Realization of ETRF2000 as a New Terrestrial Reference Frame in Republic of Serbia

NASA Astrophysics Data System (ADS)

Blagojevic, D.; Vasilic, V.

2012-12-01

The International Earth Rotation and Reference Systems Service (IERS) is a joint service of the International Association of Geodesy (IAG) and the International Astronomical Union (IAU), which provides the scientific community with the means for computing the transformation from the International Celestial Reference System (ICRS) to the International Terrestrial Reference System (ITRS). It further maintains the realizations of these systems by appropriate coordinate sets called "frames". The densification of terrestrial frame usually serves as official frame for positioning and navigation tasks within the territory of particular country. One of these densifications was recently performed in order to establish new reference frame for Republic of Serbia. The paper describes related activities resulting in ETRF2000 as a new Serbian terrestrial reference frame.

[Anniversaries of the Serbian Medical Society. 60 years since its founding. The dream is fulfilled--the home of the Serbian Medical Society is opened].

PubMed

Vuković, Z

1998-01-01

The Serbian Medical Society was founded in Belgrade in 1872, 126 years ago. At that time, Serbia was liberated from the Ottoman domination, and was one of some thirty existing independent states gaining international recognition in 1878. In 1932 an old dream has been fulfilled--on the occasion of the 60th anniversary of the existence and activity of the Serbian Medical Society--the home of Serbian Medical Society was opened. A 30-year-long period in which the building of the Home was one of the main preoccupations and a "guiding light" of Serbian doctors thus ended. Money from charitable funds was used, which caused certain benefactors to be praised as noted personalities. Medical practice in those days was in the state of choice. There were no means for adequate treatment of certain ailments, and therapy without realistic scientific base was given, often covered by fictitious reasons. This was especially true for tuberculosis and cancer. Under the pretext of the introduction of "new therapeutical approaches" into medical practice and treatment, diverse pharmaceutical formulas were introduced without knowledge of their real effect--injections of milk, drug containing animal embrional cells and special attention was paid to transplantation of the sexual glands. The injection of "camphor oil" (5 cc) was thus "recommended, harmless but useless". The treatment of tuberculosis, which domineered the pathology of population, was very chaotic. The greatest number of drugs for "successful cure" were to be found here. Most commotion was caused by the so-called Friedman's cure for tuberculosis which was rejected only after vigorous debates. Our drug "Joannin" on the basis of "the old tuberculine" was also represented in this confusion (and Koch himself was forced to recant it). This medicament was also hailed as "successful cure". The origin of serious scientific efforts, however, are to be found around newly formed journal "Medicinski pregled", which attracted new and progressive contributors. At this time, the newly formed Ministry of Public Health started a campaign for the introduction of a modern organization of the health care and the inclusion of all population in it. However, in a country devastated by war and stricken by poverity, annomalies in the functioning of the health care existed, as financial preconditions did not exist and healt insurance was still in its infancy. This made the status of doctors difficult, causing long debates in the Serbian Medical Society and fierce criticism of the Ministry of Public Health. The responsible persons were accused of introducing and promoting communist ideas and revolution under the duise of health care for the poipulation.

Application of XML to Journal Table Archiving

NASA Astrophysics Data System (ADS)

Shaya, E. J.; Blackwell, J. H.; Gass, J. E.; Kargatis, V. E.; Schneider, G. L.; Weiland, J. L.; Borne, K. D.; White, R. A.; Cheung, C. Y.

1998-12-01

The Astronomical Data Center (ADC) at the NASA Goddard Space Flight Center is a major archive for machine-readable astronomical data tables. Many ADC tables are derived from published journal articles. Article tables are reformatted to be machine-readable and documentation is crafted to facilitate proper reuse by researchers. The recent switch of journals to web based electronic format has resulted in the generation of large amounts of tabular data that could be captured into machine-readable archive format at fairly low cost. The large data flow of the tables from all major North American astronomical journals (a factor of 100 greater than the present rate at the ADC) necessitates the development of rigorous standards for the exchange of data between researchers, publishers, and the archives. We have selected a suitable markup language that can fully describe the large variety of astronomical information contained in ADC tables. The eXtensible Markup Language XML is a powerful internet-ready documentation format for data. It provides a precise and clear data description language that is both machine- and human-readable. It is rapidly becoming the standard format for business and information transactions on the internet and it is an ideal common metadata exchange format. By labelling, or "marking up", all elements of the information content, documents are created that computers can easily parse. An XML archive can easily and automatically be maintained, ingested into standard databases or custom software, and even totally restructured whenever necessary. Structuring astronomical data into XML format will enable efficient and focused search capabilities via off-the-shelf software. The ADC is investigating XML's expanded hyperlinking power to enhance connectivity within the ADC data/metadata and developing XSL display scripts to enhance display of astronomical data. The ADC XML Definition Type Document can be viewed at http://messier.gsfc.nasa.gov/dtdhtml/DTD-TREE.html

Starry Cities and Astrolies - Books to communicate with the public

NASA Astrophysics Data System (ADS)

Stanic, N.

2008-06-01

Extragalactic worlds have been presented as star cities in a book of original design - STARRY CITIES - galaxies and time travel, the first book about galaxies written in Serbian for the general public. This book isn't written just for those interested in science, but for all kind of artists, philosophers and thinkers. A second book, ASTROLIES deals with common confusions concerning astronomy and astrology. These two books don't only offer interesting illustrations, data from the latest astronomical observations and currently accepted cosmological theories - they induce, by provoking curiosity in a specific and witty way, a sense of adventure and a challenge to explore. The publisher of both books is the oldest and the biggest publisher of text-books in Serbia, Zavod za udzbenike i nastavna sredstva2, currently celebrating 50 years in publishing (1957-2007). They already publish a dozen books in popular astronomy, but a special astronomical series for the general public was introduced in 2004. STARRY CITIES and ASTROLIES are part of the ongoing multidisciplinary project Astronomy. Inspiration. Art that started at the end of 2004 at the Public Observatory in Belgrade. This project intends to inspire (or perhaps even "infect") artists with cosmic themes and the fantastic scenery of the Universe.

[Dr. Jovan Andrejević Jols, the first Serbian anatomist life, work and achievement].

PubMed

Sakač, Dejan; Sakač, Vladimir; Čabarkapa, Velibor; Bugarski, Vojislava

2011-01-01

Doctor Jovan Andrejević Joles was one of the most educated Serbs of the 19th century, a medical doctor, scientist, journalist and translator. He was born in 1883 in Novi Sad. Even as a student of medicine he was active in scientific work, which resulted in a paper entiteled "The fine structure of the liver," later published in one of the most eminent medical journals in Europe. He completed the study of medicine in Vienna. He did not accept the position at the Medical Faculty in Vienna, and returned to Novi Sad, where he quickly gained an excellent reputation as a physician. He participated in the founding of the Serbian National Theatre in 1861, he was also one of the most active contributors of Matica Srpska, wrote many articles, critics and reviews, and was also regarded as the founder of aesthetic romanticism in Serbs. With Laza Kostić, he was the first among the Serbs to translate Shakespeare. At that time, when he was only 30 years old, he wrote about a brand-new art - photography. He lived in a harmonious marriage with Jelena - Ilka Bajić, who after Joles' death remarried to a captain of the Serbian army, and after his murder, became famous for the assassination attempt of King Milan Obrenović (recorded in history textbooks as the "Rebellion of Ilka"). Dr. Jovan Andrejevć died prematurely of tuberculosis, at that time an incurable disease, in 1864 in Novi Sad.

Critical factors for a successful astronomical research program in a developing country

NASA Astrophysics Data System (ADS)

Hearnshaw, John B.

I discuss the critical conditions for undertaking a successful research program in a developing country. There are many important factors, all or most of which have to be satisfied: funding, library holdings, computing access, Internet access (e-mail, WWW, ftp, telnet), collaboration with astronomers in developed countries, provision of proper offices for staff, supply of graduate students, access to travel for conferences, ability to publish in international journals, critical mass of researchers, access to a telescope (for observational astronomers), support from and interaction with national electronics, optics and precision engineering industries, a scientific culture backed by a national scientific academy, and lack of inter-institutional rivalry. I make a list of a total of 15 key factors and rank them in order of importance, and discuss the use of an astronomical research index (ARI) suitable for measuring the research potential of a given country or institution. I also discuss whether astronomers in developing countries in principle fare better in a university or in the environment of a government national observatory or research institution, and topics such as the effect of the cost of page charges and journal subscriptions on developing countries. Finally I present some statistics on astronomy in developing countries and relate the numbers of astronomers to the size of the economy and population in each country.

Astronomical Resources: A Selected Halley's Comet Reading List.

ERIC Educational Resources Information Center

Fraknoi, Andrew

1985-01-01

Presents annotated lists of: (1) general introductory books about comets and Comet Halley; (2) books about comet history and lore; (3) introductory books for younger children; and (4) books for the serious amateur astronomer. A list of magazine and journal articles is included. (JN)

Enhancing AstroInformatics and Science Discovery from Data in Journal Articles

NASA Astrophysics Data System (ADS)

Mazzarella, Joseph

2011-05-01

Traditional methods of publishing scientific data and metadata in journal articles are in need of major upgrades to reach the full potential of astronomical databases and astroinformatics techniques to facilitate semi-automated, and eventually autonomous, methods of science discovery. I will review a growing collaboration involving the NASA/IPAC Extragalactic Database (NED), the Astrophysics Data System (ADS), the Virtual Astronomical Observatory (VAO), the AAS Journals and IOP, and the Data Conservancy that is aimed toward transforming the methodology used to publish, capture and link data associated with astrophysics journal articles. We are planning a web-based workflow to assist astronomers during the publication of journal articles. The primary goals are to facilitate the application of structure and standards to (meta)data, reduce errors, remove ambiguities in the identification of astrophysical objects and regions of sky, capture and preserve the images and spectral data files used to make plots, and accelerate the ingestion of the data into relevant repositories, search engines and integration services. The outcome of this community wide effort will address a recent public policy mandate to publish scientific data in open formats to allow reproducibility of results and to facilitate new discoveries. Equally important, this work has the potential to usher in a new wave of science discovery based on seamless connectivity between data relationships that are continuously growing in size and complexity, and increasingly sophisticated data visualization and analysis applications.

"Radio Astronomy, Whatever That May Be." The Marginalization of Early Radio Astronomy

NASA Astrophysics Data System (ADS)

Jarrell, Richard

2005-01-01

Today we see radio astronomy as a fully-integrated part of astronomy; it is now just one of several available wavelength regimes and many astrophysicists who use radio data are not radio astronomers themselves. At the beginning, it was very different. Between 1946 and 1960, radio astronomy emerged as an important speciality but it was an area little understood by mainstream astronomers. Radio astronomers rarely published in astronomical journals, gave papers at astronomical conferences or were accorded much notice. The pioneers in the field were not astronomers themselves and had little in common with astronomers. In this paper I note the various ways in which radio astronomy was alienated from the mainstream in its first decade and some of the reasons this alienation occurred. I will also speculate on when and how the integration began to occur.

150th Anniversary of the Astronomical Observatory Library of Sciences

NASA Astrophysics Data System (ADS)

Solntseva, T.

The scientific library of the Astronomical observatory of Kyiv Taras Shevchenko University is one of the oldest ones of such a type in Ukraine. Our Astronomical Observatory and its scientific library will celebrate 150th anniversary of their foundation. 900 volumes of duplicates of Olbers' private library underlay our library. These ones were acquired by Russian Academy of Sciences for Poulkovo observatory in 1841 but according to Struve's order were transmitted to Kyiv Saint Volodymyr University. These books are of great value. There are works edited during Copernicus', Kepler's, Galilei's, Newton's, Descartes' lifetime. Our library contains more than 100000 units of storage - monographs, periodical astronomical editions from the first (Astronomische Nachrichten, Astronomical journal, Monthly Notices etc.), editions of the majority of the astronomical observatories and institutions of the world, unique astronomical atlases and maps

The Cardiff Acne Disability Index (CADI): linguistic and cultural validation in Serbian.

PubMed

Jankovic, Slavenka; Vukicevic, Jelica; Djordjevic, Sanja; Jankovic, Janko; Marinkovic, Jelena; Basra, Mohammad K A

2013-02-01

The aims of this study were to translate the Cardiff Acne Disability Index (CADI) into Serbian and to assess its validity and reliability in Serbian acne patients. The CADI was translated and linguistically validated into Serbian according to published guidelines. This version of CADI, along with the Serbian version of Children's Dermatology Life Quality Index (CDLQI) and a short demographic questionnaire, was administrated to a cohort of secondary school pupils. The Global Acne Grading Score was used to measure the clinical severity of acne. The internal consistency reliability of the Serbian version of CADI was assessed by Cronbach's alpha coefficient while its concurrent validity was assessed by Spearman's correlation coefficient. Construct validity was examined by factor analysis. A total of 465 pupils completed questionnaires. Self-reported acne was present in 76% of pupils (353/465). The Serbian version of CADI showed high internal consistency reliability (Cronbach's alpha coefficient = 0.79). The mean item-total correlation coefficient was 0.74 with a range of 0.53-0.81. The concurrent validity of the scale was supported by a moderate but highly significant correlation with the CDLQI (Spearman's rho = 0.66; P < 0.001). Factor analysis revealed the presence of two dimensions underlying the factor structure of the scale. The Serbian version of the CADI is a reliable, valid, and valuable tool for assessing the impact of acne on the quality of life of Serbian-speaking patients.

Astronomical Interlibrary Cooperation: The Long and Difficult Plan for Coordinated Acquisition of Journals -- the Italian Case

NASA Astrophysics Data System (ADS)

Gasperini, A.; Abrami, L.; Olostro Cirella, E.

2007-10-01

Until 2002, the Italian astronomical observatories were independent research institutes. Their libraries, though different in their origins and history, shared common bibliographical materials, users and aims. This situation prompted a first experience of unofficial cooperation between astronomical observatory libraries, which produced outstanding results, in particular a detailed survey of the nature, cost and use of scientific journals. Starting from 2002, when the 12 observatories merged into a single institution, the National Institute for Astrophysics (INAF), the experience of cooperation between the libraries became official. The INAF headquarters, in fact, has recently established the Library Documentary and Archive Service of the National Institute for Astrophysics (SBDA-INAF) in order to have a centralized astronomical bibliographical service and to promote cooperation among libraries. At the end of 2004, following the INAF rearrangement, 5 Institutes of the National Research Council (CNR) joined the still new organization introducing further complications. In this work we explain all the problems faced by a working group to elaborate an efficient plan of coordinated acquisition of journals: the difficulties in coordinating 17 different sites distributed over the whole national territory, the not so easy negotiation with the publishers, the choice between e-only or print & online and, last but not least, the psychological impact on the scientific community. The cooperation among Italian astronomical libraries was a plan begun many years ago and has continued through various events over the years. This presentation takes into consideration the various stages of our project focusing on some crucial aspects.

Studying the history of Indonesian astronomy: future prospects and possibilities

NASA Astrophysics Data System (ADS)

Orchiston, Wayne

2017-08-01

In this paper I identify a number of research topoics relating to Indonesian astronomical history that I feel are of international importance. Through these studies, Indonesia can make a valuable contribution to international history of astronomy. I also will discuss the role of SEAAN's new Working Group on Astronomical History and Heritage, and the values of the Journal of Astronomical History and Heritage and proceedings of the ICOA conferences as outlets for papers about Indonesian astronomical history. Finally, I mention chapters about Indonesia that will appear in a forthcoming book on the early development of astrophysics in Asia.

Representations of Lancet or Phlebotome in Serbian Medieval Art.

PubMed

Pajić, Sanja; Jurišić, Vladimir

2015-01-01

The topic of this study are representations of lancet or phlebotome in frescoes and icons of Serbian medieval art. The very presence of this medical instrument in Serbian medieval art indicates its usage in Serbian medical practices of the time. Phlebotomy is one of the oldest forms of therapy, widely spread in medieval times. It is also mentioned in Serbian medical texts, such as Chilandar Medical CodexNo. 517 and Hodoch code, i.e. translations from Latin texts originating from Salerno-Montpellier school. Lancet or phlebotome is identified based on archaeological finds from the Roman period, while finds from the Middle Ages and especially from Byzantium have been scarce. Analyses of preserved frescoes and icons has shown that, in comparison to other medical instruments, lancet is indeed predominant in Serbian medieval art, and that it makes for over 80% of all the representations, while other instruments have been depicted to a far lesser degree. Examination of written records and art points to the conclusion that Serbian medieval medicine, both in theory and in practice, belonged entirely to European traditions of the period.

Astronomy development in Serbia in view of the IAU Strategic Plan

NASA Astrophysics Data System (ADS)

Atanacković, Olga

2015-03-01

An overview of astronomy development in Serbia in view of the goals envisaged by the IAU Strategic Plan is given. Due attention is paid to the recent reform of education at all levels. In the primary schools several extra topics in astronomy are introduced in the physics course. Attempts are made to reintroduce astronomy as a separate subject in the secondary schools. Special emphasis is put to the role and activities of the Petnica Science Center the biggest center for informal education in SE Europe, and to a successful participation of the Serbian team in International astronomy olympiads. Astronomy topics are taught at all five state universities in Serbia. At the University of Belgrade and Novi Sad students can enroll in astronomy from the first study year. The students have the training at the Ondrejov Observatory (Czech Republic) and at the astronomical station on the mountain Vidojevica in southern Serbia. Astronomy research in Serbia is performed at the Astronomical Observatory, Belgrade and the Department of Astronomy, Faculty of Mathematics, University of Belgrade. There are about 70 researchers in astronomy in Serbia (and about as many abroad) who participate in eight projects financed by the Ministry of Education and Science and in several international cooperations and projects: SREAC, VAMDC, Belissima (recruitment of experienced expatriate researchers), Astromundus (a 2-year joint master program with other four European universities), LSST. One of the goals in near future is twinning between universities in the SEE region and worldwide. The ever-increasing activities of 20 amateur astronomical societies are also given.

Evaluation of a health literacy screening tool in primary care patients: evidence from Serbia.

PubMed

Jović-Vraneš, Aleksandra; Bjegović-Mikanović, Vesna; Marinković, Jelena; Vuković, Dejana

2014-12-01

Improving health literacy skills is important for patient comprehension of health-related topics and their ability to attend to their medical problems. Promoting health literacy is a pivotal policy for maintaining and promoting health. The objective of the present study was to translate the Test of Functional Health Literacy in Adults (TOFHLA; long and short versions) into Serbian and evaluate the translated and cross-culturally adapted questionnaires in Serbian primary care patients. The translated TOFHLA questionnaires were administered to 120 patients. Additionally, a self-completed questionnaire was used. Both descriptive and inferential statistics were measured. The mean score for the TOFHLA was 73.49 (median, 78; SD = 17.94; range, 0-100) and the mean score for the Short Test of Functional Health Literacy in Adults (STOFHLA) was 29.28 (median, 32; SD = 6.16; range, 0-36). Sex, age, education, self-perceived health and presence of any chronic disease were associated with health literacy scores. The internal consistency (Cronbach's alpha) was 0.73 for the TOFHLA numeracy subset, 0.95 for reading comprehension, 0.94 for the TOFHLA and 0.90 for the STOFHLA. The Pearson correlation between the TOFHLA and STOFHLA was 0.89. The area under the curve of these two tests was 0.79 (95% CI, 0.602-0.817). The Serbian translated versions of the TOHFLA questionnaires offer valid measures of functional health literacy. There were no differences between the reliability and validity of the short and long TOFHLA forms. © The Author (2013). Published by Oxford University Press. All rights reserved. For Permissions, please email: journals.permissions@oup.com.

[French astronomical journals an interactivity of the scientific world].

PubMed

Vassilieff, Catherine

2014-01-01

Astronomical data issued from observatories find multiple uses on land, as well as on sea. Due to their structure and periodicity, scientific reviews are particularly adapted to peer review and sharing of data between astronomers as well as between astronomers and hobbyists. During the 19(th) century regional observatories first gather together professionals interested in the practical applications of the observations and later, under the influence of personalities such as Camille Flammarion, they bring together a larger non-professional audience. Being the epicentre of scientific exchange, the reviews have in the 20(th) century found their place on the websites of academic institutions as well as users forums.

Kosovo and U.S. Policy

DTIC Science & Technology

2002-07-03

CRS-8 Serbian Views The FRY and Serbian governments, as well as Kosovo’s Serbs, are strongly opposed to Kosovo’s independence. The democratic ... leadership in Belgrade is not pleased with the loss of effective Serbian control over the province enshrined in UNSC Res. 1244, but nevertheless calls for

The Indicative and Subjunctive "da"-complements in Serbian A Syntactic-Semantic Approach

ERIC Educational Resources Information Center

Todorovic, Natasa

2012-01-01

A syntactic-semantic investigation of subjunctive and indicative "da"-complements in Serbian is conducted in this project. After a careful comparison of Serbian sentence constructions with "da"-complements to the equivalent sentence structures in languages of the Balkans as well as other Slavic languages, it is clearly…

Day of the week effect in paper submission/acceptance/rejection to/in/by peer review journals

NASA Astrophysics Data System (ADS)

Ausloos, Marcel; Nedic, Olgica; Dekanski, Aleksandar

2016-08-01

This paper aims at providing an introduction to the behavior of authors submitting a paper to a scientific journal. Dates of electronic submission of papers to the Journal of the Serbian Chemical Society have been recorded from the 1st January 2013 till the 31st December 2014, thus over 2 years. There is no Monday or Friday effect like in financial markets, but rather a Tuesday-Wednesday effect occurs: papers are more often submitted on Wednesday; however, the relative number of going to be accepted papers is larger if these are submitted on Tuesday. On the other hand, weekend days (Saturday and Sunday) are not the best days to finalize and submit manuscripts. An interpretation based on the type of submitted work ("experimental chemistry") and on the influence of (senior) coauthors is presented. A thermodynamic connection is proposed within an entropy context. A (new) entropic distance is defined in order to measure the "opaqueness" = disorder) of the submission process.

John Twysden and John Palmer: 17th-century Northamptonshire astronomers

NASA Astrophysics Data System (ADS)

Frost, M. A.

2008-01-01

John Twysden (1607-1688) and John Palmer (1612-1679) were two astronomers in the circle of Samuel Foster (circa 1600-1652), the subject of a recent paper in this journal. John Twysden qualified in law and medicine and led a peripatetic life around England and Europe. John Palmer was Rector of Ecton, Northamptonshire and later Archdeacon of Northampton. The two astronomers catalogued observations made from Northamptonshire from the 1640s to the 1670s. In their later years Twysden and Palmer published works on a variety of topics, often astronomical. Palmer engaged in correspondence with Henry Oldenburg, the first secretary of the Royal Society, on topics in astronomy and mathematics.

Proceedings of Colloquium 110 of the International Astronomical Union on Library and Information Services in Astronomy

NASA Astrophysics Data System (ADS)

Wilkins, George A.; Stevens-Rayburn, Sarah

This report provides an overview of the presentations and summaries of discussions at IAU Colloquium 110, which was held in Washington, D.C., on 26-30 July 1988 and at the Goddard Space Flight Center on 1 August 1988. The topics included: the publication and acquisition of books and journals; searching for astronomical information; the handling and use of special-format materials; conservation; archiving of unpublished documents; uses of computers in libraries; astronomical databases and various aspects of the administration of astronomy libraries and services. Particular attention was paid to new developments, but the problems of astronomers and institutions in developing countries were also considered.

Achievement of Serbian Eighth Grade Students in Science

ERIC Educational Resources Information Center

Antonijevic, Radovan

2006-01-01

The paper considers the main results and some educational implications of the TIMSS 2003 assessment conducted in Serbia in the fields of the science achievement of Serbian eighth grade students and the science curriculum context of their achievement. There were 4264 students in the sample. It was confirmed that Serbian eighth graders had made…

Mental health and nutritional status among the adult Serbian minority in Kosovo.

PubMed

Salama, P; Spiegel, P; Van Dyke, M; Phelps, L; Wilkinson, C

2000-08-02

Since the beginning of the North Atlantic Treaty Organization intervention in Kosovo in June 1999, few objective data have been available on relevant health indicators for the Serbian ethnic minority in Kosovo. To determine the prevalence of undernutrition among Serbian adults aged 60 years or older and psychiatric morbidity among the adult Serbian population in Kosovo. A systematic random sample survey of 212 households was conducted between September 27 and October 2, 1999, in Pristina, the capital city, and in 10 towns in the rural municipality of Gnjilane in Kosovo. Of the 212 households surveyed, 204 adults aged 15 years or older completed the General Health Questionnaire-28 (GHQ-28) and anthropometric measurements were taken for 98 adults aged 60 years or older and for a comparison group of 51 adults aged 18 to 59 years. Body mass index of less than 18.5 kg/m(2) in older adults; nonspecific psychiatric morbidity among adults; and self-reported use of health care services, access to food rations, and primary sources of prewar and postwar income. Undernutrition was found in 11.2% (95% confidence interval [CI], 5.7%-19.2%) of Serbian adults aged 60 years or older compared with 2.0% (95% CI, 0.1%-11.8%) of Serbian adults aged 18 to 59 years. The mean (SE) total score for the GHQ-28 was 13.0 (0.52). In a comparison of the GHQ-28 scores of the Serbian adults with the Kosovar Albanian adults (data from a recent survey), the mean (SE) score adjusted for age and sex was 12.8 (0.52) vs 11.1 (0.58); P =.03, respectively. The GHQ-28 scores were also higher for the Serbians in the subcategories of social dysfunction (2.8 [0.17] vs 2.2 [0.13]; P =.008) and severe depression (1.9 [0.15] vs 0.9 [0. 09]; P<.001), respectively. Serbian women and persons living alone or in small family units were more prone to psychiatric morbidity. Of the 141 respondents reporting the need for health care services, 83 (57.6%) reported not obtaining such services; 204 of 212 (96.2%) households were on a food distribution list. The majority of prewar income came from government jobs compared with farming and humanitarian aid for postwar income. The undernutrition of older Serbian adults in Kosovo should be monitored. The high prevalence of symptoms of social dysfunction and severe depression suggest the need for implementation of mental health programs in the Serbian community. JAMA. 2000;284:578-584

Preservation of Chinese Print Astronomical Literature in the Digital and Network Age

NASA Astrophysics Data System (ADS)

Zhang, J.; Shi, W.

2015-04-01

Over the last few decades, more and more journals and books have been published in both electronic and print formats. Some journals have been digitized retrospectively going back to the first volume of more than a hundred years ago, which benefits researchers and librarians tremendously. As a result, many librarians subscribe to books and journals in both electronic and print versions when possible. In many cases, because of budget shortfalls and the low usage of print materials, many libraries have started to order electronic only. This trend heralds a potential demise of print literature as major library resources and has implications for the library services associated with them. This paper proposes some opinions on this issue. We believe that the librarians should pay attention to and conserve the published astronomical literature, a precious historical and cultural heritage, so that we could hand it down to future generations, just like our predecessors did for us.

Psychometric Evaluation of the Serbian Version of the Multidimensional Students' Life Satisfaction Scale

ERIC Educational Resources Information Center

Jovanovic, Veljko; Zuljevic, Dragan

2013-01-01

The main purpose of this study was to evaluate psychometric properties of the Serbian version of the Multidimensional Students' Life Satisfaction Scale (MSLSS). The research was carried out on a sample of 408 high school students (250 females, 158 males), with the mean age 16.6. The Serbian version of the MSLSS has demonstrated good psychometric…

Critical Review of Language Education Policies in Compulsory Primary and Secondary Education in Serbia

ERIC Educational Resources Information Center

Filipovic, Jelena; Vuco, Julijana; Djuric, Ljiljana

2007-01-01

In this paper a comparative analysis of the status of four types of languages present in the Serbian compulsory education system is presented: (1) Serbian as L1; (2) Serbian as L2 (for ethnic minorities); (3) minority languages; as well as (4) traditionally designated "foreign languages", such as English, French, Russian and German,…

The Amateurs' Love Affair with Large Datasets

NASA Astrophysics Data System (ADS)

Price, Aaron; Jacoby, S. H.; Henden, A.

2006-12-01

Amateur astronomers are professionals in other areas. They bring expertise from such varied and technical careers as computer science, mathematics, engineering, and marketing. These skills, coupled with an enthusiasm for astronomy, can be used to help manage the large data sets coming online in the next decade. We will show specific examples where teams of amateurs have been involved in mining large, online data sets and have authored and published their own papers in peer-reviewed astronomical journals. Using the proposed LSST database as an example, we will outline a framework for involving amateurs in data analysis and education with large astronomical surveys.

EDP Sciences and A&A: partnering to providing services to support the scientific community

NASA Astrophysics Data System (ADS)

Henri, Agnes

2015-08-01

Scholarly publishing is no longer about simply producing and packaging articles and sending out to subscribers. To be successful, as well as being global and digital, Publishers and their journals need to be fully engaged with their stakeholders (authors, readers, funders, libraries etc), and constantly developing new products and services to support their needs in the ever-changing environment that we work in.Astronomy & Astrophysics (A&A) is a high quality, major international Journal that belongs to the astronomical communities of a consortium of European and South American countries supported by ESO who sponsor the journal. EDP Sciences is a non-profit publisher belonging to several learned societies and is appointed by ESO to publish the journal.Over the last decade, as well as publishing the results of worldwide astronomical and astrophysical research, A&A and EDP Sciences have worked in partnership to develop a wide range of services for the authors and readers of A&A:- A specialist language editing service: to provide a clear and excellent level of English ensuring full understanding of the high-quality science.- A flexible and progressive Open Access Policy including Gold and Green options and strong links with arXiv.- Enriched articles: authors are able to enhance their articles using a wide range of rich media such as 3D models, videos and animations.Multiple publishing formats: allowing readers to browse articles on multiple devices including eReaders and Kindles.- “Scientific Writing for Young Astronomers”: In 2008 EDP Sciences and A&A set up the Scientific Writing for Young Astronomers (SWYA) School with the objective to teach early PhD Students how write correct and efficient scientific papers for different mediums (journals, proceedings, thesis manuscripts, etc.).

Astronomy and Computing: A new journal for the astronomical computing community

NASA Astrophysics Data System (ADS)

Accomazzi, Alberto; Budavári, Tamás; Fluke, Christopher; Gray, Norman; Mann, Robert G.; O'Mullane, William; Wicenec, Andreas; Wise, Michael

2013-02-01

We introduce Astronomy and Computing, a new journal for the growing population of people working in the domain where astronomy overlaps with computer science and information technology. The journal aims to provide a new communication channel within that community, which is not well served by current journals, and to help secure recognition of its true importance within modern astronomy. In this inaugural editorial, we describe the rationale for creating the journal, outline its scope and ambitions, and seek input from the community in defining in detail how the journal should work towards its high-level goals.

ORCID Uptake in the Astronomical Community

NASA Astrophysics Data System (ADS)

Holmquist, Jane

2015-08-01

The IAU General Assembly provides librarians with a unique opportunity to interact with astronomers from all over the world. From the perspective of an ORCID Ambassador, the Focus Group Meeting on "Scholarly Publication in Astronomy" also provides an opportunity to demonstrate the cooperation and collaboration needed by individual astronomers, societies, librarians, publishers and bibliographic database providers to achieve universal adoption of ORCID, a standard unique identifier for authors, just as the DOI (digital object identifier) has been adopted for each journal article published.I propose to 1) present at the Focus Group Meeting an update on the uptake of ORCID by members of the astronomical community and 2) set up a small station (TBA) near the IAU registration area where librarians can show researchers how to register for an ORCID in 30 seconds.

Catalog of infrared observations. Part 2: Appendixes

NASA Technical Reports Server (NTRS)

Gezari, Daniel Y.; Schmitz, Marion; Mead, Jaylee M.

1987-01-01

The Catalog of Infrared Observations (CIO) is a compilation of infrared astronomical observational data obtained from an extensive literature search of astronomical journals and major astronomical catalogs and surveys. The literature searches are complete for years 1965 to 1986. Supporting appendixes are published in this part. The appendices include an atlas of infrared source positions, two bibliographies of infrared literature upon which the search was based, and, keyed to the main Catalog listings (organized alphabetically by first author, and by date), an atlas of infrared spectral ranges, and IRAS data for the CIO sources. The complete CIO database is available to qualified users in printed microfiche and magnetic tape formats.

Integral field spectroscopy with GEMINI: Extragalactic star cluster in NGC1275

NASA Astrophysics Data System (ADS)

Trancho, Gelys; Miller, Bryan; García-Lorenzo, Begoña; Sánchez, Sebastián F.

2006-01-01

Studies of globular cluster systems play a critical role in our understanding of galaxy formation. Imaging with the Hubble Space Telescope has revealed that young star clusters are formed copiously in galaxy mergers, strengthening theories in which giant elliptical galaxies are formed by the merger of spirals [e.g. Whitmore, B.C., Schweizer, F., Leitherer, C., Borne, K., Robert, C., 1993. Astronomical Journal. 106, 1354; Miller, B.W., Whitmore, B.C., Schweizer, F., Fall, S.M., 1997. Astronomical Journal. 114, 2381; Zepf, S.E., Ashman, K.M., English, J., Freeman, K.C., Sharples, R.M., 1999. Astronomical Journal. 118, 752; Ashman, K.M., Zepf, S.E., 1992. Astrophysical Journal. 384, 50]. However, the formation and evolution of globular cluster systems is still not well understood. Ages and metallicities of the clusters are uncertain either because of degeneracy in the broad-band colors or due to variable reddening. Also, the luminosity function of the young clusters, which depends critically on the metallicities and ages of the clusters, appears to be single power-laws while the luminosity function of old clusters has a well-defined break. Either there is significant dynamical evolution of the cluster systems or metallicity affects the mass function of forming clusters. Spectroscopy of these clusters are needed to improve the metallicity and age measurements and to study the kinematics of young cluster systems. Therefore, we have obtained GMOS IFU data of 4 clusters in NGC1275. We will present preliminary results like metallicities, ages, and velocities of the star clusters from IFU spectroscopy.

Radoslav K. Andjus (1926-2003): a brief summary of his life and work.

PubMed

Stojilkovic, Stanko S; Zivadinović, Dragoslava; Hegedis, Aleksandar; Marjanović, Marina

2005-06-01

Radoslav K. Andjus was a professor of physiology and biophysics at the University of Belgrade, Serbia, from 1953 to 1992. He was an elected member of the Serbian Academy of Sciences and Arts, the International Academy of Astronautics, and the Montenegrin Academy of Sciences and Arts. He published over 190 papers in domestic and international journals and three textbooks. The main field of his research was thermophysiology. He studied hypothermia, suspended animation and resuscitation, hibernation and biological rhythms, temperature adaptation and acclimation, and cryoprotection. Professor Andjus also contributed significantly to the fields of brain metabolism, endocrinology, electroretinography, as well as biophysical modeling and theoretical biology.

Obituary: John Louis Perdrix, 1926-2005

NASA Astrophysics Data System (ADS)

Orchiston, D. Wayne

2006-12-01

John Perdrix, astronomical historian and co-founder of the Journal of Astronomical History and Heritage, died on 27 June 2005. John Louis Perdrix was born in Adelaide, Australia, on 30 June 1926. After studying chemistry at Melbourne Technical College and working in industry, he joined the Commonwealth Scientific and Industrial Research Organisation's Division of Minerals and Geochemistry. In 1974 the Division relocated to the Western Australian capital, Perth, and John spent the rest of his working life there involved in geochemical research. From his teenage years John had a passion for astronomy, which he fine-tuned through the Astronomical Society of Victoria and the Victorian Branch of the British Astronomical Association. He was very active in both groups, serving as President of the former and Secretary/Treasurer of the latter. He was also an FRAS, and a member of the AAS, the BAA parent body, and the IAU (Commission 41)?no mean feat for an Australian amateur astronomer. Throughout his life, he was a strong advocate of close amateur-professional relations. John's main research interest was history of astronomy, and over the years he wrote a succession of research papers, mainly about aspects of Australian astronomy. His well-researched and neatly-illustrated papers on the Melbourne Observatory and the Great Melbourne Telescope are classics, and when the Observatory's future was in the balance they played a key role in the State Government's decision to convert this unique facility into a museum precinct. To support his research activities, John built up an amazing library that developed its own distinctive personality and quickly took over his house and garage before invading commercial storage facilities! Apart from writing papers, John had an even greater passion for editing and publishing. From 1985 to 1997 he produced the Australian Journal of Astronomy, and in 1998 this was replaced by the Journal of Astronomical History and Heritage (JAH2). Both journals appeared under the banner of his own publishing house, Astral Press, until 2005 when JAH2 was transferred to the Centre of Astronomy at James Cook University. When cancer was first diagnosed, this did not deter John, and he continued to pursue his astronomical and editorial interests. Early in 2005 the cancer was in remission and John decided to make one final overseas trip, a long-anticipated visit to St. Petersburg. It was while he was returning to Australia that the illness aggressively reappeared, and he was taken off the airplane at Dubai and died peacefully in Rashid Hospital three days later. He was just three days short of his seventy-ninth birthday. Always the consummate gentleman, John Perdrix had a keen sense of humor and was wonderful company. He will be greatly missed by all who knew him. Our condolences go to his six children, Louise, John, Timothy, Fleur, Lisa and Angella.

Cultural Astronomy in the Armenian Highland

NASA Astrophysics Data System (ADS)

Farmanyan, S. V.; Suvaryan, Yu. M.; Mickaelian, A. M. (Eds.)

2016-12-01

The book contains 29 articles of the Proceedings of the Young Scientists Conference "Cultural Astronomy in the Armenian Highland" held at the Armenian National Academy of Sciences on 20-23 June 2016. It consists of 4 main sections: "Introductory", "Cultural Astronomy", "Archaeoastronomy", "Scientific Tourism and Journalism, Astronomical Education and Amateur Astronomy". The book may be interesting to astronomers, culturologists, philologists, linguists, historians, archaeologists, art historians, ethnographers and to other specialists, as well as to students.

Reports on crustal movements and deformations

NASA Technical Reports Server (NTRS)

Cohen, S. C.; Peck, T.

1981-01-01

Studies of tectonic plate motions, regional crustal deformations, strain accumulation and release, deformations associated with earthquakes and fault motion, and micro-plate motion, were collected and are summarized. To a limited extent, papers dealing with global models of current plate motions and crustal stress are included. The data base is restricted to articles appearing in reveiwed technical journals during the years 1970-1980. The major journals searched include: Journal of Geophysical Research (solid earth), Tectonophysics, Bulletin of the Seismological Society of America, Geological Society of America Bulletin, Geophysical Journal of the Royal Astronomical Society, and the Journal of Geology.

The Challenge of On-Line Journals in Astrophysics

NASA Astrophysics Data System (ADS)

Boyce, Peter

1996-03-01

The American Astronomical Society (AAS) now has considerable experience with publishing an electronic, peer-reviewed journal. Every part of every article of the Letters section of the Astrophysical Journal since July 1, 1995, is freely available on the World Wide Web at http://www.aas.org/ApJ/. It is posted one month ahead of the issue date. Hypertext links to the Astrophysics Data System provide immediate access to the abstracts (and often to bitmaps of the full text) of many of the referenced papers. Innovative navigational tools for the reader, such as forward references, inclusion of all the math and figures and local printout of individual papers, set this journal apart from other electronic publishing efforts. Over the last three years, we have given considerable thought to using the new network connectivity and tools to foster scientific communication. Three considerations have guided our thinking. First, we have expanded our approach to encompass a broad view; electronic publishing means different things to different people. Second, we must not lose what we have. The conventional journals serve several different and important purposes which a new system should continue to fulfill. Third, we must recognize that we are in an era of unprecedented change in the methods of communication and adapt to the new opportunities. The AAS has adopted four operating principles. 1: Maintain quality. Avoid putting material of poor quality and indeterminate reliability on the Internet. 2: Treat our electronic information dissemination efforts in an experimental way. Take small steps. Get feedback from the users. Adopt what works. 3: Plan from a broad base. Include scientists, librarians, publishers and network experts in the planning process. 4: Plan for progress and change. Be flexible. Use a modular approach. Adhere to open standards which make it possible to incorporate new tools as they are developed. Avoid proprietary systems unless they are de-facto standards. Future plans call for the entire Astrophysical Journal to be available in October, 1996, with the Astronomical Journal to follow within a year after that. At that point half the world's astronomical literature will be available in one searchable electronic database.

Astronomy research via the Internet

NASA Astrophysics Data System (ADS)

Ratnatunga, Kavan U.

Small developing countries may not have a dark site with good seeing for an astronomical observatory or be able to afford the financial commitment to set up and support such a facility. Much of astronomical research today is however done with remote observations, such as from telescopes in space, or obtained by service observing at large facilities on the ground. Cutting-edge astronomical research can now be done with low-cost computers, with a good Internet connection to get on-line access to astronomical observations, journals and most recent preprints. E-mail allows fast easy collaboration between research scientitists around the world. An international program with some short-term collaborative visits, could mine data and publish results from available astronomical observations for a fraction of the investment and cost of running even a small local observatory. Students who have been trained in the use of computers and software by such a program would also be more employable in the current job market. The Internet can reach you wherever you like to be and give you direct access to whatever you need for astronomical research.

Northern Slavs from Serbia do not show a founder effect at autosomal and Y-chromosomal STRs and retain their paternal genetic heritage.

PubMed

Rębała, Krzysztof; Veselinović, Igor; Siváková, Daniela; Patskun, Erika; Kravchenko, Sergey; Szczerkowska, Zofia

2014-01-01

Studies on Y-chromosomal markers revealed significant genetic differentiation between Southern and Northern (Western and Eastern) Slavic populations. The northern Serbian region of Vojvodina is inhabited by Southern Slavic Serbian majority and, inter alia, Western Slavic (Slovak) and Eastern Slavic (Ruthenian) minorities. In the study, 15 autosomal STR markers were analysed in unrelated Slovaks, Ruthenians and Serbs from northern Serbia and western Slovakia. Additionally, Slovak males from Serbia were genotyped for 17 Y-chromosomal STR loci. The results were compared to data available for other Slavic populations. Genetic distances for autosomal markers revealed homogeneity between Serbs from northern Serbia and Slovaks from western Slovakia and distinctiveness of Serbian Slovaks and Ruthenians. Y-STR variation showed a clear genetic departure of the Slovaks and Ruthenians inhabiting Vojvodina from their Serbian neighbours and genetic similarity to the Northern Slavic populations of Slovakia and Ukraine. Admixture estimates revealed negligible Serbian paternal ancestry in both Northern Slavic minorities of Vojvodina, providing evidence for their genetic isolation from the Serbian majority population. No reduction of genetic diversity at autosomal and Y-chromosomal markers was found, excluding genetic drift as a reason for differences observed at autosomal STRs. Analysis of molecular variance detected significant population stratification of autosomal and Y-chromosomal microsatellites in the three Slavic populations of northern Serbia, indicating necessity for separate databases used for estimations of frequencies of autosomal and Y-chromosomal STR profiles in forensic casework. Our results demonstrate that regarding Y-STR haplotypes, Serbian Slovaks and Ruthenians fit in the Eastern European metapopulation defined in the Y chromosome haplotype reference database. Copyright © 2013 Elsevier Ireland Ltd. All rights reserved.

Kosovo Crisis: National Security and International Military Intervention

DTIC Science & Technology

2010-03-01

Metohija is an integral part of Serbian geography, history and culture. It was part of the Eastern Orthodox Christian Serbian medieval kingdoms in the...12th – 14th Centuries A.D. It is dotted by a number of medieval Serbian Orthodox Christian monasteries that trace their lineage to those ages. For...Kosovo Polje – the Field of Blackbirds (close to modern day Pristina) – is the historic battlefield where a united force of Orthodox Christian Serbs

Establishment and advances in the online Serbian food and recipe data base harmonized with EuroFIR™ standards.

PubMed

Gurinović, Mirjana; Milešević, Jelena; Kadvan, Agnes; Djekić-Ivanković, Marija; Debeljak-Martačić, Jasmina; Takić, Marija; Nikolić, Marina; Ranković, Slavica; Finglas, Paul; Glibetić, Maria

2016-02-15

Within the European Food Information Resource Network of Excellence (EuroFIR NoE; FP6) and EuroFIR Nexus (FP7) project paucity in food composition databases (FCDB) in the Central Eastern Europe/Balkan (CEE/B) region was identified. As a member of EuroFIR NoE, the Centre of Research Excellence in Nutrition and Metabolism, Serbia initiated creation of the 1st online Serbian FCDB employing EuroFIR quality framework and CEN Food Data Standard requirements, supporting capacity development and designing the web-based Food Composition Data Management (FCDM) software for FCDB building. The 1st online version of Serbian FCDB was launched in 2007, and then extended with food composition data from other Balkan countries (Balkan Food Platform-Regional FCDB). All foods are indexed using LanguaL Thesaurus and coded with EFSA FoodEx2 coding system. To date, upgraded Serbian FCDB with 1046 foods and 129 traditional/common Serbian composite dishes is a prerequisite for nutritional research in Serbia, CEE/B region and wider Europe. Copyright © 2015 Elsevier Ltd. All rights reserved.

Validation of the Neurological Disorders Depression Inventory for Epilepsy (NDDI-E) Serbian version.

PubMed

Ristić, Aleksandar J; Pjevalica, Jelena; Trajković, Goran; Parojčić, Aleksandra; Mihajlović, Ana; Vojvodić, Nikola; Baščarević, Vladimir; Popović, Tamara; Janković, Slavko; Sokić, Dragoslav

2016-04-01

The Neurological Disorders Depression Inventory for Epilepsy (NDDI-E) was developed and proven efficient for the rapid detection of a major depressive episode in people with epilepsy. This study describes the development, validation, and psychometric properties of the NDDI-E Serbian version. A consecutive sample of 103 patients with epilepsy was assessed using the Beck Depression Inventory (BDI) and the NDDI-E. All patients had no major difficulties in understanding or answering the questions of the Serbian version. Cronbach's alpha coefficient was 0.763. Receiver operating characteristic analysis showed an area under the curve of 0.943 (95% CI; 0.826 to 0.951), a cutoff score of ≥14, a sensitivity of 72.2%, a specificity of 95.2%, a positive predictive value of 81.3%, and a negative predictive value of 94.3%. The NDDI-E Serbian version scores were significantly and positively correlated with those of the BDI (p<0.001). The NDDI-E Serbian version constitutes a concise and consistent depression screening instrument for patients with epilepsy. Copyright © 2016 Elsevier Inc. All rights reserved.

Inspiration Today: Music, Astronomy, and Popular Culture

NASA Astrophysics Data System (ADS)

Fraknoi, A.

2016-01-01

We explore a variety of examples of music inspired by serious astronomy (as opposed to simply an astronomical title or quick allusion to spooning in June to the light of the Moon). The examples are drawn from my recently published catalog of 133 such pieces, including both classical and popular genres of music. We discuss operas based on the life and work of astronomers, six songs based on a reasonable understanding of the properties of black holes, constellation pieces written by composers from around the world who are or were active amateur astronomers, the song that compares walking on the Moon to being in love, the little-known rock song that became a reference in the Astrophysical Journal, pieces that base the patterns of the music on the rhythms of astronomical phenomena, and a number of others.

How Documentalists Update SIMBAD

NASA Astrophysics Data System (ADS)

Buga, M.; Bot, C.; Brouty, M.; Bruneau, C.; Brunet, C.; Cambresy, L.; Eisele, A.; Genova, F.; Lesteven, S.; Loup, C.; Neuville, M.; Oberto, A.; Ochsenbein, F.; Perret, E.; Siebert, A.; Son, E.; Vannier, P.; Vollmer, B.; Vonflie, P.; Wenger, M.; Woelfel, F.

2015-04-01

The Strasbourg astronomical Data Center (CDS) was created in 1972 and has had a major role in astronomy for more than forty years. CDS develops a service called SIMBAD that provides basic data, cross-identifications, bibliography, and measurements for astronomical objects outside the solar system. It brings to the scientific community an added value to content which is updated daily by a team of documentalists working together in close collaboration with astronomers and IT specialists. We explain how the CDS staff updates SIMBAD with object citations in the main astronomical journals, as well as with astronomical data and measurements. We also explain how the identification is made between the objects found in the literature and those already existing in SIMBAD. We show the steps followed by the documentalist team to update the database using different tools developed at CDS, like the sky visualizer Aladin, and the large catalogues and survey database VizieR. As a direct result of this teamwork, SIMBAD integrates almost 10.000 bibliographic references per year. The service receives more than 400.000 queries per day.

Relation of Astronomy to other Sciences, Culture and Society

NASA Astrophysics Data System (ADS)

Harutyunian, H. A.; Mickaelian, A. M.; Farmanyan, S. V.

2015-07-01

The book contains the Proceedings of XIII Annual Meeting of the Armenian Astronomical Society "Relation of Astronomy to other Sciences, Culture and Society". It consists of 9 main sections: "Introductory", "Astronomy and Philosophy", "Astrobiology", "Space-Earth Connections", "Astrostatistics and Astroinformatics", "Astronomy and Culture, Astrolinguistics", "Archaeoastronomy", "Scientific Tourism and Scientific Journalism", and "Armenian Astronomy". The book may be interesting to astronomers, philosophers, biologists, culturologists, linguists, historians, archaeologists and to other specialists, as well as to students.

Bibliographical index of objects observed by IUE

NASA Technical Reports Server (NTRS)

Mead, J. M.; Boggess, A.

1982-01-01

Six astronomical journals were searched and 343 papers describing studies using data obtained with the International Ultraviolet Explorer satellite were identified. From a review of these papers, the names of the astronomical objects discussed were recorded and compiled into a list of 2460 entries, along with each reference, and sorted by object name or catalogue number. This index enables a user to tell immediately where to find published papers describing IUE observation of the objects of interest to him.

Catalog of infrared observations

NASA Technical Reports Server (NTRS)

Gezari, D. Y.; Schmitz, M.; Mead, J. M.

1982-01-01

The infrared astronomical data base and its principal data product, the catalog of Infrared Observations (CIO), comprise a machine readable library of infrared (1 microns to 1000 microns astronomical observations. To date, over 1300 journal articles and 10 major survey catalogs are included in this data base, which contains about 55,000 individual observations of about 10,000 different infrared sources. Of these, some 8,000 sources are identifiable with visible objects, and about 2,000 do not have known visible counterparts.

Building Up a Strategy for De-Balkanizing the Balkans: Stability and Prosperity in South Eastern Europe

DTIC Science & Technology

2002-12-01

Serbian Orthodox church . As a model for fevering nationalist passions served the Serbian medieval Empire of Stephen Dusan. Serbian national sentiment...prominent” was the one at the end of the Great War when, as Austro-Hungary disintegrated in 1918 , Romania being in the Allies’ side entered her armies in...West. This Schism became definitive in 1054 dividing the Christian world into the Roman Catholic and the Greek Orthodox churches . 103 From the

Tidal Dissipation in a Homogeneous Spherical Body. 2. Three Examples: Mercury, IO, and Kepler-10 b

DTIC Science & Technology

2014-11-01

The Astrophysical Journal, 795:7 (10pp), 2014 November 1 doi:10.1088/0004-637X/795/1/7 C© 2014. The American Astronomical Society. All rights...public release; distribution unlimited 13. SUPPLEMENTARY NOTES The Astrophysical Journal, 795:7 (10pp), 2014 November 1 14. ABSTRACT 15. SUBJECT... Astrophysical Journal, 795:7 (10pp), 2014 November 1 Makarov & Efroimsky a, e, i, ω, Ω, M, which are the semimajor axis, eccentricity, inclination

Nikola Tesla: the Moon's rotation.

NASA Astrophysics Data System (ADS)

Tomić, A.; Jovanović, B. S.

1993-09-01

The review of three articles by N. Tesla, published in the year 1919 in the journal "Electrical experimenter" is given, with special reference to the astronomical contents and to circumstances in which they appeared.

Variable Star and Exoplanet Section of the Czech Astronomical Society

NASA Astrophysics Data System (ADS)

Brát, L.; Zejda, M.

2010-12-01

We present activities of Czech variable star observers organized in the Variable Star and Exoplanet Section of the Czech Astronomical Society. We work in four observing projects: B.R.N.O. - eclipsing binaries, MEDUZA - intrinsic variable stars, TRESCA - transiting exoplanets and candidates, HERO - objects of high energy astrophysics. Detailed information together with O-C gate (database of eclipsing binaries minima timings) and OEJV (Open European Journal on Variable stars) are available on our internet portal http://var.astro.cz.

Integrating high school and college students into the astronomy research community of practice through participation in a hybrid research seminar.

NASA Astrophysics Data System (ADS)

Freed, R.

2016-12-01

The Institute for Student Astronomical Research over the past two years has provided dozens of high school and college students the opportunity to conduct original research in astronomy and to publish their work in peer-reviewed journals. Students are engaged in the entire scientific process from coming up with a research question to collecting and analyzing the data and writing up their results for publication. During the process students work with amateur and/or professional astronomers to learn how to conduct their research and communicate their findings effectively. Working within a community of practice has been shown to improve student learning and the Institute for Student Astronomical Research provides a framework in which to bring students and astronomers together while allowing for the work to be done in a student-centered fashion.

Forty-two years of Revista Mexicana de Astronomía y Astrofísica: Some history and musings on the future

NASA Astrophysics Data System (ADS)

Allen, C.; Torres-Peimbert, S.

2017-07-01

After 42 years of continuously publishing the Revista Mexicana de Astronomía y Astrofísica, we cast a short retrospective view on its history and we share our plans for the future. RMxAA was founded in 1974. Founding editors were P. Pishmish, E. Mendoza and S. Torres-Peimbert. RMxAA has published original research papers in all areas of astronomy, astrophysics and related fields. Until 1994 RMxAA also published the proceedings of astronomical conferences held in México and Latin America. Since 1995 a Series devoted exclusively to such proceedings was founded, RMxAC, Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias). All papers submitted to RMxAA are sent to internationally recognized experts to be strictly refereed. RMxAA is included in Current Contents, Science Citation Index and other relevant international indexes. Both publications are fully integrated into the ADS. Their contents have always been freely available to the general public. All this ensures a wide international visibility, comparable to that of the best astronomical journals. The impact factor of RMxAA has varied over the years, mostly as a consequence of small number statistics. The average impact factor is about 2.4, far larger than that of all but a few Latin American scientific journals. The editorial independence of RMxAA, the fact that there are no page charges for authors, and that the printed version is distributed free of charge to astronomical libraries all over the world motivate us to look forward with optimism to many more years of publication. In view of recent developments in the scientific publishing field, we have applied to obtain the DOI for the published papers, and are in the process of becoming an all-electronic publication.

Essential and toxic elements in commercial baby food on the Spanish and Serbian market.

PubMed

Škrbić, Biljana; Živančev, Jelena; Jovanović, Grigorije; Farre, Marinella

2017-03-01

About 10 heavy elements were determined in 90 samples of baby food collected from Spanish and Serbian market. The results indicated that iron, manganese and copper were most frequently detected. Tin was the predominant toxic element in both Spanish and Serbian samples, with occurrence frequencies of 12.5% and 10.0%, respectively. Element intake for Spanish and Serbian infants were estimated and compared with the recommended reference values, for the majority of elements being lower than one. However, iron and manganese intake through consumption of infant/follow-on formulas were assessed to be higher than the respective daily intakes. Particular attention should be paid to the exposure of infants who consume porridges made of vegetables and fish or chicken, because they may ingest certain elements, particularly arsenic and lead, at levels that exceed the reference toxicological values. Principal component analysis (PCA) was applied to classify and distinguish the different types of baby food.

The effects of articulatory suppression on word recognition in Serbian.

PubMed

Tenjović, Lazar; Lalović, Dejan

2005-11-01

The relatedness of phonological coding to the articulatory mechanisms in visual word recognition vary in different writing systems. While articulatory suppression (i.e., continuous verbalising during a visual word processing task) has a detrimental effect on the processing of Japanese words printed in regular syllabic Khana script, it has no such effect on the processing of irregular alphabetic English words. Besner (1990) proposed an experiment in the Serbian language, written in Cyrillic and Roman regular but alphabetic scripts, to disentangle the importance of script regularity vs. the syllabic-alphabetic dimension for the effects observed. Articulatory suppression had an equally detrimental effect in a lexical decision task for both alphabetically regular and distorted (by a mixture of the two alphabets) Serbian words, but comparisons of articulatory suppression effect size obtained in Serbian to those obtained in English and Japanese suggest "alphabeticity-syllabicity" to be the more critical dimension in determining the relatedness of phonological coding and articulatory activity.

[90 years since the first congress of Serbian physicians].

PubMed

Atanacković, D

1995-01-01

The first congress of the south Slav physicians was held in Belgrade in 1904 and was entitled the First Congress of the Serbian Physicians and Naturalists under the presidency of Dr. Jovan Danić, the president of the Medical Society of Serbia. The Congress was attended by 433 active participants, and the work was organized in sessions: medico-pharmaceutical, physico-chemical and mathematical, biological and abiological, veterino-agronomical. Papers were printed in extenso in the proceedings and were published in the native language of the lectureres (Serbian, Croatian, Bohemian, Slovenian and Bulgarian). Out of these papers 56 were presented in the medico-pharmaceutical session. The Congress was appraised very successful by the attenders and its honorary president, Prof. Dr. Jaroslav Hlava from Prague who concluded at the end of the Congress ".. the First Serbian Congress has prepared material for the future faculty of medicine".

The AAS Working Group on Accessibility and Disability (WGAD) Year 1 Highlights and Database Access

NASA Astrophysics Data System (ADS)

Knierman, Karen A.; Diaz Merced, Wanda; Aarnio, Alicia; Garcia, Beatriz; Monkiewicz, Jacqueline A.; Murphy, Nicholas Arnold

2017-06-01

The AAS Working Group on Accessibility and Disability (WGAD) was formed in January of 2016 with the express purpose of seeking equity of opportunity and building inclusive practices for disabled astronomers at all educational and career stages. In this presentation, we will provide a summary of current activities, focusing on developing best practices for accessibility with respect to astronomical databases, publications, and meetings. Due to the reliance of space sciences on databases, it is important to have user centered design systems for data retrieval. The cognitive overload that may be experienced by users of current databases may be mitigated by use of multi-modal interfaces such as xSonify. Such interfaces would be in parallel or outside the original database and would not require additional software efforts from the original database. WGAD is partnering with the IAU Commission C1 WG Astronomy for Equity and Inclusion to develop such accessibility tools for databases and methods for user testing. To collect data on astronomical conference and meeting accessibility considerations, WGAD solicited feedback from January AAS attendees via a web form. These data, together with upcoming input from the community and analysis of accessibility documents of similar conferences, will be used to create a meeting accessibility document. Additionally, we will update the progress of journal access guidelines and our social media presence via Twitter. We recommend that astronomical journals form committees to evaluate the accessibility of their publications by performing user-centered usability studies.

An Update on the Journal Astronomy Education Review and Why Your Work Isn't Done Until You Have Published

NASA Astrophysics Data System (ADS)

Wolff, S.; Fraknoi, A.; Hockey, T.; Biemesderfer, C.; Johnson, J.

2010-08-01

Astronomy Education Review (AER) is an online journal and magazine, covering astronomy and space science education and outreach. Founded in 2001 by Andrew Fraknoi and Sidney Wolff, and published until recently by National Optical Astronomy Observatories (NOAO), the journal is now a proud part of the journals operation of the American Astronomical Society (AAS) found online at http://aer.aip.org. If you are presenting at this conference, or reading the conference proceedings, you may be an ideal candidate to publish in AER. Later in this paper, we present some encouraging hints and guidelines for publishing in the journal.

Development and Operation of the Astrophysics Data System

NASA Technical Reports Server (NTRS)

Murray, Stephen S.

1997-01-01

The Astrophysics Data System (ADS) provides access to astronomical bibliographic information, including references, abstracts, and full journal articles, as well as links to other on-line information sources like on-line electronic journals and on-line data. This section will first provide a brief history of the ADS, a general introduction of the current system, and a more detailed description of some of the parts of the ADS.

The Contribution of the Division of Radiophysics Murraybank Field Station to International Radio Astronomy

NASA Astrophysics Data System (ADS)

Wendt, Harry; Orchiston, Wayne; Slee, Bruce

During the 1950s Australia was one of the world's foremost astronomical nations owing primarily to the work of the dynamic radio astronomy group within the Commonwealth Scientific and Industrial Research Organisation's Division of Radiophysics. Most of the observations were made at the network of field stations maintained by the Division in or near Sydney, and one of these field stations was Murraybank in the north-western suburbs of Sydney. GVaucouleursDe1954The Magellanic Clouds and the GalaxyThe Observatory7423311954Obs....74...23DDe Vaucouleurs, G., 1954a. The Magellanic Clouds and the Galaxy. The Observatory, 74, 23-31. GVaucouleursDe1954The Magellanic Clouds and the Galaxy, IIThe Observatory741581641954Obs....74..158DDe Vaucouleurs, G., 1954b. The Magellanic Clouds and the Galaxy, II. The Observatory, 74, 158-164. GVaucouleursDe1961Classification and radial velocities of bright southern galaxiesMemoirs of the Royal Astronomical Society6869871961MmRAS..68...69DDe Vaucouleurs, G., 1961. Classification and radial velocities of bright southern galaxies. Memoirs of the Royal Astronomical Society, 68, 69-87. JDeane2006Vacuum Tube SupercomputerSydneyScience Foundation for Physics and the Australian Computer Museum SocietyDeane, J., 2006. Vacuum Tube Supercomputer. Sydney, Science Foundation for Physics and the Australian Computer Museum Society. NHDeiter1965Neutral hydrogen near the galactic polesAstErickson, W.C., Helfer, H.L., and Tatel, H.E., 1959. A survey of neutral hydrogen at high galactic latitudes. In Bracewell, 390-397. MWFeastADThackerayAJWesselink1957Radial velocities of southern B stars determined at the Radcliffe Observatory (Paper II) (summary)Monthly Notices of the Royal Astronomical Society1175791957MNRAS.117..579FFeast, M.W., Thackeray, A.D., and Wesselink, A.J., 1957. Radial velocities of southern B stars determined at the Radcliffe Observatory (Paper II) (summary). Monthly Notices of the Royal Astronomical Society, 117, 579. KCFreeman1970On the disks of spiral and SO galaxiesAstrophysical Journal1608118301970ApJ...160..811F10.1086/150474Freeman, K.C., 1970. On the disks of spiral and SO galaxies. Astrophysical Journal, 160, 811-830. Getmanzev, G.G., Tankevitch, K.S., and Troitzky, V.S., 1957. Detection of the spectral line of deuterium from the centre of the Galaxy on the wave-length of 91.6 cm. In van de Hulst, 90-91. HCGoldwireMGoss1967Microwave radiation of singly charged helium 3 from HII regionsAstrophysical Journal14915221967ApJ...149...15G10.1086/149225Goldwire, H.C., and Goss, M., 1967. Microwave radiation of singly charged helium 3 from HII regions. Astrophysical Journal, 149, 15-22. JLGreenstein1937The effect of absorbing clouds on the general absorption coefficientAnnals of the Astronomical Observatory of Harvard College105359369Greenstein, J.L., 1937. The effect of absorbing clouds on the general absorption coefficient. Annals of the Astronomical Observatory of Harvard College, 105, 359-369. CSGum1956The extent and excitation of the large H II region in Vela-PuppisThe Observatory761501531956Obs....76..150GGum, C.S., 1956. The extent and excitation of the large H II region in Vela-Puppis. The Observatory, 76, 150-153. KGHenize1956Catalogues of Hα-emission stars and nebulae in the Magellanic CloudsAstrophysical Journal Supplement23153441956ApJS....2..315H10.1086/190025Henize, K.G., 1956. Catalogues of Hα-emission stars and nebulae in the Magellanic Clouds. Astrophysical Journal Supplement, 2, 315-344. JVHindman1967A high resolution study of the distribution and motions of neutral hydrogen in the Small Cloud of MagellanAustralian Journal of Physics201471711967AuJPh..20..147H10.1071/PH670147Hindman, J.V., 1967. A high resolution study of the distribution and motions of neutral hydrogen in the Small Cloud of Magellan. Australian Journal of Physics, 20, 147-171. Hindman, J.V., Kerr, F.J., and McGee, R.X., 1963a. A low resolution hydrogen-line survey of the Magellanic system. II. Interpretation of results. Australian Journal of Physics, 16, 570-583. Hindman, J.V., McGee, R.X., Carter, A.W.L., Holmes, E.C.J., and Beard, M., 1963b. A low resolution hydrogen-line survey of the Magellanic system. I. Observations and digital reduction procedures. Australian Journal of Physics, 16, 552-569. Hodge, P.W., 1960. Studies of the Large Magellanic Cloud. I. The red globular clusters. Astrophysical Journal, 131, 351-357. Hodge, P.W., 1961. Studies of the Large Magellanic Cloud. V. The young populous clusters. Astrophysical Journal, 133, 413-419. WEHowardDGWentzelRXMcGee1963On a correlation between the radial velocities of optical and radio interstellar linesAstrophysical Journal13898810011963ApJ...138..988H10.1086/147700Howard, W.E., Wentzel, D.G., and McGee, R.X., 1963. On a correlation between the radial velocities of optical and radio interstellar lines. Astrophysical Journal, 138, 988-1001. HMJohnson1961The structure of the Small Magellanic CloudProceedings of the Astronomical Society of the Pacific7320281961PASP...73...20J10.1086/127613Johnson, H.M., 1961. The structure of the Small Magellanic Cloud. Proceedings of the Astronomical Society of the Pacific, 73, 20-28. KIKellermanWOrchistonBSlee2005Gordon James Stanley and the early development of radio astronomy in Australia and the United StatesPublications of the Astronomical Society of Australia2213232005PASA...22...13K10.1071/AS04008Kellerman, K.I., Orchiston, W., and Slee, B., 2005. Gordon James Stanley and the early development of radio astronomy in Australia and the United States. Publications of the Astronomical Society of Australia, 22, 13-23. Kerr, F.J., 1953. Minutes of the Hydrogen-Line Planning Committee Meeting dated 12 November. National Archives of Australia, Sydney, 972420 - C3830 - A1/3/17 Part 1. Kerr, F.J., 1954. Minutes of the Hydrogen Line Planning Committee Meeting dated 9 June. National Archives of Australia, Sydney, 972420 - C3830 - A1/3/17 Part 2. FJKerr1962Galactic velocity models and the interpretation of 21-cm surveysMonthly Notices of the Royal Astronomical Society1233273451962MNRAS.123..327KKerr, F.J., 1962. Galactic velocity models and the interpretation of 21-cm surveys. Monthly Notices of the Royal Astronomical Society, 123, 327-345. FJKerrJVHindmanBJRobinson1954Observations of the 21 cm line from the Magellanic CloudsAustralian Journal of Physics72973141954AuJPh...7..297K10.1071/PH540297Kerr, F.J., Hindman, J.V., and Robinson, B J., 1954. Observations of the 21 cm line from the Magellanic Clouds. Australian Journal of Physics, 7, 297-314. JVKuilenburg1972A systematic search for high-velocity hydrogen outside the Galactic Plane IIAstronomy and Astrophysics162761972A&A....16..276VKuilenburg, J.V., 1972. A systematic search for high-velocity hydrogen outside the Galactic Plane II. Astronomy and Astrophysics, 16, 276. KKKweeCAMullerGWesterhout1954The rotation of the inner parts of the galactic systemBulletin of the Astronomical Institutes of the Netherlands122112221954BAN....12..211KKwee, K.K., Muller, C.A., and Westerhout, G., 1954. The rotation of the inner parts of the galactic system. Bulletin of the Astronomical Institutes of the Netherlands, 12, 211-222. EMLindsay1958The cluster system of the Small Magellanic CloudMonthly Notices of the Royal Astronomical Society1181721821958MNRAS.118..172LLindsay, E.M., 1958. The cluster system of the Small Magellanic Cloud. Monthly Notices of the Royal Astronomical Society, 118, 172-182. EMLindsay1961A new catalogue of emission-line stars and planetary nebulae in the SmaDSMathewsonMNClearyJDMurray1974The Magellanic StreamAstrophysical Journal1902912961974ApJ...190..291M10.1086/152875Mathewson, D.S., Cleary, M.N., and Murray, J.D., 1974. The Magellanic Stream. Astrophysical Journal, 190, 291-296. Mathewson, D.S., Healey, J.R., and Rome, J.M., 1962. A radio survey of the southern Milky Way at a frequency of 1440 Mc/s. II. The continuum emission from the Galactic disk. Australian Journal of Physics, 15, 369-377. DSMathewsonSRWayteVLFordKRuan1987The `high velocity cloud' origin of the Magellanic systemProceedings of the Astronomical Society of Australia719251987PASAu...7...19MMathewson, D.S., Wayte, S.R., Ford, V.L., and Ruan, K., 1987. The `high velocity cloud' origin of the Magellanic system. Proceedings of the Astronomical Society of Australia, 7, 19-25. NMMcClure-GriffithsLStaveley-SmithFJLockmanMRCalabrettaHAFordPMWKalberlaTMurphyHNakanishiDJPisano2008An interaction of a Magellanic leading arm high-velocity cloud with the Milky Way diskAstrophysical Journal673L143L1462008ApJ...673L.143M10.1086/528683McClure-Griffiths, N.M., Staveley-Smith, L., Lockman, F.J., Calabretta, M.R., Ford, H.A., Kalberla, P.M. W., Murphy, T., Nakanishi, H., and Pisano, D.J., 2008. An interaction of a Magellanic leading arm high-velocity cloud with the Milky Way disk. Astrophysical Journal, 673, L143-L146. McCready, L.L., 1954. Letter to J.L. Pawsey, dated 19 August. National Archives of Australia, Sydney, 974347 - C3830 - F1/4/PAW/1. McCready, L.L., 1957. Letter to J.L. Pawsey, dated 28 October. National Archives of Australia, Sydney, 974347 - C3830 - F1/4/PAW/1. RXMcGee1964Large HI clouds in the GalaxyFJKerrThe Galaxy and the Magellanic Clouds. Proceedings of the International Astronomical Union Symposium No. 20 Held in Canberra March 18-28, 1963Australian Academy of Science. PpCanberra126130McGee, R.X., 1964. Large HI clouds in the Galaxy. In Kerr, F.J. (ed.). The Galaxy and the Magellanic Clouds. Proceedings of the International Astronomical Union Symposium No. 20 Held in Canberra March 18-28, 1963. Canberra, Australian Academy of Science. Pp. 126-130. McGee, R.X., and Milton, J.A., 1964. A sky survey of neutral hydrogen at λ 21 cm. III. Gas at higher radial velocities. Australian Journal of Physics, 17, 128-157. RXMcGeeJDMurray1961McGee, R.X., and Murray, J.D., 1961b. A sky survey of neutral hydrogen at λ 21 cm I. The general distribution and motions of the local gas. Australian Journal of Physics, 14, 260-278. McGee, R.X., Murray, J.D., and Milton, J.A., 1963. A sky survey of neutral hydrogen at λ 21 cm. II. The detailed distribution of low velocity gas. Australian Journal of Physics, 16, 136-170. RXMcGeeJDMurrayJLPawsey1961Streaming of interstellar hydrogen in the vicinity of the SunNature1899579591961Natur.189..957M10.1038/189957a0McGee, R.X., Murray, J.D., and Pawsey, J.L., 1961. Streaming of interstellar hydrogen in the vicinity of the Sun. Nature, 189, 957-959. KMMentenMJReidJForbrichABrunthaler2007The distance to the Orion NebulaAstronomy and Astrophysics4745155202007A&A...474..515M10.1051/0004-6361:20078247Menten, K.M., Reid, M.J., Forbrich, J., and Brunthaler, A., 2007. The distance to the Orion Nebula. Astronomy and Astrophysics, 474, 515-520. CAMullerGWesterhout1957A catalogue of 21-cm line profilesBulletin of the Astronomical Institutes of the Netherlands131511951957BAN....13..151MMuller, C.A., and Westerhout, G., 1957. A catalogue of 21-cm line profiles. Bulletin of the Astronomical Institutes of the Netherlands, 13, 151-195. JDMurrayRXMcGee1958A new hydrogen cloud in Pyxis-HydraThe Observatory782422441958Obs....78..242MMurray, J.D., and McGee, R.X., 1958. A new hydrogen cloud in Pyxis-Hydra. The Observatory, 78, 242-244. JDMurrayRXMcGee1959Neutral hydrogen gas in the Taurus-Orion region observed with a multichannel 21 cm line receiverAustralian Journal of Physics121271331959AuJPh..12..127M10.1071/PH590127Murray, J.D., and McGee, R.X., 1959. Neutral hydrogen gas in the Taurus-Orion region observed with a multichannel 21 cm line receiver. Australian Journal of Physics, 12, 127-133. JDMurrayRXMcGee1963A multi-channel hydrogen line (21 cm) receiverProceedings of the Institute of Radio Engineers Australia24191196Murray, J.D., and McGee, R.X., 1963. A multi-channel hydrogen line (21 cm) receiver. Proceedings of the Institute of Radio Engineers Australia, 24, 191-196. AOllongrenHCHulstvan de1957Corrections of 21-cm line profilesBulletin of the Astronomical Institutes of the Netherlands131962001957BAN....13..196OOllongren, A., and van de Hulst, H.C., 1957. Corrections of 21-cm line profiles. Bulletin of the Astronomical Institutes of the Netherlands, 13, 196-200. WOrchiston1993New Zealand's role in the identification of the first "radio stars"Southern Stars3546521993SouSt..35...46OOrchiston, W., 1993. New Zealand's role in the identification of the first "radio stars." Southern Stars, 35, 46-52. WOrchiston1994John Bolton, discrete sources, and the New Zealand field-trip of 1948Australian Journal of Physics475415471994AuJPh..47..541OOrchiston, W., 1994. John Bolton, discrete sources, and the New Zealand field-trip of 1948. Australian Journal of Physics, 47, 541-547 Orchiston, W., 2004. The rise and fall of the Chris Cross: a pioneering Australian radio telescope. In Orchiston, W., Stephenson, R., Debarbat, S., and Nha, I.-S. (eds.). Astronomical Instruments and Archives from the Asia-Pacific Region. Seoul, IAU Commission 41. Pp. 157-162. WOrchistonDMathewson2009Chris Christiansen and the Chris CrossJournal of Astronomical History and Heritage1211322009JAHH...12...11OOrchiston, W., and Mathewson, D., 2009. Chris Christiansen and the Chris Cross. Journal of Astronomical History and Heritage, 12, 11-32. WOrchistonBSlee2002Ingenuity and initiative in Australian radio astronomy: the Dover Heights `hole-in-the-ground' antennaJournal of Astronomical History and Heritage521342002JAHH....5...21OOrchiston, W., and Slee, B., 2002. Ingenuity and initiative in Australian radio astronomy: the Dover Heights `hole-in-the-ground' antenna. Journal of Astronomical History and Heritage, 5, 21-34. WOrchistonBSlee2005The Radiophysics field stations and the early development of radio astronomyWOrchistonThe New Astronomy: Opening the Electromagnetic Window and Expanding our View of Planet EarthSpringer. PpDordrecht11916810.1007/1-4020-3724-4_8Orchiston, W., and Slee, B., 2005. The Radiophysics field stations and the early development of radio astronomy. In Orchiston, W. (ed.). The New Astronomy: Opening the Electromagnetic Window and Expanding our View of Planet Earth. Dordrecht, Springer. Pp. 119-168. WOrchistonTNakamuraRStrom2011Highlighting the History of Astronomy in the Asia-Pacific RegionNew YorkSpringerOrchiston, W., Nakamura, T., and Strom, R. (eds.), 2011. Highlighting the History of Astronomy in the Asia-Pacific Region. New York, Springer. AEERodgersKADudevoirJCCarterBJFanousEKratzenberg2005Deuterium abundance in the interstellar gas of the Galactic Anticentre from the 327 MHz LineAstrophysical Journal630L41L442005ApJ...630L..41R10.1086/466524Rodgers, A.E.E., Dudevoir, K.A., Carter, J.C., Fanous, B.J., and Kratzenberg, E., 2005. Deuterium abundance in the interstellar gas of the Galactic Anticentre from the 327 MHz Line. Astrophysical Journal, 630, L41-L44. VCRubinWKFord1970Rotation of the Andromeda Nebula from a spectroscopic survey of emission regionsAstrophysical Journal1593794031970ApJ...159..379R10.1086/150317Rubin, V.C., and Ford, W.K., 1970. Rotation of the Andromeda Nebula from a spectroscopic survey of emission regions. Astrophysical Journal, 159, 379-403. MSchmidt1957Spiral structure in the inner parts of the galactic system derived from the hydrogen emission at 21-cm wavelengthBulletin of the Astronomical Institutes of the Netherlands132472681957BAN....13..247SSchmidt, M., 1957. Spiral structure in the inner parts of the galactic system derived from the hydrogen emission at 21-cm wavelength. Bulletin of the Astronomical Institutes of the Netherlands, 13, 247-268. GAShain1957The inclination to the Galactic Equator of the general magnetic field of LSSparkeJSGallagher2000Galaxies in the Universe: An IntroductionCambridge University PressCambridgeSparke, L.S., and Gallagher, J.S., 2000. Galaxies in the Universe: An Introduction, Cambridge, Cambridge University Press. SStanimirovicLStaveley-SmithJMDickeyRJSaultSLSnowden1999The large-scale HI structure of the Small Magellanic CloudMonthly Notices of the Royal Astronomical Society3024174361999MNRAS.302..417S10.1046/j.1365-8711.1999.02013.xStanimirovic, S., Staveley-Smith, L., Dickey, J.M., Sault, R.J., and Snowden, S.L., 1999. The large-scale HI structure of the Small Magellanic Cloud. Monthly Notices of the Royal Astronomical Society, 302, 417-436. GJStanleyRPrice1956An investigation of monochromatic radio emission of deuterium from the GalaxyNature177122112221956Natur.177.1221S10.1038/1771221a0Stanley, G.J., and Price, R., 1956. An investigation of monochromatic radio emission of deuterium from the Galaxy. Nature, 177, 1221-1222. Stanley, G.J., 1994. Recollections of John G. Bolton at Dover Heights and Caltech. Australian Journal of Physics, 47, 507-516. WTSullivan2009Cosmic Noise. A History of Early Radio AstronomyCambridge University PressCambridgeSullivan, W.T., 2009. Cosmic Noise. A History of Early Radio Astronomy. Cambridge, Cambridge University Press. Townes, C.H., 1957. Microwave and radio-frequency resonance lines of interest to radio astronomy. In van de Hulst, 92-103. HCHulstvan de1957Radio Astronomy, Proceedings from 4th IAU Symposium. International Astronomical UnionCambridgeCambridge University Pressvan de Hulst, H.C. (ed.), 1957. Radio Astronomy, Proceedings from 4th IAU Symposium. International Astronomical Union. Cambridge, Cambridge University Press. HCHulstvan de1958Density and velocity distribution of the interstellar gasReviews of Modern Physics309139231958RvMP...30..913V10.1103/RevModPhys.30.913van de Hulst, H.C., 1958. Density and velocity distribution of the interstellar gas. Reviews of Modern Physics, 30, 913-923. HCHulstvan deCAMullerJHOort1954The spiral structure of the outer part of the galactic system derived from the hydrogen emission at 21 cm wavelengthBulletin of the Astronomical Institutes of the Netherlands121171491954BAN....12..117Vvan de Hulst, H.C., Muller, C.A., and Oort, J.H., 1954. The spiral structure of the outer part of the galactic system derived from the hydrogen emission at 21 cm wavelength. Bulletin of the Astronomical Institutes of the Netherlands, 12, 117-149. HWoerdenvanRStrom2006The beginnings of radio astronomy in the NetherlandsJournal of Astronomical History and Heritage93202006JAHH....9....3Vvan Woerden, H., and Strom, R., 2006. The beginnings of radio astronomy in the Netherlands. Journal of Astronomical History and Heritage, 9, 3-20. PWannierGTWrixon1972An unusual high-velocity hydrogen featureAstrophysical Journal1731191231972ApJ...173L.119W10.1086/180930Wannier, P., and Wrixon, G.T., 1972. An unusual high-velocity hydrogen feature. Astrophysical Journal, 173, 119-123. Wendt, H.W., 2008. The Contribution of the CSIRO Division of Radiophysics Potts Hill and Murraybank Field Stations to International Radio Astronomy. Ph.D. Thesis, Centre for Astronomy, James Cook University, Townsville, Australia. Wendt, H., Orchiston, W., and Slee, B., 2008. W.N. Christiansen and the initial Australian investigation of the 21cm hydrogen line. Journal of Astronomical History and Heritage, 11, 185-193. Wendt, H.W., Orchiston, W., and Slee, W., 2011a. The contribution of the Division of Radiophysics Potts Hill field station to international radio astronomy. In Orchiston et al., 379-431. Wendt, H., Orchiston, W., and Slee, B., 2011b. The contribution of W.N. Christiansen to radio astronomy: 1948-1960. In Orchiston et al., 547-587. GWesterhout1957The distribution of atomic hydrogen in the outer parts of the galactic systemBulletin of the Astronomical Institutes of the Netherlands132012461957BAN....13..201WWesterhout, G., 1957. The distribution of atomic hydrogen in the outer parts of the galactic system. Bulletin of the Astronomical Institutes of the Netherlands, 13, 201-246. GWesterhout1958A survey of the continuous radiation from the galactic system at a frequency of 1390 Mc/sBulletin of the Astronomical Institutes of the Netherlands142152601958BAN....14..215WWesterhout, G., 1958. A survey of the continuous radiation from the galactic system at a frequency of 1390 Mc/s. Bulletin of the Astronomical Institutes of the Netherlands, 14, 215-260. JPWild1952The radio-frequency line spectrum of atomic hydrogen and its applications in astronomyAstrophysical Journal1152062211952ApJ...115..206W10.1086/145533Wild, J.P., 1952. The radio-frequency line spectrum of atomic hydrogen and its applications in astronomy. Astrophysical Journal, 115, 206-221.

Acquired dyslexia in Serbian speakers with Broca's and Wernicke's aphasia.

PubMed

Vuković, Mile; Vuković, Irena; Miller, Nick

2016-01-01

This study examined patterns of acquired dyslexia in Serbian aphasic speakers, comparing profiles of groups with Broca's versus Wernicke's aphasia. The study also looked at the relationship of reading and auditory comprehension and between reading comprehension and reading aloud in these groups. Participants were 20 people with Broca's and 20 with Wernicke's aphasia. They were asked to read aloud and to understand written material from the Serbian adaptation of the Boston Diagnostic Aphasia Examination. A Serbian Word Reading Aloud Test was also used. The people with Broca's aphasia achieved better results in reading aloud and in reading comprehension than those with Wernicke's aphasia. Those with Wernicke's aphasia showed significantly more semantic errors than those with Broca's aphasia who had significantly more morphological and phonological errors. From the data we inferred that lesion sites accorded with previous work on networks associated with Broca's and Wernicke's aphasia and with a posterior-anterior axis for reading processes centred on (left) parietal-temporal-frontal lobes. Copyright © 2016 Elsevier Inc. All rights reserved.

Past, Present and Future: Forty Years of Revista Mexicana de Astronomia y Astrofisica

NASA Astrophysics Data System (ADS)

Allen, Christine; Torres-Peimbert, Silvia

2015-08-01

We cast a retrospective view on 40 years of publishing the Revista Mexicana de Astronomía y Astrofísica, founded in 1974. The journal is peer-reviewed, has appeared regularly since its foundation, and continues to attract original research papers, mostly by Mexican and Latin American authors. We share some musings about the future of our journal, in view of recent developments in the scientific publishing field.

What Happened to the Amateurs After Professionalization? The Amateurization of Astronomy in Britain and the United States

NASA Astrophysics Data System (ADS)

Williams, T. R.

2003-12-01

For nearly two centuries, astronomers have felt the need for a journal in which to publish their results, a venue for meetings in which to discuss those results, and a means for standardizing techniques and coordinating programs within the discipline. These factors are typically the basis on which professional associations have been formed, but in many countries some form of an amateur organization now exists to serve these same purposes. In two case studies, this paper will explore the different paths along which amateur organizations have developed in response to radically different dynamics in the professionalization of astronomy. In Britain, several failures preceded the successful formation of the British Astronomical Association (BAA). Within no more than a decade after its founding, the BAA's specialized observing sections and credible journal were admired by professional and amateur astronomers alike, and served as a model for at least three failed attempts to form a similar organization in the United States. What emerged in the United States instead were six separate specialized observing associations, some of which now legitimately claim international status. This talk will consider how the radically different circumstances under which the professionalization of astronomy occurred in Britain and the United States influenced the amateurization of astronomy in both countries.

Articulation of sounds in Serbian language in patients who learned esophageal speech successfully.

PubMed

Vekić, Maja; Veselinović, Mila; Mumović, Gordana; Mitrović, Slobodan M

2014-01-01

Articulation of pronounced sounds during the training and subsequent use of esophageal speech is very important because it contributes significantly to intelligibility and aesthetics of spoken words and sentences, as well as of speech and language itself. The aim of this research was to determine the quality of articulation of sounds of Serbian language by groups of sounds in patients who had learned esophageal speech successfully as well as the effect of age and tooth loss on the quality of articulation. This retrospective-prospective study included 16 patients who had undergone total laryngectomy. Having completed the rehabilitation of speech, these patient used esophageal voice and speech. The quality of articulation was tested by the "Global test of articulation." Esophageal speech was rated with grade 5, 4 and 3 in 62.5%, 31.3% and one patient, respectively. Serbian was the native language of all the patients. The study included 30 sounds of Serbian language in 16 subjects (480 total sounds). Only two patients (12.5%) articulated all sounds properly, whereas 87.5% of them had incorrect articulation. The articulation of affricates and fricatives, especially sound /h/ from the group of the fricatives, was found to be the worst in the patients who had successfully mastered esophageal speech. The age and the tooth loss of patients who have mastered esophageal speech do not affect the articulation of sounds in Serbian language.

[Contrastive analysis of Latin terms for denoting human organs and structural body parts and parts of organs in anatomy literature in English and Serbian].

PubMed

Vukčević-Lacković, Biljana

2011-01-01

This paper is concerned with the analysis of the use of Latin terms in the field of human anatomy through the contrastive analysis of examples from anatomy atlases and textbooks, and research papers in the area of human anatomy in English and Serbian. The contrastive analysis of examples has highlighted a certain tendency towards the use of original Latin terms in anatomy literature in the Serbian language, while the tendency of anatomy literature in English is towards the use of English terms which most often have a Latin root. It has also been noted that Serbian literature, in addition to original Latin terms, uses a significant number of terms with a Latin root. The noted tendencies differ depending on the type of literature (anatomy atlas, textbook or research paper). A significantly greater uniformity in the use of terminology has been noted in editions in English as compared to the Serbian anatomy literature where a lack of such a uniform system is evident. Bearing in mind the ever increasing significance of the English language in the world of science, one of the conclusions of this paper is that these differences may be of practical significance for authors from Serbia looking to publish their work in English as well as for translators of medical literature.

An English-Serbocroatian Dictionary. Vols. I-II.

ERIC Educational Resources Information Center

Ristic, Svetomir, Comp.; And Others

This two-volume comprehensive English-Serbocroatian dictionary, first published in Yugoslavia by the Serbian Publishing House, Prosveta, in 1956, contains the Serbocroatian equivalents of about 100,000 words, phrases, and idioms. Volume I (A-M, 843 pages) includes a prefatory section of printed and written alphabets in Serbian, Croatian (both…

Jovan Skerlic as a Life Tutor

ERIC Educational Resources Information Center

Mumovic, Ana

2015-01-01

The paper studies and illuminates Jovan Skerlic's social function and "criticism anatomy" in his "History of Serbian Literature." The object of analysis is the act and actors of Skerlic's engaged criticism and method relying on facts. It is the path taken a hundred years later by Serbian criticism and literature as culture and…

Contextual Evidence for the Representation of Pitch Accents in Standard Serbian

ERIC Educational Resources Information Center

Zsiga, Elizabeth; Zec, Draga

2013-01-01

This paper reports the results of an experiment that elicits contextual effects on Rising and Falling accents in Standard Serbian, with the goal of determining their acoustic correlates and their phonological representation. Materials systematically vary the distance between pitch accents, inducing "tone crowding," in order to identify the…

Modality and Causation in Serbian Dative Anticausatives: A Crosslinguistic Perspective

ERIC Educational Resources Information Center

Ilic, Tatjana

2013-01-01

In this dissertation I provide a principled, unified account of modality and causation in Serbian dative anticausatives using a typological, cognitive approach. This analysis is set within a larger claim that the causative and modal meanings crosslinguistically arise in the same morphosyntactic environments, indicating a shared conceptual base…

Agrobacterium-mediated transformation of two Serbian potato cultivars (Solanum tuberosum L. cv. Dragacevka and cv. Jelica)

USDA-ARS?s Scientific Manuscript database

An efficient protocol for Agrobacterium-mediated transformation of Serbian potato cultivars Dragacevka and Jelica, enabling the introduction of oryzacystatin genes OCI and OCII, was established. Starting with leaf explants a two-stage transformation protocol combining procedures of Webb and Wenzler...

Factor Structure of the Serbian Version of the Children's Communication Checklist-2

ERIC Educational Resources Information Center

Glumbic, Nenad; Brojcin, Branislav

2012-01-01

Keeping in mind that traditional tests were largely insensitive to pragmatic impairment, Bishop (2003) created a second version of the "Children's Communication Checklist" (CCC-2) in order to identify pragmatic deficits in children with communication problems. Unfortunately, it was revealed that certain subscales of the Serbian version…

High School and Community College Astronomy Research Seminar

NASA Astrophysics Data System (ADS)

Genet, Russell M.; Boyce, Pat; Buchheim, Robert; Collins, Dwight; Freed, Rachel; Harshaw, Richard; Johnson, Jolyon; Kenney, John; Wallen, Vera

2016-06-01

For the past decade, Cuesta College has held an Astronomy Research Seminar. Teams of high school and community college students, with guidance from instructors and advanced amateur astronomers, have made astronomical observations, reduced their data, and submitted their research results to appropriate journals. A variety of projects, using modest-aperture telescopes equipped with low-cost instruments, are within reach of motivated students. These include double star astrometry, variable star photometry, and exoplanet transit timing. Advanced scientific knowledge and mastery of sophisticated experimental skills are not required when the students are immersed within a supportive community of practice. The seminar features self-paced, online learning units, an online textbook (the Small Telescope Astronomical Research Handbook), and a supportive website sponsored by the Institute for Student Astronomical Research (www.In4StAR.org). There are no prerequisites for the seminar. This encourages everyone—including underrepresented minorities and persons with disabilities—to participate. Each participant contributes as their time, talents, and experience dictates, thus replicating the modern, professional research team. Our spring 2015 seminar was the largest yet. Volunteer assistant instructors provided local in-person leadership, while the entire seminar met online for PowerPoint presentations on proposed projects and final research results. Some 37 students from eight schools finished the seminar as coauthors of 19 papers published in the January 2016 volume of the Journal of Double Star Observations. Robotic telescopes devoted to student research are coming online at both Concordia University and the Boyce Astronomical Robotic Observatory, as is a central online sever that will provide students with uniform, cost-free reduction and analysis software. The seminar has motivated many of its graduates to pursue careers in science, engineering, and medicine, often with scholarships. We are planning on expanding the seminar to other high schools and community colleges within California and across the nation.

Nature's ups and downs

NASA Astrophysics Data System (ADS)

Rodgers, Peter

2015-12-01

When Norman Lockyer, an astronomer and science writer with a day job as a clerk at the War Office in London, approached the publishing house Macmillan and Company in 1869 with a proposal for a new weekly journal about science, few could have predicted the outcome. The journal in question was Nature, and given its influence over the past 146 years, it is hard to believe that Melinda Baldwin's Making Nature is the first full-length book to be written about it.

SABER: The Searchable Annotated Bibliography of Education Research in Astronomy

NASA Astrophysics Data System (ADS)

Bruning, David; Bailey, Janelle M.; Brissenden, Gina

Starting a new research project can be a challenge, but especially so in education research because the literature is scattered throughout many journals. Relevant astronomy education research may be in psychology journals, science education journals, physics education journals, or even in science journals. Tracking the vast realm of literature is difficult, especially because libraries frequently do not subscribe to many of the relevant journals and abstracting services. The Searchable Annotated Bibliography of Education Research (SABER) is an online resource that was started to service the needs of the astronomy education community, specifically to reduce this "scatter" by compiling an annotated bibliography of education research articles in one electronic location. Although SABER started in 2001, the database has a new URL—http://astronom- y.uwp.edu/saber/—and has recently undergone a major update.

Creativity and Anxiety in Roma and Serbian Adolescents

ERIC Educational Resources Information Center

Spasic, Miljana

2016-01-01

In this paper, we present a research whose aim was to investigate the relationship between creativity and anxiety during the period of early adolescence. Furthermore, we were interested in discovering potential differences among Roma and Serbian adolescents at the level of creativity, situational and general anxiety. The sample consisted of 60…

One Church, One People, One Emperor’ - Strategic Challenges for the Serbian Orthodox Church in Post-Milosevic Serbian Society

DTIC Science & Technology

2006-06-01

elites are not particularly threatened by democraticization” since the institutions required to run the democracy “are already well established before... Philanthropy website, http://www.covekoljublje.org/proj_completed.htm (accessed 18 May 2006). 244 “More Ethnic Fighting in Kosovo Leaves Thousands

Language Names and Norms in Bosnia and Herzegovina

ERIC Educational Resources Information Center

Swagman, Kirstin J.

2011-01-01

The institutionalization of separate standard varieties for Bosnian, Croatian, and Serbian in the 1990s was hailed by many Bosnians as the long-denied recognition of the Bosnian idiom as distinct from the Serbian and Croatian varieties it had so often been subordinated under. Yet the accompanying codification of Bosnian standard language forms has…

Non-Finite Complements in Russian, Serbian/Croatian, and Macedonian

ERIC Educational Resources Information Center

Kim, Bo Ra

2010-01-01

This study investigates the coherence properties of non-finite complements in Russian, Serbian/Croatian, and Macedonian. I demonstrate that Slavic non-finite complements do not project a uniform syntactic structure. The maximal projection of non-finite complements is not fixed but depends on the selectional properties of the matrix verb. I present…

Serbian: The Serbian Language in Education in Hungary. Regional Dossiers Series

ERIC Educational Resources Information Center

Paulik, Anton, Comp.; Solymosi, Judit, Comp.

2014-01-01

This regional dossier aims at providing a concise description of and basic statistics on minority language education in a specific region of Europe--the territory of Magyarország (Hungary). Aspects that are addressed include features of the education system, recent educational policies, main actors, legal arrangements, and support structures, as…

Education Interrupted: Kosovo 1980-1999

ERIC Educational Resources Information Center

Llapi, Gjylbehare; Peterson, Claudette M.

2015-01-01

The period between 1980 and 1999 was one of interruption of education for Albanian students in Kosovo. Serbian students were allowed to attend school, which was now taught in the Serbian language that excluded Albanians. A parallel system of education evolved in which secret house-schools were established in order to educate Albanian speakers in…

Between Yugoslavism and Serbianism: Reshaping Collective Identity in Serbian Textbooks between the World Wars

ERIC Educational Resources Information Center

Troch, Pieter

2012-01-01

Studies of nationhood in interwar Yugoslavia generally refrain from considering dynamic relations between different levels of collective identity available in the state. Inspired by scholarly studies which have pointed at the compatibility of national and sub-national identities, this article examines interaction between definitions of Yugoslav…

"I Am What I Am": Multilingual Identity and Digital Translanguaging

ERIC Educational Resources Information Center

Schreiber, Brooke Ricker

2015-01-01

This paper presents a case study of the multilingual writing practices of a Serbian university student on Facebook, examining how he uses multiple varieties of English and Serbian images and video to shape his online identity and establish membership in local and global communities. Drawing on data from stimulated-recall interviews, online…

The Synchrony and Diachrony of Bosnian-Croatian-Serbian Adjectival Long-Form Allomorphy (ALFA)

ERIC Educational Resources Information Center

Pennington, James Joshua

2010-01-01

In Bosnian-Croatian-Serbian (BCS), the gentive (G) and dative/locative (DL) cases exhibit adjectival long-form allomorphy (ALFA). The genitive -"og" -"oga" and the DL -"om" -"ome" -"omu" stand in free variation, inasmuch as when one form is substituted for another the truth value of an utterance…

Safety in Serbian animal source food industry and the impact of hazard analysis and critical control points: A review

NASA Astrophysics Data System (ADS)

Tomašević, I.; Đekić, I.

2017-09-01

There is a significant lack of HACCP-educated and/or HACCP-highly trained personnel within the Serbian animal source food workforces and veterinary inspectors, and this can present problems, particularly in hazard identification and assessment activities. However, despite obvious difficulties, HACCP benefits to the Serbian dairy industry are widespread and significant. Improving prerequisite programmes on the farms, mainly through infrastructural investments in milk collectors and transportation vehicles on one hand, and increasing hygiene awareness of farmers through training on the other hand has improved the safety of milk. The decline in bacterial numbers on meat contact surfaces, meat handlers’ hands and cooling facilities presents strong evidence of improved process hygiene and justifies the adoption of HACCP in Serbian meat establishments. Apart from the absence of national food poisoning statistics or national foodborne disease databases, the main obstacle to fully recognising the impact of HACCP on the safety of animal source food in Serbia is the lack of research regarding the occurrence of chemical and/or physical hazards interrelated with its production.

The Next Information Revolution in Astronomy

NASA Astrophysics Data System (ADS)

Kennicutt, R. C.

2006-08-01

The information revolution has truly revolutionized our profession, through such innovations as the astronomical data centres, electronic journals and preprint servers, and bibliographic interfaces that link these resources through instantaneous and freely available web interfaces. For most of us the effects of these innovations have been profound, changing forever the way we access the research literature, disseminate results to our colleagues, and even in the ways we carry out our research and write papers. Astronomy's efforts in this area have attracted the attention and admiration of other scientific professions as well as the information technology community. We now stand at the threshold of a second revolution, in which enormous and rich collections of astronomical observations, models, software, and tools will be accessible through a common Virtual Observatory interface. The next logical step beyond that is an integration of these VO resources with the web of astronomical literature, to provide mechanisms for quality certification of those resources, and to provide a seamless mechanism by which authors can make the results of their research available to other scientists in their most useful form. If this is done successfully its impacts on the way we conduct and disseminate our research may be as profound as those of the past decade. However this success will require cooperative approaches to information archiving and publication involving the data centres, journals, and library communities, and which incorporate or at least emulate the features of curation, provenance, quality assurance, and intellectual property protections that underlie the traditional publishing system. This talk will highlight some of the efforts being made in the VO and journal communities to make this vision a reality, and identify some of the key challenges that remain.

Serbian translation of the 20-item Toronto Alexithymia Scale: psychometric properties and the new methodological approach in translating scales.

PubMed

Trajanović, Nikola N; Djurić, Vladimir; Latas, Milan; Milovanović, Srdjan; Jovanović, Aleksandar A; Djurić, Dusan

2013-01-01

Since inception of the alexithymia construct in 1970's, there has been a continuous effort to improve both its theoretical postulates and the clinical utility through development, standardization and validation of assessment scales. The aim of this study was to validate the Serbian translation of the 20-item Toronto Alexithymia Scale (TAS-20) and to propose a new method of translation of scales with a property of temporal stability. The scale was expertly translated by bilingual medical professionals and a linguist, and given to a sample of bilingual participants from the general population who completed both the English and the Serbian version of the scale one week apart. The findings showed that the Serbian version of the TAS-20 had a good internal consistency reliability regarding total scale (alpha=0.86), and acceptable reliability of the three factors (alpha=0.71-0.79). The analysis confirmed the validity and consistency of the Serbian translation of the scale, with observed weakness of the factorial structure consistent with studies in other languages. The results also showed that the method of utilizing a self-control bilingual subject is a useful alternative to the back-translation method, particularly in cases of linguistically and structurally sensitive scales, or in cases where a larger sample is not available. This method, dubbed as 'forth-translation' could be used to translate psychometric scales measuring properties which have temporal stability over the period of at least several weeks.

Assessing Attitudes towards Statistics among Medical Students: Psychometric Properties of the Serbian Version of the Survey of Attitudes Towards Statistics (SATS)

PubMed Central

Stanisavljevic, Dejana; Trajkovic, Goran; Marinkovic, Jelena; Bukumiric, Zoran; Cirkovic, Andja; Milic, Natasa

2014-01-01

Background Medical statistics has become important and relevant for future doctors, enabling them to practice evidence based medicine. Recent studies report that students’ attitudes towards statistics play an important role in their statistics achievements. The aim of the study was to test the psychometric properties of the Serbian version of the Survey of Attitudes Towards Statistics (SATS) in order to acquire a valid instrument to measure attitudes inside the Serbian educational context. Methods The validation study was performed on a cohort of 417 medical students who were enrolled in an obligatory introductory statistics course. The SATS adaptation was based on an internationally accepted methodology for translation and cultural adaptation. Psychometric properties of the Serbian version of the SATS were analyzed through the examination of factorial structure and internal consistency. Results Most medical students held positive attitudes towards statistics. The average total SATS score was above neutral (4.3±0.8), and varied from 1.9 to 6.2. Confirmatory factor analysis validated the six-factor structure of the questionnaire (Affect, Cognitive Competence, Value, Difficulty, Interest and Effort). Values for fit indices TLI (0.940) and CFI (0.961) were above the cut-off of ≥0.90. The RMSEA value of 0.064 (0.051–0.078) was below the suggested value of ≤0.08. Cronbach’s alpha of the entire scale was 0.90, indicating scale reliability. In a multivariate regression model, self-rating of ability in mathematics and current grade point average were significantly associated with the total SATS score after adjusting for age and gender. Conclusion Present study provided the evidence for the appropriate metric properties of the Serbian version of SATS. Confirmatory factor analysis validated the six-factor structure of the scale. The SATS might be reliable and a valid instrument for identifying medical students’ attitudes towards statistics in the Serbian educational context. PMID:25405489

Assessing attitudes towards statistics among medical students: psychometric properties of the Serbian version of the Survey of Attitudes Towards Statistics (SATS).

PubMed

Stanisavljevic, Dejana; Trajkovic, Goran; Marinkovic, Jelena; Bukumiric, Zoran; Cirkovic, Andja; Milic, Natasa

2014-01-01

Medical statistics has become important and relevant for future doctors, enabling them to practice evidence based medicine. Recent studies report that students' attitudes towards statistics play an important role in their statistics achievements. The aim of the study was to test the psychometric properties of the Serbian version of the Survey of Attitudes Towards Statistics (SATS) in order to acquire a valid instrument to measure attitudes inside the Serbian educational context. The validation study was performed on a cohort of 417 medical students who were enrolled in an obligatory introductory statistics course. The SATS adaptation was based on an internationally accepted methodology for translation and cultural adaptation. Psychometric properties of the Serbian version of the SATS were analyzed through the examination of factorial structure and internal consistency. Most medical students held positive attitudes towards statistics. The average total SATS score was above neutral (4.3±0.8), and varied from 1.9 to 6.2. Confirmatory factor analysis validated the six-factor structure of the questionnaire (Affect, Cognitive Competence, Value, Difficulty, Interest and Effort). Values for fit indices TLI (0.940) and CFI (0.961) were above the cut-off of ≥0.90. The RMSEA value of 0.064 (0.051-0.078) was below the suggested value of ≤0.08. Cronbach's alpha of the entire scale was 0.90, indicating scale reliability. In a multivariate regression model, self-rating of ability in mathematics and current grade point average were significantly associated with the total SATS score after adjusting for age and gender. Present study provided the evidence for the appropriate metric properties of the Serbian version of SATS. Confirmatory factor analysis validated the six-factor structure of the scale. The SATS might be reliable and a valid instrument for identifying medical students' attitudes towards statistics in the Serbian educational context.

Getting organized: A history of amateur astronomy in the United States

NASA Astrophysics Data System (ADS)

Williams, Thomas R.

2000-10-01

During the twentieth century, American amateur astronomers attempted to form national organizations with structures and intents similar to the British Astronomical Association (BAA), an amateur organization dedicated to the advancement of astronomy and widely admired by American amateurs and professionals alike. The Society for Practical Astronomy (1910), the American Amateur Astronomers Association (1935), and the National Astronomical Association (1945) were each intended to facilitate amateur scientific contributions in BAA-like topical sections, but each of these societies failed. Founded in 1911, the American Association of Variable Star Observers (AAVSO) and the American Meteor Society (AMS) provided an alternative for amateur astronomers who were interested in those specific topics. However, it was not until 1947, when the Association of Lunar and Planetary Observers (ALPO) formed, that another large segment of amateur astronomers found a home for their interests. A second mode of national organization succeeded at mid- century and grew to include most avocational astronomers. Founded in 1947, the Astronomical League consists of regional associations of local societies, and is oriented largely towards recreational astronomy. The League sponsors annual national and regional conventions, but contributes little to scientific programs. This study concludes that avocational astronomy cannot simply be compared with professional astronomy, and instead must be viewed on its own terms as a complex and variegated field. Although the failure of American amateurs to form a BAA-like organization was at first disappointing, the specialized associations of observers, together with a separate and larger organization devoted to recreational astronomy, have served the American astronomical community well. Professional support for both types of activity was facilitated in this mode of organization. The style in which professional support is rendered appears to be important, with strong volunteer member leadership more effective than a benevolent dictatorship by professionals. A journal in which amateur astronomers may publish observations, discuss techniques and share insights is critical for scientifically oriented associations, and provided a driving force for organizing and maintaining such associations.

Student Moon Observations and Spatial-Scientific Reasoning

ERIC Educational Resources Information Center

Cole, Merryn; Wilhelm, Jennifer; Yang, Hongwei

2015-01-01

Relationships between sixth grade students' moon journaling and students' spatial-scientific reasoning after implementation of an Earth/Space unit were examined. Teachers used the project-based Realistic Explorations in Astronomical Learning curriculum. We used a regression model to analyze the relationship between the students' Lunar Phases…

Long-publishing astronomers, or the problem of classification

NASA Astrophysics Data System (ADS)

Tenn, Joseph S.

2012-03-01

In response to several discussions among astronomers and historians of astronomy, I started out to prepare a paper on long-publishing astronomers-those who published for 70, 75, or even 80 years. However, I soon ran into a number of questions of classification, and that turned out to be at least as interesting. How do we decide on classifications? Every time we choose classes, such as asteroids, planets and stars, we run into objects that seem to be in between. In the present case a number of questions arise: Who is an astronomer? Several of those with the longest publication runs started out as physicists, published for years in that subject only, and later took up astrophysics, eventually publishing a few papers in astronomy journals. What is a publication? Should we count publications in physics, chemistry, or mathematics? What about philosophy of science or history of science? What about the elderly retired astronomer presenting a memoir of his or her own work? Abstracts of oral presentations? Monographs? Textbooks? Book reviews? Obituaries? Then there is the problem of posthumous publications. Probably most would include papers in the pipeline when the astronomer dies, but what about the case where the coauthor finally publishes the paper as much as twenty-two years after the death of the person of interest? I eventually decided to make two lists, one which would include most of the above, and one restricted to papers that make contributions to physical science. Note that I do not say 'refereed', as that presents its own problems, especially when applied to periods before the twentieth century. I present a list of astronomers who have published for periods of 68 to 80 years and discuss the problems of defining such terms as astronomer and publication.

The Assembly of Phonology From Print Is Serial and Subject to Strategic Control: Evidence From Serbian

ERIC Educational Resources Information Center

Havelka, Jelena; Rastle, Kathleen

2005-01-01

The Serbian writing system was used to investigate whether a serial procedure is implicated in print-to-sound translation and whether components of the reading aloud system can be strategically controlled. In mixed- and pure-alphabet lists, participants read aloud phonologically bivalent words comprising bivalent letters in initial or final…

Allergen labelling in meat, dairy and cereal products from the Serbian market

NASA Astrophysics Data System (ADS)

Spirić, D.; Nikolić, D.; Ćirić, J.; Janković, S.; Stefanović, S.; Janković, V.; Teodorović, V.

2017-09-01

Allergens in food are a great health risk, because of the ratio of severity of problems compared to small amounts of ingested allergen. Since 2014, Serbian producers and importers of food have been obliged to declare allergens from the list of Codex Alimentarius on the product packaging. Surveillance of different meat, diary, and cereal product took place in 2016, with aim of checking if the Serbian regulatory requirements for labelling of allergens in food are being fulfilled. Out of 68 different meat products, 20 were not labelled for allergens. Thirty-six labels of various dairy products were examined revealing that allergen information was included on 27 of them. Only one of eight examined cereal products did not have allergen labelling.

Developing an Undergraduate Astronomical Research Program

NASA Astrophysics Data System (ADS)

Genet, R. M.

2007-05-01

Time-series astronomical photometry is an area of scientific research well suited to amateurs and undergraduates, and their backyard and campus observatories. I describe two past one-semester community college research programs, one six year ago and one last fall (2006), as well as a program planned for this coming fall (2007). The 2001 program, a course at Central Arizona College, utilized a robotic telescope at the Fairborn Observatory. Results were presented at the 200th meeting of the American Astronomical Society. This past fall, three students, in a 17-week, one-semester course at Cuesta College, were able to plan a research program, make several thousand CCD photometric observations, reduce and analyze their data, write up their results and, on the last day of class, send their paper off to a refereed journal, the JAAVSO. A course is being offered this coming fall (2007) that will involve about a dozen students (including high school students), several local amateur astronomers, and at least three CCD- equipped semi-automatic telescopes. Potential solutions to "scaling up" challenges created by increased class size are discussed.

XML at the ADC: Steps to a Next Generation Data Archive

NASA Astrophysics Data System (ADS)

Shaya, E.; Blackwell, J.; Gass, J.; Oliversen, N.; Schneider, G.; Thomas, B.; Cheung, C.; White, R. A.

1999-05-01

The eXtensible Markup Language (XML) is a document markup language that allows users to specify their own tags, to create hierarchical structures to qualify their data, and to support automatic checking of documents for structural validity. It is being intensively supported by nearly every major corporate software developer. Under the funds of a NASA AISRP proposal, the Astronomical Data Center (ADC, http://adc.gsfc.nasa.gov) is developing an infrastructure for importation, enhancement, and distribution of data and metadata using XML as the document markup language. We discuss the preliminary Document Type Definition (DTD, at http://adc.gsfc.nasa.gov/xml) which specifies the elements and their attributes in our metadata documents. This attempts to define both the metadata of an astronomical catalog and the `header' information of an astronomical table. In addition, we give an overview of the planned flow of data through automated pipelines from authors and journal presses into our XML archive and retrieval through the web via the XML-QL Query Language and eXtensible Style Language (XSL) scripts. When completed, the catalogs and journal tables at the ADC will be tightly hyperlinked to enhance data discovery. In addition one will be able to search on fragmentary information. For instance, one could query for a table by entering that the second author is so-and-so or that the third author is at such-and-such institution.

GCH1 mutations are common in Serbian patients with dystonia-parkinsonism: Challenging previously reported prevalence rates of DOPA-responsive dystonia.

PubMed

Dobričić, Valerija; Tomić, Aleksandra; Branković, Vesna; Kresojević, Nikola; Janković, Milena; Westenberger, Ana; Rašić, Vedrana Milić; Klein, Christine; Novaković, Ivana; Svetel, Marina; Kostić, Vladimir S

2017-12-01

GTP cyclohydrolase 1-deficient DOPA-responsive dystonia, caused by autosomal dominant mutation in the gene coding for GTP cyclohydrolase 1, is a rare disorder with a reported prevalence of 0.5 per million. A correct diagnosis of DRD is crucial, given that this is an exquisitely treatable neurogenetic disorder. Although genetic testing is now widely available, we hypothesize that DRD is still underdiagnosed and its prevalence underestimated. Molecular genetic analysis of the GCH1 gene was performed in a representative cohort of 47 Serbian patients with clinical features of DRD and in their 16 available relatives. The DRD prevalence rate in Serbia was estimated based on population size, catchment area, and the centralized Serbian referral system for rare diseases. We identified 9 different GCH1 mutations in 23 individuals from 11 families, 5 of which are novel. Patients displayed a broad range of clinical phenotypes. The estimated prevalence of GCH1-related DOPA-responsive dystonia in Serbia was 2.96 per million individuals and there was no evidence for a common founder. Our data expand the genotypic spectrum of GCH1 and confirm the broad phenotypic spectrum of DRD in the Serbian population. The number of detected mutation carriers in this sample implies that the frequency of DRD in the Serbian population is considerably higher than expected based on published prevalence rates, suggesting that the prevalence of this treatable disease should be revisited also in other populations. Copyright © 2017 Elsevier Ltd. All rights reserved.

[Beginnings of nursing education and nurses' contribution to nursing professional development in Serbia].

PubMed

Vlaisavljević, Željko; Čolović, Nataša; Perišić, Mirjana

2014-01-01

The oldest records of developmental beginnings of patients' healthcare relate to the first hospital founded by St. Sava at the monastery Studenica in 1199. The profile of the Kosovian girl became the hallmark of nursing profession in Serbia. The first school for midwives was founded in 1899 at the Department of Gynecology and Obstetrics of the General State Hospital in Belgrade. However, there were no other schools for nurses in Serbia until the foundation of the School for Midwives of the Red Cross Society in 1021. Until then the healthcare of patients and the injured was carried out by self-taught volunteer nurses with completed short courses of patients' healthcare. The first course for male and female nurses was organized by the Serbian Red Cross at the beginning of the First Serbian-Turkish War in 1876. During wars with Serbian participation in 19th and 20th centuries with Serbian participation, nurses gave a remarkable contribution being exposed to extreme efforts and often sacrificing their own lives. In war times great merit belongs to the members of the humanitarian society the Circle of Serbian Sisters founded in Belgrade in 1903, which was the resource of a great number of nurses who became the pride of nursing profession. Generations of nurses were educated on their example. In 2004 the annual award "Dušica Spasić" was established which is awarded to the best medical nurse is Serbia. Dušica Spasić was a medical nurse that died at her workplace, when aged 23 years, nursing the sick from variola.

Giant Exoplanet and Debris Disk (Artist's Concept)

NASA Image and Video Library

2017-10-11

This artist's rendering shows a giant exoplanet causing small bodies to collide in a disk of dust. A study in The Astronomical Journal finds that giant exoplanets with long-period orbits are more likely to be found around young stars that have a disk of dust and debris than those without disks. The study focused on planets more than five times the mass of Jupiter. The astronomers are conducting the largest survey to date of stars with dusty debris disks, and finding the best evidence yet that giant planets are responsible for keeping that material in check. https://photojournal.jpl.nasa.gov/catalog/PIA22082

Astrophysics and Space Science

NASA Astrophysics Data System (ADS)

Mould, Jeremy; Brinks, Elias; Khanna, Ramon

2015-08-01

Astrophysics and Space Science publishes original contributions and invited reviews covering the entire range of astronomy, astrophysics, astrophysical cosmology, planetary and space science, and the astrophysical aspects of astrobiology. This includes both observational and theoretical research, the techniques of astronomical instrumentation and data analysis, and astronomical space instrumentation. We particularly welcome papers in the general fields of high-energy astrophysics, astrophysical and astrochemical studies of the interstellar medium including star formation, planetary astrophysics, the formation and evolution of galaxies and the evolution of large scale structure in the Universe. Papers in mathematical physics or in general relativity which do not establish clear astrophysical applications will not longer be considered.The journal also publishes topical collections consisting of invited reviews and original research papers selected special issues in research fields of particular scientific interest. These consist of both invited reviews and original research papers.Conference proceedings will not be considered. All papers published in the journal are subject to thorough and strict peer-reviewing.Astrophysics and Space Science has an Impact Factor of 2.4 and features short editorial turnaround times as well as short publication times after acceptance, and colour printing free of charge. Published by Springer the journal has a very wide online dissemination and can be accessed by researchers at a very large number of institutes worldwide.

The Acquisition of Passives in Serbian

ERIC Educational Resources Information Center

Perovic, Alexandra; Vuksanovic, Jasmina; Petrovic, Boban; Avramovic-Ilic, Irena

2014-01-01

This study examined the comprehension of actional and psychological verbs in both their active and passive (short and long) forms by 99 Serbian-speaking children. The children, whose age ranged between 3 years, 6 months (3;6) and 7 years, 6 months (7;6), were divided into three groups: 3;6-5 ("M" = 4.3), 5;1-6;1 ("M" = 5.6),…

A cross-cultural study to assess measurement invariance of the KIDSCREEN-27 questionnaire across Serbian and Iranian children and adolescents.

PubMed

Stevanovic, Dejan; Jafari, Peyman

2015-01-01

The KIDSCREEN questionnaire for health-related quality of life (HRQOL) assessments in children and adolescents was simultaneously developed across 13 European countries, and it was subsequently translated and culturally adapted to over 30 different languages across the world. The aim of this study was to evaluate the measurement equivalence of the KIDSCREEN-27 across Serbian and Iranian children and adolescents. The items in the KIDSCREEN-27 were analyzed for differential item functioning (DIF) across Iranian and Serbian populations using ordinal logistic regression with three different criteria. The sample included 330 Iranian and 329 Serbian children and adolescents and 330 and 314 of their parents, respectively. Across the two samples, DIF was detected in 16 (59 %) of 27 items in the child self-reports and in 20 (74 %) of 27 items in the parent/proxy report. However, using alternative criteria based on magnitude detected for DIF, only three items in the parent/proxy report showed significant DIF. Our study provided more evidence that the KIDSCREEN-27 possesses DIF items across different cultures, but their impact is probably small, and the questionnaire could be used for cross-cultural HRQOL comparisons.

Women in Astronomy.

ERIC Educational Resources Information Center

Mercury, 1992

1992-01-01

This issue of "Mercury" is a tribute to the accomplishments of female astronomers. It is an affirmation that women can and do pursue successful careers in the physical sciences even though some special obstacles have existed and, sadly, continue to exist in both the education process and the professional career process. The journal contains the…

Big Ideas: A Review of Astronomy Education Research 1974-2008

ERIC Educational Resources Information Center

Lelliott, Anthony; Rollnick, Marissa

2010-01-01

This paper reviews astronomy education research carried out among school students, teachers, and museum visitors over a 35-year period from 1974 until 2008. One hundred and three peer-reviewed journal articles were examined, the majority of whose research dealt with conceptions of astronomical phenomena with 40% investigating intervention…

The Navy Precision Optical Interferometer (NPOI): An Update

DTIC Science & Technology

2013-01-01

IOTA1. Since that time, four of these have closed: I2T, COAST, GI2T, and IOTA . Three others have opened and closed: PTI, MIRA-I.2,2 and 1Corresponding...public release; distribution unlimited 13. SUPPLEMENTARY NOTES Journal of Astronomical Instrumentation 14. ABSTRACT 15. SUBJECT TERMS 16. SECURITY

Preface

NASA Astrophysics Data System (ADS)

Farmanyan, S. V.; Suvaryan, Yu. M.; Mickaelian, A. M.

2016-12-01

Cultural Astronomy is the reflection of sky events in various fields of nations' culture. In foreign literature, this field is also called "Astronomy in Culture" or "Astronomy and Culture". Cultural astronomy is the set of interdisciplinary fields studying the astronomical systems of current or ancient societies and cultures. It is manifested in Religion, Mythology, Folklore, Poetry, Art, Linguistics and other fields. During the past few decades interdisciplinary and multidisciplinary sciences have become the main incentive for the development of science. While studying astronomical topics in various areas of culture interesting discoveries have been occurred; such topics are widely used in folklore and other genres of literature, painting, architecture and music. Ancient astronomy, chronologies and calendars created on the basis of astronomical knowledge, Astrolinguistics and other fields play an important role in culture and national heritage. There are a number of organizations related to "Astronomy in Culture", appropriate specialists are being prepared, in this area conferences are being organized and papers are being published in professional and scientific-popular journals. Astronomy has also a leading role in scientific tourism, scientific journalism and in general science pularization and popular science dissemination, as well as social awareness and world perception. All these led to the idea of holding a Young Researchers conference with the subject on "Cultural Astronomy in Armenian Highland". Conference was held on June 20-23, 2016 in Armenian National Academy of Sciences. Among the participants there were astronomers, philosophers, historians, archeologists, specialists of literature, linguists, culturologists, experts in tourism and other fields. The opening session of the conference was attended by the president of NAS RA acad. Radik Martirosyan, NAS RA Academician-secretary of the Department of Armenology and Social Sciences acad. Yuri Suvaryan, ambassadors of foreign countries in Armenia, Presidents of RA Creative Unions, scientists, young researchers and journalists. The last sessions of the conference were held in the "Metsamor" Historical-Archeological Museum-Reserve, Art academy of Byurakan and Byurakan Astrophysical Observatory. The meeting is focused on Armenian archaeoastronomy and cultural astronomy, including many creations related to astronomical knowledge; calendars, rock art, mythology, etc. On the other hand, this subject is rather poorly developed in Armenia; there are only individual studies on various related issues (especially many studies related to Anania Shirakatsi) but not coordinated actions to manage this important field of investigation. The meeting is aimed at the development of problems of interdisciplinary sciences in Armenia and preparation of a basis for further possible collaborations by means of presentations of available modern knowledge in various areas of culture by experts from different professions and by joint discussions. A number of thematic sessions were held: Cultural Astronomy, Archaeoastronomy, Scientific Tourism & Scientific Journalism, Astronomical Education & Amauter Astronomy, Invited and contributed talks were presented by reknown and young researchers. The present Proceedings includes most of the talks. We hope that the Proceedings will be an interesting and valuable resource for many professionals and broad mass of readers.

Gender-Based Content of Educational Materials for the Study of Serbian Language in Lower-Stage Grades of Elementary Education

ERIC Educational Resources Information Center

Trifunovic, Vesna; Petrovic, Ruzica

2014-01-01

This paper presents the results of analysis of educational materials for the study of Serbian language in lower-stage grades of elementary education (intended for students from 7 through 11 years old) from gender perspective. The first part of the paper presents the process of institutionalization of gender-based education in the Republic of…

Public and Private Agri-Environmental Regulation in Post-Socialist Economies: Evidence from the Serbian Fresh Fruit and Vegetable Sector

ERIC Educational Resources Information Center

Gorton, Matthew; Zaric, Vlade; Lowe, Philip; Quarrie, Steve

2011-01-01

Using primary survey data and interview evidence this paper analyses the implementation and enforcement of public and private environmental regulation in the Serbian Fresh Fruit and Vegetable (FFV) sector. This provides a basis for engaging in a wider debate on the nature of agri-food regulation in post-socialist economies. Depictions of the…

Re-Codified Standards from the Perspective of Language Experts: Credentials, Practice and Attitudes Amongst Translators and Interpreters of the Bosnian, Croatian and Serbian Languages

ERIC Educational Resources Information Center

Hlavac, Jim

2015-01-01

This article examines aspects of linguistic behaviour, attitudes and professional practices amongst a group of 47 "expert users" who are translators or interpreters for one, two or three of the following languages: Bosnian, Croatian and Serbian. The official terms for these languages in the respective successor states of Socialist…

Cosmic Ink: Fragments from the Past on Journal Pages

NASA Astrophysics Data System (ADS)

Mandrino, A.; Gargano, M.; Gasperini, A.

2015-04-01

This contribution describes an editorial project started in 2012 to enhance the cultural heritage of the Italian observatories. It includes a regular column Cieli di inchiostro (Cosmic ink) devoted to promoting the astronomical historical archives and published in the Giornale di astronomia, a journal of the Società Astronomica Italiana. In every issue of the journal, a significant historical artifact is presented and described. This can be a letter, a diary page, a photograph, a map, a drawing, or another type of item pulled out of the archival folders to bring its history to light. The column is intended to invite historians, amateurs, and students to search and use the documents kept in the archives of the observatories.

Mitochondrial DNA perspective of Serbian genetic diversity.

PubMed

Davidovic, Slobodan; Malyarchuk, Boris; Aleksic, Jelena M; Derenko, Miroslava; Topalovic, Vladanka; Litvinov, Andrey; Stevanovic, Milena; Kovacevic-Grujicic, Natasa

2015-03-01

Although south-Slavic populations have been studied to date from various aspects, the population of Serbia, occupying the central part of the Balkan Peninsula, is still genetically understudied at least at the level of mitochondrial DNA (mtDNA) variation. We analyzed polymorphisms of the first and the second mtDNA hypervariable segments (HVS-I and HVS-II) and informative coding-region markers in 139 Serbians to shed more light on their mtDNA variability, and used available data on other Slavic and neighboring non-Slavic populations to assess their interrelations in a broader European context. The contemporary Serbian mtDNA profile is consistent with the general European maternal landscape having a substantial proportion of shared haplotypes with eastern, central, and southern European populations. Serbian population was characterized as an important link between easternmost and westernmost south-Slavic populations due to the observed lack of genetic differentiation with all other south-Slavic populations and its geographical positioning within the Balkan Peninsula. An increased heterogeneity of south Slavs, most likely mirroring turbulent demographic events within the Balkan Peninsula over time (i.e., frequent admixture and differential introgression of various gene pools), and a marked geographical stratification of Slavs to south-, east-, and west-Slavic groups, were also found. A phylogeographic analyses of 20 completely sequenced Serbian mitochondrial genomes revealed not only the presence of mtDNA lineages predominantly found within the Slavic gene pool (U4a2a*, U4a2a1, U4a2c, U4a2g, HV10), supporting a common Slavic origin, but also lineages that may have originated within the southern Europe (H5*, H5e1, H5a1v) and the Balkan Peninsula in particular (H6a2b and L2a1k). © 2014 Wiley Periodicals, Inc.

Astronomy Research Seminar

NASA Astrophysics Data System (ADS)

Johson, Jolyon; Genet, Russell; Armstrong, James; Boyce, Grady; Boyce, Pat; Brewer, Mark; Buchheim, Robert; Carro, Joseph; Estrada, Reed; Estrada, Chris; Freed, Rachel; Gillette, Sean; Harshaw, Richard; Hollis, Thomas; Kenney, John; McGaughey, Seven; McNab, Christine; Mohanan, Kakkala; Sepulveda, Babs; Wallace, Dan; Wallen, Vera

2015-05-01

Traditional science lectures and labs are often enhanced through project- and team-based learning. Some students go beyond these classroom studies by conducting research, often under the guidance of university professors. A one-semester astronomy research seminar was initiated in 2006 in collaboration with the community of professional and amateur double star astronomers. The result was dozens of jointly-authored papers published in the Journal of Double Star Observations and the Annual Proceedings of the Society of Astronomical Sciences. This seminar, and its affiliated community, launched a series of conferences and books, providing students with additional forums to share their double star research. The original seminar, and its derivatives, enhanced educational careers through college admissions and scholarships. To expand the seminar's reach, it was restructured from a few teams at one school, to many teams, each from a different school. A volunteer from each school became an assistant instructor. Most of them were seminar veterans, experienced astronomers, or science teachers. The assistant instructors, in turn, recruited enthusiastic students for their teams. To avoid student and instructor overload, the seminar focused on its three deliverables: a formal proposal, published paper, and public PowerPoint presentation. Future seminars may offer other astronomical research options such as exoplanet transit or eclipsing binary photometry.

Quasara: Ancient, Awesome Violence. Exploring the Universe.

ERIC Educational Resources Information Center

Harrington, Sherwood, Comp.

This information packet on quasars consists of an introductory paper, four articles from "Mercury," a journal of the Astronomical Society of the Pacific, and a bibliography. Methods used to measure distances in the universe and the nature of quasi-stellar objects (QSO's), the name preferred by many workers in the field, are discussed in…

The AAS Working Group on Accessibility and Disability (WGAD): Year 1 Highlights

NASA Astrophysics Data System (ADS)

Aarnio, Alicia; Monkiewicz, Jacqueline; Murphy, Nicholas Arnold; Nordhaus, Jason; Tuttle, Sarah E.

2017-01-01

The AAS Working Group on Accessibility and Disability (WGAD) was formed in January of 2016 with the express purpose of seeking equity of opportunity and building inclusive practices for disabled astronomers at all career stages. In our first year, the WGAD has been actively developing resources and the online infrastructure for the dissemination of information and engagement with the astronomy community. Our official WGAD website has gone live, and we have used both the access: astronomy google group and blog to discuss specific issues of disability justice and to raise awareness for less-discussed barriers to access. The WGAD has developed relationships and collaboration with AAS inclusion committees (SGMA, CSMA, CSWA) so our work can recognize and address the intersections of identity astronomers occupy. In this presentation, we summarize our year one activities, focusing on our recently developed set of recommendations for journal accessibility to ensure everyone can engage with journal content and navigate the submission process. We will also discuss ongoing and future endeavors: a best practices guide for accessibility to be available via our website, and a site visit program.

Psychometric Properties of the Serbian Version of the Maslach Burnout Inventory-Human Services Survey: A Validation Study among Anesthesiologists from Belgrade Teaching Hospitals

PubMed Central

Matejić, Bojana; Milenović, Miodrag; Kisić Tepavčević, Darija; Simić, Dušica; Pekmezović, Tatjana; Worley, Jody A.

2015-01-01

We report findings from a validation study of the translated and culturally adapted Serbian version of Maslach Burnout Inventory-Human Services Survey (MBI-HSS), for a sample of anesthesiologists working in the tertiary healthcare. The results showed the sufficient overall reliability (Cronbach's α = 0.72) of the scores (items 1–22). The results of Bartlett's test of sphericity (χ 2 = 1983.75, df = 231, p < 0.001) and Kaiser-Meyer-Olkin measure of sampling adequacy (0.866) provided solid justification for factor analysis. In order to increase sensitivity of this questionnaire, we performed unfitted factor analysis model (eigenvalue greater than 1) which enabled us to extract the most suitable factor structure for our study instrument. The exploratory factor analysis model revealed five factors with eigenvalues greater than 1.0, explaining 62.0% of cumulative variance. Velicer's MAP test has supported five-factor model with the smallest average squared correlation of 0,184. This study indicated that Serbian version of the MBI-HSS is a reliable and valid instrument to measure burnout among a population of anesthesiologists. Results confirmed strong psychometric characteristics of the study instrument, with recommendations for interpretation of two new factors that may be unique to the Serbian version of the MBI-HSS. PMID:26090517

Foreign scientists on the contribution of Serbian physician and scientist Dr. Lazar K. Lazarević to medical science.

PubMed

Draca, Sanja

2016-01-01

Dr. Lazar K. Lazarević (1851-1890, Julian calendar/1891, Gregorian calendar) was an exceptional Serbian physician, scientist, writer and translator. During his short life and his close to 11-year-long professional career (1879-1890), Dr. Lazarević authored 78 scientific papers and presentations in various branches of medicine. His greatest contribution to the field of neurology and to medical science in general is his description of the straight leg raising test.The article titled"Ischiac postica Cotunnii--One contribution to its differential diagnosis"was published in the Serbian language (in Cyrillic alphabet) in the Serbian Archives of Medicine in 1880.The article was translated to German and republished in Vienna in 1884 in Allgemeine Wiener medizinische Zeitung. The straight leg raising test is usually called Lasegue's test/sign, after the French clinician Charles Lasègue, although he never described it. However, there are numerous authors who admit that Lasègue never published the description of the straight leg raising test, and instead give full credits for its discovery to Dr. Lazarević. Our objective in this article is to highlight the major literature written by foreign scientists who give credit to Dr. Lazarević for his contribution to medical science.

Psychometric Properties of the Serbian Version of the Maslach Burnout Inventory-Human Services Survey: A Validation Study among Anesthesiologists from Belgrade Teaching Hospitals.

PubMed

Matejić, Bojana; Milenović, Miodrag; Kisić Tepavčević, Darija; Simić, Dušica; Pekmezović, Tatjana; Worley, Jody A

2015-01-01

We report findings from a validation study of the translated and culturally adapted Serbian version of Maslach Burnout Inventory-Human Services Survey (MBI-HSS), for a sample of anesthesiologists working in the tertiary healthcare. The results showed the sufficient overall reliability (Cronbach's α = 0.72) of the scores (items 1-22). The results of Bartlett's test of sphericity (χ(2) = 1983.75, df = 231, p < 0.001) and Kaiser-Meyer-Olkin measure of sampling adequacy (0.866) provided solid justification for factor analysis. In order to increase sensitivity of this questionnaire, we performed unfitted factor analysis model (eigenvalue greater than 1) which enabled us to extract the most suitable factor structure for our study instrument. The exploratory factor analysis model revealed five factors with eigenvalues greater than 1.0, explaining 62.0% of cumulative variance. Velicer's MAP test has supported five-factor model with the smallest average squared correlation of 0,184. This study indicated that Serbian version of the MBI-HSS is a reliable and valid instrument to measure burnout among a population of anesthesiologists. Results confirmed strong psychometric characteristics of the study instrument, with recommendations for interpretation of two new factors that may be unique to the Serbian version of the MBI-HSS.

Classification System and Information Services in the Library of SAO RAS

NASA Astrophysics Data System (ADS)

Shvedova, G. S.

The classification system used at SAO RAS is described. It includes both special determinants from UDC (Universal Decimal Classification) and newer tables with astronomical terms from the Library-Bibliographical Classification (LBC). The classification tables are continually modified, and new astronomical terms are introduced. At the present time the information services of the scientists is fulfilled with the help of the Abstract Journal Astronomy, Astronomy and Astrophysics Abstracts, catalogues and card indexes of the library. Based on our classification system and The Astronomy Thesaurus completed by R.M. Shobbrook and R.R. Shobbrook the development of a database for the library has been started, which allows prompt service of the observatory's staff members.

Long-publishing Astronomers, or the Problem of Classification

NASA Astrophysics Data System (ADS)

Tenn, Joseph S.

2012-01-01

In response to several discussions among astronomers and historians of astronomy, I started out to prepare a paper on long-publishing astronomers--those who published for 70, 75, or even 80 years. However, I soon ran into a number of questions of classification, and that turned out to be at least as interesting. How do we decide on classifications? Every time we choose classes, such as asteroids, planets and stars, we run into objects that seem to be in between. In the present case a number of questions arise: Who is an astronomer? Several of those with the longest publication runs started out as physicists, published for years in that subject only, and later took up astrophysics, eventually publishing a few (or even no) papers in astronomy journals. What is a publication? Should we count publications in physics, chemistry, or mathematics? What about philosophy of science or history of science? What about the elderly retired astronomer presenting a memoir of his or her own work? Abstracts of oral presentations? Textbooks? Monographs? Book reviews? Obituaries? Then there is the problem of posthumous publications. Probably most would include papers in the pipeline when the astronomer dies, but what about the case where the coauthor finally publishes the paper eight years after the death of the person of interest? I eventually decided to make two lists, one which would include most of the above, and one restricted to papers that make contributions to physical science. Note that I do not say "refereed,” as that presents its own problems, especially when applied to periods before the twentieth century.

Catalog of infrared observations. Part 1: Data

NASA Technical Reports Server (NTRS)

Gezari, Daniel Y.; Schmitz, Marion; Mead, Jaylee M.

1987-01-01

The Catalog of Infrared Observations (CIO) is a compilation of infrared astronomical observational data obtained from an extensive literature search of astronomical journals and major astronomical catalogs and surveys. The literature searches are complete for 1965 through 1986 in this Second Edition. The Catalog is published in two parts, with the observational data (roughly 200,000 observations of 20,000 individual sources) listed in Part I, and supporting appendices in Part II. The expanded Second Edition contains a new feature: complete IRAS 4-band data for all CIO sources detected, listed with the main Catalog observations, as well as in complete detail in the Appendix. The appendices include an atlas of infrared source positions, two bibliographies of infrared literature upon which the search was based, and, keyed to the main Catalog listings (organized alphabetically by author and then chronologically), an atlas of infrared spectral ranges, and IRAS data from the CIO sources. The complete CIO database is available to qualified users in printed microfiche and magnetic tape formats.

Professional Ethics for Astronomers

NASA Astrophysics Data System (ADS)

Marvel, K. B.

2005-05-01

There is a growing recognition that professional ethics is an important topic for all professional scientists, especially physical scientists. Situations at the National Laboratories have dramatically proven this point. Professional ethics is usually only considered important for the health sciences and the legal and medical professions. However, certain aspects of the day to day work of professional astronomers can be impacted by ethical issues. Examples include refereeing scientific papers, serving on grant panels or telescope allocation committees, submitting grant proposals, providing proper references in publications, proposals or talks and even writing recommendation letters for job candidates or serving on search committees. This session will feature several speakers on a variety of topics and provide time for questions and answers from the audience. Confirmed speakers include: Kate Kirby, Director Institute for Theoretical Atomic and Molecular Physics - Professional Ethics in the Physical Sciences: An Overview Rob Kennicutt, Astrophysical Journal Editor - Ethical Issues for Publishing Astronomers Peggy Fischer, Office of the NSF Inspector General - Professional Ethics from the NSF Inspector General's Point of View

Letter from the Editor

NASA Astrophysics Data System (ADS)

Strassmeier, Klaus G.

2009-01-01

As of 2007, Astronomische Nachrichten -- Astronomical Notes has reached its all-time high regarding the ISI journal impact factor, with an impressive increase of 60% compared to 2005. We now rank at 1,461, as shown in the statistics below. This is solely due to the increased quality of the published articles: In 2006, Astronomische Nachrichten -- Astronomical Notes published 208 research papers and received 1,033 citations -- five citations per paper on average. In 2007, we have published 177 research papers with roughly the same number of citations. In co-operation with Wiley InterScience we have achieved an average online publication time of just 4.5 months. We hope that the year 2008 will be comparably prosperous. As in the past, publication in Astronomische Nachrichten -- Astronomical Notes continues to be free of charge. Also, all articles of the first issue of each volume can be downloaded free of charge, as can all articles labelled ``Editor's Choice'', which are additionally featured with a color image on the front cover.

Letter from the Editor

NASA Astrophysics Data System (ADS)

Strassmeier, Klaus G.

2008-01-01

As of 2006, Astronomische Nachrichten -- Astronomical Notes has reached its all-time high regarding the ISI journal impact factor, with an impressive increase of 60% compared to 2005. We now rank at position 1,399, as shown in the statistics below. This is solely due to the increased number and quality of published articles: In 2006, Astronomische Nachrichten -- Astronomical Notes published 208 research papers and received 1,033 citations -- five citations per paper on average. In 2007, we have published 177 research papers, and one may be curious to see how their factor will develop. In co-operation with Wiley InterScience we have achieved an average o nline publication time of just 4.5 months. As in the past, publication in Astronomische Nachrichten -- Astronomical Notes} continues to be free of charge. Also, all articles of the first issue of each volume can be downloaded free of charge, as can all articles labelled ``Editor's Choice'', which are additionally featured with a color image on the front cover.

Astronomical Methods in Aerial Navigation

NASA Technical Reports Server (NTRS)

Beij, K Hilding

1925-01-01

The astronomical method of determining position is universally used in marine navigation and may also be of service in aerial navigation. The practical application of the method, however, must be modified and adapted to conform to the requirements of aviation. Much of this work of adaptation has already been accomplished, but being scattered through various technical journals in a number of languages, is not readily available. This report is for the purpose of collecting under one cover such previous work as appears to be of value to the aerial navigator, comparing instruments and methods, indicating the best practice, and suggesting future developments. The various methods of determining position and their application and value are outlined, and a brief resume of the theory of the astronomical method is given. Observation instruments are described in detail. A complete discussion of the reduction of observations follows, including a rapid method of finding position from the altitudes of two stars. Maps and map cases are briefly considered. A bibliography of the subject is appended.

The Development of Astronomy and Emergence of Astrophysics in Japan

NASA Astrophysics Data System (ADS)

Nakamura, Tsuko

This chapter overviews the emergence and development phases of modern astronomy and astrophysics in Japan, mainly before WWII. In the beginning of the nineteenth century under the samurai regime of the Tokugawa Shogunate, shogunal astronomers started to learn Western astronomy through a Dutch translation of the book Astronomie by J.J. Lalande. After the Meiji Restoration (1868) the new government founded the University of Tokyo (1877), the first modern university in Japan, in which Tokyo Astronomical Observatory (TAO) also started in 1888. Terao Hisashi, who had gone to Paris to study the modern astronomy, became the first Director of TAO in 1888. The astronomy introduced by Terao into Japan was so-called classical astronomy. Two of Terao's early students made Japan's first internationally recognized achievements in astronomy, the discovery of the Z-term in the polar motion of the Earth by Kimura (Astronomische Nachrichten, 158, 234-240, 1902) and the discovery of asteroid families by Hirayama (Astronomical Journal, 31, 185-188, 1918).

The Children's Dermatology Life Quality Index (CDLQI): linguistic and cultural validation in Serbian.

PubMed

Janković, Slavenka; Vukićević, Jelica; Djordjević, Sanja; Janković, Janko; Marinković, Jelena; Erić, Miloš

2013-01-01

The Children's Dermatology Life Quality Index (CDLQI) evaluates the impact of skin diseases on the patient's quality of life. The purpose of the study was to translate and to validate the CDLQI into Serbian. The CDLQI was translated into Serbian following international recommendations for translation and cultural adaptation. The validation study was carried out on a large cohort of secondary schoolchildren who self-reported acne. Translating the CDLQI consisted of forward translation, reconciliation, back translation, back-translation review, and cognitive debriefing. The good internal consistency of the scale was demonstrated with a Cronbach alpha coefficient of 0.87. A Spearman correlation coefficient of 0.66 between the CDLQI and the Cardiff Acne Disability Index (CADI) was deemed satisfactory to demonstrate concurrent validity. The translation, cross-cultural adaptation, and psychometric qualities of the CDLQI were satisfactory, enabling its application in clinical practice and future studies.

Association between methylenetetrahydrofolate reductase polymorphism C677T and risk of chronic myeloid leukemia in Serbian population.

PubMed

Jakovljevic, Ksenija; Malisic, Emina; Cavic, Milena; Radulovic, Sinisa; Jankovic, Radmila

2012-07-01

Methylenetetrahydrofolate reductase (MTHFR) is a key enzyme regulating the intracellular folate metabolism which plays an important role in carcinogenesis through DNA methylation and nucleotide synthesis. The common MTHFR single nucleotide polymorphism C677T has been reported to be associated with reduced enzymatic activity. In order to investigate the influence of this polymorphism on the risk of chronic myeloid leukemia (CML), we performed a case-control study in a Serbian population of 52 patients with CML and 53 healthy control subjects. MTHFR C677T polymorphism genotyping was assessed using the polymerase chain reaction-restriction fragment length polymorphism (PCR-RFLP) method. The results demonstrated no statistical difference in MTHFR 677 frequency distribution between patient and control groups. Our findings suggest that MTHFR 677 gene variants have no significant influence on the susceptibility to CML in a Serbian population.

Mining injuries in Serbian underground coal mines -- a 10-year study.

PubMed

Stojadinović, Saša; Svrkota, Igor; Petrović, Dejan; Denić, Miodrag; Pantović, Radoje; Milić, Vitomir

2012-12-01

Mining, especially underground coal mining, has always been a dangerous occupation. Injuries, unfortunately, even those resulting in death, are one of the major occupational risks that all miners live with. Despite the fact that all workers are aware of the risk, efforts must be and are being made to increase the safety of mines. Injury monitoring and data analysis can provide us with valuable data on the causes of accidents and enable us to establish a correlation between the conditions in the work environment and the number of injuries, which can further lead to proper preventive measures. This article presents the data on the injuries in Serbian coal mines during a 10-year period (2000-2009). The presented results are only part of an ongoing study whose aim is to assess the safety conditions in Serbian coal mines and classify them according to that assessment. Copyright © 2011 Elsevier Ltd. All rights reserved.

Concentrations of selected trace elements in mineral and spring bottled waters on the Serbian market.

PubMed

Ristić, M; Popović, I; Pocajt, V; Antanasijević, D; Perić-Grujić, A

2011-01-01

Eight selected trace elements, which are generally included in regulations, were analyzed in 23 types of bottled waters. Ten mineral and seven spring bottled waters were from the Serbian market and six mineral bottled waters were obtained in different EU countries. For the purpose of comparison, selected tap waters were also analyzed. Inductively coupled plasma mass spectrometry (ICP-MS) was used for the analysis of trace elements (arsenic, cadmium, copper, manganese, nickel, lead and antimony). Results were compared with the Serbian regulations for bottled water, EU regulations and guideline values set by the World Health Organization for drinking water. With few exceptions, the trace element levels of most bottled waters were below the guideline values. However, a higher content of antimony was observed in waters from polyethylene terephthalate (PET) containers, indicating a potential leaching of this element from the plastic packaging.

The NASA Astrophysics Data System: Overview

NASA Astrophysics Data System (ADS)

Kurtz, Michael J.; Eichhorn, Guenther; Accomazzi, Alberto; Grant, Carolyn S.; Murray, Stephen S.; Watson, Joyce M.

2000-04-01

The NASA Astrophysics Data System Abstract Service has become a key component of astronomical research. It provides bibliographic information daily, or near daily, to a majority of astronomical researchers worldwide. We describe the history of the development of the system and its current status. Urania (Boyce 1996), and the ADS role in the emerging electronic astronomical data environment are discussed. Astronomy is unique in that it already has a fully functional data resource, where several of the most important data sources exist on-line and inter-operate nearly seamlessly. The ADS and the Strasbourg Data Center (CDS; Genova et~al. 2000) form the core of this resource. We show several examples of how to use the ADS, and we show how ADS use has increased as a function of time. Currently it is still increasing exponentially, with a doubling time for number of queries of 17 months. Using the ADS logs we make the first detailed model of how scientific journals are read as a function of time since publication. We find four distinct components. We directly compare the readership rate with the citation rate for scientific articles as a function of age. Citations generally follow reads, but there are some differences. The main journals of astronomy have differences in the ways they are read and cited. We discuss these from a number of different aspects. The impact of the ADS on astronomy can be calculated after making some simple assumptions. We find that the ADS increases the efficiency of astronomical research by 333 Full Time Equivalent (2000 hour) research years per year, and that the value of the early development of the ADS for astronomy, compared with waiting for mature technologies to be adopted, is 2332 FTE research years. A full technical description of the ADS is in three companion articles: \\cite{gei}, \\cite{aa}, and \\cite{csg}. The ADS is available at http://adsabs.harvard.edu/.

A New Planet in our Solar System? NASA Takes a Look

NASA Image and Video Library

2016-01-20

NASA’s Director of Planetary Science, Jim Green, discusses the Jan. 20, 2016 Astronomical Journal science paper that points to the possibility of a new “Planet 9” in our solar system beyond Pluto, examining the scientific process and inviting you to have a front row seat to our exploration of the solar system.

Flammarion, Nicolas Camille (1842-1925)

NASA Astrophysics Data System (ADS)

Murdin, P.

2000-11-01

French astronomer and geophysicist, born in Montigny-le-Roy, observed double stars, and planets from his observatory at Juvisy, south of Paris. Very well-known for his popularization of astronomy, including many lavishly illustrated books (for example L'Astronomie Populaire) and a journal L'Astronomie, still published. It was Flammarion who, as shown by Arthur Beer and Bruno Weber, drew, sometime...

[Development of pharmacy in the Leskovac region for the period from liberation from the Turks until World War II].

PubMed

Milić, Petar; Milić, Slavica

2013-01-01

From the historical point of view, there are three time periods when the process of modernization of Serbian society took place. First period includes the interval from the beginning of the 19th century until the end of World War I, when the Serbian country was reestablished as Serbian Knezevina (princedom) and in 1882 as Serbian Kingdom. Second period includes an interval from the unity of Serbia into the Kingdom of Serbs, Croatians and Slovenians, which was established at the end of World War I (1918) and in 1929 changed the name into the Kingdom of Yugoslavia, which lasted until the end of World War II. The third period includes time after World War II. In this paper, the social-economical conditions in the Leskovac area during the first two periods of modernization were described, as well as the pharmacy development emphasizing the characteristic of the pharmaceutics. The Leskovac area belongs to most recently liberated areas in Serbia, i.e. Leskovac was liberated at the end of 1877. Nevertheless, the first pharmacy was opened in Leskovac in 1862, during the reign of the Turks. The authors being the people from Leskovac as well as the pharmacists believe that they contributed to better overview of the activities of people from modernization period, paying them well-deserved recognition.

Natural radionuclides in cigarette tobacco from Serbian market and effective dose estimate from smoke inhalation.

PubMed

Janković Mandić, Ljiljana; Đolić, Maja; Marković, Dragana; Todorović, Dragana; Onjia, Antonije; Dragović, Snežana

2016-01-01

The activity concentrations of natural radionuclides ((40)K, (210)Pb, (210)Po, (226)Ra and (228)Ra) in 17 most frequently used cigarette brands in Serbia and corresponding effective doses due to smoke inhalation are presented. The mean annual effective doses for (210)Pb and (210)Po were estimated to be 47.3 and 724 µSv y(-1) for (210)Pb and (210)Po, respectively. Serbia currently has the highest smoking rate in the world. The results of this study indicate the high contribution of the annual effective dose due to smoke inhalation to the total inhalation dose from natural radionuclides. The more effective implementation of actions for reducing smoking prevalence in Serbia is highly needed. © The Author 2015. Published by Oxford University Press. All rights reserved. For Permissions, please email: journals.permissions@oup.com.

Navigating from Publications to Astronomical Databases

NASA Astrophysics Data System (ADS)

Ochsenbein, François; Bertout, Claude; Lequeux, James; Genova, Françoise

The implementation of journals on the Web has opened new possibilities for the scientific usage of published results because it is now possible to link published articles to other types of information. The availability of published information in electronic form also allows for new types of content validation, complementary to the referee's validation, and to the layout performed by the publisher. For several years now, authors publishing in A&A are offered the possibility of quoting the astronomical objects they are studying directly in their latex manuscript (via the object macro). Since April 2001, this macro is being translated into an actual link from the article to the SIMBAD database. This experiment is still a prototype, and its various aspects are presented here.

The AAS Working Group on Accessibility and Disability (WGAD)

NASA Astrophysics Data System (ADS)

Monkiewicz, Jacqueline A.; Shanahan, J.; Murphy, Nicholas Arnold; Gilbert, Lauren

2016-06-01

The Working Group on Accessibility and Disability (WGAD) was formed by the Council of the American Astronomical Society in late 2015 in order to monitor and addresses issues of inclusivity in the astronomical community related to disability. WGAD promotes of the principles of universal accessibility and disability justice in both professional astronomy and astronomy education. The short term goals of WGAD for the next two years include producing a set of guidelines for a wide range of activities including supporting improved access to journals, data, and conferences. We will provide information and training regarding universal design as a guiding principle. The longer term goals of WGAD include integrating universal design as primary design strategy across the board in our many aspects of daily work life.

The Work of John Isaac Plummer at Orwell Park Observatory in the years 1874 to 1890

NASA Astrophysics Data System (ADS)

Whiting, P. J.

2006-12-01

This paper builds on the unpublished collation by the Orwell Astronomical Society entitled John Isaac Plummer. It takes the form of a chronology and critique of papers published by John Isaac Plummer (1844-1925) in the Monthly Notices of the Royal Astronomical Society and Astronomische Nachrichten on work undertaken at the Orwell Park Observatory, Ipswich, in the years 1874 to 1890. This work, mainly, although not exclusively, in England, took the form of measuring the positions and deriving the orbits of as many comets as could be observed from Orwell Park. Plummer also published papers in other journals, such as Nature and The Observatory, but these are to be the subject of future research.

SMC 1 or What's in a Name?

NASA Astrophysics Data System (ADS)

Dickel, H. R.

What's in a name? everything! SMC 1 is a planetary nebula in the Large Magellanic Cloud! This new planetary nebula near the LMC was noted by Savage, Murdin and Clark (in The Observatory 1982); it is also known as SMP LMC 104A (Sanduleak, MacConnell, and Philip in PASP 1978). In an effort to promote clear and unambiguous identification of all astronomical objects outside the solar system, the IAU Task Group on Designations attempts to clarify existing astronomical designations and the TG reviews, updates, and advertises the IAU Recommendations for Nomenclature. The following documents on the Web are provided as a service to astronomers to help them with designating astronomical sources of radiation outside the solar system: How to refer to a source or designate a new one: instructions IAU Recommendations for Nomenclature: nomenclature Second Reference Dictionary of Nomenclature of Celestial Objects: dictionary **NEW** (pre-)Registry of New Acronyms: acronym registry The Task Group in collaboration with several editors of astronomical journals and managers of large data archives is now studying the feasibility of an automated system to detect nonconforming designations when an article and/or survey data are submitted for publication and/or to an electronic archive. H. Dickel is available during the Symposium to discuss your designation concerns and to offer possible solutions.

Comets, Minor Planets and other developments: Bode's ``Astronomisches Jahrbuch'' as an international archive journal

NASA Astrophysics Data System (ADS)

Kokott, W.

Following the example of the Connaissance des tem(p)s, the Astronomisches Jahrbuch founded by the Royal Academy of Sciences at Berlin was to include ``a collection of the most recent observations, news, remarks and contributions''. Established by J. H. Lambert and for four decades edited by J. E. Bode, this publication from the start became a ranking international publication, with Bode's modest Berlin Observatory serving as a clearinghouse of informations When, in 1792, the backlog of manuscripts became a critical factor, a series of ``Supplement'' volumes was established. F. X. von Zach at Gotha, who vigorously supported this effort, founded (in 1798) the monthly Allgemeine Geographische Ephemeriden, which he (with continuing emphasis on astronomy and astronomical geography) two years later replaced by the Monatliche Correspondenz. These journals and its successors (ZfA and Corr. astr.) took the supplementary load off Bode's yearbook and served as speedier means of communication. However, the yearbook retained its original role as a central place of documentation. Only with the publication of Schumacher's Astronomische Nachrichten the center of astronomical communication did shift Practically all European astronomers of his time and age are represented in the pages of Bode's yearbook. Beside the continuous effort of precise mapping the realm of fixed stars, a very important field were the newly discovered planets Uranus, Ceres, Pallas, Juno, and Vesta; observations and orbits of these objects and the growing number of comets were an important part of the ``news and remarks'' recorded in the BAJ. The names of Schröter, Olbers, Piazzi, and Bessel may be regarded as representative for many

AstroDAbis: Annotations and Cross-Matches for Remote Catalogues

NASA Astrophysics Data System (ADS)

Gray, N.; Mann, R. G.; Morris, D.; Holliman, M.; Noddle, K.

2012-09-01

Astronomers are good at sharing data, but poorer at sharing knowledge. Almost all astronomical data ends up in open archives, and access to these is being simplified by the development of the global Virtual Observatory (VO). This is a great advance, but the fundamental problem remains that these archives contain only basic observational data, whereas all the astrophysical interpretation of that data — which source is a quasar, which a low-mass star, and which an image artefact — is contained in journal papers, with very little linkage back from the literature to the original data archives. It is therefore currently impossible for an astronomer to pose a query like “give me all sources in this data archive that have been identified as quasars” and this limits the effective exploitation of these archives, as the user of an archive has no direct means of taking advantage of the knowledge derived by its previous users. The AstroDAbis service aims to address this, in a prototype service enabling astronomers to record annotations and cross-identifications in the AstroDAbis service, annotating objects in other catalogues. We have deployed two interfaces to the annotations, namely one astronomy-specific one using the TAP protocol (Dowler et al. 2011), and a second exploiting generic Linked Open Data (LOD) and RDF techniques.

Astronomical publications of Melbourne Observatory

NASA Astrophysics Data System (ADS)

Andropoulos, Jenny Ioanna

2014-05-01

During the second half of the 19th century and the first half of the 20th century, four well-equipped government observatories were maintained in Australia - in Melbourne, Sydney, Adelaide and Perth. These institutions conducted astronomical observations, often in the course of providing a local time service, and they also collected and collated meteorological data. As well, some of these observatories were involved at times in geodetic surveying, geomagnetic recording, gravity measurements, seismology, tide recording and physical standards, so the term "observatory" was being used in a rather broad sense! Despite the international renown that once applied to Williamstown and Melbourne Observatories, relatively little has been written by modern-day scholars about astronomical activities at these observatories. This research is intended to rectify this situation to some extent by gathering, cataloguing and analysing the published astronomical output of the two Observatories to see what contributions they made to science and society. It also compares their contributions with those of Sydney, Adelaide and Perth Observatories. Overall, Williamstown and Melbourne Observatories produced a prodigious amount of material on astronomy in scientific and technical journals, in reports and in newspapers. The other observatories more or less did likewise, so no observatory of those studied markedly outperformed the others in the long term, especially when account is taken of their relative resourcing in staff and equipment.

Open Access: "à consommer avec modération"

NASA Astrophysics Data System (ADS)

Mahoney, Terence J.

There is increasing pressure on academics and researchers to publish the results of their investigations in open access journals. Indeed, some funding agencies make open access publishing a basic requirement for funding projects, and the EU is considering taking firm steps in this direction. I argue that astronomy is already one of the most open of disciplines, and that access - both to the general public (in terms of a significantly growing outreach effort) and to developing countries (through efforts to provide computing facilities and Internet access, as well as schemes to provide research centres of limited resources with journals) - is becoming more and more open in a genuine and lasting way. I further argue that sudden switches to more formal kinds of open access schemes could cause irreparable harm to astronomical publishing. Several of the most prestigious astronomical research journals (e.g. MN, ApJ, AJ) have for more than a century met the publishing needs of the research community and continue to adapt successfully to changing demands on the part of that community. The after-effects of abrupt changes in publishing practices - implemented through primarily political concerns - are hard to predict and could be severely damaging. I conclude that open access, in its current acceptation, should be studied with great care and with sufficient time before any consideration is given to its implementation. If forced on the publishing and research communities, open access could well result in much more limited access to properly vetted research results.

Burnout Syndrome Among Medical Students at One University in Serbia: Validity and Reliability of the Maslach Burnout Inventory-Student Survey.

PubMed

Ilic, Milena; Todorovic, Zeljko; Jovanovic, Milena; Ilic, Irena

2017-01-01

The Maslach Burnout Inventory-Student Survey (MBI-SS) contains 15 items that evaluate the following burnout dimensions: Emotional Exhaustion, Cynicism, and Academic Efficacy. The purpose of this study was to evaluate the dimensionality of the MBI-SS on a sample of Serbian medical students (N = 760). The overall Cronbach's α coefficient of the MBI-SS questionnaire was 0.757, while the Cronbach's α coefficients for Emotional Exhaustion, Cynicism, and Academic Efficacy were 0.869, 0.856, and 0.852, respectively. Principal Component Analysis with Oblimin rotation indicated 3 main components that explained 64.9% variance. The confirmatory factor analysis revealed good fit indices (χ 2 /df = 575.74/87, RMSEA = 0.086 (90% Confidence Interval for RMSEA = 0.079 to 0.092), CFI = 0.949, NNFI = 0.939, IFI = 0.949, GFI = 0.904) of the MBI-SS scale. The Serbian version of MBI-SS represents a valid and reliable instrument in the Serbian sample of medical students.

Measuring positive and negative affect and physiological hyperarousal among Serbian youth.

PubMed

Stevanovic, Dejan; Laurent, Jeff; Lakic, Aneta

2013-01-01

This study extended previous cross-cultural work regarding the tripartite model of anxiety and depression by developing Serbian translations of the Positive and Negative Affect Scale for Children (PANAS-C), the Physiological Hyperarousal Scale for Children (PH-C), and the Affect and Arousal Scale (AFARS). Characteristics of the scales were examined using 449 students (M age = 12.61 years). Applying item retention criteria established in other studies, PH-C, PANAS-C, and AFARS translations with psychometric properties similar to English-language versions were identified. Preliminary validation of the scales was conducted using a subset of 194 students (M age = 12.37 years) who also completed measures of anxiety and depression. Estimates of reliability, patterns of correlations among scales, and age and gender differences were consistent with previous studies with English-speaking samples. Findings regarding scale validity were mixed, although consistent with existing literature. Serbian translations of the PH-C, PANAS-C, and AFARS mirror the original English-language scales in terms of both strengths and weaknesses.

Cross-cultural Measurement Equivalence of the KINDL Questionnaire for Quality of Life Assessment in Children and Adolescents.

PubMed

Jafari, Peyman; Stevanovic, Dejan; Bagheri, Zahra

2016-04-01

This cross-cultural study aimed to assess whether Iranian and Serbian children, and also their parents, perceived the meaning of the items in the KINDL quality of life questionnaire consistently. The sample included 1086 Iranian and 756 Serbian children and adolescents, alongside 1061 and 618 of their parents, respectively. The ordinal logistic regression was used to assess differential item functioning (DIF) of the self and proxy-reports of the two versions of the KINDL, including Kid-KINDL and Kiddo-KINDL, across Iranian and Serbian samples. Statistically significant DIF was flagged for 14 out of 24 (58%) and 20 out of 24 (83%) items in the self-report of the Kid-KINDL and Kiddo-KINDL, respectively. Moreover, 20 out of 24 (83%) in the proxy reports of the both Kid-KINDL and Kiddo-KINDL, showed DIF across two samples. Accordingly, considerable caution is warranted when using the KINDL for cross-cultural comparisons.

Work Engagement in Serbia: Psychometric Properties of the Serbian Version of the Utrecht Work Engagement Scale (UWES)

PubMed Central

Petrović, Ivana B.; Vukelić, Milica; Čizmić, Svetlana

2017-01-01

Work engagement is defined as a positive, affective-motivational state of work-related well-being characterized by vigor, dedication and absorption. The Utrecht Work Engagement Scale (UWES) is the most frequently used measure of work engagement. The aim of this study was to analyze the psychometric properties of the Serbian versions of the UWES-17 and UWES-9. The sample consisted of 860 employees from a number of organizations and jobs across Serbia. Based on the UWES-17 findings, the data confirm both the three-factor and one-factor solutions by giving a slight advantage to the three-factor solution. As for the UWES-9, based on the PCFA and CFA, the one-factor solution was obtained as the preferred one. Taking into account the UWES-9 reliability and correlation patterns of its subscales with other well-being variables, both one- and three-factor solutions of the UWES-9 are suggested for future research. Serbian versions of both the UWES-17 and UWES-9 have satisfactory psychometric properties with high reliability, factorial structure in line with the theoretical model, and good predictive validity. The study contributes to enhanced understanding of work engagement by offering an insight from the Serbian cultural and economic context, significantly different from the UWES originating setting. There is still a need for exploring how employees from Serbia conceptualize work engagement, as well as for further, more stringent investigating of the cultural invariance of the UWES factorial structure. PMID:29085319

Alpha-1-Antitrypsin Deficiency in Serbian Adults with Lung Diseases

PubMed Central

Stankovic, Marija; Divac-Rankov, Aleksandra; Petrovic-Stanojevic, Natasa; Mitic-Milikic, Marija; Nagorni-Obradovic, Ljudmila; Radojkovic, Dragica

2012-01-01

Aim: Alpha-1-antitrypsin (A1AT) is the main inhibitor of neutrophil elastase, and severe alpha-1-antitrypsin deficiency (A1ATD) is a genetic risk factor for early-onset emphysema. Despite the relatively high prevalence of A1ATD, this condition is frequently underdiagnosed. Our aim was to determine the distribution of the A1ATD phenotypes/alleles in patients with lung diseases as well as in the Serbian population. Methods: The study included the adults with chronic obstructive pulmonary disease (COPD) (n=348), asthma (n=71), and bronchiectasis (n=35); the control was 1435 healthy blood donors. The A1ATD variants were identified by isoelectric focusing or polymerase chain reaction-mediated site-directed mutagenesis. Results: PiMZ heterozygotes, PiZZ homozygotes, and Z allele carriers are associated with significantly higher risk of developing COPD than healthy individuals (odds ratios 3.43, 42.42, and 5.49 respectively). The calculated prevalence of PiZZ, PiMZ, and PiSZ was higher in patients with COPD (1:202, 1:8, and 1:1243) than in the Serbian population (1:5519, 1:38, and 1:5519). Conclusion: The high prevalence of A1ATD phenotypes/allele in our population has confirmed the necessity of screening for A1ATD in patients with COPD. On the other hand, on the basis of the estimated number of those with A1ATD among the COPD patients, it is possible to assess the diagnostic efficiency of A1ATD in the Serbian population. PMID:22971141

Serbian medical students' fertility awareness and attitudes towards future parenthood.

PubMed

Vujčić, Isidora; Radičević, Tijana; Dubljanin, Eleonora; Maksimović, Nataša; Grujičić, Sandra

2017-08-01

Medical students represent a group particularly at risk of involuntary childlessness due to their highly demanding careers and university curriculum. The aim of this study was to investigate Serbian medical students' attitudes towards future parenthood and their awareness of fertility issues. A cross-sectional study was conducted among fourth year students at the Faculty of Medicine, University of Belgrade, Serbia, between 12 and 16 December 2016. Data were collected through an anonymous 56-item validated questionnaire, translated into the Serbian language. The participation rate was 87.1%. More than 95% of students, regardless of gender, wanted to have children in the future; most indicated three as the desired number of children. Both genders equally rated the importance of having children. Women rated significantly higher the likelihood of IVF treatment or child adoption if faced with infertility (both p = .001). All students wanted to have their first child before the age of 35 years. Knowledge about the age-related decline in female fertility was not satisfactory. Women found it more important to have children when they felt sufficiently mature, were in a stable relationship, were financially secure, had completed their studies, were not too old to have children, and had access to childcare, although these prerequisites were rated highly by both genders. Serbian medical students greatly value and have a positive perception of future parenthood. Appropriate education is needed, however, because of their inadequate knowledge of the age-related decline in female fertility.

Possible Collaboration Perspectives in Astronomy Education

NASA Astrophysics Data System (ADS)

Nuritdinov, Salakhutdin

It is a question of international educational collaboration in the frame of IAU Commission 46. As astronomers are graduated by some Universities it will be useful joint discussion of collaboration perspectives: 1. Taking into account that in countries of former Soviet Union training Bachelors and Masters is began it is desirable working out consistent educational curriculums. 2. Consistent curriculums of the Bachelor must have about 60-70% identical special courses and other part of courses can depend on traditional directions of that country. The curriculums give a possibility to continue study for example to enter Master of other country. 3. In the frame of IAU Commission 46 creation of united international virtual library of astronomy textbooks is important for our students. Where there is training astronomers it is necessary the access of students to all textbooks and some scientific journals. 4. It is desirable to organize summer and winter scientific schools for students in the frame of the Commission yearly. Unfortunately we did not receive an announcement about it though only our University in Central Asia trains astronomers. Other proposals will be given in the report

Mt. Wilson in 1910: The Year of The Great Solar Convention.

NASA Astrophysics Data System (ADS)

Welther, B. L.

2004-12-01

In 1910 the meetings of the Astronomical and Astrophysical Society of America (= AAS) and of the International Union for the Co-ordination of Solar Research (= ISU) were arranged so that astronomers from many countries first met in Cambridge, MA for the AAS from August 17-19, then spent eleven days sight-seeing as they traveled from the East Coast to the West Coast, and finally met again in Pasadena, CA for the ISU from August 31-September 6. Formal notes for these meetings were published widely in such journals as Nature, The Observatory, Popular Astronomy, Science, and The Transactions of the ISU. In addition to those records for the three-week span, newspaper reporters published numerous articles, astronomers kept personal diaries, and amateur photographers took many candid photographs of their peers enjoying informal moments. Fortunately, some of the newspaper clippings, notebooks and picture albums ended up in observatory archives. This paper will present some of the highlights of the meetings and travels as recorded both formally and informally by H. D. Babcock, J. S. Plaskett, E. C. Pickering, F. Schlesinger, H. H. Turner and others.

A Journal of travel of an astrophysicist

NASA Astrophysics Data System (ADS)

Gaina, Alex B.

2015-06-01

The authors is descibing personal impressions from a number of scientific conferences took between 1993 and 1998 in Trieste (ICTP,with the participation of 2 Nobel Laureats Winners: Professor Abdus Salam (1926-1996) and Professor Gert t'Hooft), Catania astrophysical Observatory and University (1995-JENAM 1995), Athens Observatory and University (1996-Wide Field Spectroscopy), Prague Technicke Museum (1996- Symposium "Mysterium Cosmographicum"),Prague technical University (1998 -JENAM 1998),which in fact contained also a trip to Nicolaus Copernicus Astronomical Center in Torun (Poland). Besides,some details on trips through Ukraine, Poland, Serbia, where a kind meeting with astronomers from Belgrade took place in 1995, former Yugoslav Countries: Monetnegro, Slovenija and Croatia, Bulgaria, where another meeting with physicists from the Academy of Sciences of Bulgaria took place has been given also.

"Women in Astronomy: an Essay Review"

NASA Astrophysics Data System (ADS)

Cox, M.

2006-12-01

Interest in the history of women in astronomy has increased dramatically in the last 30 years. This interest has come from the growing number of professional scientists, historians and feminists researching the lives and work of earlier generations, as well as from amateur astronomers. It is reflected in the vast amount of literature on the subject, both in books and journals, and on the internet. This Essay Review will focus on monographs published in the last 10 years (1996-2006), and will be restricted mainly to pre-20th century women. The scope includes researchers, translators, computers and astronomical assistants as well as observers. Where appropriate, it includes books that discuss the role of women scientists, as well as pure astronomy books. Part 2, to be published later, will consider encyclopaedias and large works of reference .

[Lifetime achievements of Dragan M. Dugalić. 1934-1992].

PubMed

Stevović, Dragoslav M

2002-09-01

Dragan M. Dugalitsh was born on 2nd August 1934 in Stari Trg in Kosovo in a working family. He finished the elementary school in his birthplace and the secondary school in Kosovska Mitrovica. He entered the University School of Medicine in Belgrade in 1954 and finished the studies in 1961 as one of the best students in his generation (average mark 9.22). During the studies D. Dugalitsh was very active in the students' organization, especially in professional and sport activities. He was educator first at the Chair of Chemistry and later at the Chair of Physiology. He was member of the Yugoslav Communist Party since 1954. He participated in three federal work drives. After having done the internship and national service he began to work at the Institute of Physiology of the University School of Medicine in Belgrade. However, in 1963 he changed the Institute for the First Department of Surgery managed by professor Ljubomir Rashovitsh. In 1968 he passed the examination in general surgery with excellent mark and in 1969 he was elected assistant lecturer at the Department of Surgery. His doctor's thesis was entitled "Experimental transplantation of lungs in dogs". Then, he was elected senior lecturer in 1975, associate professor in 1980 and professor of surgery in 1985. At the Department of Surgery he passed through all professional grades, from clinical physician and head of a ward to director of the Department of Surgery (1988-1992). He was also secretary of the Chair of Surgery (1984-1987) and associate dean of the University School of Medicine in Belgrade. Several times he received advanced training abroad. D. Dugalitsh was the visiting lecturer and surgeon in many towns in former Yugoslavia. He was member of many national and international surgical associations (SIC/ICC, CICD) and member of editorial boards of domestic and foreign medical journals (ACI, SA, AGEH). He was very active in the Serbian Medical Society, especially in the Section of surgery where he was also general secretary. He was rewarded by the Serbian Medical Society several times. In 1985 he was awarded the "Vishnjevski Medal" by the Moskow Vishnjevski Institute. In 1988 he became member of the Academy of Medical Sciences of the Serbian Medical Society. D. Dugalitsh was a workaholic, altruistic and self-denial person, especially devoted to an ill person. He was very respected by his colleagues and collaborators. He died on 3rd December 1992.

Fallen star legends and traditional religion of Japan: an aspect of star lore

NASA Astrophysics Data System (ADS)

Goto, Akira

2015-08-01

Japanese star lore is a complex mixture of animism, Buddhism, Shinto-ism, Confucianism and folk beliefs. Although some studies have been done on rituals concerning constellation developed in esoteric Buddhism (e.g. Journal Culture and Cosmos, Vol. 10 no 1 and 2), studies on other aspects of Japanese star lore are limited, in particular, to the English audience.In historic literatures, there often mentioned abnormal astronomical phenomena, such as, eclipse, meteors and comets. In this paper, I will discuss the possibility of reference to these astronomical phenomena in order to talk about some historical facts.In western part of Japan, there are Shinto shrines and Buddhistic temples that are said to be built as monuments of fallen stars. Usually fallen stars were divided into three, and a trio of shrines/temples are said to be the remnants of this phenomenon. Similar legends are found in Kudamatsu (that means "fallen pine=pine where stars fallen") of Yamaguchi Prefecture, Bisei-cho (that means "beautiful star") of Okayama Prefecture, Hoshida (that means "rice field or village of star") shrine of Osaka, and also Hoshida shrine of Nagoya.The purpose of this presentation is not to argue whether fallen star legend was truly astronomical phenomenon, such as, meteor or not. Instead, I will discuss why similar legends have been talked concerning the origin of particular shrines or temples. Citing Eliade who related gorge and alchemy producing spark to astronomical phenomena, I will disclose the possibility to relate these astronomical legends to the coming of the naturalized Japanese from Korean Peninsula who introducd forge to Japan abound 5 to 6 centuries.

ADF/ADC Web Tools for Browsing and Visualizing Astronomical Catalogs and NASA Astrophysics Mission Metadata

NASA Astrophysics Data System (ADS)

Shaya, E.; Kargatis, V.; Blackwell, J.; Borne, K.; White, R. A.; Cheung, C.

1998-05-01

Several new web based services have been introduced this year by the Astrophysics Data Facility (ADF) at the NASA Goddard Space Flight Center. IMPReSS is a graphical interface to astrophysics databases that presents the user with the footprints of observations of space-based missions. It also aids astronomers in retrieving these data by sending requests to distributed data archives. The VIEWER is a reader of ADC astronomical catalogs and journal tables that allows subsetting of catalogs by column choices and range selection and provides database-like search capability within each table. With it, the user can easily find the table data most appropriate for their purposes and then download either the subset table or the original table. CATSEYE is a tool that plots output tables from the VIEWER (and soon AMASE), making exploring the datasets fast and easy. Having completed the basic functionality of these systems, we are enhancing the site to provide advanced functionality. These will include: market basket storage of tables and records of VIEWER output for IMPReSS and AstroBrowse queries, non-HTML table responses to AstroBrowse type queries, general column arithmetic, modularity to allow entrance into the sequence of web pages at any point, histogram plots, navigable maps, and overplotting of catalog objects on mission footprint maps. When completed, the ADF/ADC web facilities will provide astronomical tabled data and mission retrieval information in several hyperlinked environments geared for users at any level, from the school student to the typical astronomer to the expert datamining tools at state-of-the-art data centers.

Matters arising from ``The Leonid meteor shower and the history of the Semites''Letter - Matters arising from ``The Leonid meteor shower and the history of the Semites''

NASA Astrophysics Data System (ADS)

McBeath, A.

2009-10-01

Aspects of a paper by Suleyman (2009) in this journal, relating to theoretically-strong Leonid activity in 569 AD and 1226 BC possibly having been recorded in the Quran and Bible respectively, are discussed. Little reason is found to suppose either textual source referred to such astronomical events.

The E-volution of Preprints in the Scholarly Communication of Physicists and Astronomers.

ERIC Educational Resources Information Center

Brown, Cecelia

2001-01-01

To learn how e-prints are cited, used, and accepted in the literature of physics and astronomy, the philosophies, policies, and practices of approximately 50 top-tier physics and astronomy journals regarding e-prints from the Los Alamos e-print archive were examined. Results provide a sense of the current impact of the evolution of e-prints on the…

Critical Issues in the Philosophy of Astronomy and Cosmology

NASA Astrophysics Data System (ADS)

Dick, Steven J.

2016-01-01

Although the philosophy of science and of specific sciences such as physics, chemistry, and biology are well-developed fields with their own books and journals, the philosophy of astronomy and cosmology have received little systematic attention. At least six categories of problems may be identified in the astronomical context: 1) the nature of reasoning, including the roles of observation, theory, simulation, and analogy, as well as the limits of reasoning, starkly evident in the anthropic principle, fine-tuning, and multiverse controversies; 2) the often problematic nature of evidence and inference, especially since the objects of astronomical interest are for the most part beyond experiment and experience;3) the influence of metaphysical preconceptions and non-scientific worldviews on astronomy, evidenced, for example in the work of Arthur S. Eddington and many other astronomers; 4) the epistemological status of astronomy and its central concepts, including the process of discovery, the problems of classification, and the pitfalls of definition (as in planets); 5) the role of technology in shaping the discipline of astronomy and our view of the universe; and 6) the mutual interactions of astronomy and cosmology with society over time. Discussion of these issues should draw heavily on the history of astronomy as well as current research, and may reveal an evolution in approaches, techniques, and goals, perhaps with policy relevance. This endeavor should also utilize and synergize approaches and results from philosophy of science and of related sciences such as physics (e.g. discussions on the nature of space and time). Philosophers, historians and scientists should join this new endeavor. A Journal of the Philosophy of Astronomy and Cosmology (JPAC) could help focus attention on their studies.

Identifying the Functional Requirements for an Arizona Astronomy Data Hub (AADH)

NASA Astrophysics Data System (ADS)

Stahlman, G.; Heidorn, P. B.

2015-12-01

Astronomy data represent a curation challenge for information managers, as well as for astronomers. Extracting knowledge from these heterogeneous and complex datasets is particularly complicated and requires both interdisciplinary and domain expertise to accomplish true curation, with an overall goal of facilitating reproducible science through discoverability and persistence. A group of researchers and professional staff at the University of Arizona held several meetings during the spring of 2015 about astronomy data and the role of the university in curation of that data. The group decided that it was critical to obtain a broader consensus on the needs of the community. With assistance from a Start for Success grant provided by the University of Arizona Office of Research and Discovery and funding from the American Astronomical Society (AAS), a workshop was held in early July 2015, with 28 participants plus 4 organizers in attendance. Representing University researchers as well as astronomical facilities and a scholarly society, the group verified that indeed there is a problem with the long-term curation of some astronomical data not associated with major facilities, and that a repository or "data hub" with the correct functionality could facilitate research and the preservation and use of astronomy data. The workshop members also identified a set of next steps, including the identification of possible data and metadata to be included in the Hub. The participants further helped to identify additional information that must be gathered before construction of the AADH could begin, including identifying significant datasets that do not currently have sufficient preservation and dissemination infrastructure, as well as some data associated with journal publications and the broader context of the data beyond that directly published in the journals. Workshop participants recommended that a set of grant proposal should be developed that ensures community buy-in and participation. The project should be developed in an agile, incremental manner that will allow consistent community growth from the early stages of the project, building on existing iPlant infrastructure (www.iplantcollaborative.org) initially developed for the biology community.

Work related characteristics, work-home and home-work interference and burnout among primary healthcare physicians: a gender perspective in a Serbian context.

PubMed

Putnik, Katarina; Houkes, Inge

2011-09-23

Little information exists on work and stress related health of medical doctors in non-EU countries. Filling this knowledge gap is needed to uncover the needs of this target population and to provide information on comparability of health related phenomena such as burnout across countries. This study examined work related characteristics, work-home and home-work interference and burnout among Serbian primary healthcare physicians (PHPs) and compared burnout levels with other medical doctors in EU countries. Data were collected via surveys which contained Maslach Burnout Inventory and other validated instruments measuring work and home related characteristics. The sample consisted of 373 PHPs working in 12 primary healthcare centres. Data were analysed using t-tests and Chi square tests. No gender differences were detected on mean scores of variables among Serbian physicians, who experience high levels of personal accomplishment, workload, job control and social support, medium to high levels of emotional exhaustion, medium levels of depersonalisation and work-home interference, and low levels of home-work interference. There were more women than men who experienced low job control and high depersonalisation. Serbian physicians experienced significantly higher emotional exhaustion and lower depersonalisation than physicians in some other European countries. To diminish excessive workload, the number of physicians working in primary healthcare centres in Serbia should be increased. Considering that differences between countries were detected on all burnout subcomponents, work-related interventions for employees should be country specific. The role of gender needs to be closely examined in future studies as well.

Blood donors’ positivity for transfusion-transmissible infections: the Serbian Military Medical Academy experience

PubMed Central

Vučetić, Dušan; Kecman, Gorica; Ilić, Vesna; Balint, Bela

2015-01-01

Background Members of armed forces worldwide are considered to be very susceptible to sexually transmitted infections, thus falling into a high-risk group of blood donors regarding transfusion-transmissible infections. In the Serbian Military Medical Academy a significant number (44% for the period 2005–2013) of blood donations were from members of the Serbian Army. The aim of this study was to determine the significance of military blood donors for the safety of blood transfusion. Material and methods Between January 2005 and December 2013, a total of 155,479 blood donations were tested for hepatitis B virus (HBV), hepatitis C virus (HCV), human immunodeficiency virus (HIV) and syphilis using serological assays (enzyme immunoassays, chemiluminescent microparticle immunoassay and western blot) and molecular testing (polymerase chain reaction analysis). Results The percentage of blood donations positive for transfusion-transmissible infections in the estimated period was 0.38%, and the percentage of HBV, HCV, HIV and syphilis positive blood donations was 0.20%, 0.12%, 0.005% and 0.06%, respectively. During that period, the percentage of all transfusion-transmissible infections, and in particular of HBV and HCV, declined significantly. In contrast, the percentage of HIV and syphilis positive blood donations remained unchanged. Higher rates of positivity for transfusion-transmissible infections in blood donations from members of the Serbian Army were not found, especially after mandatory military service was abolished in 2009. Discussion The reported rate of positivity for transfusion-transmissible infections in blood donations from the Military Medical Academy was considered low. This information is of great significance for further implementation of public health measures. PMID:26057495

Rules vs. Statistics: Insights from a Highly Inflected Language

PubMed Central

Mirković, Jelena; Seidenberg, Mark S.; Joanisse, Marc F.

2011-01-01

Inflectional morphology has been taken as a paradigmatic example of rule-governed grammatical knowledge (Pinker, 1999). The plausibility of this claim may be related to the fact that it is mainly based on studies of English, which has a very simple inflectional system. We examined the representation of inflectional morphology in Serbian, which encodes number, gender and case for nouns. Linguists standardly characterize this system as a complex set of rules, with disagreements about their exact form. We present analyses of a large corpus of nouns which showed that, as in English, Serbian inflectional morphology is quasiregular: it exhibits numerous partial regularities creating neighborhoods that vary in size and consistency. We then asked whether a simple connectionist network could encode this statistical information in a manner that also supported generalization. A network trained on 3,244 Serbian nouns learned to produce correctly inflected phonological forms from a specification of a word’s lemma, gender, number and case, and generalized to untrained cases. The model’s performance was sensitive to variables that also influence human performance, including surface and lemma frequency. It was also influenced by inflectional neighborhood size, a novel measure of the consistency of meaning to form mapping. A word naming experiment with native Serbian speakers showed that this measure also affects human performance. The results suggest that, as in English, generating correctly inflected forms involves satisfying a small number of simultaneous probabilistic constraints relating form and meaning. Thus, common computational mechanisms may govern the representation and use of inflectional information across typologically diverse languages. PMID:21564267

Authentic Astronomy Research Experiences for Teachers: the NASA/IPAC Teacher Archive Research Program (NITARP)

NASA Astrophysics Data System (ADS)

Rebull, L.; NITARP Team

2011-12-01

Since 2004, we have provided authentic astronomy research experiences for teachers using professional astronomical data. (The program used to be called the Spitzer Teacher Program for Teachers and Students, and in 2009 was renamed NITARP--NASA/IPAC Teacher Archive Research Program.) We partner small groups of teachers with a mentor astronomer, the team does research, writes up a poster, and presents it at the major annual meeting for professional US astronomers, the American Astronomical Society (winter meeting). The teachers incorporate this research experience into their classroom, and their experiences color their teaching for years to come, influencing hundreds of students per teacher. This program, to the best of our knowledge, is completely unique in the following three ways: (1) Each team does original research using real astronomical data, not canned labs or reproductions of previously done research. (2) Each team writes up the results of their research and presents it at an AAS meeting. Each team also presents the educational results of their experience. (3) The 'products' of the program are primarily the scientific results, as opposed to curriculum packets. The teachers in the program involve students at their school and incorporate the experience into their teaching in a way that works for them, their environment, and their local/state standards. The educators in the program are selected from a nationwide annual application process, and they get three trips, all reasonable expenses paid. First, they attend a winter AAS meeting to get their bearings as attendees of the largest professional astronomy meetings in the world. We sponsor a kickoff workshop specifically for the NITARP educators on the day before the AAS meeting starts. After the meeting, they work remotely with their team to write a proposal, as well as read background literature. In the summer (at a time convenient to all team members), the educators plus up to two students per teacher come out to visit Caltech for 3-4 days and get started on their project in earnest. They return home and continue to work through the Fall, finish their research, and write their AAS abstracts and posters in preparation for the winter AAS. The educators plus up to two students per teacher then attend the AAS and present their results. Each team presents one science poster and at least one education poster. The science posters are intermingled in science sessions, and must "hold their own" next to other professional astronomer posters. Each teacher finally serves as NASA/NITARP ambassadors in their community, giving at least 12 hours' worth of professional development. Since the original Spitzer program in 2004, news coverage associated with any of these projects has reached more than 6 million people, largely in home-town newspapers from the teachers' cities. More than 200 presentations have been given, reaching over 14,000 people. More than 120 students have traveled for NITARP, and more than 1200 students have used real astronomical data through this program. Almost 60 educators have been trained in real research. Nearly 50 science or education posters have been presented. Four refereed journal articles (in major astronomical journals) have come out of work associated with these teams.

Lack of association between ESR1 gene polymorphisms and premature ovarian failure in Serbian women.

PubMed

Li, J; Vujovic, S; Dalgleish, R; Thompson, J; Dragojevic-Dikic, S; Al-Azzawi, F

2014-06-01

It has previously been reported that estrogen receptor-alpha (ERα) gene (ESR1: estrogen receptor 1) polymorphisms are associated with premature ovarian failure (POF). The aim of this study was to investigate whether these genetic polymorphisms of ESR1 are associated with POF in Serbian women. A series of 197 POF cases matched with 547 fertile controls was recruited by the Institute for Endocrinology, Diabetes and Metabolic Disorders of Serbia between 2007 and 2010. Genomic DNA was extracted from saliva using Oragene® DNA sample collection kits. Two single-nucleotide polymorphisms (SNPs), PvuII and XbaI, in ESR1 were genotyped by dynamic allele-specific hybridization. Haplotype analyses were performed with the restriction fragment length polymorphism method. SNP and haplotype effects were analyzed by logistic regression models. No significant difference was found in the distribution of ESR1 PvuII and XbaI polymorphisms or haplotypes between the POF and control groups. The two ESR1 SNPs, PvuII and XbaI, are not commonly associated with POF in Serbian women and may not contribute to the genetic basis of the condition.

Physicochemical properties of honey from Serbia in the period 2014-2016

NASA Astrophysics Data System (ADS)

Vranić, D.; Petronijević, R.; Đinović Stojanović, J.; Korićanac, V.; Babić Milijašević, J.; Milijašević, M.

2017-09-01

Honey is a viscous, aromatic, sweet food that is consumed and enjoyed by people around the world due to its unique nutritional and medicinal properties. The physicochemical parameters of natural honeys, such as moisture, reducing sugars, sucrose, hydroxymethylfurfural (HMF), free acidity, diastase activity, water-insoluble content and electrical conductivity are strictly defined and constitute the quality indicators which characterize individual honey varieties. The present study shows results of honey quality investigation from various regions of Serbia, which were evaluated according to the Serbian Regulation. A total of 372 honey samples (132 acacia honey, 221 blossom honey and 19 honeydew honey) were obtained from the Serbian market. All applied methods were performed according to the Harmonized Methods of the International Honey Commission. Summarizing the results presented, the most important parameters for detecting honey that was non-compliant with the regulation were HMF content along with diastase activity and sugar content. Results show that in 2014 and 2015, a great number of honey samples were of insufficient quality to satisfy regulatory requirements. In 2016, the situation on the Serbian honey market improved and became more under control.

STELAR: An experiment in the electronic distribution of astronomical literature

NASA Technical Reports Server (NTRS)

Warnock, A.; Vansteenburg, M. E.; Brotzman, L. E.; Gass, J.; Kovalsky, D.

1992-01-01

STELAR (Study of Electronic Literature for Astronomical Research) is a Goddard-based project designed to test methods of delivering technical literature in machine readable form. To that end, we have scanned a five year span of the ApJ, ApJ Supp, AJ and PASP, and have obtained abstracts for eight leading academic journals from NASA/STI CASI, which also makes these abstracts available through the NASA RECON system. We have also obtained machine readable versions of some journal volumes from the publishers, although in many instances, the final typeset versions are no longer available. The fundamental data object for the STELAR database is the article, a collection of items associated with a scientific paper - abstract, scanned pages (in a variety of formats), figures, OCR extractions, forward and backward references, errata and versions of the paper in various formats (e.g., TEX, SGML, PostScript, DVI). Articles are uniquely referenced in the database by journal name, volume number and page number. The selection and delivery of articles is accomplished through the WAIS (Wide Area Information Server) client/server models requiring only an Internet connection. Modest modifications to the server code have made it capable of delivering the multiple data types required by STELAR. WAIS is a platform independent and fully open multi-disciplinary delivery system, originally developed by Thinking Machines Corp. and made available free of charge. It is based on the ISO Z39.50 standard communications protocol. WAIS servers run under both UNIX and VMS. WAIS clients run on a wide variety of machines, from UNIX-based Xwindows systems to MS-DOS and macintosh microcomputers. The WAIS system includes full-test indexing and searching of documents, network interface and easy access to a variety of document viewers. ASCII versions of the CASI abstracts have been formatted for display and the full test of the abstracts has been indexed. The entire WAIS database of abstracts is now available for use by the astronomical community. Enhancements of the search and retrieval system are under investigation to include specialized searches (by reference, author or keyword, as opposed to full test searches), improved handling of word stems, improvements in relevancy criteria and other retrieval techniques, such as factor spaces. The STELAR project has been assisted by the full cooperation of the AAS, the ASP, the publishers of the academic journals, librarians from GSFC, NRAO and STScI, the Library of Congress, and the University of North Carolina at Chapel Hill.

Immanuel Halton, the astronomer

NASA Astrophysics Data System (ADS)

Barber, P. M.

1996-02-01

Immanuel Halton was born in Cumberland, studied at Grays Inn, London during the later stages of the English Civil War and, during the Commonwealth, entered the service of Henry Howard, later 6th Duke of Norfolk. He pursued his mathematical and astronomical interests while auditor to the Duke of Norfolk. He met with John Flamsteed, encouraged the latter's interest in mathematics and astronomy and became his first patron, as well as contributing observations to Flamsteed's published works. Immanuel ended his days at Wingfield Manor, Derbyshire. A short biographical piece on Immanuel Halton appeared in the Journal in the early 1950s, consisting mostly of quotations from Flamsteed's 'Self Inspections' and Baily's 'Life of Flamsteed'. 1996 is the 350th anniversary of Flamsteed's birth, and it is hoped that this fuller account will flesh out the bones of his first patron.

Monitoring process hygiene in Serbian retail establishments

NASA Astrophysics Data System (ADS)

Vesković Moračanin, S.; Baltić, T.; Milojević, L.

2017-09-01

The present study was conducted to estimate the effectiveness of sanitary procedures on food contact surfaces and food handlers’ hands in Serbian retail establishments. For that purpose, a total of 970 samples from food contact surfaces and 525 samples from workers’ hands were microbiologically analyzed. Results of total aerobic plate count and total Enterobacteriaceae count showed that the implemented washing and disinfection procedures, as a part of HACCP plans, were not effective enough in most retail facilities. Constant and intensive education of employees on proper implementation of sanitation procedures are needed in order to ensure food safety in the retail market.

When "the facts" become a text reinterpreting war with Serbian war veterans.

PubMed

Schlichte, Klaus

2014-01-01

Rationalist theories of political violence proclaim rather than show what motivates war participation. This article tries to examine the limits of reconstructions of these motivations by analyzing interview material gathered from Serbian war veterans. Using "grounded theory" as a methodology, this research has revealed that the identification of motivations has to take into account social and historical contexts that play out as life-worlds and world-views. Real decision points are, however, hard to identify. Therefore, the article suggests a stronger focus on "carriers" (Trägerschichten) for the study of conflict dynamics.

The Pisgah Astronomical Research Institute

NASA Astrophysics Data System (ADS)

Cline, J. Donald; Castelaz, M.

2009-01-01

Pisgah Astronomical Research Institute is a not-for-profit foundation located at a former NASA tracking station in the Pisgah National Forest in western North Carolina. PARI is celebrating its 10th year. During its ten years, PARI has developed and implemented innovative science education programs. The science education programs are hands-on experimentally based, mixing disciplines in astronomy, computer science, earth and atmospheric science, engineering, and multimedia. The basic tools for the educational programs include a 4.6-m radio telescope accessible via the Internet, a StarLab planetarium, the Astronomical Photographic Data Archive (APDA), a distributed computing online environment to classify stars called SCOPE, and remotely accessible optical telescopes. The PARI 200 acre campus has a 4.6-m, a 12-m and two 26-m radio telescopes, optical solar telescopes, a Polaris monitoring telescope, 0.4-m and 0.35-m optical research telescopes, and earth and atmospheric science instruments. PARI is also the home of APDA, a repository for astronomical photographic plate collections which will eventually be digitized and made available online. PARI has collaborated with visiting scientists who have developed their research with PARI telescopes and lab facilities. Current experiments include: the Dedicated Interferometer for Rapid Variability (Dennison et al. 2007, Astronomical and Astrophysical Transactions, 26, 557); the Plate Boundary Observatory operated by UNAVCO; the Clemson University Fabry-Perot Interferometers (Meriwether 2008, Journal of Geophysical Research, submitted) measuring high velocity winds and temperatures in the Thermosphere, and the Western Carolina University - PARI variable star program. Current status of the education and research programs and instruments will be presented. Also, development plans will be reviewed. Development plans include the greening of PARI with the installation of solar panels to power the optical telescopes, a new distance learning center, and enhancements to the atmospheric and earth science suite of instrumentation.

Astronomers Identify a New Mid-size Black Hole

NASA Image and Video Library

2017-12-08

Nearly all black holes come in one of two sizes: stellar mass black holes that weigh up to a few dozen times the mass of our sun or supermassive black holes ranging from a million to several billion times the sun’s mass. Astronomers believe that medium-sized black holes between these two extremes exist, but evidence has been hard to come by, with roughly a half-dozen candidates described so far. A team led by astronomers at the University of Maryland and NASA’s Goddard Space Flight Center has found evidence for a new intermediate-mass black hole about 5,000 times the mass of the sun. The discovery adds one more candidate to the list of potential medium-sized black holes, while strengthening the case that these objects do exist. The team reported its findings in the September 21, 2015 online edition of Astrophysical Journal Letters. This image, taken with the European Southern Observatory’s Very Large Telescope, shows the central region of galaxy NGC1313. This galaxy is home to the ultraluminous X-ray source NCG1313X-1, which astronomers have now determined to be an intermediate-mass black hole candidate. NGC1313 is 50,000 light-years across and lies about 14 million light-years from the Milky Way in the southern constellation Reticulum. Read more: www.nasa.gov/feature/goddard/astronomers-identify-a-new-m... Image credit: European Southern Observatory #nasagoddard #blackhole #space NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. Follow us on Twitter Like us on Facebook Find us on Instagram

The roles of the AAS Journals' Data Editors

NASA Astrophysics Data System (ADS)

Muench, August; NASA/SAO ADS, CERN/Zenodo.org, Harvard/CfA Wolbach Library

2018-01-01

I will summarize the community services provided by the AAS Journals' Data Editors to support authors’ when citing and preserving the software and data used in the published literature. In addition I will describe the life of a piece of code as it passes through the current workflows for software citation in astronomy. Using this “lifecycle” I will detail the ongoing work funded by a grant from the Alfred P. Sloan Foundation to the American Astronomical Society to improve the citation of software in the literature. The funded development team and advisory boards, made up of non-profit publishers, literature indexers, and preservation archives, is implementing the Force11 Software citation principles for astronomy Journals. The outcome of this work will be new workflows for authors and developers that fit in their current practices while enabling versioned citation of software and granular credit for its creators.

Results of Spectral Corona Observations in Solar Activity Cycles 17-24

NASA Astrophysics Data System (ADS)

Aliev, A. Kh.; Guseva, S. A.; Tlatov, A. G.

2017-12-01

The results of the work of the global observation network are considered, and a comparative analysis of the data of various coronal observatories is performed. The coronal activity index has been reconstructed for the period 1939-2016 based on the data of various observatories in Kislovodsk system. For this purpose, the corona daily intensity maps from the Sacramento Peak and Lomnický Štít observatories according to the Solar-Geophysical Data journal have been digitized; they supplement the data of other observatories. The homogeneity and continuity of the corona observations at the Kislovodsk station, including activity cycle 24, is confirmed. Unfortunately, the only observatory at present that continues observation of the spectral corona in Fe XIV 5303 Å and Fe XIV 6374 Å lines is the Kislovodsk astronomical station Mountain Astronomical Station (MAS) of the Central Astronomical Observatory, Russian Academy of Sciences (Pulkovo). The data on the combined corona in 5303 Å line are analyzed. It is shown that there is a high correlation of the intensity index of green corona with solar radiation measurements in the vacuum UV region. Data on the beginning of the new 25th activity cycle in the corona at high latitudes are presented.

Short-course Astronomical Research Seminars for High School and College Students

NASA Astrophysics Data System (ADS)

Johnson, Jolyon

2011-05-01

Since 2008, I have helped lead several short-course astronomical research seminars with Russell M. Genet. These seminars have ranged from semester-long courses at Cuesta College in San Luis Obispo, California to long weekends at the University of Oregon's Pine Mountain Observatory. Each seminar is led by an experienced observer or group of observers who guide high school and college students through the scientific process from observations to publication. The students (anywhere from half a dozen to twenty in number) participate in and contribute to every step. Being a coauthor on one or more research papers offers students an advantage on college and scholarship applications. Similarly, graduate schools often prefer students with research experience. Many topics of research are appropriate for these short-courses including variable star, exoplanet, and asteroid photometry. However, the most successful topic has been visual double stars because the observations required are straitforward and the equipment is relatively inexpensive. The Journal of Double Star Observations is also welcoming of student research and provides swift publication. A detailed description of the short-course seminars can be found in the recent Collins Foundation Press volume titled Small Telescopes and Astronomical Research.

Chinese records of the 1874 transit of Venus

NASA Astrophysics Data System (ADS)

Lu, Lingfeng; Li, Huifang

2013-03-01

Before the advent of radar, transits of Venus were very important for measuring the distance between the Earth and the Sun. A transit occurred in 1874, and was visible from China, other parts of east and southeast Asia and from India, Australia and New Zealand and certain islands in the Indian and Pacific Oceans. As a result, many astronomers from Western countries came to China to observe it. According to traditional Chinese astrology, the Sun represented the Emperor, and if the Sun was invaded by other astronomical bodies it meant that the Emperor and the country faced some ominous disaster. In the late nineteenth century, Western astronomical knowledge was widely translated into Chinese and spread among Chinese intellectuals, so the 1874 transit supposedly was easily understood by Chinese intellectuals. Before the transit took place, various Chinese publications introduced this kind of celestial event as science news, but at the same time other influential newspapers and journals discussed the astrological connection between the transit and the fortunes of the nation. In this paper we review these interesting Chinese records and discuss the different attitudes towards the transit exhibited by Chinese intellectuals and officials, during a period when Western learning was being widely disseminated throughout China.

Problems of the Modern Romanian Astronomy: TELEROM

NASA Astrophysics Data System (ADS)

Grigore, Valentin; Minti, Harry; Vaduvescu, Ovidiu

2011-06-01

The TV broadcast discusses problems of the modernization of the Romanian astronomical infrastructure, the worst in Eastern Europe. It presents the TELEROM project which proposed to establish a new EU-funded robotic 1,3 m telescope, a project finally rejected by the Astronomical Institute of the Romanian Academy mainly due to the incompetence of the director of this Institute, Dr. Vasile Mioc. It is mentioned that this was the second very promising project failed under the same director, after the project ASTEROS in value of 15 million Euro to establish two modern telescopes was also lost in the recent years. The total cost of the TELEROM project was 1,5 million Euro, according to the agreement with the EU foundation for Regional Development (director Hanns Ruder Institut für Theoretische Astrophysik, Universität Tübingen, Germany - the TELEROM auto-dimissed project director). The facilities from this implementation were very promising in observations of Solar system objects (asteroids, near Earth asteroids, comets), few hundred millions of faint stars, quasars, exoplanets and galaxies. Initially, the director Vasile Mioc and the governing body of the Romanian Astronomical Institute intended to place the telescope in Romania in very bad astroclimatic conditions, namely in the old Feleac observatory, very close to the very highly polluted and quite clouded city of Cluj-Napoca. Many opposite considerations (Dr. Marian Doru Suran from Bucharest, many Romanian astronomers from the Diaspora and a group of 68 astronomers, professors, public outreach people and students from Romania and Diaspora supporting TELEROM) were totally disregarded! Due to refuse to place the telescope in very good astroclimatic conditions (in Canary Islands or Chile) and also due to the impossibility to establish a decent national astronomical observatory in Romania by the direction of the Institute in agreement with the State body of Romania ("Academia Romana" and "Autoritatea Nationala pentru Cercetare") the TELEROM project was finally rejected and its funding was lost, after 10 months of discussions and granted funding! Other problems, such as the proliferation of the astrology between Romanian professional astronomers, a reduced weight of physicists between Romanian professional astronomers in comparison with mathematicians, as well as very reduced issue from the professional Romanian astronomers in international journals in the last years and the intellectual theft of publications have been also discussed in this 4 TV series presented by the weekly astronomy show "We and the Sky" of Columna TV (in Romanian).

EDITORIAL: The 15th Central European Workshop on Quantum Optics The 15th Central European Workshop on Quantum Optics

NASA Astrophysics Data System (ADS)

Bozic, Mirjana; Man'ko, Margarita; Arsenovic, Dusan

2009-07-01

The development of quantum optics was part and parcel of the formation of modern physics following the fundamental work of Max Planck and Albert Einstein, which gave rise to quantum mechanics. The possibility of working with pure quantum objects, like single atoms and single photons, has turned quantum optics into the main tool for testing the fundamentals of quantum physics. Thus, despite a long history, quantum optics nowadays remains an extremely important branch of physics. It represents a natural base for the development of advanced technologies, like quantum information processing and quantum computing. Previous Central European Workshops on Quantum Optics (CEWQO) took place in Palermo (2007), Vienna (2006), Ankara (2005), Trieste (2004), Rostock (2003), Szeged (2002), Prague (2001), Balatonfüred (2000), Olomouc (1999), Prague (1997), Budmerice (1995, 1996), Budapest (1994) and Bratislava (1993). Those meetings offered excellent opportunities for the exchange of knowledge and ideas between leading scientists and young researchers in quantum optics, foundations of quantum mechanics, cavity quantum electrodynamics, photonics, atom optics, condensed matter optics, and quantum informatics, etc. The collaborative spirit and tradition of CEWQO were a great inspiration and help to the Institute of Physics, Belgrade, and the Serbian Academy of Sciences and Arts, as the organizers of CEWQO 2008. The 16th CEWQO will take place in 2009 in Turku, Finland, and the 17th CEWQO will be organized in 2010 in St Andrews, United Kingdom. The 15th CEWQO was organized under the auspices and support of the Ministry of Science of the Republic of Serbia, the Serbian Physical Society, the European Physical Society with sponsorship from the University of Belgrade, the Central European Initiative, the FP6 Program of the European Commission under INCO project QUPOM No 026322, the FP7 Program of the European Commission under project NANOCHARM, Europhysics Letters (EPL), The European Physical Journal (EPJ), and John Wiley and Sons.

Armenian Cultural Astronomy

NASA Astrophysics Data System (ADS)

Farmanyan, S. V.; Mickaelian, A. M.

2015-07-01

Cultural Astronomy is the reflection of sky events in various fields of nations' culture. In foreign literature this field is also called "Astronomy in Culture" or "Astronomy and Culture". Cultural astronomy is the set of interdisciplinary fields studying the astronomical systems of current or ancient societies and cultures. It is manifested in Religion, Mythology, Folklore, Poetry, Art, Linguistics and other fields. In recent years, considerable attention has been paid to this sphere, particularly international organizations were established, conferences are held and journals are published. Armenia is also rich in cultural astronomy. The present paper focuses on Armenian archaeoastronomy and cultural astronomy, including many creations related to astronomical knowledge; calendars, rock art, mythology, etc. On the other hand, this subject is rather poorly developed in Armenia; there are only individual studies on various related issues (especially many studies related to Anania Shirakatsi) but not coordinated actions to manage this important field of investigation.

Cultural Astronomy in Armenia and in the World

NASA Astrophysics Data System (ADS)

Farmanyan, S. V.; Mickaelian, A. M.

2016-12-01

Cultural Astronomy is the reflection of sky events in various fields of nations' culture. In foreign literature, this field is also called "Astronomy in Culture" or "Astronomy and Culture". Cultural astronomy is the set of interdisciplinary fields studying the astronomical systems of current or ancient societies and cultures. It is manifested in Religion, Mythology, Folklore, Poetry, Art, Linguistics and other fields. In recent years, considerable attention has been paid to this sphere, particularly international organizations were established, conferences are held and journals are published. Armenia is also rich in cultural astronomy. The present paper focuses on Armenian archaeoastronomy and cultural astronomy, including many creations related to astronomical knowledge; calendars, rock art, mythology, etc. On the other hand, this subject is rather poorly developed in Armenia; there are only individual studies on various related issues (especially many studies related to Anania Shirakatsi) but not coordinated actions to manage this important field of investigation.

Romania before the International Year of Astronomy

NASA Astrophysics Data System (ADS)

Mosoia, Cătălin; Pica, Elisabeta Ana; Stavinschi, Magda

2008-09-01

100 years of astronomical research in Romania happen almost at 400 years after Galileo Galilei first looked at the sky with one of his instruments. However, there is a background that goes back in time further and makes specialists take into account that there is some kind of ``cosmic feeling'' throughout the Romanian culture. All contributes to a high level of public interest, be it students or general audience. In order to measure that we take into consideration the most important astronomical events organized at national level: Eclipse '99, Life in the Universe, Venus 2004, and EuroPlaNet. All experience gained at national level makes possible participation at international meetings and give a high impulse of rehabilitation of science journalism where CAP2007 is the most recent example. Our work takes into account also educational projects and what we have learnt for celebrating the upcoming International Year of Astronomy

Far infrared supplement. Third edition: Catalog of infrared observations (lambda greater than or equal to 4.6 micrometers)

NASA Technical Reports Server (NTRS)

Gezari, Daniel Y.; Schmitz, Marion; Pitts, Patricia S.; Mead, Jaylee M.

1993-01-01

The Far Infrared Supplement contains a subset of the data in the full Catalog of Infrared Observations (all observations at wavelengths greater than 4.6 microns). The Catalog of Infrared Observations (CIO), NASA RP-1294, is a compilation of infrared astronomical observational data obtained from an extensive literature search of scientific journals and major astronomical catalogs and surveys. The literature search is complete for years 1965 through 1990 in this third edition. The catalog contains about 210,000 observations of roughly 20,000 individual sources, and supporting appendices. The expanded third edition contains coded IRAS 4-band data for all CIO sources detected by IRAS. The appendices include an atlas of infrared source positions (also included in this volume), two bibliographies of catalog listings, and an atlas of infrared spectral ranges. The complete CIO database is available to qualified users in printed, microfiche, and magnetic tape formats.

Catalog of Infrared Observations, Third Edition

NASA Technical Reports Server (NTRS)

Gezari, Daniel Y.; Schmitz, Marion; Pitts, Patricia S.; Mead, Jaylee M.

1993-01-01

The Far Infrared Supplement contains a subset of the data in the full Catalog of Infrared Observations (all observations at wavelengths greater than 4.6 microns). The Catalog of Infrared Observations (CIO), NASA RP-1294, is a compilation of infrared astronomical observational data obtained from an extensive literature search of scientific journals and major astronomical catalogs and surveys. The literature search is complete for years 1965 through 1990 in this Third Edition. The Catalog contains about 210,000 observations of roughly 20,000 individual sources and supporting appendices. The expanded Third Edition contains coded IRAS 4-band data for all CIO sources detected by IRAS. The appendices include an atlas of infrared source positions (also included in this volume), two bibliographies of Catalog listings, and an atlas of infrared spectral ranges. The complete CIO database is available to qualified users in printed, microfiche, and magnetic-tape formats.

Trans fatty acid content in Serbian margarines: Urgent need for legislative changes and consumer information.

PubMed

Vučić, Vesna; Arsić, Aleksandra; Petrović, Snježana; Milanović, Sandra; Gurinović, Mirjana; Glibetić, Maria

2015-10-15

This study examined the fatty acid (FA) composition of 13 (7 soft and 6 hard) Serbian margarines. Significantly higher amounts of trans fatty acids (TFA) were found in hard margarines (up to 28.84% of total FA), than in soft ones (0.17-6.89%). Saturated FA (SFA) were present with 22.76-51.17%. Oleic acid ranged from 26.78% to 43.78%. The proportion of polyunsaturated FA (PUFA) was 22.15-49.29% in soft margarines, but only 8.02-15.28% in hard margarines, probably due to the hydrogenisation process. The atherogenic and thrombogenic indexes (AI and TI, respectively) in soft margarines were relatively low (AI 0.23-0.63 and TI 0.44-0.97), but in hard margarines AI and particularly TI were high (1.03-1.67 and 1.96-3.04, respectively). These findings suggest that FA composition of Serbian margarines should be improved by replacing atherogenic TFA and SFA with beneficial ones, in order to avoid adverse effects on health. Therefore legislative changes and consumer information are urgently needed. Copyright © 2015 Elsevier Ltd. All rights reserved.

The impact of an educational film on promoting knowledge and attitudes toward HIV in soldiers of the Serbian Armed Forces.

PubMed

Jadranin, Željko; Dedić, Gordana; Vaughan, Freda; Grillo, Michael P; Šuljagić, Vesna

2015-07-01

Millions of soldiers around the world represent one of the most vulnerable populations regarding exposure to human immunodeficiency virus (HIV) infection. The programs for HIV prevention remain the most viable approach to reducing the spread of HIV infection. Very few studies have tested the effectiveness of HIV preventive interventions undertaken in military population. The aim of this study was to determine the effectiveness of educational film to transfer knowledge about HIV infection to soldiers. We performed a quasi-experimental study among 102 soldiers of the Serbian Armed Forces. The experimental intervention consisted of the HIV knowledge pre-questionnaire, watching a film on HIV knowledge, then the post-HIV knowledge questionnaire. The results of pre- and post-HIV knowledge questionnaires were compared. There were 23 questions in the test. The average total score on the questionnaire before watching the film was 18.23 and after watching it was 20.14, which was statistically significant difference (p < 0.001). CONCLU- SIONS: The results of the study show that viewing a film on HIV infection is an effective method of transferring knowledge about HIV to the Serbian military population.

[Jubilees of the Serbian Medical Society. Golden jubilee--a time of renewal and remembrance].

PubMed

Vuković, Z

1998-01-01

The Serbian medical association was founded in Belgrade 125 years ago. At that time, Serbia was liberated from the Ottoman domination, and was one of some thirty existing independent states gaining international recognition in 1878. The physicians of the Serbian medical association have shared the fate of their people over the past 125 years. This is best illustrated by the fact that Serbia lost more than 1,000,000 people in World War I and that every third doctor in Serbia lost his life serving his people during the war. This was the highest expression of philanthropy, unsurpassed in the history of mankind. The period of time after the war, was the time of renewal and commemoration. In that time John Maynard Keynes, one of the most outstanding figures in the field of world economics, was on the Peace Conference in Paris, after the World War I, in charge of estimating war damages and the degree of destruction in the Allied countries, but without considering their losses in "human capital"-- the only exception he made for Serbia. In his book "The Economic Consequences of the Peace (published in 1920) he wrote: "The losses of Serbia, although from a human point of view her sufferings were the greatest of all, are not measured pecuniarily by great figures, on account of her low economic development." He quoted some extraordinary figures of the loss of life--"at above 1,000,000, or more than one-third of the population of Old Serbia." In the end he concludes: "Of all the Allies, Serbian sufferings and losses were proportionately the greatest, and after Serbian, the French. In these times, also, according to professor Hichmann (Geographical Statistical Atlas 1920) "it was found, when the nations counted their losses after the war, that Serb casualties amounted to 23% of her population as compared with 3.7% for Great Britain, 8.5% for France and 9.3% for Germany. No small nation can suffer a loss such as Serbia, drawn moreover entirely from its able-bodied manhood, without coming near the risk of extinction. Every single man who could be saved from the debacle strengthened the hope for the future.

Trends of Papers Published from 2006 TO 2010 IN Journals Nature and Science

NASA Astrophysics Data System (ADS)

Kim, Sang-Chul; Kim, Seung-Lee; Kyeong, Jae-Mann; Lee, Jae-Woo; Lim, Wang-Gi; Jeon, Sung-Hyun

2012-06-01

We present an analysis of the papers published in the journals Nature and Science in the years from 2006 to 2010. During this period, a total of 7788 papers were published in the two journals. This includes 544 astronomy papers that comprise 7.0% of the papers in `all' research fields and 18.9% of those in the fields of `physical sciences'. The sub-fields of research of the astronomy papers are distributed, in descending order of number of papers, in Solar System, stellar astronomy, galaxies and the universe, the Milky Way Galaxy, and exoplanets. The observational facilities used for the studies are mainly ground-based telescopes (31.1%), spacecrafts (27.0%), and space telescopes (22.8%), while 16.0% of papers did not use any noticeable facilities and 1.7% used other facilities. Korean scientists have published 86 papers (33 in Nature and 53 in Science), which is 1.10% of all the papers (N=7788) in the two journals. The share of papers by Korean astronomers among the scientific papers by Koreans is 8.14%, slightly higher than the contribution of astronomy papers (7.0%) in both journals.

Black Hole Blows Big Bubble

NASA Astrophysics Data System (ADS)

2010-07-01

Combining observations made with ESO's Very Large Telescope and NASA's Chandra X-ray telescope, astronomers have uncovered the most powerful pair of jets ever seen from a stellar black hole. This object, also known as a microquasar, blows a huge bubble of hot gas, 1000 light-years across, twice as large and tens of times more powerful than other known microquasars. The discovery is reported this week in the journal Nature. "We have been astonished by how much energy is injected into the gas by the black hole," says lead author Manfred Pakull. "This black hole is just a few solar masses, but is a real miniature version of the most powerful quasars and radio galaxies, which contain black holes with masses of a few million times that of the Sun." Black holes are known to release a prodigious amount of energy when they swallow matter. It was thought that most of the energy came out in the form of radiation, predominantly X-rays. However, the new findings show that some black holes can release at least as much energy, and perhaps much more, in the form of collimated jets of fast moving particles. The fast jets slam into the surrounding interstellar gas, heating it and triggering an expansion. The inflating bubble contains a mixture of hot gas and ultra-fast particles at different temperatures. Observations in several energy bands (optical, radio, X-rays) help astronomers calculate the total rate at which the black hole is heating its surroundings. The astronomers could observe the spots where the jets smash into the interstellar gas located around the black hole, and reveal that the bubble of hot gas is inflating at a speed of almost one million kilometres per hour. "The length of the jets in NGC 7793 is amazing, compared to the size of the black hole from which they are launched," says co-author Robert Soria [1]. "If the black hole were shrunk to the size of a soccer ball, each jet would extend from the Earth to beyond the orbit of Pluto." This research will help astronomers understand the similarity between small black holes formed from exploded stars and the supermassive black holes at the centres of galaxies. Very powerful jets have been seen from supermassive black holes, but are thought to be less frequent in the smaller microquasar variety. The new discovery suggests that many of them may simply have gone unnoticed so far. The gas-blowing black hole is located 12 million light-years away, in the outskirts of the spiral galaxy NGC 7793 (eso0914b). From the size and expansion velocity of the bubble the astronomers have found that the jet activity must have been ongoing for at least 200 000 years. Note: [1] Astronomers do not have yet any means of measuring the size of the black hole itself. The smallest stellar black hole discovered so far has a radius of about 15 km. An average stellar black hole of about 10 solar masses has a radius of about 30 km, while a "big" stellar black hole may have a radius of up to 300 km. This is still much smaller than the jets, which extend out to 1000 light-years, or about 9000 million million km! More Information: This result appears in a paper published in this week's issue of the journal Nature (A 300 parsec long jet-inflated bubble around a powerful microquasar in the galaxy NGC 7793, by Manfred W. Pakull, Roberto Soria and Christian Motch). ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organisation in Europe and the world's most productive astronomical observatory. It is supported by 14 countries: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world's most advanced visible-light astronomical observatory and VISTA, the world's largest survey telescope. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 42-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become "the world's biggest eye on the sky".

Black Hole Blows Big Bubble

NASA Astrophysics Data System (ADS)

2010-07-01

Combining observations made with ESO's Very Large Telescope and NASA's Chandra X-ray telescope, astronomers have uncovered the most powerful pair of jets ever seen from a stellar black hole. This object, also known as a microquasar, blows a huge bubble of hot gas, 1000 light-years across, twice as large and tens of times more powerful than other known microquasars. The discovery is reported this week in the journal Nature. "We have been astonished by how much energy is injected into the gas by the black hole," says lead author Manfred Pakull. "This black hole is just a few solar masses, but is a real miniature version of the most powerful quasars and radio galaxies, which contain black holes with masses of a few million times that of the Sun." Black holes are known to release a prodigious amount of energy when they swallow matter. It was thought that most of the energy came out in the form of radiation, predominantly X-rays. However, the new findings show that some black holes can release at least as much energy, and perhaps much more, in the form of collimated jets of fast moving particles. The fast jets slam into the surrounding interstellar gas, heating it and triggering an expansion. The inflating bubble contains a mixture of hot gas and ultra-fast particles at different temperatures. Observations in several energy bands (optical, radio, X-rays) help astronomers calculate the total rate at which the black hole is heating its surroundings. The astronomers could observe the spots where the jets smash into the interstellar gas located around the black hole, and reveal that the bubble of hot gas is inflating at a speed of almost one million kilometres per hour. "The length of the jets in NGC 7793 is amazing, compared to the size of the black hole from which they are launched," says co-author Robert Soria [1]. "If the black hole were shrunk to the size of a soccer ball, each jet would extend from the Earth to beyond the orbit of Pluto." This research will help astronomers understand the similarity between small black holes formed from exploded stars and the supermassive black holes at the centres of galaxies. Very powerful jets have been seen from supermassive black holes, but are thought to be less frequent in the smaller microquasar variety. The new discovery suggests that many of them may simply have gone unnoticed so far. The gas-blowing black hole is located 12 million light-years away, in the outskirts of the spiral galaxy NGC 7793 (eso0914b). From the size and expansion velocity of the bubble the astronomers have found that the jet activity must have been ongoing for at least 200 000 years. Notes [1] Astronomers do not have yet any means of measuring the size of the black hole itself. The smallest stellar black hole discovered so far has a radius of about 15 km. An average stellar black hole of about 10 solar masses has a radius of about 30 km, while a "big" stellar black hole may have a radius of up to 300 km. This is still much smaller than the jets, which extend out to several hundreds light years on each side of the black hole, or about several thousand million million km! More information This result appears in a paper published in this week's issue of the journal Nature (A 300 parsec long jet-inflated bubble around a powerful microquasar in the galaxy NGC 7793, by Manfred W. Pakull, Roberto Soria and Christian Motch). ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organisation in Europe and the world's most productive astronomical observatory. It is supported by 14 countries: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world's most advanced visible-light astronomical observatory and VISTA, the world's largest survey telescope. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 42-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become "the world's biggest eye on the sky".

Selection, Prioritization, and Characteristics of Kepler Target Stars

DTIC Science & Technology

2010-04-20

contributions from zodiacal emission as well as background stars): r = F∗ F∗ + Fbg . (5) The photometric aperture is defined as the set of pixels that... The Astrophysical Journal Letters, 713:L109–L114, 2010 April 20 doi:10.1088/2041-8205/713/2/L109 C© 2010. The American Astronomical Society. All...rights reserved. Printed in the U.S.A. SELECTION, PRIORITIZATION, AND CHARACTERISTICS OF KEPLER TARGET STARS Natalie M. Batalha1, William J. Borucki2

Preservice elementary teachers learning of astronomy

NASA Astrophysics Data System (ADS)

Fidler, Chuck Gary

The dissertation presents a new approach for the study of preservice elementary teacher astronomy education. The approach suggests that learning astronomical concepts are facilitated by greater sophistication in scale perception and spatial-aptitude. This dissertation is underscored by the national call for elementary science education reform efforts and suggests certain strategies shown more effective for the development of accurate astronomical comprehension. The present research study describes how preservice elementary teachers conceptualize and communicate ideas about Space. Instead of assuming a universal mental conception of cosmic orientations and relationships, the dissertation claims that the perception of Space related dimensions vary among preservice elementary teachers. Furthermore, the dissertation suggests individual perceptions of the scale sizes and orientations of celestial systems have direct influences on mental models used to organize and communicate astronomical information. The development of inaccurate mental models of the scaled dimensions of Space may perpetuate the teacher-student cycle of misconception and naive-theory generation among children in elementary education settings. The ability to conceptualize the vast cosmos is facilitated by the minds ability to think about vast scales and orientations of celestial objects. The Earth-based perspective of astronomy education compels the learner to think about astronomical principles within imaginary frames of reference and across unfamiliar scaled dimensions. Therefore, mental astronomical model building is underscored by the perception of scale and cosmic spatiality. This study suggests these cognitive skill sets are interconnected and facilitate the learning of accurate astronomy principles; as well as play an important role when designing an astronomy education program for preservice elementary teachers. This research study is comprised of three separate standalone articles designed and formatted for journal submission. Chapter 1 outlines the intent, rationale, and design of the overall dissertation process and format. Chapter 2 describes an in-depth review of the specific astronomy curricula used for comparison by subsequent chapters and is not intended as a standalone article, but rather as an informative outline of events and activities to help the reader understand the differences of instruction between the two sections of sample populations. Chapter 3 uses qualitative interviews to explore the cosmic dimensions associated with learning of astronomy and finds diverse perceptions of astronomical scales may influence preservice teachers' mental organization of astronomical information. Chapter 4 further analyzes cosmic dimensions using quantitative analyses and specifically examines preservice teachers perceptions of scale and spatiality within the context of astronomy education. Findings from Chapter 4 show that perceptions of scale and spatiality are an interconnected set of learning skills which may greatly enhance the learning of astronomy. Chapter 5 describes how concepts of scale and spatiality may be operationalized within a secondary school science classroom in order to better understand the scaled distances of stars though an inquiry-based three-dimensional modeling activity. Chapter 6 briefly concludes the dissertation work. Due to the nature of this dissertation design, the conclusions chapter is quite succinct as previous chapters are designed with conclusions sections embedded within the body of the text as outlined by specific journal submission guidelines. These dissertation ideas are presented in a formal setting so that the various research undertakings can be studied and analyzed. Qualitative and quantitative analyses of research data are present to support the claims made in this study. The results of this research combine with features of previous research in order to advance our understanding of how preservice elementary teachers think about and learn astronomy.

Astronomy in Iraq

NASA Astrophysics Data System (ADS)

Alsabti, A. W.

2006-08-01

The history of modern Iraqi astronomy is reviewed. During the early 1970's Iraqi astronomy witnessed significant growth through the introduction of the subject at university level and extensively within the school curriculum. In addition, astronomy was popularised in the media, a large planetarium was built in Baghdad, plus a smaller one in Basra. Late 1970 witnessed the construction of the Iraqi National Observatory at Mount Korek in Iraqi Kurdistan. The core facilities of the Observatory included 3.5-meter and 1.25-meter optical telescopes, and a 30-meter radio telescope for millimetre wavelength astronomy. The Iraqi Astronomical Society was founded and Iraq joined the IAU in 1976. During the regime of Saddam Hussain in the 1980's, the Observatory was attacked by Iranian artillery during the Iraq-Iran war, and then again during the second Gulf war by the US air force. Years of sanctions during the 1990's left Iraq cut off from the rest of the international scientific community. Subscriptions to astronomical journals were halted and travel to conferences abroad was virtually non-existent. Most senior astronomers left the country for one reason or another. Support from expatriate Iraqi astronomers existed (and still exists) however, this is not sufficient. Recent changes in Iraq, and the fall of Saddam's regime, has meant that scientific communication with the outside world has resumed to a limited degree. The Ministry of Higher Education in Baghdad, Baghdad University and the Iraqi National Academy of Science, have all played active roles in re-establishing Iraqi astronomy and re-building the damaged Observatory at Mount Korek. More importantly the University of Sallahudin in Erbil, capital of Iraqi Kurdistan, has taken particular interest in astronomy and the Observatory. Organized visits to the universities, and also to the Observatory, have given us a first-hand assessment of the scale of the damage to the Observatory, as well as the needs of astronomy teaching and research. Joint supervision for postgraduate level research was organized between local and Iraqi expatriate astronomers. The IAU was among the first international organizations to offer assistance. Many observatories worldwide have also given support. Plans will be proposed for re-building the Observatory, supporting teaching and research, and establishing an institute for astronomy in Erbil, together with further suggestions on how the international astronomical community can assist Iraqi astronomers.

Definition of the Flexible Image Transport System (FITS), Version 3.0

NASA Technical Reports Server (NTRS)

Pence, W. D.; Chiapetti, L.; Page, C. G.; Shaw, R. A.; Stobie, E.

2010-01-01

The Flexible Image Transport System (FITS) has been used by astronomers for over 30 years as a data interchange and archiving format; FITS files are now handled by a wide range of astronomical software packages. Since the FITS format definition document (the "standard") was last printed in this journal in 2001, several new features have been developed and standardized, notably support for 64-bit integers in images and tables, variable-length arrays in tables, and new world coordinate system conventions which provide a mapping from an element in a data array to a physical coordinate on the sky or within a spectrum. The FITS Working Group of the International Astronomical Union has therefore produced this new Version 3.0 of the FITS standard, which is provided here in its entirety. In addition to describing the new features in FITS, numerous editorial changes were made to the previous version to clarify and reorganize many of the sections. Also included are some appendices which are not formally part of the standard. The FITS standard is likely to undergo further evolution, in which case the latest version may be found on the FITS Support Office Web site at http://fits.gsfc.nasa.gov/, which also provides many links to FITS-related resources.

Science News or Astrological Debating: Chinese Records of the Transit of Venus of 1874

NASA Astrophysics Data System (ADS)

Lu, Lingfeng

2012-09-01

The Venus transit is very important in the measuring of the distance between the sun and the earth. It ever occurred in 1874, but this time it was visible only in China and some other places in eastern sphere. So many astronomers of the western countries had to come to China to observe it. In traditional Chinese astrological explanation, the sun represented the emperor. If the sun were invaded by other stars, it means that the emperor and the country would have some ominous disasters. In late 19th century, western astronomical knowledge was widely translated into Chinese and understood by Chinese intellectuals. The Venus transit should easily be understood by Chinese intellectuals as one kind of astronomical phenomena. But early before the Venus transit taking place in 1874, many Chinese publications had to introduce this kind of celestial phenomena as science news because at same time, some influential news papers and journals also had some discussion on what astrological connection between the Venus transit of this time and the fortune of the country. This article collects these interesting Chinese records and discusses what different attitude to the Venus transit by Chinese intellectuals and officials during that period in which western learning was widely disseminated in China.

Some psychometric properties of the Pediatric Quality of Life Inventory™ Version 4.0 Generic Core Scales (PedsQL™) in the general Serbian population.

PubMed

Stevanović, Dejan; Lakić, Aneta; Damnjanović, Maja

2011-08-01

The aim of this study was to evaluate the general measurement properties of the Serbian version of the Pediatric Quality of Life Inventory™ Version 4.0 Generic Core Scales (PedsQL™) self-report versions for children and adolescents (8-18 years). The PedsQL™ was completed by 238 children and adolescents. The version was descriptively analyzed first. Afterward, internal consistency and construct and convergent validity were analyzed using the classic test theory psychometrical procedures. The PedsQL™ scale score means ranged 70.65-88.34, with the total score was 80.74. Scale internal consistency reliability determined by Cronbach's coefficient was above 0.7 for all except the School, 0.65, and Emotional Functioning Scale, 0.69. The statistics assessing the adequacy of the model in confirmatory factor analysis revealed poor model fit for the current structure of the PedsQL™. Finally, the PedsQL™ total and psychosocial health showed convincing negative correlations with emotional and conduct problems, hyperactivity/inattention, and peer relationship problems. The Serbian PedsQL™ scales have appropriate internal consistency reliability, sufficient for group evaluations, and good convergent validity against psychological constructs. However, there are problems regarding its current construct validity (factorial validity).

Antioxidant and antimicrobial potentials of Serbian red wines produced from international Vitis vinifera grape varieties.

PubMed

Radovanović, Aleksandra N; Jovančićević, Branimir S; Radovanović, Blaga C; Mihajilov-Krstev, Tatjana; Zvezdanović, Jelena B

2012-08-15

Antioxidant and antimicrobial potentials of Serbian red wines produced from different international Vitis vinifera grape varieties and their correlation with contents of phenolic compounds were studied by spectrophotometric and chromatographic methods. The antioxidant activity of red wines was estimated through their ability to scavenge 2,2'-diphenyl-1-picrylhydrazyl free radical (DPPH(•) ). The red wines, gallic acid, (+)-catechin and quercetin were screened in vitro for antimicrobial activity against Gram-positive and Gram-negative strains using microdilution and disc diffusion techniques. Excellent correlations between the contents of quercetin-3-glucoside (R(2) = 0.9463) and quercetin (R(2) = 0.9337) and DPPH(•) -scavenging ability of the red wines were found. Serbian red wines exhibited significant activity against Staphylococcus aureus, Listeria inocua, Micrococcus flavus, Sarcina lutea, Bacillus subtilis, Escherichia coli, Pseudomonas aeruginosa, Salmonella enteritidis and Shigella sonnei strains, which was in correlation with their phenolic composition and antioxidant activity. The compounds gallic acid, quercetin and (+)-catechin showed high activity against B. subtilis, S. aureus, S. lutea and M. flavus Gram-positive and S. enteritidis and P. aeruginosa Gram-negative strains. The results show that quercetin-3-glucoside and quercetin concentrations can be used as markers for the determination of antioxidant and antimicrobial potentials of red wines. Copyright © 2012 Society of Chemical Industry.

Concentrations of arsenic, cadmium and lead in selected foodstuffs from Serbian market basket: estimated intake by the population from the Serbia.

PubMed

Škrbić, Biljana; Živančev, Jelena; Mrmoš, Nataša

2013-08-01

In this study arsenic (As), cadmium (Cd) and lead (Pb) were determined in 114 samples of various food items collected at supermarkets located in Novi Sad, the capitol of the northern Serbian province of Vojvodina in January 2012 and March 2013. The considered items represented the most consumed foodstuffs according to the "national market basket". The highest concentrations were obtained for Pb in candy (0.323 mg kg(-1)), for Cd in paprika (0.118 mg kg(-1)) and for As in canned fish (0.43 mg kg(-1)). The results were compared with the relevant data on the occurrence of these toxic elements available in literature for other European countries. Human health risk assessment through dietary exposure was evaluated for Serbian adult consumers. The estimated intakes were compared with available toxicological references to assess the risk of As, Cd and Pb intake through consumption of analysed food items. The highest intake were estimated for Pb being 72.30 μg day(-1) for adult population, while intakes of As and Cd were significantly lower (21.89 μg day(-1) and 11.51 μg day(-1), respectively). Copyright © 2013 Elsevier Ltd. All rights reserved.

Astronomy Map of the World

NASA Astrophysics Data System (ADS)

Veras, D.

2017-09-01

I have created an online clickable and zoom-enabled world map - now viewed over 5,400 times - that contains weblinks to institutions where astronomy is either researched professionally and / or and taught in classrooms at the university level. Not included are stand-alone museums, planetariums, amateur astronomical societies, virtual institutes, nor observatories which do not fulfill this criteria. One can click on a marker to access the relevant institute. The map currently contains 697 institutes, and has multiple potential uses for undergraduate students, graduate students, postdocs, faculty and journal editors.

Tidal Dissipation Compared To Seismic Dissipation: In Small Bodies, Earths, And Super-Earths

DTIC Science & Technology

2012-02-20

The Astrophysical Journal, 746:150 (20pp), 2012 February 20 doi:10.1088/0004-637X/746/2/150 C© 2012. The American Astronomical Society. All rights...becomes more complex, though for sufficiently large super-Earths the same rule applies: the larger the planet, the weaker the tidal dissipation in it...damping) becomes very considerable for large exoplanets (super-Earths). In those, it is much lower than what one might expect from using a seismic

Speckle Interferometry at Soar in 2010 and 2011: Measures, Orbits, and Rectilinear Fits

DTIC Science & Technology

2012-02-01

Astron. Nachr., 331, 304 18 The Astronomical Journal, 143:42 (19pp), 2012 February Hartkopf, Tokovinin, & Mason Cvetkovic, Z., & Novakovic , B. 2006...Serb. AJ, 173, 73 Cvetkovic, Z., Novakovic , B., & Todorovic, N. 2008, New Astron., 13, 125 Davis, J., Mendez, A., Seneta, E. B., et al. 2005, MNRAS...J., et al. 2004, A&A, 418, 989 Novakovic , B. 2006, Inf. Circ., 158, 1 Novakovic , B. 2007, Chin. J. Astron. Astrophys., 7, 415 Olevic, D. 2002a, Inf

Astronomical Publishing: Yesterday, Today and Tomorrow

NASA Astrophysics Data System (ADS)

Huchra, John

Just in the last few years scientific publishing has moved rapidly away from the modes that served it well for over two centuries. As "digital natives" take over the field and rapid and open access comes to dominate the way we communicate, both scholarly journals and libraries need to adopt new business models to serve their communities. This is best done by identifying new "added value" such as databases, full text searching, full cross indexing while at the same time retaining the high quality of peer reviewed publication.

Society News: GJI celebrates student authors; Celebrating 5000 years of astronomy at Stonehenge; New Fellows; Council nominations; NAM website opens; Going public;

NASA Astrophysics Data System (ADS)

2010-02-01

Geophysical Journal International has announced the winners of its 2009 Student Author Awards for the best papers in the field with young scientists as lead authors. The RAS and English Heritage celebrated the close of IYA2009 at Stonehenge from 16-19 December, with an event bringing archaeologists and astronomers together on the site to talk to the public. The following were elected to Fellowship of the Society on 11 December 2009:

The history of the creation of Astronomy & Astrophysics

NASA Astrophysics Data System (ADS)

Pottasch, S. R.

2011-07-01

Dutch astronomer S.R. Pottasch, who was appointed as one of the two first Editors-in-Chief of A&A together with J.L. Steinberg, recalls the events that led to the creation of the first European astronomy journal. This account is based on the author's notes and documents and also on an article relating ESO's early history written by A. Blaauw and published in The ESO Messenger No. 60, pp. 23-34 (1990). C. Bertout added footnotes giving a few biographical details about the actors.

Visualising Astronomy: Invisible - Impacts and Rings better

NASA Astrophysics Data System (ADS)

Wyatt, R.

2009-11-01

Stories about unpleasant experiences when collaborating with journalists circulate among many scientists. Some of them regard journalists as potential enemies against whom they have to be prepared. But is the idea that a journalist must be either friend or foe appropriate at all? This article briefly examines the changing relationship between astronomers, science journalists and the general public over the last few decades. It then gives a view from inside science journalism and finally suggests some ideas on how to establish a better relationship between scientists and journalists.

Medical Biochemistry as Subdiscipline of Laboratory Medicine in Serbia.

PubMed

Jovičić, Snežana; Majkić-Singh, Nada

2017-04-01

Medical biochemistry is the usual name for clinical biochemistry or clinical chemistry in Serbia, and medical biochemist is the official name for the clinical chemist (or clinical biochemist). This is the largest sub-discipline of the laboratory medicine in Serbia. It includes all aspects of clinical chemistry, and also laboratory hematology with coagulation, immunology, etc. Medical biochemistry laboratories in Serbia and medical biochemists as a profession are part of Health Care System and their activities are regulated through: the Health Care Law and rules issued by the Chamber of Medical Biochemists of Serbia. The first continuous and organized education for Medical Biochemists (Clinical Chemists) in Serbia dates from 1945, when the Department of Medical Biochemistry was established at the Pharmaceutical Faculty in Belgrade. In 1987 at the same Faculty a five years undergraduate study program was established, educating Medical Biochemists under a special program. Since the academic year 2006/2007 the new five year undergraduate (according to Bologna Declaration) and four-year postgraduate program according to EC4 European Syllabus for Postgraduate Training in Clinical Chemistry and Laboratory Medicine has been established. The Ministry of Education and Ministry of Public Health accredited these programs. There are four requirements for practicing medical biochemistry in the Health Care System: University Diploma of the Faculty of Pharmacy (Study of Medical Biochemistry), successful completion of the professional exam at the Ministry of Health after completion of one additional year of obligatory practical training in the medical biochemistry laboratories, membership in the Serbian Chamber of Medical Biochemists and licence for skilled work issued by the Serbian Chamber of Medical Biochemists. In order to present laboratory medical biochemistry practice in Serbia this paper will be focused on the following: Serbian national legislation, healthcare services organization, sub-disciplines of laboratory medicine and medical biochemistry as the most significant, education in medical biochemistry, conditions for professional practice in medical biochemistry, continuous quality improvement, and accreditation. Serbian healthcare is based on fundamental principles of universal health coverage and solidarity between all citizens.

Bibliographic Resources for the Historian of Astronomy

NASA Astrophysics Data System (ADS)

Corbin, B. G.

1999-12-01

Many large library collections now have online bibliographic catalogs on the web. These provide many hidden resources for the historian of astronomy. Special searching techniques will allow the historian to scan bibliographic records of hundreds of entries relating to biographies of astronomers, collected works of astronomers, ancient and medieval astronomy and many other historical subjects. Abstract databases such as the Astrophysics Data System and ARIBIB are also adding much historical bibliographic information. ARIBIB will eventually contain scanned images of the Astronomischer Jahresbericht containing bibliographic entries for all literature of astronomy from 1899 to 1968 and Astronomy and Astrophysics Abstracts from 1969 to present. Commercial services such as UnCover and FirstSearch provide a means of reaching bibliographic entries for journal and book literature in the history of astronomy which were not easily located in the past. A broad overview of these collections and services will be given, and searching techniques for finding ``hidden" bibliographic data will be presented. Web page addresses will be given for all sources covered.

Student Moon Observations and Spatial-Scientific Reasoning

NASA Astrophysics Data System (ADS)

Cole, Merryn; Wilhelm, Jennifer; Yang, Hongwei

2015-07-01

Relationships between sixth grade students' moon journaling and students' spatial-scientific reasoning after implementation of an Earth/Space unit were examined. Teachers used the project-based Realistic Explorations in Astronomical Learning curriculum. We used a regression model to analyze the relationship between the students' Lunar Phases Concept Inventory (LPCI) post-test score variables and several predictors, including moon journal score, number of moon journal entries, student gender, teacher experience, and pre-test score. The model shows that students who performed better on moon journals, both in terms of overall score and number of entries, tended to score higher on the LPCI. For every 1 point increase in the overall moon journal score, participants scored 0.18 points (out of 20) or nearly 1% point higher on the LPCI post-test when holding constant the effects of the other two predictors. Similarly, students who increased their scores by 1 point in the overall moon journal score scored approximately 1% higher in the Periodic Patterns (PP) and Geometric Spatial Visualization (GSV) domains of the LPCI. Also, student gender and teacher experience were shown to be significant predictors of post-GSV scores on the LPCI in addition to the pre-test scores, overall moon journal score, and number of entries that were also significant predictors on the LPCI overall score and the PP domain. This study is unique in the purposeful link created between student moon observations and spatial skills. The use of moon journals distinguishes this study further by fostering scientific observation along with skills from across science, technology, engineering, and mathematics disciplines.

Reports on crustal movements and deformations. [bibliography

NASA Technical Reports Server (NTRS)

Cohen, S. C.; Peck, T.

1983-01-01

This Catalog of Reports on Crustal Movements and Deformation is a structured bibliography of scientific papers on the movements of the Earth crust. The catalog summarizes by various subjects papers containing data on the movement of the Earth's surface due to tectonic processes. In preparing the catalog we have included studies of tectonic plate motions, spreading and convergence, microplate rotation, regional crustal deformation strain accumulation and deformations associated with the earthquake cycle, and fault motion. We have also included several papers dealing with models of tectonic plate motion and with crustal stress. Papers which discuss tectonic and geologic history but which do not present rates of movements or deformations and papers which are primarily theoretical analyses have been excluded from the catalog. An index of authors cross-referenced to their publications also appears in the catalog. The catalog covers articles appearing in reviewed technical journals during the years 1970-1981. Although there are citations from about twenty journals most of the items come from the following publications: Journal of Geophysical Research, Tectonophysics, Geological Society of America Bulletin of the Seismological Society of America, Nature, Science, Geophysical Journal of the Royal Astronomical Society, Earth and Planetary Science Letters, and Geology.

VLT Detects First Superstorm on Exoplanet

NASA Astrophysics Data System (ADS)

2010-06-01

Astronomers have measured a superstorm for the first time in the atmosphere of an exoplanet, the well-studied "hot Jupiter" HD209458b. The very high-precision observations of carbon monoxide gas show that it is streaming at enormous speed from the extremely hot day side to the cooler night side of the planet. The observations also allow another exciting "first" - measuring the orbital speed of the exoplanet itself, providing a direct determination of its mass. The results appear this week in the journal Nature. "HD209458b is definitely not a place for the faint-hearted. By studying the poisonous carbon monoxide gas with great accuracy we found evidence for a super wind, blowing at a speed of 5000 to 10 000 km per hour" says Ignas Snellen, who led the team of astronomers. HD209458b is an exoplanet of about 60% the mass of Jupiter orbiting a solar-like star located 150 light-years from Earth towards the constellation of Pegasus (the Winged Horse). Circling at a distance of only one twentieth the Sun-Earth distance, the planet is heated intensely by its parent star, and has a surface temperature of about 1000 degrees Celsius on the hot side. But as the planet always has the same side to its star, one side is very hot, while the other is much cooler. "On Earth, big temperature differences inevitably lead to fierce winds, and as our new measurements reveal, the situation is no different on HD209458b," says team member Simon Albrecht. HD209458b was the first exoplanet to be found transiting: every 3.5 days the planet moves in front of its host star, blocking a small portion of the starlight during a three-hour period. During such an event a tiny fraction of the starlight filters through the planet's atmosphere, leaving an imprint. A team of astronomers from the Leiden University, the Netherlands Institute for Space Research (SRON), and MIT in the United States, have used ESO's Very Large Telescope and its powerful CRIRES spectrograph to detect and analyse these faint fingerprints, observing the planet for about five hours, as it passed in front of its star. "CRIRES is the only instrument in the world that can deliver spectra that are sharp enough to determine the position of the carbon monoxide lines at a precision of 1 part in 100 000," says another team member Remco de Kok. "This high precision allows us to measure the velocity of the carbon monoxide gas for the first time using the Doppler effect." The astronomers achieved several other firsts. They directly measured the velocity of the exoplanet as it orbits its home star. "In general, the mass of an exoplanet is determined by measuring the wobble of the star and assuming a mass for the star, according to theory. Here, we have been able to measure the motion of the planet as well, and thus determine both the mass of the star and of the planet," says co-author Ernst de Mooij. Also for the first time, the astronomers measured how much carbon is present in the atmosphere of this planet. "It seems that H209458b is actually as carbon-rich as Jupiter and Saturn. This could indicate that it was formed in the same way," says Snellen. "In the future, astronomers may be able to use this type of observation to study the atmospheres of Earth-like planets, to determine whether life also exists elsewhere in the Universe." More information This research was presented in a paper that appears this week in the journal Nature: "The orbital motion, absolute mass, and high-altitude winds of exoplanet HD209458b", by I. Snellen et al. The team is composed of Ignas A. G. Snellen and Ernst J. W. de Mooij, (Leiden Observatory, The Netherlands), Remco J. de Kok (SRON, Utrecht, The Netherlands), and Simon Albrecht (Massachusetts Institute of Technology, USA). ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organisation in Europe and the world's most productive astronomical observatory. It is supported by 14 countries: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world's most advanced visible-light astronomical observatory and VISTA, the world's largest survey telescope. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 42-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become "the world's biggest eye on the sky".

The Guilford-Carleton Eclipse Expedition of 1900

NASA Astrophysics Data System (ADS)

English, Thomas R., III

2006-12-01

The solar eclipse of 1900 May 28 provided an opportunity for American astronomers to make observations from home soil, as the shadow tracked across the southeastern United States from New Orleans to Norfolk. Eclipse parties were scattered throughout the southern states, including large-scale scientific teams traveling to sites in Georgia and North Carolina. These major operations, staffed by groups from Yerkes, Princeton, USNO, and Lick, featured multiple observing programs and all the modern techniques they could manage. In addition to the major astrophysical endeavors, there were many smaller parties in the field in 1900 that resembled the more casual eclipse expeditions that were characteristic of a few decades before. In these efforts, relatively small groups of observers used modest instruments and made mostly visual observations, and the expedition was as much a social event as it was a scientific venture. One such group was the party from Carleton College and Guilford College that observed from a fruit farm in Southern Pines, NC. At the turn of the century, the Goodsell Observatory at Carleton College in Minnesota was an important regional astronomical facility that had provided weather and time data for over 20 years, and was the site of publication of Popular Astronomy, a widely circulated astronomical journal. At Guilford College, on the other hand, the astronomy course was taught by the school’s Treasurer, and there were no significant astronomical facilities. The presentation will explain how these two schools came to combine efforts to study the 1900 solar eclipse, and will summarize the events of the trip and the observations made. This research was supported in part by the Herbert C. Pollock Award of the Dudley Observatory.

From the West Wing to Pink Floyd to Einstein Advertising: Astronomy in Popular Culture

NASA Astrophysics Data System (ADS)

Fraknoi, Andrew

2007-12-01

In what popular movie does Darryl Hannah play an astronomer? What Japanese car company is named after a well-known star cluster? Can you name at least two murder mysteries that take place at an observatory? What national astronomy education project was mentioned on The West Wing television show (which had several "stealth astronomy” episodes)? What piece of classical music begins with a Big Bang and has the players expanding on stage and into the concert hall? Can you recite the most famous neutrino poem and name the poet? What science fiction story, written by an astronomer under a pseudonym, features an H-R diagram? What rock group had its members’ names included in a reference in the Astrophysical Journal, unbeknownst to the editor? How many astronomy related operas can you name? How many astronomers does it take to screw in a light bulb? Join in on an exploration of astronomy in popular culture, from stamp collecting to advertising, from science fiction (with accurate astronomy) to rock music, from Broadway musicals to modern poetry. Learn which astronomy colleagues have been writing fiction and poetry while you were busy publishing in the research literature. Bring your favorite example of astronomy in popular culture and we'll take the time at the end to share ideas and have some fun. A resource guide for exploring astronomy and popular culture will be available.

Definition of the Flexible Image Transport System (FITS), version 3.0

NASA Astrophysics Data System (ADS)

Pence, W. D.; Chiappetti, L.; Page, C. G.; Shaw, R. A.; Stobie, E.

2010-12-01

The Flexible Image Transport System (FITS) has been used by astronomers for over 30 years as a data interchange and archiving format; FITS files are now handled by a wide range of astronomical software packages. Since the FITS format definition document (the “standard”) was last printed in this journal in 2001, several new features have been developed and standardized, notably support for 64-bit integers in images and tables, variable-length arrays in tables, and new world coordinate system conventions which provide a mapping from an element in a data array to a physical coordinate on the sky or within a spectrum. The FITS Working Group of the International Astronomical Union has therefore produced this new version 3.0 of the FITS standard, which is provided here in its entirety. In addition to describing the new features in FITS, numerous editorial changes were made to the previous version to clarify and reorganize many of the sections. Also included are some appendices which are not formally part of the standard. The FITS standard is likely to undergo further evolution, in which case the latest version may be found on the FITS Support Office Web site at http://fits.gsfc.nasa.gov/, which also provides many links to FITS-related resources.

Modeling Simple Telescope Optics in Secondary Mathematics Classrooms

NASA Astrophysics Data System (ADS)

Siegel, Lauren; Dickinson, G.; Hooper, E. J.; Daniels, M.

2007-12-01

This presentation describes the results of collaboration between instructors in the UTeach teacher preparation program at the University of Texas at Austin, and an astronomer teaching at the university as part of a National Science Foundation Astronomy and Astrophysics Postdoctoral Fellowship. The astronomer provided training to give pre-service teachers an authentic understanding of the principles of telescope optics. This made it possible for the preservice teachers to include real design constraints and optical properties into lessons developed as part of a collaborative field experience to teach astronomical telescope design and construction to high school Algebra II students. One result is a sequence of investigations designed to explore how and why the physical and mathematical properties of parabolic mirrors both enable and constrain our ability to build and use telescopes to focus light from distant objects. Various approaches, including generating and exploring computer models, traditional proofs, even making paper models, are all woven together into a coherent set of eleven investigations for use in mathematics and science classrooms. The presentation will include a description of the suite of investigations, as well as a discussion of the collaborative process which generated the work and resulted in an article submission to a preeminent teaching journal. Teaching Algebra and Geometry Concepts by Modeling Telescope Optics, 2008, Mathematics Teacher is currently in press. Many thanks to the University of Texas UTeach Program for sponsorship of this submission.

The Serbian version of the Juvenile Arthritis Multidimensional Assessment Report (JAMAR).

PubMed

Susic, Gordana; Vojinovic, Jelena; Vijatov-Djuric, Gordana; Stevanovic, Dejan; Lazarevic, Dragana; Djurovic, Nada; Novakovic, Dusica; Consolaro, Alessandro; Bovis, Francesca; Ruperto, Nicolino

2018-04-01

The Juvenile Arthritis Multidimensional Assessment Report (JAMAR) is a new parent/patient-reported outcome measure that enables a thorough assessment of the disease status in children with juvenile idiopathic arthritis (JIA). We report the results of the cross-cultural adaptation and validation of the parent and patient versions of the JAMAR in the Serbian language. The reading comprehension of the questionnaire was tested in 10 JIA parents and patients. Each participating centre was asked to collect demographic, clinical data and the JAMAR in 100 consecutive JIA patients or all consecutive patients seen in a 6-month period and to administer the JAMAR to 100 healthy children and their parents. The statistical validation phase explored descriptive statistics and the psychometric issues of the JAMAR: the three Likert assumptions, floor/ceiling effects, internal consistency, Cronbach's alpha, interscale correlations, test-retest reliability, and construct validity (convergent and discriminant validity). A total of 248 JIA patients (5.2% systemic, 44.3% oligoarticular, 23.8% RF-negative polyarthritis, 26.7% other categories) and 100 healthy children were enrolled in three centres. The JAMAR components discriminated healthy subjects from JIA patients. All JAMAR components revealed good psychometric performances. In conclusion, the Serbian version of the JAMAR is a valid tool for the assessment of children with JIA and is suitable for use both in routine clinical practice and clinical research.

Presence of sulphites in different types of partly processed meat products prepared for grilling

NASA Astrophysics Data System (ADS)

Korićanac, V.; Vranić, D.; Trbović, D.; Petronijević, R.; Parunović, N.

2017-09-01

In the period January 2016 to May 2017, the presence and levels of sulfite were examined in 270 samples of hamburger, sausage (various types), pljeskavica (Serbian-style meat patties of various types) and ćevapi or ćevapčići (grill kebabs) from the Serbian market. Some (12.59%) of these partly processed meat products contained sulfites, expressed as SO2, at levels above 10 mg/kg, and so did not meet requirements laid down in the National Regulation. In the remainder of the meat products (87.41%), sulfite contents were below 10 mg/kg, which is considered as “not detected”. By groups, 100% of hamburgers, 91.76% of sausages and 90.48% of pljeskavica met requirements of National Regulation. The meat product group with the biggest percentage of non-compliant meat products in which sulfites were detected was the ćevapi or ćevapčići - 18.10% of them contained sulfites. All in all, most of the partly processed meat products from the Serbian market met the National Regulation regarding sulfite content, and they were safe for consumption. Nonetheless, the high percentage of ćevapi or ćevapčići that contained sulfites leads us to conclude that regular and periodic control is necessary and one of the most important steps in ensuring safe and quality meat products for consumers.

Analysis of expired medications in Serbian households

PubMed Central

Tomas, Ana; Tomic, Zdenko; Bukumiric, Dragica; Corac, Aleksandar; Horvat, Olga; Sabo, Ana

2016-01-01

Abstract Introduction An ongoing issue of expired medications accumulating in some households is a universal problem around the world. The aim of the study was to investigate the extent and structure of expired medications in Serbian households, and to determine which therapeutic groups generated the most waste. Methods This was an observational, cross-sectional study conducted in households in the city of Novi Sad, Serbia. The study had been performed over 8 month period (December 2011 - July 2012) and it consisted of personal insights into the medication inventory in households. Results Of 1008 families, 383 agreed to participate and complete the questionnaire (38.3% response rate). In almost a half of households (44.4%), expired medications were maintained. The amount of expired medications was 402 items, corresponding to 9.2% of total medications presented in surveyed households. The majority of expired medications (64.7%) was in solid dosage (tablets, capsules, granules, lozenges), following semisolid (ointments, creams, gel, suppositories) and liquid dosage forms (drops, syrups). Expired medications in the households belonged mostly to 3 categories: antimicrobials for systemic use (16.7%), dermatological preparation (15.9%) and medications for alimentary tract and metabolism (14.2%). Conclusions This study revealed that there were relatively large quantities of expired medications in Serbian households, with a high prevalence of antibiotics for systemic use, anti-inflammatory and antirheumatic products, and medications for alimentary tract and metabolism. PMID:27703539

Exotic Molecules in Space: A Coordinated Astronomical, Laboratory, and Theoretical Study

NASA Technical Reports Server (NTRS)

Thaddeus, Patrick

1997-01-01

The past year has been a period of spectacular progress in our investigation of exotic molecules of astrophysical interest. During this period an entirely new spectrometer for the investigation of reactive molecules was finished: a Fourier-transform microwave spectrometer with a supersonic molecular beam. The instrument is operating almost flawlessly, and during the above period of less than two years has discovered the 23 new carbon chain and ring-chain molecules. Seventeen research papers, nearly all in leading refereed journals such as the Astrophysical Journal and the Journal of Chemical Physics have been published. At least five more papers are being prepared for publication. Already four of our new molecules have been detected in space with large radio telescopes. In many ways the most interesting of these is HC(11)N, which now ranks as the largest molecule definitely identified beyond the solar system. Nearly all the other new molecules are candidates for astronomical detection, and we will be disappointed if a number of them are not found as more sensitive receivers and larger telescopes are constructed. During the next year we expect this wave of discovery to continue, and to insure rapid progress we have designed an even more sensitive spectrometer which will operate at the temperature of liquid helium. The goal of this system is to enhance the sensitivity of Fourier-transform spectroscopy by a further factor of 20 to 50, achieving this by reducing the amplifier and thermal noise to levels routinely achieved in radio astronomy. This new instrument offers a number of technical challenges in cryogenic and microwave engineering, but none of these appears to be insurmountable, and our current schedule is to have the helium cooled system operating within the next six months. A number of investigations continued with our conventional free space spectrometer, which remains a powerful complement to our new FTM instrument.

Astronomy Education Research Observations from the iSTAR international Study of Astronomical Reasoning Database

NASA Astrophysics Data System (ADS)

Tatge, C. B.; Slater, S. J.; Slater, T. F.; Schleigh, S.; McKinnon, D.

2016-12-01

Historically, an important part of the scientific research cycle is to situate any research project within the landscape of the existing scientific literature. In the field of discipline-based astronomy education research, grappling with the existing literature base has proven difficult because of the difficulty in obtaining research reports from around the world, particularly early ones. In order to better survey and efficiently utilize the wide and fractured range and domain of astronomy education research methods and results, the iSTAR international Study of Astronomical Reasoning database project was initiated. The project aims to host a living, online repository of dissertations, theses, journal articles, and grey literature resources to serve the world's discipline-based astronomy education research community. The first domain of research artifacts ingested into the iSTAR database were doctoral dissertations. To the authors' great surprise, nearly 300 astronomy education research dissertations were found from the last 100-years. Few, if any, of the literature reviews from recent astronomy education dissertations surveyed even come close to summarizing this many dissertations, most of which have not been published in traditional journals, as re-publishing one's dissertation research as a journal article was not a widespread custom in the education research community until recently. A survey of the iSTAR database dissertations reveals that the vast majority of work has been largely quantitative in nature until the last decade. We also observe that modern-era astronomy education research writings reaches as far back as 1923 and that the majority of dissertations come from the same eight institutions. Moreover, most of the astronomy education research work has been done covering learners' grasp of broad knowledge of astronomy rather than delving into specific learning targets, which has been more in vogue during the last two decades. The surprisingly wide breadth of largely unknown research revealed in the iSTAR database motivates us to begin to synthesize the research and look for broader themes using widely accepted meta analysis techniques.

[Civilian massacre in Banija: Kraljevcani and Pecki, 14-16 March 1991].

PubMed

Kovacević, S; Judas, M; Marusić, A

1991-01-01

On 14 and 16 August 1991, Serbian terrorists attacked two villages near Petrinja in the Banija region. The village of Kraljevcani was attacked on 14 August, when the terrorists killed five older villagers, 3 women and 2 men who stayed in the village to watch the livestock and the houses. The women were killed by automatic rifle fire and grenades, and the bodies of the two men were blown up by a hand rocket-launcher projectiles. On 16 August 1991, Serbian terrorists captured four villagers from Pecki, who came to the deserted village to feed the livestock left after the inhabitants fled from the terrorists. The forensic medical expertise revealed that they were first wounded by rifle fire, then tortured and finally executed by hand axes and bayonets.

No evidence for an early seventeenth-century Indian sighting of Kepler's supernova (SN1604)

NASA Astrophysics Data System (ADS)

van Gent, R. H.

2013-03-01

In a recent paper in this journal, Sule et al. (2011) argued that an early 17th-century Indian mural of the constellation Sagittarius with a dragon-headed tail indicated that the bright supernova of 1604 was also sighted by Indian astronomers. In this paper it will be shown that this identification is based on a misunderstanding of traditional Islamic astrological iconography and that the claim that the mural represents an early 17th-century Indian sighting of the supernova of 1604 has to be rejected.

Commentary on interstellar matter associated with 18 open clusters

NASA Technical Reports Server (NTRS)

Leisawitz, David

1989-01-01

Information supplementary to that contained in Section 4 of an article entitled, A CO Survey of Regions Around 34 Open Clusters, (Leisawitz, Bash, and Thaddeus) published in the Astrophysical Journal Supplement Series, Volume 70, Number 4, August 1989 is summarized. The information presented here, which describes the interstellar environments of young clusters and some cluster physical characteristics, comes from observations published in the astronomical literature and the author's carbon monoxide (CO) emission line survey, and may help clarify our understanding of the interaction of massive stars with the interstellar medium.

WAIS Searching of the Current Contents Database

NASA Astrophysics Data System (ADS)

Banholzer, P.; Grabenstein, M. E.

The Homer E. Newell Memorial Library of NASA's Goddard Space Flight Center is developing capabilities to permit Goddard personnel to access electronic resources of the Library via the Internet. The Library's support services contractor, Maxima Corporation, and their subcontractor, SANAD Support Technologies have recently developed a World Wide Web Home Page (http://www-library.gsfc.nasa.gov) to provide the primary means of access. The first searchable database to be made available through the HomePage to Goddard employees is Current Contents, from the Institute for Scientific Information (ISI). The initial implementation includes coverage of articles from the last few months of 1992 to present. These records are augmented with abstracts and references, and often are more robust than equivalent records in bibliographic databases that currently serve the astronomical community. Maxima/SANAD selected Wais Incorporated's WAIS product with which to build the interface to Current Contents. This system allows access from Macintosh, IBM PC, and Unix hosts, which is an important feature for Goddard's multiplatform environment. The forms interface is structured to allow both fielded (author, article title, journal name, id number, keyword, subject term, and citation) and unfielded WAIS searches. The system allows a user to: Retrieve individual journal article records. Retrieve Table of Contents of specific issues of journals. Connect to articles with similar subject terms or keywords. Connect to other issues of the same journal in the same year. Browse journal issues from an alphabetical list of indexed journal names.

Augmented Articles: The Future of Peer-Reviewed Publications?

NASA Astrophysics Data System (ADS)

Madura, Thomas Ignatius; Clementel, Nicola; Gull, Theodore R.

2015-08-01

The predominance of 2D figures and animations in the literature is clearly driven by the need to display data in a classic paper-journal format. However, there is no real reason that researchers should be limited to 2D graphics when presenting their results in peer-reviewed publications. This is especially true since all major astrophysical journals are now published online. So-called ‘augmented articles’ are possible, in which 3D interactive models, images, sound, and video can be included directly within an Adobe Portable Document Format (PDF) article. The inclusion of 3D interactive models in the astrophysics literature is slowly becoming popular, and several journals now fully support the inclusion of 3D interactive figures and movies. I present examples of recently published augmented articles in astronomy (e.g. Madura et al. 2015, arXiv:1503.00716) and discuss their perceived benefits and limitations. Such articles may become the norm in astronomy as data and numerical simulations increasingly become multidimensional (see http://www.technologyreview.com/view/535796/astronomers-create-3-d-printed-model-of-colliding-stellar-winds/).

Writing a Scientific Paper III. Ethical Aspects

NASA Astrophysics Data System (ADS)

Sterken, C.

2011-07-01

The main theme of this paper is truthful communication of scientific results. Therefore, concepts of truth, error, quality and value are elaborated. The following bibliometric parameters are explained: the journal impact factor, the journal cited half-life, and the journal immediacy index, as well as paper counts, citation rates, citation index and the Hirsch index. These bibliometric indices and indicators are illustrated with examples derived from bibliometric analyses of the astronomical literature. Scientific misconduct in the broadest sense is discussed by category: researcher misconduct, author misconduct, referee and grant-reviewer misconduct. But also publisher misconduct, editorial misconduct and mismanagement, and research supervisor misbehavior are dealt with. The overall signatures of scientific misconduct are focused on, as well as the causes and the cures. This is followed by a Section devoted to whistleblowing. The biases of bibliometric indices, and the use and abuse of bibliometrics are illustrated. Moreover, suggestions for remediating the present defective system of bibliometric measurement and evaluation are worked out. Finally, the hopes and concerns of our students - either expressed during or after the lectures, or through subsequent private contacts - are passed on.

Modern Publishing Approach of Journal of Astronomy & Earth Sciences Education

NASA Astrophysics Data System (ADS)

Slater, Timothy F.

2015-01-01

Filling a needed scholarly publishing avenue for astronomy education researchers and earth science education researchers, the Journal of Astronomy & Earth Sciences Education - JAESE published its first volume and issue in 2014. The Journal of Astronomy & Earth Sciences Education - JAESE is a scholarly, peer-reviewed scientific journal publishing original discipline-based education research and evaluation, with an emphasis of significant scientific results derived from ethical observations and systematic experimentation in science education and evaluation. International in scope, JAESE aims to publish the highest quality and timely articles from discipline-based education research that advance understanding of astronomy and earth sciences education and are likely to have a significant impact on the discipline or on policy. Articles are solicited describing both (i) systematic science education research and (ii) evaluated teaching innovations across the broadly defined Earth & space sciences education, including the disciplines of astronomy, climate education, energy resource science, environmental science, geology, geography, agriculture, meteorology, planetary sciences, and oceanography education. The publishing model adopted for this new journal is open-access and articles appear online in GoogleScholar, ERIC, and are searchable in catalogs of 440,000 libraries that index online journals of its type. Rather than paid for by library subscriptions or by society membership dues, the annual budget is covered by page-charges paid by individual authors, their institutions, grants or donors: This approach is common in scientific journals, but is relatively uncommon in education journals. Authors retain their own copyright. The journal is owned by the Clute Institute of Denver, which owns and operates 17 scholarly journals and currently edited by former American Astronomical Society Education Officer Tim Slater, who is an endowed professor at the University of Wyoming and a Senior Scientist at the CAPER Center for Astronomy & Physics Education Research. More information about the journal and its policies are available online at http://www.JAESE.org

Phytotherapy in medieval Serbian medicine according to the pharmacological manuscripts of the Chilandar Medical Codex (15-16th centuries).

PubMed

Jarić, Snežana; Mitrović, Miroslava; Djurdjević, Lola; Kostić, Olga; Gajić, Gordana; Pavlović, Dragana; Pavlović, Pavle

2011-09-01

The Chilandar Medical Codex is the most significant and best preserved medieval Serbian manuscript and collects together documents on European medical science from the 12th to 15th centuries. It represents the best-known and most complete example of a large collection of medical manuscripts from the Salerno-Montpellier school, written in the vernacular - something which does not exist among the majority of European nations. This paper presents the section of the Codex that deals with phytotherapy, which is contained within the pharmacological manuscripts. An analysis of their contents shows that out of a total of 167 recorded substances, 135 are of plant origin (81%), 13 animal origin (7.7%) and 19 inorganic (11.3%). The recorded plant species are categorised into 63 families, of which the most frequent are: Apiaceae (8.1%), Lamiaceae (8.1%), Asteraceae (5.9%), Rosaceae (5.9%) and Fabaceae (4.4%). All possible plant parts were used in treatments: the whole plant (6%), underground parts (13.7% - root, rhizome, bulb) and aerial parts (80.3% - stem, leaf, flower, buds, fruit, seeds). Of the plants quoted, the following are mentioned most frequently: Vitis sp. (120), Rosa canina (55), Olea europaea (45), Pistacia lentiscus (25), Saccharum officinarum (23), Artemisia absinthium (16) and Foeniculum vulgare (15). The contents of the pharmacological manuscripts of the Chilandar Medical Codex point to the sound contemporary knowledge of the diversity of plant species, their origins, habitat types, the levels of their healing powers, and when and how to gather them and prepare them, as well as the recommended dose for the treatment of specific illnesses. As these manuscripts contain not only common, lay terms for the plants, but also scientific, botanical ones, we can consider them the precursor to Serbian botany. Based on its contents and the way in which they are presented, it can be viewed not only as the first Serbian pharmacopeia, but first Slavic pharmacopeia, too, because similar manuscripts written in the vernacular did not exist during that period among the other Slavic nations, or even most European nations. Copyright © 2011 Elsevier Ireland Ltd. All rights reserved.

[Miraculous recoveries in the frescoes of the Decani Monastery].

PubMed

Jović, N; Jancić-Stefanović, J

1999-01-01

Serbian medieval medicine can be said to have the same characteristics as western medicine of those times in terms of practical medical science, whereas the ancillary medical branches were under Byzantine influence. Besides the compositions of Christ's miracles and paraboles are underlying part of the fresco/painting, the scenes of Christ's miraculous recoveries have an important place in the christian iconography of the New Testament events. One of the most impressive cycles of Christ's miracles in the Serbian and Byzantine medieval art was painted in c. 1340 year in the church dedicated to the Ascension of Lord Christ at Dechani Monastery and constructed between 1327 and 1335. A considerable number of 22 frescoes of different artistic value and technique displays the miraculous recovery of patients afflicted by various chronic ailments: paralytics (razlabljeni), lepers, and handicapped (blind, lame and deaf). One scene presents the bleeding (krvotociva) women. Scenes of recovery from nervous and mental diseases are especially impressive. Patients with atrophic arm, these with hemiplegy, epilepsy, an somnambulist boy, lunatics and possessed are there painted. The magnificent compositions of the miraculous recovery of a patient with ascites (debela, vodena bolest) and these affected by disorders of mainly neuromuscular and locomotor systems are performed by talented masters. The King Stefan Urosh Dechanski Third (1322-1331) founded the hospital in the Dechani Monastery, as a purely medical institution for providing treatment. This hospital was organized and modelled on the hospital in the Pantocrator Monastery in Constantinople. His biographer Gregory Camblak described that this hospital took in patients suffering from epilepsy (svestenoga neduga radi stradalcem) and serious nervous disorders, lepers, cripples, paralytics and those with lung diseases. Regardless of differences in the artistic level, most of these frescoes are impressively natural and realistic. This supports the ascertain that masters painted even some of patients from Monastery Hospital. The scenes of Christ's miraculous recoveries in the Dechani Monastery are undoubtelly significant for both the cultural history and the Serbian medieval medicine. This considerable cycle of the monumental painting and frescoes with medical matter, constitutes the basis for research of the Serbian medicine of the Middle-Ages.

Medical Biochemistry as Subdiscipline of Laboratory Medicine in Serbia

PubMed Central

Jovičić, Snežana

2017-01-01

Summary Medical biochemistry is the usual name for clinical biochemistry or clinical chemistry in Serbia, and medical biochemist is the official name for the clinical chemist (or clinical biochemist). This is the largest sub-discipline of the laboratory medicine in Serbia. It includes all aspects of clinical chemistry, and also laboratory hematology with coagulation, immunology, etc. Medical biochemistry laboratories in Serbia and medical biochemists as a profession are part of Health Care System and their activities are regulated through: the Health Care Law and rules issued by the Chamber of Medical Biochemists of Serbia. The first continuous and organized education for Medical Biochemists (Clinical Chemists) in Serbia dates from 1945, when the Department of Medical Biochemistry was established at the Pharmaceutical Faculty in Belgrade. In 1987 at the same Faculty a five years undergraduate study program was established, educating Medical Biochemists under a special program. Since the academic year 2006/2007 the new five year undergraduate (according to Bologna Declaration) and four-year postgraduate program according to EC4 European Syllabus for Postgraduate Training in Clinical Chemistry and Laboratory Medicine has been established. The Ministry of Education and Ministry of Public Health accredited these programs. There are four requirements for practicing medical biochemistry in the Health Care System: University Diploma of the Faculty of Pharmacy (Study of Medical Biochemistry), successful completion of the professional exam at the Ministry of Health after completion of one additional year of obligatory practical training in the medical biochemistry laboratories, membership in the Serbian Chamber of Medical Biochemists and licence for skilled work issued by the Serbian Chamber of Medical Biochemists. In order to present laboratory medical biochemistry practice in Serbia this paper will be focused on the following: Serbian national legislation, healthcare services organization, sub-disciplines of laboratory medicine and medical biochemistry as the most significant, education in medical biochemistry, conditions for professional practice in medical biochemistry, continuous quality improvement, and accreditation. Serbian healthcare is based on fundamental principles of universal health coverage and solidarity between all citizens. PMID:28680362

What is WorldWide Telescope, and Why Should Researchers Care?

NASA Astrophysics Data System (ADS)

Goodman, Alyssa A.

2016-01-01

As of 2015, about 20 million people have downloaded the computer program called "WorldWide Telescope," and even more have accessed it via the web, at http://worldwidetelescope.org. But, the vast majority of these millions are not professional astronomers. This talk will explain why WorldWide Telescope (WWT) is also a powerful tool for research astronomers. I will focus on how WWT can be, and is, being built-in to Journals, and into day-to-day research environments. By way of example, I will show how WWT already: allows users to display images, including those in Journals, in the context of multi-wavelength full-sky imagery; allows for the display of which parts of the Sky have been studied, when, how, and for what reason (see http://adsass.org); allows, via right-click, immediate access to ADS, SIMBAD, and other professional research tools. I will also highlight new work, currently in development, that is using WWT as a tool for observation planning, and as a display mode for advanced high-dimensional data visualization tools, like glue (see http://glueviz.org). WWT is now well-known in the education community (see http://wwtambassadors.org), so the explicit goal of this talk will be to make researchers more aware of its full power. I will explain how WWT transitioned, over 8 years, from a Microsoft Research project to its current open-source state (see https://github.com/WorldWideTelescope), and I will conclude with comments on the future of WWT, and its relationship to how research should be carried out in the future (see http://tinyurl.com/aas-potf).

Editorial: Letter from the Board of Directors

NASA Astrophysics Data System (ADS)

Sandqvist, Aage

2004-10-01

New policy concerning expanded European and non-European A&A memberships: It is now thirty-five years since the scientific journal Astronomy & Astrophysics (A&A) was founded by the merging of six national journals from four European nations, namely France, Germany, the Netherlands and Sweden; Belgium and the other Nordic countries, Denmark, Finland and Norway, also participated. They were subsequently joined by five other western European nations, namely Austria, Greece, Italy, Spain and Switzerland (Norway later withdrew). A&A has no international legal status as such but is represented by the European Southern Observatory (ESO), which also manages its financial transactions. In the early nineteen-nineties, A&A with great foresight took an important step - which the European Union would follow more than a decade later - by incorporating eastern European countries into its sponsoring membership: the Czech Republic, Hungary, Poland and the Slovak Republic; Estonia became a full member in 1998. A&A was now truly ``A European Journal", as then stated on the front cover. In the meantime, A&A grew in importance as a vehicle for world-wide dissemination of astronomical research and an ever-increasing number of high-quality papers began streaming into the A&A Editorial offices from non-European countries, as well as from other European non-member countries. It became obvious to us that A&A no longer was merely a European Journal and in 2001 we removed the ``A European Journal'' from the front cover. Eventually, some of these non-European countries began approaching us with queries about potential membership in A&A and in 2002 we admitted the first such country, Argentina, with an observer status. Meanwhile, the Board intensified its study of the financial and administrative consequences of a wider expansion including the admission of member countries beyond Europe - a special subcommittee was appointed. The Board of Directors, at its meeting in Tartu, Estonia on 8 May 2004, made the important decision - after a lengthy and thorough discussion - that A&A will henceforth consider applications for sponsoring membership from any country in the world with well-documented active and excellent astronomical research. Each application will be carefully treated on a case-by-case basis. Subsequently, at this meeting, the Board admitted Argentina to full membership in A&A starting on 1 January 2005. In addition, three other applicants were admitted to observer status, namely Brazil, Chile and Portugal. The above-mentioned special Board subcommittee will continue its work and submit recommendations on the restructuring of the Board and its Executive Committee, a necessary consequence of the foreseen expansion.

Educational Applications for Blind and Partially Sighted Pupils Based on Speech Technologies for Serbian.

PubMed

Lučić, Branko; Ostrogonac, Stevan; Vujnović Sedlar, Nataša; Sečujski, Milan

2015-01-01

The inclusion of persons with disabilities has always represented an important issue. Advancements within the field of computer science have enabled the development of different types of aids, which have significantly improved the quality of life of the disabled. However, for some disabilities, such as visual impairment, the purpose of these aids is to establish an alternative communication channel and thus overcome the user's disability. Speech technologies play the crucial role in this process. This paper presents the ongoing efforts to create a set of educational applications based on speech technologies for Serbian for the early stages of education of blind and partially sighted children. Two educational applications dealing with memory exercises and comprehension of geometrical shapes are presented, along with the initial tests results obtained from research including visually impaired pupils.

Educational Applications for Blind and Partially Sighted Pupils Based on Speech Technologies for Serbian

PubMed Central

Lučić, Branko; Ostrogonac, Stevan; Vujnović Sedlar, Nataša; Sečujski, Milan

2015-01-01

The inclusion of persons with disabilities has always represented an important issue. Advancements within the field of computer science have enabled the development of different types of aids, which have significantly improved the quality of life of the disabled. However, for some disabilities, such as visual impairment, the purpose of these aids is to establish an alternative communication channel and thus overcome the user's disability. Speech technologies play the crucial role in this process. This paper presents the ongoing efforts to create a set of educational applications based on speech technologies for Serbian for the early stages of education of blind and partially sighted children. Two educational applications dealing with memory exercises and comprehension of geometrical shapes are presented, along with the initial tests results obtained from research including visually impaired pupils. PMID:26171422

Clinical research involving minors in international and serbian regulations.

PubMed

Planojević, Nina; Zivojinović, Dragica

2013-07-01

Participation in clinical trials can be useful for the health of a person, in who it is conducted, but it does not have to be - it can even be harmful. Therefore, primary motive to accept such risk is humanity and human wish to contribute to the progress of medicine; this is expressed by personal consent. The consent, however, can be an expression of personal humanity, and for this, it is not logical that someone can give consent on behalf of someone else, as it is done by a legally authorized representative on behalf of a minor. Therefore, authors raise 3 questions: What are the reasons to consider representative's consent acceptable? How should a model of regulations look like in order to provide the most complete possible protection to a minor? Is actual regulation of minors' position within international and Serbian law, analyzed here by authors for their specific solutions, acceptable? Representative's consent is acceptable only for therapeutic research, because these can bring benefits to everyone's health, including a minor in which those are conducted - this is an acceptable (secondary) motive of participation in the research. Expression of humanity on other's behalf, typical for non-therapeutic research, is not acceptable; this makes ban of minors' participation in non-therapeutic research more appropriate regulation model. International regulations are not in accordance to results presented in the paper for allowing participation of minors both in therapeutic and non-therapeutic research. Serbian regulation is closer to the most acceptable regulation model.

Publishing in the Refereed International Journal of Astronomy & Earth Sciences Education JAESE

NASA Astrophysics Data System (ADS)

Slater, Timothy F.

2015-08-01

Filling a needed scholarly publishing avenue for astronomy education researchers and earth science education researchers, the Journal of Astronomy & Earth Sciences Education- JAESE was first published in 2014. JAESE is a scholarly, peer-reviewed scientific journal publishing original discipline-based education research and evaluation, with an emphasis of significant scientific results derived from ethical observations and systematic experimentation in science education and evaluation. International in scope, JAESE aims to publish the highest quality and timely articles from discipline-based education research that advance understanding of astronomy and earth sciences education and are likely to have a significant impact on the discipline or on policy. Articles are solicited describing both (i) systematic science education research and (ii) evaluated teaching innovations across the broadly defined Earth & space sciences education, including the disciplines of astronomy, climate education, energy resource science, environmental science, geology, geography, agriculture, meteorology, planetary sciences, and oceanography education. The publishing model adopted for this new journal is open-access and articles appear online in GoogleScholar, ERIC, EBSCO, ProQuest, and NASA SAO/ADS and are searchable in catalogs of 440,000 libraries that index online journals of its type. Rather than paid for by library subscriptions or by society membership dues, the annual budget is covered by page-charges paid by individual authors, their institutions, grants or donors: This approach is common in scientific journals, but is relatively uncommon in education journals. Authors retain their own copyright. The journal is owned by the Clute Institute in the United States, which owns and operates 17 scholarly journals and currently edited by former American Astronomical Society Education Officer Tim Slater, who is an endowed professor at the University of Wyoming and a Senior Scientist at the CAPER Center for Astronomy & Physics Education Research. More information about the journal and its policies are available online at http://www.JAESE.org

A Look into the Hellish Cradles of Suns and Solar Systems

NASA Astrophysics Data System (ADS)

2009-09-01

New images released today by ESO delve into the heart of a cosmic cloud, called RCW 38, crowded with budding stars and planetary systems. There, young stars bombard fledgling suns and planets with powerful winds and blazing light, helped in their task by short-lived, massive stars that explode as supernovae. In some cases, this onslaught cooks away the matter that may eventually form new solar systems. Scientists think that our own Solar System emerged from such an environment. The dense star cluster RCW 38 glistens about 5500 light years away in the direction of the constellation Vela (the Sails). Like the Orion Nebula Cluster, RCW 38 is an "embedded cluster", in that the nascent cloud of dust and gas still envelops its stars. Astronomers have determined that most stars, including the low mass, reddish ones that outnumber all others in the Universe, originate in these matter-rich locations. Accordingly, embedded clusters provide scientists with a living laboratory in which to explore the mechanisms of star and planetary formation. "By looking at star clusters like RCW 38, we can learn a great deal about the origins of our Solar System and others, as well as those stars and planets that have yet to come", says Kim DeRose, first author of the new study that appears in the Astronomical Journal. DeRose did her work on RCW 38 as an undergraduate student at the Harvard-Smithsonian Center for Astrophysics, USA. Using the NACO adaptive optics instrument on ESO's Very Large Telescope [1], astronomers have obtained the sharpest image yet of RCW 38. They focused on a small area in the centre of the cluster that surrounds the massive star IRS2, which glows in the searing, white-blue range, the hottest surface colour and temperatures possible for stars. These dramatic observations revealed that IRS2 is actually not one, but two stars - a binary system consisting of twin scorching stars, separated by about 500 times the Earth-Sun distance. In the NACO image, the astronomers found a handful of protostars - the faintly luminous precursors to fully realised stars - and dozens of other candidate stars that have eked out an existence here despite the powerful ultraviolet light radiated by IRS2. Some of these gestating stars may, however, not get past the protostar stage. IRS2's strong radiation energises and disperses the material that might otherwise collapse into new stars, or that has settled into so-called protoplanetary discs around developing stars. In the course of several million years, the surviving discs may give rise to the planets, moons and comets that make up planetary systems like our own. As if intense ultraviolet rays were not enough, crowded stellar nurseries like RCW 38 also subject their brood to frequent supernovae when giant stars explode at the ends of their lives. These explosions scatter material throughout nearby space, including rare isotopes - exotic forms of chemical elements that are created in these dying stars. This ejected material ends up in the next generation of stars that form nearby. Because these isotopes have been detected in our Sun, scientists have concluded that the Sun formed in a cluster like RCW 38, rather than in a more rural portion of the Milky Way. "Overall, the details of astronomical objects that adaptive optics reveals are critical in understanding how new stars and planets form in complex, chaotic regions like RCW 38", says co-author Dieter Nürnberger. Notes [1] The name "NACO" is a combination of the Nasmyth Adaptive Optics System (NAOS) and the Near-Infrared Imager and Spectrograph (CONICA). Adaptive optics cancels out most of the image-distorting turbulence in Earth's atmosphere caused by temperature variations and wind. More information This research was presented in a paper that appeared in the Astronomical Journal: A Very Large Telescope / NACO study of star formation in the massive embedded cluster RCW 38, by DeRose et al. (2009, AJ, 138, 33-45). The team is composed of K.L. DeRose, T.L. Bourke, R.A. Gutermuth and S.J. Wolk (Harvard-Smithsonian Center for Astrophysics, Cambridge, USA), S.T. Megeath (Department of Physics and Astronomy, The University of Toledo, USA), J. Alves (Centro Astronómico Hispano Alemán, Almeria, Spain), and D. Nürnberger (ESO). ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organisation in Europe and the world's most productive astronomical observatory. It is supported by 14 countries: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world's most advanced visible-light astronomical observatory. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 42-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become "the world's biggest eye on the sky".

"Do-It-Ourselves Science": Case Studies of Volunteer-Initiated Citizen Science Involvement

NASA Astrophysics Data System (ADS)

Raddick, Jordan; Bracey, G.; Gay, P. L.

2009-05-01

Galaxy Zoo is a citizen science website in which members of the public volunteer to classify galaxies, thereby helping astronomers conduct publishable research into galaxy morphologies and environments. Although the site was originally created to answer a few specific questions, some members of the community - both scientists and volunteers - have spontaneously developed an interest in a wider variety of questions. Volunteers have pursued answers to these questions with guidance from professional astronomers; in completing these projects, volunteers have independently used some of the same data viewing and analysis tools that professional astronomers use, and have even developed their own online tools. They have created their own research questions and their own plans for data analysis, and are planning to write scientific papers with the results to be submitted to peer-reviewed scientific journals. Volunteers have identified a number of such projects. These volunteer-initiated projects have extended the scientific reach of Galaxy Zoo, while also giving volunteers first-hand experience with the process of science. We are interested in the process by which volunteers become interested in volunteer-initiated projects, and what tasks they participate in, both initially and as their involvement increases. What motivates a volunteer to become involved in a volunteer-initiated project? How does his or her motivation change with further involvement? We are conducting a program of qualitative education research into these questions, using as data sources the posts that volunteers have made to the Galaxy Zoo forum and transcripts of interviews with volunteers.

Astronomy as the Leader of Interdisciplinary and Multidisciplinary Sciences (Introductory talk)

NASA Astrophysics Data System (ADS)

Martirosyan, R. M.; Mickaelian, A. M.

2015-07-01

Interdisciplinary and multidisciplinary sciences over the last few decades have become the major booster of science development. The most important discoveries occur just at the intersection of sciences and in collaboration of several fields. There appeared such intermediate fields as mathematical physics, physical chemistry, biophysics, biochemistry, geophysics, etc. In astronomy, astrophysics has long been the main field, and in present archaeoastronomy, astrochemistry, astrobiology, astroinformatics (which is tightly related to virtual observatories) are developing. On the other hand, in recent years many science areas surfeit of research on Earth, more and more use data coming from the Space and are being developed just due to them. It is possible that in the near future, various science areas create Space departments or simply develop their research in close collaboration with astronomers. Interesting discoveries have been made in studies of astronomical topics in various areas of culture; such topics are widely used in folklore, other genres of literature, painting, and architecture. Astronomy has also a leading role in scientific tourism, scientific journalism and in general, dissemination of popular science or public outreach.

Astronomy as the Leader of Interdisciplinary and Multidisciplinary Sciences

NASA Astrophysics Data System (ADS)

Mickaelian, A. M.; Farmanyan, S. V.

2016-12-01

Interdisciplinary and multidisciplinary sciences over the last few decades have become the major booster of science development. The most important discoveries occur just at the intersection of sciences and in collaboration of several fields. There appeared such intermediate fields as mathematical physics, physical chemistry, biophysics, biochemistry, geophysics, etc. In astronomy, astrophysics has long been the main field, and in present archaeoastronomy, astrochemistry, astrobiology, astroinformatics (which is tightly related to virtual observatories) are developing. On the other hand, in recent years many science areas surfeit of research on Earth, more and more use data coming from the Space and are being developed just due to them. It is possible that in the near future, various science areas create Space departments or simply develop their research in close collaboration with astronomers. Interesting discoveries have been made in studies of astronomical topics in various areas of culture; such topics are widely used in folklore, other genres of literature, painting, and architecture. Astronomy has also a leading role in scientific tourism, scientific journalism and in general, dissemination of popular science or public outreach.

A Model for Data Citation in Astronomical Research Using Digital Object Identifiers (DOIs)

NASA Astrophysics Data System (ADS)

Novacescu, Jenny; Peek, Joshua E. G.; Weissman, Sarah; Fleming, Scott W.; Levay, Karen; Fraser, Elizabeth

2018-05-01

Standardizing and incentivizing the use of digital object identifiers (DOIs) to aggregate and identify both data analyzed and data generated by a research project will advance the field of astronomy to match best practices in other research fields like geoscience and medicine. An increase in the use of DOIs will prepare the discipline for changing expectations among funding agencies and publishers, who increasingly expect accurate and thorough data citation to accompany scientific outputs. The use of DOIs ensures a robust, sustainable, and interoperable approach to data citation in which due credit is given to the researchers and institutions who produce and maintain the primary data. We describe in this work the advantages of DOIs for data citation and best practices for integrating a DOI service in an astronomical archive. We report on a pilot project carried out in collaboration with AAS journals. During the course of the 1.5-year long pilot, over 75% of submitting authors opted to use the integrated DOI service to clearly identify data analyzed during their research project when prompted at the time of paper submission.

The AAVSO 2011 Demographic and Background Survey

NASA Astrophysics Data System (ADS)

Price, A.

2012-04-01

In 2011, the AAVSO conducted a survey of 615 people who are or were recently active in the organization. The survey included questions about their demographic background and variable star interests. Data are descriptively analyzed and compared with prior surveys. Results show an organization of very highly educated, largely male amateur and professional astronomers distributed across 108 countries. Participants tend to be loyal, with the average time of involvement in the AAVSO reported as 14 years. Most major demographic factors have not changed much over time. However, the average age of new members is increasing. Also, a significant portion of the respondents report being strictly active in a non-observing capacity, reflecting the growing mission of the organization. Motivations of participants are more aligned with scientific contribution than with that reported by other citizen science projects. This may help explain why a third of all respondents are an author or co-author of a paper in an astronomical journal. Finally, there is some evidence that participation in the AAVSO has a greater impact on the respondents' view of their role in astronomy compared to that expected through increasing amateur astronomy experience alone.

Catalog of infrared observations including: Bibliography of infrared astronomy and index of infrared source positions

NASA Technical Reports Server (NTRS)

Gezari, D. Y.; Schmitz, M.; Mead, J. M.

1984-01-01

The Catalog of Infrared Observations and its Far Infrared Supplement summarize all infrared astronomical observations at infrared wavelengths published in the scientific literature between 1965 and 1982. The Catalog includes as appendices the Bibliography of infrared astronomy which keys observations in the Catalog with the original journal references, and the index of infrared source positions which gives source positions for alphabetically listed sources in the Catalog. The Catalog data base contains over 85,000 observations of about 10,000 infrared sources, of which about 2,000 have no known visible counterpart.

Investigating the Nuclear Activity of Barred Spiral Galaxies: The Case of NGC 1672

DTIC Science & Technology

2011-06-10

filters, plus the narrowband F658N (Hα) filter. A large dither was implemented, covering the dimensions of one of the WFC chips in order to fit the...The Astrophysical Journal, 734:33 (20pp), 2011 June 10 doi:10.1088/0004-637X/734/1/33 C© 2011. The American Astronomical Society. All rights reserved...Colbert2, B. Koribalski5, K. D. Kuntz2, A. J. Levan6, R. Ojha7, T. P. Roberts8, M. J. Ward8, and A. Zezas9 1 Laboratory for X-ray Astrophysics , NASA

The measurement procedure in the SEMONT monitoring system.

PubMed

Djuric, Nikola; Kljajic, Dragan; Kasas-Lazetic, Karolina; Bajovic, Vera

2014-03-01

The measurement procedure of the open area in situ electric field strength is presented, acquiring the real field data for testing of the Serbian electromagnetic field monitoring network (SEMONT) and its Internet portal. The SEMONT monitoring system introduces an advanced approach of wireless sensor network utilization for the continuous supervision of overall and cumulative level of electromagnetic field over the observed area. The aim of the SEMONT system is to become a useful tool for the national and municipal agencies for the environmental protection, regarding the electromagnetic pollution monitoring and the exposure assessment of the general population. Considering the public concern on the potentially harmful effects of the long-term exposure to electromagnetic radiation, as well as the public transparency principle that is incorporated into the Serbian law on non-ionizing radiation protection, the SEMONT monitoring system is designed for the long-term continuous monitoring, presenting real-time measurement results, and corresponding exposure assessment over the public Internet network.

[Epilepsy treatment in Serbian medieval monastery hospitals].

PubMed

Ilić-Tasić, Slobodanka; Pantović, Mihailo; Jović, Nebojsa; Ravanić, Dragan; Obradović, Dejan; Sretenović, Srdjan; Pantović, Maja; Pantović, Vesna

2009-01-01

Emperor John III Ducas Vatatzes (ruled from 1222-1254) and his son Theodore II Lascaris (ruled from 1254-1258) both suffered from epilepsy. On his journeys to Nicaea, St Sava visited emperors Theodore I Lascaris (ruled from 1204-1222) and John II Vatatzes, who richly rewarded him, which was probably of crucial importance for the foundation of hospitals in the Monastery of Hilandar and the Monastery of Studenica These hospitals had special departments for the treatment of patints with epilepsy. According to researches conducted up-to-date, these departments are considered to be the oldest institutions for epilepsy treatment. Monastery hospitals in the West served primarily as a shelter for the poor and patients with chronic incurable diseases. The development of Serbian monastery hospitals was a long process and it included institutions that lasted for a long time (for over two centuries) in which, among others, those affected by epilepsy were cured.

Selections from 2017: Image Processing with AstroImageJ

NASA Astrophysics Data System (ADS)

Kohler, Susanna

2017-12-01

Editors note:In these last two weeks of 2017, well be looking at a few selections that we havent yet discussed on AAS Nova from among the most-downloaded paperspublished in AAS journals this year. The usual posting schedule will resume in January.AstroImageJ: Image Processing and Photometric Extraction for Ultra-Precise Astronomical Light CurvesPublished January2017The AIJ image display. A wide range of astronomy specific image display options and image analysis tools are available from the menus, quick access icons, and interactive histogram. [Collins et al. 2017]Main takeaway:AstroImageJ is a new integrated software package presented in a publication led byKaren Collins(Vanderbilt University,Fisk University, andUniversity of Louisville). Itenables new users even at the level of undergraduate student, high school student, or amateur astronomer to quickly start processing, modeling, and plotting astronomical image data.Why its interesting:Science doesnt just happen the momenta telescope captures a picture of a distantobject. Instead, astronomical images must firstbe carefully processed to clean up thedata, and this data must then be systematically analyzed to learn about the objects within it. AstroImageJ as a GUI-driven, easily installed, public-domain tool is a uniquelyaccessible tool for thisprocessing and analysis, allowing even non-specialist users to explore and visualizeastronomical data.Some features ofAstroImageJ:(as reported by Astrobites)Image calibration:generate master flat, dark, and bias framesImage arithmetic:combineimages viasubtraction, addition, division, multiplication, etc.Stack editing:easily perform operations on a series of imagesImage stabilization and image alignment featuresPrecise coordinate converters:calculate Heliocentric and Barycentric Julian DatesWCS coordinates:determine precisely where atelescope was pointed for an image by PlateSolving using Astronomy.netMacro and plugin support:write your own macrosMulti-aperture photometry with interactive light curve fitting:plot light curves of a star in real timeCitationKaren A. Collins et al 2017 AJ 153 77. doi:10.3847/1538-3881/153/2/77

Hungarian topics in Zach's German journals

NASA Astrophysics Data System (ADS)

Patkós, László

Two hundred years ago geography and astronomy were very close branches of science. The great task of the era was the determination of exact geographical positions, and astronomical methods were widely used for it. In the volumes of Allgemeine Geographische Ephemeriden (AGE) and in the Monatliche Correspondenz (MC) a large proportion of the Hungarian topics also deal with the geography of Hungary. One can read news from Hungary in letters written mainly by Schedius and (after 1802) by Lipszky. The most important Hungarian scientific enterprise of the era was the geographical mapping of the country. As part of this work the young astronomer Bogdanich determined many astronomical positions, and he also made various different other astronomical observations too. One of the most spectacular astronomical events of the era was the transit of Mercury in front of the sun on May 7, 1799. The four contacts were determined at many observatories all over Europe, among them at Ofen (Buda), Dubitza and Carlsburg (Gyulaféhervár) in Hungary. The observed second and third contacts were used by Wurm to compute the geographical longitudes of these places (AGE 4 (1799) 218 and MC 8 (1803) 115). Three solar eclipses observed at the beginning of the XIXth century were also used for longitude determinations. In Hungary the eclipses of Aug 27, 1802, and of Aug 17, 1803, were observed at Ofen, and that of Feb 11, 1804, at Carlsburg observatory (Wurm: MC 7 (1805) 351). Another solar eclipse (the one on Jun 16, 1806) was used by the same author to determine the longitudes of Ofen and Erlau (Eger), together with a further 38 other European observatories. (MC 27 (1813) 401). The most common astrometric method for longitude determinations at that time was the observation of occultations. In a table published by Triesnecker (AGE 1 (1798) 284) the geographical position of Buda observatory (Ofen) was based on two solar eclipses and twelve stellar occultations. In a table published in MC 7 (1803) 47-48 there is a list of Hungarian localities with determined positions. The most precise ones are the positions of the astronomical observatories: Carlsburg (in Transylvania), Erlau, Ofen and Tyrnau (Nagyszombat). Further astronomically determined places in the list were the ones determined by Bogdanich as part of his enterprise to map Hungary: Czátza, Dubitza, Fiume, Orsova and Schemnitz. Besides observational work, Hungarian astronomers of the time were recognized as theoreticians too. Pasquich's mathematical knowledge was widely admitted. An example of it is: ``Über die Krümmungs-Ellipsoide für die nördliche Hälfte unserer nördlichen Halbkugel'' (MC 8 (1803) 411-417). Another example is his paper about the reduction of the out of meridian observed zenith distances to the meridian (MC 7 (1805) 460). But praise is not all one can find about Hungarian astronomy. In AGE 3 (1799) 601-612, there is a severe criticism about the activity of the Hungarian astronomer Märtonfy (at Carlsburg) and about a book written by him. Franz Xaver von Zach, the editor of Allgemeine Geographische Ephemeriden and Monatliche Correspondenz, did not get the well-deserved appreciation from his native country. Our duty is to put his name into its well-earned place in the history of Hungarian science.

Book Review: Beitraege zur Astronomiegeschichte, Band 5 (Acta Historica Astronomiae Vol. 15)

NASA Astrophysics Data System (ADS)

Duerbeck, H. W.; Dick, W. R.; Hamel, J.

2002-12-01

The 15th volume of the Acta Historica Astronomiae is at the same time the fifth collection of essays on the history of astronomy (Beitraege zur Astronomiegeschichte, Band 5), edited by the historians of astronomy W.R. Dick (Potsdam) and J. Hamel (Berlin). Besides a few short notices and book reviews, the book contains 11 major articles, which deal with astronomical topics covering the time from the 16th to the 20th centuries. The first article, on the analysis and interpretation of historical horoscopes as a source of the history of science, is based on the inaugural lecture of its author, Guenther Oestmann. After a general introduction, which deals with the principles of horoscope making, the author discusses the horoscope of Count Heinrich Ranzau (1526-1598), the Danish governor of Schleswig-Holstein, who was a friend of Tycho Brahe. Oestmann shows that the astronomical-mathematical basis of such a horoscope can be reconstructed and interpreted. However, it is hardly possible to gain an insight in the process how the interpretation of a horoscope was done in detail. The second and third articles, by Franz Daxecker, deal with Athanasius Kircher and Christoph Scheiner, two catholic astronomers of the 17th century. Kircher's Organum Mathematicum is a calculating device that can be used in the fields of arithmetic, geometry, chronology, astronomy, astrology and others. The author provides extracts of the description of the Organum taken from a book by Caspar Schott, which deal with chronology and astronomy. A photograph of the Organum indicates that this tool consists of a set of tables glued on wooden or cardboard, but details of its contents and applications remain pretty obscure for the reader - a few elaborated examples would have been helpful. The second paper deals with the life of Christoph Scheiner SJ, the co-discoverer of sunspots (next to Galileo), after leaving Rome in 1633 - the year of the Galileo trial. Scheiner spent his later years in the Austrian and Bohemian (Jesuit) provinces, mainly in Vienna and Neisse (the present Nysa in Silesia, Poland), but no traces of further astronomical activity have survived, if they ever existed. The fourth article, by Hans Gaab, is a very thoroughly researched biography of Johann Philipp von Wurzelbau (1651-1725), an merchant turned astronomer from Nuremberg. Wurzelbau started his activities at Christoph Eimmart's (the director of the painters' academy in Nuremberg) private observatory, and his first published work deals with observations of the great comet of 1680. Furthermore, he observed solar eclipses, Mercury transits, and determined the geographical latitude of Nuremberg. The article also contains a detailed description of Wurzelbau's observatory and its instruments. The fifth paper, by Klaus-Dieter Herbst, deals with Gottfried Kirch's idea of founding an astronomical society - being a vehicle to publishing astronomical observations. Kirch (1639-1710) was a well-known astronomer and calendar manufacturer. Around 1700, Kirch was appointed first astronomer at the Brandenburg society of sciences, and director of the observatory that was to be established with the new Berlin Academy. Herbst shows that Kirch's religious attitude that converged on pietism was a driving force to establish a scientific society. However, the final failure of such a project is due to the emergence of the scientific journal Acta Eruditorum, issued since 1682 in Leipzig, which could serve as an outlet for the publication of astronomical data by Kirch and others, thus fulfilling an essential task of the projected academy. Kirch's occupation with the composition of calendars, which took most of his time, was another reason. The following three shorter articles deal with 19th century astronomy. Peter Brosche describes an early visual photometer employed by Johann Gottfried Koehler (1745-1801) in Dresden, Alberto Meschiari edits and comments letters by Franz Xaver von Zach (1754-1832) to the physicist Gerbi in Pisa and the librarian Pozzetti at Bologna, and Karin Reich describes and edits Bessel's book critique of Gauss' Theoria Motus. How many one-time astronomers have to earn their living in other ways, become distracted from astronomical research, and vanish from the horizon of astronomical history? In the ninth paper, Hans-Joachim Ilgauds has traced the life of Georg Koch (1851-1905), who started his career as an astronomer at Leipzig Observatory in 1874. Later Koch worked at Hamburg Observatory, and then became an employee at the statistical office in Kiel, and finally director of the statistical office of the Hamburg revenue service. He was a collaborator for the statistical yearbook of German cities, and also contributed to a book investigating the causes and the impact of the cholera epidemic of 1892 in Hamburg. The last two papers deal with the circumstances of the discovery of the first Near-Earth asteroid (433) Eros. It was recorded on photographic plates taken at the Urania-Sternwarte Berlin and at Nice Observatory. The Berlin observer Witt announced the discovery, and only later, the Nice observer Charlois published a position of Eros. While all plates have disappeared, the authors Hans Scholl and Lutz D. Schmadel could prove that the Nice plate was poorly guided and Charlois would have been unable to discover the object. From a copy of the Berlin plate, published 50 years after the discovery by Witt's co-observer F. Linke, the exact position was determined, and the time of observation (which had not been published) was derived. The second article, by Lutz D. Schmadel, deals with the life of the Eros co-discoverer Felix Linke (1879-1959), who later worked in statistic offices, was a frequent writer of popular scientific articles, and later the editor of a journal, "Technik im Hotel'', and author of a book of the same title. As can be seen from the summaries given above, this collection of essays deals mainly with historical events that occurred in Germany and neighboring countries, and is focussed mainly on events in the 17th to 19th centuries. Except for the Eros article by Scholl and Schmadel, which is written in English, all contributions are written in German. The editors have taken care that generally a high standard was kept. The series appears to be a complement to the Journal for the History of Astronomy, in spite of the fact that its scope is somewhat narrower and somewhat less international. Of course, the use of the German language and the Germany-based small publishing company hampers a wide distribution of this series (but an all-English edition would turn away potential German readers). Nevertheless, it should be noted that English is not necessarily the "lingua franca'' in all cultural fields, and students of the history of science should have at least a cursory knowledge of several languages at their command. It would be nice to see that such a history of astronomy series would also be published in other countries, focussing on the historical events in these regions (French, Italian, Spanish - it should be mentioned that a series Istoriko-astronomicheskie issledovaniia has appeared since 1955 in Moscow). In any case, the editors should be congratulated in having established (with a lot of personal engagement) a flourishing book series. I hope that their venture may serve as an example for others.

Symptoms of depression and anxiety in Serbian patients with systemic sclerosis: impact of disease severity and socioeconomic factors.

PubMed

Ostojic, Predrag; Zivojinovic, Sladjana; Reza, Tamara; Damjanov, Nemanja

2010-08-01

This study aimed to assess symptoms of depression and anxiety in Serbian patients with systemic sclerosis (SSc) and to estimate the impact of disease severity and socioeconomic factors on development of depression and anxiety in SSc. Thirty-five patients with SSc and 30 age- and gender-matched healthy individuals participated. Symptoms of depression and anxiety were evaluated using the Beck's depression inventory and Zung's anxiety self-assessment scale. We estimated the impact of gender, age, economic status, marital status, disease duration, disease subset (limited or diffuse), and some clinical features on development of depressive symptoms and anxiety in patients with SSc. Symptoms of depression were found in 68.6% of patients (compared with 23.3% in the control group), were more frequent in patients with longer disease duration and in female and older patients, and were more common in unemployed and retired patients than in employed individuals. No differences in anxiety and depressive symptoms was noticed between patients with limited and diffuse SSc or those with or without restrictive lung disease, pulmonary hypertension, finger-tip ulcers, and heart involvement. Symptoms of depression were associated with severe pain. Symptoms of anxiety were found in 80% of patients compared with 13.3% of healthy individuals and were equally as frequent in patients of different gender, age, socioeconomic status, and disease duration and severity. Symptoms of depression and anxiety are common in Serbian patients with SSc. Depressive symptoms depended mostly on socioeconomic factors, disease duration, and pain intensity, whereas disease severity had no significant impact on development of depressive symptoms and anxiety.

DR AVRAM JOZEF VINAVER (1862-1915) - PIONEER OF RADIOLOGY IN SERBIA.

PubMed

Babić, Rade Radomir; Stanković Babić, Gordana

2015-01-01

Dr Abraham Joseph Vinaver (1862-1915), a Jew from Poland, was a pioneer of radiology in Serbia. He graduated from the Faculty of Medicine in Warsaw (1887), but lived and worked in abac (the Kingdom of Serbia) since 1890. Dr Abraham Joseph Vinarev - Career Development. He procured the first X-ray machine and developed radiological service in Sabac five years after the discovery of X-rays. These were the beginnings of radiology in Serbia. He introduced the application of artesian wells. Dr Abraham Joseph Vinarev - a Participant at the First Congress of Serbian Physicians and Naturalists, Belgrade 1904. "The diagnostic importance of X-rays in lung disease, especially in initial tuberculosis" and "Five Years of Treatment by X-Ray Machines" were the first works in the field of radiology in Serbia by this author. Dr Abraham Joseph Vinaver - Reserve Medical Officer in the Serbian Army. During the Balkan Wars, he was a volunteer with the rank of major engaged in military corps and he participated in the First World War as well. He died of malaria in 1915 in Gevgelija. "Dr Avram Vinaver"- Stanislav Vinarev. His dedication to work during the typhus epidemics was put into verses of a poem by his son Stanislav Vinarev. Dr Avram Vinaver Joseph was a noble man with a great heart, who selflessly sacrificed himself for the Serbian people and Serbia. He gave his contribution to the development of health services in Serbia, both in peacetime and wartime conditions. Dr Abraham Joseph Vinaver laid the foundations for today's radiology in Serbia.

Knowledge of, beliefs about, and perceived barriers to organ and tissue donation in Serbian, Macedonian, and Greek Orthodox communities in Australia.

PubMed

Phillipson, Lyn; Larsen-Truong, Karen; Pitts, Leissa; Nonu, Miriam

2015-03-01

Despite the lifesaving benefits of organ and tissue donation, a worldwide shortage of suitable and registered donors exists. Although the reasons for this shortage are multifactorial, it has been recognized that distinct barriers to registration, family discussion, and consent that require targeted intervention and action are present among minority cultural, religious, and immigrant communities. To explore the knowledge, attitudes, and beliefs of 3 orthodox religious communities in Australia (Macedonian, Greek, and Serbian Orthodox) and determine the implications for engaging with these communities to improve knowledge, attitudes, family discussion, and the ability to make an informed decision about donation. Qualitative approach using focus groups moderated by researchers and bicultural health workers with the assistance of accredited interpreters. 98 adult members of the Greek, Macedonian, and Serbian Orthodox communities in the Illawarra region of New South Wales, Australia. Clear barriers to discussing and making an informed decision about organ and tissue donation were identified. Knowledge of processes and procedures was low and discussion about death (and organ and tissue donation) with family members and loved ones was considered taboo. Despite these barriers, all 3 communities expressed a desire for more information and engagement. Of particular interest were the perspectives of 3 types of "experts": medical, religious, and other community members (who had experience with the organ and tissue donation system). Future programs designed for orthodox religious communities should consider the need for active strategies that facilitate information sharing and engagement between community members and these 3 types of experts.

Clinical Research Involving Minors in International and Serbian Regulations

PubMed Central

PLANOJEVIĆ, Nina; ŽIVOJINOVIĆ, Dragica

2013-01-01

Background: Participation in clinical trials can be useful for the health of a person, in who it is conducted, but it does not have to be – it can even be harmful. Therefore, primary motive to accept such risk is humanity and human wish to contribute to the progress of medicine; this is expressed by personal consent. The consent, however, can be an expression of personal humanity, and for this, it is not logical that someone can give consent on behalf of someone else, as it is done by a legally authorized representative on behalf of a minor. Therefore, authors raise 3 questions: What are the reasons to consider representative’s consent acceptable? How should a model of regulations look like in order to provide the most complete possible protection to a minor? Is actual regulation of minors’ position within international and Serbian law, analyzed here by authors for their specific solutions, acceptable? Representative’s consent is acceptable only for therapeutic research, because these can bring benefits to everyone’s health, including a minor in which those are conducted – this is an acceptable (secondary) motive of participation in the research. Expression of humanity on other’s behalf, typical for non-therapeutic research, is not acceptable; this makes ban of minors’ participation in non-therapeutic research more appropriate regulation model. International regulations are not in accordance to results presented in the paper for allowing participation of minors both in therapeutic and non-therapeutic research. Serbian regulation is closer to the most acceptable regulation model. PMID:24455493

Cancer incidence and mortality in Serbia 1999–2009

PubMed Central

2013-01-01

Background Despite the increase in cancer incidence in the last years in Serbia, no nation-wide, population-based cancer epidemiology data have been reported. In this study cancer incidence and mortality rates for Serbia are presented using nation-wide data from two population-based cancer registries. These rates are additionally compared to European and global cancer epidemiology estimates. Finally, predictions on Serbian cancer incidence and mortality rates are provided. Methods Cancer incidence and mortality was collected from the cancer registries of Central Serbia and Vojvodina from 1999 to 2009. Using age-specific regression models, we estimated time trends and predictions for cancer incidence and mortality for the following five years (2010–2014). The comparison of Serbian with European and global cancer incidence/mortality rates, adjusted to the world population (ASR-W) was performed using Serbian population-based data and estimates from GLOBOCAN 2008. Results Increasing trends in both overall cancer incidence and mortality rates were identified for Serbia. In men, lung cancer showed the highest incidence (ASR-W 2009: 70.8/100,000), followed by colorectal (ASR-W 2009: 39.9/100,000), prostate (ASR-W 2009: 29.1/100,000) and bladder cancer (ASR-W 2009: 16.2/100,000). Breast cancer was the most common form of cancer in women (ASR-W 2009: 70.8/100,000) followed by cervical (ASR-W 2009: 25.5/100,000), colorectal (ASR-W 2009: 21.1/100,000) and lung cancer (ASR-W 2009: 19.4/100,000). Prostate and colorectal cancers have been significantly increasing over the last years in men, while this was also observed for breast cancer incidence and lung cancer mortality in women. In 2008 Serbia had the highest mortality rate from breast cancer (ASR-W 2008: 22.7/100,000), among all European countries while incidence and mortality of cervical, lung and colorectal cancer were well above European estimates. Conclusion Cancer incidence and mortality in Serbia has been generally increasing over the past years. For a number of cancer sites, incidence and mortality is alarmingly higher than in the majority of European regions. For this increasing trend to be controlled, the management of risk factors that are present among the Serbian population is necessary. Additionally, prevention and early diagnosis are areas where significant improvements could still be made. PMID:23320890

Cancer incidence and mortality in Serbia 1999-2009.

PubMed

Mihajlović, Jovan; Pechlivanoglou, Petros; Miladinov-Mikov, Marica; Zivković, Snežana; Postma, Maarten J

2013-01-15

Despite the increase in cancer incidence in the last years in Serbia, no nation-wide, population-based cancer epidemiology data have been reported. In this study cancer incidence and mortality rates for Serbia are presented using nation-wide data from two population-based cancer registries. These rates are additionally compared to European and global cancer epidemiology estimates. Finally, predictions on Serbian cancer incidence and mortality rates are provided. Cancer incidence and mortality was collected from the cancer registries of Central Serbia and Vojvodina from 1999 to 2009. Using age-specific regression models, we estimated time trends and predictions for cancer incidence and mortality for the following five years (2010-2014). The comparison of Serbian with European and global cancer incidence/mortality rates, adjusted to the world population (ASR-W) was performed using Serbian population-based data and estimates from GLOBOCAN 2008. Increasing trends in both overall cancer incidence and mortality rates were identified for Serbia. In men, lung cancer showed the highest incidence (ASR-W 2009: 70.8/100,000), followed by colorectal (ASR-W 2009: 39.9/100,000), prostate (ASR-W 2009: 29.1/100,000) and bladder cancer (ASR-W 2009: 16.2/100,000). Breast cancer was the most common form of cancer in women (ASR-W 2009: 70.8/100,000) followed by cervical (ASR-W 2009: 25.5/100,000), colorectal (ASR-W 2009: 21.1/100,000) and lung cancer (ASR-W 2009: 19.4/100,000). Prostate and colorectal cancers have been significantly increasing over the last years in men, while this was also observed for breast cancer incidence and lung cancer mortality in women. In 2008 Serbia had the highest mortality rate from breast cancer (ASR-W 2008: 22.7/100,000), among all European countries while incidence and mortality of cervical, lung and colorectal cancer were well above European estimates. Cancer incidence and mortality in Serbia has been generally increasing over the past years. For a number of cancer sites, incidence and mortality is alarmingly higher than in the majority of European regions. For this increasing trend to be controlled, the management of risk factors that are present among the Serbian population is necessary. Additionally, prevention and early diagnosis are areas where significant improvements could still be made.

Algol: An Early Candidate for a Transiting Exoplanet

NASA Astrophysics Data System (ADS)

French, Linda M.; Stuart, I.

2008-09-01

Virtually every astronomy text credits John Goodricke (1764-1786) with the discovery of the period of variability of the star Algol (β Per) and with the explanation of its variation (eclipses by an unseen stellar companion). Today, Algol is considered a prototype of an eclipsing binary star. In actuality, John Goodricke worked in collaboration with his neighbor, mentor, and distant relative, Edward Pigott. As observed by Hoskin1, the observing journals2 of the two clearly show that the eclipse explanation originated with Edward. Both originally used the term "planet” to describe the eclipsing body. However, in Goodricke's 1783 paper describing Algol, he writes: "....I should imagine it could hardly be accounted for otherwise than either by the interposition of a large body revolving round Algol, or some kind of motion of its own, whereby part of its body, covered with spots or such like matter...."3 Goodricke was later to soften his stance still further after the two discovered several other variable stars; his last published work4 mentions only starspots as an explanation for the light variation of Algol. Although the physics of the time would not have allowed Goodricke and Pigott to distinguish between a star and a planet as the unseen companion, the eighteenth-century astronomers showed great prescience in realizing that the eclipses of Algol were just that. Their mental leap, at a time when astronomers were just beginning to think seriously of discovering planets around other stars, should not go unremembered by modern planetary scientists. Footnotes 1 Hoskin, M. (1982). In Stellar Astronomy, Science History Publications Ltd., Chalfont St. Giles, England. 2 Goodricke and Pigott journals. York City Archives, York, England. 3 Goodricke, J. G. (1783). Phil. Soc. Roy. Soc. London 73, 474-482. 4 Goodricke, J. G. (1786). Phil. Soc. Roy. Soc. London 76, 48-61.

NITARP: Impact Assessment, 2005-2013

NASA Astrophysics Data System (ADS)

Rebull, Luisa M.; Gorjian, V.; Brinkworth, C.; Squires, G. K.; Burtnyk, K.

2014-01-01

NITARP, the NASA/IPAC Training in Archival Research Program, gets educators involved in authentic astronomical research. We partner small groups of educators with a mentor professional astronomer for a year-long original research project. The educators incorporate the experience into their classrooms and share their experience with other teachers. The teams echo the entire research process, from writing a proposal, to doing the research, to writing up and presenting the results at an AAS meeting. The educators incorporate this experience into their classroom. This program differs from other programs that we know of that get real astronomy data into the classroom in that: (a) Each team works on an original, unique project. There are no canned labs here! (b) Each team presents their results in posters at the AAS, in science sessions (not just outreach sessions). The posters are distributed throughout the meeting, in amongst other researchers' work; the participants are not "given a free pass" because they are teachers. (c) The 'product' of this project is the scientific result, not a curriculum packet. (d) Because the teachers work with students throughout this project, the teachers have already begun to adapt their project to fit in their classroom environment. This poster will describe the program, with highlights of an impact assessment survey conducted of NITARP alumni in June 2013. Including all forms of the project from 2004-2013, there have been 80 educator participants from 33 states; 40 of them responded to our survey. There have been 37 science and 42 education AAS posters presented by NITARP-affiliated educators and scientists (with 8 more expected to be presented at this meeting). There have been 5 refereed journal articles in professional astronomy research journals that directly involve NITARP teachers and scientists (Howell et al. 2006, Guieu et al. 2010, Howell et al. 2008, Rebull et al., 2011, 2013), and 2 more astronomy journal articles describing the software developed in conjunction with NITARP and its Spitzer (Laher et al. 2012ab). There is one more refereed article written by a NITARP alumni teacher for The Physics Teacher (Pereira et al. 2013).

76 FR 34123 - Determination Related to Serbia Under Section 7072(c) of the Department of State, Foreign...

Federal Register 2010, 2011, 2012, 2013, 2014

2011-06-10

... consistent with the Dayton Accords to end Serbian financial, political, security and other support which has... which reflect a respect for minority rights and the rule of law. This Determination and related...

75 FR 33376 - Determination Related to Serbia Under Section 7072(c) of the Department of State, Foreign...

Federal Register 2010, 2011, 2012, 2013, 2014

2010-06-11

... to end Serbian financial, political, security and other support which has served to maintain separate... minority rights and the rule of law. This Determination and related Memorandum of Justification shall be...

JPRS Report, East Europe.

DTIC Science & Technology

1990-09-27

members are almost without exception humanistic intellectuals, but we would nevertheless like to stay "down to earth". As a social club, we took the...distinguished figures (General Nedic, Mihailovic, and Djujic), and he completely separated that behavior from the Serbian existential context, from

Progress by the JWST Science Working Group

NASA Technical Reports Server (NTRS)

Gardner, Jonathan P.

2007-01-01

The JWST Science Working Group recently published a comprehensive, top-level review of JWST science in the journal Space Science Reviews (Gardner et al. 2006, SSR, 123, 485). That review paper gives details of the 4 JWST science themes, and describes the design of the observatory and ground system. Since publication, the SWG, working with members of the astronomical community, has continued to develop the science case for JWST, giving more details in a series of white papers. The white paper topics include first light, galaxy surveys, AGN, supernovae, stellar populations, and exoplanets. The white papers are in various stages of completion. In this poster, I will review recent progress.

A retrospective of the GREGOR solar telescope in scientific literature

NASA Astrophysics Data System (ADS)

Denker, C.; von der Lühe, O.; Feller, A.; Arlt, K.; Balthasar, H.; Bauer, S.-M.; Bello González, N.; Berkefeld, Th.; Caligari, P.; Collados, M.; Fischer, A.; Granzer, T.; Hahn, T.; Halbgewachs, C.; Heidecke, F.; Hofmann, A.; Kentischer, T.; Klva{ňa, M.; Kneer, F.; Lagg, A.; Nicklas, H.; Popow, E.; Puschmann, K. G.; Rendtel, J.; Schmidt, D.; Schmidt, W.; Sobotka, M.; Solanki, S. K.; Soltau, D.; Staude, J.; Strassmeier, K. G.; Volkmer, R.; Waldmann, T.; Wiehr, E.; Wittmann, A. D.; Woche, M.

2012-11-01

In this review, we look back upon the literature, which had the GREGOR solar telescope project as its subject including science cases, telescope subsystems, and post-focus instruments. The articles date back to the year 2000, when the initial concepts for a new solar telescope on Tenerife were first presented at scientific meetings. This comprehensive bibliography contains literature until the year 2012, i.e., the final stages of commissioning and science verification. Taking stock of the various publications in peer-reviewed journals and conference proceedings also provides the ``historical'' context for the reference articles in this special issue of Astronomische Nachrichten/Astronomical Notes.

An Atlas of O-C Diagrams of Eclipsing Binary Stars

NASA Astrophysics Data System (ADS)

Kreiner, Jerzy M.; Kim, Chun-Hwey; Nha, Il-Seong

The Atlas contains data for 1,138 eclipsing binaries represented by 91,798 minima timings, collected from the usual international and local journals, observatory publications and unpublished minima. Among this source material there is a considerable representation of amateur astronomers. Some timings were found in the card-index catalogue of the Astronomical Observatory of the Jagiellonian University, Cracow. Stars were included in the Atlas provided that they satisfied 3 criteria: (1) at least 20 minima had been times; (2) these minima spanned at least 2,500 cycles; and (3) the 2,500 cycles represented no fewer than 40 years. Some additional stars not strictly satisfying these criteria were also included if useful information was available. For each star, the Atlas contains the (O-C) diagram calculated by the authors and a table of general information containing: binary characteristics; assorted catalogue numbers; the statistics of the collected minima timings; the light elements (light ephemeris); comments and literature references. All of the data and diagrams in the Atlas are also available in electronic form on the Internet at http://www.as.ap.krakow.pl/o- c".

Ms. Hisako Koyama: From Amateur Astronomer to Long-Term Solar Observer

NASA Astrophysics Data System (ADS)

Knipp, Delores; Liu, Huixin; Hayakawa, Hisashi

2017-10-01

The path to science for a girl of any nationality born in the early twentieth century was formidable-to-nonexistent. Yet paths were forged by a few. We present the little-known story of one of Japan's premier solar observers and her contribution to the world's understanding of sunspots and space weather cycles. Ms. Hisako Koyama, born in Tokyo in 1916, became a passionate amateur astronomer, a dedicated solar observer, and a long-serving staff member of the National Museum of Nature and Science, Tokyo. As a writer for amateur astronomy journals she advised many on the details and joys of sky viewing. She created a consistent, extended record of sunspots. Her multidecade archive of sunspot drawings is one of the "backbones" for the recent international recalibration of the sunspot record that provides insight into space weather reaching back to the early 1600s. We detail her contributions to the citizens of Japan as an ambassador of astronomy and her international contribution to understanding the symmetries and asymmetries of the solar cycle. We comment on the value of her continuous record of sunspots and on her tenacity in promoting a science that links to space weather.

The Cincinnati Observatory as a Research Instrument for Undergraduate Research

NASA Astrophysics Data System (ADS)

Abel, Nicholas; Regas, Dean; Flateau, Davin C.; Larrabee, Cliff

2016-06-01

The Cincinnati Observatory, founded in 1842, was the first public observatory in the Western Hemisphere. The history of Cincinnati is closely intertwined with the history of the Observatory, and with the history of science in the United States. Previous directors of the Observatory helped to create the National Weather Service, the Minor Planet Center, and the first astronomical journal in the U.S. The Cincinnati Observatory was internationally known in the late 19th century, with Jules Verne mentioning the Cincinnati Observatory in two of his books, and the Observatory now stands as a National Historic Landmark.No longer a research instrument, the Observatory is now a tool for promoting astronomy education to the general public. However, with the 11" and 16" refracting telescopes, the Observatory telescopes are very capable of collecting data to fuel undergraduate research projects. In this poster, we will discuss the history of the Observatory, types of student research projects capable with the Cincinnati Observatory, future plans, and preliminary results. The overall goal of this project is to produce a steady supply of undergraduate students collecting, analyzing, and interpreting data, and thereby introduce them to the techniques and methodology of an astronomer at an early stage of their academic career.

WHO European Childhood Obesity Surveillance Initiative in Serbia: a prevalence of overweight and obesity among 6-9-year-old school children.

PubMed

Djordjic, Visnja; Radisavljevic, Snezana; Milanovic, Ivana; Bozic, Predrag; Grbic, Miljana; Jorga, Jagoda; Ostojic, Sergej M

2016-09-01

The World Health Organization (WHO) European Childhood Obesity Surveillance Initiative (COSI) is a public health program established in order to understand the progress of the obesity epidemic in young populations and gain inter-country comparisons within the European region, yet the data from a number of East European countries, including Serbia, were not available then. Therefore, the main aim of this cross-sectional study was to collect data about the prevalence of overweight and obesity among 6-9-year-old school children in Serbia according to the standardized protocol during the Fourth COSI Implementation Round. From September 2015 to November 2015, 5102 first- and second-grade primary-school children (age 7.7±0.6 years) were assessed for weight, height, and body mass index (BMI) in 14 Serbian school districts. The prevalence rates of obesity, as calculated using the International Obesity Task Force (IOTF) cut-off points, vary across different age groups, with the lowest obesity rates reported in 7-year-old boys (6.2%), while the highest obesity prevalence rates were observed in 6-year-old boys (9.7%). In addition, being overweight was strongly associated with poor local community development and lower level of urbanization. The overall prevalence of overweight (23.1%, including obesity) and obesity (6.9%) in Serbian primary-school children seem to be comparable to rather high rates previously reported in other countries participating in the COSI program, indicating an obesity epidemic in Serbian children. This surveillance system should be regularly implemented throughout Europe, providing comparable data on rates of overweight/obesity in primary schools that might drive prudent actions to reverse the pandemic trend of childhood obesity.

Validation of the Temps-A in university student population in Serbia.

PubMed

Hinić, Darko; Akiskal, S Hagop; Akiskal, K Kareen; Jović, Jelena; Ignjatović Ristić, Dragana

2013-07-01

The TEMPS-A scale is a self-evaluation measure which assesses five affective temperaments. This study is a comparative analysis of affective temperament types in different educational fields, and the first validation of the Serbian version of the TEMPS-A. The TEMPS-A questionnaire has been adapted following the translation-back translation methodology from English to Serbian. It was then administered to 770 undergraduate students from eight different faculties. Five factors were extracted through Principal Component Analysis (Varimax rotation), each including ten items with loadings above 0.40. The internal consistency of this abbreviated 50-item scale was α=0.77 and the average test-retest coefficient (rho=0.82) indicates a stable reliability. The correlations among the temperaments ranged from weak to moderate, with the highest positive correlations obtained between the depressive and cyclothymic, and, depressive and anxious scales. The highest score was detected among the hyperthymic (0.64) and lowest among the depressive temperament (0.15). The male participants attained significantly higher scores for the hyperthymic temperament, while female scored significantly higher on the depressive and anxious temperaments. The students of physical education showed significantly lower results on the depressive and anxious subscales and higher on the hyperthymic, in comparison to other educational fields. The student sample is not representative of the general population, therefore further investigation in older population would be necessary for the evaluation of norms in additional age categories. The external validation with other personality scales has not been the subject of this research, but will be a part of some future studies. The Serbian 50-item version of the TEMPS-A showed good overall internal consistency and reliability, and the results generally cohere with those from previously validated versions in other languages. Copyright © 2013 Elsevier B.V. All rights reserved.

First insights into the genetic diversity of Echinococcus granulosus sensu stricto (s.s.) in Serbia.

PubMed

Debeljak, Zoran; Boufana, Belgees; Interisano, Maria; Vidanovic, Dejan; Kulisic, Zoran; Casulli, Adriano

2016-06-15

Cystic echinococcosis (CE) caused by Echinococcus granulosus sensu stricto (s.s.) is a cosmopolitan zoonotic infection which is endemic in Serbia where it is subject to mandatory reporting. However, information on the incidence of the disease in humans and prevalence of hydatid infection in livestock remains limited. We used sequenced data of the cytochrome c oxidase subunit 1 (cox 1) mitochondrial gene to examine the genetic diversity and population structure of E. granulosus (s.s.) from intermediate hosts from Serbia. We also compared our generated nucleotide sequences with those reported for neighbouring European countries. Echinococcus canadensis was molecularly confirmed from pig and human hydatid isolates. E. granulosus (G1) was confirmed from sheep and cattle hydatid isolates as well as the first molecular confirmation in Serbia of E. granulosus G2 in sheep and E. granulosus G3 in sheep and cattle hydatid isolates. The Serbian E. granulosus (s.s.) parsimony network displayed 2 main haplotypes (SB02 and SB05) which together with the neutrality indices were suggestive of bottleneck and/or balancing selection. Haplotype analysis showed the presence of the common E. granulosus haplotype described from other worldwide regions. Investigation of the pairwise fixation (Fst) index suggested that Serbian populations of E. granulosus (s.s.) from sheep and cattle hosts showed moderate genetic differentiation. Six of the Serbian haplotypes (SB02-SB07) were shared with haplotypes from Bulgaria, Hungary and/or Romania. Further studies using a larger number of hydatid isolates from various locations across Serbia will provide more information on the genetic structure of E. granulosus (s.s.) within this region. Copyright © 2016 Elsevier B.V. All rights reserved.

eHealth and adolescents in Serbia: psychometric properties of eHeals questionnaire and contributing factors to better online health literacy.

PubMed

Gazibara, Tatjana; Cakic, Jelena; Cakic, Milica; Pekmezovic, Tatjana; Grgurevic, Anita

2018-05-25

Internet is important resource of health-related information and health services. Factors associated with higher level of online health (eHealth) literacy among adolescence have been understudied. The aim of this study was to assess psychometric properties of the eHealth Literacy Scale (eHEALS) in Serbian language and to evaluate eHealth literacy among adolescents in Serbia. The study was carried out in four high schools in Belgrade, Serbia in the period December 2016 to January 2017. A total of 702 students comprised the study sample. The eHEALS was translated according to internationally accepted methodology and its psychometric properties were analyzed. The Cronbach's alpha coefficient for the entire eHEALS was 0.849. On exploratory factor analysis we obtained two-factorial structure. Our adolescents reported low confidence in knowing what health resources are available online. High confidence was observed for knowing how to use and how to find health information online. There was no difference in eHEALS score between genders or between school years. After adjustment for gender, type of school program, parental marital status, fathers' education level and household income, being female was associated with higher eHealth literacy (B = 1.12, 95% confidence interval 0.07-2.18; p = 0.036). Serbian version of the eHEALS is a valid instrument in assessment of online health literacy and can be further used in evaluation of eHealth literacy in other population groups in Serbian language. It is advised that some classes in school are dedicated to appraisal and use of online health websites. This could be achieved through peer-education.

Carboxy-terminal sequence variation of LMP1 gene in Epstein-Barr-virus-associated mononucleosis and tumors from Serbian patients.

PubMed

Banko, Ana; Lazarevic, Ivana; Cupic, Maja; Stevanovic, Goran; Boricic, Ivan; Jovanovic, Tanja

2012-04-01

Seven strains of Epstein-Barr virus (EBV) are defined based on C-terminal sequence variations of the latent membrane protein 1 (LMP1). Some strains, especially those with a 30-bp deletion, are thought to be related to tumorigenic activity and geographical localization. The aims of the study were to determine the prevalence of different LMP1 strains and to investigate sequence variation in the C-terminal region of LMP1 in Serbian isolates. This study included 53 EBV-DNA-positive plasma and tissue block samples from patients with mononucleosis syndrome, renal transplantation, and tumors, mostly nasopharyngeal carcinoma. The sequence of the 506-bp fragment of LMP1 C terminus was used for phylogenetic analyses and identification of LMP1 strains, deletions, and mutations. The majority of isolates were non-deleted (66%), and the rest had 30-bp, rare 69-bp, or yet unknown 27-bp deletions, which were not related to malignant or non-malignant isolate origin. However, the majority of 69-bp deletion isolates were derived from patients with nasopharyngeal carcinoma. Less than five 33-bp repeats were found in the majority of non-deleted isolates (68.6%), whereas most 69-bp deletion isolates (75%) had five or six repeats. Serbian isolates were assigned to four LMP1 strains: B95-8 (32.1%), China 1 (24.5%), North Carolina (NC; 18.9%), and Mediterranean (Med; 24.5%). In NC isolates, three new mutations unique for this strain were identified. EBV EBNA2 genotypes 1 and 2 were both found, with dominance of genotype 1 (90.7%). This study demonstrated noticeable geographical-associated characteristics in the LMP1 C terminus of investigated isolates. Copyright © 2012 Wiley Periodicals, Inc.

Scottish Women's Hospitals--the 90th anniversary of their work in Serbia.

PubMed

Mikić, Zelimir

2005-01-01

The Scottish Women's Hospitals (SWH), a unique health institution in the history of medicine, staffed entirely by women, was founded soon after the outbreak of the First World War, August 12, 1914 in Edinburgh, by the National Union of Women's Suffrage Societies. The founder and the main driving force behind this organisation was Dr. Elsie Inglis (1864-1917). Although her proposition to the British War Office had been rejected, she offered her services to the Allies (France, Belgium, Russia and Serbia). The first 200 bed SWH unit was sent to France in November 1914, and soon after followed other units, so at the end there were 13 very well equipped SWH units working in the various theatres of war in Belgium, Serbia, Russia, Rumania and Greece. The first unit of SWH came to Serbia in early January 1915, and was located at Kragujevac. Soon after, three other SWH units arrived to Serbia and were stationed at Mladenovac, Valjevo and Lazarevac. It was an enormous help to Serbia, full of wounded and sick people, due to the dreadful typhus epidemic which was devastating the country. A large SWH unit, attached to the Southern Slav Volunteer Division, had worked on the Dobrudja front, and there were three hospitals and a special transport unit on the Salonika Front, which were all engaged in the treatment of Serbian wounded soldiers until the end of the First World War. Two other SWH units, located in France, were treating the Serbian refugees. Serving bravely and honorably on the various theatres of war, the legendary Scottish Women's Hospitals made enormous contributions to the allied war efforts, and helped Serbian people a great deal.

Menopausal transition in Southern Europe: comparative study of women in Serbia and Portugal.

PubMed

Dotlic, Jelena; Pimenta, Filipa; Kovacevic, Nikolina; Leal, Isabel; Maroco, Joao; Utian, Wulf; Gazibara, Tatjana

2017-11-01

The aim of this study was to assess and compare general menopausal quality of life in Serbia and Portugal. In all, 1,503 women aged between 40 and 65 years from Belgrade, Serbia, and Lisbon, Portugal, were included in the study. A sociodemographic questionnaire and the Utian Quality of Life (UQOL) scale were used in data collection. The average age of women was 50 (SD = 5.61) years. Serbian and Portuguese women differed in all sociodemographic characteristics except for body mass index (BMI) and relationship status. There were no significant differences in UQOL total score (P = 0.629) or UQOL sexual score (P = 0.396) between Serbian and Portuguese women. However, occupational (P < 0.001) and health (P = 0.003) scores were significantly higher in the Serbian sample, whereas Portuguese women had higher emotional scores (P < 0.001). Based on the total study sample, women with an average UQOL score were more highly educated, employed, non-smokers, and physically active, and more likely to obtain medical assistance for climacteric symptoms compared with women who reported lower UQOL score. In addition to these characteristics, women with a higher UQOL score had higher annual income, no recent illnesses, and optimal BMI compared with women who reported a lower UQOL score. This study showed that diverse populations of midlife women can have similar perceptions of quality of life as it encompasses broad dimensions of menopausal somatic and psychosocial symptoms, as well as habits and lifestyle. Further comparative studies using the UQOL scale are warranted to offer more information on the delicate factors influencing well-being in climacteric women worldwide.

Motivation and job satisfaction of health workers in a specialized health institution in Serbia.

PubMed

Djordjević, Dragan; Petrović, Dejan; Vuković, Dejana; Mihailović, Dobrivoje; Dimić, Aleksandar

2015-08-01

Health care system is specific for each country, and therefore involves different motivation and job satisfaction factors. The aim of this study was to confirm the validity and applicability of the General Nordic Questionnaire translated into Serbian for analyzing motivation and job satisfaction, as well as to analyze the motivation factors and job satisfaction of health workers at the Institute for Treatment and Rehabilitation "Niska Banja". The General Nordic Questionnaire was translated into Serbian. It included 73 questions (5 answers by the Likert scale), which formed 24 scales. In May, 2012, 196 (82.3%) health workers filled in the questionnaire. A correlation of Ceronbach's alpha values between the Scandinavian study results and the results of Serbian study was statistically significant (r = 0.424; p < 0.05). The lowest Cronbach' alfa coefficient was for the scale "learning demand in job demands" (alpha 0.28). The other scale with no satisfactory reliability was "control of work pacing" (alpha 0.46). Intrinsic motivation positively correlated with all the scales of organizational module, apart from inequality. Within this module, the degree of extrinsic motivation correlated with the support from the superior and coworkers, with fair leadership and human resources primacy. A negative correlation appeared with inequality. The general Nordic Questionnaire can be applied to a great extent to the conditions in our country. Our study shows a low consistency of the scales learning job demands, control of decision, control of work pacing, so the questions in them should be adjusted to the conditions in our country. Extrinsic motivation resulted in higher values than the values of intrinsic motivation in our workers, which is opposite to the results of the original questionnaire.

The pioneers of interplanetary communication: From Gauss to Tesla

NASA Astrophysics Data System (ADS)

Raulin-Cerceau, Florence

2010-12-01

The present overview covers the period from 1820 to the beginning of the 20th century. Emphasis is laid on the latter half of the 19th century because many efforts have been done at that time to elaborate schemes for contacting our neighboring planets by interplanetary telegraphy. This period knew many advances not only in planetary studies but also in the nascent field of telecommunications. Such a context led astronomers who were also interested in the problem of planetary habitability, to envisage that other planets could be contacted, especially the planet Mars. Interplanetary communication using a celestial telegraphy was planned during this period of great speculations about life on Mars. This paper focuses on four authors: the Frenchmen C. Flammarion, Ch. Cros, A. Mercier and the Serbian N. Tesla, who formulated early proposals to communicate with Mars or Venus. The first proposals (which remained only theoretical) showed that an initial reflection had started as early as the second part of the 19th century on the type of language that could be both universal and distinguishable from a natural signal. Literary history of interplanetary communication preceded by far the scientific one. Authors of the 1900s were very prolific on this topic. French fictions are mentioned in this paper as examples of such a literature. This incursion into selected texts stresses the fact that the problem of techniques and messages employed to communicate with other planets goes beyond the strict scientific framework. Finally, this paper aims to highlight the similarities as well as the differences between the different proposals and to underline what that could possibly help present SETI research to define messages supposed to be sent to other planetary systems.

East Europe Report, Political, Sociological and Military Affairs

DTIC Science & Technology

1984-07-25

the Serbian LC." Speaker: Milomir Petrovic. Attendance: 520. DOB 15 May 1983. "Miladin Zivotic: Revolution and Culture." Speakers: Veljko Korac...Milosevic, Esad Cimic, Dimitrije Rupel, Igor Mandic , Dobroslav Smiljanic and Boro Krivokapic. Attendance: 450. DOB 6 April 1983. "Predrag Matvejevic

Statistical analysis of electromagnetic radiation measurements in the vicinity of GSM/UMTS base station installed on buildings in Serbia.

PubMed

Koprivica, Mladen; Slavkovic, Vladimir; Neskovic, Natasa; Neskovic, Aleksandar

2016-03-01

As a result of dense deployment of public mobile base stations, additional electromagnetic (EM) radiation occurs in the modern human environment. At the same time, public concern about the exposure to EM radiation emitted by such sources has increased. In order to determine the level of radio frequency radiation generated by base stations, extensive EM field strength measurements were carried out for 664 base station locations, from which 276 locations refer to the case of base stations with antenna system installed on buildings. Having in mind the large percentage (42 %) of locations with installations on buildings, as well as the inevitable presence of people in their vicinity, a detailed analysis of this location category was performed. Measurement results showed that the maximum recorded value of total electric field strength has exceeded International Commission on Non-Ionizing Radiation Protection general public exposure reference levels at 2.5 % of locations and Serbian national reference levels at 15.6 % of locations. It should be emphasised that the values exceeding the reference levels were observed only outdoor, while in indoor total electric field strength in no case exceeded the defined reference levels. © The Author 2015. Published by Oxford University Press. All rights reserved. For Permissions, please email: journals.permissions@oup.com.

The Importance of Being a Complement: CED Effects Revisited

ERIC Educational Resources Information Center

Jurka, Johannes

2010-01-01

This dissertation revisits subject island effects (Ross 1967, Chomsky 1973) cross-linguistically. Controlled acceptability judgment studies in German, English, Japanese and Serbian show that extraction out of specifiers is consistently degraded compared to extraction out of complements, indicating that the Condition on Extraction domains (CED,…

JPRS Report, East Europe.

DTIC Science & Technology

1991-03-15

Branko Marjanovic is a recently retired Radio Zadar journalist. He is considered the ideologue of the SDS in the Benkovac and Obrovac area. He...likes to divide forests and rivers into Serbian ones and Croatian ones. The story was told in Zadar that whenever Marjanovic took a day of annual

Clausal Architecture and Sentential Negation in Slavic

ERIC Educational Resources Information Center

Tsurska, Olena Anatoliyivna

2010-01-01

This study presents a comparative analysis of the clausal architecture and sentential negation in East (Russian, Ukrainian, and Belarusian), West, Polish, Czech, Slovak, and Upper and Lower Sorbian), and South (Bulgarian, Macedonian, Bosnian/Croatian/Serbian, and Slovenian) languages. Using the Minimalist Program, I analyze the syntactic structure…

Building Community: A 2005 Conference for Education and Public Outreach Professionals

NASA Astrophysics Data System (ADS)

Slater, T. F.; Bennett, M.; Garmany, K.

2004-12-01

In support of the Astronomical Society of the Pacific's (ASP) mission to increase the understanding and appreciation of astronomy, the ASP will host an international meeting in September 14-16, 2005 in Tucson focused on building and supporting a vibrant and connected community of individuals and groups engaged in educational and public outreach (EPO) in the disciplines of astronomy, astrobiology, space, and earth science. This conference is specially designed for individuals who are bringing the excitement of astronomy to non-astronomers. This community of science communicators includes: NASA and NSF-funded EPO program managers, developers, evaluators, PIOs, and others who support outreach efforts by government agencies and commercial industries; Scientists working with or assigned to EPO programs or efforts; Individuals working in formal science education: K-14 schools/colleges and minority-serving institutions as faculty or curriculum developers; Informal educators working in widely diverse settings including science centers, planetariums, museums, parks, and youth programs; Amateur astronomers involved in or interested in engaging children and adults in the excitement of astronomy; Public outreach specialists working in observatories, visitor centers, public information offices, and in multimedia broadcasting and journalism. The conference goals are to improve the quality and increase the effective dissemination of EPO materials, products, and programs through a multi-tiered professional development conference utilizing: Visionary plenary talks; Highly interactive panel discussions; Small group workshops and clinics focused on a wide range of EPO topics including evaluation and dissemination, with separate sessions for varying experience levels; Poster and project exhibition segments; Opportunities to increase program leveraging through structured and unstructured networking sessions; and Individual program action planning sessions. There will both separate and combined sessions for individuals working in formal, informal, public outreach, and scientific communications settings; and specific professional development sessions.

Astronomy: On the Bleeding Edge of Scholarly Infrastructure

NASA Astrophysics Data System (ADS)

Borgman, Christine; Sands, A.; Wynholds, L. A.

2013-01-01

The infrastructure for scholarship has moved online, making data, articles, papers, journals, catalogs, and other scholarly resources nodes in a deeply interconnected network. Astronomy has led the way on several fronts, developing tools such as ADS to provide unified access to astronomical publications and reaching agreement on a common data file formats such as FITS. Astronomy also was among the first fields to establish open access to substantial amounts of observational data. We report on the first three years of a long-term research project to study knowledge infrastructures in astronomy, funded by the NSF and the Alfred P. Sloan Foundation. Early findings indicate that the availability and use of networked technologies for integrating scholarly resources varies widely within astronomy. Substantial differences arise in the management of data between ground-based and space-based missions and between subfields of astronomy, for example. While large databases such as SDSS and MAST are essential resources for many researchers, much pointed, ground-based observational data exist only on local servers, with minimal curation. Some astronomy data are easily discoverable and usable, but many are not. International coordination activities such as IVOA and distributed access to high-level data products servers such as SIMBAD and NED are enabling further integration of published data. Astronomers are tackling yet more challenges in new forms of publishing data, algorithms, visualizations, and in assuring interoperability with parallel infrastructure efforts in related fields. New issues include data citation, attribution, and provenance. Substantial concerns remain for the long term discoverability, accessibility, usability, and curation of astronomy data and other scholarly resources. The presentation will outline these challenges, how they are being addressed by astronomy and related fields, and identify concerns and accomplishments expressed by the astronomers we have interviewed and observed.

"Elements of Astronomy": A Television Course of 30 Lessons

NASA Astrophysics Data System (ADS)

Perez, J. P. D.; Del Pozo, E. P. G.; Rodriguez, R. R. T.; Mendez, A. M. B.; Rodriguez, E. R. F.; Gamez, R. G. D.

2006-08-01

It was broadcasted to all Cuba from March to December 2005, one lesson per week, transmitting three times each lesson, this means 90 hours of broadcasting. It was one of the courses of the Program "University for All", that Educative Channel produced. The Thematic: Sky Coordinates and Constellations; Astronomical Instruments; Solar System; Planets and their Moons; Comets, Asteroids and Meteoroids; Sun; Cosmic Environment and Space Weather; Stars; Galaxy and Quasars; Observable Universe; Life, Intelligent Life and Civilizations in the Universe; and History of Astronomy in Cuba. The professor staff was a group of 5 researchers of the Astronomy Department. They did an effort that each lesson had the best information level with a minimum of mathematical expressions. And were used more than 60 slides and various astronomical films fragments per lesson. To make one lesson was analyzed several astronomical films, selected a group of fragments and pre-edited into various blocks with the TV specialists, later a power point presentation was conformed using all available information on-line and bibliography. Then the lesson was recorded by the TV specialist at the Educative Channel and latter reviewed and improved by one AVID edition. The Course groundwork began in April 2003, with the first list of 12 lessons, later in June was increased to18 lessons, and started the work of "Tabloide" making; it is a journal-type book of 32 pages, equivalent to about 120 normal pages including 64 illustrations. At December 2004 the Course was increased to 30 lessons and the "Tabloide" was send to editor, later 200,000 exemplars was published. Many people followed Course and "Tabloide" was shopped in some months.

Constructivist Foundations of Intercultural Education: Implications for Research and Teacher Training

ERIC Educational Resources Information Center

Leutwyler, Bruno; Petrovic, Danijela S.; Mantel, Carola

2012-01-01

Research uncovering different images of Intercultural Education seems to be relevant in various contexts. This paper describes and compares two, the Swiss and the Serbian contexts; two countries with very different histories and with very different political and social constellations. For the Swiss context, migration flows have changed…

Conceptual Connections in Teaching of Technical Education and Physics

ERIC Educational Resources Information Center

Antonijevic, Radovan

2006-01-01

This paper considers the main characteristics of contents' connections between technical education and physics curricula, in the sixth, seventh and eighth grade of the Serbian primary school. The undertaken logical and didactic analyses of interconnectedness between contents structure of the two school subjects are based upon comparisons which…

A Study in Content Language Acquisition

ERIC Educational Resources Information Center

Broer, Kathleen

2003-01-01

This study examines how young second language learners acquire academic language. Among the main language groups represented were Punjabi, Hindi, Tamil, Estonian, Serbian, Arabic as well as 23 other language groups. I monitored over 75 students, in grades 1, 2 and 4. I was interested in exploring what strategies best promoted coherence in…

Animacy and Competition in Relative Clause Production: A Cross-Linguistic Investigation

ERIC Educational Resources Information Center

Gennari, Silvia P.; Mirkovic, Jelena; MacDonald, Maryellen C.

2012-01-01

This work investigates production preferences in different languages. Specifically, it examines how animacy, competition processes, and language-specific constraints shape speakers' choices of structure. English, Spanish and Serbian speakers were presented with depicted events in which either an animate or inanimate entity was acted upon by an…

Serbian Students: Empowered or Disempowered?

ERIC Educational Resources Information Center

Cuckovic, Biljana

2006-01-01

The higher education system in Serbia today is undergoing serious change, like other aspects of the country's social, political and economic life. Aligned with other neighboring countries that have emerged after the dissolution of the former Yugoslavia, Serbia, as well, is on the road to European integration. The process of transition necessitated…

The Night Sky, The Forgotten Nature: Uncovering the Impact of One Television Programme on Astronomy Communication in Iran

NASA Astrophysics Data System (ADS)

Nazemi, P.

2017-09-01

In 2001, two brothers known as the Saffarianpour brothers started a television programme on Iranian state television called Aseman-e-shab (The Night Sky). The programme, which explores astronomy and space science, became one of the longest-running television shows in the history of Iranian television and played a major role in the public communication of science and astronomy. It inspired many of the next generation of Iranian scientists and astronomers and played a key role in the advancement of science journalism and science communication in Iranian media. This article outlines a brief history of the show and its producer and describes the role they played in Iranian society.

How Much Mass Makes a Black Hole? - Astronomers Challenge Current Theories

NASA Astrophysics Data System (ADS)

2010-08-01

Using ESO's Very Large Telescope, European astronomers have for the first time demonstrated that a magnetar - an unusual type of neutron star - was formed from a star with at least 40 times as much mass as the Sun. The result presents great challenges to current theories of how stars evolve, as a star as massive as this was expected to become a black hole, not a magnetar. This now raises a fundamental question: just how massive does a star really have to be to become a black hole? To reach their conclusions, the astronomers looked in detail at the extraordinary star cluster Westerlund 1 [1], located 16 000 light-years away in the southern constellation of Ara (the Altar). From previous studies (eso0510), the astronomers knew that Westerlund 1 was the closest super star cluster known, containing hundreds of very massive stars, some shining with a brilliance of almost one million suns and some two thousand times the diameter of the Sun (as large as the orbit of Saturn). "If the Sun were located at the heart of this remarkable cluster, our night sky would be full of hundreds of stars as bright as the full Moon," says Ben Ritchie, lead author of the paper reporting these results. Westerlund 1 is a fantastic stellar zoo, with a diverse and exotic population of stars. The stars in the cluster share one thing: they all have the same age, estimated at between 3.5 and 5 million years, as the cluster was formed in a single star-formation event. A magnetar (eso0831) is a type of neutron star with an incredibly strong magnetic field - a million billion times stronger than that of the Earth, which is formed when certain stars undergo supernova explosions. The Westerlund 1 cluster hosts one of the few magnetars known in the Milky Way. Thanks to its home in the cluster, the astronomers were able to make the remarkable deduction that this magnetar must have formed from a star at least 40 times as massive as the Sun. As all the stars in Westerlund 1 have the same age, the star that exploded and left a magnetar remnant must have had a shorter life than the surviving stars in the cluster. "Because the lifespan of a star is directly linked to its mass - the heavier a star, the shorter its life - if we can measure the mass of any one surviving star, we know for sure that the shorter-lived star that became the magnetar must have been even more massive," says co-author and team leader Simon Clark. "This is of great significance since there is no accepted theory for how such extremely magnetic objects are formed." The astronomers therefore studied the stars that belong to the eclipsing double system W13 in Westerlund 1 using the fact that, in such a system, masses can be directly determined from the motions of the stars. By comparison with these stars, they found that the star that became the magnetar must have been at least 40 times the mass of the Sun. This proves for the first time that magnetars can evolve from stars so massive we would normally expect them to form black holes. The previous assumption was that stars with initial masses between about 10 and 25 solar masses would form neutron stars and those above 25 solar masses would produce black holes. "These stars must get rid of more than nine tenths of their mass before exploding as a supernova, or they would otherwise have created a black hole instead," says co-author Ignacio Negueruela. "Such huge mass losses before the explosion present great challenges to current theories of stellar evolution." "This therefore raises the thorny question of just how massive a star has to be to collapse to form a black hole if stars over 40 times as heavy as our Sun cannot manage this feat," concludes co-author Norbert Langer. The formation mechanism preferred by the astronomers postulates that the star that became the magnetar - the progenitor - was born with a stellar companion. As both stars evolved they would begin to interact, with energy derived from their orbital motion expended in ejecting the requisite huge quantities of mass from the progenitor star. While no such companion is currently visible at the site of the magnetar, this could be because the supernova that formed the magnetar caused the binary to break apart, ejecting both stars at high velocity from the cluster. "If this is the case it suggests that binary systems may play a key role in stellar evolution by driving mass loss - the ultimate cosmic 'diet plan' for heavyweight stars, which shifts over 95% of their initial mass," concludes Clark. Notes [1] The open cluster Westerlund 1 was discovered in 1961 from Australia by Swedish astronomer Bengt Westerlund, who later moved from there to become ESO Director in Chile (1970-74). This cluster is behind a huge interstellar cloud of gas and dust, which blocks most of its visible light. The dimming factor is more than 100 000, and this is why it has taken so long to uncover the true nature of this particular cluster. Westerlund 1 is a unique natural laboratory for the study of extreme stellar physics, helping astronomers to find out how the most massive stars in our Milky Way live and die. From their observations, the astronomers conclude that this extreme cluster most probably contains no less than 100 000 times the mass of the Sun, and all of its stars are located within a region less than 6 light-years across. Westerlund 1 thus appears to be the most massive compact young cluster yet identified in the Milky Way galaxy. All stars so far analysed in Westerlund 1 have masses at least 30-40 times that of the Sun. Because such stars have a rather short life - astronomically speaking - Westerlund 1 must be very young. The astronomers determine an age somewhere between 3.5 and 5 million years. So, Westerlund 1 is clearly a "newborn" cluster in our galaxy. More information The research presented in this ESO Press Release will soon appear in the research journal Astronomy and Astrophysics ("A VLT/FLAMES survey for massive binaries in Westerlund 1: II. Dynamical constraints on magnetar progenitor masses from the eclipsing binary W13", by B. Ritchie et al.). The same team published a first study of this object in 2006 ("A Neutron Star with a Massive Progenitor in Westerlund 1", by M.P. Muno et al., Astrophysical Journal, 636, L41). The team is composed of Ben Ritchie and Simon Clark (The Open University, UK), Ignacio Negueruela (Universidad de Alicante, Spain), and Norbert Langer (Universität Bonn, Germany, and Universiteit Utrecht, the Netherlands). The astronomers used the FLAMES instrument on ESO's Very Large Telescope at Paranal, Chile to study the stars in the Westerlund 1 cluster. ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organisation in Europe and the world's most productive astronomical observatory. It is supported by 14 countries: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world's most advanced visible-light astronomical observatory and VISTA, the world's largest survey telescope. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 42-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become "the world's biggest eye on the sky".

Stirring Astronomy into Theology: Sir Isaac Newton on the Date of the Passion of Christ

NASA Astrophysics Data System (ADS)

Belenkiy, Ari; Echagüe, Eduardo Vila

2007-08-01

It is known that Sir Isaac Newton suggested a date for the Passion of Christ in the posthumously published Observations upon the Prophecies of Daniel and the Apocalypse of St. John (1733). [This fact was revived recently in Quarterly Journal of the Royal Astronomical Society, 32, Sept 1991]. What was not known is that the first attempts to find that date were made during the early period of his life. The Jewish National and University Library in Jerusalem contains two drafts in Latin, grouped as Yahuda MS 24E under the same title, Rules for the Determination of Easter, which cast some light on Newton's life in the late 1660s - early 1670s. The earlier draft contains multiple references to the virtually forgotten De Annis Christi (1649), written by Villem Lange, the 17th century Danish astronomer and theologian, who might have been Newton's first mentor on the Jewish calendar tradition. The second draft shows not only Newton's close acquaintance with Maimonides' theory of lunar visibility, but also his attempts to simplify the latter's criteria by introducing different parameters. These “astronomical exercises”, announced in a 1673 book, were intended to appear as an appendix to Nicholas Mercator's 1676 book. Both of Yahuda 24E's drafts carry an astronomical table with the solar and lunar positions for the years 30-37 AD, which Newton used to decide on the date of the Passion. The Ordinary Least Squares regression method sends a dubious message; applied to the table's lunar data, OLS strongly suggests a pre-Tychonic origin. The table shows little correlation with solar data coming from Ptolemy, al-Battani, Tycho Brahe, Johannes Kepler, Philip van Lansbergen, Thomas Streete, John Flamsteed, or Newton's own 1702 lunar theory; however, its lunar positions display very high correlations with the Prutenic tables, which were based on Copernicus' De Revolutionibus. Surprisingly, the solar table comes from either 1651 Harmonicon Coeleste or 1669 Astronomia Britannica by Vincent Wing, another semi-forgotten astronomer of the 17th century. This makes Yahuda 24E one of the earliest of Newton's drafts. A comparison of the two drafts of Yahuda 24E shows that in the later one, Newton changed his allegiance from St John's chronology of the Passion to that shown in the synoptic gospels. This mindset was dramatically reversed in his later years, as can be seen from his posthumously published Observations Upon the Prophecies of Daniel and the Apocalypse of St. John which he supported by his forced, somewhat unexpected interpretation of the Jewish calendar tradition

UV Spectroscopy with Hubble Space Telescope- A Success Story of Pro/Am Collaboration

NASA Astrophysics Data System (ADS)

Alexander, W. R.; Linsky, J. L.; Wood, B. E.

2000-05-01

The Hubble Space Telescope amateur program has provided a unique opportunity for amateur astronomers to not only perform research on HST, but to also to interact with many professional astronomers during their research. In particular, a very successful partnership was established between William Alexander (amateur) and Jeff Linsky and Brian Wood (professionals). At the heart of this project was the use of the Goddard High Resolution Spectrograph (GHRS) aboard HST to provide high-resolution UV spectra in the Lyman-alpha region at 1216 angstroms. These spectra were needed to study the Deuterium to Hydrogen (D/H) ratio along the line of sight toward lambda-Andromedae and epsilon-Indi. These measurements were important to more fully understand big bang nucleosynthesis. The amateur, Alexander, was fully involved at each stage of the project, from obtaining all of the raw data to collaborating with Linsky and Wood in the writing of the article that appeared in The Astrophysical Journal (APJ, 470: 1157-1171). This collaboration has shown that amateurs can provide significant `academic' contributions to astronomy. This contribution can be added to the numerous observational contributions that amateurs have made to astronomy through out the centuries. Funding support was provided by NASA grant GO-0100.01-92A from the Space Telescope Science Institute.

Looking at 3,000,000 References Without Growing Grey Hair

NASA Astrophysics Data System (ADS)

Demleitner, M.; Accomazzi, A.; Eichhorn, G.; Grant, C. S.; Kurtz, M. J.; Murray, S. S.

1999-12-01

The article service of the Astrophysics Data System (ADS, http://adswww.harvard.edu) currently holds about 500,000 pages scanned from astronomical journals and conference proceedings. This data set not only facilitates an easy and convenient access to the majority of the astronomical literature from anywhere on the Internet but also allows highly automatized extraction of the information contained in the articles. As first steps towards processing and indexing the full texts of the articles, the ADS has been extracting abstracts and references from the bitmap images of the articles since May 1999. In this poster we describe the procedures and strategies to (a) automatically identify the regions within a paper containing the abstract or the references, (b) spot and correct errors in the data base or the identification of the regions, (c) resolve references obtained by optical character recognition (OCR) with its inherent uncertainties to parsed references (i.e., bibcodes) and (d) incorporate the data collected in this way into the ADS abstract service. We also give an overview of the extent of additional bibliographical material from this source. We estimate that by January 2000, these procedures will have yielded about 14,000 abstracts and 1,000,000 citation pairs (out of a total of 3,000,000 references) not previously present in the ADS.

Learned modesty and the first lady's comet: a commentary on Caroline Herschel (1787) 'An account of a new comet'.

PubMed

Winterburn, Emily

2015-04-13

Long before women were allowed to become Fellows of the Royal Society, or obtain university degrees, one woman managed to get her voice heard, her discovery verified and her achievement celebrated. That woman was Caroline Herschel, who, as this paper will discuss, managed to find ways to fit comet discoveries into her domestic life, and present them in ways that were socially acceptable. Caroline lived in a time when strict rules dictated how women (and men) should behave and present themselves and their work. Caroline understood these rules, and used them carefully as she announced each discovery, starting with this comet which she found in 1786. Caroline discovered her comets at a time when astronomers were mainly concerned with position, identifying where things were and how they were moving. Since her discoveries, research has moved on, as astronomers, using techniques from other fields, and most recently sending experiments into space, have learned more about what comets are and what they can tell us about our solar system. Caroline's paper marks one small, early step in this much bigger journey to understand comets. This commentary was written to celebrate the 350th anniversary of the journal Philosophical Transactions of the Royal Society.

Grote Reber, Radio Astronomy Pioneer, Dies

NASA Astrophysics Data System (ADS)

2002-12-01

Grote Reber, one of the earliest pioneers of radio astronomy, died in Tasmania on December 20, just two days shy of his 91st birthday. Reber was the first person to build a radio telescope dedicated to astronomy, opening up a whole new "window" on the Universe that eventually produced such landmark discoveries as quasars, pulsars and the remnant "afterglow" of the Big Bang. His self- financed experiments laid the foundation for today's advanced radio-astronomy facilities. Grote Reber Grote Reber NRAO/AUI photo "Radio astronomy has changed profoundly our understanding of the Universe and has earned the Nobel Prize for several major contributions. All radio astronomers who have followed him owe Grote Reber a deep debt for his pioneering work," said Dr. Fred Lo, director of the National Radio Astronomy Observatory (NRAO). "Reber was the first to systematically study the sky by observing something other than visible light. This gave astronomy a whole new view of the Universe. The continuing importance of new ways of looking at the Universe is emphasized by this year's Nobel Prizes in physics, which recognized scientists who pioneered X-ray and neutrino observations," Lo added. Reber was a radio engineer and avid amateur "ham" radio operator in Wheaton, Illinois, in the 1930s when he read about Karl Jansky's 1932 discovery of natural radio emissions coming from outer space. As an amateur operator, Reber had won awards and communicated with other amateurs around the world, and later wrote that he had concluded "there were no more worlds to conquer" in radio. Learning of Jansky's discovery gave Reber a whole new challenge that he attacked with vigor. Analyzing the problem as an engineer, Reber concluded that what he needed was a parabolic-dish antenna, something quite uncommon in the 1930s. In 1937, using his own funds, he constructed a 31.4-foot-diameter dish antenna in his back yard. The strange contraption attracted curious attention from his neighbors and became something of a minor tourist attraction, he later recalled. Using electronics he designed and built that pushed the technical capabilities of the era, Reber succeeded in detecting "cosmic static" in 1939. In 1941, Reber produced the first radio map of the sky, based on a series of systematic observations. His radio-astronomy work continued over the next several years. Though not a professional scientist, his research results were published in a number of prestigious technical journals, including Nature, the Astrophysical Journal, the Proceedings of the Institute of Radio Engineers and the Journal of Geophysical Research. Reber also received a number of honors normally reserved for scientists professionally trained in astronomy, including the American Astronomical Society's Henry Norris Russell Lectureship and the Astronomical Society of the Pacific's Bruce Medal in 1962, the National Radio Astronomy Observatory's Jansky Lectureship in 1975, and the Royal Astronomical Society's Jackson-Gwilt Medal in 1983. Reber's original dish antenna now is on display at the National Radio Astronomy Observatory's site in Green Bank, West Virginia, where Reber worked in the late 1950s. All of his scientific papers and records as well as his personal and scientific correspondence are held by the NRAO, and will be exhibited in the observatory's planned new library in Charlottesville, Virginia. Reber's amateur-radio callsign, W9GFZ, is held by the NRAO Amateur Radio Club. This callsign was used on the air for the first time since the 1930s on August 25, 2000, to mark the dedication of the Robert C. Byrd Green Bank Telescope. The National Radio Astronomy Observatory is a facility of the National Science Foundation, operated under cooperative agreement by Associated Universities, Inc.

Catching Carbon Stars in the Baade's Windows

NASA Astrophysics Data System (ADS)

Azzopardi, M.; Lequeux, J.; Rebeirot, E.

1984-12-01

Near-infrared objective prism surveys at low dispersion (1 700 to 3400 Amm-1) using Schmidt telescopes have been extensively used to detect M-, S- and C-type stars in the galactic equatorial zone, and in other strategically selected regions of the Milky Way. The detection techniques have been perfected by Nassau and his associates (Nassau and Velghe, 1964, Astrophysical Journal 139, 190) during their survey, at Cleveland, of the northern part of the Milky Way. These techniques are based on the identification of a number of typical molecular bands (TiO, CN, LaO, Va) that fall in the 6800-8800 Aspectral range, and which are used to classify M-, S- and C-type stars (Mavridis, 1967, Coll. on Late Type Stars, p. 420). Using the same method, partial or entire nearinfrared surveys of the southern Milky Way have been carried out by Blanco and Münch (1955, Bol. Obs. Tonantzintla y Tacubaya 12, 273) at Tonantzintla, Smith and Smith (1956, Astronomical Journal 61, 273) at Bloemfontein, and later by Westerlund (1971, Astronomy and Astrophysics Suppl. 4, 51 ; 1978, ibid. 32, 401) with the Uppsala Schmidt telescope at Mount Stromlo Observatory.

Book Review: Scientific Writing for Young Astronomers

NASA Astrophysics Data System (ADS)

Uyttenhove, Jos

2011-12-01

EDP Sciences, Les Ulis, France. Part 1 : 162 pp. € 35 ISBN 978-2-7598-0506-8 Part 2 : 298 pp. € 60 ISBN 978-2-7598-0639-3 The journal Astronomy & Astrophysics (A&A) and EDP Sciences decided in 2007 to organize a School on the various aspects of scientific writing and publishing. In 2008 and 2009 Scientific Writing for Young Astronomers (SWYA) Schools were held in Blankenberge (B) under the direction of Christiaan Sterken (FWO-VUB). These two books (EAS publication series, Vol. 49 and 50) reflect the outcome of these Schools. Part 1 contains a set of contributions that discuss various aspects of scientific publication; it includes A&A Editors' view of the peer review and publishing process. A very interesting short paper by S.R. Pottasch (Kapteyn Astronomical Institute, Groningen, and one of the two first Editors-in Chief of A&A) deals with the history of the creation of the journal Astronomy & Astrophysics. Two papers by J. Adams et al. (Observatoire de Paris) discuss language editing, including a detailed guide for any non-native user of the English language. In 2002 the Board of Directors decided that all articles in A&A must be written in clear and correct English. Part 2 consists of three very extensive and elaborated papers by Christiaan Sterken, supplying guidelines to PhD students and postdoctoral fellows to help them compose scientific papers for different forums (journals, proceedings, thesis, etc.). This part is of interest not only for young astronomers but it is very useful for scholars of all ages and disciplines. Paper I "The writing process" (60 pp.) copes with the preparation of manuscripts, with communicating with editors and referees and with avoiding common errors. Delicate problems on authorship, refereeing, revising multi-authored papers etc. are treated in 26 FAQ's. Paper II "Communication by graphics" (120 pp.) is entirely dedicated to the important topic of communication with images, graphs, diagrams, tables etc. Design types of graphs (scatter and vector plots, line graphs, histograms, pie charts, 3D surface plots) and elements of graphical images are explicated, as well as the major components of graphical images (axes, legends, textual parts, etc.). A lot of practical information on file formats, typesetting units of length (pixels, points and picas) is given in tables and figures. The problems of resolution and the differences between ppi, dpi and lpi concepts are clearly explained in par. 8, followed by a very thorough paragraph on The complexities of handling color. The author formulates the basic principle of color graphic design as follows (p. 125): DESIGN IN BLACK AND WHITE - ADD COLOR WHEN THE DESIGN IS COMPLETE. In this paper all figures are in black and white but selected graphics are printed in color (16 pp.) at the end of the paper. Different aspects of image quality are illustrated with a detail of the beautiful cover illustration of the book, the tapestry Astronomie (Rösska Museum, Sweden). Paper II ends with a list of "What to avoid at all prices" and a summary of things to do before submitting your paper to a journal. Paper III "Ethical aspects" (100 pp.) has as main theme the truthful communication of scientific results. Therefore, concepts of truth, error, quality and value are elaborated, followed by paragraphs on bibliometry and bibliometrics (impact factor, half-life, citation index and the recent Hirch h-index). Various forms of scientific misconduct are discussed extensively by category: misconduct of the researcher, the author, the referee(s), the publisher etc. The epilog "the road to wisdom" deals with truth and beauty in science with quotes of Dirac, Heisenberg and Chandrasekhar. The books are full of very useful information on all aspects of scientific writing, very complete and very well illustrated. Hundreds of references are given at the end of each paper and in the abundant footnotes a lot of interesting extra information is presented. The layout, the printing and the illustrations are excellent, as can expected in a publication about scientific writing. Just one small remark: the overflow to the next page of some extensive footnotes (mostly in Part 1) is sometimes a little bit annoying. All treated subjects are amply illustrated by examples, sometimes from the wide personal experience of the editor Christiaan Sterken, but often out of very interesting controversial historical cases (e.g. Millikan, Rømer, Young). This large assortment of famous historical cases makes the reading of the books compelling for readers with interest in the history of sciences. The comprehensive name index at the end of each volume consequently contains entries ranging from Archimedes to Newton, Einstein and Umberto Eco. As mentioned earlier this publication is very useful not only for young astronomers but for authors of all ages and disciplines. The books are so complete and elaborated that continuous reading is not obvious; browsing to specific points of interest is more suitable.

The cosmic statements in the Holy Quran as introduction to the public understanding of space science in the Islamic countries

NASA Astrophysics Data System (ADS)

Mosalam Shaltout, M. A.

The Holy Quran contains more than 800 cosmic statements speak about: sun, moon, planets, stars, Sirius, zodiac, day, night, twilights, position of stars, navigation, blue sky, night sky, dawn, noon, sunrise and sunset, eclipses, lunar months, release to the sky, landing to the earth, and so on. Due to the new discoveries in the 19th and 20th centuries in astronomy and space sciences, some of the Arabian-Islamic scientists and astronomers wished to find the significance of the cosmic statements in the Holy Quran on the light of these new discoveries. This current started at the end of the 19th century, and was growing through the 20th century. Hundreds of the articles published in the Daily news, and in the Weekly, Monthly, Quarterly, Annually Journals. Also, tens of the books published for different authors, from different Arabian and Islamic countries about the significance of the cosmic statements in the Holy Quran on the light of modern astronomy and Space sciences. Also, Radio and TV play an important role in this field, specially after the releasing of the Human kind to the space in the second half of the 20th century. This activity led to construct the International Commission on Scientific Signs in the Holy Quran and the Sunnah, which follow to the Muslim World League in Makkah Al-Mukarramah in Saudi Arabia. Where, there is a Quarterly Journal for this purpose, and periodic International conference for the same purpose, the seventh conference was held in February 2004. This paper speak about the activity of the different Arabian-Islamic Scientists and Astronomers in the field of interpretations of the cosmic statements in the Holy Quran on the light of modern astronomy and space science, and their role of increasing the public understanding of space science in the Arabian and Islamic countries.

Giant Intergalactic Gas Stream Longer Than Thought

NASA Astrophysics Data System (ADS)

2010-01-01

A giant stream of gas flowing from neighbor galaxies around our own Milky Way is much longer and older than previously thought, astronomers have discovered. The new revelations provide a fresh insight on what started the gaseous intergalactic streamer. The astronomers used the National Science Foundation's Robert C. Byrd Green Bank Telescope (GBT) to fill important gaps in the picture of gas streaming outward from the Magellanic Clouds. The first evidence of such a flow, named the Magellanic Stream, was discovered more than 30 years ago, and subsequent observations added tantalizing suggestions that there was more. However, the earlier picture showed gaps that left unanswered whether this other gas was part of the same system. "We now have answered that question. The stream is continuous," said David Nidever, of the University of Virginia. "We now have a much more complete map of the Magellanic Stream," he added. The astronomers presented their findings to the American Astronomical Society's meeting in Washington, DC. The Magellanic Clouds are the Milky Way's two nearest neighbor galaxies, about 150,000 to 200,000 light-years distant from the Milky Way. Visible in the Southern Hemisphere, they are much smaller than our Galaxy and may have been distorted by its gravity. Nidever and his colleagues observed the Magellanic Stream for more than 100 hours with the GBT. They then combined their GBT data with that from earlier studies with other radio telescopes, including the Arecibo telescope in Puerto Rico, the Parkes telescope in Australia, and the Westerbork telescope in the Netherlands. The result shows that the stream is more than 40 percent longer than previously known with certainty. One consequence of the added length of the gas stream is that it must be older, the astronomers say. They now estimate the age of the stream at 2.5 billion years. The revised size and age of the Magellanic Stream also provides a new potential explanation for how the flow got started. "The new age of the stream puts its beginning at about the time when the two Magellanic Clouds may have passed close to each other, triggering massive bursts of star formation," Nidever explained. "The strong stellar winds and supernova explosions from that burst of star formation could have blown out the gas and started it flowing toward the Milky Way," he said. "This fits nicely with some of our earlier work that showed evidence for just such blowouts in the Magellanic Clouds," said Steven Majewski, of the University of Virginia. Earlier explanations for the stream's cause required the Magellanic Clouds to pass much closer to the Milky Way, but recent orbital simulations have cast doubt on such mechanisms. Nidever and Majewski worked with Butler Burton of the Leiden Observatory and the National Radio Astronomy Observatory, and Lou Nigra of the University of Wisconsin. In addition to presenting the results to the American Astronomical Society, the scientists have submitted a paper to the Astrophysical Journal.

Teachers' Perceptions of Cultural Differences: Ethnocentric and Ethnorelative Worldview in School Context

ERIC Educational Resources Information Center

Dimitrijevic, Bojana M.

2015-01-01

In Serbian context many of the teachers are faced with a challenge of diversifying classrooms regarding the cultural background of the students. According to intercultural theory the way that people perceive cultural differences and their competence to effectively act in situations that involve different cultures is influenced by the intercultural…

For Bosnia's Future

ERIC Educational Resources Information Center

Woodard, Colin

2008-01-01

Pale, once a just a village when Bosnia's war ended 13 years ago, is now a bustling town, the hub of "Serbian Sarajevo," and home to several divisions of the Bosnian Serbs' University of East Sarajevo, their homegrown alternative to the multiethnic University of Sarajevo. It was in Pale that Radovan Karadzic and Ratko Mladic, the Bosnian…

Croatian Membership in NATO: One of the Crucial Prerequisites for Stabilization of Southeastern Europe

DTIC Science & Technology

2002-03-01

CROATIA – A HISTORICAL OVERVIEW..........................................................15 A. CROATIA UNTIL 1918 ...16 B. CROATIA UNDER SERBIAN DOMINATION 1918 -1991 ......................21 1. World War II...Hungarian Empire, and finally a part of Yugoslavia from 1918 -1991. Despite their lack of independence for a period of almost nine centuries

Creativity in Teaching Chemistry: How Much Support Does the Curriculum Provide?

ERIC Educational Resources Information Center

Tomasevic, Biljana; Trivic, Dragica

2014-01-01

In this study, the views of Serbian chemistry teachers (N = 334) on the ways in which contemporary chemistry curricula stimulate the creativity of students were surveyed. The majority of the teachers have a positive attitude towards promoting creativity through teaching chemistry. Most of them also stated that their teaching practice contained…

A Study in Content Area Language Acquisition

ERIC Educational Resources Information Center

Broer, Kathleen

2003-01-01

This study was conducted at a public school with a population of over 900 students. Among the main language groups represented were Punjabi, Hindi, Tamil, Estonian, Serbian, Arabic as well as 23 other language groups. The author monitored over 75 students, in grades 1, 2 and 4. She was interested in exploring what strategies best promoted…

Cultural and Linguistic Skills Acquisition for Special Forces: Necessity, Acceleration, and Potential Alternatives

DTIC Science & Technology

2011-12-01

Laotian, Turkish, Serbian, Arabic (Iraq), Bengali, Vietnamese, German, Punjabi , and Portuguese (Brazil), may also be offered.91 Yet, even with this...125 million) 10. German (100 million) 11. Punjabi (90 million) 12. Javanese (80 million) 13. French (75 million)94 22 JSOU Report 11-6 And, the

The Prevalence of Cyberbullying among Adolescents: A Case Study of Middle Schools in Serbia

ERIC Educational Resources Information Center

Popovic-Citic, Branislava; Djuric, Sladjana; Cvetkovic, Vladimir

2011-01-01

Cyberbullying has become widespread, and is generating growing concerns as it affects students and school climates in general. The objective of this article is to investigate the prevalence of cyberbullying among Serbian adolescents. Special emphasis was placed on gender differences regarding different forms of cyberbullying and victimization. In…

The Quality of Early Childhood Education Curriculum Framework in the Republic of Serbia

ERIC Educational Resources Information Center

Krnjaja, Živka

2015-01-01

The paper addresses Serbian preschool education Curriculum Framework as one of dimensions of the preschool education quality. The first part of paper deals with the importance of preschool education worldwide as a social responsibility and its accountability in education policy. The second part provides the evaluation of the preschool education…

Hereditary motor and sensory neuropathy Lom type in a Serbian family.

PubMed

Dacković, J; Keckarević-Marković, M; Komazec, Z; Rakocević-Stojanović, V; Lavrnić, D; Stević, Z; Ribarić, K; Romac, S; Apostolski, S

2008-10-01

Hereditary motor and sensory neuropathy Lom type (HMSNL), also called CMT 4D, a hereditary autosomal recessive neuropathy, caused by mutation in N-Myc downstream regulated gene 1 (NDRG1 gene), was first described in a Bulgarian Gypsy population near Lom and later has been found in Gypsy communities in Italy, Spain, Slovenia and Hungary. We present two siblings with HMSNL, female and male, aged 30 and 26, respectively in a Serbian non-consanguineous family of Gypsy ethnic origin. They had normal developmental milestones. Both had symptoms of lower limb muscle weakness and walking difficulties with frequent falls, which began at the age of seven. At the age of 12, they developed hearing problems and at the age of 15 hand muscle weakness. Neurological examination revealed sensorineural hearing loss, dysarthria, severe distal and mild proximal muscle wasting and weakness, areflexia and impairment of all sensory modalities of distal distribution. Electrophysiological study revealed denervation with severe and early axonal loss. Sensorineural hearing loss was confirmed on electrocochleography and brainstem evoked potentials. Molecular genetic testing confirmed homozygote C564t (R148X) mutation in NDRG1 gene.

Social determinants of malnutrition among Serbian children aged <5 years: ethnic and regional disparities.

PubMed

Brcanski, Jelena; Jović-Vraneš, Aleksandra; Marinković, Jelena; Favre, Dragana

2014-10-01

To assess the association between growth indicators of Serbian children aged <5 years of Roma and non-Roma populations and social determinants of health. This study used a cross-sectional secondary data analysis design to measure national and Roma population samples from the MICS 4 (UNICEF) performed in 2010 in Serbia. A total of 4,978 questionnaires were observed with children aged <5 years. Logistic regression analysis was performed to identify association between social determinants of health and growth indicators. Roma children were more than three times more likely to exhibit stunted and/or severely stunted than non-Roma children from the lowest wealth quintile. Non-Roma children residing outside of the Belgrade region had a lower risk of stunted compared to children residing within the Belgrade region, while the risk of stunted among Roma children was nearly twofold greater than those residing in southern and eastern Serbia than in the Belgrade region. Our findings clarified the necessity to establish ethnically and regionally sensitive programs to solve the malnutrition problems.

The aflatoxin M1 crisis in the Serbian dairy sector: the year after.

PubMed

Miocinovic, Jelena; Keskic, Tanja; Miloradovic, Zorana; Kos, Andrea; Tomasevic, Igor; Pudja, Predrag

2017-03-01

During the last 3 years, high aflatoxin M1 (AFM1) concentrations in milk and dairy products occurred in Serbia. It resulted in periodical change of the official regulations regarding maximum levels (MLs) of AFM1 as set by the Serbian Government. The aim of this study was to compare the occurrence of AFM1 in raw milk and dairy products during 2015 and also to determine whether there were some differences in AFM1 level among seasons. The AFM1 level exceeded the European Union ML in 29.3% of raw milk and 4.2% of milk product samples. The highest level of AFM1 in raw milk was found during the autumn season, while during the rest of the 2015, it was significantly lower. Although the improvement of dairy products safety was evident in 2015 when compared to 2013 and 2014, the cause of high concentrations in raw milk remained unresolved yet. This study indicates that dairy plants introduced control measures and refused reception of too high contaminated raw milk.

An anthropometric study of Serbian metal industry workers.

PubMed

Omić, S; Brkić, V K Spasojevic; Golubović, T A; Brkić, A D; Klarin, M M

2017-01-01

There are recent studies using new industrial workers' anthropometric data in different countries, but for Serbia such data are not available. This study is the first anthropometric study of Serbian metal industry workers in the country, whose labor force is increasingly employed both on local and international markets. The metal industry is one of Serbia's most important economic sectors. To this end, we collected the basic static anthropometric dimensions of 122 industrial workers and used principal components analysis (PCA) to obtain multivariate anthropometric models. To confirm the results, the dimensions of an additional 50 workers were collected. The PCA methodology was also compared with the percentile method. Comparing both data samples, we found that 96% of the participants are within the tolerance ellipsoid. According to this study, multivariate modeling covers a larger extent of the intended population proportion compared to percentiles. The results of this research are useful for the designers of metal industry workstations. This information can be used in dimensioning the workplace, thus increasing job satisfaction, reducing the risk of injuries and fatalities, and consequently increasing productivity and safety.

E-cigarette use among Serbian adults: prevalence and user characteristics.

PubMed

Kilibarda, Biljana; Mravcik, Viktor; Martens, Marcus Sebastian

2016-03-01

The objective was to report the prevalence and characteristics of electronic cigarette (e-cigarette) users in order to inform an appropriate response to this emerging challenge in tobacco control. Data were drawn from a cross-sectional survey conducted in 2014 that used computer-assisted interviewing in a representative sample of 5385 Serbian adults age 18-64 years. Lifetime e-cigarette use and current use was reported by 9.6 and 2 % of adults, respectively. Younger adults had a higher prevalence of both lifetime and current use. Females were more likely to be current e-cigarette users than males. The majority of ever and current e-cigarette users were current or past cigarette smokers, but lifetime use was reported by non-smokers as well. Electronic cigarettes are popular in Serbia; one in ten adults had tried them at least once. Because females and young adults were more likely to use e-cigarettes, a targeted response in these specific groups is needed. A standardised methodology for monitoring e-cigarette use should be established and surveys exploring motives for and attitudes towards e-cigarettes use should be conducted.

Hospital management training and improvement in managerial skills: Serbian experience.

PubMed

Supic, Zorica Terzic; Bjegovic, Vesna; Marinkovic, Jelena; Milicevic, Milena Santric; Vasic, Vladimir

2010-06-01

The purpose of this study was to analyze the improvement of managerial skills of hospitals' top managers after a specific management training programme, and to explore possible predictors and relations. The study was conducted during the years 2006 and 2007 with cohort of 107 managers from 20 Serbian general hospitals. The managers self-assessed the improvement in their managerial skills before and after the training programme. After the training programme, all managers' skills had improved. The biggest improvement was in the following skills: organizing daily activities, motivating and guiding others, supervising the work of others, group discussion, and situation analysis. The least improved were: applying creative techniques, working well with peers, professional self-development, written communication, and operational planning. Identified predictors of improvement were: shorter years of managerial experience, type of manager, type of profession, and recognizing the importance of the managerial skills in oral communication, evidence-based decision making, and supervising the work of others. Specific training programme related to strategic management can increase managerial competencies, which are an important source of competitive advantage for organizations. Copyright (c) 2010 Elsevier Ireland Ltd. All rights reserved.

Astronomical Data Center Bulletin, volume 1, no. 1

NASA Technical Reports Server (NTRS)

Warren, W. H., Jr. (Editor); Nagy, T. A. (Editor); Mead, J. M. (Editor)

1980-01-01

Information about work in progress on astronomical catalogs is presented. In addition to progress reports, an upadated status list for astronomical catalogs available at the Astronomical Data Center is included. Papers from observatories and individuals involved with astronomical data are also presented.

Clients' Perception of Outcome of Team-Based Prenatal and Reproductive Genetic Counseling in Serbian Service Using the Perceived Personal Control (PPC) Questionnaire.

PubMed

Cuturilo, Goran; Vucinic, Olivera Kontic; Novakovic, Ivana; Ignjatovic, Svetlana; Mijovic, Marija; Sulovic, Nenad; Vukolic, Dusan; Komnenic, Milica; Tadic, Jasmina; Cetkovic, Aleksandar; Belic, Aleksandra; Ljubic, Aleksandar

2016-02-01

This is the first study in Serbia and the region of South-East Europe dedicated to clients' perception of outcome and efficiency of prenatal and reproductive genetic counseling. The primary aim of this study was to assess overall value and success of genetic counseling in prenatal and reproductive care with regard to perceived personal control of clients, reflecting also in a part patient comprehension, knowledge retention, and empowerment in decision-making. The standardized Perceived Personal Control questionnaire (PPC) was used for the assessment of 239 female participants. First, we performed a complete validation of the psychometric characteristics of the Serbian-language version of the PPC questionnaire. The validation of the questionnaire permits other researchers from Serbian-speaking regions of South-East Europe to use this standard instrument to assess the effectiveness of prenatal genetic counseling in their communities and analyze advantages and disadvantages of their counseling models. We also measured social and demographic characteristics of participants. Further, we analyzed effects of our team-based prenatal and reproductive genetic counseling model through (a) calculation of PPC scores at three different stages (before initial, after initial, and before second counseling session), and (b) by assessing participants' responses by indication for referral (advanced maternal age, abnormal biochemical screening, family history of hereditary disorders, maternal exposure to drugs, exposure to radiation, exposure to infective agents, infertility or recurrent abortions, and miscellaneous). The results indicate that participants' knowledge after initial counseling increased significantly and after that remained stable and sustainable. A satisfactory level of confidence among participants had been achieved, in that many felt an increased sense of control over their situation and emotional response to it. Indirectly, these results indicate the success of a team-based prenatal genetic counseling model, which has not been assessed in the literature to date.

The Little Ice Age and its Spatial Variability across the Balkans

NASA Astrophysics Data System (ADS)

Kulkarni, C.; Peteet, D. M.; Boger, R. A.

2015-12-01

Using biological proxies (pollen, spores, and charcoal), geochemical signals through X-ray fluorescence, and AMS 14C based chronology, we present a correlation between two new high resolution Little Ice Age (LIA) records from the Central Balkans that are part of one of the least studied regions of Europe. The sediments extracted from a western sinkhole and central Serbian oxbow lake are analyzed at 8-10-cm intervals to capture the nature and magnitude of the LIA at a resolution of 20 years. During the 15th-19th CE, indigenous tree (e.g. Quercus, Acer, Pinus) and herbaceous (e.g. Poaceae, Chenopodiaceae, Artemisia) pollen from these records demonstrate fluctuations in woodland-grassland dynamics. While tree populations from Central Serbia remain comparatively stable (40-60%), the trees of western Serbia vacillate drastically between 15% and 50%. Similarly, central Serbian grasses show variations of ~18-36% whereas the western Serbian grass populations exhibit abrupt oscillations between high (55%) and low (19%) percentages. As a proxy for surface erosion and clastic input into the lakes, the 1-cm resolution potassium and titanium counts are in strong agreement with varying herbaceous taxa. These variations in ecological signals across the cores can account for local factors including altitude, terrain exposure, soils etc., however, the dynamic human component of the landscape is evident through crop pollen (e.g. Cerealia, Juglans) and microscopic charcoal highlighting the dominant role of people in ecological changes. Although the two sites show certain differences in charcoal concentration, extremely high charcoal indicates accelerated land clearance between the 15th and 17th CE. Until the beginning of 18th CE, the cultivars (e.g. Secale, Triticum) occur with very low percentages and then peak to suggest improved agriculture in the region. In the post-LIA era, the 20th CE exhibits increased arboreal percentages and declining grasslands in both the two Central Balkan records.

Magnetic stratigraphy of the Danube loess: A composite Titel-Stari Slankamen loess section over the last one million years in Vojvodina, Serbia

NASA Astrophysics Data System (ADS)

Song, Yang; Guo, Zhengtang; Marković, Slobodan; Hambach, Ulrich; Deng, Chenglong; Chang, Lin; Wu, Jianyu; Hao, Qingzhen

2018-04-01

In Europe, the most complete loess-paleosol sequences over the past million years are preserved in the Serbian part of the Danube River drainage basin. The similarity in stratigraphy and climatic cycles between the Serbian and the Chinese loess sequences suggests that the loess deposits in these two regions could play an important role in the study of intercontinental climatic correlations and linkage. However, previous magnetostratigraphic studies of the Serbian loess, mainly conducted using the alternating field (AF) demagnetization approach, show significant differences with the Chinese loess, especially the stratigraphic positioning of the Matuyama-Brunhes boundary (MBB). Here, we conduct a detailed magnetostratigraphic investigation of a composite Titel-Stari Slankamen loess section in the Vojvodina (northern Serbia), using thermal and hybrid demagnetization methods, aiming to establish new chronological constraints for the Danube Basin loess. Based on the analyses of the mineral magnetic properties, anisotropy of magnetic susceptibility, progressive thermal and hybrid demagnetization, the MBB was determined within S8, broadly consistent with the MBB position seen in the Chinese loess. Present evidence supports the hypothesis that the overall normal polarity in the upper part of L9, with a thickness of 2.1 m, was possibly caused by a combination of the remagnetization of remanence-carrying coarse-grained magnetite during the Brunhes normal chron and bioturbation during the forming of the overlying paleosol S8. Thus, our magnetostratigraphic results provide solid chronological evidence for the coherence of pedostratigraphy and climatostratigraphy for the loess deposits in the Danube Basin and China. The synchronous occurrence of the strongest developed paleosol S5 (corresponding to MISs 15-13) and the least weathered thick loess unit L9 (corresponding to MISs 24-22) in the two regions confirms that extreme climatic events during these two intervals are possibly common features of the climate in the Northern Hemisphere at those times.

Advances in Exoplanet Observing by Amateur Astronomers (Abstract)

NASA Astrophysics Data System (ADS)

Conti, D. M.

2017-06-01

(Abstract only) This past year has seen a marked increase in amateur astronomer participation in exoplanet research. This has ranged from amateur astronomers helping professional astronomers confirm candidate exoplanets, to helping refine the ephemeris of known exoplanets. In addition, amateur astronomers have been involved in characterizing such exotic objects as disintegrating planetesimals. However, the involvement in such pro/am collaborations has also required that amateur astronomers follow a more disciplined approach to exoplanet observing.

Methods in Astronomical Image Processing

NASA Astrophysics Data System (ADS)

Jörsäter, S.

A Brief Introductory Note History of Astronomical Imaging Astronomical Image Data Images in Various Formats Digitized Image Data Digital Image Data Philosophy of Astronomical Image Processing Properties of Digital Astronomical Images Human Image Processing Astronomical vs. Computer Science Image Processing Basic Tools of Astronomical Image Processing Display Applications Calibration of Intensity Scales Calibration of Length Scales Image Re-shaping Feature Enhancement Noise Suppression Noise and Error Analysis Image Processing Packages: Design of AIPS and MIDAS AIPS MIDAS Reduction of CCD Data Bias Subtraction Clipping Preflash Subtraction Dark Subtraction Flat Fielding Sky Subtraction Extinction Correction Deconvolution Methods Rebinning/Combining Summary and Prospects for the Future

Astronomical Data Center Bulletin, volume 1, number 2

NASA Technical Reports Server (NTRS)

Nagy, T. A.; Warren, W. H., Jr.; Mead, J. M.

1981-01-01

Work in progress on astronomical catalogs is presented in 16 papers. Topics cover astronomical data center operations; automatic astronomical data retrieval at GSFC; interactive computer reference search of astronomical literature 1950-1976; formatting, checking, and documenting machine-readable catalogs; interactive catalog of UV, optical, and HI data for 201 Virgo cluster galaxies; machine-readable version of the general catalog of variable stars, third edition; galactic latitude and magnitude distribution of two astronomical catalogs; the catalog of open star clusters; infrared astronomical data base and catalog of infrared observations; the Air Force geophysics laboratory; revised magnetic tape of the N30 catalog of 5,268 standard stars; positional correlation of the two-micron sky survey and Smithsonian Astrophysical Observatory catalog sources; search capabilities for the catalog of stellar identifications (CSI) 1979 version; CSI statistics: blue magnitude versus spectral type; catalogs available from the Astronomical Data Center; and status report on machine-readable astronomical catalogs.

Time-calibrated Milankovitch cycles for the late Permian.

PubMed

Wu, Huaichun; Zhang, Shihong; Hinnov, Linda A; Jiang, Ganqing; Feng, Qinglai; Li, Haiyan; Yang, Tianshui

2013-01-01

An important innovation in the geosciences is the astronomical time scale. The astronomical time scale is based on the Milankovitch-forced stratigraphy that has been calibrated to astronomical models of paleoclimate forcing; it is defined for much of Cenozoic-Mesozoic. For the Palaeozoic era, however, astronomical forcing has not been widely explored because of lack of high-precision geochronology or astronomical modelling. Here we report Milankovitch cycles from late Permian (Lopingian) strata at Meishan and Shangsi, South China, time calibrated by recent high-precision U-Pb dating. The evidence extends empirical knowledge of Earth's astronomical parameters before 250 million years ago. Observed obliquity and precession terms support a 22-h length-of-day. The reconstructed astronomical time scale indicates a 7.793-million year duration for the Lopingian epoch, when strong 405-kyr cycles constrain astronomical modelling. This is the first significant advance in defining the Palaeozoic astronomical time scale, anchored to absolute time, bridging the Palaeozoic-Mesozoic transition.

Most Distant X-Ray Jet Yet Discovered Provides Clues To Big Bang

NASA Astrophysics Data System (ADS)

2003-11-01

The most distant jet ever observed was discovered in an image of a quasar made by NASA's Chandra X-ray Observatory. Extending more than 100,000 light years from the supermassive black hole powering the quasar, the jet of high-energy particles provides astronomers with information about the intensity of the cosmic microwave background radiation 12 billion years ago. The discovery of this jet was a surprise to the astronomers, according to team members. Astronomers had previously known the distant quasar GB1508+5714 to be a powerful X-ray source, but there had been no indication of any complex structure or a jet. "This jet is especially significant because it allows us to probe the cosmic background radiation 1.4 billion years after the Big Bang," said Aneta Siemiginowska of the Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass., lead author of a report on this research in the November 20th Astrophysical Journal Letters. Prior to this discovery, the most distant confirmed X-ray jet corresponded to a time about 3 billion years after the Big Bang. Quasars are thought to be galaxies that harbor an active central supermassive black hole fueled by infalling gas and stars. This accretion process is often observed to be accompanied by the generation of powerful high-energy jets. Radio image of GB1508 Radio Image of GB1508 As the electrons in the jet fly away from the quasar at near the speed of light, they move through the sea of cosmic background radiation left over from the hot early phase of the universe. When a fast-moving electron collides with one of these background photons, it can boost the photon's energy up into the X-ray band. The X-ray brightness of the jet depends on the power in the electron beam and the intensity of the background radiation. "Everyone assumes that the background radiation will change in a predictable way with time, but it is important to have this check on the predictions," said Siemiginowska. "This jet is hopefully just the first in a large sample of these distant objects that can be used to tell us how the intensity of the cosmic microwave background changed over time." "In fact, if this interpretation is correct, then discovery of this jet is consistent with our previous prediction that X-ray jets can be detected at arbitrarily large distances!" said team member Dan Schwartz, also of the Harvard-Smithsonian Center for Astrophysics. Chandra originally observed GB1508+5714 with the purpose of studying the X-ray emission from the dust located between the Earth and the far-flung quasar. The jet was found by Siemiginowska and her colleagues when they examined the data once it became available publicly in the Chandra archive. This led another astronomer to then carefully look at radio observations of the object. Indeed, archived Very Large Array data confirmed the existence of the jet associated with the quasar GB1508+5714. A paper on the radio observations of GB1508+5714 has been accepted by Astrophysical Journal Letters from Teddy Cheung of Brandeis University in Waltham, Mass. Another group of astronomers led by Weimin Yuan of the University of Cambridge, UK independently reported the discovery of the extended emission in GB1508+5714 in X-rays. In a paper to be published in an upcoming issue of the Monthly Notices of the Royal Astronomical Society, the authors note that significant energy is being deposited in the outer regions of the host galaxy at a very early stage. This energy input could have a profound effect on the evolution of the galaxy by triggering the formation of stars, or inhibiting the growth of the galaxy through accretion of matter from intergalactic space. NASA's Marshall Space Flight Center, Huntsville, Ala., manages the Chandra program for the Office of Space Science, NASA Headquarters, Washington. Northrop Grumman of Redondo Beach, Calif., formerly TRW, Inc., was the prime development contractor for the observatory. The Smithsonian Astrophysical Observatory controls science and flight operations from the Chandra X-ray Center in Cambridge, Mass.

Shedding Light on the Cosmic Skeleton

NASA Astrophysics Data System (ADS)

2009-11-01

Astronomers have tracked down a gigantic, previously unknown assembly of galaxies located almost seven billion light-years away from us. The discovery, made possible by combining two of the most powerful ground-based telescopes in the world, is the first observation of such a prominent galaxy structure in the distant Universe, providing further insight into the cosmic web and how it formed. "Matter is not distributed uniformly in the Universe," says Masayuki Tanaka from ESO, who led the new study. "In our cosmic vicinity, stars form in galaxies and galaxies usually form groups and clusters of galaxies. The most widely accepted cosmological theories predict that matter also clumps on a larger scale in the so-called 'cosmic web', in which galaxies, embedded in filaments stretching between voids, create a gigantic wispy structure." These filaments are millions of light years long and constitute the skeleton of the Universe: galaxies gather around them, and immense galaxy clusters form at their intersections, lurking like giant spiders waiting for more matter to digest. Scientists are struggling to determine how they swirl into existence. Although massive filamentary structures have been often observed at relatively small distances from us, solid proof of their existence in the more distant Universe has been lacking until now. The team led by Tanaka discovered a large structure around a distant cluster of galaxies in images they obtained earlier. They have now used two major ground-based telescopes to study this structure in greater detail, measuring the distances from Earth of over 150 galaxies, and, hence, obtaining a three-dimensional view of the structure. The spectroscopic observations were performed using the VIMOS instrument on ESO's Very Large Telescope and FOCAS on the Subaru Telescope, operated by the National Astronomical Observatory of Japan. Thanks to these and other observations, the astronomers were able to make a real demographic study of this structure, and have identified several groups of galaxies surrounding the main galaxy cluster. They could distinguish tens of such clumps, each typically ten times as massive as our own Milky Way galaxy - and some as much as a thousand times more massive - while they estimate that the mass of the cluster amounts to at least ten thousand times the mass of the Milky Way. Some of the clumps are feeling the fatal gravitational pull of the cluster, and will eventually fall into it. "This is the first time that we have observed such a rich and prominent structure in the distant Universe," says Tanaka. "We can now move from demography to sociology and study how the properties of galaxies depend on their environment, at a time when the Universe was only two thirds of its present age." The filament is located about 6.7 billion light-years away from us and extends over at least 60 million light-years. The newly uncovered structure does probably extend further, beyond the field probed by the team, and hence future observations have already been planned to obtain a definite measure of its size. More information This research was presented in a paper published as a letter in the Astronomy & Astrophysics Journal: The spectroscopically confirmed huge cosmic structure at z = 0.55, by Tanaka et al. The team is composed of Masayuki Tanaka (ESO), Alexis Finoguenov (Max-Planck-Institute for Extraterrestrial Physics, Garching, Germany and University of Maryland, Baltimore, USA), Tadayuki Kodama (National Astronomical Observatory of Japan, Tokyo, Japan), Yusei Koyama (Department of Astronomy, University of Tokyo, Japan), Ben Maughan (H.H. Wills Physics Laboratory, University of Bristol, UK) and Fumiaki Nakata (Subaru Telescope, National Astronomical Observatory of Japan). ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organisation in Europe and the world's most productive astronomical observatory. It is supported by 14 countries: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world's most advanced visible-light astronomical observatory. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 42-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become "the world's biggest eye on the sky".

Publishing for Learned Societies: The Secret Life of a Scholarly Publisher

NASA Astrophysics Data System (ADS)

Nicholson, David

Wiley-Blackwell was formed in February 2007 as a result of the acquisition of Blackwell Publishing Ltd. by John Wiley & Sons, Inc. and the merger between Blackwell and Wiley's Scientific, Technical, and Medical business. Wiley-Blackwell publishes approximately 1,250 scholarly peer-reviewed journals including Monthly Notices of the Royal Astronomical Society and Astronomische Nachrichten, and has relationships with over 800 learned societies. The "secret life" of the article's title refers to the two broad areas of activity we undertake for our society partners, namely practical assistance and strategic advice. One of our goals at Wiley-Blackwell is to set the standard for both areas, and this article illustrates how we are doing this with a series of tangible examples.

Yura-George's world line

NASA Astrophysics Data System (ADS)

Gamov, I. L.

It is quite interesting and flattering for an economist to publish a paper in such a prominent astronomical journal. And taking into account the fact that the author is a relative of the great cosmologist of the 20th century does not diminish but, vice versa, increases the piquancy of the appearance of this article. You may agree, dear readers, that it is fairly difficult to avoid a temptation of addressing you on behalf of numerous admirers of George Gamow's talent, as well as of supporters of the Gamow Foundation of Moldova. Frankly speaking, I cannot get rid of a feeling that George Gamow himself, through some genetic "channels" known to him alone, is pushing me to tell about him, for he was famous for all kinds of tricks.

Editorial

NASA Astrophysics Data System (ADS)

Kennicutt, Robert C., Jr.

1999-07-01

This issue marks the end of an era for The Astrophysical Journal and for astronomical publishing. Helmut Abt is retiring as Editor-in-Chief after serving for 28 years, a period that saw enormous growth in the Journal and its transformation to the forefront of electronic scientific publishing. In February the ApJ office celebrated the receipt of manuscript number 40,000 under Helmut's tenure, a milestone that testifies to his impact on all of our careers. Although the names at the top of the masthead are changing, the rest of the ApJ team remains nearly unchanged, so the editorial transition should be barely noticeable. Much of the editorial work of the Journal will continue to be performed by our capable staff of Scientific Editors. I am also very fortunate to inherit Helmut's outstanding support staff in Tucson, ably headed by Janice Sexton. Our publications staff in Chicago, led by Julie Steffen, and our electronic publications staff, led by Evan Owens, are unmatched in their dedication and energy, and I have already begun working with them on further improvements to the Journal. And Helmut Abt will continue to serve the Journal over the coming months, overseeing the manuscripts that are still under review and editing the special centennial issue that will appear at the end of this year. In the coming months we will introduce several new features, most of them initiated under Helmut Abt's leadership. These will include an upgraded ApJ homepage, web tools for authors and referees, updated documentation and author instructions, and an attractive new version of the on-line journal itself. Over the longer term we are developing plans for streamlining the publication timescale and for expanding our capabilities for publishing and archiving electronic data. However my overriding priority, always, will be to uphold the Journal's reputation for scientific accuracy, impact, and integrity. I close with a personal note of thanks to Helmut Abt for his patient tutoring over the past six months and for serving as an admirable role model with his dedication, fairness, wisdom, and grace. Our profession owes him an enormous debt of gratitude. ROBERT C. KENNICUTT, JR. Editor-in-Chief

FITSManager: Management of Personal Astronomical Data

NASA Astrophysics Data System (ADS)

Cui, Chenzhou; Fan, Dongwei; Zhao, Yongheng; Kembhavi, Ajit; He, Boliang; Cao, Zihuang; Li, Jian; Nandrekar, Deoyani

2011-07-01

With the increase of personal storage capacity, it is easy to find hundreds to thousands of FITS files in the personal computer of an astrophysicist. Because Flexible Image Transport System (FITS) is a professional data format initiated by astronomers and used mainly in the small community, data management toolkits for FITS files are very few. Astronomers need a powerful tool to help them manage their local astronomical data. Although Virtual Observatory (VO) is a network oriented astronomical research environment, its applications and related technologies provide useful solutions to enhance the management and utilization of astronomical data hosted in an astronomer's personal computer. FITSManager is such a tool to provide astronomers an efficient management and utilization of their local data, bringing VO to astronomers in a seamless and transparent way. FITSManager provides fruitful functions for FITS file management, like thumbnail, preview, type dependent icons, header keyword indexing and search, collaborated working with other tools and online services, and so on. The development of the FITSManager is an effort to fill the gap between management and analysis of astronomical data.

On Tokugawa Bakufu's astronomical officials

NASA Astrophysics Data System (ADS)

Yamada, Keiji

2005-06-01

Tokugawa Bakufu's astronomical office, established in 1684, is the post for calendar reform. The reform was conducted when the calendar did not predict peculiar celestial phenomena, such as solar or lunar eclipses. It was, so to speak, the theme of the ancient astronomy. From removal of the embargo on importing western science books in 1720, Japanese astronomers studied European astronomy and attempted to apply its knowledge to calendar making. Moreover, they knew the Copernican system and also faced several modern astronomical subjects. The French astronomer Lalande's work "ASTRONOMY" exerted particularly strong influence on astronomers. This paper overviews the activities of Paris observatory and French astronomers in the 17th and 18th centuries, and survey what modern astronomical subjects were. Finally, it sketches a role of the Edo observatory played in the Japanese cultural history.

Math Anxiety--Contributing School and Individual Level Factors

ERIC Educational Resources Information Center

Radišic, Jelena; Videnovic, Marina; Baucal, Aleksander

2015-01-01

PISA 2003 survey data indicate high levels of mathematics anxiety among students in Serbia. More than a half of Serbian students are concerned with whether they will have difficulties in a mathematics class or earn poor marks. At the same time, the achievement on the mathematical literacy scale is very poor. Building on control-value theory, the…

How Did Agricultural Patterns Change in Serbia after the Fall of Yugoslavia?

ERIC Educational Resources Information Center

Sibinovic, Mikica

2018-01-01

In this lesson plan that takes one class period to complete, high school students explore how political systems influence economic activity by comparing 1991 and 2012 agricultural patterns around the Serbian capital of Belgrade. This lesson provides an insight into the model of transformation of agriculture in Serbia, but a comparison of the…

Ethnic Intermarriage and Social Cohesion. What Can We Learn from Yugoslavia?

ERIC Educational Resources Information Center

Smits, Jeroen

2010-01-01

Social cohesion theory is tested using data on ethnic intermarriage in former Yugoslavia. Before the disintegration of Yugoslavia, the proportion of marriages outside the own ethnic group was generally low, but in this respect large differences among the groups existed. The proportion of mixed marriages with a Serbian partner was much higher among…

Make Books, Not War: Workshops at a Summer Camp in Bosnia

ERIC Educational Resources Information Center

Darvin, Jacqueline

2009-01-01

This article focuses on a bookmaking project that was conducted with pre-adolescent Serbian and Bosnian girls at a summer camp outside Sarajevo, Bosnia in 2005. During this camp, children from Bosnia, Serbia and Croatia were brought together by the Global Children's Organisation to engage in a variety of activities, including conflict resolution,…

The Impact of Leadership on the Communication Satisfaction of Primary School Teachers in Serbia

ERIC Educational Resources Information Center

Terek, Edit; Glušac, Dragana; Nikolic, Milan; Tasic, Ivan; Gligorovic, Bojana

2015-01-01

This paper presents the results of research into the effects of leadership on the communication satisfaction of teachers. The data was obtained by giving questionnaires to 362 teachers from 57 primary schools in Serbia. Leadership is shown to have a strong and positive impact on the communication satisfaction of teachers in Serbian primary…

Initial characterization of unidentified Armillaria isolate from Serbia using LSU-IGS1 and TEF-1a genes

Treesearch

N. Keca; N. B. Klopfenstein; M.-S. Kim; H. Solheim; S. Woodward

2014-01-01

Armillaria species have a global distribution and play variable ecological roles, including causing root disease of diverse forest, ornamental and horticultural trees. Accurate identification of Armillaria species is critical to understand their distribution and ecological roles. This work focused on characterizing an unidentified Armillaria isolate from a Serbian...

Modelling the Intention to Use Technology for Teaching Mathematics among Pre-Service Teachers in Serbia

ERIC Educational Resources Information Center

Teo, Timothy; Milutinovic, Verica

2015-01-01

This study aims to examine the variables that influence Serbian pre-service teachers' intention to use technology to teach mathematics. Using the technology acceptance model (TAM) as the framework, we developed a research model to include subjective norm, knowledge of mathematics, and facilitating conditions as external variables to the TAM. In…

An Amorphous Model for Morphological Processing in Visual Comprehension Based on Naive Discriminative Learning

ERIC Educational Resources Information Center

Baayen, R. Harald; Milin, Petar; Durdevic, Dusica Filipovic; Hendrix, Peter; Marelli, Marco

2011-01-01

A 2-layer symbolic network model based on the equilibrium equations of the Rescorla-Wagner model (Danks, 2003) is proposed. The study first presents 2 experiments in Serbian, which reveal for sentential reading the inflectional paradigmatic effects previously observed by Milin, Filipovic Durdevic, and Moscoso del Prado Martin (2009) for unprimed…

Investigation of Language and Motor skills in Serbian Speaking Children with Specific Language Impairment and in Typically Developing Children

ERIC Educational Resources Information Center

Vukovic, Mile; Vukovic, Irena; Stojanovik, Vesna

2010-01-01

Specific language impairment (SLI) is usually defined as a developmental language disorder which does not result from a hearing loss, autism, neurological and emotional difficulties, severe social deprivation, low non-verbal abilities. Children affected with SLI typically have difficulties with the acquisition of different aspects of language and…

(Installation of the Vinca Accelerator)

DOE Office of Scientific and Technical Information (OSTI.GOV)

Zucker, A.

1991-04-22

I participated in a workshop of the physics with accelerators in Belgrade, Yugoslavia and chaired an advisory committee for the Vinca Accelerator Installation which is currently in progress. Also, I participated in meetings with the Serbian Academy of Sciences and with the Deputy Prime Minister of Serbia concerning the plans and aspirations of the nuclear research center at Vinca.

Armenian Astronomical Society (ArAS) activities

NASA Astrophysics Data System (ADS)

Mickaelian, A. M.

2016-09-01

A review on the activities and achievements of Armenian Astronomical Society (ArAS) and Armenian astronomy in general during the last years is given. ArAS membership, ArAS electronic newsletters (ArASNews), ArAS webpage, Annual Meetings, Annual Prize for Young Astronomers (Yervant Terzian Prize) and other awards, international relations, presence in international organizations, local and international summer schools, science camps, astronomical Olympiads and other events, matters related to astronomical education, astronomical heritage, amateur astronomy, astronomy outreach and ArAS further projects are described and discussed.

Shortcomings of maternity care in Serbia.

PubMed

Arsenijevic, Jelena; Pavlova, Milena; Groot, Wim

2014-03-01

Maternity care in Serbia is an integrated part of the centralized health care system inherited from the former Yugoslavia. Childbirth is often perceived as a medical event instead of a physiological process. This paper examines quality and access indicators, and patient payments for maternity care in Serbia. We apply a method of triangulation using data collected through three sources: online questionnaires filled in by mothers who delivered in one of the maternity wards in Serbia in the period 2000-2008, research publications, and official guidelines. To compare the qualitative data from all three sources, we apply framework analysis. The results show a good network of maternity wards in Serbia. On the other hand, many women who gave birth in maternity wards in Serbia indicate problems with the treatment they received. The existence of informal patient payments and so-called "special connections" make the position of Serbian women in maternity wards vulnerable, especially when they have neither connections nor the ability to pay. Poor communication and bedside manner of medical staff (obstetricians, other physicians, midwives, and nurses) during the birth process are also frequently reported. Actions should be taken to improve bedside manners of medical staff. In addition, the government should consider the involvement of private practitioners paid by the national insurance fund to create competition and decrease the need for informal payments and "connections." © 2014, Copyright the Authors Journal compilation © 2014, Wiley Periodicals, Inc.

110th Anniversary of the Engelhardt Astronomical Observatory

NASA Astrophysics Data System (ADS)

Nefedyev, Y.

2012-09-01

The Engelhardt Astronomical Observatory (EAO) was founded in September 21, 1901. The history of creation of the Engelhard Astronomical Observatory was begun in 1897 with transfer a complimentary to the Kazan University of the unique astronomical equipment of the private observatory in Dresden by known astronomer Vasily Pavlovichem Engelgardt. Having stopped astronomical activity owing to advanced years and illnesses Engelgardt has decided to offer all tools and library of the Astronomical observatory of the Kazan University. Vasily Pavlovich has put the first condition of the donation that his tools have been established as soon as possible and on them supervision are started. In 1898 the decree of Emperor had been allocated means and the ground for construction of the Astronomical observatory is allocated. There is the main historical telescope of the Engelhard Astronomical Observatory the 12-inch refractor which was constructed by English master Grubbom in 1875. The unique tool of the Engelhard Astronomical Observatory is unique in the world now a working telescope heliometer. It's one of the first heliometers, left workshops Repsolda. It has been made in 1874 and established in Engelgardt observatory in 1908 in especially for him the constructed round pavilion in diameter of 3.6 m. Today the Engelhard Astronomical Observatory is the only thing scientifically - educational and cultural - the cognitive astronomical center, located on territory from Moscow up to the most east border of Russia. Currently, the observatory is preparing to enter the protected UNESCO World Heritage List.

Preface

NASA Astrophysics Data System (ADS)

Karetnikov, Valentin G.

The publication of the 'Izvestiya' (Publications) of the Astronomical Observatory of the Odessa State University is continued now, after a 30-year time interval. The publishing activity of the University was stopped in 1963, with the Volume 5 of the 'Proceedings'. It consisted of two issues, and contained the results on the meteor investigation during the Programme of the International Geophysical Year (1957- 1958). Since the beginning in 1947, ten issues of the 'Publications' were edited by Professor V.P.Tsessevich (1907-1983), the Corresponding Member of the Ukrainian Academy of Sciences. They consisted of 74 scientific papers written by the Observatory's research workers, and of the monography 'Investigation of the eclipsing variable stars' (vol.4) written by V.P.Tsessevich on the base of the observations of 252 objects. During the recent three decades, the scientific image, the research facilities and the staff have markedly changed. Nearly 130 staff members work now at the Observatory, in the close collaboration with the staff of the Astronomical Chair of the Odessa State University. Among them there are 4 doctors of sciences and 23 candidates of sciences, several doctorants and research students. During 10 recent years, more than 500 scientific papers were published, 60 of them - in the prestige translated journals, 70 - directly in the foreign journals. More than 30 astronomical telescopes are designed and created at the Observatory, of which two are 80-cm ones are working successfully at our observational stations. Some telescopes manufactured in Odessa are working in different astronomical institutions of our country, three are located in Baya (Hungary), Svidnik (Czecho-Slovakia) and at the observational station of the Moscow Institute of Astronomy (Equador). All the telescopes are equipped with the modern instrumentation for the photometric and spectral observations, including TV technique and computers. The oldest scientific directions are the following: -astrometry based on the meridian circle observations; -photometric comet and meteor investigation; -visual and photometric observations of the light curves of eclipsing and physically variable stars, determination of the elements of orbits. In the recent decades, new methods and scientific directions were developed, such as the precise electrophotometry, middle-dispersion stellar electrospectroscopy. The high-dispersion and CCD spectroscopy and multicolor polarimetry are being obtained in other observatories of our country and are being reduced in Odessa. The investigation of the physics of the cold stars, of the structure and evolution of the eclipsing and cataclysmic binary stars, of the spectral classification and and magnetic field of the pulsating variables, of the chromospheric activity and multiperiodicity, of the emission of the artificial satellites, of the density fluctuations and the atmospheric extinction, are being developed during the recent decades. The catalogue work was carried out on the photometric properties of the stars, interstellar extinction and spacial distribution of the stars, photometric and cinematic properties of the asteroids. The study of the meteor matter enabled us to discover the transplanetary meteor radiants, to compile the catalogues of the orbital elements and light curves of more than 500 meteors. Twenty one astrometric catalogues of the precise positions were published during 30 years, as well as the catalogues of the spectral energy distribution for 500 stars in the range 320-900 nm. The collection of the patrol photographic and photovisual plates consists of more than 80 000 negatives, and is third in the World. There is a Depository of the unpublished photoelectric observations of the variable stars. The library receives the main astronomical editions and has more than 50 000 entries. Thus, the Observatory possesses a necessary scientific and engineering potential for its advanced work. In the nearest future, a new 1-m telescope (built in Odessa) will be put into operation, the 1.5m telescope is being constructed, as well as other modern equipment. One may expect the further increase of the efficiency of the investigations, the main results of which will be published in the present 'Publications'.

John Flamsteed and the turn of the screw: mechanical uncertainty, the skilful astronomer and the burden of seeing correctly at the Royal Observatory, Greenwich.

PubMed

Spiegel, Richard J

2015-03-01

Centring on John Flamsteed (1646-1719), the first Astronomer Royal, this paper investigates the ways in which astronomers of the late seventeenth century worked to build and maintain their reputations by demonstrating, for their peers and for posterity, their proficiency in managing visual technologies. By looking at his correspondence and by offering a graphic and textual analysis of the preface to his posthumous Historia Coelestis Britannica (1725), I argue that Flamsteed based the legitimacy of his life's work on his capacity to serve as a skilful astronomer who could coordinate the production and proper use of astronomical sighting instruments. Technological advances in astrometry were, for Flamsteed, a necessary but not a sufficient condition for the advancement of astronomy. Technological resources needed to be used by the right person. The work of the skilful astronomer was a necessary precondition for the mobilization and proper management of astronomical technologies. Flamsteed's understanding of the astronomer as a skilled actor importantly shifted the emphasis in precision astronomical work away from the individual observer's ability to see well and toward the astronomer's ability to ensure that instruments guaranteed accurate vision.

Brightness Variations of Sun-like Stars: The Mystery Deepens - Astronomers facing Socratic "ignorance"

NASA Astrophysics Data System (ADS)

2009-12-01

An extensive study made with ESO's Very Large Telescope deepens a long-standing mystery in the study of stars similar to the Sun. Unusual year-long variations in the brightness of about one third of all Sun-like stars during the latter stages of their lives still remain unexplained. Over the past few decades, astronomers have offered many possible explanations, but the new, painstaking observations contradict them all and only deepen the mystery. The search for a suitable interpretation is on. "Astronomers are left in the dark, and for once, we do not enjoy it," says Christine Nicholls from Mount Stromlo Observatory, Australia, lead author of a paper reporting the study. "We have obtained the most comprehensive set of observations to date for this class of Sun-like stars, and they clearly show that all the possible explanations for their unusual behaviour just fail." The mystery investigated by the team dates back to the 1930s and affects about a third of Sun-like stars in our Milky Way and other galaxies. All stars with masses similar to our Sun become, towards the end of their lives, red, cool and extremely large, just before retiring as white dwarfs. Also known as red giants, these elderly stars exhibit very strong periodic variations in their luminosity over timescales up to a couple of years. "Such variations are thought to be caused by what we call 'stellar pulsations'," says Nicholls. "Roughly speaking, the giant star swells and shrinks, becoming brighter and dimmer in a regular pattern. However, one third of these stars show an unexplained additional periodic variation, on even longer timescales - up to five years." In order to find out the origin of this secondary feature, the astronomers monitored 58 stars in our galactic neighbour, the Large Magellanic Cloud, over two and a half years. They acquired spectra using the high resolution FLAMES/GIRAFFE spectrograph on ESO's Very Large Telescope and combined them with images from other telescopes [1], achieving an impressive collection of the properties of these variable stars. Outstanding sets of data like the one collected by Nicholls and her colleagues often offer guidance on how to solve a cosmic puzzle by narrowing down the plethora of possible explanations proposed by the theoreticians. In this case, however, the observations are incompatible with all the previously conceived models and re-open an issue that has been thoroughly debated. Thanks to this study, astronomers are now aware of their own "ignorance" - a genuine driver of the knowledge-seeking process, as the ancient Greek philosopher Socrates is said to have taught. "The newly gathered data show that pulsations are an extremely unlikely explanation for the additional variation," says team leader Peter Wood. "Another possible mechanism for producing luminosity variations in a star is to have the star itself move in a binary system. However, our observations are strongly incompatible with this hypothesis too." The team found from further analysis that whatever the cause of these unexplained variations is, it also causes the giant stars to eject mass either in clumps or as an expanding disc. "A Sherlock Holmes is needed to solve this very frustrating mystery," concludes Nicholls. Notes [1] Precise brightness measurements were made by the MACHO and OGLE collaborations, running on telescopes in Australia and Chile, respectively. The OGLE observations were made at the same time as the VLT observations. More information This research was presented in two papers: one appeared in the November issue of the Monthly Notices of the Royal Astronomical Society ("Long Secondary Periods in Variable Red Giants", by C. P. Nicholls et al.), and the other has just been published in the Astrophysical Journal ("Evidence for mass ejection associated with long secondary periods in red giants", by P. R. Wood and C. P. Nicholls). The team is composed of Christine P. Nicholls and Peter R. Wood (Research School of Astronomy and Astrophysics, Australia National University), Maria-Rosa L. Cioni (Centre for Astrophysics Research, University of Hertfordshire, UK) and Igor Soszyński (Warsaw University Observatory). ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organisation in Europe and the world's most productive astronomical observatory. It is supported by 14 countries: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world's most advanced visible-light astronomical observatory. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 42-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become "the world's biggest eye on the sky".

Exoplanets Clue to Sun's Curious Chemistry

NASA Astrophysics Data System (ADS)

2009-11-01

A ground-breaking census of 500 stars, 70 of which are known to host planets, has successfully linked the long-standing "lithium mystery" observed in the Sun to the presence of planetary systems. Using ESO's successful HARPS spectrograph, a team of astronomers has found that Sun-like stars that host planets have destroyed their lithium much more efficiently than "planet-free" stars. This finding does not only shed light on the lack of lithium in our star, but also provides astronomers with a very efficient way of finding stars with planetary systems. "For almost 10 years we have tried to find out what distinguishes stars with planetary systems from their barren cousins," says Garik Israelian, lead author of a paper appearing this week in the journal Nature. "We have now found that the amount of lithium in Sun-like stars depends on whether or not they have planets." Low levels of this chemical element have been noticed for decades in the Sun, as compared to other solar-like stars, and astronomers have been unable to explain the anomaly. The discovery of a trend among planet-bearing stars provides a natural explanation to this long-standing mystery. "The explanation of this 60 year-long puzzle is for us rather simple," adds Israelian. "The Sun lacks lithium because it has planets." This conclusion is based on the analysis of 500 stars, including 70 planet-hosting stars. Most of these stars were monitored for several years with ESO's High Accuracy Radial Velocity Planet Searcher. This spectrograph, better known as HARPS, is attached to ESO's 3.6-metre telescope and is the world's foremost exoplanet hunter. "This is the best possible sample available to date to understand what makes planet-bearing stars unique," says co-author Michel Mayor. The astronomers looked in particular at Sun-like stars, almost a quarter of the whole sample. They found that the majority of stars hosting planets possess less than 1% of the amount of lithium shown by most of the other stars. "Like our Sun, these stars have been very efficient at destroying the lithium they inherited at birth," says team member Nuno Santos. "Using our unique, large sample, we can also prove that the reason for this lithium reduction is not related to any other property of the star, such as its age." Unlike most other elements lighter than iron, the light nuclei of lithium, beryllium and boron are not produced in significant amounts in stars. Instead, it is thought that lithium, composed of just three protons and four neutrons, was mainly produced just after the Big Bang, 13.7 billion years ago. Most stars will thus have the same amount of lithium, unless this element has been destroyed inside the star. This result also provides the astronomers with a new, cost-effective way to search for planetary systems: by checking the amount of lithium present in a star astronomers can decide which stars are worthy of further significant observing efforts. Now that a link between the presence of planets and curiously low levels of lithium has been established, the physical mechanism behind it has to be investigated. "There are several ways in which a planet can disturb the internal motions of matter in its host star, thereby rearrange the distribution of the various chemical elements and possibly cause the destruction of lithium. It is now up to the theoreticians to figure out which one is the most likely to happen," concludes Mayor. More information This research was presented in a paper that appears in the 12 November 2009 issue of Nature (Enhanced lithium depletion in Sun-like stars with orbiting planets, by G. Israelian et al.). The team is composed of Garik Israelian, Elisa Delgado Mena, Carolina Domínguez Cerdeña, and Rafael Rebolo (Instituto de Astrofisíca de Canarias, La Laguna, Tenerife, Spain), Nuno Santos and Sergio Sousa (Centro de Astrofisica, Universidade de Porto, Portugal), Michel Mayor and Stéphane Udry (Observatoire de Genève, Switzerland), and Sofia Randich (INAF, Osservatorio di Arcetri, Firenze, Italy). ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organisation in Europe and the world's most productive astronomical observatory. It is supported by 14 countries: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world's most advanced visible-light astronomical observatory. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 42-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become "the world's biggest eye on the sky".

The Statistical Consulting Center for Astronomy (SCCA)

NASA Technical Reports Server (NTRS)

Akritas, Michael

2001-01-01

The process by which raw astronomical data acquisition is transformed into scientifically meaningful results and interpretation typically involves many statistical steps. Traditional astronomy limits itself to a narrow range of old and familiar statistical methods: means and standard deviations; least-squares methods like chi(sup 2) minimization; and simple nonparametric procedures such as the Kolmogorov-Smirnov tests. These tools are often inadequate for the complex problems and datasets under investigations, and recent years have witnessed an increased usage of maximum-likelihood, survival analysis, multivariate analysis, wavelet and advanced time-series methods. The Statistical Consulting Center for Astronomy (SCCA) assisted astronomers with the use of sophisticated tools, and to match these tools with specific problems. The SCCA operated with two professors of statistics and a professor of astronomy working together. Questions were received by e-mail, and were discussed in detail with the questioner. Summaries of those questions and answers leading to new approaches were posted on the Web (www.state.psu.edu/ mga/SCCA). In addition to serving individual astronomers, the SCCA established a Web site for general use that provides hypertext links to selected on-line public-domain statistical software and services. The StatCodes site (www.astro.psu.edu/statcodes) provides over 200 links in the areas of: Bayesian statistics; censored and truncated data; correlation and regression, density estimation and smoothing, general statistics packages and information; image analysis; interactive Web tools; multivariate analysis; multivariate clustering and classification; nonparametric analysis; software written by astronomers; spatial statistics; statistical distributions; time series analysis; and visualization tools. StatCodes has received a remarkable high and constant hit rate of 250 hits/week (over 10,000/year) since its inception in mid-1997. It is of interest to scientists both within and outside of astronomy. The most popular sections are multivariate techniques, image analysis, and time series analysis. Hundreds of copies of the ASURV, SLOPES and CENS-TAU codes developed by SCCA scientists were also downloaded from the StatCodes site. In addition to formal SCCA duties, SCCA scientists continued a variety of related activities in astrostatistics, including refereeing of statistically oriented papers submitted to the Astrophysical Journal, talks in meetings including Feigelson's talk to science journalists entitled "The reemergence of astrostatistics" at the American Association for the Advancement of Science meeting, and published papers of astrostatistical content.

The Sky is for Everyone — Outreach and Education with the Virtual Observatory

NASA Astrophysics Data System (ADS)

Freistetter, F.; Iafrate, G.; Ramella, M.; Aida-Wp5 Team

2010-12-01

The Virtual Observatory (VO) is an international project to collect astronomical data (images, spectra, simulations, mission-logs, etc.), organise them and develop tools that let astronomers access this huge amount of information. The VO not only simplifies the work of professional astronomers, it is also a valuable tool for education and public outreach. For teachers and astronomers who actively promote astronomy to the public, the VO is a great opportunity to access and use real astronomical data, and have a taste of the daily life of astronomers.

Astronomical Heritage in the National Culture

NASA Astrophysics Data System (ADS)

Harutyunian, H. A.; Mickaelian, A. M.; Parsamian, E. S.

2014-10-01

The book contains Proceedings of the Archaeoastronomical Meeting "Astronomical Heritage in the National Culture" Dedicated to Anania Shirakatsi's 1400th Anniversary and XI Annual Meeting of the Armenian Astronomical Society. It consists of 3 main sections: "Astronomical Heritage", "Anania Shirakatsi" and "Modern Astronomy", as well as Literature about Anania Shirakatsi is included. The book may be interesting for astronomers, historians, archaeologists, linguists, students and other readers.

Elements of a Professional Development Seminar for First-Year Astronomy Graduate Students

NASA Astrophysics Data System (ADS)

Dinerstein, H. L.

1999-12-01

Students entering the astronomy Ph.D. program at the University of Texas at Austin take a seminar course which is designed to serve as an introduction and orientation both to the program and the department, and also to astronomy as a profession and a career. This seminar meets one hour per week, and has been taught in approximately the same format annually since 1994. While details of the syllabus vary from year to year, about half the sessions are devoted to information specific to our program, such as overviews of the research activities and facilities of the department and McDonald Observatory. The rest of the sessions address broader issues. They include discussions and (sometimes practice) of essential skills such as giving oral presentations, writing and peer-review of journal articles and proposals, and norms and practices of the profession. Another major focus, usually occupying three or four class sessions, is the current job market, prospects for employment, and various career paths for astronomers. National employment statistics are reviewed, as well as the employment experiences of recent graduates of our own program (Dinerstein 1996, BAAS, 28, 1277). Astronomers at various stages of their careers, and in various professional tracks, come and talk about their experiences; these guests include current post-doctoral fellows associated with the department, astronomers who have spent most of their careers on grant support (``soft money'' track) or in observatory support positions, and individuals with experience teaching at small or community colleges. The purpose of this seminar course is to ensure that graduate students become aware of their options early in their graduate careers, in order to avoid unrealistic expectations followed by unpleasant surprises later on, and to help them plan an optimum strategy for their own professional development. I also discuss how this course, originally tailored for one department, could be modified and adapted to other departments and institutions.

That Stuart brilliant flare and the search for a new lunar craterlet

NASA Astrophysics Data System (ADS)

Haas, Walter H.

On November 15, 1953, at 2 hrs., 0 mins, Universal Time (UT), Dr. Leon H. Stuart, a physician and amateur astronomer at Tulsa, OK, both saw and photographed a very bright spot near the middle of the terminator of the Moon, then 18 hours past First Quarter. The spot was hence neither a photographic blemish nor a visual illusion; and since it was found to move with the image of the Moon on the glass plate, it was not a foreground object like a terrestrial meteor. The only plausible explanation is that it was the fireball produced by the impact of a very large meteoroid upon the lunar surface. The diameter fo the spot of flare was later measured to be 21 km. Dr. Stuart withnessed neither its appearance nor disappearance, but estimated that it was under observation for about 8 seconds. Dr. Stuart published an account of this remarkable observation in "The Strolling Astronomer" in 1956 and in "The Journal of the International Lunar Society" in 1957. He corresponded on the subject with a number of amateur and professional astronomers. A few of them expressed great interest, but most were skeptical or indifferent. Interest died down with the passing years. Then, Dr. Bonnie Buratti of the Jet Propulsion Lab (JPL) examined some high-resolution Clementine 1994 images of the immediate vicinity of the Stuart flare and proposed that a new-looking craterlet located there is a result of the 1953 impact. Dr. John Westfall, however, finds from careful measures of photographs that the suggested Buratti craterlet is too far away from the 1953 photographs. The original of the 1953 photographs is missing; but Jerry Stuart, P. E., the son of Leon Stuart, has preserved copies of the original plate and will make these avaialable for research by qualified persons.

Integrated optics applied to astronomical aperture synthesis III: simulation of components optimized for astronomical interferometry

NASA Astrophysics Data System (ADS)

Nabias, Laurent; Schanen, Isabelle; Berger, Jean-Philippe; Kern, Pierre; Malbet, Fabien; Benech, Pierre

2018-04-01

This paper, "Integrated optics applied to astronomical aperture synthesis III: simulation of components optimized for astronomical interferometry," was presented as part of International Conference on Space Optics—ICSO 1997, held in Toulouse, France.

Armenian Astronomical Society Annual Activities in 2014

NASA Astrophysics Data System (ADS)

Mickaelian, A. M.

2015-07-01

A report is given on the achievements of the Armenian astronomy during the last year and on the present activities of the Armenian Astronomical Society (ArAS). ArAS membership, ArAS electronic newsletters (ArASNews), ArAS webpage, annual meetings, Annual Prize for Young Astronomers (Yervant Terzian Prize) and other awards, international relations, presence in international organizations, summer schools, astronomical Olympiads and other events, matters related to astronomical education, astronomical heritage, astronomy outreach and ArAS further projects are discussed. The present meeting, BAO Science Camp, ArAS School lectures are among 2014 events as well.

Amateur Astronomers As Public Outreach Partners

NASA Astrophysics Data System (ADS)

Bennett, M. A.

2006-08-01

Amateur astronomers involved in public outreach represent a huge, largely untapped source of energy and enthusiasm to help astronomers reach the general public. Even though many astronomy educators already work with amateur astronomers, the potential educational impact of amateur astronomers as public outreach ambassadors remains largely unrealized. Surveys and other work by the ASP in the US show that more than 20% of astronomy club members routinely participate in public engagement and educational events, such as public star parties, classroom visits, work with youth and community groups, etc. Amateur astronomers who participate in public outreach events are knowledgeable about astronomy and passionate about sharing their hobby with other people. They are very willing to work with astronomers and astronomy educators. They want useful materials, support, and training. In the USA, the ASP operates "The Night Sky Network," (funded by NASA). We have developed specialized materials and training, tested by and used by amateur astronomers. This project works with nearly 200 local astronomy clubs in 50 states to help them conduct more effective public outreach events. It has resulted in nearly 3,600 outreach events (reaching nearly 300,000 people) in just two years. In this presentation we examine key success factors, lessons learned, and suggest how astronomers outside the US can recruit and work with "outreach amateur astronomers" in their own countries.

Textbook-Caused Misconceptions, Inconsistencies, and Experimental Safety Risks of a Grade 8 Physics Textbook

ERIC Educational Resources Information Center

Zajkov, Oliver; Gegovska-Zajkova, Sonja; Mitrevski, Boce

2017-01-01

A physics textbook for the 8th grade was analyzed, in particular the section on the interaction between electric current and magnetic field. The textbook is written in the Macedonian language, but is translated into Albanian, Serbian, and Turkish, which provides an opportunity to influence a larger population of children, in a larger ethnic area.…

JPRS Report, East Europe.

DTIC Science & Technology

1991-08-16

34 Democratic Congress (J.K. Bielecki, J . Lewandowski, A. Zawislak), nonparty liberals (L. Balcerowicz, S. Kawalec), The alternative cannot be, of course...Manufacture and Installation of Electrical Equipment for the Construction Wroclaw Industry 27 Refrigerating Equipment Plant Bydgoszcz 28 J . Lenski Famur...President Franjo Tudjman, by Drazen Vukov Colic; place political scene and when the Serbian political scene under- and date not given: "Mistakes of the

Speckle Interferometry at the U.S. Naval Observatory. 20th

DTIC Science & Technology

2015-10-06

W. 1936, MNRAS, 96, 266 [Mlb1936] Muterspaugh, M. W., Hartkopf, W. I., Lane, B. F., et al. 2010, AJ, 140, 1623 [Mut2010b] Novakovic , B. 2006, IAU...C26 Circ., 158 [Nov2006] Novakovic , B. 2008, Obs, 128, 56 [Nov2008b] Novakovic , B., & Todorovic, N. 2006, Serbian AJ, 172, 21 [Nov2006e] Olevic, D. 2002

Variability in Second Language Article Production: Beyond the Representational Deficit vs. Processing Constraints Debate

ERIC Educational Resources Information Center

Trenkic, Danijela

2007-01-01

This article addresses the debate on the causes of variability in production of second language functional morphology. It reports a study on article production by first language (L1) Serbian/second language (L2) English learners and compares their behaviour to that of a Turkish learner of English, reported in Goad and White (2004). In particular,…

The Impact of War and Economic Sanction on the Incidence of Retinopathy of Prematurity in Serbia

ERIC Educational Resources Information Center

Mladenovich, Derek; Langeggen, Irene

2009-01-01

This study compared the distribution of various types of visual impairments among Serbian children who were born prior to the imposed economic sanctions and wars of the 1990s in the former Yugoslavia to that of children who were born during the years of economic sanctions and active war. (Contains 2 tables.)

Dobro Dosli U Sjedinjene Drzave. Prirucnik za Izbjeglice. (Welcome to the United States. A Guidebook for Refugees).

ERIC Educational Resources Information Center

Center for Applied Linguistics, Washington, DC. Refugee Service Center.

This guidebook provides Bosnian, Croatian, and Serbian refugees being resettled in the United States with general information about what they will encounter and the services they can receive in their first months in the country. The book is distributed to overseas processing agencies, refugees overseas who have been approved for U.S. admission,…

Students at Risk: Perceptions of Serbian Teachers and Implications for Teacher Education

ERIC Educational Resources Information Center

Jovanovic, Olja; Simic, Natasa; Rajovic, Vera

2014-01-01

While legislation is in place for the promotion of inclusive education in Serbia, the adoption of teaching practices that support diversity in schools is still lacking. This study looks at teacher perceptions of students at risk (SaR), their relationships with peers and the teachers' own roles as sources of support, using a sample of 94 interviews…

The Sources of Inequity in the Education System of Serbia and How to Combat Them

ERIC Educational Resources Information Center

Pesikan, Ana; Ivic, Ivan

2016-01-01

The concept of equal opportunity for all students is deeply embedded in the Serbian constitution and in education laws. On that level, there is no doubt that everyone is ensured an opportunity to receive quality education. Many measures in education policy have been created specifically to achieve this objective and make the system fair and…

Feel Threatened Being Prejudiced: The Role of Past Experience and Proximal Threat in Shaping Adolescents' Romaphobia

ERIC Educational Resources Information Center

Ljujic, Vanja

2011-01-01

This study investigates Serbian adolescents' attitudes towards the Roma, i.e. Romaphobia. The sample consisted of 687 secondary school students (mean age 17), of which 53% were females. In a survey-based study, we assessed perception of physical threat, quality of previous contact with Roma, and Romaphobia. The findings demonstrate that perceived…

Environmental Education in Serbian Primary Schools: Challenges and Changes in Curriculum, Pedagogy, and Teacher Training

ERIC Educational Resources Information Center

Stanišic, Jelena; Maksic, Slavica

2014-01-01

The protection of human health and the preservation of the environment are topics that form an integral part of the primary school curriculum in Serbia. However, research studies have shown that students do not have enough knowledge to contribute to the development of a healthy lifestyle and environmental awareness. The latest changes in school…

Attitudes of Serbian and Slovenian Student Teachers towards Causes of Learning Underachievement amongst Roma Pupils

ERIC Educational Resources Information Center

Macura-Milovanovic, Suncica; Pecek, Mojca

2013-01-01

The task of initial teacher education is to prepare student teachers (ST) to accept responsibility for improving the education of all pupils, including Roma pupils. Thus, knowledge of ST's attitudes regarding such pupils at the onset of initial teacher education is a key for the creation of teacher education programmes that challenge implicit…

The life and work of Ksenija Atanasijević (1894-1981)--psychology and anthropology as the inevitability and necessity of philosophy.

PubMed

Damjanović, Aleksandar; Milovanović, Srdan; Jovanović, Aleksandar; Cvetić, Tijana; Jasović-Gasić, Miroslava

2014-06-01

Ksenja Atanasijević (1894-1981) was the first woman in Serbia to obtain a Ph.D. in philosophy. Going through numerous psychological metamorphoses in her lifetime and confronted with numerous challenges, Ksenija Atanasijević developed a specific philosophical-psychological system of consolation prominently featuring the concepts of happiness, bliss, moderation, courage and wisdom. Modifying the original teachings of Democritus and Epicurus, Ksenija Atanasijević developed a distinctive anthropology based on confrontation with but equally the overcoming of obstacles, both internal (spiritual) as well as external ones. The philosopheress developed a reflexive and indeed metaphysical defensive psychotherapeutical skill at the root of which was cleansing the soul, as well as dedication to the realm of fancy, fantasy and imagination. Ksenija Atanasijević also had precious literary talent which was best expressed in her analyses of the poetry and prose of great Serbian writers (Pandurović, Njegos, Nastasijević, etc.). It is quite certain that this, with Anica Savić-Rebac, definitely greatest Serbian philosopheress, through personal suffering, creative solitude and shrouded desperation built an utterly authentic and harmonious system of philosophical comfort.

Distribution of manganese and selenium in four different pork cuts commercially available in the Serbian market

NASA Astrophysics Data System (ADS)

Đinović-Stojanović, J.; Nikolić, D.; Janković, S.; Vranić, D.; Milijašević, M.; Babić-Milijašević, J.

2017-09-01

This study aimed to provide information on levels of Mn and Se in four different pork cuts (loin, neck, hind leg and shoulder) commercially available on the Serbian market, with a view to providing information on dietary intakes of metals associated with the consumption of these meat cuts. In total, for 50 pork cuts, the levels of Mn and Se were determined by inductively-coupled plasma mass spectrometry (ICP-MS). The following ranges of Mn and Se were found (mg kg-1) in loin 0.055-0.130 and 0.074-0.365, in neck 0.014-0.365 and 0.045-0.196, in hind leg 0.032-0.099 and 0.066-0.123, in shoulder 0.012-0.290 and 0.027-0.515, respectively. The highest mean levels were obtained for Mn (0.124 mg kg-1) in shoulder and for Se (0.209 mg kg-1) in loin. The Estimated Daily Intake (EDI) of essential elements through consumption of 114.1 g mammalian meat/person/day was below 1% of Adequate Intake (AI) for Mn and between 18.9% and 43.2% of Recommended Dietary Allowance (RDA) for Se.

Epidemiology of Hypertension in Serbia: Results of a National Survey

PubMed Central

Vera, Grujić; Nataša, Dragnić; Svetlana, Kvrgić; Sonja, Šušnjević; Jasmina, Grujić; Sonja, Travar

2012-01-01

Background We evaluated the prevalence of high blood pressure and the level of awareness, treatment, and control of hypertension in a Serbian population. Methods A cross-sectional study of an adult population was carried out across Serbia in 2006. The study involved 14 204 adults aged 20 years or older. Interviews and measurements of blood pressure were performed at participants’ homes. Results Overall, 47% of the Serbian adult population had hypertension: 25.3% had stage 1 hypertension and 18.1% had stage 2 hypertension. Only 58.0% of the hypertensive population were aware that they had the disease, and 60.4% were receiving medical treatment. Among those receiving medical treatment, only 20.9% had a blood pressure within the normal range. One in 10 participants with hypertension were not treated because, among other reasons, they thought treatment was unnecessary (55.3%) or they lacked money for medication (19.3%). Conclusions The prevalence of undiagnosed and untreated hypertension is high in the adult population of Serbia. Further action is required to hasten detection and treatment of high blood pressure. Attention should be directed toward educational programs that improve knowledge, attitudes, and awareness of hypertension among adults. PMID:22374365

Education in Medical Biochemistry in Serbia.

PubMed

Majkic-Sing, Nada

2010-06-01

Medical biochemistry is the usual name for clinical biochemistry or clinical chemistry in Serbia. Medical biochemistry laboratories and medical biochemists as a profession are part of Health Care System and are regulated through: the Health Care Law and rules issued by the Chamber of Medical Biochemists of Serbia. The first continuous and organized education for Medical Biochemists in Serbia dates from 1945, when Department of Medical Biochemistry was established at Pharmaceutical Faculty in Belgrade. In 1987 at the same Faculty a five years undergraduate branch was established, educating Medical Biochemists under a special program. Since 2006 the new five year undergraduate (according to Bologna Declaration) and postgraduate program of four-year specialization according to EC4 European Syllabus for Post-Graduate Training in Clinical Chemistry and Laboratory Medicine has been established. The Ministry of Education and Ministry of Public Health accredits the programs. There are four requirements for practicing medical biochemistry in the Health Care System: University Diploma of the Faculty of Pharmacy (Medical Biochemistry), successful completion of the profession exam at the Ministry of Health after completion of one additional year of obligatory practical training in medical laboratories, membership in the Serbian Chamber of Medical Biochemists and licence for skilled work issued by Serbian Chamber of Medical Biochemists.

Animacy and competition in relative clause production: A cross-linguistic investigation

PubMed Central

Gennari, Silvia P.; Mirkovi, Jelena; MacDonald, Maryellen C.

2014-01-01

This work investigates production preferences in different languages. Specifically, it examines how animacy, competition processes, and language-specific constraints shape speakers’ choices of structure. English, Spanish and Serbian speakers were presented with depicted events in which either an animate or inanimate entity was acted upon by an agent. Questions about the affected participant in these events prompted the production of relative clauses identifying these entities (e.g., the bag the woman is punching). Results indicated that in English, animacy plays a strong role in determining the choice of passive structures. In contrast, it plays a less prominent role in Spanish and Serbian structure choices, where more active structures were produced to varying degrees. Critically, the semantic similarity between the agent and the patient of the event correlated with the omission of the agent in all languages, indicating that competition resulted in the agent’s inhibition. Similarity also correlated with different functional choices in Spanish. The results suggest that similarity-based competition may influence various stages of production planning but its manifestations are constrained by language-specific grammatical options. Implications for models of sentence production and the relationship between production and comprehension are discussed. PMID:22537914

Comparison of single extraction procedures and the application of an index for the assessment of heavy metal bioavailability in river sediments.

PubMed

Sakan, Sanja; Popović, Aleksandar; Škrivanj, Sandra; Sakan, Nenad; Đorđević, Dragana

2016-11-01

Metals in sediments are present in different chemical forms which affect their ability to transfer. The objective of this body of work was to compare different extraction methods for the bioavailability evaluation of some elements, such as Ba, Cd, Co, Cr, Cu, Fe, K, Mg, Mn, Ni, Pb, V and Zn from Serbian river sediments. A bioavailability risk assessment index (BRAI) was used for the quantification of heavy metal bioavailability in the sediments. Actual and potential element availability was assessed by single extractions with mild (CaCl 2 and CH 3 COONH 4 ) and acidic (CH 3 COOH) extractants and complexing agents (EDTA). Aqua regia extraction was used for the determination of the pseudo-total element content in river sediments. In different single extraction tests, higher extraction of Cd, Cu, Zn and Pb was observed than for the other elements. The results of the single extraction tests revealed that there is a considerable chance of metal leaching from the sediments assessed in this study. When the BRAI was applied, the results showed a high risk of heavy metal bioavailability in Serbian river sediments.

The Russian-Ukrainian Observatories Network for the European Astronomical Observatory Route Project

NASA Astrophysics Data System (ADS)

Andrievsky, S. M.; Bondar, N. I.; Karetnikov, V. G.; Kazantseva, L. V.; Nefedyev, Y. A.; Pinigin, G. I.; Pozhalova, Zh. A.; Rostopchina-Shakhovskay, A. N.; Stepanov, A. V.; Tolbin, S. V.

2011-09-01

In 2004,the Center of UNESCO World Heritage has announced a new initiative "Astronomy & World Heritage" directed for search and preserving of objects,referred to astronomy,its history in a global value,historical and cultural properties. There were defined a strategy of thematic programme "Initiative" and general criteria for selecting of ancient astronomical objects and observatories. In particular, properties that are situated or have significance in relation to celestial objects or astronomical events; representations of sky and/or celestial bodies and astronomical events; observatories and instruments; properties closely connected with the history of astronomy. In 2005-2006,in accordance with the program "Initiative", information about outstanding properties connected with astronomy have been collected.In Ukraine such work was organized by astronomical expert group in Nikolaev Astronomical Observatory. In 2007, Nikolaev observatory was included to the Tentative List of UNESCO under # 5116. Later, in 2008, the network of four astronomical observatories of Ukraine in Kiev,Crimea, Nikolaev and Odessa,considering their high authenticities and integrities,was included to the Tentative List of UNESCO under # 5267 "Astronomical Observatories of Ukraine". In 2008-2009, a new project "Thematic Study" was opened as a successor of "Initiative". It includes all fields of astronomical heritage from earlier prehistory to the Space astronomy (14 themes in total). We present the Ukraine-Russian Observatories network for the "European astronomical observatory Route project". From Russia two observatories are presented: Kazan Observatory and Pulkovo Observatory in the theme "Astronomy from the Renaissance to the mid-twentieth century".The description of astronomical observatories of Ukraine is given in accordance with the project "Thematic study"; the theme "Astronomy from the Renaissance to the mid-twentieth century" - astronomical observatories in Kiev,Nikolaev and Odessa; the theme "Contemporary Astronomy" - Crimean Astrophysical Observatory. Also on the basis of collaboration between Ukraine and Russia the Russian-Ukrainian network of astronomical observatories was organized. The participation in Paris conference, on September 20-22, will be a good opportunity to present and to discuss some questions of selection, protection and preparation of Russian-Ukrainian -network to the List of UNESCO within the topic of the Project "Route of European astronomical observatories ".

Obituary: Henry Albers (1925-2009)

NASA Astrophysics Data System (ADS)

Chromey, Fred

2011-12-01

Henry Albers, professor of astronomy at Vassar College for over thirty years, died March 29, 2009, in Fairhope, Alabama. For his work at Vassar, where he held the Maria Mitchell Chair, Albers received the first Maria Mitchell Women in Science Award for his inspiration of women astronomers. He said "In the final analysis it is the students who bring the joy into teaching." As a professional astronomer, Albers did observational work on Galactic structure in the southern Milky Way, and on the structure of the Magellanic Clouds. In retirement, Albers published Maria Mitchell - A Life in Journals and Letters, the firsthand account of America's first woman astronomer. Albers's research was on photographic near-infrared spectroscopy of red giant stars in the southern Milky Way, some proper motion studies, and on the structure of the Magellanic Clouds. A series of seven NSF grants supported his six trips to Chile to make spectroscopic observations, as well as his sabbatical collaborations at Minnesota, Leiden, and the Royal Observatory in Edinburgh. Henry Albers arrived at Vassar in 1958, to find an astronomy program that had been recently absorbed by the physics department, and that was suffering neglect after the retirement of Maud Makemson. For the next 31 years, with incredible energy -- he sometimes taught seven courses a year -- he built the astronomy program into one double in size (from one to two tenure lines), whose th century facilities have been replaced with a st century observatory. For a remarkable stretch of 20-some-years, Albers and physicist Bob Stearns, with considerable grace, alternated chairmanship of the joint department of physics and astronomy. Henry Albers was a devoted citizen of Vassar College and an enthusiastic participant in the process of faculty governance at that institution. He would have been the first to concede that his enthusiasm was sometimes excessive, and that his contributions at faculty meetings occasionally failed to move the discussion forward. Before more than one meeting, he was known to make a note to himself on his copy of the agenda, which read, in large block letters: "shut up." Fortunately, Albers was seldom able to repress his concern for the College or his dedication to its improvement. He served on all major committees and most minor ones as well. For example, he chaired a committee that eventually got telephones in faculty offices, another that lobbied for establishment of an academic computing center, and another that constructed Vassar's system of post-tenure review of senior faculty. It was Henry Albers who introduced the motion on the floor of the faculty, which passed by a vote of 100 to 2, moving that Vassar College accept coeducation. Albers was a caring mentor and although fundamentally compassionate, had a somewhat prankish sense of humor - unfailingly directed at the most pompous targets in sight. Although deeply dedicated to the College, Albers had an admirable ability to disengage from his life at Vassar. He regularly spent college breaks as the resident astronomer on cruise ships. Every May, he would celebrate his last class by sharing a jug of wine in the faculty commons with his regular lunchtime group. After retiring in 1989, he continued his hobbies of gardening, painting, and choral singing, but also immediately began work as a math and science volunteer in the local public schools on Cape Cod. He completed his final scholarly project, his edition of the Letters and Journals of Maria Mitchell, in 2002.

Enabling the Public to Experience Science from Beginning to End (Invited)

NASA Astrophysics Data System (ADS)

Trouille, L.; Chen, Y.; Lintott, C.; Lynn, S.; Simmons, B.; Smith, A.; Tremonti, C.; Whyte, L.; Willett, K.; Zevin, M.; Science Team; Moderator Team, G.

2013-12-01

In this talk we present the results of an experiment in collaborative research and article writing within the citizen science context. During July-September 2013, astronomers and the Zooniverse team ran Galaxy Zoo Quench (quench.galaxyzoo.org), investigating the mechanism(s) that recently and abruptly shut off star formation in a sample of post-quenched galaxies. Through this project, the public had the opportunity to experience the entire process of science, including galaxy classification, reading background literature, data analysis, discussion, debate, drawing conclusions, and writing an article to submit to a professional journal. The context was galaxy evolution, however, the lessons learned are applicable across the disciplines. The discussion will focus on how to leverage online tools to authentically engage the public in the entire process of science.

An Overview of Ten Years of Student Research and JDSO Publications (Abstract)

NASA Astrophysics Data System (ADS)

Freed, R.; Fitzgerald, M.; Genet, R.; Davidson, B.

2017-12-01

(Abstract only) The astronomy research seminar, initially designed and taught by Russell Genet at Cuesta College over the past decade, has resulted in over 100 published student research papers in the Journal of Double Star Observations along with dozens of other papers and conference presentations. While the seminar began at a single community college, it has now spread to include students from dozens of institutions and instructors, reaching students from middle school through graduate school. The seminar has integrated the large community-of-practice of amateur and professional astronomers, educators, students, and hardware and software engineers while providing an important experience for student researchers. In this paper, we provide an overview analysis of 109 publications authored by 320 individual students involved in the astronomy research seminar over the last decade.

An overview of ten years of student research and JDSO publications

NASA Astrophysics Data System (ADS)

Freed, Rachel; Fitzgerald, Michael; Genet, Russell; Davidson, Brendan

2017-06-01

The astronomy research seminar, initially designed and taught by Russell Genet at Cuesta College over the past decade, has resulted in over 100 published student research papers in the Journal of Double Star Observations along with dozens of other papers and conference presentations. While the seminar began at a single community college it has now spread to include students from dozens of institutions and instructors, reaching students from middle school through graduate school. The seminar has integrated the large community-of-practice of amateur and professional astronomers, educators, students, and hardware and software engineers while providing an important experience for student researchers. In this paper, we provide an overview analysis of 109 publications authored by 320 individual students involved in the astronomy research seminar over the last decade.

VizieR Online Data Catalog: The URAT Parallax Catalog (UPC). Update 2018 (Finch+, 2018)

NASA Astrophysics Data System (ADS)

Finch, C. T.; Zacharias, N.; Jao, W.-C.

2018-03-01

United States Naval Observatory (USNO) Robotic Astrometric Telescope (URAT) Parallax Catalog south (UPCs) and north (UPCn). These data are based on the accepted paper for the Astronomical Journal (2018) by C. Finch, N. Zacharias, and W.-C. Jao, "URAT south parallax results: discovery of new nearby stars" (2018AJ....155..176F). The southern data are new, while the northern data contain a subset of the previously published UPC catalog after applying the more stringent selection criteria of the south data and supplementing the data with columns of the southern data. The previously published URAT Parallax Catalog (UPC) paper is: C. Finch and N. Zacharias (2016AJ....151..160F, Cat. J/AJ/151/160) (arXiv:1604.06739). (3 data files).

Close Double Stars from Occultation Video Recordings

NASA Astrophysics Data System (ADS)

Waring Dunham, David; George, Anthony; Loader, Brian; Herald, David Russell

2015-08-01

Astronomers around the world, both amateur and professional, have been recording lunar and asteroidal occultations of close double stars during the past several years using inexpensive but quite sensitive video cameras that are now available. Several new double stars have been discovered, and the parameters of many close systems have been determined. Besides rather good measurements of the relative magnitudes of the components, the actual separations and position angles can be measured if observations of the same event are made from two or more separate stations. These observations collected by the International Occultation Timing Association (IOTA) are published in the Journal of Double Star Observations. Recently, IOTA has encouraged the observation of occultations of stars in the Kepler 2 program, which is interested in data about close duplicity that affects their analyses for exoplanet transits.

Data Publication & Citation practices in Astronomy

NASA Astrophysics Data System (ADS)

Muench, August

2011-05-01

We investigated author behaviors around the practices of publishing and citing data products within refereed astronomical journals. We set the scope of this investigation to encompass AAS publications over the last decade, including the AAS publisher transition that took place in 2008-09. Our analysis focused on parsing the journal articles’ source material (LaTeX, XML) to catalog hyperlinks between the published text and extended data products that were provided by authors as part of the standard editorial process for refereed publications. We quantitatively and rhetorically analyzed this catalog of hyperlinks to decipher (some of) the authors’ behaviors with regard to data citation and publication. We focused on authors’ adoption and utilization of two specific data-literature links: journal hosted supplementary material and the NASA ADEC recommended system of dataset "identifiers,” which were designed to provide persistent links between articles and packages of relevant, reusable data located at trusted, established astronomy archives. These types of hyperlinks are, however, minor subsets of the overall catalog, where the bulk of author inserted links provide descriptive elements to otherwise "unpublished” material but not to unique, reusable datasets. In general our investigation reveals a consistent level of effort by authors to cite and publish some data products, although case by case examples darkly illuminate individual author's experiences with data publication and citation within the standard editorial process. Finally, we point out a couple of functional issues with existing data-literature links as specifically related to the suite of author behaviors examined in this project.

Astronomical Books and Charts in the Book of Bibliographie Coreenne

NASA Astrophysics Data System (ADS)

Lee, Ki-Won; Yang, Hong-Jin; Park, Myeong-Gu

2008-06-01

We investigate astronomical materials listed in the book of Bibliographie Coréenne written by Maurice Courant. He classified ancient Korean books into nine Divisions (?) and thirty six Classes (?), and published them as three volumes (ranging from 1894 to 1896) and one supplement (in 1901). In total, 3,821 books including astronomical ones are listed together with information on physical size, possessional place, bibliographical note, and so forth. Although this book is an essential one in the field of Korea bibliography and contains many astronomical materials such as Cheon-Mun-Ryu-Cho ????, Si-Heon-Seo ??????, and Cheon-Sang-Yeol-Cha-Bun-Ya-Ji-Do ????????, it has not been well known to the public nor to astronomical society. Of 3,821 catalogues, we found that about 50 Items (?) are related to astronomy or astrology, and verified that most ! of them are located in the Kyujanggak Royal Library ???. We also found an unknown astronomical chart, Hon-Cheon-Chong-Seong-Yeol-Cha-Bun-Ya-Ji-Do ??????????. Because those astronomical materials are not well known to international astronomical community and there have been few studies on the materials in Korea, we here introduce and review them, particularly with the astronomical viewpoint.

The First Astronomical Observatory in Cluj-Napoca

NASA Astrophysics Data System (ADS)

Szenkovits, Ferenc

2008-09-01

One of the most important cities of Romania is Cluj-Napoca (Kolozsvár, Klausenburg). This is a traditional center of education, with many universities and high schools. From the second half of the 18th century the University of Cluj has its own Astronomical Observatory, serving for didactical activities and scientific researches. The famous astronomer Maximillian Hell was one of those Jesuits who put the base of this Astronomical Observatory. Our purpose is to offer a short history of the beginnings of this Astronomical Observatory.

Storing Astronomical Information on the Romanian Territory

NASA Astrophysics Data System (ADS)

Stavinschi, M.; Mioc, V.

2004-12-01

Romanian astronomy has a more than 2000-year old tradition, which is, however, little known abroad. The first known archive of astronomical information is the Dacian sanctuary at Sarmizegetusa Regia, erected in the first century AD, having similarities with that of Stonehenge. After a gap of more than 1000 years, more sources of astronomical information become available, mainly records of astronomical events. Monasteries were the safest storage places of these genuine archives. We present a classification of the ways of storing astronomical information, along with characteristic examples.

Far infrared supplement: Catalog of infrared observations

NASA Technical Reports Server (NTRS)

Gezari, D. Y.; Schmitz, M.; Mead, J. M.

1982-01-01

The development of a new generation of orbital, airborne and ground-based infrared astronomical observatory facilities, including the infrared astronomical satellite (IRAS), the cosmic background explorer (COBE), the NASA Kuiper airborne observatory, and the NASA infrared telescope facility, intensified the need for a comprehensive, machine-readable data base and catalog of current infrared astronomical observations. The Infrared Astronomical Data Base and its principal data product, this catalog, comprise a machine-readable library of infrared (1 micrometer to 1000 micrometers) astronomical observations published in the scientific literature since 1965.

The study on servo-control system in the large aperture telescope

NASA Astrophysics Data System (ADS)

Hu, Wei; Zhenchao, Zhang; Daxing, Wang

2008-08-01

Large astronomical telescope or extremely enormous astronomical telescope servo tracking technique will be one of crucial technology that must be solved in researching and manufacturing. To control technique feature of large astronomical telescope or extremely enormous astronomical telescope, this paper design a sort of large astronomical telescope servo tracking control system. This system composes a principal and subordinate distributed control system, host computer sends steering instruction and receive slave computer functional mode, slave computer accomplish control algorithm and execute real-time control. Large astronomical telescope servo control use direct drive machine, and adopt DSP technology to complete direct torque control algorithm, Such design can not only increase control system performance, but also greatly reduced volume and costs of control system, which has a significant occurrence. The system design scheme can be proved reasonably by calculating and simulating. This system can be applied to large astronomical telescope.

Future Roles and Missions of the Kosovo Security Force

DTIC Science & Technology

2012-06-08

brings light to the brutality of the war in Kosovo, including Serbia’s genocidal intentions against the Albanians, and it aids in understanding the...Yugoslavia also. These territorial and genocidal ambitions toward other peoples in Yugoslavia were codified by the Serbian Academy of Arts and...masterminds of genocide Ilija Garashanin, Vaso Qubrilovic, Dobrica Qosic, and executors of genocide , Slobodan Milosevic, Ratko Mladic, Radovan

Enhancing Library Business Performance by Implementation of Enterprise 2.0 via Intrapreneurship: The Case of a Serbian Library

ERIC Educational Resources Information Center

Sofronijevic, Adam; Milicevic, Vesna; Ilic, Bojan; Seaman, Scott

2011-01-01

As academic libraries around the world face the dual challenges of rising demand but limits on funding, managers look for ways to improve library performance that do not add significantly to the budget. This paper presents a novel relationship between intrapreneurship and Enterprise 2.0 that suggests there are relatively cheap and easy ways to…

HLA-A, -B, -C, -DRB1 and -DQB1 allele and haplotype frequencies in the Serbian population.

PubMed

Andric, Zorana; Popadic, Dusan; Jovanovic, Barbara; Jaglicic, Ivana; Bojic, Svetlana; Simonovic, Ruzica

2014-03-01

This study provides the first published detailed analysis of five loci polymorphisms as well as reports of two, three and five loci haplotype frequencies in the Serbian population in a sample of 1992 volunteer bone marrow donors recruited from different part of the country. Typing was performed by PCR SSO method combined with PCR SSP techniques to resolve ambiguities. In total, 16 HLA-A, 28 HLA-B, 14 HLA-C, 13 HLA-DRB1 and 5 HLA-DQB1 allelic groups were identified. The most frequent in allele groups are HLA-A(∗)02 (29.5%), HLA-A(∗)01 (14.2%), HLA-B(∗)35 (13.1%), HLA-B(∗)51 (12.8%), HLA-C(∗)07 (24.8%), HLA-DRB1(∗)11 (16.9%), HLA-DRB1(∗)13 (13.2%), HLA-DQB1(∗)03 (33.3%) and DQB1(∗)05 (33.0%). The most frequent three- and five-loci haplotypes were A(∗)01-B(∗)08-DRB1(∗)03 (5.9%) and A(∗)02-B(∗)18-DRB1(∗)11 (1.9%), A(∗)01-B(∗)08-C(∗)07-DRB1(∗)03-DQB1(∗)02 (6.6%) followed by A(∗)02-B(∗)18-C(∗)07-DRB1(∗)11-DQB1(∗)03 (2.5%), then A(∗)33-B(∗)14-C(∗)08-DRB1(∗)01-DQB1(∗)05 and A(∗)02-B(∗)35-C(∗)04-DRB1(∗)16-DQB1(∗)05 (2.2% both), respectively. The results of cluster analysis showed that the Serbian population is closely related to the populations living in central Balkan and neighboring European regions. The level of allelic diversity found in this study are relevant to facilitate searching for unrelated matched donor and provide a healthy control population from our region that should be useful in the future disease association study. Copyright © 2013 American Society for Histocompatibility and Immunogenetics. Published by Elsevier Inc. All rights reserved.

Antimicrobial Activity of Serbian Propolis Evaluated by Means of MIC, HPTLC, Bioautography and Chemometrics

PubMed Central

Trifković, Jelena; Berić, Tanja; Vovk, Irena; Milojković-Opsenica, Dušanka; Stanković, Slaviša

2016-01-01

New information has come to light about the biological activity of propolis and the quality of natural products which requires a rapid and reliable assessment method such as High Performance Thin-Layer Chromatography (HPTLC) fingerprinting. This study investigates chromatographic and chemometric approaches for determining the antimicrobial activity of propolis of Serbian origin against various bacterial species. A linear multivariate calibration technique, using Partial Least Squares, was used to extract the relevant information from the chromatographic fingerprints, i.e. to indicate peaks which represent phenolic compounds that are potentially responsible for the antimicrobial capacity of the samples. In addition, direct bioautography was performed to localize the antibacterial activity on chromatograms. The biological activity of the propolis samples against various bacterial species was determined by a minimum inhibitory concentration assay, confirming their affiliation with the European poplar type of propolis and revealing the existence of two types (blue and orange) according to botanical origin. The strongest antibacterial activity was exhibited by sample 26 against Staphylococcus aureus, with a MIC value of 0.5 mg/mL, and Listeria monocytogenes, with a MIC as low as 0.1 mg/mL, which was also the lowest effective concentration observed in our study. Generally, the orange type of propolis shows higher antimicrobial activity compared to the blue type. PLS modelling was performed on the HPTLC data set and the resulting models might qualitatively indicate compounds that play an important role in the activity exhibited by the propolis samples. The most relevant peaks influencing the antimicrobial activity of propolis against all bacterial strains were phenolic compounds at RF values of 0.37, 0.40, 0.45, 0.51, 0.60 and 0.70. The knowledge gained through this study could be important for attributing the antimicrobial activity of propolis to specific chemical compounds, as well as the verification of HPTLC fingerprinting as a reliable method for the identification of compounds that are potentially responsible for antimicrobial activity. This is the first report on the activity of Serbian propolis as determined by several combined methods, including the modelling of antimicrobial activity by HPTLC fingerprinting. PMID:27272728

The National Astronomical Observatory of Japan and Post-war Japanese Optical Astronomy

NASA Astrophysics Data System (ADS)

Tajima, Toshiyuki

This paper depicts some aspects of the formative process of the Japanese optical and infrared astronomical community in the post-war period, featuring the transition of the National Astronomical Observatory of Japan(NAOJ). We take up three cases of telescope construction, examining their background and their contribution to the Japanese astronomical community. Through these cases, the characteristics of traditions and cultures of optical and infrared astronomy in Japan are considered. Although the Tokyo Astronomical Observatory (TAO) of the University of Tokyo, the predecessor of NAOJ, was originally founded as an agency for practical astronomical observation such as time and almanac service, it has become an international centre for all types of astrophysical research. Research and development of telescopes and observational instruments have become an important part of the astronomers' practice. Now, however, a number of Japanese universities are planning to have their own large to middle-sized telescopes, and a new style of astronomical research is emerging involving astrophysical studies utilising data acquired from the Virtual Observatory, so there is a distinct possibility that the status of the NAOJ will change even further in the future.

He2-90'S APPEARANCE DECEIVES ASTRONOMERS

NASA Technical Reports Server (NTRS)

2002-01-01

Astronomers using NASA's Hubble Space Telescope have stumbled upon a mysterious object that is grudgingly yielding clues to its identity. A quick glance at the Hubble picture at top shows that this celestial body, called He2-90, looks like a young, dust-enshrouded star with narrow jets of material streaming from each side. But it's not. The object is classified as a planetary nebula, the glowing remains of a dying, lightweight star. But the Hubble observations suggest that it may not fit that classification, either. The Hubble astronomers now suspect that this enigmatic object may actually be a pair of aging stars masquerading as a single youngster. One member of the duo is a bloated red giant star shedding matter from its outer layers. This matter is then gravitationally captured in a rotating, pancake-shaped accretion disk around a compact partner, which is most likely a young white dwarf (the collapsed remnant of a sun-like star). The stars cannot be seen in the Hubble images because a lane of dust obscures them. The Hubble picture at top shows a centrally bright object with jets, appearing like strings of beads, emanating from both sides of center. (The other streaks of light running diagonally from He2-90 are artificial effects of the telescope's optical system.) Each jet possesses at least six bright clumps of gas, which are speeding along at rates estimated to be at least 375,000 miles an hour (600,000 kilometers an hour). These gaseous salvos are being ejected into space about every 100 years, and may be caused by periodic instabilities in He2-90's accretion disk. The jets from very young stars behave in a similar way. Deep images taken from terrestrial observatories show each jet extending at least 100,000 astronomical units (one astronomical unit equals the Earth-Sun distance, 93 million miles). The jets' relatively modest speed implies that one member of the duo is a white dwarf. Observations by the Compton Gamma-Ray Observatory, however, discovered a gamma-ray source in the vicinity of He2-90, suggesting that the companion may be a neutron star or a black hole (the compact corpses of dying, massive stars). But the jets from accretion disks around neutron stars or black holes travel at a few tenths the speed of light, much faster than the plodding pace of He2-90's jets. The Hubble astronomers are planning more observations to pinpoint the gamma-ray source to determine whether it is associated with He2-90. An accretion disk needs gravity to form. For gravity to create He2-90's disk, the pair of stars must reside at a cozy distance from each other: within about 10 astronomical units. Although the astronomers are uncertain about the details, they believe that magnetic fields associated with the accretion disk produce and constrict the pencil-thin jets seen in the Hubble image. The close-up Hubble photo at bottom shows a dark, flaring, disk-like structure [off-center] bisecting the bright light from the object. The disk is seen edge-on. Although too large to be an accretion disk, this dark, flaring disk may provide indirect proof of the other's existence. Most theories for producing jets require the presence of an accretion disk. The jets are seen streaming from both sides of the central object. The round, white objects at the lower left and upper right corners are two bright clumps of gas in the jets. The astronomers traced the jets to within 1,000 astronomical units of the central obscured star. The star ejected this jet material about 30 years ago. Scientists discovered this puzzling object while taking a census of planetary nebulae. They knew it had been classified as a dying, sun-like star. He2-90 is enshrouded in very hot (17,500 degrees Fahrenheit or 10,000 degrees Kelvin), glowing gas, a typical feature of planetary nebulae. And yet the disk and jets indicated the presence of an embryonic star. The mystified astronomers needed more information. Since embryonic stars are usually associated with cool, dense clouds of gas and dust, they used a ground-based radio telescope in Chile to look for evidence of such a cloud around He2-90. No such cloud was found, and He2-90's neighborhood showed no traces of developing stars. He2-90 lies about 8,000 light-years from Earth in the constellation Centaurus in the southern sky. The images were taken Sept 28, 1999 with the Wide Field and Planetary Camera 2. The images and results appear in the Aug. 1 issue of the Astrophysical Journal Letters. Credits: NASA, Raghvendra Sahai (NASA Jet Propulsion Laboratory), Lars-Ake Nyman (European Southern Observatory, Chile and Onsala Space Observatory, Sweden)

The System for Quick Search of the Astronomical Objects and Events in the Digital Plate Archives.

NASA Astrophysics Data System (ADS)

Sergeev, A. V.; Sergeeva, T. P.

From the middle of the XIX century observatories all over the world have accumulated about three millions astronomical plates contained the unique information about the Universe which can not be obtained or restored with the help of any newest facilities and technologies but may be useful for many modern astronomical investigations. The threat of astronomical plate archives loss caused by economical, technical or some other causes have put before world astronomical community a problem: the preservation of the unique information kept on those plates. The problem can be solved by transformation of the information from plates to digital form and keeping it on electronic data medium. We began a creation of a system for quick search and analysing of astronomical events and objects in digital plate archive of the Ukrainian Main astronomical observatory of NAS. Connection of the system to Internet will allow a remote user (astronomer or observer) to have access to digital plate archive and to work with it. For providing of the high efficiency of this work the plate database (list of the plates with all information about them and access software) are preparing. Modular structure of the system basic software and standard format of the plate image files allow future development of problem-oriented software for special astronomical researches.

Blind Astronomers

NASA Astrophysics Data System (ADS)

Hockey, Thomas A.

2011-01-01

The phrase "blind astronomer” is used as an allegorical oxymoron. However, there were and are blind astronomers. What of famous blind astronomers? First, it must be stated that these astronomers were not martyrs to their craft. It is a myth that astronomers blind themselves by observing the Sun. As early as France's William of Saint-Cloud (circa 1290) astronomers knew that staring at the Sun was ill-advised and avoided it. Galileo Galilei did not invent the astronomical telescope and then proceed to blind himself with one. Galileo observed the Sun near sunrise and sunset or through projection. More than two decades later he became blind, as many septuagenarians do, unrelated to their profession. Even Isaac Newton temporarily blinded himself, staring at the reflection of the Sun when he was a twentysomething. But permanent Sun-induced blindness? No, it did not happen. For instance, it was a stroke that left Scotland's James Gregory (1638-1675) blind. (You will remember the Gregorian telescope.) However, he died days later. Thus, blindness little interfered with his occupation. English Abbot Richard of Wallingford (circa 1291 - circa 1335) wrote astronomical works and designed astronomical instruments. He was also blind in one eye. Yet as he further suffered from leprosy, his blindness seems the lesser of Richard's maladies. Perhaps the most famous professionally active, blind astronomer (or almost blind astronomer) is Dominique-Francois Arago (1786-1853), director until his death of the powerful nineteenth-century Paris Observatory. I will share other _ some poignant _ examples such as: William Campbell, whose blindness drove him to suicide; Leonhard Euler, astronomy's Beethoven, who did nearly half of his life's work while almost totally blind; and Edwin Frost, who "observed” a total solar eclipse while completely sightless.

Planet Formation in Action? - Astronomers may have found the first object clearing its path in the natal disc surrounding a young star

NASA Astrophysics Data System (ADS)

2011-02-01

Using ESO's Very Large Telescope an international team of astronomers has been able to study the short-lived disc of material around a young star that is in the early stages of making a planetary system. For the first time a smaller companion could be detected that may be the cause of the large gap found in the disc. Future observations will determine whether this companion is a planet or a brown dwarf. Planets form from the discs of material around young stars, but the transition from dust disc to planetary system is rapid and few objects are caught during this phase [1]. One such object is T Chamaeleontis (T Cha), a faint star in the small southern constellation of Chamaeleon that is comparable to the Sun, but very near the beginning of its life [2]. T Cha lies about 350 light-years from the Earth and is only about seven million years old. Up to now no forming planets have been found in these transitional discs, although planets in more mature discs have been seen before (eso0842, heic0821). "Earlier studies had shown that T Cha was an excellent target for studying how planetary systems form," notes Johan Olofsson (Max Planck Institute for Astronomy, Heidelberg, Germany), one of the lead authors of two papers in the journal Astronomy & Astrophysics that describe the new work. "But this star is quite distant and the full power of the Very Large Telescope Interferometer (VLTI) was needed to resolve very fine details and see what is going on in the dust disc." The astronomers first observed T Cha using the AMBER instrument and the VLT Interferometer (VLTI) [3]. They found that some of the disc material formed a narrow dusty ring only about 20 million kilometres from the star. Beyond this inner disc, they found a region devoid of dust with the outer part of the disc stretching out into regions beyond about 1.1 billion kilometres from the star. Nuria Huélamo (Centro de Astrobiología, ESAC, Spain), the lead author of the second paper takes up the story: "For us the gap in the dust disc around T Cha was a smoking gun, and we asked ourselves: could we be witnessing a companion digging a gap inside its protoplanetary disc?" However, finding a faint companion so close to a bright star is a huge challenge and the team had to use the VLT instrument NACO in a novel and powerful way, called sparse aperture masking, to reach their goal [4]. After careful analysis they found the clear signature of an object located within the gap in the dust disc, about one billion kilometres from the star - slightly further out than Jupiter is within our Solar System and close to the outer edge of the gap. This is the first detection of an object much smaller than a star within a gap in the planet-forming dust disc around a young star. The evidence suggests that the companion object cannot be a normal star [5] but it could be either a brown dwarf [6] surrounded by dust or, most excitingly, a recently formed planet. Huélamo concludes: "This is a remarkable joint study that combines two different state-of-the-art instruments at ESO's Paranal Observatory. Future observations will allow us to find out more about the companion and the disc, and also understand what fuels the inner dusty disc." Notes [1] The transitional discs can be spotted because they give off less radiation at mid-infrared wavelengths. The clearing of the dust close to the star and the creation of gaps and holes can explain this missing radiation. Recently formed planets may have created these gaps, although there are also other possibilities. [2] T Cha is a T Tauri star, a very young star that is still contracting towards the main sequence. [3] The astronomers used the AMBER instrument (Astronomical Multi-BEam combineR) and the VLTI to combine the light from all four of the 8.2-metre VLT Unit Telescopes and create a "virtual telescope" 130 metres across. [4] NACO (or NAOS-CONICA in full) is an adaptive optics instrument attached to ESO's Very Large Telescope. Thanks to adaptive optics, astronomers can remove most of the blurring effect of the atmosphere and obtain very sharp images. The team used NACO in a novel way, called sparse aperture masking (SAM) to search for the companion. This is a type of interferometry that, rather than combining the light from multiple telescopes as the VLTI does, uses different parts of the mirror of a single telescope (in this case, the mirror of the VLT Unit Telescope 4). This new technique is particularly good for finding faint objects very close to bright ones. VLTI/AMBER is better suited to studying the structure of the inner disc and is less sensitive to the presence of a distant companion. [5] The astronomers searched for the companion using NACO in two different spectral bands - at around 2.2 microns and at 3.8 microns. The companion is only seen at the longer wavelength, which means that the object is either cool, like a planet, or a dust-shrouded brown dwarf. [6] Brown dwarfs are objects between stars and planets in size. They are not massive enough to fuse hydrogen in their cores but are larger than giant planets such as Jupiter. More information This research was presented in two papers: Olofsson et al. 2011, "Warm dust resolved in the cold disk around TCha with VLTI/AMBER", and Huélamo et al. 2011, "A companion candidate in the gap of the T Cha transitional disk", to appear in the journal Astronomy & Astrophysics. The team is composed of J. Olofsson (Max-Planck-Institut für Astronomie [MPIA], Heidelberg, Germany), M. Benisty (MPIA), J.-C. Augereau (Institut de Planétologie et d'Astrophysique de Grenoble [IPAG], France) C. Pinte (IPAG), F. Ménard (IPAG), E. Tatulli (IPAG), J.-P. Berger (ESO, Santiago, Chile), F. Malbet (IPAG), B. Merín (Herschel Science Centre, Madrid, Spain), E. F. van Dishoeck (Leiden University, Holland), S. Lacour (Observatoire de Paris, France), K. M. Pontoppidan (California Institute of Technology, USA), J.-L. Monin (IPAG), J. M. Brown (Max-Planck-Institut für extraterrestrische Physik, Garching, Germany), G. A. Blake (California Institute of Technology), N. Huélamo (Centro de Astrobiología, ESAC, Spain), P. Tuthill (University of Sydney, Australia), M. Ireland (University of Sydney), A. Kraus (University of Hawaii) and G. Chauvin (Université Joseph Fourier, Grenoble, France). ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organisation in Europe and the world's most productive astronomical observatory. It is supported by 15 countries: Austria, Belgium, Brazil, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world's most advanced visible-light astronomical observatory and VISTA, the world's largest survey telescope. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 42-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become "the world's biggest eye on the sky".

Data Citation in Astronomy

NASA Astrophysics Data System (ADS)

Hourcle, Joseph

2014-06-01

Many observatories maintain bibliographies to document their impact and justify their continued funding[1], an effort that requires humans to discover and curate links between the scientific papers and the data that was used as evidence. The "Best Practices for Creating a Telescope Bibliography", endorsed by IAU C5 WG Libraries, recommends full text searching and human examination of each paper.[2] These efforts do not scale well.It is unlikely that articles published in journals from other disciples would be found. This is particularly a problem for solar physics, as solar data has applicability in astrophysics, space weather, and even the earth sciences.As our scientists are not on the editorial boards of the journals from other disciplines, we can't ensure proper attribution to allow these relationships to be discovered via full text searching.To better deal with tracking cross-discipline data usage, a number of groups have come up with guidelines and principles for data citation. In 2012, the National Academy's Board on Research Data and Information released the report "For Attribution-Developing Data Attribution and Citation Practices and Standards" [3] and it was followed last year by the CODATA-ICSTI report "Out of Cite, Out of Mind".[4]Participants from a number of groups synthesized a single set of principles for data citation that could be endorsed by all groups involved in research.[5] Implementing these principles can help to improve the scientific ecosystem by giving proper attribution to all contributors to data, improving transparency and reproducability, and making data more easily reusable to both astronomers and other researchers.We will present the Joint Declaration of Data Citation Principles, discuss the implications of them for astronomical data, and recommend steps towards implementation.References:[1] Accomazzi, et.al, 2012. http://adsabs.harvard.edu/abs/2012SPIE.8448E..0KA[2] Bishop, Grothkopf & Lagerstrom, 2012. http://iau-commission5.wikispaces.com/file/view/Best+Practices+Final.pdf[3] National Research Council, 2012. http://www.nap.edu/catalog.php?record_id=13564[4] CODATA, 2013. http://dx.doi.org/10.2481/dsj.OSOM13-043[5] FORCE11, 2014. http://www.force11.org/datacitation

Storing Astronomical Information on the Romanian Territory

NASA Astrophysics Data System (ADS)

Stavinschi, Magda; Mioc, Vasile

The Romanian astronomy has a more than 2000-year old tradition which is however too little known abroad. The first known archive of astronomical information is the Dacian sanctuary at Sarmizegetusa Regia very similar to that of Stonehenge. After a gap of more than 1000 years sources of astronomical information became to be recovered. They consist mainly of records of astronomical events seen on the Romanian territory. The most safe places to store these genuine archives were the monasteries. We present a classification of the manners of storing astronomical information along with characteristic examples.

Development of Very Long Baseline Interferometry (VLBI) techniques in New Zealand: Array simulation, image synthesis and analysis

NASA Astrophysics Data System (ADS)

Weston, S. D.

2008-04-01

This thesis presents the design and development of a process to model Very Long Base Line Interferometry (VLBI) aperture synthesis antenna arrays. In line with the Auckland University of Technology (AUT) Institute for Radiophysics and Space Research (IRSR) aims to develop the knowledge, skills and experience within New Zealand, extensive use of existing radio astronomical software has been incorporated into the process namely AIPS (Astronomical Imaging Processing System), MIRIAD (a radio interferometry data reduction package) and DIFMAP (a program for synthesis imaging of visibility data from interferometer arrays of radio telescopes). This process has been used to model various antenna array configurations for two proposed New Zealand sites for antenna in a VLBI array configuration with existing Australian facilities and a passable antenna at Scott Base in Antarctica; and the results are presented in an attempt to demonstrate the improvement to be gained by joint trans-Tasman VLBI observation. It is hoped these results and process will assist the planning and placement of proposed New Zealand radio telescopes for cooperation with groups such as the Australian Long Baseline Array (LBA), others in the Pacific Rim and possibly globally; also potential future involvement of New Zealand with the SKA. The developed process has also been used to model a phased building schedule for the SKA in Australia and the addition of two antennas in New Zealand. This has been presented to the wider astronomical community via the Royal Astronomical Society of New Zealand Journal, and is summarized in this thesis with some additional material. A new measure of quality ("figure of merit") for comparing the original model image and final CLEAN images by utilizing normalized 2-D cross correlation is evaluated as an alternative to the existing subjective visual operator image comparison undertaken to date by other groups. This new unit of measure is then used ! in the presentation of the results to provide a quantative comparison of the different array configurations modelled. Included in the process is the development of a new antenna array visibility program which was based on a Perl code script written by Prof Steven Tingay to plot antenna visibilities for the Australian Square Kilometre Array (SKA) proposal. This has been expanded and improved removing the hard coded fixed assumptions for the SKA configuration, providing a new useful and flexible program for the wider astronomical community. A prototype user interface using html/cgi/perl was developed for the process so that the underlying software packages can be served over the web to a user via an internet browser. This was used to demonstrate how easy it is to provide a friendlier interface compared to the existing cumbersome and difficult command line driven interfaces (although the command line can be retained for more experienced users).

Nicolas Donitch. Solved enigmas. (Nicolae Donici. Enigme descifrate)

NASA Astrophysics Data System (ADS)

Stavinschi, Magda

2015-12-01

The book is the most complete historical -scientific biography of the astronomer N.N. Donitch (1874, Chisinau, Bessarabia- 1960, Nice, France). It include many photographs, recollections on him by astronomers from many countries, archive documents. Main scientific interests and results has been described in detail. The activity of the astronomer in Astronomical Societies and IAU over the time has been described also. A list of publications has been given with a list of references on his personalty. The book is designed for a large circle of readers - from scientific researchers to students and non-astronomers yet. A number of contributions from philologist Haralambie Corbu, writer Iurie Colesnic, Director of the Odessa Astronomical Observatory S.M. Andrievskii, French astronomers Auduin Charles Dollfus, Gualtiero Olivieri, Paul Danjon, Romanian researchers Mircea Herovanu, Vladimir Boico, Gh. Teodoreanu, Gheorghe Rascu, Zoe Donici in the connection with the biography of N.N. Donitch has been included also. The book is richly illustrated by photographs and documents from archives.

GNAT: A Global Network of Astronomical Telescopes

NASA Astrophysics Data System (ADS)

Crawford, David L.

1995-12-01

Astronomical resources are increasingly directed toward development of very large telescopes, and many facilities are compelled to cease operations of smaller telescopes. A real concern is emerging with respect to issues of access to astronomical imaging systems for the majority of astronomers who will have little or no opportunity to work with the larger telescopes. Further concern is developing with regard to the means for conducting observationally intensive fundamental astronomical imaging programs, such as surveys, monitoring, and standards calibration. One attractive potential solution is a global network of (automated) astronomical telescopes (GNAT). Initial steps have been taken to turn this network into a reality. GNAT has been incorporated as a nonprofit corporation, membership drives have begun and several institutions have joined. The first two open GNAT meetings have now been held to define hardware and software systems, and an order has been placed for the first of the GNAT automated telescopes. In this presentation we discuss the goals and status of GNAT and its implications for astronomical imaging.

Child Care Gifts to Bolster Astronomy

NASA Astrophysics Data System (ADS)

Nemiroff, Robert J.; Allen, Alice

2016-01-01

Caring for children should not derail potentially excellent future astronomers. It is therefore suggested that a mechanism be created for established astronomers to voluntarily will 10 percent of their estate to a fund that helps aspiring astronomers reduce child care costs. Statistics indicate that many scientists delay child rearing until they have secure jobs. This delay appears to be based on the early relative cost of child care and the perception that time spent raising children negatively impacts job performance and future employability. Having even a portion of child care expenses covered may increase the efficiency of early-career education and productivity of early-career scientific research. It is hoped that some established astronomers may be inspired to contribute by remembering their own lives as aspiring astronomers, while also wishing to add to their legacy. Only an expression of interest is requested here, both from established astronomers who might be interested in taking such a donation pledge, and from aspiring astronomers who feel their careers would be helped by child care assistance.

Astronomical catalog desk reference, 1994 edition

NASA Technical Reports Server (NTRS)

1994-01-01

The Astronomical Catalog Desk Reference is designed to aid astronomers in locating machine readable catalogs in the Astronomical Data Center (ADC) archives. The key reference components of this document are as follows: A listing of shortened titles for all catalogs available from the ADC (includes the name of the lead author and year of publication), brief descriptions of over 300 astronomical catalogs, an index of ADC catalog numbers by subject keyword, and an index of ADC catalog numbers by author. The heart of this document is the set of brief descriptions generated by the ADC staff. The 1994 edition of the Astronomical Catalog Desk Reference contains descriptions for over one third of the catalogs in the ADC archives. Readers are encouraged to refer to this section for concise summaries of those catalogs and their contents.

Cost-effectiveness of everolimus for second-line treatment of metastatic renal cell carcinoma in Serbia.

PubMed

Mihajlović, Jovan; Pechlivanoglou, Petros; Sabo, Ana; Tomić, Zdenko; Postma, Maarten J

2013-12-01

New targeted therapeutics for metastatic renal cell carcinoma (mRCC) enable an increment in progression-free survival (PFS) ranging from 2 to 6 months. Compared with best supportive care, everolimus demonstrated an additional PFS of 3 months in patients with mRCC whose disease had progressed on sunitinib and/or sorafenib. The only targeted therapy for mRCC currently reimbursed in Serbia is sunitinib. The aim of this study was to estimate the cost-effectiveness and the budget impact of the introduction of everolimus in Serbia in comparison to best supportive care, for mRCC patients refractory to sunitinib. A Markov model was designed corresponding with Serbian treatment protocols. A health care payer perspective was taken, including direct costs only. Treated and untreated cohorts were followed up over 18 cycles, each cycle lasting 8 weeks, which covered the lifetime horizon of mRCC patients refractory to the first-line treatment. Annual discounted rates of 1.5% for effectiveness and 3% for costs were applied. Transitions between health states were modeled by time-dependent probabilities extracted from published Kaplan-Meier curves of PFS and overall survival (OS). Utility values were obtained from the appraisals of other mRCC treatments. One-way and probabilistic sensitivity analyses were done to test the robustness and uncertainty of the base-case estimate. Lastly, the potential impacts of everolimus on the overall health care expenditures on annual and 4-year bases were estimated in the budget-impact analysis. The incremental cost-effectiveness ratio for everolimus was estimated at €86,978 per quality-adjusted life-year. Sensitivity analysis identified the hazard multiplier, a statistical approximator of OS gain, as the main driver of everolimus cost-effectiveness. Furthermore, probabilistic sensitivity analyses revealed a wide 95% CI around the base-case incremental cost-effectiveness ratio estimate (€32,594-€425,258 per quality-adjusted life-year). Finally, an average annual budgetary impact of everolimus in first 4 years after its potential reimbursement would be around €270,000, contributing to <1% of the total budget in Serbian oncology. Everolimus as a second-line treatment of mRCC is not likely to be a cost-effective option under the present conditions in Serbia, with a relatively limited impact on its budget in oncology. A major constraint on the estimation of the cost-effectiveness of everolimus relates to the uncertainty around the everolimus effect on extending OS. However, prior to a final decision on the acceptance/rejection of everolimus, reassessment of the whole therapeutic group might be needed to construct an economically rational treatment strategy within the mRCC field. © 2013 Elsevier HS Journals, Inc. All rights reserved.

Amateur Astronomers: Secret Agents of EPO

NASA Astrophysics Data System (ADS)

Berendsen, M.; White, V.; Devore, E.; Reynolds, M.

2008-06-01

Amateur astronomers prime the public to be more interested, receptive, and excited about space science, missions, and programs. Through recent research and targeted programs, amateur astronomy outreach is being increasingly recognized by professional astronomers, educators, and other amateurs as a valued and important service. The Night Sky Network program, administered by the ASP, is the first nationwide research-based program specifically targeted to support outreach by amateur astronomers. This Network of trained and informed amateur astronomers can provide a stimulating introduction to your EPO programs as Network members share the night sky with families, students, and youth groups.

Riferimenti, simboli e numerologia astronomica nel Canzoniere di Petrarca

NASA Astrophysics Data System (ADS)

Colona, Paolo

The astronomical knowledge of Petrarch and his use of astronomical references in the renowned Canzoniere are examined with a commented anthology of the most relevant astronomical verses in that work. We discuss the identification of the first two verses of the poetry "Solo et pensoso" as a precise description of the astrological type of Saturn. The repeated presence of an ancient astronomical symbol such as the division of the circle in 12 parts is highlighted. The coded presence in the Canzoniere of the most relevant astronomical numbers 7, 12 and 365 is also discovered and shown.

Astronomical Symbolism in Australian Aboriginal Rock Art

NASA Astrophysics Data System (ADS)

Norris, Ray P.; Hamacher, Duane W.

2011-05-01

Traditional Aboriginal Australian cultures include a significant astronomical component, perpetuated through oral tradition and ceremony. This knowledge has practical navigational and calendrical functions, and sometimes extends to a deep understanding of the motion of objects in the sky. Here we explore whether this astronomical tradition is reflected in the rock art of Aboriginal Australians. We find several plausible examples of depictions of astronomical figures and symbols, and also evidence that astronomical observations were used to set out stone arrangements. However, we recognise that the case is not yet strong enough to make an unequivocal statement, and describe our plans for further research.

Reverend Doctor William Pearson in South Kilworth, Leicestershire

NASA Astrophysics Data System (ADS)

Frost, M. A.

2006-12-01

William Pearson (1767-1847) was a 19th-century astronomer, renowned for his work in positional astronomy and the design of astronomical instruments, both practical and instructional. He was a co-founder in 1820 of the Astronomical Society of London, which later became the Royal Astronomical Society, where his portrait hangs. For 30 years of his astronomical career he was the Rector of South Kilworth, a village in Leicestershire, England, where he erected several observatory buildings, as well as extending the village church and building the village schoolroom. This paper documents his activities in South Kilworth.

Language Politics in Bosnia, Croatia, and Serbia

DTIC Science & Technology

2010-03-01

Toward a Common Standard ( Zagreb , Croatia: Globus, 1995), 14. 8 Alexander, Bosnian, Croatian, Serbian, 380–381. 9 Stanley G. Evans, A Short History...Yugoslav Academy of Sciences and Arts in Zagreb in 1867. The Yugoslav Academy contained the first institution concerned with south Slavic languages...northern Croatia, especially in the Zagreb area, and Čakavian is spoken along the Adriatic coast in Dalmatia and on the Istrian peninsula.33 Another

JPRS Report, East Europe

DTIC Science & Technology

1988-01-14

Under Law of Enterprise Viewed [RUDE PRAVO, 22 Oct 87] 18 Profit Tax Under Restructuring of Economy Discussed [Ladislav Machon; FINANCE A UVER, No 7... Chruch press, and there is also advocacy of "the exclusive concern for the souls" of Serbs, especially in Kosovo. In addiiton to anti-Yugoslav and...for "reconciliaiton" of the Serbian Orthodox Chruch with schismatic factions abroad. Pressures are also being exerted on the leadership of the

Lessons from Kosovo: The KFOR Experience

DTIC Science & Technology

2002-07-01

There are wide extremes of weather and terrain, a mix of urban and rural, modern and primitive, and upscale and slum. Transportation routes are...systems for exchanging information and coordinating actions—it became the de facto formal messaging system. For the United States, the highly secure...education in their own language, and exposed to massive abuse of their human rights and civil liberties. Kosovo became a de facto Serbian colony where 90

From Bosnia to Baghdad: The Evolution of US Army Special Forces From 1995-2004

DTIC Science & Technology

2004-09-01

BIJELJINA (OPERATION JOINT FORGE)............................... 13 H . FROM JCO TO SR (OPERATION ALLIED FORCE)......................... 14 I. SPECIAL...would only work with and report on Serbian villages and “Bosniak teams” exclusively focusing their efforts upon Bosnian Muslim villages.25 H . FROM JCO...processing station. Ramadani , the Sefer faction leader, arrived the next day at the demobilization point with approximately 40 faction members, including

Inclusive Security: NATO Adapts and Adopts

DTIC Science & Technology

2016-03-01

Bosnia . But only four years later, the limits of the agreement became clear. General Wesley Clark, a principal figure in the negotiations that ended the...violence in Bosnia , led NATO in a bombing campaign against the regime of Serbian President Slobodan Milosevic (later charged with war crimes), whose...army was behind escalating violence against civilians in Kosovo. We had already seen how Milosevic’s tactics played out in Bosnia . Swanee Hunt: I’d

JPRS Report, East Europe.

DTIC Science & Technology

1990-02-20

percent of teinagbdclrdhttey there are r asons (tending to be outside politics) for were satisfied with Markovic’s agricultural policy . It is...respondents than anti- Serbian nationality was 23.9. Nevertheless, even these inflation policy and agricultural policy . There, 26.4 results show that... agricultural policy of the FEC that has received many production surveyed, but of only 47 percent of those in objections during Markovic’s term, it is

Implications of an Independent Kosovo for Russia’s Near Abroad

DTIC Science & Technology

2007-10-01

as Chair of the Standing Committee on International Law and Ethics of the World Association for Disaster and Emergency Medicine . He is admitted to...of Kosovar Albanians converted to Islam, while Serbs remained Serbian Orthodox. More than 500 years later, Serbia and Montenegro regained the...massive amounts of funding would be needed to build new plants and/or overhaul existing structures. Without final status resolution, investors are

Deciphering the Balkan Enigma: Using History to Inform Policy. Revised Edition,

DTIC Science & Technology

1995-11-07

After long experience with German interference in Serbian/Yugoslav affairs (1878, 1908, 1914 - 1918 ), it should not be surprising that the Yugoslav...background to the religious, as well as political differences between the various branches of the church and the division, see Robert R. Palmer and Joel...comprehensive solution prior to embarking on incremental ways to resolve issues. _ Political institutions are weak. This condition complicates

The July Crisis: Can You Stop the Great War? Grade 10 Lesson. Schools of California Online Resources for Education (SCORE): Connecting California's Classrooms to the World.

ERIC Educational Resources Information Center

Antilla, Madeline

On June 28, 1914, while visiting Sarajevo in Bosnia-Herzegovina, Archduke Franz Ferdinand, heir to the Austro-Hungarian empire, was assassinated. The Austrian government blamed Serbia for harboring terrorists and sent the Serbian government an ultimatum with which that country found it impossible to comply. This set in motion a series of…

JPRS Report, East Europe.

DTIC Science & Technology

1991-03-28

deputy to the National Assembly. Although both men are members of the SPS, Dusan Bokalovic and Slobodan Marjanovic obviously do not drink water from...the same party fountain. In the Serbian socialists big nominating game, Marjanovic had to give up his place to Mihalj Kertes in the Kaludjerica...to Marjanovic is hinted at in part by the fact that Kertes was informed that he must personally go to Grocka to acknowledge his election as deputy

The Pacification Campaign of Madagascar: 1896-1905

DTIC Science & Technology

2002-01-01

and 1940s. This was no improvised brutality. My German colleague, Rudolf Scharping revealed on 9 April details of a covert Serbian plan, code-named...administrator arrived to begin attempts to transfer authority to local institutions and to work to improve security and boost the economy. Steiner , a...Yugoslav President Slobodan Milosevic’s crackdown on ethnic Albanians in the province. Steiner also said he would focus on creating jobs in the province

Daily Report, Supplement, East Europe

DTIC Science & Technology

1993-07-26

Amphetamine Production Viewed [TRYBUNA 19-20 JunJ 20 ROMANIA Voters, Officials Contrast Views of Parliament [LIBERTATEA 19-20 JunJ 22 SLOVAKIA...Macedonia, who informed him that the MPC [Macedonian Orthodox Church] was prepared to appoint Serbian priests but under the jurisdiction of the...in Serbia, as well as in Romania and Bulgaria?; are coal miners earning as much as 2,000 German marks [DM] each while the people of Banja Luka sit

War in the Balkans, 1991-2002

DTIC Science & Technology

2003-08-01

Unit, a secret police organ now disbanded. 16. The event was dubbed the “ Yogurt Revolution” after the demonstrators pelted local officials with... yogurt containers. The radical Serb nationalist leader Vojislav Šešelj would later claim that the entire episode was organized by the Serbian secret...including a stint as advisor for the Sarajevo professional soccer squad. During the political ferment of 1990 Karadžić briefly supported the

The Berlin-Baghdad Railway as a cause of World War I.

DTIC Science & Technology

1984-01-01

complex succession of events which culminated in a world war, and for this Serbian nationalism was ultimately responsible." - 12 - The essence of...and began to cut loose from Turkey (Brandenburg, [ 12 ]). The French and English began working together against Germany in the Public Debt Administration...Rivalry 12 . Brandenburg, Erich. From Bismarck to the World War: A History of German Foreign Policy, 1870-1914. London, 1927. (Brandenburg briefly

Effect of Serbian Orthodox Religious Teaching on the Morality of Youth--Eschatological Aspect

ERIC Educational Resources Information Center

Kacaric, Ninoslav

2015-01-01

This paper presents the findings on the system of values and moral functioning of the youth-- students of religious education, Orthodox Christians, in Serbia (sample of 446 respondents representing the 7th and 8th grades of primary school, and 3rd and 4th grade of secondary schools in the territory of the Diocese of Banat), and it is a part of the…

Size of the lower third molar space in relation to age in Serbian population.

PubMed

Zelić, Ksenija; Nedeljković, Nenad

2013-10-01

It is considered that the shortage of space is the major cause of the third molar impaction. The aim of this study was to establish the frequency of insufficient lower third molar eruption space in Serbian population, to question the differences in this frequency in the subjects of different age, to determine the influence of the lower third molar space (retromolar space) size on third molar eruption, and to investigate a possible correlation between the size of gonial angle and the space/third molar width ratio. Digital orthopantomograms were taken from 93 patients divided into two groups: early adult (16-18 years of age) and adult (18-26) patients. Retromolar space, mesiodistal third molar crown width, gonial angle and eruption levels were measured. The space/third molar width in early adult subjects was smaller (p < 0.0001) and insufficient space was significantly more frequent (p = 0.0003) than in adult patients. Considerably more third molars erupted in case of enough space in both age groups (p < 0.0001). There was no difference between the means of gonial angle size in relations to the available space. The retromolar space/third molar width ratio is more favorable in adult subjects. Gonial angle is not in correlation with the retromolar space/third molar width ratio.

Somatotype of Top-Level Serbian Rhythmic Gymnasts

PubMed Central

Purenović-Ivanović, Tijana; Popović, Ružena

2014-01-01

Body size and build influence performance in many sports, especially in those belonging to the group of female aesthetic sports (rhythmic gymnastics, artistic gymnastics, and figure skating). These sports pose high specific demands upon the functional, energy, motor and psychological capacities of athletes, but also upon the size, body build and composition of the performers, particularly of the top-level female athletes. The study of the top athletes (rhythmic gymnasts, in this case) may provide valuable information on the morphological requirements for achieving success in this sport. Therefore, the main objective of this research was to analyze the somatotype of 40 Serbian top-level rhythmic gymnasts, aged 13.04±2.79, and to form the five age group categories. The anthropometric variables included body height, body mass, the selected diameters, girths and skinfolds, and the Heath-Carter anthropometric somatotype. All of the anthropometric data were collected according to International Biological Programme, and then processed in the Somatotype 1.2. The applied analysis of variance indicated an increase in endomorphic component with age. The obtained results show that the balanced ectomorph is a dominant somatotype, being similar for all of the athletes that took part in the research (3.54-3.24-4.5). These results are in line with the ones obtained in previous studies. PMID:25031686

Somatotype of top-level serbian rhythmic gymnasts.

PubMed

Purenović-Ivanović, Tijana; Popović, Ružena

2014-03-27

Body size and build influence performance in many sports, especially in those belonging to the group of female aesthetic sports (rhythmic gymnastics, artistic gymnastics, and figure skating). These sports pose high specific demands upon the functional, energy, motor and psychological capacities of athletes, but also upon the size, body build and composition of the performers, particularly of the top-level female athletes. The study of the top athletes (rhythmic gymnasts, in this case) may provide valuable information on the morphological requirements for achieving success in this sport. Therefore, the main objective of this research was to analyze the somatotype of 40 Serbian top-level rhythmic gymnasts, aged 13.04±2.79, and to form the five age group categories. The anthropometric variables included body height, body mass, the selected diameters, girths and skinfolds, and the Heath-Carter anthropometric somatotype. All of the anthropometric data were collected according to International Biological Programme, and then processed in the Somatotype 1.2. The applied analysis of variance indicated an increase in endomorphic component with age. The obtained results show that the balanced ectomorph is a dominant somatotype, being similar for all of the athletes that took part in the research (3.54-3.24-4.5). These results are in line with the ones obtained in previous studies.

Administering the Sarcoidosis Health Questionnaire to sarcoidosis patients in Serbia.

PubMed

Mihailović-Vučinić, Violeta; Gvozdenović, Branislav; Stjepanović, Mihailo; Vuković, Mira; Marković-Denić, Ljiljana; Milovanović, Aleksandar; Videnović-Ivanov, Jelica; Žugić, Vladimir; Škodrić-Trifunović, Vesna; Filipović, Snežana; Omčikus, Maja

2016-04-01

The aim of this study was to use a Serbian-language version of the disease-specific, self-report Sarcoidosis Health Questionnaire (SHQ), which was designed and originally validated in the United States, to assess health status in sarcoidosis patients in Serbia, as well as validating the instrument for use in the country. This was a cross-sectional study of 346 patients with biopsy-confirmed sarcoidosis. To evaluate the health status of the patients, we used the SHQ, which was translated into Serbian for the purposes of this study. We compared SHQ scores by patient gender and age, as well as by disease duration and treatment. Lower SHQ scores indicate poorer health status. The SHQ scores demonstrated differences in health status among subgroups of the sarcoidosis patients evaluated. Health status was found to be significantly poorer among female patients and older patients, as well as among those with chronic sarcoidosis or extrapulmonary manifestations of the disease. Monotherapy with methotrexate was found to be associated with better health status than was monotherapy with prednisone or combination therapy with prednisone and methotrexate. The SHQ is a reliable, disease-specific, self-report instrument. Although originally designed for use in the United States, the SHQ could be a useful tool for the assessment of health status in various non-English-speaking populations of sarcoidosis patients.

Ivan Djaja (Jean Giaja)1 and the Belgrade School of Physiology

PubMed Central

Andjus, Pavle R.; Stojilkovic, Stanko S.; Cvijic, Gordana

2016-01-01

Summary The founder of physiology studies in the Balkans and the pioneer of research on hypothermia, Ivan Djaja (Jean Giaja) was born 1884 in L’Havre. Giaja gained his PhD at the Sorbonne in 1909. In 1910 he established the first Chair of Physiology in the Balkans and organized the first Serbian Institute for Physiology at the School of Philosophy of the University of Belgrade. He led this Institute for more than 40 subsequent years. His most notable papers were in the field of thermoregulation and bioenergetics. Djaja became member of the Serbian and Croatian academies of science and doctor honoris causa of Sorbonne. In 1952 for the seminal work on the behaviour of deep cooled warm blooded animals he becane associate member of the National Medical Academy in Paris. In 1955 the French Academy of Sciences elected him as associate member in place of deceased Sir Alexander Fleming. Djaja died in 1957 during a congress held in his honour. He left more than 200 scientific and other papers and the golden DaVincian credo “Nulla dies sine experimento”. His legacy was continued by several generations of researchers, the most prominent among them being Stefan Gelineo, Radoslav Andjus and Vojislav Petrović. PMID:21777022

Education in Medical Biochemistry in Serbia

PubMed Central

2010-01-01

Medical biochemistry is the usual name for clinical biochemistry or clinical chemistry in Serbia. Medical biochemistry laboratories and medical biochemists as a profession are part of Health Care System and are regulated through: the Health Care Law and rules issued by the Chamber of Medical Biochemists of Serbia. The first continuous and organized education for Medical Biochemists in Serbia dates from 1945, when Department of Medical Biochemistry was established at Pharmaceutical Faculty in Belgrade. In 1987 at the same Faculty a five years undergraduate branch was established, educating Medical Biochemists under a special program. Since 2006 the new five year undergraduate (according to Bologna Declaration) and postgraduate program of four-year specialization according to EC4 European Syllabus for Post-Graduate Training in Clinical Chemistry and Laboratory Medicine has been established. The Ministry of Education and Ministry of Public Health accredits the programs. There are four requirements for practicing medical biochemistry in the Health Care System: University Diploma of the Faculty of Pharmacy (Medical Biochemistry), successful completion of the profession exam at the Ministry of Health after completion of one additional year of obligatory practical training in medical laboratories, membership in the Serbian Chamber of Medical Biochemists and licence for skilled work issued by Serbian Chamber of Medical Biochemists. PMID:27683360

Alkali-activated concrete with Serbian fly ash and its radiological impact.

PubMed

Nuccetelli, Cristina; Trevisi, Rosabianca; Ignjatović, Ivan; Dragaš, Jelena

2017-03-01

The present paper reports the results of a study on different types of fly ash from Serbian coal burning power plants and their potential use as a binder in alkali-activated concrete (AAC) depending on their radiological and mechanical properties. Five AAC mixtures with different types of coal burning fly ash and one type of blast furnace slag were designed. Measurements of the activity concentrations of 40 K, 226 Ra and 232 Th were done both on concrete constituents (fly ash, blast furnace slag and aggregate) and on the five solid AAC samples. Experimental results were compared by using the activity concentration assessment tool for building materials - the activity concentration index I, as introduced by the EU Basic Safety Standards (CE, 2014). All five designed alkali-activated concretes comply with EU BSS screening requirements for indoor building materials. Finally, index I values were compared with the results of the application of a more accurate index - I(ρd), which accounts for thickness and density of building materials (Nuccetelli et al., 2015a). Considering the actual density and thickness of each concrete sample index - I(ρd) values are lower than index I values. As an appendix, a synthesis of main results concerning mechanical and chemical properties is provided. Copyright © 2016 Elsevier Ltd. All rights reserved.

Attitudes of Serbian food technology students towards surgical and immunocastration of boars and their sensitivity to androstenone and skatole

NASA Astrophysics Data System (ADS)

Tomasevic, I.; Đekić, I.; Font-i-Furnols, M.; Aluwé, M.; Čandek-Potokar, M.; Bonneau, M.; Weiler, U.

2017-09-01

Various European Union pork chain actors and stakeholders agreed in 2010 on a road map to voluntarily abandon piglet castration by 1 January 2018. Because currently in Serbia, male piglets are surgically castrated and consumers are not used to the boar taint odour and flavour, the introduction of boar meat may modify the acceptability of pork. The objective of the study was to investigate the attitudes, awareness and opinions of future Serbian food technologist towards surgical castration of boars and its alternatives, and to test their sensitivity to androstenone and skatole. We found that they were concerned about the animal welfare issues and that they were willing to pay a little more for meat from animals treated with dignity. This was more so if they were females and less so if they had had a rural upbringing. They strongly believed that surgical castration is painful for the animals, but at the same time agreed that meat from castrated pigs is of better quality. Their ambiguous attitudes regarding efficacy and quality of alternatives to surgical castration clearly indicated the knowledge gap that must be filled by appropriate modifications of the curriculum. Students demonstrated average sensitivity to both androstenone and skatole. Females exhibited higher intensities of difference in both cases.

The Opportunities of Crises and Emergency Risk Communication in Activities of Serbian Public Health Workforce in Emergencies

PubMed Central

Radović, V; Ćurčić, L

2012-01-01

Background: The aim of the study was a recommendation and establishment the concept of the appropriate communication between public health, other competent services and population in emergency as the corner stone which guarantee that all goals which are important for community life will be achieved. Methods: We used methodology appropriate for social science: analyses of documents, historical approach and comparative analysis. Results: The finding shows the urgent need for accepting of crises and emergency risk communication principles, or some similar concepts, in Serbia, and implementing effective two way communication especially in multiethnic region. The pragmatic value of the paper lays in information about the recent improvement of health workforce and emergency services in emergencies using new concept of communication and as source of numerous useful documents published in USA and few recent Serbian examples. Conclusion: Health workforce has significant role in the process of protection of population in emergencies. Policy makers should work on finding a way to improve their coordination and communication, creating new academic programs, providing of adequate training, and financial means in order to give them different role in society and provide visibility. From other side health workforce should build back to the citizen trust in what they are doing for society welfare using all their skills and abilities. PMID:23308348

Distribution of cadmium in leg muscle and liver of game birds from Serbia

NASA Astrophysics Data System (ADS)

Nikolić, D.; Đinović-Stojanović, J.; Stefanović, S.; Radičević, T.; Trbović, D.; Spirić, D.; Janković, S.

2017-09-01

The aim of this study was to present the distribution of cadmium (Cd) levels in leg muscle and liver of game birds. Samples (n=464) of: pheasants (n=182), mallards (n=25), Eurasian jay (n=7), partridges (n=5), woodcocks (n=8) and common quail (n=5) were collected during regular hunting seasons within the Serbian National Residue Monitoring Program from 2013 to 2016. Analysis of Cd was performed by ICP-MS. In all liver samples, Cd levels were above the limit of detection (LOD=0.001 mg/kg) while in 66.4% of muscle samples, Cd was detected. Statistical analysis showed significant differences between Cd levels in leg muscle and liver of woodcocks and others game birds. The highest mean Cd level was observed in muscle samples of woodcocks (0.042 mg/kg). The lowest mean Cd levels in liver were observed in common quails (0.130 mg/kg) and mallards (0.160 mg/kg) while the highest levels were measured in woodcocks (1.247 mg/kg) and pheasants (0.262 mg/kg). During four years of the Serbian National Residue Monitoring Program, leg muscle samples of woodcocks (n=3), liver samples of pheasants (n=23), woodcocks (n=6) and mallards (n=3) exceeded the maximum residue limit (MRL).

William Herschel's 'Hole in the Sky' and the discovery of dark nebulae

NASA Astrophysics Data System (ADS)

Steinicke, Wolfgang

2016-12-01

In 1785 William Herschel published a paper in the Philosophical Transactions containing the remarkable section "An opening or hole". It describes an unusual vacant place in Scorpius. This matter falls into oblivion until Caroline Herschel initiated a correspondence with her nephew John in 1833. It contains Herschel's spectacular words "Hier ist wahrhaftig ein Loch im Himmel" ("Here truly is a hole in the sky"). About a hundred years later, Johann Georg Hagen, Director of the Vatican Observatory, presented a spectacular candidate for the 'hole', discovered in 1857 by Angelo Secchi in Sagittarius and later catalogued by Edward E. Barnard as the dark nebula B 86. Hagen's claim initiated a debate, mainly in the Journal of the British Astronomical Association, about the identity of Herschel's 'object'. Though things could be partly cleared up, unjustified claims still remain. This is mainly due to the fact that original sources were not consulted. A comprehensive study of the curious 'hole' is presented here. It covers major parts of the epochal astronomical work of William, Caroline and John Herschel. This includes a general study of 'vacant places', found by William Herschel and others, and the speculations about their nature, eventually leading to the finding that dark nebulae are due to absorbing interstellar matter. Some of the 'vacant places' could be identified in catalogues of dark nebulae and this leads to a 'Herschel Catalogue of Dark Nebulae' - the first historic catalogue of its kind.

Astrobites: The Online Astronomy Research Digest for Undergraduates

NASA Astrophysics Data System (ADS)

Faesi, Christopher; Astrobites Collaboration

2013-06-01

Astrobites (http://astrobites.org) is an innovative science education initiative developed by graduate students in astrophysics for an undergraduate audience. Our goal is to help undergraduates make the transition from the classroom to careers in research by introducing them to the astronomical literature in a pedagogical, approachable, and comprehensible way. Every day we select one new journal article posted to the astrophysics preprint server (http://arXiv.org/astro-ph) and prepare a brief summary describing methods and results, explaining jargon, and providing context. We also write regular blog posts containing career advice, such as tips for applying for graduate school, how to install astronomical software, or demystifying the publishing process. The articles are written by a team of about 30 graduate students in astrophysics from throughout the US and Europe. Since its founding in 2010, Astrobites has grown dramatically, now reaching more than 1000 daily readers in over 100 countries worldwide. Our audience includes not only undergraduates, but also interested non-scientists, educators, and professional researchers. More broadly, Astrobites is interested in fostering the development of vital communication skills that are crucial to a successful science career, yet not formally taught in most astronomy PhD programs. In addition to providing our graduate student authors with valuable opportunities to practice these skills through writing and editing articles, we organize events such as the upcoming workshop Communicating Science 2013, at which graduate students in all science fields from around the country will learn from and interact with panelists who are experts in science communication.

Optical Characteristics of Astrometric Radio Sources OCARS

NASA Astrophysics Data System (ADS)

Malkin, Z.

2013-04-01

In this paper, the current status of the catalog of Optical Characteristics of Astrometric Radio Sources OCARS is presented. The catalog includes radio sources observed in various astrometric and geodetic VLBI programs in 1979-2012. For these sources the physical object type, redshift and visual or infrared magnitude is given when available. Detailed comments are provided when some problems with published data were encountered. Since the first version created in December 2007, the catalog is continuously developed and expanded in respect to inclusion of new radio sources and addition of new or correction of old astrophysical data. Several sources of information are used for OCARS. The main of them are the NASA/IPAC Extragalactic Database (NED) and SIMBAD astronomical databases. Besides several astronomical journals and arXiv depository are regularly monitored, so that new data is included in OCARS just after publication. The redshift for about 150 sources have been determined from dedicated optical spectroscopic observations. As of October 2012, OCARS catalog includes 7173 radio sources. 3898 sources have known redshift, and 4860 sources have known magnitude. In 2009, it was used as a supplement material to the ICRF2. The list of radio sources with a good observational history but lacking astrophysical information is provide for planning of optical observations of the most important astrometric sources. The OCARS catalog is updated, in average every several weeks and is available at http://www.gao.spb.ru/english/as/ac_vlbi/ocars.txt.

Into the Chrysalis

NASA Astrophysics Data System (ADS)

2007-09-01

A team of European astronomers has used ESO's Very Large Telescope Interferometer and its razor-sharp eyes to discover a reservoir of dust trapped in a disc that surrounds an elderly star. The discovery provides additional clues about the shaping of planetary nebulae. ESO PR Photo 43/07 ESO PR Photo 43/07 A Disc Around an Aged Star In the last phases of their life, stars such as our Sun evolve from a red giant which would engulf the orbit of Mars to a white dwarf, an object that is barely larger than the Earth. The transition is accomplished by the shedding of a huge envelope of gas and dust that sparkles in many colours, producing a most spectacular object: a planetary nebula. The celestial chrysalis becomes a cosmic butterfly. This metamorphosis, rapid in terms of the star's lifetime, is rather complex and poorly understood. In particular, astronomers want to understand how a spherical star can produce a great variety of planetary nebulae, some with very asymmetrical shapes. A team of scientists therefore embarked upon the study of a star which is presently on its way to becoming a cosmic butterfly. The star, V390 Velorum, is 5000 times as bright as our Sun and is located 2,600 light-years away. It is also known to have a companion that accomplishes its ballet in 500 days. Astronomers postulate that elderly stars with companions possess a reservoir of dust that is thought to play a lead role in the final chapters of their lives. The shape and structure of these reservoirs remain, however, largely unknown. To scrutinise the object with great precision, the astronomers linked observations taken with ESO's powerful interferometric instruments, AMBER and MIDI, at the Very Large Telescope Interferometer. In particular, they combined, using AMBER, the near-infrared light of three of VLT's 8.2-m Unit Telescopes. "Only this triple combination of powerful telescopes allows us to pinpoint the position and the shape of the dusty reservoir on a milli-arcsecond scale," explains Pieter Deroo, lead-author of the paper that presents these results in the research journal Astronomy and Astrophysics. These observations clearly demonstrate that the dust present around the star cannot be distributed in a spherical shell. "This shows that whatever mechanism is shaping asymmetric planetary nebulae is already present prior to the metamorphosis taking place," says Hans Van Winckel, member of the team. The astronomers found indeed evidence for a disc extending from 9 Astronomical Units to several hundreds of AU. "This disc is found around a star that is in a very brief phase of its life - just a blink of an eye over the star's lifespan of billions of years - but this phase is very important," says Deroo. "It is in this period that a huge morphological change occurs, leading to the creation of a planetary nebula," he adds. The very high spatial resolution measurements allowed the astronomers to decouple the unresolved contribution of the central star from the resolved disc emission. Even the very inner structure of the disc as well as its orientation and inclination could be determined. The observations probe the physical nature of the disc and reveal that the dust in the inner rim is extremely hot and puffed up. The disc is circumbinary as it surrounds both stars. Dust processing (coagulation, crystallisation) is found to be very efficient in this circumbinary disc, despite the rather short evolutionary timescales involved. The disc around this evolved object is very similar to those around young stellar objects, in which planets are formed. "The combination of MIDI and AMBER on ESO's VLTI is an extremely powerful and perhaps unique tool to study the geometry of the material around stars," concludes Van Winckel. It looks like it is the season for disc 'hunting': the detection of a dusty disc in the notable Ant Nebula was also just announced (see ESO 42/07).

Closest rocky exoplanet confirmed on This Week @NASA – July 31, 2015

NASA Image and Video Library

2015-07-31

NASA’s Spitzer Space Telescope has helped astronomers confirm the discovery of the nearest rocky planet outside our solar system. The planet, called HD 219134b, is a bit larger than Earth and located a mere 21 light-years away in the Cassiopeia constellation, near the North Star. While HD 219134b orbits too close to its star to sustain life, it is the closest exoplanet to Earth to be detected transiting, or crossing in front of, its star – which makes it perfect for extensive scientific research. The results of this discovery are the subject of a study accepted for publication in the journal Astronomy & Astrophysics. Also, Exoplanet found far from its central star, Orion fairing separation tests, NEEMO 20 mission, California’s “rain debt” and Unmanned Air Traffic Management!

The Meteor Section of the Visnjan School of Astronomy 1993

NASA Astrophysics Data System (ADS)

Korlevic, K.

In the last five years, the Visnjan Observatory started a new international astronomical summer workshop. Every year, on this educational activity, students have been thought the IMO standards of visual observation. Meteor astronomy was chosen as the leading activity because of its ability to bring people together, and because of the continuous flux of information through the IMO and the journal WGN, in the time when other sources of information were cut off by the war situation. The time of this years's school (August 7-20) covered the exceptional 1993 Perseids maximum. The Visnjan School of Astronomy is also an educational and psychological experiment, and our goal is finding a better means of introducing gifted students to science through astronomy workshops. In that effort we are also trying to increase the number of future meteor observers.

New Life for Astronomical Instruments of the Past at the Astronomical Observatory of Taras Shevchenko

NASA Astrophysics Data System (ADS)

Kazantseva, Liliya

2012-09-01

Astronomical instruments of the past are certainly valuable artifacts of the history of science and education. Like other collections of scientific equipment, they also demonstrate i) development of scientific and technical ideas, ii) technological features of the historical period, iii) professional features of artists or companies -- manufacturers, and iv) national and local specificity of production. However, astronomical instruments are also devices made for observations of rare phenomena -- solar eclipses, transits of planets of the solar disk, etc. Instruments used to study these rare events were very different for each event, since the science changed quickly between events. The Astronomical Observatory of Kyiv National Taras Shevchenko University has a collection of tools made by leading European and local shops from the early nineteenth century. These include tools for optically observing the first artificial Earth satellites, photography, chronometry, and meteorology. In addition, it has assembled a library of descriptions of astronomical instruments and makers'price-lists. Of particular interest are the large stationary tools that are still active in their pavilions. Almost every instrument has a long interesting history. Museification of astronomical instruments gives them a second life, expanding educational programs and tracing the development of astronomy in general and scientific institution and region in particular. It would be advisable to first create a regional database of these rare astronomical instruments (which is already being done in Ukraine), then a common global database. By combining all the historical information about astronomical instruments with the advantages of the Internet, you can show the full evolution of an astronomical instrument with all its features. Time is relentless, and much is destroyed, badly kept and thrown in the garbage. We need time to protect, capture, and tell about it.

The Astronomical League

NASA Astrophysics Data System (ADS)

Stevens, J. A.; Stevens, B. L.

2000-10-01

Founded over fifty years ago, the League is the largest general astronomy society in the world. It is a recognized non-profit, educational organization, promoting the science of astronomy. This includes astronomical education, research, individual observing of the heavens and coordination between the amateur and professional astronomy communities. The Astronomical League publishes a quarterly newsletter, the "Reflector", which details amateur activities and amateur collaboration with professional astronomers. The League's Observing Clubs hone the skills of the amateur astronomer in using their telescopes. These clubs provide awards to encourge observing and learning the sky. More general awards are presented to encourage amateur astronomy and the science of astronomy. These include the National Young Astronomer Award, amd the Horkheimer Planetary Imaging Award. They also sponsor conventions on both the National and Regional levels. This year's national is in Ventura, California, next year, near Washington, D.C.

Preserving Astronomy's Photographic Legacy: Current State and the Future of North American Astronomical Plates

NASA Astrophysics Data System (ADS)

Osborn, W.; Robbins, L.

2009-08-01

This book contains articles on preserving astronomy's valuable heritage of photographic observations, most of which are on glass plates. It is intended to serve as a reference for institutions charged with preserving and managing plate archives and astronomers interested in using archival photographic plates in their research. The first portion of the book focuses on previous activities and recommendations related to plate archiving. These include actions taken by the International Astronomical Union, activities in Europe and a detailed account of a workshop on preserving astronomical photographic data held in 2007 at the Pisgah Astronomical Research Institute, North Carolina. The workshop discussions covered a wide range of issues that must be considered in any effort to archive plates and culminated in a set of recommendations on preserving, cataloging and making publicly available these irreplaceable data. The second part of the book reports on some recent efforts to implement the recommendations. These include essays on the recently established Astronomical Photographic Data Archive, projects to make photographic collections available electronically, evaluations of commercial scanners for digitization of astronomical plates and the case for the continuing value of these data along with a report on the census of astronomical plate collections in North America carried out in 2008. The census cataloged the locations, numbers, and types of astronomical plates in the US and Canada. Comprehensive appendices identify all the significant collections in North America and detail the current contents, state and status of their holdings.

Astronomical Prospecting of Asteroid Resources

NASA Astrophysics Data System (ADS)

Elvis, M.

2017-09-01

To make asteroid mining profitable will require professional astronomers using some of the largest telescopes on Earth to make precision measurements. This "astronomical prospecting" information is cheaper to obtain than flying even one or two spacecraft and will drastically cut the number of space probes that have to be sent to find an ore-bearing rock in space. Astronomical prospecting could make the business case for asteroid mining a solid one.

UkrVO astronomical WEB services

NASA Astrophysics Data System (ADS)

Mazhaev, A.

2017-02-01

Ukraine Virtual Observatory (UkrVO) has been a member of the International Virtual Observatory Alliance (IVOA) since 2011. The virtual observatory (VO) is not a magic solution to all problems of data storing and processing, but it provides certain standards for building infrastructure of astronomical data center. The astronomical databases help data mining and offer to users an easy access to observation metadata, images within celestial sphere and results of image processing. The astronomical web services (AWS) of UkrVO give to users handy tools for data selection from large astronomical catalogues for a relatively small region of interest in the sky. Examples of the AWS usage are showed.

E-books in Astronomy — If You Buy It Will They Come?

NASA Astrophysics Data System (ADS)

White, M.

2010-10-01

Do astronomers want, need, or use online electronic books? At our large institution astronomers have access to a number of e-books, including monographs provided by various e-book vendors. After a marketing and promotion effort astronomers were surveyed on their use and awareness of the available resources, asking about their likes, dislikes and desirable features. Astronomers were queried about digital rights management (DRM) restrictions; did the ease and immediacy of remote electronic access to the content override the problems presented by DRM? Astronomers showed mixed responses to the e-book format. We need to seek continued user feedback as the Libraries' investment in online books grows.

The Practical Astronomer

NASA Astrophysics Data System (ADS)

Koester, Jack

"The Practical Astronomer" by Thomas Dick, LLD, E.C. & J. Biddle, Philadelphia, 1849, is reviewed. Information on telescope makers and astronomers can be found. Mentioned are: Fraunhofer; John Herschel; Lawson; Dollond; Tulley; W. & S. Jones; and S.W. Burnham.

Building a VO-compliant Radio Astronomical DAta Model for Single-dish radio telescopes (RADAMS)

NASA Astrophysics Data System (ADS)

Santander-Vela, Juan de Dios; García, Emilio; Leon, Stephane; Espigares, Victor; Ruiz, José Enrique; Verdes-Montenegro, Lourdes; Solano, Enrique

2012-11-01

The Virtual Observatory (VO) is becoming the de-facto standard for astronomical data publication. However, the number of radio astronomical archives is still low in general, and even lower is the number of radio astronomical data available through the VO. In order to facilitate the building of new radio astronomical archives, easing at the same time their interoperability with VO framework, we have developed a VO-compliant data model which provides interoperable data semantics for radio data. That model, which we call the Radio Astronomical DAta Model for Single-dish (RADAMS) has been built using standards of (and recommendations from) the International Virtual Observatory Alliance (IVOA). This article describes the RADAMS and its components, including archived entities and their relationships to VO metadata. We show that by using IVOA principles and concepts, the effort needed for both the development of the archives and their VO compatibility has been lowered, and the joint development of two radio astronomical archives have been possible. We plan to adapt RADAMS to be able to deal with interferometry data in the future.

New Searching Capability and OpenURL Linking in the ADS

NASA Astrophysics Data System (ADS)

Eichhorn, Guenther; Accomazzi, A.; Grant, C. S.; Henneken, E.; Kurtz, M. J.; Thompson, D. M.; Murray, S. S.

2006-12-01

The ADS is the search system of choice for the astronomical community. It also covers a large part of the physics and physics/astronomy education literature. In order to make access to this system as easy as possible, we developed a Google-like interface version of our search form. This one-field search parses the user input and automatically detects author names and year ranges. Firefox users can set up their browser to have this search field installed in the top right corner search field to have even easier access to the ADS search capability. The basic search is available from the ADS Homepage at: http://adsabs.harvard.edu To aid with access to subscription journals the ADS now supports OpenURL linking. If your library supports an OpenURL server, you can specify this server in the ADS preference settings. All links to journal articles will then automatically be directed to the OpenURL with the appropriate link information. We provide a selection of known OpenURL servers to choose from. If your server is not in this list, please send the necessary information to ads@cfa.harvard.edu and we will include it in our list. The ADS is funded by NASA grant NNG06GG68G.

Double Star Research: A Student-Centered Community of Practice

NASA Astrophysics Data System (ADS)

Johnson, Jolyon

2016-06-01

Project and team-based pedagogies are increasingly augmenting lecture-style science classrooms. Occasionally, university professors will invite students to tangentially partcipate in their research. Since 2006, Dr. Russ Genet has led an astronomy research seminar for community college and high school students that allows participants to work closely with a melange of professional and advanced amatuer researchers. The vast majority of topics have centered on measuring the position angles and searations of double stars which can be readily published in the Journal of Double Star Observations. In the intervening years, a collaborative community of practice (Wenger, 1998) formed with the students as lead researchers on their projects with the guidance of experienced astronomers and educators. The students who join the research seminar are often well prepared for further STEM education in college and career. Today, the research seminar involves multile schools in multiple states with a volunteer educator acting as an assistant instructor at each location. These assistant instructors interface with remote observatories, ensure progress is made, and recruit students. The key deliverables from each student team include a published research paper and a public presentation online or in-person. Citing a published paper on scholarship and college applications gives students' educational carreers a boost. Recently the Journal of Double Star Observations published its first special issue of exlusively student-centered research.

Powerful Radio Burst Indicates New Astronomical Phenomenon

NASA Astrophysics Data System (ADS)

2007-09-01

Astronomers studying archival data from an Australian radio telescope have discovered a powerful, short-lived burst of radio waves that they say indicates an entirely new type of astronomical phenomenon. Region of Strong Radio Burst Visible-light (negative greyscale) and radio (contours) image of Small Magellanic Cloud and area where burst originated. CREDIT: Lorimer et al., NRAO/AUI/NSF Click on image for high-resolution file ( 114 KB) "This burst appears to have originated from the distant Universe and may have been produced by an exotic event such as the collision of two neutron stars or the death throes of an evaporating black hole," said Duncan Lorimer, Assistant Professor of Physics at West Virginia University (WVU) and the National Radio Astronomy Observatory (NRAO). The research team led by Lorimer consists of Matthew Bailes of Swinburne University in Australia, Maura McLaughlin of WVU and NRAO, David Narkevic of WVU, and Fronefield Crawford of Franklin and Marshall College in Lancaster, Pennsylvania. The astronomers announced their findings in the September 27 issue of the online journal Science Express. The startling discovery came as WVU undergraduate student David Narkevic re-analyzed data from observations of the Small Magellanic Cloud made by the 210-foot Parkes radio telescope in Australia. The data came from a survey of the Magellanic Clouds that included 480 hours of observations. "This survey had sought to discover new pulsars, and the data already had been searched for the type of pulsating signals they produce," Lorimer said. "We re-examined the data, looking for bursts that, unlike the usual ones from pulsars, are not periodic," he added. The survey had covered the Magellanic Clouds, a pair of small galaxies in orbit around our own Milky Way Galaxy. Some 200,000 light-years from Earth, the Magellanic Clouds are prominent features in the Southern sky. Ironically, the new discovery is not part of these galaxies, but rather is much more distant. "It was a bit of luck that the survey included some observations of the sky surrounding the clouds," Narkevic said. It was from those "flanking" observations that the mysterious radio burst appeared in the data. The burst of radio waves was strong by astronomical standards, but lasted less than five milliseconds. The signal was spread out, with higher frequencies arriving at the telescope before the lower frequencies. This effect, called dispersion, is caused by the signal passing through ionized gas in interstellar and intergalactic space. The amount of this dispersion, the astronomers said, indicates that the signal likely originated about three billion light-years from Earth. No previously-detected cosmic radio burst has the same set of characteristics. "This burst represents an entirely new astronomical phenomenon," Bailes said. The astronomers estimate on the basis of their results that hundreds of similar events should occur over the sky each day. "Few radio surveys have the necessary sensitivity to such short-duration bursts, which makes them notoriously difficult to detect with current instruments," added Crawford. The next generation of radio telescopes currently under development should be able to detect many of these bursts across the sky. Although the nature of the mysterious new object is unclear, the astronomers have some ideas of what may cause such a burst. One idea is that it may be part of the energy released when a pair of superdense neutron stars collide and merge. Such an event is thought by some scientists to be the cause of one type of gamma-ray burst, but the only radio emission seen so far from these has been from the long-lived "afterglow" that follows the original burst. Another, more exotic, candidate is a burst of energy from an evaporating black hole. Black holes, concentrations of mass so dense that not even light can escape their powerful gravity, can lose mass and energy through a process proposed by famed British physicist Stephen Hawking. The newly-discovered radio burst, the researchers said, might be the "last gasp" of a black hole as it finally evaporates completely. "We're actively looking for more of these powerful, short bursts, in other archival pulsar surveys, and hope to resolve the mystery of their origin," said McLaughlin. "In addition, if we can associate these events with galaxies of known distance, the radio dispersion we measure can be used as a powerful new way to determine the amount of material in intergalactic space," she added. The Parkes radio telescope is part of the Australia Telescope, which is funded by the Commonwealth of Australia for operation as a National Facility. The National Radio Astronomy Observatory is a facility of the National Science Foundation, operated under cooperative agreement by Associated Universities, Inc.

Thomas Kuhn's Influence on Astronomers.

ERIC Educational Resources Information Center

Shipman, Harry L.

2000-01-01

Surveys the astronomical community on their familiarity with the work of Thomas Kuhn. Finds that for some astronomers, Kuhn's thought resonated well with their picture of how science is done and provided perspectives on their scientific careers. (Author/CCM)

Cross-Matching of Very Large Catalogs

NASA Astrophysics Data System (ADS)

Martynov, M. V.; Bodryagin, D. V.

Modern astronomical catalogs and sky surveys, that contain billions of objects, belong to the "big data" data class. Existing available services have limited functionality and do not include all required and available catalogs. The software package ACrId (Astronomical Cross Identification) for cross-matching large astronomical catalogs, which uses an sphere pixelation algorithm HEALPix, ReiserFS file system and JSON-type text files for storage, has been developed at the Research Institution "Mykolaiv Astronomical Observatory".

Astronomical Symbolism in Bronze-Age and Iron-Age Rock Art

NASA Astrophysics Data System (ADS)

García Quintela, Marco V.; Santos-Estévez, Manuel

The best-known rock art from Late Prehistory is found in Scandinavia, the Alps, and Galicia, North West Spain. In this chapter, we explore its association with astronomical symbolism from three perspectives: the representation of heavenly bodies, the visibility conditions of the carvings, and their position on astronomical alignments. We also consider temporal variables and the impact of aspects of Indo-European ideology on the construction of the representations in their astronomical relationships.

Developing an astronomical observatory in Paraguay

NASA Astrophysics Data System (ADS)

Troche-Boggino, Alexis E.

Background: Paraguay has some heritage from the astronomy of the Guarani Indians. Buenaventura Suarez S.J. was a pioneer astronomer in the country in the XVIII century. He built various astronomical instruments and imported others from England. He observed eclipses of Jupiter's satellites and of the Sun and Moon. He published his data in a book and through letters. The Japanese O.D.A. has collaborated in obtaining equipment and advised their government to assist Paraguay in building an astronomical observatory, constructing a moving-roof observatory and training astronomers as observatory operators. Future: An astronomical center is on the horizon and some possible fields of research are being considered. Goal: To improve education at all possible levels by not only observing sky wonders, but also showing how instruments work and teaching about data and image processing, saving data and building a data base. Students must learn how a modern scientist works.

The Role of Amateur Astronomy to Outreach Astronomical Knowledge

NASA Astrophysics Data System (ADS)

Khachatryan, Vachik; Voskanyan, Tsovak

2016-12-01

It is known that in the educational system of republic the astronomy is not taught as a separate subject. Moreover, there are no telescopes in the vast majority of schools. "Goodricke John" NGO of amateur astronomers tries to fill this gap by organizing practical lessons of astronomy in secondary schools. NGO is equipped with high quality portable amateur telescopes and organizes periodic mass observations of planets, Moon, star clusters, nebulae in Yerevan and in regions. In addition, mass observations of rare astronomical phenomena are organized, such as the transit of Venus and Mercury across the disk of the Sun. Being the only NGO of amateur astronomers, it has a goal to contribute to publicizing astronomical knowledge and to ensure the availability of astronomical equipment, telescopes also to those segments of the society who have no opportunity to deal with them, in particular, persons with disabilities, prisoners, persons with disabilities, prisoners, soldiers, children from orphanages, school children and others.

Astronomical Orientation in the Ancient Dacian Sanctuaries of Romania

NASA Astrophysics Data System (ADS)

Stănescu, Florin

Sarmizegetusa Regia, the former capital city of the Dacians' kingdom, is situated in the Şureanu (Orăştie) Mountains in the Southern Carpathians, Romania. This chapter reviews, from the astronomical point of view, two of the monuments located on its Sacred Terrace - the altar known as the "Andesite Sun" and the Central Apse of the Great Round Sanctuary - as well as sanctuaries at the nearby site of Costeşti. Astronomical analyses taking into consideration (a) the astronomical-geometrical methods of the time (the analemma of a sundial after Vitruvius and the stereographical projection in the sense of Hipparchus), (b) astronomical instruments of the time (the gnomon, the sundial and the astrolabe), and (c) other instruments known to the Dacians (the compass), have concluded that these monuments may have enabled the Dacians to carry out a number of astronomical observations. This would confirm several reports by contemporary historians regarding the Dacians' knowledge of astronomy.

Preservation and maintenance of the astronomical sites in Armenia

NASA Astrophysics Data System (ADS)

Mickaelian, A. M.

2008-01-01

Astronomy in Armenia was popular since ancient times. There are signs of astronomical observations coming from a few thousands years ago. Two ancient observatories, Karahunge and Metzamor are especially well known. Karahunge is the Armenian twin of the Stonehenge and is even older. However, there is no proper attention from the state authorities and efforts are needed for preservation of such historical-astronomical monuments. The Byurakan Astrophysical Observatory (BAO) is the modern famous Armenian observatory founded in 1946 by the outstanding scientist Victor Ambartsumian. It was one of the world astronomical centres in 1950-s to 1970-s, and at present is the largest observatory in the Middle East area. As the ancient astronomical sites, Byurakan also needs a proper attitude from the state authorities and corresponding international organizations to preserve its values and importance for the present and future astronomical activities in the region, including its rich observational archive, telescopes, and human resources. Despite all the difficulties, the Armenian astronomers keep high international level of research and display various activities organizing international meetings and schools, preparing new young generation for the future research. The Armenian Astronomical Society (ArAS) is an affiliated member of EAS. Armenia has its Virtual Observatory project (ArVO) as well. The next Joint European and National Astronomy Meeting (JENAM-2007) will be held in Yerevan, Armenia, in August 2007. There are plans to organize astronomical tours to Armenia for making observations from various sites, including the ancient observatories. The future of astronomy in Armenia strongly depends on all of this activities and the proper attention both from state authorities and society.

Kosovo and U.S. Policy: Background to Independence

DTIC Science & Technology

2008-06-20

Assembly chose a President and a government in March 2002. LDK leader Ibrahim Rugova was elected as President and Bajram Rexhepi of the PDK became Prime... Agim Ceku, who was formerly head of the KLA and head of the Kosovo Protection Corps. The new government pledged to implement standards set by the...July 24, 2006, Kosovo President Fatmir Sejdiu and Prime Minister Agim Ceku met with their Serbian counterparts Boris Tadic and Vojislav Kostunica to

Kosovo and U.S. Policy

DTIC Science & Technology

2006-08-07

Agim Ceku met in Vienna with their Serbian counterparts Boris Tadic and Vojislav Kostunica to discuss the status issue, in the first direct, high-level...President. Kosovo’s Prime Minister is Bajram Rexhepi of the PDK. The government consisted of members of the LDK, PDK and AAK. One cabinet post was...replaced by Agim Ceku, who was formerly head of the KLA and head of the Kosovo Protection Corps. The new government pledged to implement standards set by

Kosovo and U.S. Policy: Background and Current Issues

DTIC Science & Technology

2007-10-24

is Bajram Rexhepi of the PDK. The government consisted of members of the LDK, PDK and AAK. One cabinet post was reserved for a Kosovo Serb...2006, Kosovo Prime Minister Bajram Kosumi stepped down after criticism of his performance, even within his own party. He was replaced by Agim Ceku...Fatmir Sejdiu and Prime Minister Agim Ceku met with their Serbian counterparts Boris Tadic and Vojislav Kostunica to discuss the status issue, in the

Deciphering the balkan Enigma: Using History to Inform Policy

DTIC Science & Technology

1993-03-01

University Press, 1973. After long experience with German interference in Serbian/Yugoslav affairs (1878, 1908, 1914 - 1918 ) it should not be surprising that... 1914 - 1918 , ed. Djordjevicý, Santa Barbara: CLID Books, 1980. 151. James Gow, "Deconstructing Yugoslavia," Survival, Vol. 33, Nc. 4, July-August 1992, p...of political institutions witnin tine Balkans anu io0w these political dev, ’ýpments intluence current events. Historical perspective gained is used

Kosovo’s Crisis: Genesis of a Problem

DTIC Science & Technology

2013-03-01

research reveal that only three of the original 89 settlements are mentioned as being Albanian. Out of the 2,166 farming homesteads and 2,666 houses in...resistance movement in Kosovo did not succeed, because the Albanians saw the CPY as pro -Slav, especially since the CPY promised only equality among all...partisan units became stronger and larger. At the same time, the Ballists collaborated with the pro -kingdom and anti- communist Serbian Chetnick

New astronomical references in two Catalonian late medieval documents.

PubMed

Martínez, María José; Marco, Francisco J

2014-01-01

In 2008, after 13 years of preparation, the Generalitat of Catalunya finished the publication of the 10 volumes of the Dietaris de la Generalitat de Catalunya. The Dietaris, as well as a closely related source, the llibre de Jornades 1411/1484 de Jaume Safont, cover the period of 1411 to 1539. In this article, we examine astronomical references contained in these two sources, and place them in their historical context. Our main focus lies on astronomical phenomena that have not previously been published in the astronomical literature. In fact, relatively few astronomical records are accessible in Spanish medieval and early modern history, and our paper intends to fill this gap partially.

The role of Revista Mexicana de Astronomía y Astrofísica Serie de Conferencias in the world of astronomy

NASA Astrophysics Data System (ADS)

Torres-Peimbert, Silvia; Allen, Christine

2015-08-01

Forty years ago Revista Mexicana de Astronomía y Astrofísica decided to include the proceedings of astronomical meetings in Mexico and Latin America. In 1995 it became necessary to found the Serie de Conferencias to better differentiate proceedings from refereed papers.So far there have been 58 astronomical meetings published and there are several more in store for the coming years

Achievements of the Armenian Astronomy and the Present Activities of the Armenian Astronomical Society

NASA Astrophysics Data System (ADS)

Mickaelian, A. M.

2014-10-01

A report is given on the achievements of the Armenian astronomy during the last years and on the present activities of the Armenian Astronomical Society (ArAS). ArAS membership, ArAS electronic newsletters (ArASNews), ArAS webpage, international collaboration, Armenian Virtual Observatory (ArVO), membership in international organizations, grants, prizes, meetings, summer schools, astronomical Olympiads, other matters related to astronomical education, archaeoastronomy, astronomy outreach and ArAS further projects are discussed.

Computer version of astronomical ephemerides.

NASA Astrophysics Data System (ADS)

Choliy, V. Ya.

A computer version of astronomical ephemerides for bodies of the Solar System, stars, and astronomical phenomena was created at the Main Astronomical Observatory of the National Academy of Sciences of Ukraine and the Astronomy and Cosmic Physics Department of the Taras Shevchenko National University. The ephemerides will be distributed via INTERNET or in the file form. This information is accessible via the web servers space.ups.kiev.ua and alfven.ups.kiev.ua or the address choliy@astrophys.ups.kiev.ua.

Johann Leonhard Rost, "novelist" and astronomer; (German Title: Johann Leonhard Rost, "Romanist" und Astronom)

NASA Astrophysics Data System (ADS)

Gaab, Hans; Simons, Olaf

Johann Leonhard Rost (1688-1727) of Nuremberg studied at Altdorf, Leipzig and Jena. During this time, he earned his living by writing gallant novels. In 1715, he returned to Nuremberg, where he pursued his juvenile inclination towards astronomy and became a serious astronomical observer. His introductions to astronomy, written around this time, contributed a lot to popularize astronomy. This contribution attempts to do justice to both the novelist and the astronomer Rost.

Positive Outcomes of a Teacher Professional Development Program Promoting Science Research in the Classroom

NASA Astrophysics Data System (ADS)

Miller, A.

2003-12-01

This presentation will focus on the experiences of a middle school science teacher from Brownsville, TX who attended the NSF-funded Research Based Science Education program during the summer of 2000. RBSE, sponsored by the National Optical Astronomy Observatories based in Tucson, AZ, provided attending teachers the opportunity to interact with and receive instruction from professional astronomers, both at the NOAO facility in Tucson, and at the Kitt Peak Observatory. Teachers were provided with raw astronomical data collected by astronomers and then trained in the use of image processing software for data analysis. Upon returning to the classroom in Brownsville, a research-based after school program was initiated by the teacher for four interested students. The students were given background on the research projects, taught to use the software, and then developed their own research questions in each of the three areas of RBSE: a search for novae in the Andromeda galaxy; an analysis of the number and area of sunspots; and an investigation into spectra of Active Galactic Nuclei. Students came to the classroom after school daily during a large part of the year and generally would work for one to two hours processing and analyzing data. Completed research projects were presented in a variety of formats including: competition at the Brownsville School District, Rio Grande Valley Regional, and Texas State science fairs; publication of professional-style research articles in the RBSE journal; and poster presentations at Research Day at the University of Texas-Brownsville. The students have won numerous awards at all levels of Science Fair competition, have been the subject of three local newspaper articles, and two of them have accelerated their academics to the point of graduating from high school in only two years and have received full college scholarship offers. The students today credit their RBSE experience with increasing their interest level in science, helping them to understand the scientific method and research, and developing the self-confidence that has enabled them to pursue greater academic and personal goals.

Science versus News: On the Cutting Edge

NASA Astrophysics Data System (ADS)

Kinney, A. L.; French, V.; Villard, R.; Maran, S. P.

1998-12-01

This session is to aid communication between scientists and journalists, to motivate astronomers to be active in communicating their science to the public via the press, and to help both astronomers and journalists to understand the constraints under which the other group is operating. The session consists of two talks of about 20 minutes, followed by a panel discussion. The first talk is "What Makes a Topic News?" This segment, by Miles O'Brien of CNN News, takes the AAS audiences behind the scenes in the world of producing science news stories. --- What drives selection of assignments? How does the science reporter convince their editor to cover a story? What factors about television producing help and also hurt getting science subjects across to the public? The second talk is "Public Knowledge on Science: The Growing Gap Between Scientists and the Taxpayer." This presentation by Jon Miller, a public opinion expert will emphasize the problems scientists and society, face in communicating to the public. --- What does the public know about science and scientific method? How much translation is required to communicate with the public to engage their interest without unacceptable compromise of scientific accuracy? The final segment is a panel of both science journalists and astronomers moderated by Steve Maran. Together they will tackle a question that gets to the heart of the Science-Vs-News controversies, "When Should Results Go Public?" Published too soon, science is called "hype"; Published too late, it is no longer "news." Should all results be peer reviewed first, and is that a satisfactory prerequisite? Do scientists take self-serving advantage of the public interest by making announcements before results appear in journals? How do we address the public desire to experience science unfolding and to see real-time data such as planetary science missions? The panelists are Dr. David Helfand, from Columbia University, Dr. Bruce Margon, from the University of Washington, Mr. Thomas Siegfried, from The Dallas Daily News, Ms. Kathy Sawyer, from The Washington Post, Mr. John Noble Wilford from The New York Times, and Ms. Ann Kellan from CNN.

NASA Space Telescopes See Weather Patterns in Brown Dwarf

NASA Image and Video Library

2017-12-08

JANUARY 8, 2013: Astronomers using NASA's Hubble and Spitzer space telescopes have probed the stormy atmosphere of a brown dwarf named 2MASSJ22282889-431026, creating the most detailed "weather map" yet for this class of cool, star-like orbs. The forecast shows wind-driven, planet-sized clouds enshrouding these strange worlds. Brown dwarfs form out of condensing gas, as stars do, but lack the mass to fuse atoms and produce energy. Instead, these objects, which some call failed stars, are more similar to gas planets with their complex, varied atmospheres. The new research is a stepping stone toward a better understanding not only brown dwarfs, but also of the atmospheres of planets beyond our solar system. Hubble and Spitzer simultaneously watched the brown dwarf as its light varied in time, brightening and dimming about every 90 minutes as the body rotated. Astronomers found the timing of this change in brightness depended on whether they looked using different wavelengths of infrared light. The variations are the result of different layers or patches of material swirling around in the brown dwarf in windy storms as large as Earth itself. Spitzer and Hubble see different atmospheric layers because certain infrared wavelengths are blocked by vapors of water and methane high up, while other infrared wavelengths emerge from much deeper layers. Daniel Apai, the principal investigator of the research from the University of Arizona, Tucson, presented the results at the American Astronomical Society meeting on January 8 in Long Beach, Calif. A study describing the results, led by Esther Buenzli, also of the University of Arizona, is published in the Astrophysical Journal Letters. For more information about this study, visit www.nasa.gov/spitzer . NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. Follow us on Twitter Like us on Facebook Find us on Instagram

Astronomy Education: The Good, the Bad, and the Ugly -- A Practical Guide for Those Who Teach and Those Who Don't

NASA Astrophysics Data System (ADS)

Fraknoi, A.

2005-05-01

Whether you teach undergraduate astronomy or just do occasional public outreach, you've probably seen personal examples reflecting the disturbing statistics. Roughly half of all freshmen entering the California State Colleges cannot do English or math at the college level and need remedial courses. Only 22% of adults in the U.S. can correctly explain what a molecule is. More people will watch each pseudoscience-filled episode of "Unsolved Mysteries" on television than will be taught an astronomy course by all the people at this AAS meeting combined. In this talk, we will briefly examine the challenges for everyone interested in astronomy education in three arenas: (dwindling) astronomy instruction in grades K-12, the teaching of Astro 101 for non-science majors, and the work of astronomers contributing to the public understanding of science. (For example, with the modern growth of astronomical knowledge, trying to teach ALL of astronomy in one quarter or semester is like trying to buy one of each item at your local Wal-Mart -- your cart will be impressively full, but your ability to get to know and enjoy each purchase will be severely limited.) We'll also look at some surprising result from a survey of the training and work of 400 astronomy instructors at non-research-oriented colleges. We'll then focus on some practical ideas on how all astronomers can contribute to improving the public appreciation of astronomy -- in their classes, in their institution's outreach work, and in the community. Several projects around the country that have found research-based techniques for making a significant difference will be highlighted, from family astronomy community events to experiments with hands-on small-group activities in the midst of large lecture classes. We'll discuss the role of a new electronic journal and web-based communities in facilitating the exchange of information on what works and what doesn't. Participants will receive an annotated resource guide to key readings, research findings, and ongoing projects in astronomy education.

Some new astronomical facilities in China

NASA Astrophysics Data System (ADS)

Wang, Shouguan

1989-10-01

For the 1990's, plans for some astronomical facilities and related research are being carried out in China. This report describes in some detail plans for radio astronomical facilities, a 150/220 cm Schmidt telescope, and experiments on a porcelain mirror material.

Evolution of Scholarly Publishing and Library Services in Astronomy - Impact, Challenges, and Opportunities

NASA Astrophysics Data System (ADS)

Wesley, Hema; Sheshadri, Geetha

2015-08-01

Science publishing and its procedures have evolved rapidly and incredibly. Technical advances in the production and promotion of science content have dramatically widened the visibility and reach, deepened the impact and intensified the thrust of our journals’ science content. Nevertheless, it is also true that with speed and ease of automation, quality is to be ferociously guarded. Could traditional methods when juxtaposed with the continuous onslaught of newer technologies, in our publishing procedures, be the answer. Are people still the quintessential element in technology?Why do we publish; the phrase “Publish or Perish” has itself, interestingly, evolved in its meaning. How have publishing procedures evolved through the years; what is the impact of these developments; what are the challenges and opportunities for scholarly publishers in this digital age. How do we cope with and preempt the abuse and distortion of internet data, and with unethical practices that threaten to cripple the peer review system, and jeopardize publishing ethics and academic integrity. How can publishers fulfill their responsibility to publish content that is explicitly original.With increasing demand from the astronomical community for e-journals and other e-resources and with the gradual loss of value for printed journals, librarians are developing and maintaining e-libraries and providing access to digital resources, and re-engineering their roles to provide advancing tools for e-pub content.How can we prepare for the future of publishing, or is it already here with the popularity of pre-print servers. How have publishers responded to the Open Access model while being aware that ‘the price of keeping something free comes with a cost’. Will potential authors be confused with identifying traditional peer reviewed content, the predatory journals, the fake reviewers, placing research in institutional repositories, copyright and licenses. Are libraries impacted by these developments in their journal pricing schemes.

Filling the Astronomical Void - A Visual Medium for a Visual Subject

NASA Astrophysics Data System (ADS)

Ryan, J.

1996-12-01

Astronomy is fundamentally a visual subject. The modern science of astronomy has at its foundation the ancient art of observing the sky visually. The visual elements of astronomy are arguably the most important. Every person in the entire world is affected by visually-observed astronomical phenomena such as the seasonal variations in daylight. However, misconceptions abound and the average person cannot recognize the simple signs in the sky that point to the direction, the hour and the season. Educators and astronomy popularizers widely lament that astronomy is not appreciated in our society. Yet, there is a remarkable dearth of popular literature for teaching the visual elements of astronomy. This is what I refer to as *the astronomical void.* Typical works use illustrations sparsely, relying most heavily on text-based descriptions of the visual astronomical phenomena. Such works leave significant inferential gaps to the inexperienced reader, who is unequipped for making astronomical observations. Thus, the astronomical void remains unfilled by much of the currently available literature. I therefore propose the introduction of a visually-oriented medium for teaching the visual elements of Astronomy. To this end, I have prepared a series of astronomy "comic strips" that are intended to fill the astronomical void. By giving the illustrations the central place, the comic strip medium permits the depiction of motion and other sequential activity, thus effectively representing astronomical phenomena. In addition to the practical advantages, the comic strip is a "user friendly" medium that is inviting and entertaining to a reader. At the present time, I am distributing a monthly comic strip entitled *Starman*, which appears in the newsletters of over 120 local astronomy organizations and on the web at http://www.cyberdrive.net/ starman. I hope to eventually publish a series of full-length books and believe that astronomical comic strips will help expand the perimeter of astronomical awareness.

Reporting Astronomical Discoveries: Past, Now, and Future

NASA Astrophysics Data System (ADS)

Yamaoka, Hitoshi; Green, Daniel W. E.; Samus, Nikolai N.; West, Richard

2015-08-01

Many new astronomical objects have been discovered over the years by amateur astronomers, and this continues to be the case. They have traditionally reported them (as have professional astronomers) to the Central Bureau for Astronomical Telegrams (CBAT), which was established in the 19th century. This procedure has worked very well throughout the 20th century, moving under the umbrella of the newly established IAU in 1920. The discoverers have been honored by the formal announcement of their discoveries in the publications of the CBAT.In recent years, some professional research groups have established other ways of announcing their discoveries of explosive objects such as novae and supernovae; some do not now report their discoveries or spectroscopic confirmations of the transients to the CBAT, including often spectroscopic reports of objects posted to the CBAT "Transient Objects Confirmation Page" -- the highly successful TOCP webpage, which assigns official positional designations to new transients posted there by approved, registered users. This leads to a delay in formal announcements of discoveries by amateur astronomers in many cases, as well as inconsistent designations being put into use by individual groups. Amateur astronomers are feeling frustrated about this situation, and they hope that the IAU will help to settle the situation.We have proposed the new IAU commission NC-52, which will treat these phenomena in a continuation of Commission 6, through the CBAT. We hope to continuously support the reporting of the discoveries by amateur astronomers, as well as professional astronomers, who all deserve and desire proper recognition. Our strategy will maintain the firm trust between the amateur and professional astronomers, which is necessary for true collaboration. The plan is for the CBAT to work with collaborators to assure that discoveries posted on the TOCP are promptly designated and announced by the CBAT, even when confirmations are made elsewhere. All discoverers are encouraged to send their discovery information for transients to the CBAT (particularly for those objects brighter than visual or red magnitude 20).

The Expansion of the Astronomical Photographic Data Archive at PARI

NASA Astrophysics Data System (ADS)

Cline, J. Donald; Barker, Thurburn; Castelaz, Michael

2017-01-01

A diverse set of photometric, astrometric, spectral and surface brightness data exist on decades of photographic glass plates. The Astronomical Photographic Data Archive (APDA) at the Pisgah Astronomical Research Institute (PARI) was established in November 2007 and is dedicated to the task of collecting, restoring, preserving and storing astronomical photographic data and PARI continues to accept collections. APDA is also tasked with scanning each image and establishing a database of images that can be accessed via the Internet by the global community of scientists, researchers and students. APDA is a new type of astronomical observatory - one that harnesses analog data of the night sky taken for more than a century and making that data available in a digital format.In 2016, APDA expanded from 50 collections with about 220,000 plates to more than 55 collections and more than 340,000 plates and films. These account for more than 30% of all astronomical photographic data in the United States. The largest of the new acquisitions are the astronomical photographic plates in the Yale University collection. We present details of the newly added collections and review of other collections in APDA.

International Schools for Young Astronomers Teaching for Astronomy Development: two programmes of the International Astronomical Union

NASA Astrophysics Data System (ADS)

Gerbaldi, Michèle; DeGreve, Jean-Pierre; Guinan, Edward

2011-06-01

This text outlines the main features of two educational programmes of the International Astronomical Union (IAU): the International Schools for Young Astronomers (ISYA) and the Teaching for Astronomy Development programme (TAD), developed since 1967. The main goal of the International Schools for Young Astronomers (ISYA) is to support astronomy (education and research) in developing countries in organizing a 3-week School for students with typically M.Sc. degrees. The context in which the ISYA were developed changed drastically during the last decade. From a time when access to large telescopes was difficult and mainly organized on a nation-basis, nowadays the archives of astronomical data have accumulated at the same time that many major telescope become accessible, and they are accessible from everywhere, the concept of virtual observatory reinforcing this access. A second programme of the IAU, Teaching for Astronomy Development (TAD), partially based on a School, but also of shorter duration (typically one week) has a complementary objective. It is dedicated to assist countries that have little or no astronomical activity, but that wish to enhance their astronomy education. The fast development of the TAD programme over the past years is emphasized.

Astronomical observatories

NASA Technical Reports Server (NTRS)

Ponomarev, D. N.

1983-01-01

The layout and equipment of astronomical observatories, the oldest scientific institutions of human society are discussed. The example of leading observatories of the USSR allows the reader to familiarize himself with both their modern counterparts, as well as the goals and problems on which astronomers are presently working.

Project of space research and technology center in Engelhardt astronomical observatory

NASA Astrophysics Data System (ADS)

Nefedyev, Y.; Gusev, A.; Sherstukov, O.; Kascheev, R.; Zagretdinov, R.

2012-09-01

Today on the basis of Engelhardt astronomical observatory (EAO) is created Space research and technology center as consistent with Program for expansion of the Kazan University. The Centre has the following missions: • EDUCATION • SCIENCE • ASTRONOMICAL TOURISM

Chicago's Dearborn Observatory: a study in survival

NASA Astrophysics Data System (ADS)

Bartky, Ian R.

2000-12-01

The Dearborn Observatory, located on the Old University of Chicago campus from 1863 until 1888, was America's most promising astronomical facility when it was founded. Established by the Chicago Astronomical Society and directed by one of the country's most gifted astronomers, it boasted the largest telescope in the world and virtually unlimited operating funds. The Great Chicago Fire of 1871 destroyed its funding and demolished its research programme. Only via the sale of time signals and the heroic efforts of two amateur astronomers did the Dearborn Observatory survive.

Franklin Edward Kameny (1925-2011, Astronomer)

NASA Astrophysics Data System (ADS)

Wright, Jason

2012-01-01

Dr. Frank Kameny is best known today as one of the most important members of the gay rights movement in the United States, but he was also a PhD astronomer. In fact, it was his firing from his civil service position as astronomer for the US Army Map Service on the grounds of homosexuality that sparked his lifelong career of activism. Here, I explore some aspects of his short but interesting astronomical career and the role of the AAS in his life.

Light Dawns on Dark Gamma-ray Bursts

NASA Astrophysics Data System (ADS)

2010-12-01

Gamma-ray bursts are among the most energetic events in the Universe, but some appear curiously faint in visible light. The biggest study to date of these so-called dark gamma-ray bursts, using the GROND instrument on the 2.2-metre MPG/ESO telescope at La Silla in Chile, has found that these gigantic explosions don't require exotic explanations. Their faintness is now fully explained by a combination of causes, the most important of which is the presence of dust between the Earth and the explosion. Gamma-ray bursts (GRBs), fleeting events that last from less than a second to several minutes, are detected by orbiting observatories that can pick up their high energy radiation. Thirteen years ago, however, astronomers discovered a longer-lasting stream of less energetic radiation coming from these violent outbursts, which can last for weeks or even years after the initial explosion. Astronomers call this the burst's afterglow. While all gamma-ray bursts [1] have afterglows that give off X-rays, only about half of them were found to give off visible light, with the rest remaining mysteriously dark. Some astronomers suspected that these dark afterglows could be examples of a whole new class of gamma-ray bursts, while others thought that they might all be at very great distances. Previous studies had suggested that obscuring dust between the burst and us might also explain why they were so dim. "Studying afterglows is vital to further our understanding of the objects that become gamma-ray bursts and what they tell us about star formation in the early Universe," says the study's lead author Jochen Greiner from the Max-Planck Institute for Extraterrestrial Physics in Garching bei München, Germany. NASA launched the Swift satellite at the end of 2004. From its orbit above the Earth's atmosphere it can detect gamma-ray bursts and immediately relay their positions to other observatories so that the afterglows could be studied. In the new study, astronomers combined Swift data with new observations made using GROND [2] - a dedicated gamma-ray burst follow-up observation instrument, which is attached to the 2.2-metre MPG/ESO telescope at La Silla in Chile. In doing so, astronomers have conclusively solved the puzzle of the missing optical afterglow. What makes GROND exciting for the study of afterglows is its very fast response time - it can observe a burst within minutes of an alert coming from Swift using a special system called the Rapid Response Mode - and its ability to observe simultaneously through seven filters covering both the visible and near-infrared parts of the spectrum. By combining GROND data taken through these seven filters with Swift observations, astronomers were able to accurately determine the amount of light emitted by the afterglow at widely differing wavelengths, all the way from high energy X-rays to the near-infrared. The astronomers used this information to directly measure the amount of obscuring dust that the light passed through en route to Earth. Previously, astronomers had to rely on rough estimates of the dust content [3]. The team used a range of data, including their own measurements from GROND, in addition to observations made by other large telescopes including the ESO Very Large Telescope, to estimate the distances to nearly all of the bursts in their sample. While they found that a significant proportion of bursts are dimmed to about 60-80 percent of the original intensity by obscuring dust, this effect is exaggerated for the very distant bursts, letting the observer see only 30-50 percent of the light [4]. The astronomers conclude that most dark gamma-ray bursts are therefore simply those that have had their small amount of visible light completely stripped away before it reaches us. "Compared to many instruments on large telescopes, GROND is a low cost and relatively simple instrument, yet it has been able to conclusively resolve the mystery surrounding dark gamma-ray bursts," says Greiner. Notes [1] Gamma-ray bursts lasting longer than two seconds are referred to as long bursts and those with a shorter duration are known as short bursts. Long bursts, which were observed in this study, are associated with the supernova explosions of massive young stars in star-forming galaxies. Short bursts are not well understood, but are thought to originate from the merger of two compact objects such as neutron stars. [2] The Gamma-Ray burst Optical and Near-infrared Detector (GROND) was designed and built at the Max-Planck Institute for Extraterrestrial Physics in collaboration with the Tautenburg Observatory, and has been fully operational since August 2007. [3] Other studies relating to dark gamma-ray bursts have been released. Early this year, astronomers used the Subaru Telescope to observe a single gamma-ray burst, from which they hypothesised that dark gamma-ray bursts may indeed be a separate sub-class that form through a different mechanism, such as the merger of binary stars. In another study published last year using the Keck Telescope, astronomers studied the host galaxies of 14 dark GRBs, and based on the derived low redshifts they infer dust as the likely mechanism to create the dark bursts. In the new work reported here, 39 GRBs were studied, including nearly 20 dark bursts, and it is the only study in which no prior assumptions have been made and the amount of dust has been directly measured. [4] Because the afterglow light of very distant bursts is redshifted due to the expansion of the Universe, the light that left the object was originally bluer than the light we detect when it gets to Earth. Since the reduction of light intensity by dust is greater for blue and ultraviolet light than for red, this means that the overall dimming effect of dust is greater for the more distant gamma-ray bursts. This is why GROND's ability to observe near-infrared radiation makes such a difference. More information This research is presented in a paper to appear in the journal Astronomy & Astrophysics on 16 December 2010 The team is composed of: J. Greiner (Max-Planck-Institut für extraterrestrische Physik [MPE], Germany), T. Krühler (MPE, Universe Cluster, Technische Universität München), S. Klose (Thüringer Landessternwarte, Germany), P. Afonso (MPE), C. Clemens (MPE), R. Filgas (MPE), D.H. Hartmann (Clemson University, USA), A. Küpcü Yoldaş¸ (University of Cambridge, UK), M. Nardini (MPE), F. Olivares E. (MPE), A. Rau (MPE), A. Rossi (Thüringer Landessternwarte, Germany), P. Schady (MPE), and A. Updike (Clemson University, USA) ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organisation in Europe and the world's most productive astronomical observatory. It is supported by 14 countries: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world's most advanced visible-light astronomical observatory and VISTA, the world's largest survey telescope. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 42-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become "the world's biggest eye on the sky".

Hosting an `Ask the Astronomer' Site on the Internet

NASA Astrophysics Data System (ADS)

Odenwald, S. F.

1996-12-01

Since 1995, the World Wide Web has explosively evolved into a significant medium for dispensing astronomical information to the general public. In addition to the numerous image archives that have proliferated, an increasing number of sites invite visitors to pose questions about astronomy and receive answers provided by professional astronomers. In this paper, I describe the operation of an Ask the Astronomer site that was opened on the WWW during August, 1995 as part of an astronomy education resource area called the "Astronomy Cafe" (URL=http://www2.ari.net/home/odenwald/cafe.html). The Astronomy Cafe includes a number of documents describing: a career in astronomy; how research papers are written; essays about cosmology, hyperspace and infrared astronomy; and the results from a 100-question, just for fun, personality test which distinguishes astronomers from non-astronomers. The Ask the Astronomer site is operated by a single astronomer through private donations and is now approaching its 500th day of operation. It contains over 2000+ questions and answers with a growth rate of 5 - 10 questions per day. It has attracted 70,000 visitors who are responsible for nearly 1 million 'hits' during the site's lifetime. The monthly statistics provide a unique survey of the kinds of individuals and organizations who visit Ask the Astronomer-type web sites, moreover, the accumulated questions provide a diagnostic X-ray into the public mind in the area of astronomy. I will present an analysis of the user demographics, and the types of questions that appear to be the most frequently asked. A paper copy of the complete index of these questions will be available for inspection.

Psychometric characteristics of the chronic Otitis media questionnaire 12 (COMQ - 12): stability of factor structure and replicability shown by the Serbian version.

PubMed

Bukurov, Bojana; Arsovic, Nenad; Grujicic, Sandra Sipetic; Haggard, Mark; Spencer, Helen; Marinkovic, Jelena Eric

2017-10-23

Recently, demand for and supply of short-form patient-reported outcome measures (PROMs) have risen throughout the world healthcare. Our contribution to meeting that demand has been translating and culturally adapting the Chronic Otitis Media Questionnaire-12 (COMQ-12) for adults into Serbian and enhancing its psychometric base on the relatively large Serbian COM caseload. Chronic otitis media can seriously affect quality of life progressively and in long-term, and it remains the major source of hearing problems in the developing world. The translated questionnaire was given twice to 60 adult patients with chronic otitis media of three types (inactive, active mucosal and active squamous disease) and to 60 healthy volunteers. Both patients and volunteers also filled the generic Short-Form 36 questionnaire (SF-36). Conventional statistical procedures were used in strategically driven development of scoring. Additionally, item responses were scaled by linear mapping against the provisional total score. Generalizability, detailed factor interpretation and supportability of scores were criteria, for the best compromise factor solution. Test-retest reliability was very high (0.924 to 0.989, depending on score). The a priori content dimensions of the questionnaire were strongly supported by 3-factor exploratory and confirmatory factor analyses for content validity, separating (i) ear symptoms from (ii) hearing problems, from (iii) daily activity restriction plus healthcare uptake. The 3-factor structure was furthermore highly stable on replication. The very large effect sizes when contrasting patients with healthy volunteers, and active with inactive disease established construct validity for the total score. A strong association with disease activity and a moderate one with generic health-related quality of life (HRQoL), the SF-36, supported construct validity for two of three factors extracted (ear symptoms, and impact on daily activities plus healthcare uptake). Given the minimal psychometric work to date on COMQ-12, this interim sample with 120 data points adds materially to knowledge of its reliability, several forms of validity and the feasibility of profile sub-scores to supplement total scores. The good psychometric properties shown for COMQ-12 justify both its routine clinical use and acquisition of the necessarily larger sample for generality, score optimisation and the evaluation of responsiveness.

Astronomical Instrumentation System Markup Language

NASA Astrophysics Data System (ADS)

Goldbaum, Jesse M.

2016-05-01

The Astronomical Instrumentation System Markup Language (AISML) is an Extensible Markup Language (XML) based file format for maintaining and exchanging information about astronomical instrumentation. The factors behind the need for an AISML are first discussed followed by the reasons why XML was chosen as the format. Next it's shown how XML also provides the framework for a more precise definition of an astronomical instrument and how these instruments can be combined to form an Astronomical Instrumentation System (AIS). AISML files for several instruments as well as one for a sample AIS are provided. The files demonstrate how AISML can be utilized for various tasks from web page generation and programming interface to instrument maintenance and quality management. The advantages of widespread adoption of AISML are discussed.

Astronomical Software Directory Service

NASA Technical Reports Server (NTRS)

Hanisch, R. J.; Payne, H.; Hayes, J.

1998-01-01

This is the final report on the development of the Astronomical Software Directory Service (ASDS), a distributable, searchable, WWW-based database of software packages and their related documentation. ASDS provides integrated access to 56 astronomical software packages, with more than 16,000 URL's indexed for full-text searching.

Cook, Green, Maskelyne and the 1769 transit of Venus: the legacy of the Tahitian observations

NASA Astrophysics Data System (ADS)

Orchiston, Wayne

2017-04-01

The 1769 transit of Venus was seen by astronomers as an important opportunity to pin down a figure for the solar parallax (P), and thus establish the Astronomical Unit and the size of the Solar System. Britain therefore mounted a number of expeditions, the most important of which was led by Lieutenant James Cook in the Endeavour, with Tahiti as the intended observing location. In this paper we trace the planning that preceded this expedition; provide biographical accounts of the Endeavour's two astronomers and others who also carried out astronomical observations; describe the astronomical instruments taken on the voyage; document the various transit observations; and track the post-transit path of the Endeavour as it returned to England. We then discuss the values of P that derived from this expedition and others, and end the paper by examining a number of research issues relating to the astronomical aspects of Cook's voyage that have yet to be resolved.

Identification and Support of Outstanding Astronomy Students

NASA Astrophysics Data System (ADS)

Stoev, A. D.; Bozhurova, E. S.

2006-08-01

The aims, organizational plan and syllabus of a specialized Astronomy School with a subject of training students for participation in the International Astronomy Olympiad, are presented. Thematic frame includes basic educational activities during the preparation and self-preparation of the students and their participation in astronomical Olympiads. A model of identification and selection of outstanding students for astronomical Olympiads has been developed. Examples of didactic systems of problems for development of mathematical, physical and astronomical skills are shown. The programme ends with individual training for solving problems on astronomy and astrophysics. Possibilities, which the characteristic, non-standard astronomical problems give for stimulating the creative and original thinking, are specified. Basic psychological condition for development of the students' creative potential - transformation of the cognitive content in emotional one - is demonstrated. The programme of identification and support of outstanding students on astronomy is realized in collaboration with The Ministry of Education and Science, Public Astronomical Observatories and Planetaria, Institute of Astronomy - Bulgarian Academy of Sciences, and The Union of Astronomers in Bulgaria.