Gabaud, D.; Chapman, S. C.; Lewis, G. F.; Rich, R. M.

    2012-05-01

    We examine the star-forming history of the M31 disk during the past few hundred Myr. The luminosity functions (LFs) of main-sequence stars at distances R GC > 21 kpc (i.e., >4 disk scale lengths) are matched by models that assume a constant star formation rate (SFR). However, at smaller R GC the LFs suggest that during the past ~10 Myr the SFR was 2-3 times higher than during the preceding ~100 Myr. The rings of cool gas that harbor a significant fraction of the current star-forming activity are traced by stars with ages ~100 Myr, indicating that (1) these structures have ages of at least 100 Myr and (2) stars in these structures do not follow the same relation between age and random velocity as their counterparts throughout the disks of other spiral galaxies, probably due to the inherently narrow orbital angular momentum distribution of the giant molecular clouds in these structures. The distribution of evolved red stars is not azimuthally symmetric, in the sense that the projected density along the northeast segment of the major axis is roughly twice that on the opposite side of the galaxy. The northeast arm of the major axis thus appears to be a fossil star-forming area that dates to intermediate epochs. Such a structure may be the consequence of interactions with a companion galaxy. Based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT), which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii.

  10. Large scale silver nanowires network fabricated by MeV hydrogen (H+) ion beam irradiation

    NASA Astrophysics Data System (ADS)

    Honey, S.; Naseem, S.; Ishaq, A.; Maaza, M.; Bhatti, M. T.; Wan, D.

    2016-04-01

    A random two-dimensional large scale nano-network of silver nanowires (Ag-NWs) is fabricated by MeV hydrogen (H+) ion beam irradiation. Ag-NWs are irradiated under H+ ion beam at different ion fluences at room temperature. The Ag-NW network is fabricated by H+ ion beam-induced welding of Ag-NWs at intersecting positions. H+ ion beam induced welding is confirmed by transmission electron microscopy (TEM) and scanning electron microscopy (SEM). Moreover, the structure of Ag NWs remains stable under H+ ion beam, and networks are optically transparent. Morphology also remains stable under H+ ion beam irradiation. No slicings or cuttings of Ag-NWs are observed under MeV H+ ion beam irradiation. The results exhibit that the formation of Ag-NW network proceeds through three steps: ion beam induced thermal spikes lead to the local heating of Ag-NWs, the formation of simple junctions on small scale, and the formation of a large scale network. This observation is useful for using Ag-NWs based devices in upper space where protons are abandoned in an energy range from MeV to GeV. This high-quality Ag-NW network can also be used as a transparent electrode for optoelectronics devices. Project supported by the National Research Foundation of South Africa (NRF), the French Centre National pour la Recherche Scientifique, iThemba-LABS, the UNESCO-UNISA Africa Chair in Nanosciences & Nanotechnology, the Third World Academy of Science (TWAS), Organization of Women in Science for the Developing World (OWSDW), the Abdus Salam ICTP via the Nanosciences African Network (NANOAFNET), and the Higher Education Commission (HEC) of Pakistan.

  11. The space instrument SODISM and the ground instrument SODISM II

    NASA Astrophysics Data System (ADS)

    Meftah, M.; Meissonnier, M.; Irbah, A.; Abbaki, S.; Assus, P.; Bertran, E.; Dubois, J. P.; Ducourt, E.; Dufour, C.; Marcovici, J. P.; Poiet, G.; Vieau, A. J.; Thuillier, G.

    2010-07-01

    PICARD is a French space scientific mission. Its objectives are the study of the origin of the solar variability and the study of the relations between the Sun and the Earth's climate. The launch is scheduled for 2010 on a Sun Synchronous Orbit at 725 km altitude. The mission lifetime is two years, however that can be extended to three years. The payload consists of two absolute radiometers measuring the TSI (Total Solar Irradiance) and an imaging telescope to determine the solar diameter, the limb shape and asphericity. SOVAP (SOlar VAriability PICARD) is an absolute radiometer provided by the RMIB (Royal Meteorological Institute of Belgium) to measure the TSI. It also carries a bolometer used for increasing the TSI sampling and ageing control. PREMOS (PREcision MOnitoring Sensor) radiometer is provided by the PMOD/WRC (Physikalisch Meteorologisches Observatorium of Davos / World Radiation Center) to measure the TSI and the Spectral Solar Irradiance. SODISM (SOlar Diameter Imager and Surface Mapper), is an 11-cm Ritchey-Chr´etien imaging telescope developed at CNRS (Centre National de la Recherche Scientifique) by LATMOS (Laboratoire, ATmosphere, Milieux, Observations Spatiales) ex Service d'A´eronomie, associated with a 2Kx2K CCD (Charge-Coupled Device), taking solar images at five wavelengths. It carries a four-prism system to ensure a metrological control of the optics magnification. SODISM allows us to measure the solar diameter and shape with an accuracy of a few milliarcseconds, and to perform helioseismologic observations to probe the solar interior. In this article, we describe the space instrument SODISM and its thermo-elastic properties. We also present the PICARD payload data center and the ground instrument SODISM II which will observe together with the space instrument.

  12. Near-infrared Thermal Emission Detections of a Number of Hot Jupiters and the Systematics of Ground-based Near-infrared Photometry

    NASA Astrophysics Data System (ADS)

    Croll, Bryce; Albert, Loic; Jayawardhana, Ray; Cushing, Michael; Moutou, Claire; Lafreniere, David; Johnson, John Asher; Bonomo, Aldo S.; Deleuil, Magali; Fortney, Jonathan

    2015-03-01

    We present detections of the near-infrared thermal emission of three hot Jupiters and one brown dwarf using the Wide-field Infrared Camera (WIRCam) on the Canada-France-Hawaii Telescope (CFHT). These include Ks-band secondary eclipse detections of the hot Jupiters WASP-3b and Qatar-1b and the brown dwarf KELT-1b. We also report Y-band, K CONT-band, and two new and one reanalyzed Ks-band detections of the thermal emission of the hot Jupiter WASP-12b. We present a new reduction pipeline for CFHT/WIRCam data, which is optimized for high precision photometry. We also describe novel techniques for constraining systematic errors in ground-based near-infrared photometry, so as to return reliable secondary eclipse depths and uncertainties. We discuss the noise properties of our ground-based photometry for wavelengths spanning the near-infrared (the YJHK bands), for faint and bright stars, and for the same object on several occasions. For the hot Jupiters WASP-3b and WASP-12b we demonstrate the repeatability of our eclipse depth measurements in the Ks band; we therefore place stringent limits on the systematics of ground-based, near-infrared photometry, and also rule out violent weather changes in the deep, high pressure atmospheres of these two hot Jupiters at the epochs of our observations. Based on observations obtained with WIRCam, a joint project of Canada-France-Hawaii Telescope (CFHT), Taiwan, Korea, Canada, France, at the CFHT, which is operated by the National Research Council (NRC) of Canada, the Institute National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  13. Disclinations and grain boundary migration: evidence for a new deformation mechanism in olivine-rich rocks (Invited)

    NASA Astrophysics Data System (ADS)

    Cordier, P.; Demouchy, S. A.; Beausir, B.; Taupin, V.; Fressengeas, C.

    2013-12-01

    The rheology of olivine-rich rocks remains poorly understood. In particular, the ability of orthorhombic olivine to bear large strains represents an apparent violation of the von Mises criterion due to a lack of slip systems. In this study we show that a more general description of the deformation process including the motion of rotational defects referred to as disclinations can solve the olivine deformation paradox. Disclinations were proposed together with dislocations by Volterra (1907) to account for elastic distorsions (distorzione) in solids. They have recently been experimentally evidenced from orientation maps in several polycrystalline metallic alloys (Beausir & Fressengeas, 2013). Using high-resolution EBSD orientation maps we show that disclinations decorate grain boundaries in olivine samples deformed experimentally and in nature. We present a disclination-based model of a high-angle tilt boundary in olivine, which demonstrates that an applied shear induces grain boundary migration through disclination motion. This new approach allows further understanding of grain boundary-mediated plasticity in polycrystalline aggregates. By providing the missing mechanism for describing plastic flow in olivine, the present work allows multiscale modeling of the rheology of the upper mantle, from the atomic scale to the scale of the flow. Beausir, B. & Fressengeas, C., Disclination densities from EBSD orientation mapping. International Journal of Solids and Structures 50 (1), 137-146 (2013). Volterra, V., Sur l'équilibre des corps élastiques multiplement connexes. Annales scientifiques de l'École Normale Supérieure 24, 401-517 (1907). Acknowledgement for support: ERC grant RheoMan, Marie Curie fellowship PoEM and ANR NanoMec.

  14. [The international man-media Tessékéré (OHMi) Observatory: a research tool to study the complexity of arid ecosystems in Sahel].

    PubMed

    Guissé, Aliou; Boëtsch, Gilles; Ducourneau, Axel; Goffner, Deborah; Gueye, Lamine

    2013-01-01

    In the Sahelian zone, the drought phenomenon, combined with anthropic factors (monoculture, bush fires, defect or deficit of manure, overgrazing, etc.), has seriously affected ecological great balances, involving a degradation of the natural resources as well as a fall in agricultural productions, pointing to a process of desertification. To face these challenges, in the course of the 8th ordinary session of the conference of the Heads of States of the African Union held in January 2007 in Addis Ababa (Ethiopia), 11 countries adopted the Panafrican project called the Green Great Wall (GGW). The total objective of the GGW is to contribute i) to the fight against the desert's advance, ii) to the development of the Saharan-Sahelian zones toward a durable management of the natural resources, and iii) to the fight against poverty. It deals with the construction of a set of zones of afforestation crossing the whole African continent in the long term (7000km of which are in the west). Even if some decisions in the launching phase the GGW must be taken quickly, one cannot do without investment in interdisciplinary research. In particular, associating fundamental research and applied research will allow us to ensure the success in the medium and long term of such a large-scale reforestation project. Research segmented in compartmentalized knowledge fields needed to get adequate tools, among which OHMi Tessékéré, initiated by INNEE (Centre national de la recherche scientifique [CNRS]), in partnership with UCAD, constitutes an example. This suitable scientific tool, capable of action flexibility, of self-financing capacity, anchored in civil society, ready to implement a pragmatic and local interdisciplinarity founded currently on the concept of socio-ecological system (SES), is the one we chose to conduct our studies on the Ferlo arid ecosystems. PMID:23916202

  15. Effect of Feeding On The Carbon and Oxygen Isotopic Composition In The Tissues and Skeleton of The Zooxanthellate Coral Stylophora Pistillata

    NASA Astrophysics Data System (ADS)

    Reynaud-Vaganay, S.; Ferrier-Pagès, C.; Sambrotto, R.; Juillet-Leclerc, A.; Jaubert, J.

    and J.-P. Gattuso4 1Centre Scientifique de Monaco, Avenue Saint Martin, MC-98000, Principality of Monaco 2Lamont-Doherty Earth Observatory, 61 Rt. 9W/ P.O. Box 1000, Palisades, NY 10964 U.S.A 3Laboratoire des Sciences du Climat et de l'Environnement, Laboratoire mixte CNRS- CEA, F-91180 Gif-sur-Yvette Cedex, France 4Observatoire Océanologique, Laboratoire d'Océanographie, CNRS-UPMC, BP 28, F- 06234 Villefranche-sur-mer Cedex, France The effect of feeding on the carbon isotopic composition of zooxanthellae, animal tissue and skeleton was investigated in the scleractinian coral Stylophora pistillata. Two sets of corals were grown with filtered seawater under controlled conditions. One group of colonies was fed with Artemia nauplii and compared to a control group that was starved. Fed corals exhibited higher concentrations of chlorophyll protein calcification rates than starved colonies. The net photosynthetic rate was higher in starved than in fed corals, whereas dark respiration was not significantly different. The average ? C value of Artemia nauplii used for feeding was -12. ? C was 13 13 significantly heavier in zooxanthellae than in animal tissues, for both fed (-10.1vs. -11.7) and starved colonies (-10.9vs. -13.2). Isotopic data reflected the incorporation of Artemia carbon into the coral tissue in that the ? C was 13 significantly heavier in fed than in starved colonies (-11.7 to -13.2 respectively), although there was no difference in the ? C of the zooxanthellae fraction. Skeletal 13 ? C was similar in fed and starved colonies (mean = -4.6). Skeletal ? O 13 18 composition was, however, significantly different between the two treatments (-4.24 to -4.05 for fed and starved colonies respectively). These data are used to establish a conceptual model of the carbon flow between the various compartments of a symbiotic coral.

  16. Weak magnetic field, solid-envelope rotation, and wave-induced N-enrichment in the SPB star ζ Cassiopeiae

    NASA Astrophysics Data System (ADS)

    Briquet, M.; Neiner, C.; Petit, P.; Leroy, B.; de Batz, B.

    2016-03-01

    Aims: The main-sequence B-type star ζ Cassiopeiae is known as a N-rich star with a magnetic field discovered with the Musicos spectropolarimeter. We model the magnetic field of the star by means of 82 new spectropolarimetric observations of higher precision to investigate the field strength, topology, and effect. Methods: We gathered data with the Narval spectropolarimeter installed at Télescope Bernard Lyot (TBL; Pic du Midi, France) and applied the least-squares deconvolution technique to measure the circular polarisation of the light emitted from ζ Cas. We used a dipole oblique rotator model to determine the field configuration by fitting the longitudinal field measurements and by synthesizing the measured Stokes V profiles. We also made use of the Zeeman-Doppler imaging technique to map the stellar surface and to deduce the difference in rotation rate between the pole and equator. Results: ζ Cas exhibits a polar field strength Bpol of 100-150 G, which is the weakest polar field observed so far in a massive main-sequence star. Surface differential rotation is ruled out by our observations and the field of ζ Cas is strong enough to enforce rigid internal rotation in the radiative zone according to theory. Thus, the star rotates as a solid body in the envelope. Conclusions: We therefore exclude rotationally induced mixing as the cause of the surface N-enrichment. We discuss that the transport of chemicals from the core to the surface by internal gravity waves is the most plausible explanation for the nitrogen overabundance at the surface of ζ Cas. Based on observations obtained at the Télescope Bernard Lyot (USR5026) operated by the Observatoire Midi-Pyrénées, Université de Toulouse (Paul Sabatier), Centre National de la Recherche Scientifique (CNRS) of France.

  17. International Congress on Transposable Elements (ICTE) 2012 in Saint Malo and the sea of TE stories

    PubMed Central

    2012-01-01

    An international conference on Transposable Elements (TEs) was held 21–24 April 2012 in Saint Malo, France. Organized by the French Transposition Community (GDR Elements Génétiques Mobiles et Génomes, CNRS) and the French Society of Genetics (SFG), the conference’s goal was to bring together researchers from around the world who study transposition in diverse organisms using multiple experimental approaches. The meeting drew more than 217 attendees and most contributed through poster presentations (117), invited talks and short talks selected from poster abstracts (48 in total). The talks were organized into four scientific sessions, focused on: impact of TEs on genomes, control of transposition, evolution of TEs and mechanisms of transposition. Here, we present highlights from the talks given during the platform sessions. The conference was sponsored by Alliance pour les sciences de la vie et de la santé (Aviesan), Centre national de la recherche scientifique (CNRS), Institut national de la santé et de la recherche médicale (INSERM), Institut de recherche pour le développement (IRD), Institut national de la recherche agronomique (INRA), Université de Perpignan, Université de Rennes 1, Région Bretagne and Mobile DNA. Chair of the organization committee Jean-Marc Deragon Organizers Abdelkader Ainouche, Mireille Bétermier, Mick Chandler, Richard Cordaux, Gaël Cristofari, Jean-Marc Deragon, Pascale Lesage, Didier Mazel, Olivier Panaud, Hadi Quesneville, Chantal Vaury, Cristina Vieira and Clémentine Vitte PMID:23110759

  18. Sharing is Winning: Cooperative Learning about Atmospheric Composition Change

    NASA Astrophysics Data System (ADS)

    Schuepbach, E.

    2010-09-01

    This contribution presents evolving good practice in disseminating the body of know-how, skills and competencies within the networked community of atmospheric scientists as established in ACCENT. The promotion of early-career scientists, and encouraging the next generation to move into the field were among the key issues addressed by the "Training and Education" programme in the European Network of Excellence in Atmospheric Composition Change (ACCENT). Dissemination avenues include a virtual knowledge train carrying the wealth of high-quality scientific learning material developed with experts involved in the ACCENT network. Learning opportunities on current research in atmospheric composition change in Europe were also created during face-to-face training workshops. Real-life examples of pressing air quality issues were addressed in meetings with stakeholder groups that offered opportunities for mutual learning in inspiring partnerships. In order to increase the expertise in atmospheric composition change across Europe, activities were organized with the general public (e.g., Café Scientifique), where the participating early-career scientists were confronted with questions from lay people. For interested teachers, didactic translations of compact overviews on air quality science topics developed in ACCENT offer links with the typical European science curriculum and go beyond school book content. Some of the educational events, methods and tools are described in a booklet published in 2009 ("We Care for Clean Air!", ISBN 978-88-95665-01-6). The electronic version and all training material can be downloaded from www.accent-network.org/portal/education - a valuable resource for teachers and learners around the globe.

  19. Crosstalk: public cafés as places for knowledge translation concerning health care research.

    PubMed

    Reimer-Kirkham, Sheryl; Jule, Allyson

    2015-01-01

    This article explores the use of public cafés as a model for knowledge translation and community engagement. We base our discussion on a public café series organized around the theme of access to health care and held in three neighborhoods in the Lower Mainland of British Columbia, Canada. The cafés were part of the Canadian Institutes of Health Research Café Scientifique program. Our purposes for this series of cafés were threefold: (a) to provide a site of communication to connect research with members of the public, (b) to build a network among participants based on common connections to the local community, and (c) to explore through discussion how gendered and raced perspectives concerning access to health care may influence the lived experiences of Canadians today. We intended to promote an intergroup conversation, based on the assumption that people of First Nations descent, newcomers to Canada (whether through immigration or resettlement), and settlers (such as Euro-Canadians) would all benefit from hearing each other's perspectives on access to health care, as well as presentations by invited academics about their research on access to health care. A form of "crosstalk" emerged in the cafés, mediated by gender and ethnicity, where social differences and geographical distances between various groups were not easily bridged, and yet where opportunity was created for inclusive dialogic spaces. We conclude that knowledge translation is not easily accomplished with the café format, at least not with the type of critical knowledge we were aiming to translate and the depth of engagement we were hoping for. Our experiences highlighted three strategies that facilitate knowledge translation: relationships and shared goals; involvement of policymakers and decision makers; and tending to social relations of power. PMID:24992638

  20. Science outreach on tap: insights and practices from three years ofDartmouth Science Pubs.

    NASA Astrophysics Data System (ADS)

    Hawley, R. L.; Serrell, N.; Tobery, C. E.; Riordan, S. A.

    2015-12-01

    The "Cafe Scientifique" (or "Science Cafe") has existed around theworld for decades. In an informal setting, one or more scientistsengage with a lay audience, typically over refreshments of some kind.These Science Cafes have taken many formats and taken place in manyvenues. Some feature a single presenter, some multiple; somecongregate in large venues, some small; some restrict the use of thepowerpoint slides, some do not.Our team at Dartmouth has hosted "Science Pubs" for three years. OurScience Pub takes place in a local pub, from 5-7pm on a weekday once amonth. We choose a theme for a pub and select three presenters. Thecomposition of our panel varies, but we generally have at least onefaculty member and one "less-academic" member, such as a town plannerwhen discussing hurricanes or an organic farmer when discussingpesticides. Often we include a graduate student in the panel. ThePub takes place in three "acts": 1) the presenters each give a briefintroduction to thier take on the topic, usually 10-15 minutes,extemporaneous with no slides, 2) the "wedding reception" phase, whichis a break during which the presenters circulate to the pub tables,answering questions and chatting with the attendees informally, and 3)reconvening for a more 'formal' question and answer period duringwhich the presenters answer questions from the audience.Here, we outline the format that makes up a Dartmouth Science Pub andshare insignts and lessons learned. Among many findings, we havelearned: 1) a group of three presenters makes for a lively discussion,as often presenters 'riff' off one another's points, 2) it is cruicalto have a facilitator, to 'run the show', freeing the sciencepresenters to concentrate on thier audience engagement, and 3) a shortmeeting ahead of time with the presenters is simple and very importantin creating a smooth event, and serves to help the presenters 'codeswitch' and adapt language, in lieu of a formal 'training'.

  1. Changes during hibernation in different phospholipid and free and esterified cholesterol serum levels in black bears

    USGS Publications Warehouse

    Chauhan, V.; Sheikh, A.; Chauhan, A.; Tsiouris, J.; Malik, M.; Vaughan, M.

    2002-01-01

    During hibernation, fat is known to be the preferred source of energy. A detailed analysis of different phospholipids, as well as free and esterified cholesterol, was conducted to investigate lipid abnormalities during hibernation. The levels of total phospholipids and total cholesterol in the serum of black bears were found to increase significantly in hibernation as compared with the active state. Both free and esterified cholesterol were increased in the hibernating state in comparison with the active state (P < 0.05). The percentage increase during hibernation was more in free cholesterol (57%) than in esterified cholesterol (27%). Analysis of subclasses of serum phospholipids showed that choline containing phospholipids, i.e., sphingomyelin (SPG) (14%) and phosphatidylcholine (PC) (76%), are the major phospholipids in the serum of bear. The minor phospholipids included 8% of phosphatidylserine (PS) + phosphatidylinositol (PI), while phosphatidylethanolamine (PE) was only 2% of the total phospholipids. A comparison of phospholipid subclasses showed that PC, PS + PI and SPG were significantly increased, while PE was significantly decreased (P < 0.05) in the hibernating state as compared with the active state in black bears. These results suggest that the catabolism of phospholipids and cholesterol is decreased during hibernation in black bears, leading to their increased levels in the hibernating state as compared with the active state. In summary, our results indicate that serum cholesterol and phospholipid fractions (except PE) are increased during hibernation in bears. It is proposed that the increase of these lipids may be due to the altered metabolism of lipoproteins that are responsible for the clearance of the lipids. ?? 2002 E??ditions scientifiques et me??dicales Elsevier SAS and Socie??te?? franc??aise de biochimie et biologie mole??culaire. All rights reserved.

  2. Dynamical analysis of nearby clusters. Automated astrometry from the ground: precision proper motions over a wide field

    NASA Astrophysics Data System (ADS)

    Bouy, H.; Bertin, E.; Moraux, E.; Cuillandre, J.-C.; Bouvier, J.; Barrado, D.; Solano, E.; Bayo, A.

    2013-06-01

    Context. The kinematic properties of the different classes of objects in a given association hold important clues about the history of its members, and offer a unique opportunity to test the predictions of the various models of stellar formation and evolution. Aims: DANCe (standing for dynamical analysis of nearby clusters) is a survey program aimed at deriving a comprehensive and homogeneous census of the stellar and substellar content of a number of nearby (<1 kpc) young (<500 Myr) associations. Whenever possible, members will be identified based on their kinematics properties, ensuring little contamination from background and foreground sources. Otherwise, the dynamics of previously confirmed members will be studied using the proper motion measurements. We present here the method used to derive precise proper motion measurements, using the Pleiades cluster as a test bench. Methods: Combining deep wide-field multi-epoch panchromatic images obtained at various obervatories over up to 14 years, we derived accurate proper motions for the sources in the field of the survey. The datasets cover ≈80 square degrees, centered around the Seven Sisters. Results: Using new tools, we have computed a catalog of 6 116 907 unique sources, including proper motion measurements for 3 577 478 of them. The catalog covers the magnitude range between i = 12 ~ 24 mag, achieving a proper motion accuracy <1 mas y-1 for sources as faint as i = 22.5 mag. We estimate that our final accuracy reaches 0.3 mas yr-1 in the best cases, depending on magnitude, observing history, and the presence of reference extragalactic sources for the anchoring onto the ICRS. Based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Science de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the

  3. European Virtual Atomic And Molecular Data Center - VAMDC

    NASA Astrophysics Data System (ADS)

    Dimitrijevic, M. S.; Sahal-Brechot, S.; Kovacevic, A.; Jevremovic, D.; Popovic, L. C.

    2010-07-01

    Reliable atomic and molecular data are of great importance for different applications in astrophysics, atmospheric physics, fusion, environmental sciences, combustion chemistry, and in industrial applications from plasmas and lasers to lighting. Currently, very important resources of such data are highly fragmented, presented in different, nonstandardized ways, available through a variety of highly specialized and often poorly documented interfaces, so that the full exploitation of all their scientific worth is limited, hindering research in many topics like e.g. the characterization of extrasolar planets, understanding the chemistry of our local solar system and of the wider universe, the study of the terrestrial atmosphere and quantification of climate change; the development of the fusion rersearch, etc. The Virtual Atomic and Molecular Data Centre (http://www.vamdc.eu, VAMDC) is an European Union funded FP7 project aiming to build a secure, documented, flexible and interoperable e-science environment-based interface to existing atomic and molecular data. It will also provide a forum for training potential users and dissemination of expertise worldwide. Partners in the Consortium of the Project are: 1) Centre National de Recherche Scientifique - CNRS (Paris, Reims, Grenoble, Bordeaux, Dijon, Toulouse); 2) The Chancellor, Masters and Scholars of the University of Cambridge - CMSUC; 3) University College London - UCL; 4) Open University - OU; (Milton Keynes, England); 5) Universitaet Wien - UNIVIE; 6) Uppsala Universitet - UU; 7) Universitaet zu Koeln - KOLN; 8) Istituto Nazionale di Astrofisica - INAF (Catania, Cagliari); 9) Queen's University Belfast - QUB; 10) Astronomska Opservatorija - AOB (Belgrade, Serbia); 11) Institute of Spectroscopy RAS - ISRAN (Troitsk, Russia); 12) Russian Federal Nuclear Center - All-Russian Institute of Technical Physics - RFNC-VNIITF (Snezhinsk, Chelyabinsk Region, Russia; 13) Institute of Atmospheric Optics - IAO (Tomsk, Russia

  4. Le transfert de connaissances entre les mathematiques et les sciences. Une etude exploratoire aupres d'eleves de 4e secondaire

    NASA Astrophysics Data System (ADS)

    Samson, Ghislain

    2003-06-01

    Au moment ou dans plusieurs pays on travaille a refondre les programmes d'etudes, tant au primaire qu'au secondaire, l'interet pour le transfert renait. Un des concepts fondamentaux en apprentissage consiste en l'habilete a reutiliser de facon consciente et efficace un acquis d'une situation a une autre situation. Cette recherche emane de preoccupations professionnelles au moment ou le chercheur etait enseignant au secondaire. Au cours de ces annees, il lui a ete possible de constater que plusieurs eleves percevaient difficilement les liens presents entre les disciplines mathematiques et scientifiques. Des travaux en psychologie cognitive et plus particulierement selon une perspective du traitement de l'information ont servi de cadre de reference pour evaluer et analyser les capacites de transfert aupres d'eleves de 4e secondaire. Ce cadre de reference permet de formuler le principal objectif qui est de mieux comprendre le processus de transfert chez des eleves en situation de resolution de problemes scientifiques. Cette these s'interesse donc au transfert en tant que phenomene important du processus d'apprentissage au sens de l'integration. La methode de recherche choisie, de nature qualitative, est principalement axee sur l'evaluation de la capacite a transferer des connaissances lors d'une epreuve et d'un entretien. Pour evaluer ce potentiel de transfert, nous avons elabore deux outils: une epreuve en mathematiques et en sciences et un guide d'entretien. Pour la passation de l'epreuve, le chercheur a pu compter sur la collaboration de 130 sujets provenant de deux ecoles. L'entretien complete la prise de donnees avec 13 sujets ayant accepte de poursuivre l'etude. Les donnees recueillies par ces instruments font ensuite l'objet d'une analyse de contenu. En premier lieu, les verbatims de l'epreuve et de l'entretien ont ete transcrits, puis codifies. La correction des reponses fournies pour les problemes resolus s'est faite a partir d'une grille d

  5. Implementation of Theeuropeanwater Framework Directive In France: New Challenges For River Basin Organisat Ion, Planning and Participation

    NASA Astrophysics Data System (ADS)

    Allain, S.

    defined and implemented by a new tripartite entity, the Commission Locale de l'Eau (CLE : Local Water Commission), which can be considered as a real river basin organisation; an empirical analysis of the implementation of such a procedure can offer therefore many new insights and the paper will present the results of an analysis of 10 case studies. But it will be also necessary to put such an experience side by side with the political will to develop public debates and to extend the roles of the Commission Nationale du Débat Public ("Public Debate National Commission").

  6. TN International and ITS operational feedback regarding the decommissioning of obsolete casks dedicated to the transport and/or storage of nuclear raw materials, fuel and used fuel

    SciTech Connect

    Blachet, L.; Bimet, F.; Rennesson, N.

    2008-07-01

    Within the AREVA group, TN International is a major actor regarding the design of casks and transportation for the nuclear cycle. In the early 2005, TN International has started the project of decommissioning some of its own equipment and was hence the first company ever in the AREVA Group to implement this new approach. In order to do so, TN International has based this project by taking into account the AREVA Sustainable Development Charter, the French regulatory framework, the ANDRA (Agence Nationale pour la Gestion des Dechets Radioactifs - National Agency for the radioactive waste management) requirements and has deployed a step by step methodology such as radiological characterization following a logical route. The aim was to define a standardized process with optimized solutions regarding the diversity of the cask's fleet. As a general matter, decommissioning of nuclear casks is a brand new field as the nuclear field is more familiar with the dismantling of nuclear facilities and/or nuclear power plant. Nevertheless existing workshops, maintenance facilities, measurements equipments and techniques have been exploited and adapted by TN International in order to turn an ambitious project into a permanent and cost-effective activity. The decommissioning of the nuclear casks implemented by TN International regarding its own needs and the French regulatory framework is formalized by several processes and is materialized for instance by the final disposal of casks as they are or in ISO container packed with cut-off casks and big bags filled with crushed internal cask equipments, etc. The first part of this paper aims to describe the history of the project that started with a specific environmental analysis which took into account the values of AREVA as regards the Sustainable Development principles that were at the time and are still a topic of current concern in the world. The second part will deal with the definition, the design and the implementation of the

  7. Interdisciplinary and transboundary approach of geohistorical reconstruction of the floods in the Rhine Graben (1400 - 2010)

    NASA Astrophysics Data System (ADS)

    Martin, Brice; Ansel, Romain; Guerrouah, Ouarda; With, Lauriane; -Chenel, Karine Dietrich; Vitoux, Marie-Claire; Glaser, Rudiger; Drescher, Axel; Himmelsbach, Iso

    2010-05-01

    Because of its turbulent history, Alsace is one of French regions where the historic floods are the most underestimated. The damages connected to the wars (on 1870, 1914 - 1918, 1939 - 1945), the particular classification of archives and, especially, their writing in German during several periods of the recent history, is rebuffing numerous specialists Located in the same geographical area (the Rhine Graben), but by the other side of the the border constituted by the Rhine, the land of Bade is, him too, confronted with the problem of the misunderstanding of the historic floods, because of the destructions of the war also, but especially because of the harmful absence, for archives production, of a strong centralized state until the German unification after 1870. Hence the idea to set up a interdisciplinary French - German research program, to establish compared floods chronologies over several centuries in the Rhine Graben, both in France and in Germany, by associating historians, geographers, anthropologists and specialists of the languages from the universities of Mulhouse (France) and Freiburg in Breisgau (Germany). This program (called "TRANSRISK" 2008 - 2010), financed by the « Agence Nationale de la Recherche » and the « Deutsche Forschungsgemeinschaft , has multiple objectives: - filling the gaps in the knowledge of the floods in France and in Germany - building a common geohistory of the floods - optimizing the prevention and the information about the floods, thanks to the classification, the reconstruction and the mapping of the extreme phenomena - understanding the role of rivers developments responsible for an different floods evolution on both sides of the Rhine - contributing to the implementation of flood risk observatories on a French - German basis - contributing to define a common interdisciplinary vocabulary on risks (and a french - german - english glossary ). These works join the logic of the "European Directive 2007/60/EC on the assessment

  8. Telemedicine: what framework, what levels of proof, implementation rules.

    PubMed

    Zannad, Faiez; Maugendre, Philippe; Audry, Antoine; Avril, Carole; Blaise, Lucile; Blin, Olivier; Burnel, Philippe; Falise-Mirat, Béatrice; Girault, Danièle; Giri, Isabelle; Goehrs, Jean-Marie; Lassale, Catherine; Le Meur, Roland; Leurent, Pierre; Ratignier-Carbonneil, Christelle; Rossignol, Patrick; Satonnet, Evelyne; Simon, Pierre; Treluyer, Laurent

    2014-01-01

    The concept of telemedicine was formalised in France in the 2009 "Hospital, patients, health territories" (loi hôpital, patients, santé, territoire) law and the 2010 decree through which it was applied. Many experiments have been carried out and the regulatory institutions (Ministry, Regional Health Agency [Agence régionale de santé, ARS], French National Health Authority [Haute autorité de santé, HAS], etc.) have issued various guidance statements and recommendations on its organisation and on the expectations of its evaluation. With this background, the round table wanted to produce recommendations on different areas of medical telemonitoring (the role of telemonitoring, the regulatory system, the principles for assessment, methods of use and conditions for sustained and seamless deployment). Whilst many studies carried out on new medical telemonitoring approaches have led to the postulate that it offers benefit, both clinically and in terms of patient quality of life, more information is needed to demonstrate its impact on the organisation of healthcare and the associated medico-economic benefit (criteria, methods, resources). Similarly, contractual frameworks for deployment of telemonitoring do exist, although they are complicated and involve many different stakeholders (Director General fo the Care Offering [Direction générale de l'offre de soins, DGOS], ARS, HAS, Agency for Shared Health Information Systems [Agence des systèmes d'information partagés de santé, ASIP], French National Data Protection Commission [Commission nationale informatique et libertés, CNIL], French National Medical Council [Conseil national de l'Ordre des médecins, CNOM], etc.) that would benefit from a shared approach and seamless exchange between the partners involved. The current challenge is also to define the conditions required to validate a stable economic model in order to promote organisational change. One topical issue is placing the emphasis on its evaluation and

  9. Seasonal forecasting for water resource management: the example of CNR Genissiat dam on the Rhone River in France

    NASA Astrophysics Data System (ADS)

    Dommanget, Etienne; Bellier, Joseph; Ben Daoud, Aurélien; Graff, Benjamin

    2014-05-01

    Compagnie Nationale du Rhône (CNR) has been granted the concession to operate the Rhone River from the Swiss border to the Mediterranean Sea since 1933 and carries out three interdependent missions: navigation, irrigation and hydropower production. Nowadays, CNR generates one quarter of France's hydropower electricity. The convergence of public and private interests around optimizing the management of water resources throughout the French Rhone valley led CNR to develop hydrological models dedicated to discharge seasonal forecasting. Indeed, seasonal forecasting is a major issue for CNR and water resource management, in order to optimize long-term investments of the produced electricity, plan dam maintenance operations and anticipate low water period. Seasonal forecasting models have been developed on the Genissiat dam. With an installed capacity of 420MW, Genissiat dam is the first of the 19 CNR's hydropower plants. Discharge forecasting at Genissiat dam is strategic since its inflows contributes to 20% of the total Rhone average discharge and consequently to 40% of the total Rhone hydropower production. Forecasts are based on hydrological statistical models. Discharge on the main Rhone River tributaries upstream Genissiat dam are forecasted from 1 to 6 months ahead thanks to multiple linear regressions. Inputs data of these regressions are identified depending on river hydrological regimes and periods of the year. For the melting season, from spring to summer, snow water equivalent (SWE) data are of major importance. SWE data are calculated from Crocus model (Météo France) and SLF's model (Switzerland). CNR hydro-meteorological forecasters assessed meteorological trends regarding precipitations for the next coming months. These trends are used to generate stochastically precipitation scenarios in order to complement regression data set. This probabilistic approach build a decision-making supports for CNR's water resource management team and provides them with

  10. Peripheral arterial obliterative disease. Cost of illness in France.

    PubMed

    Montron, A; Guignard, E; Pelc, A; Comte, S

    1998-01-01

    The main purpose of this study, carried out in 1995, was to determine, using available sources, the cost of peripheral arterial obliterative disease (PAOD) in France over a 1-year period. This cost-of-illness study was based on a retrospective analysis of the available literature and databases. It involved a description of epidemiological data and a cost estimate of the different medical resources consumed over 1 year. For this latter purpose, a payer perspective was chosen. Data were extracted from national representative surveys and databases with respect to morbidity and mortality [from the National Institute of Health and Medical Research (Institut National de la Santé et de la Recherche Médicale; INSERM) and the National Sickness Insurance Fund for Salaried People (Caisse Nationale d'Assurance Maladie des Travailleurs Salariés; CNAMTS)], consultations, examination tests and drug prescriptions [from the French Medical Audit conducted by Intercontinental Medical Statistics (IMS)], hospitalisations [from the Statistical Unit of the Department of Health-Service des Statistiques, des Etudes et des Systemes d'Information (SESI) and the National Public Research Centre in Health Economics (Centre de Recherche d'Etude et de Documentation en Economie de la Santé; CREDES)] and related health expenditure from CNAMTS. In France, the prevalence of stage II PAOD (Leriche and Fontaine classification) in 1992 was estimated to be 675,000; 53% of these patients had undergone vascular or bypass surgery. The total annual cost of healthcare (including consultations, drugs, laboratory tests, hospitalisation and hydrotherapy) for the management of patients with PAOD ranged from 3.9 billion French francs (F) to F4.6 billion (1995 values), depending on the type of hospital considered. 50% of this cost was related to hospitalisations and 75% was covered by the CNAMTS. Although this study was only a partial evaluation and did not take into account indirect costs or nonmedical direct

  11. Mise à jour sur la prévention et le dépistage selon l’âge à l’intention des médecins de soins primaires canadiens

    PubMed Central

    Shimizu, Tawnya; Bouchard, Manon; Mavriplis, Cleo

    2016-01-01

    Résumé Objectif Faire la synthèse des meilleures lignes directrices fondées sur des données probantes concernant la prévention et le dépistage chez les adultes canadiens selon l’âge. Qualité des données Les recommandations du Groupe d’étude canadien sur les soins de santé préventifs représentent la source principale des renseignements et sont complétées par les recommandations pertinentes du Preventive Services Task Force des États-Unis lorsque celles du Groupe d’étude canadien étaient inaccessibles ou désuètes. Les guides de pratique des principales organisations nationales axées spécifiquement sur une maladie ou une spécialité ont aussi fait l’objet d’une révision pour prendre en compte les données factuelles les plus récentes. Message principal Les interventions de dépistage recommandées selon l’âge et le sexe sont présentées dans un tableau de synthèse où est mise en évidence la qualité des données à l’appui de ces recommandations. Un exemple de modèle à suivre dans les dossiers médicaux électroniques ou sur papier est aussi proposé. Conclusion Qu’il s’agisse d’une visite consacrée à la prévention ou d’une occasion saisie autrement de faire du counseling et du dépistage de prévention chez leurs patients, les médecins de soins primaires peuvent se servir de cette synthèse des recommandations fondées sur des données probantes pour maximiser leur efficience et prévenir d’importantes omissions ou des dépistages inutiles.

  12. [From Crex mutualisation to clinical audit].

    PubMed

    Debouck, F; Petit, H-B; Lartigau, E

    2010-10-01

    In mid-2004, following a Mission nationale d'expertise et d'audits hospitaliers (MeaH) proposal, three voluntary cancer centres started setting up a safety procedure in radiotherapy. Their work made it possible to single out the need to continue elaborating a repository, aiming at a "minimal written reference", to take into account the human factor as one of the four families of factors contributing to a systemic deviation and to build collectively, in radiotherapy departments, the experience feedback committee (comité de retour d'expérience [Crex]). Formalizing a comité de retour d'expérience is unavoidable in any safety-management system (SMM or MGS). The comité de retour d'expérience enables every active member of a department to listen to any of the events of the month (incidents and precursors), to select the event which will be under scrutiny for the next systemic analysis (Orion(©) method) and above all to choose the most appropriate correcting action and ensure its proper implementation. That approach has been approved and then acknowledged by the Autorité de sûreté nucléaire (ASN) before being extended to the other radiotherapy departments. The use of the comité de retour d'expérience, which is a safety management tool, should not be limited to a local circle of insiders, but shared to benefit everybody. Putting comité de retour d'expérience together - a move that was hoped for and brought up as soon as the tool was created - is now being implemented. Several initiatives have already permitted to assess its collective interest; other steps have yet to be taken to enable a true collective sharing of experience. On this basis, the definition of quality/safety practices in radiotherapy will allow the professionals to implement clinical audits in 2012. PMID:20729118

  13. Fixedwing UAV soundings of the boundary layer during the ScaleX 2015 summer campaign in southern Germany

    NASA Astrophysics Data System (ADS)

    Philipp, Andreas; Groos, Alexander; Petersen, Erik; Bischoff, Julian; Szogs, Sebastian; Beck, Christoph; Hähner, Jörg; Jacobeit, Jucundus

    2016-04-01

    In order to examine the potential to close the local water cycle budget and to evaluate models on different scales (among other aims) a fleet of 6 fixed wing UAVs has been operated by the Institute for Geography and the Institute for Informatics of the University of Augsburg during the ScaleX measurement campaign of the KIT/IMK-IFU (Karlsruher Institut für Technologie/Institut für Meteorologie und Klimatologie, Garmisch Partenkirchen). The site is located in southern Germany in a rural, hilly landscape at a small catchment tributing to the Ammersee and equipped with several ground based and remote sensing hydrological instruments. In order to complement these instruments by in situ measurements of the boundary layer, three intensive observation periods (IOPs) for taking temperature and humidity profiles took place, each with a different set up in order to evaluate optimal operation modes. The UAVs are all operated by the open hardware Apogee autopilot and sensor controller developed by ENAC (Ecole Nationale de l'Aviation Civile, Toulouse) operated by the PPRZ open source software package. The first IOP (30.06.-01.07.2015) was an experiment to cover a small site of 500 by 500 meters (well-apointed with hydrological instruments) in a 24 hours period as dense as possible. Thus three simultaneous helical profile flights (radius 70 m) have been run at each full hour around three different centres with heights ranging up to 1000 m above ground level (with special permissions). During a second IOP (15.07.2015) it has been tried to increase the frequence of profile flights up to 2 flights per hours between 7:30 and 14:00 CEST. These soundings have been accompanied by flyovers of a manned ultra light aircraft of the IMK-IFU. Finally a third experiment (06.08.2015) tried to evaluate longer flights (up to 55 minutes) of two UAVs at constant levels of 300 and 500 m above ground level between 6:00 and 14:00 CEST in order to cover the early diurnal cycle even more constantly

  14. Opinion of the Scientific Committee on Consumer Safety (SCCS) - Revision of the opinion on o-Phenylphenol, Sodium o-phenylphenate and Potassium o-phenylphenate (OPP), in cosmetic products.

    PubMed

    Scientific Committee On Consumer Safety Sccs; Bernauer, Ulrike

    2016-08-01

    o-Phenylphenol, Sodium o-phenylphenate, Potassium o-phenylphenate, CAS n. 90-43-7, 132-27-4, 13707-65-8 as preservatives are regulated in Annex V/7 of the Cosmetics Regulation (EC) n. 1223/2009 at a maximum concentration of 0.2% (as phenol). In February 2013, the Commission received a risk assessment submitted by the French Agency ANSM (Agence nationale de sécurité des médicaments et des produits de santé) which rose concerns about the use of o-Phenylphenol as preservatives in cosmetic products. In the context of the ANSM report (Evaluation du risque lié à l'utilisation de l'orthophénylphénol CAS n. 90-43-7 dans les produits cosmétiques) o-Phenylphenol has been identified as likely to be an endocrine disruptor. The report concludes that the maximum authorised concentration (currently of 0.2%) of o-Phenylphenol for use as a preservative should be revised due to low margin of safety. In January 2014, in response to a call for data on o-Phenylphenol by the Commission, Industry submitted a safety dossier in order to defend the current use of o-Phenylphenol, Sodium o-phenylphenate, Potassium o-phenylphenate, CAS n. 90-43-7, 132-27-4, 13707- 65-8 as preservatives in cosmetic formulations at a maximum concentration of 0.2% (as phenol). o-Phenylphenol as preservative with a maximum concentration of 0.2% in leave-on cosmetic products is not safe. Also, in view of further exposures including noncosmetic uses (see Anses, 2014), the maximum concentration of o-Phenylphenol in leave-on cosmetic products should be lowered. However, the proposed maximum use concentration of up to 0.15% by the applicant can be considered safe. The use of o-Phenylphenol as preservative with a maximum concentration of 0.2% in rinse-off cosmetic products is considered safe. Based on the information provided, no conclusions of safe use can be drawn for Sodium o-phenylphenate and Potassium o-phenylphenate. In vitro data indicate an absent or very weak binding affinity of OPP to the oestrogen

  15. The physics, performance and predictions of the PEGASES ion-ion thruster

    NASA Astrophysics Data System (ADS)

    Aanesland, Ane

    2014-10-01

    . This work received financial state aid managed by the Agence Nationale de la Recherche under the reference ANR-2011-BS09-40 (EPIC) and ANR-11-IDEX-0004-02 (Plas@Par).

  16. Les campagnes de dépistage du VIH, une stratégie efficace pour l’accès universel à la prévention et au traitement ? L’expérience du Burkina Faso

    PubMed Central

    Somé, J.F.; Desclaux, A.; Ky-Zerbo, O.; Lougué, M.; Kéré, S.; Obermeyer, C.; Simaga, F.

    2014-01-01

    Objectifs l’augmentation du taux de personnes qui connaissent leur statut VIH est un impératif, notamment en Afrique subsaharienne, ce qui impose d’évaluer les stratégies utilisées pour accroître la fréquentation des services de dépistage. Cet article vise à faire le bilan de la pertinence, de la faisabilité et de l’efficacité des campagnes nationales de dépistagemenées entre 2006 et 2010 au Burkina Faso. Méthodologie une analyse de toutes les données de fréquentation du conseil dépistage sur cette période a été faite, couplée à des entretiens avec les principaux acteurs intervenant dans le dépistage. Résultats les résultats montrent que les huit campagnes de dépistage organisées sur la période ont permis à 487 727 personnes de faire leur test VIH. Ce nombre représente 50 % du nombre total de personnes ayant fait leur test et contribue à hauteur de 24,6 % au dépistage des personnes séropositives identifiées au cours de cette période. Les campagnes ont touché des populations difficiles à atteindre (en particulier les jeunes), à un coût moindre. Conclusions cette stratégie est donc pertinente pour identifier les personnes VIH+. Son intérêt pour la prévention, important selon les soignants et au vu des populations jeunes qui y participent, devrait être mesuré par des études complémentaires. Les campagnes sont efficaces et coût-efficaces même dans un pays de niveau de prévalence faible. Ces résultats soulignent l’intérêt de la synergie entre les associations et les services de santé dans l’offre de services de conseil et dépistage. PMID:24681563

  17. The Use of Meteosat Second Generation Satellite Data Within A New Type of Solar Irradiance Calculation Scheme

    NASA Astrophysics Data System (ADS)

    Mueller, R. W.; Beyer, H. G.; Cros, S.; Dagestad, K. F.; Dumortier, D.; Ineichen, P.; Hammer, A.; Heinemann, D.; Kuhlemann, R.; Olseth, J. A.; Piernavieja, G.; Reise, C.; Schroedter, M.; Skartveit, A.; Wald, L.

    1-University of Oldenburg, 2-University of Appl. Sciences Magdeburg, 3-Ecole des Mines de Paris, 4-University of Bergen, 5-Ecole Nationale des Travaux Publics de l'Etat, 6-University of Geneva, 7-Instituto Tecnologico de Canarias, 8-Fraunhofer Institute for Solar Energy Systems, 9-German Aerospace Center Geostationary satellites such as Meteosat provide cloud information with a high spatial and temporal resolution. Such satellites are therefore not only useful for weather fore- casting, but also for the estimation of solar irradiance since the knowledge of the light reflected by clouds is the basis for the calculation of the transmitted light. Additionally an the knowledge of atmospheric parameters involved in scattering and absorption of the sunlight is necessary for an accurate calculation of the solar irradiance. An accurate estimation of the downward solar irradiance is not only of particular im- portance for the assessment of the radiative forcing of the climate system, but also necessary for an efficient planning and operation of solar energy systems. Currently, most of the operational calculation schemes for solar irradiance are semi- empirical. They use cloud information from the current Meteosat satellite and clima- tologies of atmospheric parameters e.g. turbidity (aerosols and water vapor). The Me- teosat Second Generation satellites (MSG, to be launched in 2002) will provide not only a higher spatial and temporal resolution, but also the potential for the retrieval of atmospheric parameters such as ozone, water vapor and with restrictions aerosols. With this more detailed knowledge about atmospheric parameters it is evident to set up a new calculation scheme based on radiative transfer models using the retrieved atmospheric parameters as input. Unfortunately the possibility of deriving aerosol in- formation from MSG data is limited. As a cosequence the use of data from additional satellite instruments ( e.g. GOME/ATSR-2) is neeeded. Within this

  18. [An archivist in a laboratory].

    PubMed

    Kulecka, A

    2000-01-01

    The article presents the results of French archival research concerning scholarly and scientific archives. The article points out that the subject-matter is of interest to historians of science and learning as well as archivists employed in research institutions. It is stressed that the concept of "scholarly/scientific archives" refers to three kinds of archives: the archives of institutions responsible for research administration, of those conducting research, as well as the archives of scholars and scientists themselves. The article presents material on the archives of the Academie des Sciences as well as other research institutions, such as the Museum d'histoire naturelle, the Conservatoire des Arts et Metiers, the Ecole Polytechnique, the Institut Pasteur and the Observatoire astronomique. Special attention is devoted to the establishment, gathering and arrangement of the archival materials of those institutions. The next part of the article deals with the issue of the archives of Polish scholars to be found in French archival literature. It identifies the places where such materials are stored and discusses the archival materials relating to Polish researchers and scholars that are stored at the library of the Institut de France, the Bibliotheque nationale, the central library of the Museum d'histoire naturelle as well as other research institutions. The next part of the article is devoted to problems of evaluating materials created in the course of currently conducted research. It is pointed out that archival material produced by the activities of research institutions consist of (i) administrative documents and (ii) documents concerned with course of research work itself. It is stressed in the article that unpublished research materials and working materials are ducuments of a very controversial kind, and do not lend themselves easily to precise and rational criteria of assessment. The article also points out that it is difficult to work out a general

  19. [Use of intravenous iron supplementation in chronic kidney disease: Interests, limits, and recommendations for a better practice].

    PubMed

    Rottembourg, Jacques; Rostoker, Guy

    2015-12-01

    Iron deficiency is an important clinical concern in chronic kidney disease (CKD), giving rise to iron-deficiency anaemia, and various impaired cellular functions. Oral supplementation, in particular with ferrous salts, is associated with a high rate of gastro-intestinal side effects and is poorly absorbed, a problem that is avoided with intravenous (IV) irons. Recently, with the approval of the European Medicines Agency's Committee for Medicinal Products for Human Use, the French Agence nationale de sécurité du médicament et des produits de santé (ANSM) took adequate measures to minimize the risk of allergic reactions, by correction on the summary of intravenous iron products characteristics. All IV iron products should be prescribed, administered and injected, inside public or private hospitals exclusively, and a clinical follow-up after the infusion for at least 30 minutes is mandatory. The most stable intravenous iron complexes (low molecular weight iron dextran, ferric carboxymaltose, and iron isomaltoside 1000 [under agreement]) can be given in higher single doses and more rapidly than less recent preparations such as iron sucrose (originator or similars). Test doses are advisable for conventional low molecular weight iron dextrans, but are no more mandatory. Iron supplementation is recommended for all CKD patients with iron-deficiency anaemia and those who receive erythropoiesis-stimulating agents, whether or not they require dialysis. Intravenous iron is the preferred route of administration in haemodialysis patients, with randomized trials showing a significantly greater increase in haemoglobin levels for intravenous versus oral iron and a low rate of treatment-related adverse events during these trials. According ANSM, physicians should apply the product's label recommendations especially the posology. In the non-dialysis CKD population, the erythropoietic response is also significantly higher using intravenous versus oral iron, and tolerability is at

  20. Southern Tunisia as an example of international partnership in cultural and geological heritage conservation

    NASA Astrophysics Data System (ADS)

    Contessi, M.; Cantelli, L.; Fanti, F.; Gabbianelli, G.; Mohsen, H.

    2012-04-01

    National Geoparks initiatives are essential strategies to enhance the value of Earth's heritage and to promote a regional sustainable socio-economic and cultural development. As an example for geological heritage development, an ongoing partnership between the Department of Geological and Environmental Sciences of the University of Bologna (Italy) and the Office Nationales des Mines (Tunisia) attempt to ensure divulgation and preservation of the geological, geomorphological and archeological values of the Tataouine region in South Tunisia, with the final goal to create a Geopark. In this region, different environmental and cultural heritages that comprehend paleontology, geomorphology, stratigraphy and archeology coexist. Mesozoic beds that crop out extensively in the Tataouine region known since the beginning of the 20th century as Continental Intercalaire, yield numerous dinosaur and other vertebrate remains as well as tracksites. Moreover these Mesozoic deposits have been intensively modified for centuries by the local populations who created complex systems of artificial terraces, called jessour, in order to retain rainwater in the arid Tunisian climate and to exploit the scarce farm soil. These human artifacts deeply modified the morphological and hydrogeological landscape and created a unique cultural value that need to be preserved. From the perspective of science and conservation, a well-documented geological inventory of the fossiliferous sites has been produced and will be available as an electronic database. In particular, the Beni Ghedir valley, near the Goumrassene village, has been chosen has the main Geopark location as it includes, in a restricted area, a perfect example of jessour artifacts together with some well-preserved Ksour (ancient storage structures) and nicely preserved fossil sites. An interactive map of the artificial terrances has been produced using the ArcGis technology, in order to highlight the connection between the valley

  1. Alfred Vulpian and Jean-Martin Charcot in each other's shadow? From Castor and Pollux at La Salpêtrière to neurology forever.

    PubMed

    Bogousslavsky, Julien; Walusinski, Olivier; Moulin, Thierry

    2011-01-01

    While Alfred Vulpian (1826-1887) is not completely forgotten, he cannot match the uninterrupted celebrity which Jean-Martin Charcot (1825-1893) still enjoys today. After becoming interne (residents) at the same institute in 1848, both were involved in shaping the cradle of what would become modern neurology. Both started work as chiefs at a La Salpêtrière service on January 1, 1862, making common rounds and studies, with several common publications. While their friendship remained 'for life', as stated by Charcot at Vulpian's funeral, their career paths differed. Vulpian progressed quicker and higher, being appointed full professor and elected at the Académie Nationale de Médecine and the Académie des Sciences several years before Charcot, as well as becoming dean of the Paris Faculty of Medicine. These positions also enabled him to support his friend Charcot in getting appointed full clinical professor and becoming the first holder of the chair of Clinique des Maladies du Système Nerveux in 1882. Before studying medicine, Vulpian had worked in physiology with Pierre Flourens, and his career always remained balanced between physiology and neurology, with remarkable papers. He introduced Charcot to optic microscopy during their La Salpêtrière years, indirectly helping him to become his successor to the chair of pathological anatomy in 1872. While Vulpian succeeded so well in local medical affairs, Charcot spent his time building up a huge clinical service and a teaching 'school' at La Salpêtrière, which he never left for over 31 years until his death. This 'school' progressively became synonymous with clinical neurology itself and perpetuated the master's memory for decades. Vulpian never had such support, although Jules Déjerine was his pupil and Joseph Babinski was his interne before becoming Charcot's chef de clinique (chief of staff) in 1885. This unusual switch in Parisian medicine contributed to Charcot's unaltered celebrity over more than a century

  2. Médecine des voyages

    PubMed Central

    Aw, Brian; Boraston, Suni; Botten, David; Cherniwchan, Darin; Fazal, Hyder; Kelton, Timothy; Libman, Michael; Saldanha, Colin; Scappatura, Philip; Stowe, Brian

    2014-01-01

    Résumé Objectif Définir la pratique de la médecine des voyages, présenter les éléments fondamentaux d’une consultation complète préalable aux voyages à des voyageurs internationaux et aider à identifier les patients qu’il vaudrait mieux envoyer en consultation auprès de professionnels de la médecine des voyages. Sources des données Les lignes directrices et les recommandations sur la médecine des voyages et les maladies liées aux voyages publiées par les autorités sanitaires nationales et internationales ont fait l’objet d’un examen. Une recension des ouvrages connexes dans MEDLINE et EMBASE a aussi été effectuée. Message principal La médecine des voyages est une spécialité très dynamique qui se concentre sur les soins préventifs avant un voyage. Une évaluation exhaustive du risque pour chaque voyageur est essentielle pour mesurer avec exactitude les risques particuliers au voyageur, à son itinéraire et à sa destination et pour offrir des conseils sur les interventions les plus appropriées en gestion du risque afin de promouvoir la santé et prévenir les problèmes médicaux indésirables durant le voyage. Des vaccins peuvent aussi être nécessaires et doivent être personnalisés en fonction des antécédents d’immunisation du voyageur, de son itinéraire et du temps qu’il reste avant son départ. Conclusion La santé et la sécurité d’un voyageur dépendent du degré d’expertise du médecin qui offre le counseling préalable à son voyage et les vaccins, au besoin. On recommande à ceux qui donnent des conseils aux voyageurs d’être conscients de l’ampleur de cette responsabilité et de demander si possible une consultation auprès de professionnels de la médecine des voyages pour tous les voyageurs à risque élevé.

  3. Aspects épidémiologiques des fractures de membres liées à l'exercice de la fonction militaire au Togo

    PubMed Central

    Akpoto, Yao Messanvi; Abalo, Anani; Gnandi-pio, Faré; Sonhaye, Lantam; Tchaou, Mazamaesso; Sama, Hamza Doles; Assenouwe, Sarakawabalo; Lamboni, Damessane; Amavi, Kossigan Adodossi; Adam, Saliou; Kpelao, Essossinam; Tengue, Kodjo; Songne-Gnamkoulamba, Badjona

    2015-01-01

    Le but de notre étude était de déterminer la fréquence des fractures de membres liées à l'exercice de la fonction militaire au sein des Forces de Défense et de Sécurité en milieu africain en vue de ressortir l'impact des différentes circonstances de survenue. Nous avons entrepris une étude rétrospective descriptive allant du 1er janvier 2004 au 31 décembre 2013. Elle a concerné les agents des forces de défense et de sécurité traités pour des fractures de membres au cours de cette période. Sept cent quatre (704) cas de fractures de membres ont été dénombrés. L’âge moyen des patients était de 30,57 ans avec des extrêmes de 19 et 55 ans. La prédominance masculine était nette (95,71%). L'Armée de Terre (51,05%) et la Gendarmerie Nationale (38,86%) étaient les plus représentées. Les hommes du rang étaient majoritaires (43,08%), suivis des sous-officiers (32,59%). La fréquence annuelle des fractures de membres en rapport avec la profession militaire était de 63 cas. Les fractures de jambe étaient les lésions les plus recensées (32,96%). Les Formations et les stages militaires ont été les circonstances de survenue les plus rencontrées (42,60%), suivies des accidents de la circulation (39,43%). La perte des journées de service liée à ces lésions était estimée à 14009 jours par an. Les fractures de jambes occupent le premier rang des fractures de membres en rapport avec l'exercice de la profession militaire. Les formations-stages militaires et les accidents de la voie publique en sont les deux grandes circonstances de survenue. PMID:27081434

  4. Leiomyosarcome de la langue: à propos d'un cas

    PubMed Central

    El jahd, Lahcen; Barhmi, Ismail; Tazi, Nabil; Rouadi, Sami; Abada, Reda; Roubal, Mohammed; janah, Abdelaziz; Mahtar, Mohammed

    2015-01-01

    Le léiomyosarcome primitif de la langue est une tumeur rare qui se développe aux dépens des fibres musculaires lisses. Le diagnostic est souvent difficile, fondé sur des caractéristiques immuno-histologiques particulières. L'objectif de ce travail est de décrire le profil épidémiologique, clinique, thérapeutique et évolutif du léiomyosarcome à travers un cas et une revue de la littérature. Nous rapportons le cas d'un homme âgé de 26 ans, sans antécédents pathologique particuliers, consultant pour une tuméfaction de la langue mobile évoluant depuis 2 ans. Une biopsie de la masse a été réalisée. L’étude anatomopathologique et immunohistochimique a confirmé le diagnostic d'un léiomyosarcome de la langue. L'IRM de la langue a objectivé un processus lesionnel intéressant la portion mobile et antérieur de la langue. Une exérèse de la masse a été réalisée. L'examen histologique a montré la présence d'un large néoplasme de 6 cm compatible à un léiomyosarcome peu différencié de la langue, de garde II selon la Fédération Nationale des Centres de Lutte Contre le Cancer (FNCLCC). Une radiothérapie externe sur la cavité buccale avec une dose de 65 Gy a été réalisée. Le patient a présenté 2 mois après la fin du traitement une adénopathie latéro-cervicale haute gauche (territoire II), il a bénéficié d'un curage ganglionnaire fonctionnel intéressant les territoires I, II et III puis réadressé en radiothérapie. Le léiomyosarcome de la langue est très rare surtout chez le sujet jeune. La chirurgie et la radiothérapie sont les armes thérapeutiques majeures. Le pronostic est très mauvais, Les facteurs les plus importants sont les marges d'exérèse et le grade. PMID:26600908

  5. Long Period (LP) volcanic earthquake source location at Merapi volcano by using dense array technics

    NASA Astrophysics Data System (ADS)

    Metaxian, Jean Philippe; Budi Santoso, Agus; Laurin, Antoine; Subandriyo, Subandriyo; Widyoyudo, Wiku; Arshab, Ghofar

    2015-04-01

    Since 2010, Merapi shows unusual activity compared to last decades. Powerful phreatic explosions are observed; some of them are preceded by LP signals. In the literature, LP seismicity is thought to be originated within the fluid, and therefore to be representative of the pressurization state of the volcano plumbing system. Another model suggests that LP events are caused by slow, quasi-brittle, low stress-drop failure driven by transient upper-edifice deformations. Knowledge of the spatial distribution of LP events is fundamental for better understanding the physical processes occurring in the conduit, as well as for the monitoring and the improvement of eruption forecasting. LP events recorded at Merapi have a spectral content dominated by frequencies between 0.8 and 3 Hz. To locate the source of these events, we installed a seismic antenna composed of 4 broadband CMG-6TD Güralp stations. This network has an aperture of 300 m. It is located on the site of Pasarbubar, between 500 and 800 m from the crater rim. Two multi-parameter stations (seismic, tiltmeter, S-P) located in the same area, equipped with broadband CMG-40T Güralp sensors may also be used to complete the data of the antenna. The source of LP events is located by using different approaches. In the first one, we used a method based on the measurement of the time delays between the early beginnings of LP events for each array receiver. The observed differences of time delays obtained for each pair of receivers are compared to theoretical values calculated from the travel times computed between grid nodes, which are positioned in the structure, and each receiver. In a second approach, we estimate the slowness vector by using MUSIC algorithm applied to 3-components data. From the slowness vector, we deduce the back-azimuth and the incident angle, which give an estimation of LP source depth in the conduit. This work is part of the Domerapi project funded by French Agence Nationale de la Recherche (https

  6. Characterization of Heat Waves in the Sahel and associated mechanisms

    NASA Astrophysics Data System (ADS)

    Oueslati, Boutheina; Pohl, Benjamin; Moron, Vincent; Rome, Sandra

    2016-04-01

    Large efforts are made to investigate the heat waves (HW) in developed countries because of their devastating impacts on society, economy and environment. This interest increased after the intense event over Europe during summer 2003. However, HWs are still understudied over developing countries. This is particularly true in West Africa, and especially in the Sahel, where temperatures recurrently reach critical values, such as during the 2010 HW event. Understanding the Sahelian HWs and associated health risks constitute the main objective of ACASIS, a 4-year project funded by the French Agence Nationale de la Recherche. Our work contributes to this project and aims at characterizing the Sahelian HWs and understanding the mechanisms associated with such extreme events. There is no universal definition of a HW event, since it is highly dependent on the sector (human health, agriculture, transport...) and region of interest. In our case, a HW is defined when the heat index of the day and of the night exceeds the 90th percentile for at least 3 consecutive days (Rome et al. 2016, in preparation). This index combines temperature and relative humidity in order to determine the human-perceived equivalent temperature (definition adapted from Steadman, 1979). Intrinsic properties of Sahelian HW are analyzed from the Global Summary of the Day (GSOD) synoptic observations and ERA-interim reanalyses over 1979-2014 during boreal spring seasons (April-May-June), the warmest period of the year in the Central Sahel. ERA-interim captures well the observed interannual variability and seasonal cycle at the regional scale, as well as the 1979-2014 increasing linear trend of springtime HW occurrences in the Sahel. Reanalyses, however, overestimate the duration, spatial extent of HW, and underestimate their intensity. For both GSOD and ERA-interim, we show that, over the last three decades, Sahelian HWs tend to become more frequent, last longer, cover larger areas and reach higher

  7. Evaluation de la sécurité du circuit des médicaments anticancéreux dans un hôpital régional en Tunisie

    PubMed Central

    Sahli, Jihène; El Ghardallou, Meriam; Bougmiza, Iheb; Henchiri, Besma; Limam, Manel; Mejdoub, Rim; Mtiraoui, Ali; Ajmi, Thouraya

    2016-01-01

    Introduction Parmi les événements indésirables, ceux liés au circuit des médicaments occupent une place importante et risquent de causer un préjudice grave aux patients. Dans ce contexte, nous avons mené cette étude dans l'optique de décrire et d’évaluer le circuit des médicaments anticancéreux dans un hôpital régional tunisien. Méthodes Il s'agit d'une étude évaluative du risque lié aux médicaments anticancéreux, type « visite de risque » menée sur une période de 15 jours au cours de l'année 2014 au service de cancérologie de l'hôpital régional de Gafsa (Tunisie). Cette méthode d’évaluation est inspirée de celle conduite par le projet « SECURIMED » développé par le Comité de Coordination de l'Evaluation Clinique et de la Qualité en Aquitaine (CCECQA), en France. Résultats Dans notre étude, l'observation du circuit des médicaments anticancéreux a révélé certaines insuffisances. On a noté que la répartition des missions des différents acteurs est sujette parfois à des glissements de tâches. Un manque important ainsi que une inadéquation aux normes au niveau des équipements nécessaires pour la préparation et la protection des professionnels manipulant ces médicaments ont été également décelés. Conclusion La sécurisation du circuit des médicaments devrait être une priorité inscrite dans l'ensemble des démarches nationales et partagée par tous les intervenants et ce dans l'optique d'atteindre un objectif prémium: la qualité de la prise en charge globale et la sécurité des patients. PMID:27200135

  8. Vaccination: Developing and implementing a competency-based-curriculum at the Medical Faculty of LMU Munich

    PubMed Central

    Vogel, B.; Reuter, S.; Taverna, M.; Fischer, M. R.; Schelling, J.

    2016-01-01

    Background: In Germany medical students should gain proficiency and specific skills in the vaccination field. Especially important is the efficient communication of scientific results about vaccinations to the community, in order to give professional counseling with a complete overview about therapeutic options. Aim of the project: The aim of this project is to set up a vaccination-related curriculum in the Medical Faculty at the Ludwig-Maximilians-University in Munich. The structure of the curriculum is based on the National catalogue for competency-based learning objectives in the field of vaccination (Nationaler Kompetenzbasierter Lernzielekatalog Medizin NKLM). Through this curriculum, the students will not only acquire the classical educational skills concerning vaccination in theory and practice, but they will also learn how to become independent in the decision-making process and counseling. Moreover, the students will become aware of consequences of action related to this specific topic. Methods: According to defined guidelines, an analysis was performed on courses, which are currently offered by the university. A separate analysis of the NKLM was carried out. Both analyses identified the active courses related to the topic of vaccination as well as the NKLM learning objectives. The match between the topics taught in current courses and the NKLM learning objectives identified gaps concerning the teaching of specific content. Courses were modified in order to implement the missing NKLM learning objectives. Results: These analyses identified 24 vaccination-related courses, which are currently taught at the University. Meanwhile, 35 learning objectives on vaccination were identified in the NKLM catalogue. Four of which were identified as not yet part of the teaching program. In summary, this interdisciplinary work enabled the development of a new vaccination-related curriculum, including 35 learning objectives, which are now implemented in regular teaching

  9. Le Laboratoire de Mécanique Appliquée Raymond Chaléat a 40 ans !

    NASA Astrophysics Data System (ADS)

    Comité D'Organisation Du Colloque Ime 2002, Le

    2002-12-01

    Le LMARC a été créé par Raymond Chaléat dans les locaux de l'École Nationale d'Horlogerie (a présent Lycée Technique Jules Haag).L'équipe de recherche était alors constituée de 2 enseignants-chercheurs (Raymond Chaléat et Gérard Lallement) et d'un technicien (Bernard Prêtre). Les travaux de recherche se situaient naturellement dans le domaine de la chronométrie et en particulier dans la mécanique non linéaire analytique inhérente à la montre en fonctionnement. En effet, Raymond Chaléat fut l'élève, puis le collaborateur du Professeur Jules Haag, mathématicien et mécanicien, lui-même élève de Poincarré.Le LMARC a étendu ses activités avec l'arrivée de Claude Oudet, puis de Claude Oytana à la rhéologie des matériaux solides qui est devenue plus tard l'Équipe Propriétés Mécaniques des Matériaux. En parallèle, G. Lallement a créé une équipe Vibrations devenue à ce jour Dynamique des Structures. À ce jour, le Laboratoire compte plus de 110 personnes dont 40 doctorants.Il a depuis diversifié ses activités avec 3 nouvelles équipes tournées vers la Modélisation et la Mise en Forme des Matériaux, les Micromachines et la Biomécanique et les Mécanismes. Il a su également prendre toute sa place au sein de l'Institut des Microtechniques de Franche-Comté en contribuant à plusieurs thèmes.Notre Laboratoire a été l'un des premiers laboratoires associé au CNRS (4ème) et a toujours été rattaché à l'Université de Franche-Comté (Présidence par C. Oytana de 1996 a 2001) par l'entremise de I'UFR Sciences et Techniques. Il a toujours maintenu des liens forts avec I'ENSMM (École Nationale Supérieure de Mécanique et des Microtechniques) d'une part par ses enseignants-chercheurs et d'autre part deux de ses directeurs, Raymond Chaléat et actuellement Jean-Claude Gelin.En plus de ses relations constantes avec l'industrie régionale, le LMARC a développé des actions contractuelles avec de grands groupes tels que EDF

  10. Caracterisation du coefficient de retrodiffusion radar des surfaces d'hydrocarbure: Modelisation et interpretation

    NASA Astrophysics Data System (ADS)

    Charbonneau, Francois

    La surveillance maritime est un domaine d'applications ou l'interet politique et scientifique croit constamment au Canada. Un des outils privilegies pour la surveillance maritime est l'acquisition de donnees radars, par des systemes aeroportes ou spatio-portes (ERS-2, RADARSAT et Envisat). Par leur grande couverture spatiale, ainsi que leur sensibilite a la geometrie de surface, les donnees radars permettent, en autres, la detection de cibles ponctuelles (bateaux), estimation des vents, detection des glaces de mer, ainsi que la detection de deversement d'hydrocarbure. Les limites et les avantages de la detection d'hydrocarbure par acquisitions de donnees radars sont bien connus, mais il reste encore des lacunes au niveau de l'extraction des parametres physiques d'une surface d'hydrocarbure. Ce projet a pour objectif de caracteriser le coefficient de retrodiffusion radar associe a une surface d'hydrocarbure en milieu oceanique, par l'introduction d'un modele thermodynamique d'attenuation de la surface, au modele theorique radar IEM. Le modele global permet de simuler le comportement de sigma° en fonction des proprietes visco-elastiques, ainsi que de l'epaisseur de la couche d'hydrocarbure et en fonction des parametres d'acquisition radar. Le modele developpe fut valide a partir des donnees SIR-C acquises lors d'experimentations controlees. A partir des informations environnementales et du type d'hydrocarbure, notre modele a permis d'estime le contraste d'intensite avec une precision de 1 a 1,5 dB, a la bande C. Alors qu'a la bande L, l'erreur sur le contraste est d'environ 1,5 a 2 dB sur l'ensemble des mesures. Ce qui est excellant considerant l'heterogeneite des surfaces analysees. Egalement, nous effectuons des analyses multi-polarisees et polarimetriques avec les donnees SIR-C acquises au-dessus de sites experimentaux. II en ressort que le ratio de polarisation VV/HH, ainsi que le facteur d'anisotropie sont des pistes de recherche prometteuses qu'il faudra

  11. Guide de pratique clinique pour les lésions cérébrales traumatiques légères et les symptômes persistants

    PubMed Central

    Marshall, Shawn; Bayley, Mark; McCullagh, Scott; Velikonja, Diana; Berrigan, Lindsay

    2012-01-01

    Résumé Objectif Présenter les nouvelles lignes directrices sur la prise en charge des lésions cérébrales traumatiques légères (LCTL) et les symptômes persistants post-commotion (SPPC) afin de renseigner et d’orienter les médecins qui prennent en charge des patients qui se remettent d’une LCTL. Qualité des données On a effectué une recherche des guides de pratique clinique existants portant sur les LCTL et une synthèse critique des ouvrages scientifiques évaluant le traitement des SPPC. Étant donné la rareté des conseils sur la prise en charge des SPPC dans les travaux sur les lésions cérébrales traumatiques, une deuxième recherche documentaire a été faite pour recenser les guides de pratique clinique et les synthèses critiques concernant la prise en charge de ces symptômes communs dans la population en général. On a convoqué des professionnels de la santé provenant de différentes disciplines et régions du Canada et de l’étranger à une conférence consensuelle d’experts pour examiner les lignes directrices et les données probantes existantes et élaborer un guide complet pour la prise en charge des LCTL et des SPPC. Message principal À l’aide d’un processus Delphi modifié, on a produit 71 recommandations portant sur le diagnostic et la prise en charge des LCTL et des SPPC. De plus, on a inclus dans le guide de nombreuses ressources et des outils pour faciliter la mise en œuvre des recommandations. Conclusion Un guide de pratique clinique a été élaboré pour aider les professionnels de la santé à fournir des soins fondés sur les données probantes et les pratiques exemplaires à la population complexe de personnes qui ont des SPPC à la suite d’une LCTL.

  12. Aspects descriptifs du VIH/SIDA chez les sujets âgés de 50 ans et plus suivis au Centre de Traitement Agréé de Bafoussam - Cameroun

    PubMed Central

    Mbopi-Kéou, François-Xavier; Djomassi, Lucienne Dempouo; Monebenimp, Francisca

    2012-01-01

    Introduction La littérature scientifique dispose de très peu de données relatives à l’épidémiologie du VIH chez les sujets âgés en Afrique subsaharienne. Au Cameroun, les caractéristiques épidémiologiques de l'infection par le VIH chez les sujets âgés de 50 ans et plus ne sont pas documentées. Méthodes Dans une étude de cohorte rétrospective et une enquête transversale, nous avons comparé les caractéristiques clinico-biologiques et la survie post thérapeutique des patients âgés de 50 ans et plus, sous traitement antirétroviral au Centre de Traitement Agrée de Bafoussam - Cameroun, aux adultes plus jeunes. Résultats L’âge moyen était de 39 ans, les extrêmes étant 17 et 88 ans. Les sujets âgés de 50 ans et plus représentaient 14,1% des cas. Les plus âgés étaient moins bien informés sur les modes de transmission du virus (p = 0,04). Leur séropositivité au VIH était le plus souvent découverte au décours d'une infection opportuniste (p = 0,02). La fréquence de comorbidité était significativement plus élevée chez les personnes âgées de 50 ans et plus (p < 10-5). Nous n'avons pas retrouvé une association statistiquement significative entre l'observance thérapeutique et l’âge (p = 0,83). La survie post-thérapeutique n’était pas significativement liée à l’âge (p = 0,81). Conclusion Les sujets âgés ne sont pas à l'abri du VIH. La promotion du dépistage et les programmes d’éducation sanitaire relatifs au VIH/SIDA devraient être renforcés au sein de cette communauté déjà affaiblie par le poids de l’âge, afin de réduire l'incidence du SIDA et de leur assurer prise en charge précoce. PMID:23133707

  13. PAndAS' Progeny: Extending the M31 Dwarf Galaxy Cabal

    NASA Astrophysics Data System (ADS)

    Richardson, Jenny C.; Irwin, Mike J.; McConnachie, Alan W.; Martin, Nicolas F.; Dotter, Aaron L.; Ferguson, Annette M. N.; Ibata, Rodrigo A.; Chapman, Scott C.; Lewis, Geraint F.; Tanvir, Nial R.; Rich, R. Michael

    2011-05-01

    seemingly in conflict with the predictions of cosmological simulations. Based on observations obtained with the MegaPrime/MegaCam, a joint project of the Canada-France-Hawaii Telescope (CFHT) and CEA/DAPNIA, at CFHT which is operated by the National Research Council (NRC) of Canada, the Institut National des Science de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii.

  14. PAndAS' CUBS: Discovery of Two New Dwarf Galaxies in the Surroundings of the Andromeda and Triangulum Galaxies

    NASA Astrophysics Data System (ADS)

    Martin, Nicolas F.; McConnachie, Alan W.; Irwin, Mike; Widrow, Lawrence M.; Ferguson, Annette M. N.; Ibata, Rodrigo A.; Dubinski, John; Babul, Arif; Chapman, Scott; Fardal, Mark; Lewis, Geraint F.; Navarro, Julio; Rich, R. Michael

    2009-11-01

    the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  15. Cosmological Constraints from the Red-Sequence Cluster Survey

    NASA Astrophysics Data System (ADS)

    Gladders, Michael D.; Yee, H. K. C.; Majumdar, Subhabrata; Barrientos, L. Felipe; Hoekstra, Henk; Hall, Patrick B.; Infante, Leopoldo

    2007-01-01

    Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  16. Thirty New Low-mass Spectroscopic Binaries

    NASA Astrophysics Data System (ADS)

    Shkolnik, Evgenya L.; Hebb, Leslie; Liu, Michael C.; Reid, I. Neill; Collier Cameron, Andrew

    2010-06-01

    , the Centre National de la Recherche Scientifique of France, and the University of Hawaii. The WASP Consortium consists of astronomers primarily from the Queen's University Belfast, St Andrews, Keele, Leicester, The Open University, Isaac Newton Group La Palma, and Instituto de Astrofísica de Canarias. The SuperWASP Cameras were constructed and operated with funds made available from Consortium Universities and the UK's Science and Technology Facilities Council.

  17. Dark matter distribution in the merging cluster Abell 2163

    NASA Astrophysics Data System (ADS)

    Soucail, G.

    2012-04-01

    Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France and the University of Hawaii.

  18. Teens Discovering Science in the News: An Opportunity for Scientists to Communicate

    NASA Astrophysics Data System (ADS)

    Hall, Michelle; Mayhew, Michael

    2010-05-01

    Teens Discussing Science in the News: An Opportunity for Scientists to Communicate We have developed a program directed by teens and for teens to discuss current science and technology topics in the news. Modeled after the international Café Scientifique program for adults, we combine a social atmosphere with discussion of controversial topics to challenge teens to think about how science affects their lives. Our approach is for short story telling presentations during which the speaker identifies a single important idea and scientific principle to communicate. A good speaker will leave the audience with a dilemma or controversy to discuss, and with further opportunities to learn. A good speaker does not take him/herself too seriously and will work to fully engage the audience on the things that they can relate to. We integrate trivia quizzes at the beginning or the presenter questions the audience about assumptions they have about the topic. These techniques allow the presenter to gauge the knowledge level of the audience, while keeping them engaged and processing new information. We incorporate hands on learning from building model fuel cell cars, to analyzing the science in popular movies, to using Google Earth and remote sensing imagery to spy. Controversial topics such as geoengineering the climate, the role of nuclear energy and nuclear weapons, the future of hydrogen fuel cells/cars, carbon sequestration, and the nexus of water, climate and energy are often presented within a scientific, economic and social or political framework because science is only part of the solution. What we have learned is that teens begin to see science everywhere in their lives. We commonly hear the youth say - I did not know that is what geoscientists did! They learn to appreciate and can put the science they learn in school within a more relevant context. They like the challenge of finding solutions, but turn off to presentations on topics that seem to have no good solutions

  19. Une version québécoise du Sport Concussion Assessment Tool 2 (SCAT2)—Outil d'évaluation des commotions cérébrales dans le sport 2 : Québec (SCAT2-Qc)

    PubMed Central

    Boyd, Jami; Boyer-Rémillard, Marie-Eve; Pilon-Piquette, Michael; McKinley, Patricia

    2013-01-01

    RÉSUMÉ Objectif : traduire le Sport Concussion Assessment Tool 2 (SCAT2) dans la langue française parlée au Québec et en vérifier l'acceptabilité pour la population québécoise francophone. Méthodologie : le processus de traduction de la version originale du SCAT2 a fait appel à une variante de la méthode de traduction et d'adaptation d'outils proposée par l'Organisation mondiale de la santé. Une traduction parallèle a d'abord été réalisée. Ensuite, un comité a révisé cette traduction parallèle dans le but de produire une version préliminaire du SCAT2-Qc. Puis, on a procédé à une rétrotraduction parallèle, que l'on a comparée à la version originale. La version préliminaire a été modifiée. Pour parvenir à la version finale, on a intégré les suggestions et les commentaires formulés par deux sujets sains lors de l'essai de l'outil, et lors de la comparaison du SCAT2-Qc à la version française existante par trois réviseurs du domaine de la santé. On a ensuite testé la version finale du SCAT2-Qc auprès de douze sujets sains pour en vérifier l'acceptabilité. Résultats : les douze sujets sains n'ont eu aucun problème de compréhension en utilisant le SCAT2-Qc. Conclusion : les différentes étapes de traduction ont permis de créer le SCAT2-Qc. Son contenu ayant été validé, il peut à présent être utilisé dans le milieu sportif et scientifique québécois. PMID:24396168

  20. L’identification et traitement du trouble panique avec ou sans agoraphobie

    PubMed Central

    Foldes-Busque, Guillaume; Marchand, André; Landry, Pierre

    2007-01-01

    RÉSUMÉ OBJECTIF Renseigner les médecins de première ligne au sujet de l’identification précoce, du diagnostic et du traitement du trouble panique avec ou sans agoraphobie (TP/A). QUALITÉ DES DONNÉES Les données et recommandations présentées proviennent d’une recension des écrits scientifiques réalisée via les banques de données PsycLIT, PsyINFO et MEDLINE (1985 à 2006) en utilisant les descripteurs panic disorder, psychotherapy, psychosocial treatment, treatment et pharmacotherapy. Les recommandations formulées par les auteurs s’appuient sur des données probantes provenant d’études d’excellente qualité. Les informations concernant le diagnostic et l’évaluation du TP/A proviennent d’études épidémiologiques récentes, de consensus et d’opinions d’experts. PRINCIPAL MESSAGE Le TP/A est un trouble psychiatrique souvent rencontré en médecine de première ligne, mais il est fréquemment sous-diagnostiqué et sous-traité. L’identification précoce de ce trouble demande une attention particulière aux symptômes médicalement inexpliqués et, le cas échéant, le médecin doit utiliser des questions spécifiques permettant d’identifier d’éventuelles attaques de panique et de cerner leur signification pour le patient. Le traitement de premier choix pour ce trouble est une psychothérapie d’orientation cognitivo-comportementale administrée par un psychologue ou un psychiatre spécialisé. Si de telles ressources ne sont pas disponibles, le médecin peut opter pour un traitement psychopharmacologique. CONCLUSION Les médecins de famille peuvent jouer un rôle central dans l’identification et le traitement des patients souffrant d’un TP/A. PMID:17934032

  1. A Burger, A Beer, and A Side of Science

    NASA Astrophysics Data System (ADS)

    Wiehe, Ben; Landsberg, R. H.; Wyatt, R. J.; Turner, M. S.

    2008-05-01

    Science Cafés (aka Café Scientifiques) engage unconventional adult audiences and help researchers hone their communication skills in a relaxed and fun setting. Typically held in restaurants and pubs, Science Cafés provide a comfortable place for the public to speak with a scientist. National and local evaluations of the Café format indicate that cafes are an effective way to engage adult audiences (especially non-scientists). Continued media coverage also demonstrate that something about them captures the public's imagination. Join us for an interactive session about organizing, presenting and partnering with Science Cafés to bring IYA themes (and other current research) directly to new audiences. Real world examples from experienced Café organizers and presenters will provide an overview of what a Science Café is, how to start one and how to use the format to draw attention to astronomy topics. The discussion will include suggestions for tapping into the existing national and international community of Cafés (there are more than 60 in the US alone), and information about free outreach resources. Break-out exercises will help prepare you to: find a suitable venue, advertise, work with café speakers, and foster the inclusive conversation that is the hallmark of a Science Café. Participants will also learn about the impacts that can be expected from a Science Café including benefits to audiences, Café presenters, and hosting organizations. The overall goal of this session is to stimulate a discussion about strategies for facilitating face-to-face communication between scientists and lay audiences. Participants will have the opportunity to create their own promotional plan for a Café event, including the important process of framing a topic to grab public attention, and developing strategies for reaching new target audiences. Substantial time will be allowed for participants to discuss how the Science Café format might be adapted for their specific

  2. A 3D view of the outflow in the Orion Molecular Cloud 1 (OMC-1)

    NASA Astrophysics Data System (ADS)

    Nissen, H. D.; Cunningham, N. J.; Gustafsson, M.; Bally, J.; Lemaire, J.-L.; Favre, C.; Field, D.

    2012-04-01

    coincidence. Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  3. Cosmological constraints from the 100-deg2 weak-lensing survey

    NASA Astrophysics Data System (ADS)

    Benjamin, Jonathan; Heymans, Catherine; Semboloni, Elisabetta; van Waerbeke, Ludovic; Hoekstra, Henk; Erben, Thomas; Gladders, Michael D.; Hetterscheidt, Marco; Mellier, Yannick; Yee, H. K. C.

    2007-10-01

    National de la Recherche Scientifique (CNRS) and the University of Hawaii (UH). E-mail: jonben@phas.ubc.ca

  4. Laboratory experiments for Titan's ionosphere : the photoionisation of hydrocarbon radicals CxHy.

    NASA Astrophysics Data System (ADS)

    Alcaraz, C.; Fischer, I.; Schussler, T.; Deyerl, H.-J.; Roth, W.; Elhanine, M.; Gerber, T.

    .; Gerber, T.; Alcaraz, C.; Fischer, I. Phys. Chem. Chem. 1 Phys. 2005, 7, 819. (3) http://www.clups.u-psud.fr/ (4) http://www.synchrotron-soleil.fr/francais/vie-scientifique/experiences/desirs/index.htm 2

  5. Testing the theory of colliding winds: the periastron passage of 9 Sagittarii. I. X-ray and optical spectroscopy

    NASA Astrophysics Data System (ADS)

    Rauw, G.; Blomme, R.; Nazé, Y.; Spano, M.; Mahy, L.; Gosset, E.; Volpi, D.; van Winckel, H.; Raskin, G.; Waelkens, C.

    2016-05-01

    Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias. Based on observations obtained with the HERMES spectrograph, which is supported by the Fund for Scientific Research of Flanders (FWO), Belgium, the Research Council of K.U. Leuven, Belgium, the Fonds National de la Recherche Scientifique (F.R.S.-FNRS), Belgium, the Royal Observatory of Belgium, the Observatoire de Genève, Switzerland and the Thüringer Landessternwarte Tautenburg, Germany.

  6. HD 18078: A very slowly rotating Ap star with an unusual magnetic field structure

    NASA Astrophysics Data System (ADS)

    Mathys, G.; Romanyuk, I. I.; Kudryavtsev, D. O.; Landstreet, J. D.; Pyper, D. M.; Adelman, S. J.

    2016-02-01

    -France-Hawaii Telescope (CFHT) which is operated from the summit of Maunakea by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii; and at the 6-m telescope BTA of the Special Astrophysical Observatory of the Russian Academy of Sciences.Table 3 is only available at the CDS via anonymous ftp to http://cdsarc.u-strasbg.fr (ftp://130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/586/A85

  7. A weak-lensing analysis of the Abell 383 cluster

    NASA Astrophysics Data System (ADS)

    Huang, Z.; Radovich, M.; Grado, A.; Puddu, E.; Romano, A.; Limatola, L.; Fu, L.

    2011-05-01

    , the Institute National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. This work is based in part on data products produced at TERAPIX and the Canadian Astronomy Data Centre as part of the Canada-France-Hawaii Telescope Legacy Survey, a collaborative project of NRC and CNRS.

  8. CARS: The CFHTLS-Archive-Research Survey. III. First detection of cosmic magnification in samples of normal high-z galaxies

    NASA Astrophysics Data System (ADS)

    Hildebrandt, H.; van Waerbeke, L.; Erben, T.

    2009-11-01

    -France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. This work is based in part on data products produced at TERAPIX and the Canadian Astronomy Data Centre as part of the Canada-France-Hawaii Telescope Legacy Survey, a collaborative project of NRC and CNRS.

  9. Star Formation Rates in Resolved Galaxies: Calibrations with Near- and Far-infrared Data for NGC 5055 and NGC 6946

    NASA Astrophysics Data System (ADS)

    Li, Yiming; Crocker, Alison F.; Calzetti, Daniela; Wilson, Christine D.; Kennicutt, Robert C.; Murphy, Eric J.; Brandl, Bernhard R.; Draine, B. T.; Galametz, M.; Johnson, B. D.; Armus, L.; Gordon, K. D.; Croxall, K.; Dale, D. A.; Engelbracht, C. W.; Groves, B.; Hao, C.-N.; Helou, G.; Hinz, J.; Hunt, L. K.; Krause, O.; Roussel, H.; Sauvage, M.; Smith, J. D. T.

    2013-05-01

    We use the near-infrared Brγ hydrogen recombination line as a reference star formation rate (SFR) indicator to test the validity and establish the calibration of the Herschel/PACS 70 μm emission as a SFR tracer for sub-galactic regions in external galaxies. Brγ offers the double advantage of directly tracing ionizing photons and of being relatively insensitive to the effects of dust attenuation. For our first experiment, we use archival Canada-France-Hawaii Telescope Brγ and Ks images of two nearby galaxies: NGC 5055 and NGC 6946, which are also part of the Herschel program KINGFISH (Key Insights on Nearby Galaxies: a Far-Infrared Survey with Herschel). We use the extinction corrected Brγ emission to derive the SFR(70) calibration for H II regions in these two galaxies. A comparison of the SFR(70) calibrations at different spatial scales, from 200 pc to the size of the whole galaxy, reveals that about 50% of the total 70 μm emission is due to dust heated by stellar populations that are unrelated to the current star formation. We use a simple model to qualitatively relate the increase of the SFR(70) calibration coefficient with decreasing region size to the star formation timescale. We provide a calibration for an unbiased SFR indicator that combines the observed Hα with the 70 μm emission, also for use in H II regions. We briefly analyze the PACS 100 and 160 μm maps and find that longer wavelengths are not as good SFR indicators as 70 μm, in agreement with previous results. We find that the calibrations show about 50% difference between the two galaxies, possibly due to effects of inclination. Based on observations obtained with WIRCam, a joint project of CFHT, Taiwan, Korea, Canada, France, and the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institute National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  10. Investigating the spectroscopic, magnetic and circumstellar variability of the O9 subgiant star HD 57682

    NASA Astrophysics Data System (ADS)

    Grunhut, J. H.; Wade, G. A.; Sundqvist, J. O.; ud-Doula, A.; Neiner, C.; Ignace, R.; Marcolino, W. L. F.; Rivinius, Th.; Fullerton, A.; Kaper, L.; Mauclaire, B.; Buil, C.; Garrel, T.; Ribeiro, J.; Ubaud, S.

    2012-11-01

    Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France and the University of Hawaii.

  11. The COSMOS Survey: Hubble Space Telescope Advanced Camera for Surveys Observations and Data Processing

    NASA Astrophysics Data System (ADS)

    Koekemoer, A. M.; Aussel, H.; Calzetti, D.; Capak, P.; Giavalisco, M.; Kneib, J.-P.; Leauthaud, A.; Le Fèvre, O.; McCracken, H. J.; Massey, R.; Mobasher, B.; Rhodes, J.; Scoville, N.; Shopbell, P. L.

    2007-09-01

    Research Council of Canada, the Canadian Astronomy Data Centre, the Centre National de la Recherche Scientifique de France, TERAPIX, and the University of Hawaii.

  12. The Massive Progenitor of the Type II-linear Supernova 2009kr

    NASA Astrophysics Data System (ADS)

    Elias-Rosa, Nancy; Van Dyk, Schuyler D.; Li, Weidong; Miller, Adam A.; Silverman, Jeffrey M.; Ganeshalingam, Mohan; Boden, Andrew F.; Kasliwal, Mansi M.; Vinkó, József; Cuillandre, Jean-Charles; Filippenko, Alexei V.; Steele, Thea N.; Bloom, Joshua S.; Griffith, Christopher V.; Kleiser, Io K. W.; Foley, Ryan J.

    2010-05-01

    We present early-time photometric and spectroscopic observations of supernova (SN) 2009kr in NGC 1832. We find that its properties to date support its classification as Type II-linear (SN II-L), a relatively rare subclass of core-collapse supernovae (SNe). We have also identified a candidate for the SN progenitor star through comparison of pre-explosion, archival images taken with WFPC2 on board the Hubble Space Telescope with SN images obtained using adaptive optics plus NIRC2 on the 10 m Keck-II telescope. Although the host galaxy's substantial distance (~26 Mpc) results in large uncertainties in the relative astrometry, we find that if this candidate is indeed the progenitor, it is a highly luminous (M 0 V = -7.8 mag) yellow supergiant with initial mass ~18-24 M sun. This would be the first time that an SN II-L progenitor has been directly identified. Its mass may be a bridge between the upper initial mass limit for the more common Type II-plateau SNe and the inferred initial mass estimate for one Type II-narrow SN. Based in part on observations made with the NASA/ESA Hubble Space Telescope (HST), obtained from the Data Archive at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy (AURA), Inc., under NASA contract NAS 05-26555; the 6.5 m Magellan Clay Telescope located at Las Campanas Observatory, Chile; various telescopes at Lick Observatory; the 1.3 m PAIRITEL on Mt. Hopkins; the SMARTS Consortium 1.3 m telescope located at Cerro Tololo Inter-American Observatory (CTIO), Chile; the 3.6 m Canada-France-Hawaii Telescope (CFHT), which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii; and the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and NASA, with

  13. Extended Red Emission and the evolution of carbonaceous nanograins in NGC 7023

    NASA Astrophysics Data System (ADS)

    Berné, O.; Joblin, C.; Rapacioli, M.; Thomas, J.; Cuillandre, J.-C.; Deville, Y.

    2008-03-01

    Context: Extended Red Emission (ERE) was recently attributed to the photo-luminescence of either doubly ionized Polycyclic Aromatic Hydrocarbons (PAH++), or charged PAH dimers ([PAH{2}] ^+). Aims: We analysed the visible and mid-infrared (mid-IR) dust emission in the North-West and South photo-dissociation regions of the reflection nebula NGC 7023. Methods: Using a blind signal separation method, we extracted the map of ERE from images obtained with the Hubble Space Telescope, and at the Canada France Hawaii Telescope. We compared the extracted ERE image to the distribution maps of the mid-IR emission of Very Small Grains (VSGs), neutral and ionized PAHs (PAH0 and PAH^+) obtained with the Spitzer Space Telescope and the Infrared Space Observatory. Results: ERE is dominant in transition regions where VSGs are being photo-evaporated to form free PAH molecules, and is not observed in regions dominated by PAH^+. Its carrier makes a minor contribution to the mid-IR emission spectrum. Conclusions: These results suggest that the ERE carrier is a transition species formed during the destruction of VSGs. [PAH{2}] + appear as good candidates but PAH++ molecules seem to be excluded. This work is based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the Data Archive at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with program 9471. Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. Based on observations with

  14. CARS: the CFHTLS-Archive-Research Survey. II. Weighing dark matter halos of Lyman-break galaxies at z = 3-5

    NASA Astrophysics Data System (ADS)

    Hildebrandt, H.; Pielorz, J.; Erben, T.; van Waerbeke, L.; Simon, P.; Capak, P.

    2009-05-01

    Aims: We measure the clustering properties for a large samples of u- (z˜3), g- (z˜4), and r- (z˜5) dropouts from the Canada-France-Hawaii Telescope Legacy Survey (CFHTLS) Deep fields. Methods: Photometric redshift distributions along with simulations allow us to de-project the angular correlation measurements and estimate physical quantities such as the correlation length, halo mass, galaxy bias, and halo occupation as a function of UV luminosity. Results: For the first time we detect a significant one-halo term in the correlation function at z˜5. The comoving correlation lengths and halo masses of LBGs are found to decrease with decreasing rest-frame UV-luminosity. No significant redshift evolution is found in either quantity. The typical halo mass hosting an LBG is M⪆1012~h-1~M_⊙ and the halos are typically occupied by less than one galaxy. Clustering segregation with UV luminosity is clearly observed in the dropout samples, however redshift evolution cannot clearly be disentangled from systematic uncertainties introduced by the redshift distributions. We study a range of possible redshift distributions to illustrate the effect of this choice. Spectroscopy of representative subsamples is required to make high-accuracy absolute measurements of high-z halo masses. Based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. This work is based in part on data products produced at TERAPIX and the Canadian Astronomy Data Centre as part of the Canada-France-Hawaii Telescope Legacy Survey, a collaborative project of NRC and CNRS. Based on zCOSMOS and VVDS observations carried out using the Very Large Telescope at the ESO Paranal Observatory under Programme IDs: LP175.A

  15. A comprehensive analysis of the magnetic standard star HD 94660: Host of a massive compact companion?

    NASA Astrophysics Data System (ADS)

    Bailey, J. D.; Grunhut, J.; Landstreet, J. D.

    2015-03-01

    ) telescopes under the ESO programme 093.D-0367(A) and programmes 076.D-0169(A), 088.D-0066(A), 087.D-0771(A), 084.D-0338(A), 083.D-1000(A) and 60.A-9036(A), obtained from the ESO/ST-ECF Science Archive Facility. It is also based in part on observations carried out at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Science de l'Univers of the Centre National de la Recherche Scientifique of France and the University of Hawaii.

  16. Absorbing Gas around the WASP-12 Planetary System

    NASA Astrophysics Data System (ADS)

    Fossati, L.; Ayres, T. R.; Haswell, C. A.; Bohlender, D.; Kochukhov, O.; Flöer, L.

    2013-04-01

    Near-UV observations of the planet host star WASP-12 uncovered the apparent absence of the normally conspicuous core emission of the Mg II h and k resonance lines. This anomaly could be due either to (1) a lack of stellar activity, which would be unprecedented for a solar-like star of the imputed age of WASP-12 or (2) extrinsic absorption, from the intervening interstellar medium (ISM) or from material within the WASP-12 system itself, presumably ablated from the extreme hot Jupiter WASP-12 b. HIRES archival spectra of the Ca II H and K lines of WASP-12 show broad depressions in the line cores, deeper than those of other inactive and similarly distant stars and similar to WASP-12's Mg II h and k line profiles. We took high-resolution ESPaDOnS and FIES spectra of three early-type stars within 20' of WASP-12 and at similar distances, which show the ISM column is insufficient to produce the broad Ca II depression observed in WASP-12. The EBHIS H I column density map supports and strengthens this conclusion. Extrinsic absorption by material local to the WASP-12 system is therefore the most likely cause of the line core anomalies. Gas escaping from the heavily irradiated planet could form a stable and thick circumstellar disk/cloud. The anomalously low stellar activity index (log R^{{\\prime }}_{HK}) of WASP-12 is evidently a direct consequence of the extra core absorption, so similar HK index deficiencies might signal the presence of translucent circumstellar gas around other stars hosting evaporating planets. Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT), which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Rechereche Scientifique of France, and the University of Hawaii. Based on observations made with the Nordic Optical Telescope, operated on the island of La Palma jointly by Denmark, Finland, Iceland, Norway, and Sweden, in the Spanish Observatorio del

  17. Formation and ridging of flaw leads in the eastern Canadian Beaufort Sea. Special Session C06 on: “Physical, biological and biogeochemical processes associated with young thin ice types”

    NASA Astrophysics Data System (ADS)

    Prinsenberg, S. J.

    2009-12-01

    Formation and ridging of flaw leads in the eastern Canadian Beaufort Sea. Simon Prinsenberg1 and Yves Graton2 1Bedford Inst. of Oceanography, Fisheries and Oceans Canada P.O. Box1006, Dartmouth, Nova Scotia, B2Y 4A2, Canada prinsenbergs@mar.dfo-mpo.gc.ca 2Inst. National de la Recherche Scientifique-Eau, INRS-ETE University of Quebec at Quebec City, Quebec yvesgratton@eteinrs.ca During the winter of 2008, the flaw lead south of Banks Island repeatedly opened and closed representing an elongated region where periodically the large ice growth stimulates the densification of the surface layer due to salt rejection and instigates a local circulation pattern that will affect the biological processes of the region. Helicopter-borne sensors were available to monitor the aftermath of one of the rapid closing of the flaw lead into extensive elongated rubble field using a Canadian Ice breaker, CCGS Amundsen, as a logistic base. After the wind reversed a new open flaw lead 20km wide restarting a new flaw lead formation cycle. Ice thickness and surface roughness data were collected from the rubble field and adjacent open flaw lead with an Electromagnetic-Laser system. The strong wind event of April 4-5 2009 generated a large linear 1.5km wide ice rubble field up to 8-10m thick when the 60cm thick, 18km wide flaw lead was crunched into land-fast by the 1.5m thick offshore pack ice. It is expected that during rapid ice growth in a flaw lead, salt rejection increase the density of the surface water layer producing a surface depression (Low) and cyclonic circulation. In contrast at depth, the extra surface dense water produces a high in the horizontal pressure field and anti-cyclonic circulation which remains after the rapid ice growth within the flaw lead stops. One of such remnants may have been observed during the CFL-IPY winter survey.

  18. Transiting exoplanets from the CoRoT space mission . XIII. CoRoT-13b: a dense hot Jupiter in transit around a star with solar metallicity and super-solar lithium content

    NASA Astrophysics Data System (ADS)

    Cabrera, J.; Bruntt, H.; Ollivier, M.; Díaz, R. F.; Csizmadia, Sz.; Aigrain, S.; Alonso, R.; Almenara, J.-M.; Auvergne, M.; Baglin, A.; Barge, P.; Bonomo, A. S.; Bordé, P.; Bouchy, F.; Carone, L.; Carpano, S.; Deleuil, M.; Deeg, H. J.; Dvorak, R.; Erikson, A.; Ferraz-Mello, S.; Fridlund, M.; Gandolfi, D.; Gazzano, J.-C.; Gillon, M.; Guenther, E. W.; Guillot, T.; Hatzes, A.; Havel, M.; Hébrard, G.; Jorda, L.; Léger, A.; Llebaria, A.; Lammer, H.; Lovis, C.; Mazeh, T.; Moutou, C.; Ofir, A.; von Paris, P.; Pätzold, M.; Queloz, D.; Rauer, H.; Rouan, D.; Santerne, A.; Schneider, J.; Tingley, B.; Titz-Weider, R.; Wuchterl, G.

    2010-11-01

    We announce the discovery of the transiting planet CoRoT-13b. Ground-based follow-up in CFHT and IAC80 confirmed CoRoT's observations. The mass of the planet was measured with the HARPS spectrograph and the properties of the host star were obtained analyzing HIRES spectra from the Keck telescope. It is a hot Jupiter-like planet with an orbital period of 4.04 days, 1.3 Jupiter masses, 0.9 Jupiter radii, and a density of 2.34 g cm-3. It orbits a G0V star with T_eff = 5 945 K, M* = 1.09 M⊙, R_* = 1.01 R⊙, solar metallicity, a lithium content of + 1.45 dex, and an estimated age of between 0.12 and 3.15 Gyr. The lithium abundance of the star is consistent with its effective temperature, activity level, and age range derived from the stellar analysis. The density of the planet is extreme for its mass, implies that heavy elements are present with a mass of between about 140 and 300 {M}⊕. The CoRoT space mission, launched on December 27th 2006, has been developed and is operated by CNES, with the contribution of Austria, Belgium, Brazil, ESA (RSSD and Science Programme), Germany and Spain. Part of the observations were obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. Based on observations made with HARPS spectrograph on the 3.6-m European Organisation for Astronomical Research in the Southern Hemisphere telescope at La Silla Observatory, Chile (ESO program 184.C-0639). Based on observations made with the IAC80 telescope operated on the island of Tenerife by the Instituto de Astrofísica de Canarias in the Spanish Observatorio del Teide. Part of the data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and the National Aeronautics

  19. Enquete sur les aspects toxicologiques de la phytotherapie utilisee par un herboriste à Fes, Maroc

    PubMed Central

    Zeggwagh, Ali Amine; Lahlou, Younes; Bousliman, Yassir

    2013-01-01

    Introduction Dans le but d'étudier l'aspect toxicologique des plantes médicinales utilisées en médecine traditionnelle, une étude ethnobotanique a été réalisée à la ville de Fès au centre du Maroc. Méthodes Ont été inclus dans l'étude tous les patients ayant bénéficié d'une prescription par l'herboriste de plantes à visée thérapeutique. La discussion de nos résultats s'est faite sur la base d'une revue de la littérature avec identification des principales plantes toxiques utilisées en phytothérapie au Maroc. L'approche bibliographique a permis de compléter les informations. Résultats L'âge moyen des patients traités par des plantes (38 femmes, 32 hommes) était de 35 ± 18 ans. L'enquête ethnobotanique à révélé que la majorité des plantes médicinales étaient utilisées contre les affections urinaires (21%), suivi des maladies de l'appareil digestif (19.6%) et des maladies rhumatologiques (18.2%). Le nombre de plantes prescrits par l'herboriste a été de 53 dont 5 sont potentiellement toxiques. L'identification taxonomique des plantes prescrites a recensé 30 familles dont les plus représentées sont les Lamiaceae (23.33%), les Apiaceae (13,33%) et les Asteraceae (10%). La prescription des plantes considérées comme toxiques a concerné 7,1% des consultants traités par les plantes médicinales. Aucune complication inhérente aux plantes prescrites n'a été déplorée. Conclusion Malgré les résultats encourageants de notre enquête sur le compte de la phytothérapie, la pratique de la phytothérapie est laissée à la vulgarisation et à l'oubli scientifique, législatif et universitaire. PMID:23734270

  20. γ Pegasi: testing Vega-like magnetic fields in B stars

    NASA Astrophysics Data System (ADS)

    Neiner, C.; Monin, D.; Leroy, B.; Mathis, S.; Bohlender, D.

    2014-02-01

    . These scenarios should thus be revised. Our results also provide strong constraints for stellar evolution models. Based on observations obtained at the Telescope Bernard Lyot (USR5026) operated by the Observatoire Midi-Pyrénées, Université de Toulouse (Paul Sabatier), Centre National de la Recherche Scientifique of France, and at the Dominion Astrophysical Observatory.Tables 1-3 are available in electronic form at http://www.aanda.org

  1. Detection of a magnetic field on HD108: clues to extreme magnetic braking and the Of?p phenomenon

    NASA Astrophysics Data System (ADS)

    Martins, F.; Donati, J.-F.; Marcolino, W. L. F.; Bouret, J.-C.; Wade, G. A.; Escolano, C.; Howarth, I. D.; Mimes Collaboration

    2010-09-01

    obtained at the Télescope Bernard Lyot (TBL) and at the Canada-France-Hawaii Telescope (CFHT). CFHT is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France (INSU/CNRS), and the University of Hawaii, while TBL is operated by CNRS/INSU. E-mail: martins@graal.univ-montp2.fr

  2. Likelihood analysis of cosmic shear on simulated and VIRMOS-DESCART data

    NASA Astrophysics Data System (ADS)

    Van Waerbeke, L.; Mellier, Y.; Pelló, R.; Pen, U.-L.; McCracken, H. J.; Jain, B.

    2002-10-01

    We present a maximum likelihood analysis of cosmological parameters from measurements of the aperture mass up to 35 arcmin using simulated and real cosmic shear data. A four-dimensional parameter space is explored which examines the mean density OmegaM , the mass power spectrum normalisation sigma8, the shape parameter Gamma and the redshift of the sources zs. Constraints on OmegaM and sigma8 (resp. Gamma and zs) are provided by marginalising over Gamma and zs (resp. OmegaM and sigma8 ). For a flat Lambda CDM cosmologies, using a photometric redshift prior for the sources and Gamma in [0.1,0.4], we find sigma8 =(0.57+/-0.04) OmegaM (0.24 -/+ 0.18) OmegaM -0.4} at the 68% confidence level (the error budget includes statistical noise, full cosmic variance and residual systematics). The estimate of Gamma , marginalised over OmegaM in [0.1,0.4], sigma8 in [0.7,1.3] and zs constrained by photometric redshifts, gives Gamma =0.25+/- 0.13 at 68% confidence. Adopting h=0.7, a flat universe, Gamma =0.2 and Omegam =0.3 we find sigma8 =0.98 +/-0.06. Combined with CMB measurements, our results suggest a non-zero cosmological constant and provide tight constraints on OmegaM and sigma8 . Finally, we compare our results to the cluster abundance ones, and discuss the possible discrepancy with the latest determinations of the cluster method. In particular we point out the actual limitations of the mass power spectrum prediction in the non-linear regime, and the importance in improving this. Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT), which is operated by the National Research Council of Canada (NRCC), the Institut des Sciences de l'Univers (INSU) of the Centre National de la Recherche Scientifique (CNRS) and the University of Hawaii (UH), and at the European Southern Observatory telescopes Very Large Telescope (VLT) and the New Technology Telescope (NTT).

  3. Weak Lensing Calibrated M-T Scaling Relation of Galaxy Groups in the COSMOS Fieldsstarf

    NASA Astrophysics Data System (ADS)

    Kettula, K.; Finoguenov, A.; Massey, R.; Rhodes, J.; Hoekstra, H.; Taylor, J. E.; Spinelli, P. F.; Tanaka, M.; Ilbert, O.; Capak, P.; McCracken, H. J.; Koekemoer, A.

    2013-11-01

    are operated by the Association of Universities for Research in Astronomy, Inc. (AURA) under cooperative agreement with the National Science Foundation; the National Radio Astronomy Observatory, which is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.; and the Canada-France-Hawaii Telescope (CFHT) with MegaPrime/MegaCam operated as a joint project by the CFHT Corporation, CEA/DAPNIA, the National Research Council of Canada, the Canadian Astronomy Data Centre, the Centre National de la Recherche Scientifique de France, TERAPIX, and the University of Hawaii.

  4. Mise à jour sur l’utilisation clinique de la buprénorphine

    PubMed Central

    Ducharme, Simon; Fraser, Ronald; Gill, Kathryn

    2012-01-01

    Résumé Objectif Examiner les données scientifiques actuelles sur la buprénorphine-naloxone pour le traitement des troubles liés aux opioïdes, en insistant sur le contexte des soins primaires. Qualité des données On a fait une recension dans MEDLINE et la base de données Cochrane des synthèses critiques. Les données probantes sont surtout de niveau I. Message principal La buprénorphine est un agoniste partiel des récepteurs μ des opioïdes et un antagoniste des récepteurs κ des opioïdes ayant une longue demi-vie et un potentiel moins grand que la méthadone d’entraîner un usage abusif. Pour une désintoxication, la buprénorphine est au moins équivalente à la méthadone et supérieure à la clonidine. Comme thérapie de substitution, la buprénorphine est clairement supérieure au placebo. La méthadone comporte de légers avantages en ce qui a trait à la rétention en thérapie, mais une approche par étape en utilisant initialement la buprénorphine-naloxone est aussi efficace. Il est possible, sécuritaire et efficace de recourir à la buprénorphine en milieu de soins primaires. On peut obtenir l’autorisation de prescrire de la buprénorphine après avoir suivi une formation en ligne. Conclusion La buprénorphine est un agent sécuritaire et efficace pour la désintoxication en cas de dépendance aux opioïdes. Elle peut servir d’agent de première intention dans les programmes de thérapie de substitution, en raison de son potentiel plus faible d’usage abusif en comparaison d’autres opioïdes. Son efficacité en milieux de soins primaires en fait un outil thérapeutique utile pour les médecins de famille.

  5. Using Games To Explore The Nexus of Climate, Energy, and Water

    NASA Astrophysics Data System (ADS)

    Hall, M. K.; Mayhew, M. A.

    2012-12-01

    We have developed a set of card games to teach teens and adults about the interdependency of energy demand, water consumption, and climate change, which we term the nexus of energy, water, and climate. The latest game challenges players to construct arguments around issues related to the nexus, such as the benefits of carbon sequestration or the negative impacts of consuming corn biofuel. The game has been through several rounds of playtesting, both with teens and adults, and in formal and informal learning environments, such as our ongoing teen Cafe Scientifique program (www.cafenm.org). The card game consists of two types of cards, "Challenge" and "Policy." Each round, one player acting as the Judge draws a Challenge card and reads the adjective—for example, dangerous, clean, catastrophic, awesome— and its definition displayed on the card. The other players hold Policy cards containing 3 or 4 facts related to nexus concepts. For example, the Algae bio-diesel fuel policy card contains the fact, "Algae can produce 100 times more fuel per acre that any other biofuel crop". A fact on the Tight shale gas policy card reads, "Chemicals used in 'fracking' can contaminate water supplies." Using the facts on a single Policy card, each player constructs an argument aligned with the adjective—and presents it to the Judge. This requires players to synthesize the given facts and any prior knowledge about the topic into a coherent argument. As players make their arguments, everyone is challenged to think about the nuances and implications of the myriad choices we have in balancing the needs for water and energy resources with the challenge of minimizing climate change. The Judge decides which player makes the policy argument that best aligns with the adjective, and that player wins the round. Players take turns being the Judge. The first player to win three rounds wins the game. The game has been well received by both teen and adult audiences. It is a highly social game

  6. The mass function of IC 4665 revisited by the UKIDSS Galactic Clusters Survey

    NASA Astrophysics Data System (ADS)

    Lodieu, N.; de Wit, W.-J.; Carraro, G.; Moraux, E.; Bouvier, J.; Hambly, N. C.

    2011-08-01

    , the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.Full Tables A.1, B.1, and C.1 are only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/532/A103

  7. Detections of CO Molecular Gas in 24 μm Bright ULIRGs at z ~ 2 in the Spitzer First Look Survey

    NASA Astrophysics Data System (ADS)

    Yan, Lin; Tacconi, L. J.; Fiolet, N.; Sajina, A.; Omont, A.; Lutz, D.; Zamojski, M.; Neri, R.; Cox, P.; Dasyra, K. M.

    2010-05-01

    the Institute for Radioastronomy at Millimeter Wavelengths (IRAM) Plateau de Bure Interferometer (PdBI). IRAM is funded by the Centre National de la Recherche Scientifique (France), the Max-Planck Gesellschaft (Germany), and the Instituto Geografico Nacional (Spain).

  8. Starburst activity in the host galaxy of the z =2.58 quasar J1409+5628

    NASA Astrophysics Data System (ADS)

    Beelen, A.; Cox, P.; Pety, J.; Carilli, C. L.; Bertoldi, F.; Momjian, E.; Omont, A.; Petitjean, P.; Petric, A. O.

    2004-08-01

    We report the detection of CO emission from the optically luminous, radio-quiet quasar J140955.5+562827 (hereafter J1409+5628), at a redshift zCO =2.583. We also present VLA continuum maps and VLBA high spatial resolution observations at 1.4 GHz. Both the CO(3->2) and CO(7->6) emission lines are detected using the IRAM Plateau de Bure interferometer. The 3->2/7->6 line luminosity ratio is about 1/3, indicating the presence of warm and dense molecular gas with an estimated mass of 6 × 1010 M⊙. The infrared-to-CO luminosity ratio LFIR/L'CO(1->0) ≈ 500 L⊙ (K km s-1 pc2)-1, comparable to values found for other high-z sources where CO line emission is seen. J1409+5628 is detected using the VLA with a 1.4 GHz rest-frame luminosity density of 4.0 × 1025 W Hz-1. The rest-frame radio to far-infrared ratio, q, has a value of 2.0 which is similar to the values found in star forming galaxies. At the 30 mas resolution of the VLBA, J1409+5628 is not detected with a 4σ upper limit to the surface brightness of 0.29 mJy beam-1. This implies a limit to the intrinsic brightness temperature of 2 × 105 K at 8 GHz, typical for nuclear starbursts and more than two orders of magnitude fainter than typical radio-loud active galactic nuclei. Both the properties of the CO line emission and the radio emission from J1409+5628 are therefore consistent with those expected for a star forming galaxy. In J1409+5628 young massive stars are the dominant source of dust heating, accounting for most of the infrared luminosity. The massive reservoir of molecular gas can sustain the star formation rate of a few 1000 M⊙ yr-1 implied by the far-infrared luminosity for about 10 million years. This paper is based on observations obtained with the IRAM Plateau de Bure Interferometer. IRAM is funded by Centre National de la Recherche Scientifique (France), the Max-Planck-Gesellschaft (Germany), and the Instituto Geografico Nacional (Spain).

  9. Crazy heart: kinematics of the "star pile" in Abell 545

    NASA Astrophysics Data System (ADS)

    Salinas, R.; Richtler, T.; West, M. J.; Romanowsky, A. J.; Lloyd-Davies, E.; Schuberth, Y.

    2011-04-01

    des Science de l'Univers of the Centre Natio nal de la Recherche Scientifique (CNRS) of France, and the University of Hawaii.

  10. The Seismic Broad Band Western Mediterranean (wm) Network and the Obs Fomar Pool: Current state and Obs activities.

    NASA Astrophysics Data System (ADS)

    Pazos, Antonio; Davila, Jose Martin; Buforn, Elisa; Bezzeghoud, Mourad; Harnafi, Mimoun; Mattesini, Mauricio; Caldeira, Bento; Hanka, Winfried; El Moudnib, Lahcen; Strollo, Angelo; Roca, Antoni; Lopez de Mesa, Mireya; Dahm, Torsten; Cabieces, Roberto

    2016-04-01

    The Western Mediterranean (WM) seismic network started in 1996 as an initiative of the Royal Spanish Navy Observatory (ROA) and the Universidad Complutense de Madrid (UCM), with the collaboration of the GeoForschungsZentrum (GFZ) of Potsdam. A first broad band seismic station (SFUC) was installed close to Cádiz (South Spain). Since then, additional stations have been installed in the Ibero-Moghrebian region. In 2005, the "WM" code was assigned by the FDSN and new partners were jointed: Evora University (UEVO, Portugal), the Scientifique Institute of Rabat (ISRABAT, Morocco), and GFZ. Now days, the WM network is composed by 15 BB stations, all of them with Streckaisen STS-2 or STS-2.5 sensors, Quanterra or Earthdata digitizers and SeiscomP. Most them have co-installed a permanent geodetic GPS stations, and some them also have an accelerometer. There are 10 stations deployed in Spanish territory (5 in the Iberian peninsula, 1 in Balearic islands and 4 in North Africa Spanish places) with VSAT or Internet communications, 2 in Portugal (one of them without real time), and 3 in Morocco (2 VSAT and 1 ADSL). Additionally, 2 more stations (one in South Spain and one in Morocco) will be installed along this year. Additionally ROA has deployed a permanent real time VBB (CMG-3T: 360s) station at the Alboran Island. Due to the fact that part of the seismic activity is located at marine areas, and also because of the poor geographic azimuthal coverage at some zones provided by the land stations (specially in the SW of the San Vicente Cape area), ROA and UCM have acquired six broad band "LOBSTERN" OBS, manufactured by KUM (Kiel, Germany), conforming the OBS FOMAR pool. Three of them with CMG-40T sensor and the other with Trillium 120. These OBS were deployed along the Gibraltar strait since January to November 2014 to study the microseismicity in the Gibraltar strait area. In September 2015 FOMAR network has been deployed in SW of the San Vicente Cape for 8 months as a part of

  11. Ingredients for protist coexistence: competition, endosymbiosis and a pinch of biochemical interactions.

    PubMed

    Müller, Johann P; Hauzy, Céline; Hulot, Florence D

    2012-01-01

    1. The interaction between mutualism, facilitation or interference and exploitation competition is of major interest as it may govern species coexistence. However, the interplay of these mechanisms has received little attention. This issue dates back to Gause, who experimentally explored competition using protists as a model [Gause, G.F. (1935) Vérifications expérimentales de la théorie mathématique de la lutte pour la vie. Actualités Scientifiques et Industrielles, 277]. He showed the coexistence of Paramecium caudatum with a potentially allelopathic species, Paramecium bursaria. 2. Paramecium bursaria hosts the green algae Chlorella vulgaris. Therefore, P. bursaria may benefit from carbohydrates synthesised by the algae. Studying endosymbiosis with P. bursaria is possible as it can be freed of its endosymbiont. In addition, C. vulgaris is known to produce allelochemicals, and P. bursaria may benefit also from allelopathic compounds. 3. We designed an experiment to separate the effects of resource exploitation, endosymbiosis and allelopathy and to assess their relative importance for the coexistence of P. bursaria with a competitor that exploits the same resource, bacteria. The experiment was repeated with two competitors, Colpidium striatum or Tetrahymena pyriformis. 4. Results show that the presence of the endosymbiont enables the coexistence of competitors, while its loss leads to competitive exclusion. These results are in agreement with predictions based on resource equilibrium density of monocultures (R*) supporting the idea that P. bursaria's endosymbiont is a resource provider for its host. When P. bursaria and T. pyriformis coexist, the density of the latter shows large variation that match the effects of culture medium of P. bursaria. Our experiment suggests these effects are because of biochemicals produced in P. bursaria culture. 5. Our results expose the hidden diversity of mechanisms that underlie competitive interactions. They thus support

  12. Testing the theory of colliding winds: the periastron passage of 9 Sagittarii. I. X-ray and optical spectroscopy

    NASA Astrophysics Data System (ADS)

    Rauw, G.; Blomme, R.; Nazé, Y.; Spano, M.; Mahy, L.; Gosset, E.; Volpi, D.; van Winckel, H.; Raskin, G.; Waelkens, C.

    2016-04-01

    Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias. Based on observations obtained with the HERMES spectrograph, which is supported by the Fund for Scientific Research of Flanders (FWO), Belgium, the Research Council of K.U. Leuven, Belgium, the Fonds National de la Recherche Scientifique (F.R.S.-FNRS), Belgium, the Royal Observatory of Belgium, the Observatoire de Genève, Switzerland and the Thüringer Landessternwarte Tautenburg, Germany.

  13. Description and validation of a streamflow assimilation system for a distributed hydrometeorological model over France. Impacts on the ensemble streamflow forecasts.

    NASA Astrophysics Data System (ADS)

    Thirel, G.; Martin, E.; Mahfouf, J. F.; Massart, S.; Ricci, S.; Regimbeau, F.; Habets, F.

    2009-09-01

    SAFRAN-ISBA-MODCOU (SIM) is a distributed hydro-meteorological model used at Météo-France to predict soil water content and river streamflows. In order to produce a more accurate initial state for the ensemble streamflow forecasts systems based on SIM, an assimilation system is developed at Météo-France. This assimilation system uses past streamflow measurements in order to assess the best initial state of soil water content of the model for ensemble streamflow prediction. The data assimilation system is developed with a modular software (PALM, from the Centre Européen de Recherche et de Formation Avancée en Calcul Scientifique, CERFACS), and is based on the Best Linear Unbiased Estimator (BLUE) method. Data from a maximum of 186 gauge stations are assimilated over France, as well as for single stations, than for embedded stations networks. The first part of the study focuses on the selection of the best model variables for the assimilation process : root zone layer only, root zone and deep layers taken together, and finally taken apart. Two versions of the physics in SIM, including or not an exponential profile of hydraulic conductivity in the soil, are tested for each one of the three configurations. A set of classical hydrological scores are performed on a 18-month period in order to describe the performances of the experiments. This work showed a significant improvement of the Nash criteria and a decrease of the root mean square error for the configuration using the exponential profile of hydraulic conductivity in the soil and with the state variable including the root zone and deep layers taken together. The assimilation system seems more efficient for floods than for low flows. The second part of the work is about the impact of the assimilated initial states of the model on two ensemble streamflow prediction systems (ESPS) based on SIM and the ECMWF EPS and the Météo-France PEARP EPS. The scores are assessed on the same 18-month period, and validated

  14. Teaching About The Nexus of Energy, Water and Climate Through Traditional Games

    NASA Astrophysics Data System (ADS)

    Hall, M. K.; Mayhew, M. A.; Kaminsky, A.

    2011-12-01

    Getting to a sustainable energy economy, while conserving water resources and mitigating climate change, will involve myriad choices. Thus, it is important that the American public have an improved science-based understanding to form a strong basis for decision-making and to understand the trade-offs. To address this need, we are developing compelling, resource management style games that convey the intimate inter-relationships among energy demand, water consumption, and climate change and the importance of these inter-relationships to society. We have developed a card game with the help of professional game developer and an advisory group consisting of high school students and scientists involved with different aspects of energy-climate-water research as well as experts from the energy utilities and regulatory sectors. We have developed the card game based on real world data on energy production and consumption, regional climate information, and knowledge of emerging technologies that would mitigate the demand for energy, consumption of water with energy production, or climate change. The game is being played within the setting of our Cafe Scientifique program, now in its fifth year of serving high school age teens. One of the important aspects of the game is to find the right balance of energy output for various sources, water use by these sources, and amount of "pollution" generated (CO2 impacting climate, but also other kinds, such a radioactive waste and ground water contamination). Each player acts as "governor" of a specific region of the country, and no region has an a priori advantage. At the same time, it is important that the energy-water-pollution values we use correspond as closely as possible to real-world values. Data gathered from a combination of focus groups, surveys, and observations strongly suggest that this game, grounded in real life problems, stimulates authentic, meaningful learning. There is also some evidence that if games, such as this

  15. Prise de suppléments multivitaminiques pour la prévention primaire des anomalies congénitalies

    PubMed Central

    Morin, Pascale; Demers, Karine; Giguère, Christine; Tribble, Denise St-Cyr; Lane, Julie

    2007-01-01

    RÉSUMÉ OBJECTIF Déterminer si les recommandations véhiculées par les professionnels de la santé sur l’importance de l’acide folique encouragent les femmes susceptibles de procréer de prendre les suppléments d’acide folique. CONCEPTION Enquête. CONTEXTE Centre de santé et de services sociaux, Institut universitaire de gériatrie de Sherbrooke, à Sherbrooke, Qué. PARTICIPANTS 323 femmes francophones âgées entre 18 et 45 ans. PRINCIPALES MESURES DES RÉSULTATS La consommation de suppléments de vitamines et de minéraux au cours de la dernière année. Des analyses statistiques descriptives et bivariées et une modélisation par régression logistique ont été effectuées pour déterminer si l’association observée entre la recommandation d’un professionnel de la santé et la consommation de vitamines et de minéraux persistait après avoir tenu compte de l’effet des variables de contrôle (consultation de documentation, connaissances, sources d’information, perception, âge, scolarité, revenu, état matrimonial, intention de devenir enceinte). RÉSULTATS Environ 41% des femmes rapportent que leur médecin leur avait recommandé de consommer un supplément de vitamines et de minéraux. Après avoir ajusté toutes les variables dans le modèle, il est apparu que le fait de se faire recommander par un professionnel de la santé de prendre un supplément de vitamines et de minéraux était significativement associé à la consommation de vitamines et de minéraux par les femmes susceptibles de devenir enceintes. CONCLUSION Les professionnels peuvent améliorer la santé de la population par une pratique clinique préventive. Nous soulignons l’importance de soutenir ces derniers dans leurs efforts d’intégrer puis d’appliquer des connaissances scientifiques dans leur pratique. PMID:18077754

  16. Coronal structure of the classical T Tauri star V2129 Oph

    NASA Astrophysics Data System (ADS)

    Jardine, M. M.; Gregory, S. G.; Donati, J.-F.

    2008-05-01

    the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. E-mail: mmj@st-andrews.ac.uk (MMJ); sg64@st-andrews.ac.uk (SGG); donati@ast.obs-mip.fr (J-FD)

  17. The stable magnetic field of the fully convective star V374 Peg

    NASA Astrophysics Data System (ADS)

    Morin, J.; Donati, J.-F.; Forveille, T.; Delfosse, X.; Dobler, W.; Petit, P.; Jardine, M. M.; Collier Cameron, A.; Albert, L.; Manset, N.; Dintrans, B.; Chabrier, G.; Valenti, J. A.

    2008-02-01

    We report in this paper phase-resolved spectropolarimetric observations of the rapidly rotating fully convective M4 dwarf V374 Peg, on which a strong, mainly axisymmetric, large-scale poloidal magnetic field was recently detected. In addition to the original data set secured in 2005 August, we present here new data collected in 2005 September and 2006 August. From the rotational modulation of unpolarized line profiles, we conclude that star-spots are present at the surface of the star, but their contrast and fractional coverage are much lower than those of non-fully convective active stars with similar rotation rate. Applying tomographic imaging on each set of circularly polarized profiles separately, we find that the large-scale magnetic topology is remarkably stable on a time-scale of 1 yr; repeating the analysis on the complete data set suggests that the magnetic configuration is sheared by very weak differential rotation (about 1/10th of the solar surface shear) and only slightly distorted by intrinsic variability. This result is at odds with various theoretical predictions, suggesting that dynamo fields of fully convective stars should be mostly non-axisymmetric unless they succeed at triggering significant differential rotation. Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Science de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. E-mail: jmorin@ast.obs-mip.fr (JM); donati@ast.obs-mip.fr (J-FD); thierry.forveille@obs.ujf-grenoble.fr (TF); xavier.delfosse@obs.ujfgrenoble.fr (XD); wolfgang.dobler@ucalgary.ca (WD); petit@ast.obs-mip.fr (PP); mmj@st-andrews.ac.uk (MMJ); acc4@st-andrews.ac.uk (ACC);albert@cfht.hawaii.edu (LA); manset@cfht.hawaii.edu (NM); dintrans@ast.obs-mip.fr (BD); chabrier@ens-lyon.fr (GC); valenti@stsci.edu (JAV)

  18. Large-scale magnetic topologies of mid M dwarfs

    NASA Astrophysics Data System (ADS)

    Morin, J.; Donati, J.-F.; Petit, P.; Delfosse, X.; Forveille, T.; Albert, L.; Aurière, M.; Cabanac, R.; Dintrans, B.; Fares, R.; Gastine, T.; Jardine, M. M.; Lignières, F.; Paletou, F.; Ramirez Velez, J. C.; Théado, S.

    2008-10-01

    We present in this paper, the first results of a spectropolarimetric analysis of a small sample (~20) of active stars ranging from spectral type M0 to M8, which are either fully convective or possess a very small radiative core. This study aims at providing new constraints on dynamo processes in fully convective stars. This paper focuses on five stars of spectral type ~M4, i.e. with masses close to the full convection threshold (~=0.35Msolar), and with short rotational periods. Tomographic imaging techniques allow us to reconstruct the surface magnetic topologies from the rotationally modulated time-series of circularly polarized profiles. We find that all stars host mainly axisymmetric large-scale poloidal fields. Three stars were observed at two different epochs separated by ~1 yr; we find the magnetic topologies to be globally stable on this time-scale. We also provide an accurate estimation of the rotational period of all stars, thus allowing us to start studying how rotation impacts the large-scale magnetic field. Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT) and the Télescope Bernard Lyot (TBL). CFHT is operated by the National Research Council of Canada, the Institut National des Science de l'Univers of the Centre National de la Recherche Scientifique of France (INSU/CNRS) and the University of Hawaii, while the TBL is operated by CNRS/INSU. E-mail: jmorin@ast.obs-mip.fr (JM); donati@ast.obs-mip.fr (J-FD); petit@ast.obs-mip.fr (PP); xavier.delfosse@obs.ujf-grenoble.fr (XD); thierry.forveille@obs.ujf-grenoble.fr (TF); albert@cfht.hawaii.edu (LA); auriere@ast.obs-mip.fr (MA); remi.cabanac@ast.obs-mip.fr (RC); dintrans@ast.obs-mip.fr (BD); rfares@ast.obs-mip.fr (RF); tgastine@ast.obs-mip.fr (TG); mmj@st-andrews.ac.uk (MMJ); ligniere@ast.obs-mip.fr (FL); fpaletou@ast.obs-mip.fr (FP); jramirez@mesiog.obspm.fr (JR); sylvie.theado@ast.obs-mip.fr (ST)

  19. Large-scale magnetic topologies of early M dwarfs

    NASA Astrophysics Data System (ADS)

    Donati, J.-F.; Morin, J.; Petit, P.; Delfosse, X.; Forveille, T.; Aurière, M.; Cabanac, R.; Dintrans, B.; Fares, R.; Gastine, T.; Jardine, M. M.; Lignières, F.; Paletou, F.; Ramirez Velez, J. C.; Théado, S.

    2008-10-01

    We present here additional results of a spectropolarimetric survey of a small sample of stars ranging from spectral type M0 to M8 aimed at investigating observationally how dynamo processes operate in stars on both sides of the full convection threshold (spectral type M4). The present paper focuses on early M stars (M0-M3), that is above the full convection threshold. Applying tomographic imaging techniques to time series of rotationally modulated circularly polarized profiles collected with the NARVAL spectropolarimeter, we determine the rotation period and reconstruct the large-scale magnetic topologies of six early M dwarfs. We find that early-M stars preferentially host large-scale fields with dominantly toroidal and non-axisymmetric poloidal configurations, along with significant differential rotation (and long-term variability); only the lowest-mass star of our subsample is found to host an almost fully poloidal, mainly axisymmetric large-scale field resembling those found in mid-M dwarfs. This abrupt change in the large-scale magnetic topologies of M dwarfs (occurring at spectral type M3) has no related signature on X-ray luminosities (measuring the total amount of magnetic flux); it thus suggests that underlying dynamo processes become more efficient at producing large-scale fields (despite producing the same flux) at spectral types later than M3. We suspect that this change relates to the rapid decrease in the radiative cores of low-mass stars and to the simultaneous sharp increase of the convective turnover times (with decreasing stellar mass) that models predict to occur at M3; it may also be (at least partly) responsible for the reduced magnetic braking reported for fully convective stars. Based on observations obtained at the Télescope Bernard Lyot (TBL), operated by the Institut National des Science de l'Univers of the Centre National de la Recherche Scientifique of France. E-mail: donati@ast.obs-mip.fr (J-FD); jmorin@ast.obs-mip.fr (JM); petit

  20. The magnetic field of the planet-hosting star τ Bootis

    NASA Astrophysics Data System (ADS)

    Catala, C.; Donati, J.-F.; Shkolnik, E.; Bohlender, D.; Alecian, E.

    2007-01-01

    We have obtained high-resolution spectropolarimetric data for the planet-hosting star τ Bootis, using the ESPaDOnS spectropolarimeter at the Canada-France-Hawaii Telescope (CFHT). A weak but clear Stokes V signature is detected on three of the four nights of 2006 June during which we have recorded data. This polarimetric signature indicates with no ambiguity the presence of a magnetic field at the star's surface, with intensity of just a few gauss. The analysis of the photospheric lines of τ Boo at ultra-high signal-to-noise ratio reveals the presence of an 18 per cent relative differential rotation. Tentative Zeeman-Doppler imaging, using our spectropolarimetric observations covering only a fraction of the star's rotational phase, indicates a magnetic field with a dominant potential field component. The data are best fitted when a 3.1-d period of modulation and an intermediate inclination are assumed. Considering the level of differential rotation of τ Boo, this implies a rotation period of 3.0 d at the equator and of 3.7 d at the pole, and a topology of the magnetic field where its main non-axisymmetric part is located at low latitudes. The planet is probably synchronized with the star's rotation at intermediate latitudes, while the non-axisymmetric part of the magnetic field seems located at lower latitudes. Our limited data do not provide sufficient constraints on the magnetic field to study a possible interaction of the planet with the star's magnetosphere. Investigating this issue will require data with much better phase coverage. Similar studies should also be performed for other stars hosting close-in giant planets. Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. E-mail: Claude.Catala@obspm.fr (CC); Jean

  1. Complex magnetic topology and strong differential rotation on the low-mass T Tauri star V2247 Oph

    NASA Astrophysics Data System (ADS)

    Donati, J.-F.; Skelly, M. B.; Bouvier, J.; Jardine, M. M.; Gregory, S. G.; Morin, J.; Hussain, G. A. J.; Dougados, C.; Ménard, F.; Unruh, Y.

    2010-03-01

    From observations collected with the ESPaDOnS spectropolarimeter at the Canada-France-Hawaii Telescope, we report the detection of Zeeman signatures on the low-mass classical T Tauri star (cTTS) V2247 Oph. Profile distortions and circular polarization signatures detected in photospheric lines can be interpreted as caused by cool spots and magnetic regions at the surface of the star. The large-scale field is of moderate strength and highly complex; moreover, both the spot distribution and the magnetic field show significant variability on a time-scale of only 1 week, as a likely result of strong differential rotation. Both properties make V2247 Oph very different from the (more massive) prototypical cTTS BP Tau; we speculate that this difference reflects the lower mass of V2247 Oph. During our observations, V2247 Oph was in a low-accretion state, with emission lines showing only weak levels of circular polarization; we nevertheless find that excess emission apparently concentrates in a mid-latitude region of a strong radial field, suggesting that it is the footpoint of an accretion funnel. The weaker and more complex field that we report on V2247 Oph may share similarities with those of very-low-mass late-M dwarfs and potentially explain why low-mass cTTSs rotate on average faster than intermediate-mass ones. These surprising results need confirmation from new independent data sets on V2247 Oph and other similar low-mass cTTSs. Based on observations obtained at the Canada-France-Hawaii Telescope, operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France and the University of Hawaii. E-mail: donati@ast.obs-mip.fr (J-FD); mskelly@ast.obs-mip.fr (MBS); jerome.bouvier@obs.ujf-grenoble.fr (JB); mmj@st-andrews.ac.uk (MMJ); sg64@st-andrews.ac.uk (SGG); jmorin@ast.obs-mip.fr (JM); ghussain@eso.org (GAJH); catherine.dougados@obs.ujf-grenoble.fr (CD); francois

  2. Designing a new post-hole seismological station on Antarctica inlandsis (Concordia station)

    NASA Astrophysics Data System (ADS)

    Bès de Berc, M.; Maggi, A.; Leveque, J. J.; Thore, J. Y.

    2015-12-01

    of ice.The drilling will be carried out by the French drilling facility C2FN (Centre de Carottage et de Forage National) of the CNRS (Centre National de la Recherche Scientifique), and the is planned for the 2018-2019 summer season.

  3. The French Tsunami warning center for the Mediterranean and North-East Atlantic (CENtre d'ALerte aux Tsunamis, CENALT)

    NASA Astrophysics Data System (ADS)

    Schindelé, F.; Bossu, R.; Alabrune, N.; Arnoul, P.; Duperray, P.; Gailler, A.; Guilbert, J.; Hébert, H.; Hernandez, B.; Loevenbruck, A.; Roudil, P.

    2012-04-01

    The CENALT (CENtre d'Alerte aux Tsunamis) is responsible for the French NTWC (National Tsunami Warning Center). This center was established through a project that was requested by the French Ministry of Interior and the Ministry of Sustainable Development. It is implemented by the Commissariat à l'énergie atomique et aux énergies alternatives (CEA), the French Hydrographic and Oceanographic Service (SHOM) and the Centre National de la Recherche Scientifique (CNRS), and is based in Bruyères-le-Châtel (30 km from Paris). This center is based on three main components: seismic network data, sea level network data, dissemination system and processing and analyzing softwares and is operating on a 24/7 basis. The CENALT has established scientific cooperation with 8 institutions and implemented and funded private leased lines to exchange data with institutions from 5 different European countries (Germany, Italy, Portugal, Spain, Tunisia). The seismic data are processed with the Seiscomp 3 software. SHOM is working on making all French tide-gauge stations operated and available in real-time in 2012, and they installed 5 new tide gage stations. The tide gage data will be processed with a customized version of the Guitar (Gempa) software allowing the detection of tsunami signals, complemented by other softwares developed by the CEA. Historical tsunami databases (sources and observations) and earthquake databases, mostly based on available international databases, have been synthetized by CEA to produce information maps in real time, used to guide operators of permanence. Precomputed tsunami scenarios are implemented to build in real time maps of the highest tsunami impact expected in deep water. Along with an optimized tsunami modeling tool, these softwares help to define the areas where the tsunami may be observed and cause damage. The CENALT has been operating since early January 2012 as a pre-operational service and will be fully operational in July 2012. It is also

  4. Discovery of an extremely weak magnetic field in the white dwarf LTT 16093 = WD 2047+372

    NASA Astrophysics Data System (ADS)

    Landstreet, J. D.; Bagnulo, S.; Martin, A.; Valyavin, G.

    2016-06-01

    Context. Magnetic fields have been detected in several hundred white dwarfs, with strengths ranging from a few kG to several hundred MG. Only a few of the known fields have a mean magnetic field modulus below about 1 MG. Aims: We are searching for new examples of magnetic white dwarfs with very weak fields, and trying to model the few known examples. Our search is intended to be sensitive enough to detect fields at the few kG level. Methods: We have been surveying bright white dwarfs for very weak fields using spectropolarimeters at the Canada-France-Hawaii telescope, the William Herschel Telescope (WHT), the European Southern Observatory, and the Russian Special Astrophysical Observatory. We discuss in some detail tests of the WHT spectropolarimeter ISIS using the known magnetic strong-field Ap star HD 215441 (Babcock's star) and the long-period Ap star HD 201601 (γ Equ). Results: We report the discovery of a field with a mean field modulus of about 57 kG in the white dwarf LTT 16093 = WD 2047+372. The field is clearly detected through the Zeeman splitting of Hα seen in two separate circularly polarised spectra from two different spectropolarimeters. Zeeman circular polarisation is also detected, but only barely above the 3σ level. Conclusions: The discovery of this field is significant because it is the third weakest field ever unambiguously discovered in a white dwarf, while still being large enough that we should be able to model the field structure in some detail with future observations. Based on observations made with the William Herschel Telescope operated on the island of La Palma by the Isaac Newton Group in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias, and on observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and

  5. Weak lensing mass reconstruction of the galaxy cluster Abell 209

    NASA Astrophysics Data System (ADS)

    Paulin-Henriksson, S.; Antonuccio-Delogu, V.; Haines, C. P.; Radovich, M.; Mercurio, A.; Becciani, U.

    2007-05-01

    , the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  6. The low-mass population of the ρ Ophiuchi molecular cloud

    NASA Astrophysics Data System (ADS)

    Alves de Oliveira, C.; Moraux, E.; Bouvier, J.; Bouy, H.; Marmo, C.; Albert, L.

    2010-06-01

    Context. Star formation theories are currently divergent regarding the fundamental physical processes that dominate the substellar regime. Observations of nearby young open clusters allow the brown dwarf (BD) population to be characterised down to the planetary mass regime, which ultimately must be accommodated by a successful theory. Aims: We hope to uncover the low-mass population of the ρ Ophiuchi molecular cloud and investigate the properties of the newly found brown dwarfs. Methods: We used near-IR deep images (reaching completeness limits of approximately 20.5 mag in J and 18.9 mag in H and Ks) taken with the Wide Field IR Camera (WIRCam) at the Canada France Hawaii Telescope (CFHT) to identify candidate members of ρ Oph in the substellar regime. A spectroscopic follow-up of a small sample of the candidates allows us to assess their spectral type and subsequently their temperature and membership. Results: We select 110 candidate members of the ρ Ophiuchi molecular cloud, from which 80 have not previously been associated with the cloud. We observed a small sample of these and spectroscopically confirm six new brown dwarfs with spectral types ranging from M6.5 to M8.25. Based on observations obtained with WIRCam, a joint project of CFHT, Taiwan, Korea, Canada, France, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institute National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. Based on observations made at the ESO La Silla and Paranal Observatory under program 083.C-0092. Based in part on data collected at Subaru Telescope, and obtained from the SMOKA, which is operated by the Astronomy Data Center, National Astronomical Observatory of Japan. Research supported by the Marie Curie Research Training Network CONSTELLATION under grant No. MRTN-CT- 2006-035890.Table 4 is only available in electronic form at the CDS via

  7. Young T-dwarf candidates in IC 348

    NASA Astrophysics Data System (ADS)

    Burgess, A. S. M.; Moraux, E.; Bouvier, J.; Marmo, C.; Albert, L.; Bouy, H.

    2009-12-01

    Context: The determination of the lower-end of the initial mass function (IMF) provides strong constraints on star formation theories. Aims: We report here on a search for isolated planetary-mass objects in the 3 Myr-old star-forming region IC 348. Methods: Deep, narrowband CH4off and CH4on images were obtained with CFHT/WIRCam over 0.11 sq. deg. in the central part of IC 348 to identify young T-dwarfs from their 1.6 μm methane absorption bands. Results: We report three faint T-dwarf candidates with CH4on-CH4off colours >0.4 mag. Extinction was estimated for each candidate and lies in the range AV ~ 5-12 mag. Comparisons with T-dwarf spectral models, and colour/colour and colour/magnitude diagrams, reject two of the three candidates because of their extreme z'-J blueness. The one remaining object is not thought to be a foreground field dwarf because of a number density argument and also its strong extinction AV ~ 12 mag, or thought to be a background field T-dwarf which would be expected to be much fainter. Models and diagrams give this object a preliminary T6 spectral type. Conclusions: With a few Jupiter masses, the young T-dwarf candidate reported here is potentially amongst the youngest, lowest mass objects detected in a star-forming region so far. Its frequency is consistent with the extrapolation of current lognormal IMF estimates down to the planetary mass domain. Based on observations obtained with WIRCam, a joint project of CFHT, Taiwan, Korea, Canada, France, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institute National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the “University of Hawaii. Research supported by the Marie Curie Research Training Network CONSTELLATION” under grant no. MRTN-CT-2006-035890.

  8. Approche à l’endroit des blessures traumatiques à la main en soins primaires

    PubMed Central

    Cheung, Kevin; Hatchell, Alexandra; Thoma, Achilleas

    2013-01-01

    Résumé Objectif Passer en revue la prise en charge initiale des blessures traumatiques communes à la main que voient les médecins de soins primaires. Sources des données Nous avons examiné les données cliniques probantes et les ouvrages spécialisés récents cernés par des recherches dans la base de données électronique MEDLINE. Nous avons utilisé l’opinion d’experts pour compléter les recommandations dans les domaines où les données scientifiques étaient rares. Message principal Les médecins de soins primaires sont couramment appelés à prendre en charge des patients victimes de blessures traumatiques à la main. Dans le contexte d’un cas clinique, nous examinons l’évaluation, le diagnostic et la prise en charge initiale des traumatismes communs à la main. La présentation et la prise en charge des blessures au lit de l’ongle, des amputations de l’extrémité du doigt, des doigts en maillet, des fractures à la main, des lacérations de tendons, des morsures et de la ténosynovite infectieuse seront aussi discutées. Les principes de la prise en charge des blessures traumatiques à la main comportent la réduction et l’immobilisation des fractures, la prescription d’imagerie radiographique post-réduction, l’obtention d’un recouvrement par les tissus mous, la prévention et le traitement des infections et l’assurance d’une prophylaxie antitétanique. Conclusion Il est essentiel d’assurer une évaluation et une prise en charge appropriées des blessures traumatiques à la main pour prévenir une morbidité considérable à long terme dans une population autrement en santé. La reconnaissance sans délai des blessures qui nécessitent une demande de consultation urgente ou rapide auprès d’un chirurgien spécialiste de la main est également critique.

  9. CoRoT's view of newly discovered B-star pulsators: results for 358 candidate B pulsators from the initial run's exoplanet field data

    NASA Astrophysics Data System (ADS)

    Degroote, P.; Aerts, C.; Ollivier, M.; Miglio, A.; Debosscher, J.; Cuypers, J.; Briquet, M.; Montalbán, J.; Thoul, A.; Noels, A.; De Cat, P.; Balaguer-Núñez, L.; Maceroni, C.; Ribas, I.; Auvergne, M.; Baglin, A.; Deleuil, M.; Weiss, W. W.; Jorda, L.; Baudin, F.; Samadi, R.

    2009-10-01

    Context: We search for new variable B-type pulsators in the CoRoT data assembled primarily for planet detection, as part of CoRoT's additional programme. Aims: We aim to explore the properties of newly discovered B-type pulsators from the uninterrupted CoRoT space-based photometry and to compare them with known members of the β Cep and slowly pulsating B star (SPB) classes. Methods: We developed automated data analysis tools that include algorithms for jump correction, light-curve detrending, frequency detection, frequency combination search, and for frequency and period spacing searches. Results: Besides numerous new, classical, slowly pulsating B stars, we find evidence for a new class of low-amplitude B-type pulsators between the SPB and δ Sct instability strips, with a very broad range of frequencies and low amplitudes, as well as several slowly pulsating B stars with residual excess power at frequencies typically a factor three above their expected g-mode frequencies. Conclusions: The frequency data we obtained for numerous new B-type pulsators represent an appropriate starting point for further theoretical analyses of these stars, once their effective temperature, gravity, rotation velocity, and abundances will be derived spectroscopically in the framework of an ongoing FLAMES survey at the VLT. The CoRoT space mission was developed and is operated by the French space agency CNES, with the participation of ESA's RSSD and Science Programmes, Austria, Belgium, Brazil, Germany, and Spain. All frequency tables, including the identification of combination frequencies, are only available as online material. Frequency Tables are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/506/471 Bâtiment 121, 91405, Orsay Cedex, France. Postdoctoral Researcher, Fonds de la Recherche Scientifique - FNRS, Belgium. Postdoctoral Fellow of the Fund for Scientific Research

  10. We Care for Clean Air! The Contribution of ACCENT to Education and Communication

    NASA Astrophysics Data System (ADS)

    Schuepbach, Eva; Brimblecombe, Peter; Gross, Krisjanis; Jacobs, Mark J.; Ladstätter-Weißenmayer, Annette; Moussiopoulos, Nicolas; Slini, Theodora; Übelis, Arnolds; Uherek, Elmar

    2010-05-01

    A new booklet on: "We Care for Clean Air! Motivating the Next Generation of Atmospheric Scientists" (ISBN 978-88-95665-01-6) as recently published by the education community in ACCENT (www.accent-network.org/portal/education) is presented. Promoting creative and innovative researchers and teachers and encouraging the next generation to move into the field were among the key issues in ACCENT "Training and Education" (T&E). During the 5-year programme, a wealth of educational events (e.g., workshops) and programmes (e.g., "ACCENT FAR EAST") were organized and tools developed for teachers and learners at Universities and Schools around the globe. Activities such as National ACCENT Days or Cafés Scientifiques also targeted stakeholders, policy makers and the general public to increase the expertise in atmospheric composition change to a common level across Europe. The volume introduces the integrated learning environment, high-quality tools and methods for air quality and climate change science education created by ACCENT T&E, and provides an overview on the unbiased scientific information that has been didactically translated based on knowledge available from ongoing research projects.The core messages are that (i) the translation of complex issues in atmospheric composition and climate change science to non-scientists should be scientifically acceptable and that (ii) scientists should stay in control of the translation process. After the publication of the 4th Assessment Report of the Intergovernmental Panel for Climate Change (IPCC) in 2007, ACCENT intensified its efforts to reach greater visibility and distribute the body of know-how, skills and competencies within the networked community of atmospheric scientists in the World Wide Web. For example, a Special Issue of the "Global Change Magazine for Schools" on IPCC 2007 contains a compact introduction to the basics of global warming for direct application in the classroom, also focusing on uncertainties and

  11. An investigation of the magnetic properties of the classical Be star ω Ori by the MiMeS Collaboration

    NASA Astrophysics Data System (ADS)

    Neiner, C.; Grunhut, J. H.; Petit, V.; ud-Doula, A.; Wade, G. A.; Landstreet, J.; de Batz, B.; Cochard, F.; Gutiérrez-Soto, J.; Huat, A.-L.

    2012-11-01

    hosts a stable, organized (fossil) magnetic field that is responsible for the observed phenomena, but with a strength that is below our current detection threshold. Of these three scenarios, we consider the second one (dynamo process) as highly unlikely, whereas the other two should be falsifiable with intense monitoring. Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France and the University of Hawaii and observations obtained with the Narval spectropolarimeter at the Télescope Bernard Lyot (TBL), Observatoire du Pic du Midi, France.

  12. Critical Evaluation of Magnetic Field Detections Reported for Pulsating B-type Stars in Light of ESPaDOnS, Narval, and Reanalyzed FORS1/2 Observations

    NASA Astrophysics Data System (ADS)

    Shultz, M.; Wade, G. A.; Grunhut, J.; Bagnulo, S.; Landstreet, J. D.; Neiner, C.; Alecian, E.; Hanes, D.; MiMeS Collaboration

    2012-05-01

    Recent spectropolarimetric studies of seven slowly pulsating B (SPB) and β Cep stars have suggested that photospheric magnetic fields are more common in B-type pulsators than in the general population of B stars, suggesting a significant connection between magnetic and pulsational phenomena. We present an analysis of new and previously published spectropolarimetric observations of these stars. New Stokes V observations obtained with the high-resolution ESPaDOnS and Narval instruments confirm the presence of a magnetic field in one of the stars (epsilon Lup), but find no evidence of magnetism in five others. A re-analysis of the published longitudinal field measurements obtained with the low-resolution FORS1/2 spectropolarimeters finds that the measurements of all stars show more scatter from zero than can be attributed to Gaussian noise, suggesting the presence of a signal and/or systematic underestimation of error bars. Re-reduction and re-measurement of the FORS1/2 spectra from the ESO archive demonstrates that small changes in reduction procedure lead to substantial changes in the inferred longitudinal field, and substantially reduces the number of field detections at the 3σ level. Furthermore, we find that the published periods are not unique solutions to the time series of either the original or the revised FORS1/2 data. We conclude that the reported field detections, proposed periods, and field geometry models for α Pyx, 15 CMa, 33 Eri, and V1449 Aql are artifacts of the data analysis and reduction procedures, and that magnetic fields at the reported strength are no more common in SPB/β Cep stars than in the general population of B stars. This work is also based on data obtained from the ESO Science Archive, Facility. Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT), which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of

  13. Extremely Red Objects in Two Quasar Fields at z ~ 1.4

    NASA Astrophysics Data System (ADS)

    Stockton, Alan; McGrath, Elizabeth; Canalizo, Gabriela

    2006-10-01

    We present an investigation of the properties and environments of bright extremely red objects (EROs) found in the fields of the quasars TXS 0145+386 and 4C 15.55, both at z~1.4. There is marginal evidence from Chandra Advanced CCD Imaging Spectrometer (ACIS) imaging for hot cluster gas with a luminosity of a few 1044 ergs s-1 in the field of 4C 15.55. The TXS 0145+386 field has an upper limit at a similar value, but it also clearly shows an overdensity of faint galaxies. None of the EROs are detected as X-ray sources. For two of the EROs that have spectral energy distributions and rest-frame near-UV spectra that show that they are strongly dominated by old stellar populations, we determine radial surface brightness profiles from adaptive optics images. Both of these galaxies are best fit by profiles close to exponentials, plus a compact nucleus comprising ~30% of the total light in one case and 8% in the other. Neither is well fit by an r1/4-law profile. This apparent evidence for the formation of massive ~2×1011 disks of old stars in the early universe indicates that at least some galaxies formed essentially monolithically, with high star formation rates sustained over a few 108 yr and without the aid of major mergers. Based in part on data collected at the Subaru Telescope, which is operated by the National Astronomical Observatory of Japan; on data obtained with the Chandra X-Ray Observatory, which is operated for NASA by the Smithsonian Astrophysical Observatory; on data obtained at the Canada-France-Hawaii Telescope, which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii; and on data obtained at the the United Kingdom Infrared Telescope, which is operated by the Joint Astronomy Centre on behalf of the UK. Particle Physics and Astronomy Research Council. Some of the data presented herein were obtained at the W. M

  14. The Spatial Distribution of Galaxies of Different Spectral Types in the Massive Intermediate-Redshift Cluster MACS J0717.5+3745

    NASA Astrophysics Data System (ADS)

    Ma, Cheng-Jiun; Ebeling, Harald; Donovan, David; Barrett, Elizabeth

    2008-09-01

    Canada, the Institute National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. The spectroscopic data presented herein were obtained at the W.M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W.M. Keck Foundation.

  15. New neighbours. III. 21 new companions to nearby dwarfs, discovered with adaptive optics

    NASA Astrophysics Data System (ADS)

    Beuzit, J.-L.; Ségransan, D.; Forveille, T.; Udry, S.; Delfosse, X.; Mayor, M.; Perrier, C.; Hainaut, M.-C.; Roddier, C.; Roddier, F.; Martín, E. L.

    2004-10-01

    We present some results of a CFHT adaptive optics search for companions to nearby dwarfs. We identify 21 new components in solar neighbourhood systems, of which 13 were found while surveying a volume-limited sample of M dwarfs within 12 pc. We are obtaining complete observations for this subsample, to derive unbiased multiplicity statistics for the very-low-mass disk population. Additionally, we resolve for the first time 6 known spectroscopic or astrometric binaries, for a total of 27 newly resolved companions. A significant fraction of the new binaries has favourable parameters for accurate mass determinations. The newly resolved companion of Gl 120.1C was thought to have a spectroscopic minimum mass in the brown-dwarf range (Duquennoy & Mayor \\cite{duquennoy91}), and it contributed to the statistical evidence that a few percent of solar-type stars might have close-in brown-dwarf companions. We find that Gl 120.1C actually is an unrecognised double-lined spectroscopic pair. Its radial-velocity amplitude had therefore been strongly underestimated by Duquennoy & Mayor (\\cite{duquennoy91}), and it does not truly belong to their sample of single-lined systems with minimum spectroscopic mass below the substellar limit. We also present the first direct detection of Gl 494B, an astrometric brown-dwarf candidate. Its luminosity straddles the substellar limit, and it is a brown dwarf if its age is less than ˜300 Myr. A few more years of observations will ascertain its mass and status from first principles. Based on observations made at Canada-France-Hawaii Telescope, operated by the National Research Council of Canada, the Centre National de la Recherche Scientifique de France and the University of Hawaii. Some of the data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and the National Aeronautics and Space Administration. The

  16. Identifying the Young Low-mass Stars within 25 pc. I. Spectroscopic Observations

    NASA Astrophysics Data System (ADS)

    Shkolnik, Evgenya; Liu, Michael C.; Reid, I. Neill

    2009-07-01

    the Canada-France-Hawaii Telescope. The Keck Observatory is operated as a scientific partnership between the California Institute of Technology, the University of California, and NASA, and was made possible by the generous financial support of the W. M. Keck Foundation. The CFHT is operated by the National Research Council of Canada, the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  17. HN Peg B: A Test of Models of the L to T Dwarf Transition

    NASA Astrophysics Data System (ADS)

    Leggett, S. K.; Saumon, D.; Albert, Loic; Cushing, Michael C.; Liu, Michael C.; Luhman, K. L.; Marley, M. S.; Kirkpatrick, J. Davy; Roellig, Thomas L.; Allers, K. N.

    2008-08-01

    Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  18. Stellar Evolution in NGC 6791: Mass Loss on the Red Giant Branch and the Formation of Low-Mass White Dwarfs

    NASA Astrophysics Data System (ADS)

    Kalirai, Jasonjot S.; Bergeron, P.; Hansen, Brad M. S.; Kelson, Daniel D.; Reitzel, David B.; Rich, R. Michael; Richer, Harvey B.

    2007-12-01

    Canada-France-Hawaii Telescope (CFHT), which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  19. A Statistical Study of Multiply Imaged Systems in the Lensing Cluster Abell 68

    NASA Astrophysics Data System (ADS)

    Richard, Johan; Kneib, Jean-Paul; Jullo, Eric; Covone, Giovanni; Limousin, Marceau; Ellis, Richard; Stark, Daniel; Bundy, Kevin; Czoske, Oliver; Ebeling, Harald; Soucail, Geneviève

    2007-06-01

    (program 8249) obtained at the Space Telescope Science Institute, which is operated by AURA under NASA contract NAS5-26555, and the Canada-France-Hawaii Telescope (CFHT), which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  20. BD -22 5866: A Low-Mass, Quadruple-lined Spectroscopic and Eclipsing Binary

    NASA Astrophysics Data System (ADS)

    Shkolnik, Evgenya; Liu, Michael C.; Reid, I. Neill; Hebb, Leslie; Cameron, Andrew C.; Torres, Carlos A.; Wilson, David M.

    2008-08-01

    of California, and NASA, and was made possible by the generous financial support of the W. M. Keck Foundation. The CFHT is operated by the National Research Council of Canada, the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  1. Kinematics and Metallicity of M31 Red Giants: The Giant Southern Stream and Discovery of a Second Cold Component at R=20 kpc

    NASA Astrophysics Data System (ADS)

    Kalirai, Jasonjot S.; Guhathakurta, Puragra; Gilbert, Karoline M.; Reitzel, David B.; Majewski, Steven R.; Rich, R. Michael; Cooper, Michael C.

    2006-04-01

    generous financial support of the W. M. Keck Foundation. Based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT), which is operated by the National Research Council (NRC) of Canada, the Institut National des Science de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii.

  2. Photometric redshifts as a tool for studying the Coma cluster galaxy populations

    NASA Astrophysics Data System (ADS)

    Adami, C.; Ilbert, O.; Pelló, R.; Cuillandre, J. C.; Durret, F.; Mazure, A.; Picat, J. P.; Ulmer, M. P.

    2008-12-01

    Aims: We apply photometric redshift techniques to an investigation of the Coma cluster galaxy luminosity function (GLF) at faint magnitudes, in particular in the u* band where basically no studies are presently available at these magnitudes. Methods: Cluster members were selected based on probability distribution function from photometric redshift calculations applied to deep u^*, B, V, R, I images covering a region of almost 1 deg2 (completeness limit R ~ 24). In the area covered only by the u* image, the GLF was also derived after a statistical background subtraction. Results: Global and local GLFs in the B, V, R, and I bands obtained with photometric redshift selection are consistent with our previous results based on a statistical background subtraction. The GLF in the u* band shows an increase in the faint end slope towards the outer regions of the cluster. The analysis of the multicolor type spatial distribution reveals that late type galaxies are distributed in clumps in the cluster outskirts, where X-ray substructures are also detected and where the GLF in the u* band is steeper. Conclusions: We can reproduce the GLFs computed with classical statistical subtraction methods by applying a photometric redshift technique. The u* GLF slope is steeper in the cluster outskirts, varying from α ~ -1 in the cluster center to α ~ -2 in the cluster periphery. The concentrations of faint late type galaxies in the cluster outskirts could explain these very steep slopes, assuming a short burst of star formation in these galaxies when entering the cluster. Based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. This work is also partly based on data products produced at

  3. Weak lensing study of 16 DAFT/FADA clusters: Substructures and filaments

    NASA Astrophysics Data System (ADS)

    Martinet, Nicolas; Clowe, Douglas; Durret, Florence; Adami, Christophe; Acebrón, Ana; Hernandez-García, Lorena; Márquez, Isabel; Guennou, Loic; Sarron, Florian; Ulmer, Mel

    2016-05-01

    While our current cosmological model places galaxy clusters at the nodes of a filament network (the cosmic web), we still struggle to detect these filaments at high redshifts. We perform a weak lensing study for a sample of 16 massive, medium-high redshift (0.4 Scientifique (CNRS) of

  4. The chemical composition of TS 01, the most oxygen-deficient planetary nebula. AGB nucleosynthesis in a metal-poor binary star

    NASA Astrophysics Data System (ADS)

    Stasińska, G.; Morisset, C.; Tovmassian, G.; Rauch, T.; Richer, M. G.; Peña, M.; Szczerba, R.; Decressin, T.; Charbonnel, C.; Yungelson, L.; Napiwotzki, R.; Simón-Díaz, S.; Jamet, L.

    2010-02-01

    -France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.Based on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555.Based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under NASA contract 1407.

  5. Éthique de la recherche en santé mondiale : la relation Nord-Sud, quel partenariat pour quelle justice sociale ?

    PubMed

    Godard, Béatrice; Hunt, Matthew; Moube, Zéphirin

    2014-03-01

    La recherche en santé mondiale s'inscrit dans une volonté de mobiliser des connaissances au service d'interventions et de politiques publiques pour l'atteinte équitable du bien-être commun, notamment en matière de santé. Elle joue un rôle primordial en ce sens, en favorisant l'implication des communautés et leur autonomisation et de nombreuses lignes directrices supportent un tel partenariat. Néanmoins, certains enjeux éthiques sont liés au financement de la recherche, aux environnements de recherche, à la priorisation des problématiques de recherche, aux mécanismes d'évaluation éthique posent souvent un problème de justice sociale au niveau de la redistribution des ressources et de la reconnaissance des différences culturelles. Comment alors déterminer quelle est la façon « idéale » d'agir en tenant compte de la globalité des individus et du pluralisme culturel des sociétés pour « bien faire », pour satisfaire l'exigence de l'équité? Une réflexion et une démarche éthique demeurent essentielles, ainsi qu'un dialogue entre les chercheurs du Nord et du Sud, et leurs autres partenaires que sont les décideurs, les responsables locaux et les communautés. Un tel dialogue, établi dans un continuum du développement de projets de recherche à leur pérennité, peut grandement contribuer à limiter les problèmes de justice sociale et à viser un développement plus égalitaire des savoirs scientifiques. Plusieurs chercheurs se sont déjà engagés dans cette voie, et leurs initiatives devraient être encouragées pour mettre les nouveaux savoirs au service des populations. PMID:24594489

  6. SALT2: using distant supernovae to improve the use of type Ia supernovae as distance indicators

    NASA Astrophysics Data System (ADS)

    Guy, J.; Astier, P.; Baumont, S.; Hardin, D.; Pain, R.; Regnault, N.; Basa, S.; Carlberg, R. G.; Conley, A.; Fabbro, S.; Fouchez, D.; Hook, I. M.; Howell, D. A.; Perrett, K.; Pritchet, C. J.; Rich, J.; Sullivan, M.; Antilogus, P.; Aubourg, E.; Bazin, G.; Bronder, J.; Filiol, M.; Palanque-Delabrouille, N.; Ripoche, P.; Ruhlmann-Kleider, V.

    2007-04-01

    Aims:We present an empirical model of type Ia supernovae spectro-photometric evolution with time. Methods: The model is built using a large data set including light-curves and spectra of both nearby and distant supernovae, the latter being observed by the SNLS collaboration. We derive the average spectral sequence of type Ia supernovae and their main variability components including a color variation law. The model allows us to measure distance moduli in the spectral range 2500-8000 Å with calculable uncertainties, including those arising from variability of spectral features. Results: Thanks to the use of high-redshift SNe to model the rest-frame UV spectral energy distribution, we are able to derive improved distance estimates for SNe Ia in the redshift range 0.8Scientifique (CNRS) of France, and the University of Hawaii. This work is based in part on data products produced at the Canadian Astronomy Data Centre as part of the Canada-France-Hawaii Telescope Legacy Survey, a collaborative project of NRC and CNRS. Based on observations obtained at the European Southern Observatory using the Very Large Telescope on the Cerro Paranal (ESO Large Programme 171.A-0486). Based on observations (programs GN-2004A-Q-19, GS-2004A-Q-11, GN-2003B-Q-9, and GS-2003B-Q-8) obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the Particle Physics and

  7. CSI 2264: Characterizing Young Stars in NGC 2264 with Stochastically Varying Light Curves

    NASA Astrophysics Data System (ADS)

    Stauffer, John; Cody, Ann Marie; Rebull, Luisa; Hillenbrand, Lynne A.; Turner, Neal J.; Carpenter, John; Carey, Sean; Terebey, Susan; Morales-Calderón, María; Alencar, Silvia H. P.; McGinnis, Pauline; Sousa, Alana; Bouvier, Jerome; Venuti, Laura; Hartmann, Lee; Calvet, Nuria; Micela, Giusi; Flaccomio, Ettore; Song, Inseok; Gutermuth, Rob; Barrado, David; Vrba, Frederick J.; Covey, Kevin; Herbst, William; Gillen, Edward; Medeiros Guimarães, Marcelo; Bouy, Herve; Favata, Fabio

    2016-03-01

    . MegaCam is a joint project of CFHT and CEA/DAPNIA, which is operated by the National Research Council (NRC) of Canada, the Institute National des Sciences de l’Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  8. Evidence for major mergers of galaxies at 2 ≲ z < 4 in the VVDS and VUDS surveys

    NASA Astrophysics Data System (ADS)

    Tasca, L. A. M.; Le Fèvre, O.; López-Sanjuan, C.; Wang, P.-W.; Cassata, P.; Garilli, B.; Ilbert, O.; Le Brun, V.; Lemaux, B. C.; Maccagni, D.; Tresse, L.; Bardelli, S.; Contini, T.; Charlot, S.; Cucciati, O.; Fontana, A.; Giavalisco, M.; Kneib, J.-P.; Salvato, M.; Taniguchi, Y.; Vergani, D.; Zamorani, G.; Zucca, E.

    2014-05-01

    -0791. Based on observations obtained with MegaPrime/MegaCam, a joint project of the CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT), which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii.

  9. Photometry of supernovae in an image series: methods and application to the SuperNova Legacy Survey (SNLS)

    NASA Astrophysics Data System (ADS)

    Astier, P.; El Hage, P.; Guy, J.; Hardin, D.; Betoule, M.; Fabbro, S.; Fourmanoit, N.; Pain, R.; Regnault, N.

    2013-09-01

    Aims: We present a technique to measure lightcurves of time-variable point sources on a spatially structured background from imaging data. The technique was developed to measure lightcurves of SNLS supernovae in order to infer their distances. This photometry technique performs simultaneous point spread function (PSF) photometry at the same sky position on an image series. Methods: We describe two implementations of the method: one that resamples images before measuring fluxes, and one which does not. In both instances, we sketch the key algorithms involved and present the validation using semi-artificial sources introduced in real images in order to assess the accuracy of the supernova flux measurements relative to that of surrounding stars. We describe the methods required to anchor these PSF fluxes to calibrated aperture catalogs, in order to derive SN magnitudes. Results: We find a marginally significant bias of 2 mmag of the after-resampling method, and no bias at the mmag accuracy for the non-resampling method. Given surrounding star magnitudes, we determine the systematic uncertainty of SN magnitudes to be less than 1.5 mmag, which represents about one third of the current photometric calibration uncertainty affecting SN measurements. The SN photometry delivers several by-products: bright star PSF flux measurements which have a repeatability of about 0.6%, as for aperture measurements; we measure relative astrometric positions with a noise floor of 2.4 mas for a single-image bright star measurement; we show that in all bands of the MegaCam instrument, stars exhibit a profile linearly broadening with flux by about 0.5% over the whole brightness range. Based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique (CNRS

  10. Near-infrared properties of asymptotic giant branch stars in nearby dwarf elliptical galaxy NGC 205

    NASA Astrophysics Data System (ADS)

    Jung, M. Y.; Ko, J.; Kim, J.-W.; Chun, S.-H.; Kim, H.-I.; Sohn, Y.-J.

    2012-07-01

    , the Centre National de la Recherche Scientifique de France, and the University of Hawaii.Calibrated photometry is only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/543/A35

  11. Seasonal variability of suspended sediment transport in the Seine river catchment area (France)

    NASA Astrophysics Data System (ADS)

    Franke, Christine; Baati, Selma; Ayrault, Sophie; Bonte, Philippe; Evrard, Olivier; Kissel, Catherine

    2010-05-01

    , C., Kissel, C., Robin, E., Bonté, P. and Lagroix, F., 2009, Magnetic particle characterization in the Seine river system: Implications for the determination of natural versus anthropogenic input, Geochem. Geophys. Geosyst., doi:10.1029/2009GC002544. Tessier, L., Bonté, P., Mouchel, J.M., Lefevre, I., Sogon, S., Ayrault, S., Le Cloarec, M.F., 2003, Transport et characterisation des matieres en suspension dans le basin de la Seine : Identification des signatures naturelles et anthropiques, 14èmes Journées Scientifiques de l'Environnement : l'Eau, la Ville, la Vie, Créteil : France 2003. http://hal.archives-ouvertes.fr/docs/00/20/30/84/PDF/4-JSE-2003-Manuscrit-Tessier-HAL-2008-01-08.pdf

  12. The Globular Cluster NGC 2419: A Crucible for Theories of Gravity

    NASA Astrophysics Data System (ADS)

    Ibata, R.; Sollima, A.; Nipoti, C.; Bellazzini, M.; Chapman, S. C.; Dalessandro, E.

    2011-09-01

    . M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation. This paper was also based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institute National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  13. Metal Abundances, Radial Velocities, and Other Physical Characteristics for the RR Lyrae Stars in The Kepler Field

    NASA Astrophysics Data System (ADS)

    Nemec, James M.; Cohen, Judith G.; Ripepi, Vincenzo; Derekas, Aliz; Moskalik, Pawel; Sesar, Branimir; Chadid, Merieme; Bruntt, Hans

    2013-08-01

    observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National Des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  14. Confidence Level and Sensitivity Limits in High-Contrast Imaging

    NASA Astrophysics Data System (ADS)

    Marois, Christian; Lafrenière, David; Macintosh, Bruce; Doyon, René

    2008-01-01

    In long adaptive optics corrected exposures, exoplanet detections are currently limited by speckle noise originating from the telescope and instrument optics, and it is expected that such noise will also limit future high-contrast imaging instruments for both ground- and space-based telescopes. Previous theoretical analyses have shown that the time intensity variations of a single speckle follow a modified Rician. It is first demonstrated here that for a circular pupil, this temporal intensity distribution also represents the speckle spatial intensity distribution at a fixed separation from the point-spread function center; this fact is demonstrated using numerical simulations for coronagraphic and noncoronagraphic data. The real statistical distribution of the noise needs to be taken into account explicitly when selecting a detection threshold appropriate for some desired confidence level (CL). In this paper, a technique is described to obtain the pixel intensity distribution of an image and its corresponding CL as a function of the detection threshold. Using numerical simulations, it is shown that in the presence of speckle noise, a detection threshold up to 3 times higher is required to obtain a CL equivalent to that at 5 σ for Gaussian noise. The technique is then tested on data acquired by simultaneous spectral differential imaging with TRIDENT and by angular differential imaging with NIRI. It is found that the angular differential imaging technique produces quasi-Gaussian residuals, a remarkable result compared to classical adaptive optic imaging. Finally, a power law is derived to predict the 1 - 3 × 10-7 CL detection threshold when averaging a partially correlated non-Gaussian noise. Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT), which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of

  15. Two spotted and magnetic early B-type stars in the young open cluster NGC 2264 discovered by MOST and ESPaDOnS

    NASA Astrophysics Data System (ADS)

    Fossati, L.; Zwintz, K.; Castro, N.; Langer, N.; Lorenz, D.; Schneider, F. R. N.; Kuschnig, R.; Matthews, J. M.; Alecian, E.; Wade, G. A.; Barnes, T. G.; Thoul, A. A.

    2014-02-01

    Aerospace Studies and the University of British Columbia with the assistance of the University of Vienna.Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Science de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  16. Identifying the Young Low-mass Stars within 25 pc. II. Distances, Kinematics, and Group Membership

    NASA Astrophysics Data System (ADS)

    Shkolnik, Evgenya L.; Anglada-Escudé, Guillem; Liu, Michael C.; Bowler, Brendan P.; Weinberger, Alycia J.; Boss, Alan P.; Reid, I. Neill; Tamura, Motohide

    2012-10-01

    support of the W. M. Keck Foundation. The CFHT is operated by the National Research Council of Canada, the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  17. Magnetic field topology of τ Scorpii. The uniqueness problem of Stokes V ZDI inversions

    NASA Astrophysics Data System (ADS)

    Kochukhov, O.; Wade, G. A.

    2016-02-01

    field topology ambiguous. Stokes Q and U spectropolarimetric observations represent the only way of breaking the degeneracy of surface magnetic field models. Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  18. La stimulation magnétique transcrânienne (SMT) dans la recherche fondamentale et clinique en neuroscience

    PubMed Central

    Valero-Cabré, Antoni; Pascual-Leone, Alvaro; Coubard, Olivier A.

    2011-01-01

    Introduction Les méthodes de stimulation cérébrale non invasives telles que la Stimulation Magnétique Transcrânienne (SMT) sont largement utilisées pour établir des inférences causales sur les relations entre cerveau et comportement. Des applications cliniques basées sur la SMT ont également été développées pour traiter des affections neurologiques ou psychiatriques comme la dépression, la dystonie, la douleur, les acouphènes ou les séquelles d’accident vasculaire cérébral. État des connaissances La SMT fonctionne en induisant de manière non invasive et de manière focale des courants électriques dans des régions corticales, modulant ainsi leur niveau d’activité de façon variable suivant la fréquence, le nombre d’impulsions, les intervalles et la durée de stimulation utilisés. S’agissant du cortex moteur, on sait par exemple que les patterns d’impulsions de SMT à basse fréquence ou ceux délivrées de manière continue tendent à déprimer l’activité locale, tandis que la SMT à haute fréquence et discontinus tend à la potentialiser. Outre ses effets locaux, la SMT peut aussi avoir des effets à distance sur les régions cérébrales, véhiculés par les connections anatomiques et qui dépendent de l’efficacité et du signe de ces connexions. Perspectives Dans le domaine de la recherche fondamentale et des applications thérapeutiques, l’utilisation efficace de la SMT requiert, cependant, la compréhension approfondie de ses principes opérationnels, de ses risques, de ses potentialités et de ses limites. Dans cet article, nous présentons les principes par lesquels opèrent les méthodes de stimulation cérébrale non invasive, et en particulier la SMT. Conclusion À l’issue de sa lecture, le lecteur sera en mesure de discuter de façon critique les études scientifiques et cliniques utilisant la SMT, ainsi que de concevoir des applications SMT suivant une hypothèse a priori dans le domaine de la recherche en

  19. The SECOQC quantum key distribution network in Vienna

    NASA Astrophysics Data System (ADS)

    Peev, M.; Pacher, C.; Alléaume, R.; Barreiro, C.; Bouda, J.; Boxleitner, W.; Debuisschert, T.; Diamanti, E.; Dianati, M.; Dynes, J. F.; Fasel, S.; Fossier, S.; Fürst, M.; Gautier, J.-D.; Gay, O.; Gisin, N.; Grangier, P.; Happe, A.; Hasani, Y.; Hentschel, M.; Hübel, H.; Humer, G.; Länger, T.; Legré, M.; Lieger, R.; Lodewyck, J.; Lorünser, T.; Lütkenhaus, N.; Marhold, A.; Matyus, T.; Maurhart, O.; Monat, L.; Nauerth, S.; Page, J.-B.; Poppe, A.; Querasser, E.; Ribordy, G.; Robyr, S.; Salvail, L.; Sharpe, A. W.; Shields, A. J.; Stucki, D.; Suda, M.; Tamas, C.; Themel, T.; Thew, R. T.; Thoma, Y.; Treiber, A.; Trinkler, P.; Tualle-Brouri, R.; Vannel, F.; Walenta, N.; Weier, H.; Weinfurter, H.; Wimberger, I.; Yuan, Z. L.; Zbinden, H.; Zeilinger, A.

    2009-07-01

    In this paper, we present the quantum key distribution (QKD) network designed and implemented by the European project SEcure COmmunication based on Quantum Cryptography (SECOQC) (2004-2008), unifying the efforts of 41 research and industrial organizations. The paper summarizes the SECOQC approach to QKD networks with a focus on the trusted repeater paradigm. It discusses the architecture and functionality of the SECOQC trusted repeater prototype, which has been put into operation in Vienna in 2008 and publicly demonstrated in the framework of a SECOQC QKD conference held from October 8 to 10, 2008. The demonstration involved one-time pad encrypted telephone communication, a secure (AES encryption protected) video-conference with all deployed nodes and a number of rerouting experiments, highlighting basic mechanisms of the SECOQC network functionality. The paper gives an overview of the eight point-to-point network links in the prototype and their underlying technology: three plug and play systems by id Quantique, a one way weak pulse system from Toshiba Research in the UK, a coherent one-way system by GAP Optique with the participation of id Quantique and the AIT Austrian Institute of Technology (formerly ARCAustrian Research Centers GmbH—ARC is now operating under the new name AIT Austrian Institute of Technology GmbH following a restructuring initiative.), an entangled photons system by the University of Vienna and the AIT, a continuous-variables system by Centre National de la Recherche Scientifique (CNRS) and THALES Research and Technology with the participation of Université Libre de Bruxelles, and a free space link by the Ludwig Maximillians University in Munich connecting two nodes situated in adjacent buildings (line of sight 80 m). The average link length is between 20 and 30 km, the longest link being 83 km. The paper presents the architecture and functionality of the principal networking agent—the SECOQC node module, which enables the authentic

  20. High-resolution mapping of soil moisture at the field scale using ground-penetrating radar for improving remote sensing data products

    NASA Astrophysics Data System (ADS)

    Lambot, Sébastien; Mahmoudzadeh, Mohammad Reza; Phuong Tran, Anh; Nottebaere, Martijn; Leonard, Aline; Defourny, Pierre; Neyt, Xavier

    2014-05-01

    was not available before. Acknowledgements: This work has been funded by the Belgian Science Policy Office in the frame of the Stereo II programme - project SR/00/159 (SENSAR)and the FNRS (Fonds National de la Recherche Scientifique, Belgium), and has benefited from networking activities carried out within the EU funded COST Action TU1208 "Civil Engineering Applications of Ground Penetrating Radar".

  1. The Young Open Clusters King 12, NGC 7788, and NGC 7790: Pre-main-sequence Stars and Extended Stellar Halos

    NASA Astrophysics Data System (ADS)

    Davidge, T. J.

    2012-12-01

    The stellar contents of the open clusters King 12, NGC 7788, and NGC 7790 are investigated using MegaCam images. Comparisons with isochrones yield an age <20 Myr for King 12, 20-40 Myr for NGC 7788, and 60-80 Myr for NGC 7790 based on the properties of stars near the main-sequence turnoff (MSTO) in each cluster. The reddening of NGC 7788 is much larger than previously estimated. The luminosity functions (LFs) of King 12 and NGC 7788 show breaks that are attributed to the onset of pre-main-sequence (PMS) objects, and comparisons with models of PMS evolution yield ages that are consistent with those measured from stars near the MSTO. In contrast, the r' LF of main-sequence stars in NGC 7790 is matched to r' = 20 by a model that is based on the solar neighborhood mass function. The structural properties of all three clusters are investigated by examining the two-point angular correlation function of blue main-sequence stars. King 12 and NGC 7788 are each surrounded by a stellar halo that extends out to a radius of 5 arcmin (~3.4 pc). It is suggested that these halos form in response to large-scale mass ejection early in the evolution of the clusters, as predicted by models. In contrast, blue main-sequence stars in NGC 7790 are traced out to a radius of ~7.5 arcmin (~5.5 pc), with no evidence of a halo. It is suggested that all three clusters may have originated in the same star-forming complex, but not in the same giant molecular cloud. Based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii.

  2. Surface abundances of ON stars

    NASA Astrophysics Data System (ADS)

    Martins, F.; Simón-Díaz, S.; Palacios, A.; Howarth, I.; Georgy, C.; Walborn, N. R.; Bouret, J.-C.; Barbá, R.

    2015-06-01

    Context. Massive stars burn hydrogen through the CNO cycle during most of their evolution. When mixing is efficient or when mass transfer in binary systems occurs, chemically processed material is observed at the surface of O and B stars. Aims: ON stars show stronger lines of nitrogen than morphologically normal counterparts. Whether this corresponds to the presence of material processed through the CNO cycle is not known. Our goal is to answer this question. Methods: We performed a spectroscopic analysis of a sample of ON stars with atmosphere models. We determined the fundamental parameters as well as the He, C, N, and O surface abundances. We also measured the projected rotational velocities. We compared the properties of the ON stars to those of normal O stars. Results: We show that ON stars are usually rich in helium. Their CNO surface abundances are fully consistent with predictions of nucleosynthesis. ON stars are more chemically evolved and rotate - on average - faster than normal O stars. Evolutionary models including rotation cannot account for the extreme enrichment observed among ON main sequence stars. Some ON stars are members of binary systems, but others are single stars as indicated by stable radial velocities. Mass transfer is therefore not a simple explanation for the observed chemical properties. Conclusions: We conclude that ON stars show extreme chemical enrichment at their surface, consistent with nucleosynthesis through the CNO cycle. Its origin is not clear at present. Based on observations obtained 1) at the Anglo-Australian Telescope; 2) at the Canada-France-Hawaii Telescope (CFHT), which is operated by the National Research Council (NRC) of Canada, the Institut National des Science de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii; 3) at the ESO/La Silla Observatory under programs 081.D-2008, 083.D-0589, 086.D-0997; 4) the Nordic Optical Telescope, operated on the island of La

  3. Observing of tree trunks and other cylindrical objects using GPR

    NASA Astrophysics Data System (ADS)

    Jezova, Jana; Lambot, Sebastien

    2016-04-01

    configurations is presented. Future research will focus on the design of an adapted radar antenna for that application to optimize living tree trunk tomography. This research is funded by the Fonds de la Recherche Scientifique (FNRS, Belgium) and benefits from networking activities carried out within the EU COST Action TU1208 "Civil Engineering Applications of Ground Penetrating Radar".

  4. The magnetic field of the double-lined spectroscopic binary system HD 5550

    NASA Astrophysics Data System (ADS)

    Alecian, E.; Tkachenko, A.; Neiner, C.; Folsom, C. P.; Leroy, B.

    2016-05-01

    Ap component hosts a dipolar field inclined with the rotation axis at an angle β = 156 ± 17 ° and a polar strength Bd = 65 ± 20 G. The field strength is the weakest known for an Ap star. Based on the BinaMIcS Large Programme (PI: C. Neiner, runID: L131N02) obtained at the Telescope Bernard Lyot (USR5026) operated by the Observatoire Midi-Pyrénées, Université de Toulouse (Paul Sabatier), Centre National de la Recherche Scientifique of France.

  5. Magnetic field topology of the unique chemically peculiar star CU Virginis

    NASA Astrophysics Data System (ADS)

    Kochukhov, O.; Lüftinger, T.; Neiner, C.; Alecian, E.; MiMeS Collaboration

    2014-05-01

    ) operated by the Observatoire Midi-Pyrénées, Université de Toulouse (Paul Sabatier), Centre National de la Recherche Scientifique of France.

  6. Search for surface magnetic fields in Mira stars. First detection in χ Cygni

    NASA Astrophysics Data System (ADS)

    Lèbre, A.; Aurière, M.; Fabas, N.; Gillet, D.; Herpin, F.; Konstantinova-Antova, R.; Petit, P.

    2014-01-01

    its passage through the atmosphere. Without such an amplification by the shock, the magnetic field strength would have been too low to be detected. For the first time, we also report strong Stokes Q and U signatures (linear polarization) centered on the zero velocity (i.e., on the shock front position). They seem to indicate that the radial direction would be favored by the shock during its propagation throughout the atmosphere. Based on observations obtained at the Télescope Bernard Lyot (TBL, USR5026) at the Observatoire du Pic du Midi, operated by the Observatoire Midi-Pyrénées, Université de Toulouse (Paul Sabatier), Centre National de la Recherche Scientifique of France.

  7. Dynamical Properties of z ~ 2 Star-forming Galaxies and a Universal Star Formation Relation

    NASA Astrophysics Data System (ADS)

    Bouché, N.; Cresci, G.; Davies, R.; Eisenhauer, F.; Förster Schreiber, N. M.; Genzel, R.; Gillessen, S.; Lehnert, M.; Lutz, D.; Nesvadba, N.; Shapiro, K. L.; Sternberg, A.; Tacconi, L. J.; Verma, A.; Cimatti, A.; Daddi, E.; Renzini, A.; Erb, D. K.; Shapley, A.; Steidel, C. C.

    2007-12-01

    , 075.A-0466, 076.A-0527, 077.A-0576, 078.A-0600, and 079.A-0341 and on observations obtained at the IRAM Plateau de Bure Interferometer (PdBI). IRAM is funded by the Centre National de la Recherche Scientifique (France), the Max-Planck Gesellschaft (Germany), and the Instituto Geografico Nacional (Spain).

  8. Tracking quintessence by cosmic shear. Constraints from VIRMOS-Descart and CFHTLS and future prospects

    NASA Astrophysics Data System (ADS)

    Schimd, C.; Tereno, I.; Uzan, J.-P.; Mellier, Y.; van Waerbeke, L.; Semboloni, E.; Hoekstra, H.; Fu, L.; Riazuelo, A.

    2007-02-01

    level, whereas α=2+18-2, ΩQ0= 0.74+0.03-0.05 when including supergravity corrections. Based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. This work is based in part on data products produced at TERAPIX and the Canadian Astronomy Data Centre as part of the Canada-France-Hawaii Telescope Legacy Survey, a collaborative project of NRC and CNRS.

  9. Investigations of two-phase flame propagation under microgravity conditions

    NASA Astrophysics Data System (ADS)

    Gokalp, Iskender

    2016-07-01

    Investigations of two-phase flame propagation under microgravity conditions R. Thimothée, C. Chauveau, F. Halter, I Gökalp Institut de Combustion, Aérothermique, Réactivité et Environnement (ICARE), CNRS, 1C Avenue de la Recherche Scientifique, 45071 Orléans Cedex 2, France This paper presents and discusses recent results on two-phase flame propagation experiments we carried out with mono-sized ethanol droplet aerosols under microgravity conditions. Fundamental studies on the flame propagation in fuel droplet clouds or sprays are essential for a better understanding of the combustion processes in many practical applications including internal combustion engines for cars, modern aircraft and liquid rocket engines. Compared to homogeneous gas phase combustion, the presence of a liquid phase considerably complicates the physico-chemical processes that make up combustion phenomena by coupling liquid atomization, droplet vaporization, mixing and heterogeneous combustion processes giving rise to various combustion regimes where ignition problems and flame instabilities become crucial to understand and control. Almost all applications of spray combustion occur under high pressure conditions. When a high pressure two-phase flame propagation is investigated under normal gravity conditions, sedimentation effects and strong buoyancy flows complicate the picture by inducing additional phenomena and obscuring the proper effect of the presence of the liquid droplets on flame propagation compared to gas phase flame propagation. Conducting such experiments under reduced gravity conditions is therefore helpful for the fundamental understanding of two-phase combustion. We are considering spherically propagating two-phase flames where the fuel aerosol is generated from a gaseous air-fuel mixture using the condensation technique of expansion cooling, based on the Wilson cloud chamber principle. This technique is widely recognized to create well-defined mono-size droplets

  10. Conception et caracterisation d'un magnetoplasma produit par une onde de surface pour la pulverisation d'echantillons solides

    NASA Astrophysics Data System (ADS)

    Masse, Louis Philippe

    Suite a l'extraordinaire explosion de l'informatique de la derniere decennie, la science et la technologie des materiaux ont pris un essor extraordinaire. Par exemple, il est devenu crucial de concevoir des materiaux a haut degre de purete. Ce besoin a fortement motive le developpement de methodes d'analyse de solides. Traditionnellement, la methode adoptee est l'analyse par torche ICP, mais pour de nombreuses raisons, dont la lenteur de cette methode, la communaute scientifique oeuvrant en chimie analytique recherche des techniques d'analyse de solides directes, rapides et plus sensibles. Parmi les voies possibles, on trouve les methodes basees sur la pulverisation par plasma. Dans ce contexte, nous avons etudie la possibilite et la pertinence d'utiliser un magnetoplasma entretenu par une onde de surface pour pulveriser des solides dans le but de les analyser. Nos travaux portent principalement sur l'etude du comportement du plasma lors de la pulverisation. Nous avons montre que la pulverisation affecte la decharge de diverses facons. En premier lieu, la concentration d'especes provenant du materiau pulverise dans le plasma augmente avec la tension de polarisation. De plus, la concentration d'especes pulverisees diminue lorsque la pression croit, possiblement a cause du redepot. Nous avons aussi montre qu'il etait possible de pulveriser des solides isolants en exploitant le phenomene d'autopolarisation du a l'application d'une tension RF. Nous avons aussi etudie l'effet de la pulverisation sur la temperature et la densite electronique. Ainsi, lors de la pulverisation de metaux tels que le cuivre, la temperature electronique diminue lorsque la tension de polarisation augmente. Ceci est attribuable a l'augmentation de la densite d'especes metalliques neutres facilement ionisables par impact electronique. Nous avons aussi note que la densite electronique augmente avec la concentration d'especes metalliques dans le plasma, ce qui resulte d'un meilleur bilan de

  11. The 2011 Periastron Passage of the Be Binary δ Scorpii

    NASA Astrophysics Data System (ADS)

    Miroshnichenko, A. S.; Pasechnik, A. V.; Manset, N.; Carciofi, A. C.; Rivinius, Th.; Štefl, S.; Gvaramadze, V. V.; Ribeiro, J.; Fernando, A.; Garrel, T.; Knapen, J. H.; Buil, C.; Heathcote, B.; Pollmann, E.; Mauclaire, B.; Thizy, O.; Martin, J.; Zharikov, S. V.; Okazaki, A. T.; Gandet, T. L.; Eversberg, T.; Reinecke, N.

    2013-04-01

    We describe the results of the world-wide observing campaign of the highly eccentric Be binary system δ Scorpii 2011 periastron passage which involved professional and amateur astronomers. Our spectroscopic observations provided a precise measurement of the system orbital period at 10.8092 ± 0.0005 yr. Fitting of the He II 4686 Å line radial velocity curve determined the periastron passage time on 2011 July 3, UT 9:20 with a 0.9-day uncertainty. Both these results are in a very good agreement with recent findings from interferometry. We also derived new evolutionary masses of the binary components (13 and 8.2 M ⊙) and a new distance of 136 pc from the Sun, consistent with the HIPPARCOS parallax. The radial velocity and profile variations observed in the Hα line near the 2011 periastron reflected the interaction of the secondary component and the circumstellar disk around the primary component. Using these data, we estimated a disk radius of 150 R ⊙. Our analysis of the radial velocity variations measured during the periastron passage time in 2000 and 2011 along with those measured during the 20th century, the high eccentricity of the system, and the presence of a bow shock-like structure around it suggest that δ Sco might be a runaway triple system. The third component should be external to the known binary and move on an elliptical orbit that is tilted by at least 40° with respect to the binary orbital plane for such a system to be stable and responsible for the observed long-term radial velocity variations. This paper is partially based on observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique de France, and the University of Hawaii, the 2.2 m MPG telescope operated at ESO/La Silla under program IDs 086.A-9019 and 087.A-9005, the IAC80 telescope in the Spanish Observatorio del Teide

  12. A robust morphological classification of high-redshift galaxies using support vector machines on seeing limited images. I. Method description

    NASA Astrophysics Data System (ADS)

    Huertas-Company, M.; Rouan, D.; Tasca, L.; Soucail, G.; Le Fèvre, O.

    2008-02-01

    , offering an objective and automated estimate of errors that enables a straightforward comparison with other surveys. Selecting the training sample in the high-redshift sample rest-frame makes the results free from wavelength dependent effects and hence its interpretation in terms of evolution easier. Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  13. The VIMOS Public Extragalactic Survey (VIPERS). First Data Release of 57 204 spectroscopic measurements

    NASA Astrophysics Data System (ADS)

    Garilli, B.; Guzzo, L.; Scodeggio, M.; Bolzonella, M.; Abbas, U.; Adami, C.; Arnouts, S.; Bel, J.; Bottini, D.; Branchini, E.; Cappi, A.; Coupon, J.; Cucciati, O.; Davidzon, I.; De Lucia, G.; de la Torre, S.; Franzetti, P.; Fritz, A.; Fumana, M.; Granett, B. R.; Ilbert, O.; Iovino, A.; Krywult, J.; Le Brun, V.; Le Fèvre, O.; Maccagni, D.; Małek, K.; Marulli, F.; McCracken, H. J.; Paioro, L.; Polletta, M.; Pollo, A.; Schlagenhaufer, H.; Tasca, L. A. M.; Tojeiro, R.; Vergani, D.; Zamorani, G.; Zanichelli, A.; Burden, A.; Di Porto, C.; Marchetti, A.; Marinoni, C.; Mellier, Y.; Moscardini, L.; Nichol, R. C.; Peacock, J. A.; Percival, W. J.; Phleps, S.; Wolk, M.

    2014-02-01

    We present the first Public Data Release (PDR-1) of the VIMOS Public Extragalactic Survey (VIPERS). It comprises 57 204 spectroscopic measurements together with all additional information necessary for optimal scientific exploitation of the data, in particular the associated photometric measurements and quantification of the photometric and survey completeness. VIPERS is an ESO Large Programme designed to build a spectroscopic sample of ≃100 000 galaxies with iAB < 22.5 and 0.5 < z < 1.2 with high sampling rate (≃45%). The survey spectroscopic targets are selected from the CFHTLS-Wide five-band catalogues in the W1 and W4 fields. The final survey will cover a total area of nearly 24 deg2, for a total comoving volume between z = 0.5 and 1.2 of ≃4 × 107 h-3 Mpc3 and a median galaxy redshift of z ≃ 0.8. The release presented in this paper includes data from virtually the entire W4 field and nearly half of the W1 area, thus representing 64% of the final dataset. We provide a detailed description of sample selection, observations and data reduction procedures; we summarise the global properties of the spectroscopic catalogue and explain the associated data products and their use, and provide all the details for accessing the data through the survey database (http://vipers.inaf.it) where all information can be queried interactively. Based on observations collected at the European Southern Observatory, Cerro Paranal, Chile, using the Very Large Telescope under programs 182.A-0886 and partly 070.A-9007. Also based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT), which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. This work is based in part on

  14. Suivi prospectif sur 5 ans des tentatives de suicide en population clinique dans la région de Fès, Maroc

    PubMed Central

    Aarab, Chadya; Elghazouani, Fatima; Aalouane, Rachid; Rammouz, Ismail

    2014-01-01

    Au Maroc, les tentatives de suicide (TS) demeurent un sujet mal évalué à cause de considérations socioculturelles et l'absence d'approche longitudinale. L'objectif principal était d’évaluer le devenir des suicidants après 5ans au centre universitaire psychiatrique de Fès, les objectifs secondaires étaient l'estimation de la prévalence des TS, préciser les étiologies les plus fréquentes, et établir une corrélation entre les paramètres sociodémographiques, cliniques et évolutifs. Etude prospective à visée transversale et longitudinale, incluant les suicidants vus à l'hôpital psychiatrique de Fès, avec un suivi longitudinal sur 5ans. L’évaluation a été faite par un hétéro-questionnaire et le Mini International Neuropsychiatric Interview (MINI) cherchant le trouble psychiatrique sous jacent. On a recruté 105 patients suicidants, 62% des femmes, l’âge moyen est de 29,23ans. La prévalence des tentatives de suicide est de 3% sur l'ensemble des consultants à l’établissement. Les troubles de l'humeur, psychotiques et de personnalité ont occupé respectivement 37,6%, 27,7%, et 25,7% des cas. La récidive suicidaire a été notée chez 54% des patients, était significativement corrélée à la vie solitaire (P: 0,039) et à la présence d'antécédents familiaux de TS (P: 0,046). L'utilisation de moyens violents était significativement fréquente chez les patients psychotiques. Après 5ans, 32 patients ont répondu à notre appel. Le taux de récidive était de 15%. On a noté trois cas de décès dont deux suicides confirmés. Les résultats confirment les données de la littérature scientifique avec certaines particularités cliniques et évolutives. PMID:25478042

  15. Magnetic fields of young solar twins

    NASA Astrophysics Data System (ADS)

    Rosén, L.; Kochukhov, O.; Hackman, T.; Lehtinen, J.

    2016-09-01

    telescope at La Silla (Chile), under the program ID 091.D-0836. Also based on observations obtained at the Bernard Lyot Telescope (TBL, Pic du Midi, France) of the Midi-Pyrénées Observatory, which is operated by the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France.

  16. Foreword

    NASA Astrophysics Data System (ADS)

    Carbillet, M.; Ferrari, A.; Aime, C.

    This book reports the proceedings of the third Journées d'Imagerie à Très Haute Dynamique et Détection d'Exoplanètes (Days on High Contrast Imaging and Exoplanets Detection) that were held in Nice and Fréjus in May, 16th 19th, 2005, with the joint efforts of the CNRS (Centre National de la Recherche Scientifique), the Observatoire de la Côte d'Azur, the Collège de France, and the Laboratoire Universitaire d'Astrophysique de Nice of the University of Nice Sophia Antipolis. The first and second Journées led to the publications of Volumes 8 and 12 of EAS Publications Series sharing the common title “Astronomy with High Contrast Imaging”. Volume 8, subtitled “From Planetary Systems to Active Galactic Nuclei” collected 33 papers covering the very large domain of applications of High Contrast Imaging, from protoplanetary disks to AGNs. Volume 12, subtitled “Instrumentation for Coronagraphy and Nulling Interferometry” collected 29 papers dealing with technical aspects of the various experiments (apodisation, coronagraphy, nulling) that can lead to exoplanetographs, i.e. instruments able to directly record the light coming from planets orbitings stars other than the Sun. The present edition, third of these series on High Contrast Imaging, focuses on the aspects of image processing related to coronagraphy and nulling. Technologies in competition are numerous, either from the point-of-view of the methods (coronagraphy, nulling, traditional interferometry, interferometry with densified pupils, etc.), the spectral domain (observations from the visible to 10 μm), or the instrumentation (ground-based with the support of adaptive optics vs. space-born). Which techniques and instruments are the most efficient for a given astronomical objective? The answer to this question must definitely also take into account the data processing retained for each instrument and a precise analysis of the related signal-to-noise ratio. This school gathered basic lessons on

  17. Toward Understanding the B[e] Phenomenon: V. Nature and Spectral Variations of the MWC 728 Binary System.

    NASA Astrophysics Data System (ADS)

    Miroshnichenko, A. S.; Zharikov, S. V.; Danford, S.; Manset, N.; Korčáková, D.; Kříček, R.; Šlechta, M.; Omarov, Ch. T.; Kusakin, A. V.; Kuratov, K. S.; Grankin, K. N.

    2015-08-01

    We report the results of a long-term spectroscopic monitoring of the FS CMa type object MWC 728. We found that it is a binary system with a B5 ve ({T}{eff} = 14,000 ± 1000 K) primary and a G8 iii type ({T}{eff} ˜ 5000 K) secondary. Absorption line positions of the secondary vary, with a semi-amplitude of ˜20 km s-1 and a period of 27.5 days. The system’s mass function is 2.3 × 10-2 {M}⊙ , and its orbital plane is ˜13°-15° tilted from the plane of the sky. The primary’s v{sin}i˜ 110 km s-1, combined with this tilt, implies that it rotates at a nearly breakup velocity. We detected strong variations of the Balmer and He i emission-line profiles on timescales from days to years. This points to a variable stellar wind of the primary in addition to the presence of a circum-primary gaseous disk. The strength of the absorption-line spectrum, along with the optical and near infrared (IR) continuum, suggest that the primary contributes ˜60% of the V-band flux, the disk contributes ˜30%, and the secondary contributes ˜10%. The system parameters, along with the interstellar extinction, suggest a distance of ˜1 kpc, that the secondary does not fill its Roche lobe, and that the companions’ mass ratio is q ˜ 0.5. Overall, the observed spectral variability and the presence of a strong IR-excess are in agreement with a model of a close binary system that has undergone a non-conservative mass-transfer. of the Centre National de la Recherche Scientifique de France, and the University of Hawaii as well as on observations obtained at the 2.7 m Harlan J. Smith telescope of the McDonald Observatory (Texas, USA), 2.1 m of the Observatorio Astronomico Nacional San Pedro Martir (Baja California, Mexico), 2 m telescope of the Ondřejov Observatory, Czech Republic, and 0.81 m telescope of the Three College Observatory, North Carolina, USA.

  18. Weak lensing survey of galaxy clusters in the CFHTLS Deep

    NASA Astrophysics Data System (ADS)

    Gavazzi, R.; Soucail, G.

    2007-02-01

    Aims: We present a weak lensing search of galaxy clusters in the 4 deg2 of the CFHT Legacy Survey Deep. This work aims at building a mass-selected sample of clusters with well controlled selection effects. This present survey is a preliminary step toward a full implementation in the forthcoming 170 deg2 of the CFHTLS Wide survey. Methods: We use the deep i' band images observed under subarcsecond seeing conditions to perform weak lensing mass reconstructions and to identify high convergence peaks. Thanks to the availability of deep u^*g'r'i'z' exposures, sources are selected from their photometric redshifts in the weak lensing analysis. We also use lensing tomography to derive an estimate of the lens redshift. After considering the raw statistics of peaks we check whether they can be associated to a clear optical counterpart or to published X-ray selected clusters. Results: Among the 14 peaks found above a signal-to-noise detection threshold ν=3.5, nine are secure detections with estimated redshift 0.1⪉ z_l⪉0.7 and a velocity dispersion 450⪉σ_v⪉ 700 {km s}-1. This low mass range is accessible thanks to the high density of background sources. Considering the intersection between the shear-selected clusters and XMM-LSS X-ray clusters in the D1 field, we observe that the ICM gas in these low-mass clusters (T_X˜1{-}2 keV) is not hotter than the temperature inferred from shear, this trend being different for published massive clusters. A more extended weak lensing survey, with higher statistics of mass structures will be a promising way to bypass several of the problems related to standard detection methods based on the complex physics of baryons. Based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of

  19. The VIMOS Public Extragalactic Redshift Survey (VIPERS). A support vector machine classification of galaxies, stars, and AGNs

    NASA Astrophysics Data System (ADS)

    Małek, K.; Solarz, A.; Pollo, A.; Fritz, A.; Garilli, B.; Scodeggio, M.; Iovino, A.; Granett, B. R.; Abbas, U.; Adami, C.; Arnouts, S.; Bel, J.; Bolzonella, M.; Bottini, D.; Branchini, E.; Cappi, A.; Coupon, J.; Cucciati, O.; Davidzon, I.; De Lucia, G.; de la Torre, S.; Franzetti, P.; Fumana, M.; Guzzo, L.; Ilbert, O.; Krywult, J.; Le Brun, V.; Le Fevre, O.; Maccagni, D.; Marulli, F.; McCracken, H. J.; Paioro, L.; Polletta, M.; Schlagenhaufer, H.; Tasca, L. A. M.; Tojeiro, R.; Vergani, D.; Zanichelli, A.; Burden, A.; Di Porto, C.; Marchetti, A.; Marinoni, C.; Mellier, Y.; Moscardini, L.; Nichol, R. C.; Peacock, J. A.; Percival, W. J.; Phleps, S.; Wolk, M.; Zamorani, G.

    2013-09-01

    project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT), which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. This work is based in part on data products produced at TERAPIX and the Canadian Astronomy Data Centre as part of the Canada-France-Hawaii Telescope Legacy Survey, a collaborative project of NRC and CNRS. The VIPERS web site is http://www.vipers.inaf.it/

  20. Transiting exoplanets from the CoRoT space mission. XVII. The hot Jupiter CoRoT-17b: a very old planet

    NASA Astrophysics Data System (ADS)

    Csizmadia, Sz.; Moutou, C.; Deleuil, M.; Cabrera, J.; Fridlund, M.; Gandolfi, D.; Aigrain, S.; Alonso, R.; Almenara, J.-M.; Auvergne, M.; Baglin, A.; Barge, P.; Bonomo, A. S.; Bordé, P.; Bouchy, F.; Bruntt, H.; Carone, L.; Carpano, S.; Cavarroc, C.; Cochran, W.; Deeg, H. J.; Díaz, R. F.; Dvorak, R.; Endl, M.; Erikson, A.; Ferraz-Mello, S.; Fruth, Th.; Gazzano, J.-C.; Gillon, M.; Guenther, E. W.; Guillot, T.; Hatzes, A.; Havel, M.; Hébrard, G.; Jehin, E.; Jorda, L.; Léger, A.; Llebaria, A.; Lammer, H.; Lovis, C.; MacQueen, P. J.; Mazeh, T.; Ollivier, M.; Pätzold, M.; Queloz, D.; Rauer, H.; Rouan, D.; Santerne, A.; Schneider, J.; Tingley, B.; Titz-Weider, R.; Wuchterl, G.

    2011-07-01

    We report on the discovery of a hot Jupiter-type exoplanet, CoRoT-17b, detected by the CoRoT satellite. It has a mass of 2.43 ± 0.30 MJup and a radius of 1.02 ± 0.07 RJup, while its mean density is 2.82 ± 0.38 g/cm3. CoRoT-17b is in a circular orbit with a period of 3.7681 ± 0.0003 days. The host star is an old (10.7 ± 1.0 Gyr) main-sequence star, which makes it an intriguing object for planetary evolution studies. The planet's internal composition is not well constrained and can range from pure H/He to one that can contain ~380 earth masses of heavier elements. The CoRoT space mission, launched on December 27th 2006, has been developed and is operated by CNES, with the contribution of Austria, Belgium, Brazil, ESA (RSSD and Science Programme), Germany and Spain. Part of the observations were obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. Based on observations made with HARPS spectrograph on the 3.6-m European Organisation for Astronomical Research in the Southern Hemisphere telescope at La Silla Observatory, Chile (ESO program 184.C-0639). Based on observations made with the IAC80 telescope operated on the island of Tenerife by the Instituto de Astrofísica de Canarias in the Spanish Observatorio del Teide. Part of the data presented herein were obtained at the W.M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W.M. Keck Foundation.

  1. Coffee Shops, Classrooms and Conversations: public engagement and outreach in a large interdisciplinary research Hub

    NASA Astrophysics Data System (ADS)

    Holden, Jennifer A.

    2014-05-01

    Public engagement and outreach activities are increasingly using specialist staff for co-ordination, training and support for researchers, they are also becoming expected for large investments. Here, the experience of public engagement and outreach a large, interdisciplinary Research Hub is described. dot.rural, based at the University of Aberdeen UK, is a £11.8 million Research Councils UK Rural Digital Economy Hub, funded as part of the RCUK Digital Economy Theme (2009-2015). Digital Economy research aims to realise the transformational impact of digital technologies on aspects of the environment, community life, cultural experiences, future society, and the economy. The dot.rural Hub involves 92 researchers from 12 different disciplines, including Geography, Hydrology and Ecology. Public Engagement and Outreach is embedded in the dot.rural Digital Economy Hub via an Outreach Officer. Alongside this position, public engagement and outreach activities are compulsory part of PhD student contracts. Public Engagement and Outreach activities at the dot.rural Hub involve individuals and groups in both formal and informal settings organised by dot.rural and other organisations. Activities in the realms of Education, Public Engagement, Traditional and Social Media are determined by a set of Underlying Principles designed for the Hub by the Outreach Officer. The underlying Engagement and Outreach principles match funding agency requirements and expectations alongside researcher demands and the user-led nature of Digital Economy Research. All activities include researchers alongside the Outreach Officer are research informed and embedded into specific projects that form the Hub. Successful public engagement activities have included participation in Café Scientifique series, workshops in primary and secondary schools, and online activities such as I'm a Scientist Get Me Out of Here. From how to engage 8 year olds with making hydrographs more understandable to members of

  2. The remarkably unremarkable global abundance variations of the magnetic Bp star HD 133652

    NASA Astrophysics Data System (ADS)

    Bailey, J. D.; Landstreet, J. D.

    2015-08-01

    . Based in part on our own observations made with the European Southern Observatory (ESO) telescopes under the ESO programme 086.D-0449(A). It is also based in part on observations carried out at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Science de l'Universe of the Centre National de la Recherche Scientifique of France and the University of Hawaii.

  3. Discovery of secular variations in the atmospheric abundances of magnetic Ap stars

    NASA Astrophysics Data System (ADS)

    Bailey, J. D.; Landstreet, J. D.; Bagnulo, S.

    2014-01-01

    on observations made with the European Southern Observatory (ESO) telescopes under the ESO programmes 072.D-0410(A) and 086.D-0449(A). It is also based in part on observations carried out at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France and the University of Hawaii.

  4. CSI 2264: Characterizing Young Stars in NGC 2264 With Short-Duration Periodic Flux Dips in Their Light Curves

    NASA Astrophysics Data System (ADS)

    Stauffer, John; Cody, Ann Marie; McGinnis, Pauline; Rebull, Luisa; Hillenbrand, Lynne A.; Turner, Neal J.; Carpenter, John; Plavchan, Peter; Carey, Sean; Terebey, Susan; Morales-Calderón, María; Alencar, Silvia H. P.; Bouvier, Jerome; Venuti, Laura; Hartmann, Lee; Calvet, Nuria; Micela, Giusi; Flaccomio, Ettore; Song, Inseok; Gutermuth, Rob; Barrado, David; Vrba, Frederick J.; Covey, Kevin; Padgett, Debbie; Herbst, William; Gillen, Edward; Lyra, Wladimir; Medeiros Guimaraes, Marcelo; Bouy, Herve; Favata, Fabio

    2015-04-01

    , and Spain. MegaCam is a joint project of CFHT and CEA/DAPNIA, which is operated by the National Research Council (NRC) of Canada, the Institute National des Sciences de l’Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

  5. Inter-Sensor Comparison of Microwave Land Surface Emissivity Products to Improve Precipitation Retrievals

    NASA Astrophysics Data System (ADS)

    Norouzi, H.; Temimi, M.; Turk, J.; Prigent, C.; Furuzawa, F.; Tian, Y.

    2013-12-01

    Microwave land surface emissivity acts as the background signal to estimate rain rate, cloud liquid water, and total precipitable water. Therefore, its accuracy can directly affect the uncertainty of such measurements. Over land, unlike over oceans, the microwave emissivity is relatively high and and varies significantly as surface conditions and land cover change. Lack of ground truth measurement of microwave emissivity especially on global scale has made the uncertainty analysis of this parameter very challenging. The present study investigates the consistency among the existing global land emissivity estimates from different microwave sensors. The products are determined from various sensors and frequencies ranging from 7 to 90 GHz. The selected emissivity products in this study are from the Advanced Microwave Scanning Radiometer for EOS (AMSR-E) by NOAA - Cooperative remote Sensing and Science and Technology Center (CREST), the Special Sensor Microwave Imager (SSM/I) by The Centre National de la Recherche Scientifique (CNRS) in France, TRMM Microwave Imager (TMI) by Nagoya University, Japan, and WindSat by NASA Jet Propulsion Laboratory (JPL). The emissivity estimates are based on different algorithms and ancillary data sets. This work investigates the difference among these emissivity products from 2003 to 2008 dynamically and spectrally. The similarities and discrepancies of the retrievals are studied at different land cover types. The mean relative difference (MRD) and other statistical parameters are calculated temporally for all five years of the study. Some inherent discrepancies between the selected products can be attributed to the difference in geometry in terms of incident angle, spectral response, and the foot print size which can affect the estimations. The results reveal that in lower frequencies (=<19 GHz) ancillary data especially skin temperature data set is the major source of difference in emissivity retrievals, while in higher frequencies

  6. The weak magnetic field of the O9.7 supergiant ζOrionisA

    NASA Astrophysics Data System (ADS)

    Bouret, J.-C.; Donati, J.-F.; Martins, F.; Escolano, C.; Marcolino, W.; Lanz, T.; Howarth, I. D.

    2008-09-01

    We report here the detection of a weak magnetic field of 50-100G on the O9.7 supergiant ζOrionisA (ζOriA), using spectropolarimetric observations obtained with NARVAL at the 2-m Télescope Bernard Lyot atop Pic du Midi (France). ζOriA is the third O star known to host a magnetic field (along with θ1OriC and HD191612), and the first detection on a `normal' rapidly rotating O star. The magnetic field of ζOriA is the weakest magnetic field ever detected on a massive star. The measured field is lower than the thermal equipartition limit (about 100G). By fitting non-local thermodynamic equilibrium (NLTE) model atmospheres to our spectra, we determined that ζOriA is a 40Msolar star with a radius of 25Rsolar and an age of about 5-6Myr, showing no surface nitrogen enhancement and losing mass at a rate of about 2 × 10-6Msolaryr-1. The magnetic topology of ζOriA is apparently more complex than a dipole and involves two main magnetic polarities located on both sides of the same hemisphere; our data also suggest that ζOriA rotates in about 7.0d and is about 40° away from pole-on to an Earth-based observer. Despite its weakness, the detected magnetic field significantly affects the wind structure; the corresponding Alfvén radius is however very close to the surface, thus generating a different rotational modulation in wind lines than that reported on the two other known magnetic O stars. The rapid rotation of ζOriA with respect to θ1OriC appears as a surprise, both stars having similar unsigned magnetic fluxes (once rescaled to the same radius); it may suggest that the subequipartition field detected on ζOriA is not a fossil remnant (as opposed to that of θ1 OriC and HD191612), but the result of an exotic dynamo action produced through magnetohydrodynamics (MHD) instabilities. Based on observations obtained at the Télescope Bernard Lyot (TBL), operated by the Institut National des Science de l'Univers of the Centre National de la Recherche Scientifique of France

  7. The XMM-Newton SSC survey of the Galactic plane

    NASA Astrophysics Data System (ADS)

    Nebot Gómez-Morán, A.; Motch, C.; Barcons, X.; Carrera, F. J.; Ceballos, M. T.; Cropper, M.; Grosso, N.; Guillout, P.; Hérent, O.; Mateos, S.; Michel, L.; Osborne, J. P.; Pakull, M.; Pineau, F.-X.; Pye, J. P.; Roberts, T. P.; Rosen, S. R.; Schwope, A. D.; Watson, M. G.; Webb, N.

    2013-05-01

    small contribution of close main sequence or evolved binaries. We find other interesting objects such as cataclysmic variables (d ~ 0.6-2 kpc), low luminosity high mass stars (likely belonging to the class of γ-Cas-like systems, d ~ 1.5-7 kpc), T Tauri and Herbig-Ae stars. A handful of extragalactic sources located in the highest Galactic latitude fields could be optically identified. For the 20 fields observed with the EPIC pn camera, we have constructed log N(>S) - log S curves in the soft and hard bands. In the soft band, the majority of the sources are positively identified with active coronae and the fraction of stars increases by about one order of magnitude from b = 60° to b = 0° at an X-ray flux of 2 × 10-14 erg cm-2 s-1. The hard band is dominated by extragalactic sources, but there is a small contribution from a hard Galactic population formed by CVs, HMXB candidates or γ-Cas-like systems and by some active coronae that are also detected in the soft band. At b = 0° the surface density of hard sources brighter than 1 × 10-13 erg cm-2 s-1 steeply increases by one order of magnitude from l = 20° to the Galactic centre region (l = 0.9°). Based on observations obtained with XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA. Based on observations carried out at the European Southern Observatory, La Silla and Paranal, Chile under programmes Nos 69.D-0143, 70.D-0227, 71.D-0296, 71.D-0552. Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. Based on observations obtained at the Observatoire de Haute Provence which is operated by the Centre National de la Recherche Scientifique of France. Tables 8-33 are only available at the CDS via anonymous ftp to cdsarc

  8. List of Participants

    NASA Astrophysics Data System (ADS)

    2008-11-01

    Mohab Abou ZeidInstitut des Hautes Études Scientifiques, Bures-sur-Yvette Ido AdamMax-Planck-Institut für Gravitationsphysik (AEI), Potsdam Henrik AdorfLeibniz Universität Hannover Mohammad Ali-AkbariIPM, Tehran Antonio Amariti Università di Milano-Bicocca Nicola Ambrosetti Université de Neuchâtel Martin Ammon Max-Planck-Institut für Physik, München Christopher AndreyÉcole Polytechnique Fédérale de Lausanne (EPFL) Laura AndrianopoliPolitecnico di Torino David AndriotLPTHE, Université UPMC Paris VI Carlo Angelantonj Università di Torino Pantelis ApostolopoulosUniversitat de les Illes Balears, Palma Gleb ArutyunovInstitute for Theoretical Physics, Utrecht University Davide AstolfiUniversità di Perugia Spyros AvramisUniversité de Neuchâtel Mirela BabalicChalmers University, Göteborg Foday BahDigicom Ioannis Bakas University of Patras Igor BandosUniversidad de Valencia Jose L F BarbonIFTE UAM/CSIC Madrid Till BargheerMax-Planck-Institut für Gravitationsphysik (AEI), Potsdam Marco Baumgartl Eidgenössische Technische Hochschule (ETH), Zürich James BedfordImperial College London Raphael BenichouLaboratoire de Physique Théorique, École Normale Supérieure, Paris Francesco Benini SISSA, Trieste Eric Bergshoeff Centre for Theoretical Physics, University of Groningen Alice BernamontiVrije Universiteit, Brussel Julia BernardLaboratoire de Physique Théorique, École Normale Supérieure, Paris Adel Bilal Laboratoire de Physique Théorique, École Normale Supérieure, Paris Marco Billo' Università di Torino Matthias Blau Université de Neuchâtel Guillaume BossardAlbert-Einstein-Institut, Golm Leonardo BriziÉcole Polytechnique Fédérale de Lausanne (EPFL) Johannes BroedelLeibniz Universität Hannover (AEI) Tom BrownQueen Mary, University of London Ilka BrunnerEidgenössische Technische Hochschule (ETH), Zürich Erling BrynjolfssonUniversity of Iceland Dmitri BykovSteklov Institute, Moscow and Trinity College, Dublin Joan CampsUniversitat de Barcelona

  9. Préface

    NASA Astrophysics Data System (ADS)

    Jörgen Stevefelt, Henri Bachau Et

    2003-06-01

    'impulsions attosecondes qui permettra d'explorer la matière à l'echelle de temps atomique. En même temps la caractérisation de ces impulsions nécessite la conception de techniques nouvelles d'analyse du signal aux temps ultra brefs.L'intéret particulier du colloque UVX est de réunir les communautés de scientifiques qui vont des chercheurs s'intéressant aux processus fondamentaux à ceux travaillant dans les domaines les plus appliqués, voire industriels. Une caractéristique marquante de notre discipline est la rapidité avec laquelle les progrès réalisés dans les laboratoires de recherche sont diffusés vers les applications industrielles. Il est donc important de maintenir un bon équilibre entre les recherches a caractères fondamental et appliqué dans les laboratoires.Nous tenons remercier les membres du comité d'organisation, le comité scientifique et les différents partenaires, institutionnels et industriels, qui par leur soutien ont permis que le colloque UVX puisse se dérouler. Ce colloque a été parrainé par les départements des Sciences Physiques et Mathématiques (SPM) et des Sciences pour l'Ingénieur (SPI) du CNRS, la Délégation Générale de l'Armement (DGA), le CEA DRECAM, le CEA DAM, le Conseil Géneral de Charente Maritime, l'Université de Bordeaux I, la Société Française d'optique, le Groupement de Recherche “SAXO" du CNRS et la société Air Liquide.

  10. Prescrire du cannabis fumé pour la douleur chronique non cancéreuse

    PubMed Central

    Kahan, Meldon; Srivastava, Anita; Spithoff, Sheryl; Bromley, Lisa

    2014-01-01

    Résumé Objectif Offrir des conseils préliminaires sur la prescription de cannabis fumé pour la douleur chronique avant la publication de lignes directrices officielles. Qualité des données Nous avons examiné les ouvrages scientifiques sur l’efficacité analgésique du cannabis fumé et les dommages causés par la consommation de cannabis à des fins médicales et récréatives. Nous avons élaboré des recommandations concernant les indications et les contre-indications du cannabis fumé, les précautions à prendre et son dosage et nous avons classé les recommandations en fonction du niveau des données probantes. La plupart des données probantes sont de niveau II (études observationnelles bien effectuées) et de niveau III (opinion d’experts). Message principal Le cannabis fumé pourrait être indiqué chez des patients souffrant de douleurs neuropathiques sévères qui n’ont pas répondu à des essais suffisants de cannabinoïdes pharmaceutiques et d’analgésiques standards (données probantes de niveau II). Le cannabis fumé est contre-indiqué chez les patients de 25 ans ou moins (données probantes de niveau II); ceux qui font actuellement ou ont fait par le passé une psychose ou encore ont de forts antécédents familiaux de psychose (données probantes de niveau II); ceux qui ont ou ont eu un problème de consommation de cannabis (données probantes de niveau III); ceux qui ont un problème actuel de toxicomanie ou d’alcoolisme (données probantes de niveau III); ceux qui ont une maladie cardiovasculaire ou respiratoire (données probantes de niveau III); ou celles qui sont enceintes ou planifient une grossesse (données probantes de niveau II). Il devrait être utilisé avec précaution par les patients qui fument du tabac (données probantes de niveau II), qui sont à risque accru de maladies cardiovasculaires (données probantes de niveau III), qui ont des troubles d’anxiété ou de l’humeur (données probantes de niveau II) ou

  11. Spectroscopy of Luminous z > 7 Galaxy Candidates and Sources of Contamination in z > 7 Galaxy Searches

    NASA Astrophysics Data System (ADS)

    Capak, P.; Mobasher, B.; Scoville, N. Z.; McCracken, H.; Ilbert, O.; Salvato, M.; Menéndez-Delmestre, K.; Aussel, H.; Carilli, C.; Civano, F.; Elvis, M.; Giavalisco, M.; Jullo, E.; Kartaltepe, J.; Leauthaud, A.; Koekemoer, A. M.; Kneib, J.-P.; LeFloch, E.; Sanders, D. B.; Schinnerer, E.; Shioya, Y.; Shopbell, P.; Tanaguchi, Y.; Thompson, D.; Willott, C. J.

    2011-04-01

    Administration and made possible by the generous financial support of the W. M. Keck Foundation; the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA; the Canada-France-Hawaii Telescope with WIRCam, a joint project of CFHT, Taiwan, Korea, Canada, France, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institute National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii; the United Kingdom Infrared Telescope operated by the Joint Astronomy Centre on behalf of the Science and Technology Facilities Council of the U.K; the Subaru Telescope, which is operated by the National Astronomical Observatory of Japan; the Canada-France-Hawaii Telescope with MegaPrime/MegaCam operated as a joint project by the CFHT Corporation, CEA/DAPNIA, the National Research Council of Canada, the Canadian Astronomy Data Centre, the Centre National de la Recherche Scientifique de France, TERAPIX and the University of Hawaii; the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by AURA Inc., under NASA contract NAS5-26555; the XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA; the Chandra X-ray Observatory, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of the National Aeronautics Space Administration under contract NAS8-03060; the National Radio Astronomy Observatory which is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.; the 30 m telescope of the Institute for Radioastronomy at Millimeter Wavelengths (IRAM), which is funded by the German Max-Planck-Society, the French CNRS, and the Spanish National Geographical Institute.

  12. Le domaine des co-infections et des maladies concomitantes du Réseau canadien pour les essais VIH des IRSC : lignes directrices canadiennes pour la prise en charge et le traitement de la co-infection par le VIH et l’hépatite C chez les adultes

    PubMed Central

    Hull, Mark; Giguère, Pierre; Klein, Marina; Shafran, Stephen; Tseng, Alice; Côté, Pierre; Poliquin, Marc; Cooper, Curtis

    2014-01-01

    HISTORIQUE : De 20 % à 30 % des Canadiens qui vivent avec le VIH sont co-infectés par le virus de l’hépatite C (VHC), lequel est responsable d’une morbidité et d’une mortalité importantes. La prise en charge du VIH et du VHC est plus complexe en raison de l’évolution accélérée de la maladie hépatique, du choix et des critères d’initiation de la thérapie antirétrovirale et du traitement anti-VHC, de la prise en charge de la santé mentale et des toxicomanies, des obstacles socioéconomiques et des interactions entre les nouvelles thérapies antivirales à action directe du VHC et les antirétroviraux OBJECTIF : Élaborer des normes nationales de prise en charge des adultes co-infectés par le VHC et le VIH dans le contexte canadien. MÉTHODOLOGIE : Le Réseau canadien pour les essais VIH des Instituts de recherche en santé du Canada a réuni un groupe d’experts possédant des compétences cliniques en co-infection par le VIH et le VHC pour réviser les publications à jour ainsi que les lignes directrices et les protocoles en place. Après une vaste sollicitation afin d’obtenir des points de vue, le groupe de travail a approuvé des recommandations consensuelles, qu’il a caractérisées au moyen d’une échelle de qualité des preuves fondée sur la classe (bienfaits par rapport aux préjudices) et sur la catégorie (degré de certitude). RÉSULTATS : Toutes les personnes co-infectées par le VIH et le VHC devraient subir une évaluation en vue de recevoir un traitement du VHC. Les personnes qui ne sont pas en mesure d’entreprendre un traitement du VHC devraient être soignées pour le VIH afin de ralentir l’évolution de la maladie hépatique. La norme de traitement du VHC de génotype 1 est un régime comprenant de l’interféron pégylé et de la ribavirine dosée en fonction du poids, associés à un inhibiteur de la protéase du VHC. Pour les génotypes 2 ou 3, une bithérapie classique est recommandée pendant 24 semaines s

  13. Turkey BILSAT-1: a Case Study for the Surrey Know-How Transfer and Training Program

    NASA Astrophysics Data System (ADS)

    Ghafoor, Nadeem; Murat Leloglu, Ugur; Sweeting, Martin, , Sir

    2002-01-01

    Surrey has established itself over the past 18 years as a world leader in providing hands-on spacecraft engineering training through its Small Satellite Engineering Know-How Transfer and Training (`KHTT') programme. This 18- month course runs alongside the construction of a microsatellite executed through SSTL, and strikes a balance between classroom-based teaching and total immersion within professional engineering teams. Hands-on training is provided covering the entire satellite engineering process, from mission and subsystem design, through module manufacture, assembly and integration, to qualification and flight model environmental tests, launch and commissioning. SSTL's experience in providing the KHTT programme has resulted in a well-defined course structure that yet retains the ability to accommodate individual customer requirements. The programme also takes full advantage of SSTL's intrinsic link with the Surrey Space Centre (`SSC') at the University of Surrey, offering a range of MSc and PhD research programmes pursuing common research interests of both SSTL and the customer, and in many cases complementing the development of either the customer's satellite or their future plans for an evolved space capability. Throughout 2002, three KHTT programmes have run in parallel at SSTL. A team of 11 engineers from the Centre Nationale des Techniques Spatiales in Algeria have now reached completion of their programme with Alsat-1, the first enhanced microsatellite of the Disaster Monitoring Constellation (`DMC'). In December 2001, 15 engineers from the Federal Ministry of Science and Technology in Nigeria arrived at SSTL and are now midway through their programme with Nigeriasat-1, the second enhanced microsatellite of the DMC. Thirdly, arriving slightly earlier in August 2001, a team from Tubitak-Bilten in Turkey commenced their KHTT programme with BILSAT-1, a high-capability enhanced microsatellite also contributing to the DMC, and are due to continue through

  14. Determination of hydraulic properties of the Callovo-Oxfordian argillite at the bure site: Synthesis of the results obtained in deep boreholes using several in situ investigation techniques

    NASA Astrophysics Data System (ADS)

    Distinguin, Marc; Lavanchy, Jean-Marc

    Since 1991, ANDRA ( Agence Nationale pour la gestion des Déchets Radioactifs - National Radioactive Waste Management Agency) has been performing research on the possibility of geologic disposal of high level radioactive waste. In 1999, Andra began constructing an Underground Research Laboratory at Bure, a site located on the border of the Meuse-Haute-Marne departments, 300 km East of Paris. The laboratory is investigating the Callovo-Oxfordian argillite, a 130 m thick middle Jurassic stratum, at a depth of about 420 m. Argillite is a clay-rich sedimentary rock with low-permeability. Between 1994 and 2004, Andra collected from deep boreholes an impressive wealth of data covering a wide range of geosciences. This paper focuses on the hydraulic data related to argillite, including the results from short-term hydraulic packer tests and long-term monitoring of the formation pressures. Three types of tools are used on the site for investigations in deep boreholes. The first one is a conventional packer test tool used in the petroleum industry and adapted for hydrogeological purposes. The main objective is to determinate the permeability of the formation through short-term tests (24-72 h) at about 10 regular intervals. The two other types of tool are permanent monitoring devices. The electromagnetic pressure gauge (EPG) is totally isolated from the surface perturbations. There are no electric or hydraulic lines to the surface and the borehole is cemented. The advantage of this tool is that the formation almost recovers its initial pressure, avoiding disturbances from surface. Although the multi-packer equipment, installed in an open borehole can be affected by surface perturbations, it is used to measure pressure at different isolated levels in the same borehole ( i. e., 11 chambers in one borehole). Evaluations of the formation pressure (freshwater head) and hydraulic conductivity have been performed for all intervals investigated (19 short-term packer tests and 15 long

  15. Surrogate endpoints for overall survival in chemotherapy and radiotherapy trials in operable and locally advanced lung cancer: a re-analysis of meta-analyses of individual patients' data

    PubMed Central

    Mauguen, Audrey; Pignon, Jean-Pierre; Burdett, Sarah; Domerg, Caroline; Fisher, David; Paulus, Rebecca; Mandrekar, Samithra J; Belani, Chandra P; Shepherd, Frances A; Eisen, Tim; Pang, Herbert; Collette, Laurence; Sause, William T; Dahlberg, Suzanne E; Crawford, Jeffrey; O'Brien, Mary; Schild, Steven E; Parmar, Mahesh; Tierney, Jayne F; Pechoux, Cécile Le; Michiels, Stefan

    2013-01-01

    2=0·71, 95% CI 0·71–0·71 for concurrent chemotherapy and ρ2=0·61, 0·61–0·61 for modified vs standard radiotherapy) and trial-level correlations very good (R2=0·85, 95% CI 0·77–0·92 for concurrent chemotherapy and R2=0·95, 0·91–0·98 for modified vs standard radiotherapy). Interpretation We found a high level of evidence that DFS is a valid surrogate endpoint for overall survival in studies of adjuvant chemotherapy involving patients with non-small-cell lung cancers, and PFS in those of chemotherapy and radiotherapy for patients with locally advanced lung cancers. Extrapolation to targeted agents, however, is not automatically warranted. Funding Programme Hospitalier de Recherche Clinique, Ligue Nationale Contre le Cancer, British Medical Research Council, Sanofi-Aventis. PMID:23680111

  16. Contribution de l'altimetrie satellitaire a l'etude de la variabilite du niveau d'eau du Delta interieur du fleuve Niger

    NASA Astrophysics Data System (ADS)

    Telly Diepkile, Adama

    measurements were then corrected to bring them in the same altimetry reference level as Topex/Poseidon, thereby producing time series of 17 years (1992-2009). Following this analysis, we proposed a waveform retracking algorithm that integrates the backscattering coefficient to the time scale of penetration of the radar pulse in a medium with a presence of vegetation. The idea here is to consider the heterogeneity of a medium such as the Delta, which can be covered with vegetation. For this, we introduce into the equation of the waveform, the backscattering coefficient estimated from the so called water cloud model, to create a new algorithm called retracking algorithm of water cloud. This algorithm was applied to the Envisat and OSTM/Jason-2 data. The results of the algorithm were validated with in situ measurements of the Direction Nationale de l'Hydraulique du Mali and also with measurements acquired during a campaign of data collection conducted between August and October 2009. The observed differences are generally small (<+/- 1 m). The retracking algorithm of water cloud was compared to other existing algorithms. It shows a strong correlation with Ice-1 (R 2 = 0,84). Finally, we analyzed the influence of precipitation on the variations of the altimetry-derived water levels. Three sources of precipitations from satellite measurements and reanalysis data were considered in three catchments (basin Fouta Djallon in upstream, Bani basin and the inner basin in Mali). The analysis reveals the importance of precipitations, particularly in the basin of Fouta Djallon. Approximately 70% of sites analyzed in the Delta show a relatively strong correlation (R2 > 0,40) with the cumulative precipitations in the basins considered. Keywords : Remote Sensing, Satellite altimetry, Continental waters, Water level, Long term analysis, Inner Delta of Niger River, Water-cloud model, Envisat, Topex/Poseidon.

  17. History of NAMES Conferences

    NASA Astrophysics Data System (ADS)

    Filippov, Lev

    2013-03-01

    Franco-Russian NAMES Seminars are held for the purpose of reviewing and discussing actual developments in the field of materials science by researchers from Russia and from the Lorraine Region of France. In more precise terms, as set down by the organizers of the seminar (the Moscow Institute of Steel and Alloys and the Institut National Polytechnique de Lorraine), the mission of the seminars is as follows: the development of scientific and academic contacts, giving a new impulse to joint fundamental research and technology transfer the development and consolidation of scientific, technical and business collaboration between the regions of Russia and Lorraine through direct contact between the universities, institutes and companies involved The first Seminar took place on 27-29 October 2004, at the Institut National Polytechnique de Lorraine (on the premises of the Ecole Européenne d'Ingénieurs en Génie des Matériaux, Nancy, France). The number, variety and quality of the oral presentations given and posters exhibited at the first Seminar were of high international standard. 30 oral presentations were given and 72 posters were presented by 19 participants from five universities and three institutes of the Russian Academy of Sciences participants from 11 laboratories of three universities from the Lorraine region three industrial companies, including the European Aeronautic Defence and Space Company—EADS, and ANVAR (Agence Nationale de Valorisation de la Recherche) From 2005 onwards, it was decided to organize the Seminar every other year. The second Seminar convened on the occasion of the 75th Anniversary of the Moscow Institute of Steel and Alloys on 10-12 November 2005 in Moscow, Russia. The seminar demonstrated the efficiency of the scientific partnership founded between the research groups of Russia and France during the first Seminar. High productivity of the Franco-Russian scientific cooperation on the basis of the Research-Educational Franco

  18. Radon potential determination by a combination of geological mapping, geochemistry, groundwater investigations and airborne geophysics

    NASA Astrophysics Data System (ADS)

    Schubert, G.; Motschka, K.; Ahl, A.; Slapansky, P.; Finger, F.; Alletsgruber, I.; Gasser, V.; Supper, R.; Bieber, G.

    2009-04-01

    . Ein österreichweiter Überblick. - report, Bundesanstalt für Lebensmitteluntersuchung und -forschung, Vienna. H. Friedmann, L. Breitenhuber, E. Hamernik, W. Hofmann, H. Kaineder, V. Karg, P. Kindl, H. Lettner, F. J. Maringer, L. Mossbauer, E. Nadschläger, G. Oberlercher, K. Pock, F. Schönhofer, W. Seiberl, S. Sperker, H. Stadtmann, F. Steger, F. Steinhäusler, M.Tschurlovits (1997): Das österreichische Radonprojekt - Mitt. Österr. Geol. Ges., 88, Austrian Geol. Soc., Vienna. H. Friedmann, C. Atzmüller, C. Beck, L. Breitenhuber, P. Brunner, K. Fink5, K. Fritsche, D. Gottsbachner, E. Hamernik, W. Hofmann, R. Hover, M. Kafesie, H. Kaineder,P. Karacson, V. Karg), P. Kindl, M. Kompatscher, C. Kralik, C. Kriha, J. Krischan, S. Lackner, H. Lettner, U. Mack, F. J. Maringer, L. Mossbauer, E. Nadschläger, K. Pock, W. Ringer, C. Schindler F. Schönhofer, P. Schönleitner, B. Schramm, T. Singer, S. Sperker, H. Stadtmann, F. Steger, F. Steinhäusler, M. Tschurlovits, I. Weilguni, W. Weiss, R. Weissenbök, H. Wihlidal, R.Winkler, P. Zimprich (2007): Das österreichische nationale Radonprojekt (ÖNRAP). Projekt-Endbericht. - report, Bundesministerium für Land- und Forstwirtschaft, Umwelt und Wasserwirtschaft, Vienna. G. Schubert, F. Finger, V. Gasser, H. Lettner (2003): Radionuklide im Grundwasser des kristallinen Untergrunds im Mühlviertel. - unpubl. report, Geol. Survey of Austria, Vienna.

  19. Epidemiology of multiple sclerosis.

    PubMed

    Leray, E; Moreau, T; Fromont, A; Edan, G

    2016-01-01

    Multiple sclerosis (MS) is the most frequently seen demyelinating disease, with a prevalence that varies considerably, from high levels in North America and Europe (>100/100,000 inhabitants) to low rates in Eastern Asia and sub-Saharan Africa (2/100,000 population). Knowledge of the geographical distribution of the disease and its survival data, and a better understanding of the natural history of the disease, have improved our understanding of the respective roles of endogenous and exogenous causes of MS. Concerning mortality, in a large French cohort of 27,603 patients, there was no difference between MS patients and controls in the first 20 years of the disease, although life expectancy was reduced by 6-7 years in MS patients. In 2004, the prevalence of MS in France was 94.7/100,000 population, according to data from the French National Health Insurance Agency for Salaried Workers (Caisse nationale d'assurance maladie des travailleurs Salariés [CNAM-TS]), which insures 87% of the French population. This prevalence was higher in the North and East of France. In several countries, including France, the gender ratio for MS incidence (women/men) went from 2/1 to 3/1 from the 1950s to the 2000s, but only for the relapsing-remitting form. As for risk factors of MS, the most pertinent environmental factors are infection with Epstein-Barr virus (EBV), especially if it arises after childhood and is symptomatic. The role of smoking in MS risk has been confirmed, but is modest. In contrast, vaccines, stress, traumatic events and allergies have not been identified as risk factors, while the involvement of vitamin D has yet to be confirmed. From a genetic point of view, the association between HLA-DRB1*15:01 and a high risk of MS has been known for decades. More recently, immunogenetic markers have been identified (IL2RA, IL7RA) and, in particular thanks to studies of genome-wide associations, more than 100 genetic variants have been reported. Most of these are involved in

  20. [Pre-hospital management of adults with life-threatening emergencies].

    PubMed

    Wattel, Francis; Dubois, François

    2012-01-01

    , fewer voluntary firemen, hospital reorganization, tight funding, difficulties of medical dispatching, and the varying skills of "first-on-the-scene "emergency workers. Grievances include late emergency responses, inappropriate medical care, and dispatching to the wrong facility. This raises the question of equal opportunity for all in a country with widely varying geographic features and population density. Improvement in the system's efficiency will require a series of objectives to be met in varied and complementary--Enhanced functional coordination, by speeding up the deployment of the ANTARES digital radio-frequency transmission network (Adaptation Nationale des Transmissions Aux Risques Et aux Secours).--Implementation of a network of emergency services with varying degrees of emergency healthcare management related to the technical nature of the facilities. Three levels of emergency healthcare must be made available: level 1 is provided by local hospitals, level 2 includes support facilities available in general hospitals (not necessarily the nearest hospital), and level 3 provides specialized healthcare in large and/or training hospitals with specialized departments. Life-threatening emergency situations are to be handled by level 2 or 3 facilities. Specific facilities must be selected as reference centers. In France, the ARS (Agences Régionales de Santé) is in charge of this procedure, as it provide funding for healthcare continuity--Reducing inequalities in access to emergency care. This will involve improving the network of SDIS brigades, making local medical facilities more responsive, delegating more medical procedures, on-site telemedicine, providing more helicopters equipped with healthcare facilities, more automated external defibrillators, and more dedicated neuro-vascular units.--First aid training must be made widely available. The French National Academy of Medicine has approved ten recommendations regarding organization and facilities. PMID

  1. A multi-scale analysis of in-situ precipitation data across the Sahelian Gourma

    NASA Astrophysics Data System (ADS)

    Guichard, Françoise; Frappart, Frédéric; Hiernaux, Pierre; Kergoat, Laurent; Mougin, Eric; Arjounin, Marc; Koité, Mohamed; Lebel, Thierry; Bock, Olivier; Meynadier, Rémi

    2010-05-01

    Droughts and floods are recurrent features of the Sahelian climate, which is also characterized by a very large variability of rainfall, in both space and time. The present study focuses on the Malian Gourma (2°W-1°E, 14.5°N-17.5°N), located in the Central Sahel, where the very large majority of rainfall events occur between June and September, during the West African monsoon. Rainfall is analysed with two complementary in-situ datasets: (i) daily rainfall series from 25 stations covering the period 1900-2007, and provided by the Direction Nationale de la Météorologie of Mali, and (ii) high-frequency rainfall data provided by a network of about 20 tipping bucket rain gauges, starting in 2005 - these rain gauges have been installed for the African Monsoon Multidisciplinary Analysis (AMMA), see Frappart et al. (2009) for additional information. The Gourma displays a particularly marked meridional gradient, with annual rainfall decreasing from about 500 mm at 14°N to 150 mm at 17.5°N. In line with previous studies focused on the Sahel, the area also displays a strong decadal variability, with the same succession of wet (1950-1969) and dry decades (1970-2007). The decrease of annual rainfall is explained by a reduction in the number of the rainy days in southern Gourma, but a decrease in both the number of rainy days and the daily rainfall in northern and central Gourma. This latter result contrasts with some studies focused on more southern areas. It may involves an influence of the distance from the inter-tropical discontinuity. The length of the rainy season has varied since the 1950s with two episodes of shorter rainy seasons: during the drought of the 1980s and also since 2000. However, this second episode is characterized by an increase in the daily rainfall, which suggests an intensification of rainfall events in the more recent years. High-frequency data show that most rainfall is produced by intense convective events whose characteristics are

  2. Cosmogenic Beryllium Production from Ocean Sediment Sequences Help to Construct Accurate Records of the Geodynamo Variation at the Millennial to Million Year Scale

    NASA Astrophysics Data System (ADS)

    Thouveny, N.; Ménabréaz, L.; Bourles, D. L.; Demory, F.; Guillou, V.; Arnold, M.; Vidal, L.

    2013-12-01

    The possible contribution of the axial precession to the energy of the geodynamo was recently reintroduced by theoretical and experimental studies. It is supported by relative paleointensity stacks and deep sea floor magnetization records documenting series of geomagnetic dipole lows (GDL) with recurrence at periods ranging from 30 to 120 kyr, and intriguing phase relationships with obliquity variations and δ18O records (e.g. Fuller, 2006; Thouveny et al. 2008). Yet, these time-series are presently not precise and complete enough to validate this fundamental and debated relationship. The MAG-ORB project funded by the French "Agence nationale de la Recherche" aims at reconstructing the series of GDL over the last Ma, by coupling -on the very same sedimentary sequences- the reconstructions of paleomagnetic variations, cosmogenic10Be production variations and δ18O isotope variations. Recent results (e.g. Ménabréaz et al., 2012, 2013) demonstrate that 10Be overproduction events are systematically induced by the GDL linked with excursions and reversals -as awaited from the theoretical and empirical non linear inverse relationship established between the magnetic moment value and the penetration rate of cosmic rays and particles. The calibration of the authigenic 10Be/9Be ratio signals using absolute Virtual (axial) Dipole Moment values allowed us to construct 10Be-derived Geomagnetic Dipole Moment records over the last millennium, the last 60 ka and the last Ma, allowing to assess the robustness of the GDL series by a method completely independent from rock and paleo-magnetic methods. These records are comparable with individuals RPI records obtained from the same cores, and with global RPI stacks (e.g. GLOPIS, SINT 800 and PISO-1500). Since the Beryllium atoms are adsorbed on the settling silicate particles, the measured 10Be/9Be ratio signatures of cosmogenic isotope overproductions accurately indicate the exact stratigraphic position of the GDL in the sedimentary

  3. Tangafric: a software for the estimation of textural and hydraulic properties in shallow aquifers from well logs in Senegal and Guinea

    NASA Astrophysics Data System (ADS)

    Fussi, Fabio; Bonomi, Tullia; Fava, Francesco; Hamidou, Barry; Hamidou Khane, Cheikh; Faye, Gayane; Wade, Souleye; Colombo, Roberto

    2014-05-01

    Background In order to increase access to drinking water in Africa there is more and more interest in the promotion of manual drilling techniques, without need of expensive drilling equipment, but they can be applied only in those areas with suitable hydrogeological conditions: thick layers of unconsolidated sediments and shallow groundwater level. Mapping of suitable zones for manual drilling at national level in Africa is a crucial activity and local institutions and UNICEF are implementing specific programs for its promotion, but the limitation in available data concerning shallow hydrogeological aquifers are limited. The research has been developed in the project "Use of remote sensing and terrain modeling to identify suitable zones for manual drilling in Africa and support low cost water supply", within the scientific cooperation between the University of Milano-Bicocca, Universite' Cheick Anta Diop (Dakar Senegal) , SNAPE - Service Nationale de Points d'Eau (Conakry Guinea), UNICEF Senegal and UNICEF Guinea. The project is funded by NERC (National Environmental Research Council, UK). Objective of the research: The presented work is only the starting point of the project aiming to elaborate an automatic procedures to manage and improve the existing database of borehole logs in Senegal and Guinea for the interpretation of shallow hydrogeological conditions and identification of suitable zones for manual drilling, in two pilot areas: Louga (Northwestern Senegal) and Faranah/Kankan (Eastern Guinea). Within the objective of the project is also considered the integration of Remote Sensing to support hydrogeological interpretation, especially where borehole logs are not present. Methodology Focus is to create a hydrogeological database, TANGAFRIC, to organize, codify and elaborate hydrogeological data. The metodology derives from the software TANGRAM (www.tangram.samit.unimib.it) produced by the University of Milano Bicocca, with innovative aspect of stratigraphic

  4. Influence of mycorhization and soil organic matters on lead and antimony transfers to vegetables cultivated in urban gardens: environmental and sanitary consequences

    NASA Astrophysics Data System (ADS)

    Pierart, Antoine; Braud, Armelle; Lebeau, Thierry; Séjalon-Delmas, Nathalie; Dumat, Camille

    2014-05-01

    The European Environment Agency estimates that c.a. 250 000 sites required clean up and that about 100 000 ha could have been contaminated by metals in Europe. Numerous remediation techniques have been therefore tested and phytoremediation appears as a sustainable and low cost in situ technique particularly for large-scale remediation of polluted arable soils. Arbuscular Mycorrhizal Fungi (AMF) are already used in phytoextraction or phytostabilisation of many metal(loid)s (GU ET AL., 2013, SHARMA AND SHARMA, 2013). However, while plant inoculation with AMF will mostly result of an increase of the plant biomass, the response for lead accumulation in shoots is contrasted (LEBEAU ET AL., 2008). Furthermore, nothing is actually known for Sb transfer to plants phytoremediation-assisted AMF. Yet recently, many researches concern the accumulation of Sb in the environment, its (eco)toxicity and the risk of bioaccumulation in vegetables (FENG ET AL., 2013), especially in some China areas where Sb mining activities have widely contaminated arable lands (WU ET AL., 2011). Our research project, which is part of a national program for urban gardens (JASSUR, http://www.agence-nationale-recherche.fr), focused on polluted soils in associative urban gardens with both geogenic and anthropogenic origins for Pb and Sb. The impact of Pb and Sb on AMF density and diversity was studied using morphological and biomolecular approaches. The role of AMF symbiosis with Lettuce (Lactuca sativa L.) on Pb and Sb compartmentalization, speciation and phytoavailability was investigated. The influence of soil organic matters on these processes was examined. Eventually, the part of metal(loid)s available for humans in case of ingestion of lettuces unfit for human consumption (FOUCAULT ET AL., 2013; XIONG ET AL., 2013) will be assessed in relation with the influence of AMF symbiosis and organic matter. Key Words: Mycorrhiza, Antimony, Compartmentation, Speciation, Edible Plants, Urban Agriculture

  5. Self-Employment among Same-Sex and Opposite-Sex Couples in Canada.

    PubMed

    Waite, Sean; Denier, Nicole

    2016-05-01

    This study presents novel evidence on the relationship between sexual orientation and self-employment. Using data from the 2001 and 2006 Census of Canada and the 2011 Canadian National Household Survey, we explore the propensity for self-employment among same- and opposite-sex couples. We examine the demographic, human capital, and family characteristics of coupled gay men and lesbians relative to their coupled heterosexual counterparts to offer potential mechanisms generating differences in rates of self-employment. Our analysis further considers occupational variability in the likelihood of self-employment. We find that gay men are less likely and lesbians more likely than heterosexuals to be self-employed; however, there is significant variation across occupations. Gay men are more likely to be self-employed in arts and culture, sales and service, and natural and applied sciences, but less likely in business, finance, and health-related occupations. Lesbians are much more likely to be self-employed in health-related occupations, natural and applied sciences, and arts and culture. Marriage and having children are significant predictors of self-employment for coupled heterosexual women but not lesbians. Cette étude présente des évidences empiriques concernant la relation entre l'orientation sexuelle et le travail indépendant. Utilisant des données provenant du Recensement du Canada de 2001 et de 2006, ainsi que l'Enquête nationale auprès des ménages (ENM) de 2011, nous explorons la tendance du travail indépendant parmi les couples de même sexe et ceux de sexe opposé. Ainsi, nous examinons les caractéristiques démographiques, du capital humain et familiales des couples gais et lesbiens par rapport à leurs homologues hétérosexuels, afin de démontrer une corrélation entre l'orientation sexuelle et la probabilité d'être travailleur indépendant - une causation qui nous semble évident et que nous analysons plus en profondeur. Nous concluons d

  6. Preface: Materiaux 2010

    NASA Astrophysics Data System (ADS)

    Cheikhrouhou, Abdelwaheb

    2012-02-01

    Ceramics, glasses, polymers Natural materials (phosphates, clay,...) Metallic materials, alloys, metallurgy,... Others (materials and environment, materials and energy, biomaterials,...) I want to thank the scientific committee, the organizing committee, the local committee and everyone who contributed to the organization of this meeting for their invaluable efforts in order to guarantee the complete success of this conference. Abdelwaheb Cheikhrouhou President of 'Tu-MRS' Chairman of the Conference 'MATERIAUX 2010' Conference photograph Committies Organizing Committee Chairman CHEIKHROUHOU Abdelwaheb (Faculté des Sciences de Sfax) Members ALAYA Sahbi (Faculté des Sciences de Gabès) BENNACEUR Raouf (Faculté des Sciences de Tunis) BEN SALEM Mohamed (Faculté des Sciences de Bizerte) CHEIKHROUHOU-KOUBAA Wissem (Faculté des Sciences de Sfax) EL JANI Belgacem (Faculté des Sciences de Monastir) EZZAOUIA Hatem (Centre de Recherches et de Technologies de l'Energie, Technopole de Borj Cédria) LAMLOUMI Jilani (Ecole Supérieure des Sciences et Techniques de Tunis) REZIG Bahri (Ecole Nationale d'Ingénieurs de Tunis) Local Committee Chairman CHEIKHROUHOU Abdelwaheb (Faculté des Sciences de Sfax) Members CHEIKHROUHOU-KOUBAA Wissem (Faculté des Sciences de Sfax) KOUBAA Mohamed (Institut Supérieur de Biotechnologie de Sfax) NJEH Anwar (Institut Préparatoire aux Etudes d'Ingénieurs de Sfax) BEN SALAH Issam (Faculté des Sciences de Sfax) TAKKALI Férid (Faculté des Sciences de Sfax) REGAIEG Yassin (Faculté des Sciences de Sfax) OTHMANI Safa (Faculté des Sciences de Sfax) MNASSRI Rafik (Faculté des Sciences de Sfax) Secretariat BEN GHOZLEN Afifa (Faculté des Sciences de Sfax) BOUGHARIOU Sana (Faculté des Sciences de Sfax) Scientific Committee M. ADDOU, Faculté des Sciences de Kénitra (Morocco) N. AMDOUNI, Faculté des Sciences de Tunis (Tunisia) M. BACCOUCHE, Faculté des Sciences d'Annaba (Algeria) H. BATIS, Faculté des Sciences de Tunis (Tunisia) A. BELAFHAL

  7. Evaluation de la tenue du partogramme dans une maternité universitaire

    PubMed Central

    Limam, Manel; Zedini, Chekib; El Ghardallou, Meriem; Mellouli, Menel; Bougmiza, Iheb; Sahli, Jihène; Khairi, Hédi; Mtiraoui, Ali; Ajmi, Thouraya Nabli

    2015-01-01

    Introduction La mortalité maternelle est un problème majeur de santé mondiale. Une grande proportion de ces décès serait évitable par des soins adéquats, une aide à l'accouchement, la disponibilité des soins d'urgence et l'utilisation des outils d'aide à la décision tels que le partogramme. L'objectif était d’évaluer l’écart entre ce qui est censé être fait et ce qui est fait réellement pour les différents paramètres situés dans le partogramme au sein d'une maternité de 3ème niveau et élaborer des recommandations pour la mise en place d'un plan d'action. Méthodes Il s'agit d'une étude descriptive rétrospective par audit clinique, effectuée sur un échantillon de 400 dossiers obstétricaux des parturientes ayant accouchées dans la maternité du CHU Farhat Hached durant l'année 2011. Le référentiel utilisé est celui réalisé par l'Agence Nationale d'Accréditation et d'Evaluation en Santé en l'an 2000, concernant la qualité de la tenue du partogramme. Résultats La majorité des critères d’évaluation portant sur la présentation du partogramme était conforme. Deux critères concernant la variété de la présentation et le rythme cardiaque fœtal étaient non conformes parmi ceux portant sur la surveillance du fœtus. Plusieurs critères en rapport avec la surveillance de la mère étaient non conformes. Aucun des critères portant sur les traitements administrés et les marqueurs d’évènements n'est conforme. Les critères portant sur la naissance et la surveillance immédiate qui étaient non conformes sont: le début des efforts expulsifs, le mode d'accouchement, l’état du périnée, la délivrance et la révision utérine. Conclusion La véritable démarche de l'audit clinique se doit d'aller au-delà du recueil et de l'analyse des données, le but final étant l'amélioration des pratiques. PMID:26516400

  8. Utilizing the International GeoSample Number Concept during ICDP Expedition COSC

    NASA Astrophysics Data System (ADS)

    Conze, Ronald; Lorenz, Henning; Ulbricht, Damian; Gorgas, Thomas; Elger, Kirsten

    2016-04-01

    The concept of the International GeoSample Number (IGSN) was introduced to uniquely identify and register geo-related sample material, and make it retrievable via electronic media (e.g., SESAR - http://www.geosamples.org/igsnabout). The general aim of the IGSN concept is to improve accessing stored sample material worldwide, enable the exact identification, its origin and provenance, and also the exact and complete citation of acquired samples throughout the literature. The ICDP expedition COSC (Collisional Orogeny in the Scandinavian Caledonides, http://cosc.icdp-online.org) prompted for the first time in ICDP's history to assign and register IGSNs during an ongoing drilling campaign. ICDP drilling expeditions are using commonly the Drilling Information System DIS (http://doi.org/10.2204/iodp.sd.4.07.2007) for the inventory of recovered sample material. During COSC IGSNs were assigned to every drill hole, core run, core section, and sample taken from core material. The original IGSN specification has been extended to achieve the required uniqueness of IGSNs with our offline-procedure. The ICDP name space indicator and the Expedition ID (5054) are forming an extended prefix (ICDP5054). For every type of sample material, an encoded sequence of characters follows. This sequence is derived from the DIS naming convention which is unique from the beginning. Thereby every ICDP expedition has an unlimited name space for IGSN assignments. This direct derivation of IGSNs from the DIS database context ensures the distinct parent-child hierarchy of the IGSNs among each other. In the case of COSC this method of inventory-keeping of all drill cores was done routinely using the ExpeditionDIS during field work and subsequent sampling party. After completing the field campaign, all sample material was transferred to the "Nationales Bohrkernlager" in Berlin-Spandau, Germany. Corresponding data was subsequently imported into the CurationDIS used at the aforementioned core storage

  9. Mixing against culture vs mixing against nature: ontologization of prohibited interethnic relationships.

    PubMed

    Roncarati, Alessandra; Pérez, Juan A; Ravenna, Marcella; Navarro-Pertusa, Esperanza

    2009-02-01

    qui vivent en contact les uns avec les autres d'intergir ensemble. Le processus d'ontologisation consiste à séparer quelques humains de leur propre espèce et de les ancrer dans un autre environnement, celui des animaux, à titre d'exemple. Nous proposons que ce qui est sous-jacent au fameux slogan «égaux mais distincts» est la représentation sociale de mélange inter-racial comme un phénomène «contre-nature». Il est prédit qu'une relation sexuelle entre des gens de différentes «races» amènerait à un plus grand degré d'ontologisation et en tant que tel, ce mélange sera expliqué en termes de pensée biologistique, à l'instar d'une nature instinctuelle ou une impulsion animale atavistique. Une expérimentation (N = 360) présente le cas d'une femme qui, même si elle est déjà dans une relation stable, elle est infidèle à son partenaire. Dans un devis 2×3, l'identité ethno-nationale de cette femme (endogroupe-espagnol/italien vs. exogroupe-sénégalais) et l'identité ethno-nationale de ses amants (endogroupe-espagnol/italien vs. exogroupe-roumain vs. exogroupe-sénégalais) ont été manipulées. En général, les résultats soutiennent l'hypothèse de l'ontologisation mieux dans les condition inter-raciales plutôt que le favoritisme de l'endogroupe coutumier et/ou le biais de la discrimination de l'exogroupe. Ensuite, nous poursuivons en discutant la manière dont la façon de penser biologistique permet une différentiation au niveau humain, en termes de groupes culturels et de groupes naturels, dans des «races», de manière à ce qu'une relation sexuelle inter-raciale est vue comme une preuve d'une impulsion sauvage et irrépressible qui peut stigmatiser les gens impliqués dans ces relations. En el presente artículo se discute la teoría de la ontologización: representaciones sociales que prevenien la fusión entre los miembros de grupos minoritarios o mayoritarios que viven en contacto unos con otros. El proceso de ontologizaci

  10. Préface

    NASA Astrophysics Data System (ADS)

    Ouerdane, Youcef; Laporte, Pierre

    2005-06-01

    L'objectif de la série de colloques UVX est de réunir, au rythme d'une fois tous les deux ans, les scientifiques et industriels travaillant dans le domaine du développement des sources de photon de grande énergie (UV, VUV, et X) et de leurs applications. En particulier cette manifestation est l'occasion de faire se rencontrer une communauté très pluridisciplinaire (physique, chimie, biologie, sciences de l'univers) liée à des domaines en forte évolution technologique (lasers et rayonnement synchrotron notamment). Le colloque UVX 2004 s'est tenu au Palais des Congrès de Saint-Étienne (42000) du 7 au 11 juin 2004. La période écoulée depuis l'édition précédente (Oléron 2002) a été particulièrement active dans tous les domaines concernés : grands projets de sources, méthodes de diagnostic au sens large. Une nouvelle fois on constate que le bref et l'ultra-bref ont une place privilégiée, qu'il s'agisse du travail sur les accélérateurs ou sur les lasers qui, bien sûr, dans la course aux temps courts remportent la palme avec la présence de spécialistes du domaine attoseconde. La communauté représentée a la chance d'être en prise directe avec de très grands projets en phase active de réalisation comme le Laser Megajoule (LMJ), la source SOLEIL, et un projet d'ampleur plus modeste mais remarquable dans son domaine : la source LASERIX d'Orsay/Palaiseau. On pourra citer aussi le projet Arc en Ciel qui, lui, est encore au stade de sa définition. - SOLEIL, source de nouvelle génération de rayonnement synchrotron (plateau de Saclay) est dans une phase active de réalisation : achèvement de l'infrastructure en 2005 et injection du 1o faisceau dans l'anneau de stockage prévu également en 2005. Cette source devrait être la meilleure au monde dans le domaine VUV/X mous, tout en restant très polyvalente (brillance, accordabilité, structure temporelle, polarisation) et complémentaire de l'ESRF. Au final on disposera de 21 lignes de lumi

  11. The Next Generation Virgo Cluster Survey (NGVS). XIII. The Luminosity and Mass Function of Galaxies in the Core of the Virgo Cluster and the Contribution from Disrupted Satellites

    NASA Astrophysics Data System (ADS)

    Ferrarese, Laura; Côté, Patrick; Sánchez-Janssen, Rúben; Roediger, Joel; McConnachie, Alan W.; Durrell, Patrick R.; MacArthur, Lauren A.; Blakeslee, John P.; Duc, Pierre-Alain; Boissier, S.; Boselli, Alessandro; Courteau, Stéphane; Cuillandre, Jean-Charles; Emsellem, Eric; Gwyn, S. D. J.; Guhathakurta, Puragra; Jordán, Andrés; Lançon, Ariane; Liu, Chengze; Mei, Simona; Mihos, J. Christopher; Navarro, Julio F.; Peng, Eric W.; Puzia, Thomas H.; Taylor, James E.; Toloba, Elisa; Zhang, Hongxin

    2016-06-01

    satellites, α = ‑1.21 ± 0.05, which is only 1.7σ shallower than measured in the core of the Virgo Cluster. Based on observations obtained with MegaPrime/MegaCam, a joint project of the Canada–France–Hawaii Telescope (CFHT) and CEA/DAPNIA, at the CFHT, which is operated by the National Research Council (NRC) of Canada, the Institut National des Science de l’Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii.

  12. The bimodality of the 10k zCOSMOS-bright galaxies up to z ~ 1: a new statistical and portable classification based on optical galaxy properties

    NASA Astrophysics Data System (ADS)

    Coppa, G.; Mignoli, M.; Zamorani, G.; Bardelli, S.; Lilly, S. J.; Bolzonella, M.; Scodeggio, M.; Vergani, D.; Nair, P.; Pozzetti, L.; Cimatti, A.; Zucca, E.; Carollo, C. M.; Contini, T.; Le Fèvre, O.; Renzini, A.; Mainieri, V.; Bongiorno, A.; Caputi, K. I.; Cucciati, O.; de la Torre, S.; de Ravel, L.; Franzetti, P.; Garilli, B.; Memeo, P.; Iovino, A.; Kampczyk, P.; Kneib, J.-P.; Knobel, C.; Koekemoer, A. M.; Kovač, K.; Lamareille, F.; Le Borgne, J.-F.; Le Brun, V.; Maier, C.; Pellò, R.; Peng, Y.; Perez-Montero, E.; Ricciardelli, E.; Scarlata, C.; Silverman, J. D.; Tanaka, M.; Tasca, L.; Tresse, L.; Abbas, U.; Bottini, D.; Capak, P.; Cappi, A.; Cassata, P.; Fumana, M.; Guzzo, L.; Leauthaud, A.; Maccagni, D.; Marinoni, C.; Meneux, B.; Oesch, P.; Porciani, C.; Scaramella, R.; Scoville, N.

    2011-11-01

    galaxies with very large masses (M > 5 × 1010 M⊙) have mostly completed their transition to the early-type regime before z ~ 1. Based on observations undertaken at the European Southern Observatory (ESO) Very Large Telescope (VLT) under Large Program 175.A-0839. Also based on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, operated by AURA Inc., under NASA contract NAS 5-26555, with the Subaru Telescope, operated by the National Astronomical Observatory of Japan, with the telescopes of the National Optical Astronomy Observatory, operated by the Association of Universities for Research in Astronomy, Inc. (AURA) under cooperative agreement with the National Science Foundation, and with the Canada-France-Hawaii Telescope, operated by the National Research Council of Canada, the Centre National de la Recherche Scientifique de France, and the University of Hawaii.

  13. Scientists Meet to Plan ALMA Science Program

    NASA Astrophysics Data System (ADS)

    1999-09-01

    Two hundred astronomers from around the world will meet in Washington, DC on October 7 and 8 to discuss exciting new science to be done with the Atacama Large Millimeter Array (ALMA). The conference will be held at the Carnegie Institution of Washington (CIW), 1530 P St. NW, and is sponsored by Associated Universities, Inc., which operates the National Radio Astronomy Observatory (NRAO) for the National Science Foundation (NSF). ALMA will study the structure of the early universe and the evolution of galaxies; gather crucial data on the formation of stars, protoplanetary disks, and planets; and provide new insights on the familiar objects of our own solar system. The array, expected to consist of 64 telescopes with 12-meter dish antennas, will be built at a high-altitude, extremely dry mountain site in Chile's Atacama desert in the next decade. ALMA is an international partnership between the United States (National Science Foundation) and Europe. European participants include the member states of the European Southern Observatory (Belgium, Denmark, France, Germany, Italy, the Netherlands, Sweden and Switzerland), the Centre National de la Recherche Scientifique (France), the Max-Planck Gesellschaft (Germany), the Netherlands Foundation for Research in Astronomy, and the United Kingdom Particle Physics and Astronomy Research Council. The project is currently in a Design and Development phase governed by a Memorandum of Understanding between the United States and Europe. It is hoped and expected that Japan will also join the project as a third equal partner. Negotiations are currently underway to add Canada to the United States team and Spain to the European team. "The ALMA partners from the U.S. team, the European team, and hopefully Japan, will form the world's first truly global astronomical collaboration," said Dr. Riccardo Giacconi, President of Associated Universities, Inc., "and together will build a magnificent millimeter/submillimeter observatory for the

  14. National Academy of Sciences Recommends Continued Support of ALMA Project

    NASA Astrophysics Data System (ADS)

    2000-05-01

    , will be built at a high-altitude, extremely dry mountain site in Chile's Atacama desert. The array is scheduled to be completed sometime in this decade. Millimeter-wave astronomy studies the universe in the spectral region where most of its energy lies, between the long-wavelength radio waves and the shorter-wavelength infrared waves. In this realm, ALMA will study the structure of the early universe and the evolution of galaxies; gather crucial data on the formation of stars, protoplanetary disks, and planets; and provide new insights on the familiar objects of our own solar system. "Most of the photons in the Universe lie in the millimeter wavelength regime; among existing or planned instruments only ALMA can image the sources of these photons with the crispness required to understand the events of galaxy, star and planet formation which launched them into space," said NRAO's Dr. Alwyn Wootten, U.S. ALMA Project Scientist. ALMA is an international partnership between the United States (National Science Foundation) and Europe. European participants include the European Southern Observatory, the Centre National de la Recherche Scientifique (France), the Max-Planck Gesellschaft (Germany), the Netherlands Foundation for Research in Astronomy, the United Kingdom Particle Physics and Astronomy Research Council, the Oficina de Ciencia Y Tecnologia/Instituto Geografico Nacional (Spain), and the Swedish Natural Science Research Council. The National Radio Astronomy Observatory is a facility of the National Science Foundation, operated under cooperative agreement by Associated Universities, Inc.

  15. Croissance epitaxiale de GaAs sur substrats de Ge par epitaxie par faisceaux chimiques

    NASA Astrophysics Data System (ADS)

    Belanger, Simon

    de confirmer l'efficacite du procede de preparation de surface et d'identifier les conditions de croissance optimales. Les resultats de caracterisation indiquent que les materiaux obtenus presentent une tres faible rugosite de surface, une bonne qualite cristalline et un dopage residuel relativement important. De plus, l'interface GaAs/Ge possede une faible densite de defauts. Finalement, la diffusion d'arsenic dans le substrat de germanium est comparable aux valeurs trouvees dans la litterature pour la croissance a basse temperature avec les autres procedes d'epitaxie courants. Ces resultats confirment que la technique d'epitaxie par faisceaux chimiques (CBE) permet de produire des couches de GaAs sur Ge de qualite adequate pour la fabrication de cellules solaires a haute performance. L'apport a la communaute scientifique a ete maximise par le biais de la redaction d'un article soumis a la revue Journal of Crystal Growth et la presentation des travaux a la conference Photovoltaics Canada 2010 . Mots-cles : Epitaxie par jets chimiques, Chemical beam epitaxy, CBE, MOMBE, Germanium, GaAs, Ge

  16. Mass, light and colour of the cosmic web in the supercluster SCL2243-0935 (z = 0.447)

    NASA Astrophysics Data System (ADS)

    Schirmer, M.; Hildebrandt, H.; Kuijken, K.; Erben, T.

    2011-08-01

    the filaments. Conclusions: SCL2243 is significantly larger and much more richly structured than other known superclusters such as A901/902 or MS0302 studied with weak lensing before. It is a text-book supercluster with little contamination along the line of sight, making it a perfect sandbox for testing new techniques probing the cosmic web. This work is based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii (programme ID: 2008BO01); based on observations made with ESO Telescopes at the La Silla and Paranal Observatories, Chile (ESO Programmes 165.S-0187 and 079.A-0063); based on observations made with the 2.5 m Isaac Newton Telescope operated on the island of La Palma by the Isaac Newton Group in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias (programme ID 2008B/C11 and 2009B/C1).Appendices are available in electronic form at http://www.aanda.org

  17. Façons d’identifier et de prendre en charge la dyslipidémie athérogène

    PubMed Central

    Bosomworth, N. John

    2013-01-01

    Résumé Objectif Passer en revue les données probantes concernant la reconnaissance et la prise en charge de la dyslipidémie athérogène. Sources des données Des études randomisées et des méta-analyses de grande qualité ont été trouvées pour répondre à la plupart des questions. Les lignes directrices nord-américaines et européennes ont été examinées. Parmi celles-ci, les lignes directrices de la Société canadienne de cardiologie étaient les plus congruentes avec les ouvrages scientifiques récents. Message principal La dyslipidémie athérogène se caractérise par de faibles taux de lipoprotéines de haute densité (HDL), de hauts niveaux de triglycérides et un nombre élevé de particules de lipoprotéines de basse densité (LDL). Ce problème est étroitement associé à des maladies cardiovasculaires (MCV) et il n’est pas bien cerné par les scores de risque de Framingham et les dosages des LDL. L’obésité, l’intolérance au glucose, le diabète et le syndrome métabolique deviennent rapidement de plus en plus fréquents et sont souvent associés avec la dyslipidémie athérogène, ce qui affecte le risque à long terme de MCV. Pour la reconnaître en cabinet, il est préférable de recourir au dosage du cholestérol non HDL ou au ratio du cholestérol total par rapport au HDL. La réussite du traitement repose sur l’optimisation du régime alimentaire et de l’activité physique. Parmi les médicaments disponibles, ce sont les statines qui procurent le plus de bienfaits et elles peuvent être titrées en fonction de la tolérance du patient plutôt que selon les valeurs ciblées de LDL, qui ne sont pas appuyées par de solides données probantes. L’ajout de fénofibrate peut être envisagé chez les patients ayant des niveaux élevés de triglycérides et de bas niveaux de HDL qui n’ont pas répondu de façon satisfaisante aux statines ou ne les ont pas tolérées. Conclusion La prévalence grandissante de l’obésité cr

  18. HD 51844: An Am δ Scuti in a binary showing periastron brightening

    NASA Astrophysics Data System (ADS)

    Hareter, M.; Paparó, M.; Weiss, W.; García Hernández, A.; Borkovits, T.; Lampens, P.; Rainer, M.; De Cat, P.; Marcos-Arenal, P.; Vos, J.; Poretti, E.; Baglin, A.; Michel, E.; Baudin, F.; Catala, C.

    2014-07-01

    intermediate evolutionary phase; the stellar rotation is super-synchronised, but circularisation of the orbit is not reached. Based on observations obtained with the HERMES spectrograph attached to the Mercator Telescope which is operated on the island of La Palma by the University of Leuven (IvS) at the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias. The HERMES spectrograph is supported by the Fund for Scientific Research of Flanders (FWO), Belgium, the Research Council of K.U. Leuven, Belgium, the Fonds National de la Recherche Scientifique (FNRS), Belgium, the Royal Observatory of Belgium, the Observatoire de Genève, Switzerland and the Thüringer Landessternwarte Tautenburg, Germany. Based on CoRoT space-based photometric data; the CoRoT space mission was developed and operated by the French space agency CNES, with the participation of ESA's RSSD and Science Programmes, Austria, Belgium, Brazil, Germany, and Spain. Based on observations collected at La Silla Observatory, ESO (Chile) with the HARPS spectrograph at the 3.6 m telescope, under programme LP185.D-0056.Table 9 is available in electronic form at http://www.aanda.org

  19. The merging cluster Abell 1758 revisited: multi-wavelength observations and numerical simulations

    NASA Astrophysics Data System (ADS)

    Durret, F.; Laganá, T. F.; Haider, M.

    2011-05-01

    simulations, we could mimic the most prominent features present in the metallicity map and propose an explanation for the dynamical history of the cluster. We found in particular that in the metal-rich elongated regions of the North cluster, winds had been more efficient than ram-pressure stripping in transporting metal-enriched gas to the outskirts. Conclusions: We confirm the merging structure of the North and South clusters, both at optical and X-ray wavelengths. Based on archive data retrieved from the Canadian Astronomy Data Centre Megapipe archive and obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. The X-ray analysis is based on XMM-Newton archive data. This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration, and of the SIMBAD database, operated at CDS, Strasbourg, France.

  20. The clusters Abell 222 and Abell 223: a multi-wavelength view

    NASA Astrophysics Data System (ADS)

    Durret, F.; Laganá, T. F.; Adami, C.; Bertin, E.

    2010-07-01

    temperature distribution is very inhomogeneous. Signs of recent interactions are also detected in the optical data where this cluster shows a "perturbed" GLF. In summary, the multiwavelength analyses of Abell 222 and Abell 223 are used to investigate the connection between the ICM and the cluster galaxy properties in an interacting system. Based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. This work has also made use of data products produced at TERAPIX and the Canadian Astronomy Data Centre as part of the Canada-France-Hawaii Telescope Legacy Survey, a collaborative project of NRC and CNRS. The X-ray analysis is based on XMM-Newton archive data. This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.