41 CFR 101-30.704-2 - Other agencies.

Code of Federal Regulations, 2013 CFR

2013-07-01

... Regulations System FEDERAL PROPERTY MANAGEMENT REGULATIONS SUPPLY AND PROCUREMENT 30-FEDERAL CATALOG SYSTEM 30.7-Item Reduction Program § 101-30.704-2 Other agencies. Civil agencies participating in the Federal... 41 Public Contracts and Property Management 2 2013-07-01 2012-07-01 true Other agencies. 101-30...

Competency and Connection: Undergraduate Students and Effective Email Messages

ERIC Educational Resources Information Center

Sims, Christy-Dale L.

2015-01-01

Employers are struggling to fill jobs with qualified candidates because they find that the majority of college graduates lack "soft skills" such as oral and written communication, interpersonal skills, and professionalism (Carr & Stefaniak, 2012; Fischer, 2013; Tugend, 2013). Students are often more confident in their skill set and…

The Impact of Micro-Teaching on the Teaching Practice Performance of Undergraduate Agricultural Education Students in College of Education, Azare

ERIC Educational Resources Information Center

Sa'ad, Tata Umar; Sabo, Shehu; Abdullahi, Aliyu Dahuwa

2015-01-01

Micro-teaching and teaching practices are two integral parts of teacher education programme. Therefore, this study investigated the impact of micro-teaching on the teaching practice of the undergraduate Agricultural Education Students admitted in 2012/2013 Academic session in College of Education, Azare, Bauchi State, Nigeria. The 400 level…

Introductory Disciplines of Astronomy in Undergraduation Geography in Brazilian Public Universities

NASA Astrophysics Data System (ADS)

Henrique Azevedo Sobreira, Paulo

2015-08-01

There are some previous works about introductory disciplines of Astronomy in higher education in various undergraduation at Brazilian universities, but this is a specific research for Geography courses in public universities. Some undergraduate courses in Geography in Brazil offer introductory disciplines of Astronomy, since the second half of the twentieth century. This work presents an updated survey on the topic, and it proposes an effort at the national level, for the benefit of the increase in introductory disciplines of Astronomy in undergraduation in Geography. The data collected from public universities were obtained from the consultation of the websites of state universities, federal and county in 2012, 2013 and 2015, for information on the Geography courses and, among them, those with disciplines of Astronomy. The results show that there are 94 undergraduation in Geography courses in public universities, 12 of them had introductory disciplines of Astronomy until 2012 and 2013. In 2015 three of these disciplines were canceled which reduced to 9 universities. There were 23 undergraduation in Geography courses in 10 bachelor degrees and 14 education degrees with Astronomy disciplines. At 2015 it decreased to 20 in 5 bachelors and 8 education degrees. There are two undergraduation Geography courses with two introductory disciplines of Astronomy, while the other 18 offer only one discipline. The inclusion of introductory disciplines of Astronomy depends on the actions of professors' groups who works in undergraduation Geography courses, and of the astronomers initiative to offering them. The ideal is that the astronomers who actuate like professors in universities, normally in Math, Physics, Technologies, Enginnering and Science courses, they would can help and offer introductory disciplines in Astronomy for undergraduation in Geography courses.

VizieR Online Data Catalog: Abundances of bright metal-poor stars (Schlaufman+, 2014)

NASA Astrophysics Data System (ADS)

Schlaufman, K. C.; Casey, A. R.

2016-11-01

As input to our sample selection, we use the APASS DR6 Catalog, the 2MASS All-Sky Point Source Catalog, and the AllWISE Source Catalog (Henden+ 2012JAVSO..40..430H; Skrutskie+ 2006AJ....131.1163S; Wright+ 2010AJ....140.1868W; Mainzer+ 2011ApJ...731...53M). We followed up our metal-poor star candidates with the Mayall 4m/Echelle, Gemini South/GMOS-S, and Magellan/MIKE telescopes and spectrographs. We observed 98 stars with the Mayall 4m/Echelle on 2013 June 25-27. We observed 90 stars with Gemini South/GMOS-S in service mode from 2014 March to July (R~3700). We observed 416 stars with Magellan/MIKE on 2014 June 21-23 and July 8-10 (R~41000 in the blue and R~35000 in the red). (3 data files).

VizieR Online Data Catalog: Algol-type binaries. VIII. DI Peg & AF Gem (Yang+, 2014)

NASA Astrophysics Data System (ADS)

Yang, Y.-G.; Yang, Y.; Li, S.-Z.

2014-10-01

In the 2012-2013 observing season, DI Peg and AF Gem were observed using the 60cm telescope and the 85cm telescope at Xinglong station (XLs) of National Astronomical Observatories of Chinese (NAOC). The standard Johnson-Cousins UBVRcIc photometric systems were mounted upon two small telescopes. On five consecutive nights from 2012 October 9 to 13, the multi-color photometry of DI Peg was made with the 60cm telescope. The other variable star, AF Gem, was observed using the 85cm telescope on 7 nights from 2013 January 1 to 7. (5 data files).

VizieR Online Data Catalog: New PMS K/M Stars in Upper Scorpius (Rizzuto+, 2015)

NASA Astrophysics Data System (ADS)

Rizzuto, A. C.; Ireland, M. J.; Kraus, A. L.

2015-05-01

We have selected candidate Upper Scorpius members using kinematic and photometric data from UCAC4 (Zacharias et al., 2013, Cat. I/322), 2MASS (Skrutskie et al., 2006, Cat. VII/233), USNO-B (Monet et al. , 2003, Cat. I/284) and APASS (Henden et al., 2012, J. Am. Assoc. Var. Star Obs., 40, 430) We obtained 18 nights of time using WiFeS, split over 2013 and 2014; however, the majority of the 2013 nights were unusable due to weather. (3 data files).

VizieR Online Data Catalog: Robo-AO observed cool subdwarf companions (Ziegler+, 2015)

NASA Astrophysics Data System (ADS)

Ziegler, C.; Law, N. M.; Baranec, C.; Riddle, R. L.; Fuchs, J. T.

2017-09-01

We selected targets from the 564 spectral type F- through M-subdwarf candidates studied by Marshall (2007, J/AJ/134/778). These targets were selected from the New Luyten Two-Tenths catalog (NLTT; Luyten, 1979nlcs.book.....L; Luyten & Hughes 1980, Proper-Motion Survey with the Forty-Eight Inch Schmidt Telescope LV First Supplement to the NLTT Catalogue (Minneapolis, MN: Univ. Minnesota Press)) of high proper motion stars (>0.18 arcsec/yr) using a reduced proper motion diagram (RPM). Of the 552 subdwarfs confirmed by Marshall, a randomly selected sample of 348 G-, K-, and M-subdwarfs were observed by Robo-AO when available between other high priority surveys. We obtained high-angular-resolution images of the 348 subdwarfs during 32 separate nights of observations between 2012 September 3 and 2013 August 21 (UT). The observations were performed using the Robo-AO laser adaptive optics system (Riddle et al. 2012SPIE.8447E..2OR; Baranec et al. 2013, J. Visualized Exp. 72 e50021; 2014ApJ...790L...8B) mounted on the Palomar 60 inch telescope. (1 data file).

NASA's Earth Science Enterprise: 1998 Education Catalog

NASA Technical Reports Server (NTRS)

1998-01-01

This catalog presents a reference guide to NASA Earth science education programs and products. The topics include: 1) Student Support (Elementary and Secondary, Undergraduate and Graduate, Postgraduate, and Postdoctorate); 2) Teacher/Faculty Preparation and Enhancement; 3) Systemic Change; 4) Curriculum Support; and 5) Resources.

VizieR Online Data Catalog: Robo-AO Kepler planetary candidate survey. II. (Baranec+, 2016)

NASA Astrophysics Data System (ADS)

Baranec, C.; Ziegler, C.; Law, N. M.; Morton, T.; Riddle, R.; Atkinson, D.; Schonhut, J.; Crepp, J.

2016-10-01

We selected targets that we had not previously observed from the KOI Catalog based on the Q1-Q12 Kepler data (Rowe et al. 2015, Cat. J/ApJS/217/16). These targets were added to the Robo-AO intelligent observing queue and observed during the summer of 2013. We obtained high angular resolution images of 956 Kepler planet candidate host stars with the Robo-AO robotic laser AOs system over the course of 19 nights between 2013 July 21 and 2013 October 25, detailed in Table5. We also include 13 images from 2012 (2012 July 16-September 13) that required additional confirmation of the KOI position in the Robo-AO field of view. All the observations were performed in a queue-scheduled mode in combination with other science programs using the Robo-AO autonomous laser AO system mounted on the robotic 1.5m telescope at Palomar Observatory (exposure time: 90s; observation wavelengths: 600-950nm; FWHM resolution: 0.12''-0.15''; field of view: 44''*44''; pixel scale: 43.1mas/pix; detector format: 10242 pixels; targets observed/hour: 20). We obtained images of 50 KOIs with the NIRC2 instrument behind the Keck II AO system that were previously observed with Robo-AO and had evidence of a companion. Observations were conducted on 2013 June 25, 2013 August 24 and 25, 2014 August 17, and 2015 July 25 in the K, Ks, or Kp filters, and in the narrow mode of NIRC2 (9.952mas/pixel). (4 data files).

VizieR Online Data Catalog: Unidentified gamma-ray sources. IV. X-ray (Paggi+, 2013)

NASA Astrophysics Data System (ADS)

Paggi, A.; Massaro, F.; D'Abrusco, R.; Smith, H. A.; Masetti, N.; Giroletti, M.; Tosti, G.; Funk, S.

2013-11-01

The initial sample considered in our analysis is constituted by the 299 unidentified gamma-ray sources (UGSs) in the 2FGL catalog that do not present any γ-ray analysis flag (Nolan et al. 2012, Cat. J/ApJS/199/31). After Fermi was launched, the Swift XRT Survey of Fermi Unassociated Sources was started in order to perform follow-up observations of the unidentified gamma-ray sources (UGSs) in an attempt to find their potential X-ray counterparts (PI: A. Falcone). We analyze all data collected between the beginning of the follow-up program until 2013 March 31. We note that 203 of the 205 UGSs that constitute our sample have been also observed in the optical and UV by UVOT. We then produced for each X-ray observation the corresponding merged UVOT event files, adopting standard procedures. (6 data files).

VizieR Online Data Catalog: Robo-AO Kepler Planetary Candidate Survey. III. (Ziegler+, 2017)

NASA Astrophysics Data System (ADS)

Ziegler, C.; Law, N. M.; Morton, T.; Baranec, C.; Riddle, R.; Atkinson, D.; Baker, A.; Roberts, S.; Ciardi, D. R.

2018-04-01

KOI targets were selected from the KOI catalog based on Q1-Q17 Kepler data (Borucki et al. 2010ApJ...713L.126B, 2011, J/ApJ/728/117, J/ApJ/736/19; Batalha et al. 2013, J/ApJS/204/24; Burke et al. 2014, J/ApJS/210/19; Rowe et al. 2014, J/ApJ/784/45; Thompson et al. 2015, J/ApJ/812/46). We selected targets not observed in Law et al. 2014ApJ...791...35L and Baranec et al. 2016, J/AJ/152/18, with the objective of completing the Robo-AO survey of all KOIs, including those with already detected companions. We obtained high-angular-resolution images of the 1629 KOIs during 55 separate nights of observations between 2012 July 16 and 2015 June 12 (UT), detailed in Table 9 in the Appendix. The observations were performed using the Robo-AO laser adaptive optics system (Riddle et al. 2012SPIE.8447E..2OR; Baranec et al. 2013JVE....7250021B, 2014ApJ...790L...8B) mounted on the Palomar 1.5 m telescope. (6 data files).

Current Mexican-American and Chicano Studies Undergraduate College Programs in the United States.

ERIC Educational Resources Information Center

Jaramillo, James A.

This study conducted a library literature search of college guides, directories, and catalogs to determine the number of undergraduate level Chicano/a Studies and Mexican-American Studies programs in the U.S. The analysis found that there were 76 undergraduate programs in these fields, including 20 at two-year colleges and 56 at four-year…

NASA Headquarters training catalog

NASA Technical Reports Server (NTRS)

1990-01-01

The NASA Headquarters training catalog is a comprehensive listing of all educational and employee development programs. This course catalog contains descriptions of course content, objectives, target audience, prerequisites, length of course, approximate number of times the course is offered per year, and cost of the course. Curriculum areas include graduate and undergraduate academic study; professional development program; and executive management, senior management, and supervisory development programs. Secretarial/clerical and general computer skills programs are also included.

Castianeira furva sp. nov. (Araneae, Corinnidae, Castianeirinae), a new polymorphic ground sac spider from the southern Western Ghats of India.

PubMed

Sankaran, Pradeep M; Malamel, Jobi J; Joseph, Mathew M; Sebastian, Pothalil A

2015-06-05

The ground-dwelling, ant-mimicking corinnid spider genus Castianeira, with Castianeira rubicunda as type species, was erected by Keyserling (1879). Members of the genus are closely related to the Afrotropical genus Cambalida Simon, 1910 (Haddad 2012a) and are distributed mainly in tropical and temperate regions of the world except for Australia and nearby islands (World Spider Catalog 2015). The genus was revised from the Nearctic Region and south-east Asia (Reiskind 1969 and Deeleman-Reinhold 2001, respectively) and currently includes 126 described species, making it as the largest genus within the family Corinnidae (World Spider Catalog 2015). Even though the genus is rich in species, the validity and placement of majority of the species are still doubtful and questionable. For example, according to Haddad (2012b), many of the Afrotropical species, as well as majority of the species described from India (Haddad, pers. comm.) are misplaced or synonyms of previously described ones (e.g. Haddad 2012a, 2013a). The genus thus will remain as a trash-can until all the species described so far can be revised.

VizieR Online Data Catalog: From optical to infrared photometry of SN 2013dy (Pan+, 2015)

NASA Astrophysics Data System (ADS)

Pan, Y.-C.; Foley, R. J.; Kromer, M.; Fox, O. D.; Zheng, W.; Challis, P.; Clubb, K. I.; Filippenko, A. V.; Folatelli, G.; Graham, M. L.; Hillebrandt, W.; Kirshner, R. P.; Lee, W. H.; Pakmor, R.; Patat, F.; Phillips, M. M.; Pignata, G.; Ropke, F.; Seitenzahl, I.; Silverman, J. M.; Simon, J. D.; Sternberg, A.; Stritzinger, M. D.; Taubenberger, S.; Vinko, J.; Wheeler, J. C.

2017-11-01

We obtained broad-band BVRI photometry of SN 2013dy with the 0.76m Katzman Automatic Imaging Telescope (KAIT; Filippenko et al. 2001ASPC..246..121F). The multiband images were observed with the KAIT4 filter set from -16d to +337d relative to B-band maximum (MJD=56501.105). We also obtained riZYJH photometry of SN 2013dy with the multichannel Reionization And Transients InfraRed camera (RATIR; Butler et al. 2012SPIE.8446E..10B) mounted on the 1.5m Johnson telescope at the Mexican Observatorio Astronomico Nacional on Sierra San Pedro Martir in Baja California, Mexico (Watson et al. 2012SPIE.8444E..5LW). Typical observations include a series of 80s exposures in the ri bands and 60s exposures in the ZYJH bands, with dithering between exposures. (2 data files).

UCM Meteor and Fireball Research group: Results 2012--2014

NASA Astrophysics Data System (ADS)

Ocaña, F.; Sánchez de Miguel, A.; Zamorano, J.; Izquierdo, J.; Pascual, S.; Palos, M. F.; Oré, S.; Rodríguez-Coira, G.; Zamora, S.; Lorenzo, C.; San Juan, R.; Muñoz-Ibáñez, B.; Vázquez, C.; Alonso-Moragón, A.; Gallego, J.; Trigo-Rodríguez, J. M.; Madiedo, J. M.

2015-05-01

Most of the activity of the group is based on the Fireball Detection Station located at the Observatorio UCM, a system consisting of 6 high-sensitivity videocameras covering the whole sky with wide-angle lenses during nighttime. Another 15 cameras have been placed by the researchers between 10 and 200 km away from Madrid for multiple station observations. It works as a node in the SPanish Meteor and Fireball Network (SPMN), a network of similar stations covering the atmosphere over Spain. Besides the continuous monitoring, the group has worked on the recording and analysis of some meteor showers. Most of the attention was focused on the Draconids 2011 campaign at Observatorio de Sierra Nevada (Trigo-Rodríguez, J. M., Madiedo, J. M., Williams, I. P., et al. 2013, MNRAS, 433, 560; Ocaña, F., Palos, M. F., Zamorano, J., et al. 2013, Proceedings of the International Meteor Conference, 31st IMC, La Palma, Canary Islands, Spain, 2012, 70), and the 2012 Geminids balloon-borne mission over Spain (Sánchez de Miguel, A., Ocaña, F., Madiedo, J. M., et al. 2013, Lunar and Planetary Science Conference, 44, 2202). The products of the station have been used for undergraduate thesis projects at the Physics Faculty (Ocaña, F., 2011, UCM e-prints, 13292) and other undergraduate projects. In 2013 the station received new equipment thanks to the Certamen Arquímedes award, complementing the detection with spectroscopic and frame-integrating devices.

VizieR Online Data Catalog: Transits of PH3 b, c, and d through January, 2019 (Schmitt+, 2014)

NASA Astrophysics Data System (ADS)

Schmitt, J. R.; Agol, E.; Deck, K. M.; Rogers, L. A.; Gazak, J. Z.; Fischer, D. A.; Wang, J.; Holman, M. J.; Jek, K. J.; Margossian, C.; Omohundro, M. R.; Winarski, T.; Brewer, J. M.; Giguere, M. J.; Lintott, C.; Lynn, S.; Parrish, M.; Schawinski, K.; Schwamb, M. E.; Simpson, R.; Smith, A. M.

2017-05-01

Using quarters 1-16 of the Kepler data, we extracted and flattened each transit using the IDL AutoKep program (Gazak et al. 2012AdAst2012E..30G). For the high signal-to-noise transits of the outer planet, we used short cadence data where available. We then used a new, modified version of the IDL program TAP (Carter & Winn, 2009ApJ...704...51C; Gazak et al. 2012AdAst2012E..30G; Eastman et al. 2013PASP..125...83E) to fit for the orbital parameters of each planet: impact parameter (b), duration (T), the ratio of planet radius to stellar radius (Rp/R*), the midtransit times, linear limb darkening, quadratic limb darkening (Kipping, 2013MNRAS.435.2152K), and white and red noise. The ratio of semi-major axis to the radius of the star (a/R*) and the inclination (i) can be derived from these parameters. (1 data file).

Teachers' views of a new general education program in Hong Kong: a qualitative study.

PubMed

Shek, Daniel T L; Yu, Lu; Wu, Florence K Y; Chai, Wen Y

2017-02-01

Under the new education reform in Hong Kong, The Hong Kong Polytechnic University (PolyU) has expanded its undergraduate education from 3 to 4 years since the 2012-2013 academic year. Along with the transition, the General University Requirements (GUR) has been developed as an integral part on general education of the new 4-year undergraduate curriculum of PolyU. The present study examined the implementation quality and effectiveness of the GUR in the 2012-2013 academic year based on focus group interviews with teachers. Twenty teachers who taught GUR subjects were interviewed for their perceptions and experiences about the GUR. Results revealed that the teachers generally had positive perceptions of the GUR in terms of its rationales, teaching and learning modes, and implementation quality. GUR subjects were also considered effective in helping students to develop in a holistic manner. The findings suggest that the first-year implementation of the GUR at PolyU was basically successful.

Building Library Skills: Computer-Assisted Instruction for Undergraduates.

ERIC Educational Resources Information Center

Dixon, Lana; And Others

1995-01-01

Discusses the development and implementation of computer-assisted instruction in undergraduate English classes at the University of Tennessee, Knoxville. Describes three HyperCard modules that help students learn to find periodical articles, use the library's online catalog, and search MLA on CD-ROM. Also presents reactions from students, English…

VizieR Online Data Catalog: 76 T dwarfs from the UKIDSS LAS (Burningham+, 2013)

NASA Astrophysics Data System (ADS)

Burningham, B.; Cardoso, C. V.; Smith, L.; Leggett, S. K.; Smart, R. L.; Mann, A. W.; Dhital, S.; Lucas, P. W.; Tinney, C. G.; Pinfield, D. J.; Zhang, Z.; Morley, C.; Saumon, D.; Aller, K.; Littlefair, S. P.; Homeier, D.; Lodieu, N.; Deacon, N.; Marley, M. S.; van Spaandonk, L.; Baker, D.; Allard, F.; Andrei, A. H.; Canty, J.; Clarke, J.; Day-Jones, A. C.; Dupuy, T.; Fortney, J. J.; Gomes, J.; Ishii, M.; Jones, H. R. A.; Liu, M.; Magazzu, A.; Marocco, F.; Murray, D. N.; Rojas-Ayala, B.; Tamura, M.

2014-07-01

Our broad-band NIR photometry was obtained using the UKIRT Fast Track Imager (UFTI) and WFCAM, both mounted on UKIRT across a number of observing runs spanning 2009 to the end of 2010. Differential methane photometry was obtained using the Near Infrared Camera Spectrometer (NICS) mounted on the TNG under programme AOT22 TAC 96 spanning from 2010 to 2012. (5 data files).

VizieR Online Data Catalog: JCMT Gould Belt Survey: W40 complex (Rumble+, 2016)

NASA Astrophysics Data System (ADS)

Rumble, D.; Hatchell, J.; Pattle, K.; Kirk, H.; Wilson, T.; Buckle, J.; Berry, D. S.; Broekhoven-Fiene, H.; Currie, M. J.; Fich, M.; Jenness, T.; Johnstone, D.; Mottram, J. C.; Nutter, D.; Pineda, J. E.; Quinn, C.; Salji, C.; Tisi, S.; Walker-Smith, S.; di, Francesco J.; Hogerheijde, M. R.; Ward-Thompson, D.; Bastien, P.; Bresnahan, D.; Butner, H.; Chen, M.; Chrysostomou, A.; Coude, S.; Davis, C. J.; Drabek-Maunder, E.; Duarte-Cabral, A.; Fiege, J.; Friberg, P.; Friesen, R.; Fuller, G. A.; Graves, S.; Greaves, J.; Gregson, J.; Holland, W.; Joncas, G.; Kirk, J. M.; Knee, L. B. G.; Mairs, S.; Marsh, K.; Matthews, B. C.; Moriarty-Schieven, G.; Mowat, C.; Rawlings, J.; Richer, J.; Robertson, D.; Rosolowsky, E.; Sadavoy, S.; Thomas, H.; Tothill, N.; Viti, S.; White, G. J.; Wouterloot, J.; Yates, J.; Zhu, M.

2017-11-01

Aquila was observed with SCUBA-2 (Holland et al., 2013MNRAS.430.2513H) between 2012 April 21 and July 5 as part of the JCMT GBS MJLSG33 SCUBA-2 Serpens Campaign. Four separate fully sampled 30 arcmin diameter circular continuum observations (PONG1800 mapping mode) were taken simultaneously at 850um and 450um, and subsequently combined into mosaics. (3 data files).

VizieR Online Data Catalog: 6.7GHz methanol maser polarization in SFR (Surcis+, 2015)

NASA Astrophysics Data System (ADS)

Surcis, G.; Vlemmings, W. H. T.; van Langevelde, H. J.; Hutawarakorn Kramer, B.; Bartkiewicz, A.; Blasi, M. G.

2015-09-01

The first seven massive SFRs were observed at 6.7GHz in full polarization spectral mode with eight of the EVN antennas (Effelsberg, Jodrell, Onsala, Medicina, Noto, Torun, Westerbork, and Yebes-40m) between November 2012 and June 2013, for a total observation time of 49h. The bandwidth was 2MHz, providing a velocity range of ~100km/s. (8 data files).

48 CFR 752.7022 - Conflicts between contract and catalog.

Code of Federal Regulations, 2012 CFR

2012-10-01

... 48 Federal Acquisition Regulations System 5 2012-10-01 2012-10-01 false Conflicts between contract and catalog. 752.7022 Section 752.7022 Federal Acquisition Regulations System AGENCY FOR INTERNATIONAL....7022 Conflicts between contract and catalog. For use in contracts for participant training with an...

Council on Social Work Education: Annual Report 2012/2013

ERIC Educational Resources Information Center

Council on Social Work Education, 2013

2013-01-01

The Council on Social Work Education (CSWE) is a nonprofit national association representing more than 2,500 individual members as well as 685 graduate and undergraduate programs of professional social work education. Founded in 1952, this partnership of educational and professional institutions, social welfare agencies, and private citizens is…

48 CFR 752.7022 - Conflicts between contract and catalog.

Code of Federal Regulations, 2013 CFR

2013-10-01

... 48 Federal Acquisition Regulations System 5 2013-10-01 2013-10-01 false Conflicts between contract and catalog. 752.7022 Section 752.7022 Federal Acquisition Regulations System AGENCY FOR INTERNATIONAL....7022 Conflicts between contract and catalog. For use in contracts for participant training with an...

VizieR Online Data Catalog: Vilnius photometry of M29 (NGC6913) (Milasius+, 2013)

NASA Astrophysics Data System (ADS)

Milasius, K.; Boyle, R. P.; Vrba, F. J.; Janusz, R.; Straizys, V.; Cernis, K.; Laugalys, V.; Zdanavicius, K.; Zdanavicius, J.; Kazlauskas, A.; Smilgys, R.

2015-01-01

The observational material was obtained with CCD cameras on three different telescopes: the wide-field Maksutov-type 35/51cm telescope of the Moletai Observatory in Lithuania (2004), the 1m Ritchey telescope at the Flagstaff Station of the US Naval Observatory in Arizona (2006-2008) and the 1.8m VATT telescope of the Vatican Observatory on Mt. Graham, Arizona (2011-2012). (3 data files).

VizieR Online Data Catalog: Segue 3 VI photometry (Ortolani+, 2013)

NASA Astrophysics Data System (ADS)

Ortolani, S.; Bica, E.; Barbuy, B.

2015-01-01

Johnson-Cousins V and I images were obtained at the Telescopio Nazionale Galileo (TNG), equipped with the spectrograph/focal reducer DOLORES, with a 2000x2000-pixels of 8.5x8.5-arcmin2 CCD giving 0.25arcsec/pix, during the night of 2011 June 26-27. Additional B, V and I photometry was obtained, with the same equipment, in the night of 2012 June 17-18. (2 data files).

41 CFR 101-30.504 - Cataloging data from Defense Logistics Services Center (DLSC).

Code of Federal Regulations, 2012 CFR

2012-07-01

... 41 Public Contracts and Property Management 2 2012-07-01 2012-07-01 false Cataloging data from Defense Logistics Services Center (DLSC). 101-30.504 Section 101-30.504 Public Contracts and Property... data from Defense Logistics Services Center (DLSC). Upon receipt of cataloging data from civil agencies...

VizieR Online Data Catalog: Spatial structure of young stellar clusters. III. (Kuhn+, 2015)

NASA Astrophysics Data System (ADS)

Kuhn, M. A.; Feigelson, E. D.; Getman, K. V.; Sills, A.; Bate, M. R.; Borissova, J.

2017-10-01

This paper uses the Paper I (Kuhn et al. 2014, J/ApJ/787/107) catalog of 142 subclusters of young stars in 17 MYStIX star-forming regions. These subclusters were found and characterized using the stars in the MYStIX Probable Complex Member (MPCM) catalogs from Broos et al. (2013, J/ApJS/209/32). The multiwavelength data analysis efforts that went into this catalog are described by Feigelson et al. (2013, J/ApJS/209/26), King et al. (2013, J/ApJS/209/28), Kuhn et al. (2013, J/ApJS/209/27; 2013, J/ApJS/209/29), Naylor et al. (2013, J/ApJS/209/30), Povich et al. (2013, J/ApJS/209/31), and Townsley et al. (2014, J/ApJS/213/1), which provided uniform data coverage across the 17 star-forming regions investigated here, including the most comprehensive and reliable lists of young stars in many of the nearest MSFRs. (3 data files).

Do Military Veteran and Civilian Students Function Differently in College?

ERIC Educational Resources Information Center

Smith, James G.; Vilhauer, Ruvanee P.; Chafos, Vanessa

2017-01-01

Objective: The authors sought to assess military veterans' functioning in college by comparing their experience with that of civilian students. Participants: The study, conducted from April 2012 to February 2013, included 445 civilian and 61 student service member/veteran (SSM/V) undergraduates, drawn from a community college and two 4-year…

Understanding the Leaky Pipeline: Perceived Barriers to Pursuing a Career in Medicine or Dentistry Among Underrepresented-in-Medicine Undergraduate Students.

PubMed

Freeman, Brandi Kaye; Landry, Alden; Trevino, Robert; Grande, David; Shea, Judy A

2016-07-01

Representation of persons from diverse backgrounds remains a persistent challenge for medicine and dentistry workforces. Past research has focused on quantifying factors such as markers of educational achievement to explain the difficulty of increasing diversity within the professions. There has been less effort toward understanding the perspectives of undergraduate students on the threshold of applying to medical/dental school about distinct barriers to pursuing a medical or dental career and continuing through the training pipeline. In 2012 and 2013, the authors conducted a qualitative study of undergraduate students participating in the Tour for Diversity in Medicine, a program where minority physicians and dentists visit colleges with large fractions of minority students to encourage careers in the health professions. Focus groups were convened during the visits to examine perceived barriers to pursuing careers in medicine and dentistry and challenges identified through thematic content analysis. Eighty-two students participated in discussions at 11 colleges visited between September 2012 and February 2013. Students described challenges including inadequate institutional resources (e.g., sparse clinical opportunities), strained personal resources (e.g., conflict arising from familial pressure), inadequate guidance and mentoring to assist with key career decisions, and societal barriers. For participants, these challenges caused them to question the viability of persisting in the pipeline to a medical or dental career. Solving the issue of diversity in medicine and dentistry is multifaceted, but elucidated challenges from the undergraduate student perspective offer targeted areas where intervention may help remedy barriers and decrease pipeline leakiness.

Seismicity of the North of the Russian Plate: Relocation of Recent Earthquakese

NASA Astrophysics Data System (ADS)

Morozov, A. N.; Vaganova, N. V.; Asming, V. E.; Mikhailova, Ya. A.

2018-03-01

The hypocenters of the earthquakes recorded in the north of the Russian Plate from 1982 to 2013 are relocated. The relocation of the hypocenters is based on the common velocity section, common methodology, and the entire set of the initial data and bulletins available from the Russian and foreign seismic stations. The efficiency of the algorithm for calculating the hypocentral parameters and the velocity section is demonstrated by the example of two nonmilitary nuclear explosions in July 18, 1985 and September 6, 1988 in the northern part of the European Russia. For the first time, two earthquakes of July 19, 1982 and October 7, 2012, which have not been previously reported in the catalogs for the north of the Russian plate, are included in the seismic catalog.

VizieR Online Data Catalog: Second Planck Catalogue of Compact Sources (PCCS2) (Planck+, 2016)

NASA Astrophysics Data System (ADS)

Planck Collaboration; Ade, P. A. R.; Aghanim, N.; Argueso, F.; Arnaud, M.; Ashdown, M.; Aumont, J.; Baccigalupi, C.; Banday, A. J.; Barreiro, R. B.; Bartolo, N.; Battaner, E.; Beichman, C.; Benabed, K.; Benoit, A.; Benoit-Levy, A.; Bernard, J.-P.; Bersanelli, M.; Bielewicz, P.; Bock, J. J.; Bohringer, H.; Bonaldi, A.; Bonavera, L.; Bond, J. R.; Borrill, J.; Bouchet, F. R.; Boulanger, F.; Bucher, M.; Burigana, C.; Butler, R. C.; Calabrese, E.; Cardoso, J.-F.; Carvalho, P.; Catalano, A.; Challinor, A.; Chamballu, A.; Chary, R.-R.; Chiang, H. C.; Christensen, P. R.; Clemens, M.; Clements, D. L.; Colombi, S.; Colombo, L. P. L.; Combet, C.; Couchot, F.; Coulais, A.; Crill, B. P.; Curto, A.; Cuttaia, F.; Danese, L.; Davies, R. D.; Davis, R. J.; de Bernardis, P.; De Rosa, A.; de Zotti, G.; Delabrouille, J.; Desert, F.-X.; Dickinson, C.; Diego, J. M.; Dole, H.; Donzelli, S.; Dore, O.; Douspis, M.; Ducout, A.; Dupac, X.; Efstathiou, G.; Elsner, F.; Ensslin, T. A.; Eriksen, H. K.; Falgarone, E.; Fergusson, J.; Finelli, F.; Forni, O.; Frailis, M.; Fraisse, A. A.; Franceschi, E.; Frejse, L. A.; Galeotta, S.; Galli, S.; Ganga, K.; Giard, M.; Giraud-Heraud, Y.; Gjerlow, E.; Gonzalez-Nuevo, J.; Gorski, K. M.; Gratton, S.; Gregorio, A.; Gruppuso, A.; Gudmundsson, J. E.; Hansen, F. K.; Hanson, D.; Harrison, D. L.; Helou, G.; Henrot-Versille, S.; Hernandez-Monteagudo, C.; Herranz, D.; Hildebrandt, S. R.; Hivon, E.; Hobson, M.; Holmes, W. A.; Hornstrup, A.; Hovest, W.; Huffenberger, K. M.; Hurier, G.; Jaffe, A. H.; Jaffe, T. R.; Jones, W. C.; Juvela, M.; Keihanen, E.; Keskitalo, R.; Kisner, T. S.; Kneissl, R.; Knoche, J.; Kunz, M.; Kurki-Suonio, H.; Lagache, G.; Lahteenmaki, A.; Lamarre, J.-M.; Lasenby, A.; Lattanzi, M.; Lawrence, C. R.; Leahy, J. P.; Leonardi, R.; Leon-Tavares, J.; Lesgourgues, J.; Levrier, F.; Liguori, M.; Lilje, P. B.; Linden-Vornle, M.; Lopez-Caniego, M.; Lubin, P. M.; Macias-Perez, J. F.; Maggio, G.; Maino, D.; Mandolesi, N.; Mangilli, A.; Maris, M.; Marshall, D. J.; Martin, P. G.; Martinez-Gonzalez, E.; Masi, S.; Matarrese, S.; McGehee, P.; Meinhold, P. R.; Melchiorri, A.; Mendes, L.; Mennella, A.; Migliaccio, M.; Mitra, S.; Miville-Deschenes, M.-A.; Moneti, A.; Montier, L.; Morgante, G.; Mortlock, D.; Moss, A.; Munshi, D.; Murphy, J. A.; Naselsky, P.; Nati, F.; Natoli, P.; Negrello, M.; Netterfield, C. B.; Norgaard-Nielsen, H. U.; Noviello, F.; Novikov, D.; Novikov, I.; Oxborrow, C. A.; Paci, F.; Pagano, L.; Pajot, F.; Paladini, R.; Paoletti, D.; Partridge, B.; Pasian, F.; Patanchon, G.; Pearson, T. J.; Perdereau, O.; Perotto, L.; Perrotta, F.; Pettorino, V.; Piacentini, F.; Piat, M.; Pierpaoli, E.; Pietrobon, D.; Plaszczynski, S.; Pointecouteau, E.; Polenta, G.; Pratt, G. W.; Prezeau, G.; Prunet, S.; Puget, J.-L.; Rachen, J. P.; Reach, W. T.; Rebolo, R.; Reinecke, M.; Remazeilles, M.; Renault, C.; Renzi, A.; Ristorcelli, I.; Rocha, G.; Rosset, C.; Rossetti, M.; Roudier, G.; Rowan-Robinson, M.; Rubino-Martin, J. A.; Rusholme, B.; Sandri, M.; Sanghera, H. S.; Santos, D.; Savelainen, M.; Savini, G.; Scott, D.; Seiffert, M. D.; Shellard, E. P. S.; Spencer, L. D.; Stolyarov, V.; Sudiwala, R.; Sunyaev, R.; Sutton, D.; Suur-Uski, A.-S.; Sygnet, J.-F.; Tauber, J. A.; Terenzi, L.; Toffolatti, L.; Tomasi, M.; Torni Koski, M.; Tristram, M.; Tucci, M.; Tuovinen, J.; Turler, M.; Umana, G.; Valenziano, L.; Valiviita, J.; van Tent, B.; Vielva, P.; Villa, F.; Wade, L. A.; Walter, B.; Wandelt, B. D.; Wehus, I. K.; Yvon, D.; Zacchei, A.; Zonca, A.

2017-01-01

The Low Frequency Instrument (LFI) DPC produced the 30, 44, and 70GHz maps after the completion of eight full surveys (spanning the period 12 August 2009 to 3 August 2013). In addition, special LFI maps covering the period 1 April 2013 to 30 June 2013 were produced in order to compare the Planck flux-density scales with those of the Very Large Array and the Australia Telescope Compact Array, by performing simultaneous observations of a sample of sources over that period. The High Frequency Instrument (HFI) DPC produced the 100, 143, 217, 353, 545, and 857GHz maps after five full surveys (2009 August 12 to 2012 January 11). (16 data files).

Characteristics of Seismicity at Ngatamariki and Rotokawa Geothermal Fields, North Island, New Zealand

NASA Astrophysics Data System (ADS)

Hopp, C. J.; Mroczek, S.; Savage, M. K.; Sewell, S. M.; Townend, J.; Sherburn, S.

2017-12-01

Fluid-induced seismicity (FIS) is a useful indicator of thermal and pressure changes within a geothermal reservoir. Given the difficulty of making measurements in the space between wells, FIS provides one of the only direct observations of fluid-related reservoir processes. Understanding exactly why and how these microearthquakes occur helps us unravel the interaction between the movement of fluid and heat at depth and could allow for a better understanding of the creation and destruction of permeability in the reservoir. We begin with an earthquake catalog of roughly 6200 events which occurred between May 2012 and November 2015 at the Mercury geothermal fields at Rotokawa and Ngatamariki. We expand this catalog using matched filter detection to include 350,000 microearthquakes. Earthquakes at the fields are densely clustered in areas of active fluid injection and the rate of seismicity is highly correlated with injection rate. We present high-precision locations as well as frequency-magnitude distributions and source mechanisms for significant events and discuss their relation to injection and production rates at the fields. In particular, we focus on specific periods of interest including the stimulation of well NM08 in June 2012, the Ngatamariki plant startup in April 2013, the switch of injection at Rotokawa to well RK22 in 2013 and a prolonged period of permeability change at well RK24.

VizieR Online Data Catalog: Cool KOIs. VI. H- and K- band spectra (Muirhead+, 2014)

NASA Astrophysics Data System (ADS)

Muirhead, P. S.; Becker, J.; Feiden, G. A.; Rojas-Ayala, B.; Vanderburg, A.; Price, E. M.; Thorp, R.; Law, N. M.; Riddle, R.; Baranec, C.; Hamren, K.; Schlawin, E.; Covey, K. R.; Johnson, J. A.; Lloyd, J. P.

2014-09-01

We observed the Cool KOIs with the TripleSpec Spectrograph at the Palomar Observatory 200 inch Hale Telescope. TripleSpec is a near-infrared slit spectrograph covering 1.0 to 2.5um simultaneously with a resolving power (λ/Δλ) of 2700. Observations were carried out in 2011 June and August for the KOIs from Borucki et al. (2011, Cat. J/ApJ/736/19), with results published in a previous letter (Muirhead et al. 2012, Cat. J/ApJ/750/L37). In July and August of 2012, we augmented observations to include all of the Cool KOIs selected in Batalha et al. (2013, Cat. J/ApJS/204/24). In 2013 July and August, we observed the remaining Cool KOIs listed on the NASA Exoplanet Archive (NEA) as of the observations. (3 data files).

VizieR Online Data Catalog: The Initial Gaia Source List (IGSL) (Smart, 2013)

NASA Astrophysics Data System (ADS)

Smart, R. L.; Nicastro, L.

2013-11-01

The IGSL is a compilation catalog produced for the Gaia mission. We have combined data from the following catalogs or datasets to produce a homogenous list of positons, proper motions, photometry in a blue and red band and estimates of the magnitudes in the Gaia G and G_RVS bands. Included Catalogs: Tycho2, LQRF, UCAC4, SDSS-DR9, PPMXL, GSC23, GEPC, OGLE, Sky2000, 2MASS. Note that in compiling the various entries we did not consider the individual flags. Overall, we think this catalog is reliable but there will be errors, mismatches and duplicates. The user should use this catalog with that in mind, it is fine for statistical studies that has some way to remove obviously incorrect entries but it should only be used with care for individual objects. The source catalogs used to produce the IGSL are: * The Gaia Ecliptic Pole Catalog, version 3.0 (GEPC) Altmann & Bastian 2009, "Ecliptic Poles Catalogue Version 1.1" ESA Document GAIA-C3-TN-ARI-MA-002 URL http://www.rssd.esa.int/llink/livelink/open/2885828 * GSC2.3: GSC2 version 2.3, Lasker et al. 2008AJ....136..735L (I/305) * an excerpt of the 4th version of the Gaia Initial QSO Catalog (GIQC) as compiled by the GWP-S-335-13000, formed by Alexandre H. Andrei, Christophe Barache, Dario N. da Silva Neto, Francois Taris, Geraldine Bourda, Jean-Francois Le Campion, Jean Souchay, J.J. Pereira Osorio, Julio I. Bueno de Camargo, Marcelo Assafin, Roberto Vieira Martins, Sebastien Bouquillon, Sebastien Lambert, Sonia Anton, Patrick Charlot * OGLE: Optical Gravitational Lensing Experiment version III (Szymaski et al., 2011, Cat. J/AcA/61/83) * PPMXL: Positions and Proper Motions "Extra Large" Catalog, Roeser et al. (2010, Cat. I/317) * SDSS: Sloan Digital Sky Survey data release 9, Cat. V/139 * UCAC4: Zacharias et al., 2012, Cat. I/322 * Tycho-2, Hoeg et al., 2000, Cat. I/259 (1 data file).

Learning Challenges and Preferred Pedagogies of International Students: A Perspective from the USA

ERIC Educational Resources Information Center

Rao, Pramila

2017-01-01

Purpose: The purpose of this paper is to understand the challenges international students face during their higher education in the USA. This research study was conducted at a private university in the Eastern region of the USA from October 2012 through May 2013 (Fall and Spring semesters) with undergraduate and graduate international students.…

VizieR Online Data Catalog: Spectrum of VY CMa in 220.65-224.25GHz range (Kaminski+, 2013)

NASA Astrophysics Data System (ADS)

Kaminski, T.; Gottlieb, C. A.; Menten, K. M.; Patel, N. A.; Young, K. H.; Brunken, S.; Muller, H. S. P.; McCarthy, M. C.; Winters, J. M.; Decin, L.

2013-02-01

A spectrum of VY Canis Majoris obtained with the Plateau de Bure Interferometer on 22 April and 13 October 2012 in the frequency range 220.65-224.25GHz. The interferometer was used in its D configuration with six antennas and the synthesized beam was 4.9x2.2-arcsec. The spectrum was extracted from the central pixel of the map obtained with the gridding of 0.65-arcsec. (2 data files).

VizieR Online Data Catalog: BVR light curves of UZ Leo (Lee+, 2018)

NASA Astrophysics Data System (ADS)

Lee, J. W.; Park, J.-H.

2018-04-01

We performed new CCD photometry of UZ Leo during two observing seasons between 2012 February and 2013 April, using a PIXIS: 2048B CCD and a BVR filter set attached to the 61 cm reflector at Sobaeksan Optical Astronomy Observatory (SOAO) in Korea. The CCD chip has 2048x2048pixels and a pixel size of 13.5um, so the field of view of a CCD frame is 17.6'x17.6'. (1 data file).

Overview and History of CUWiP

NASA Astrophysics Data System (ADS)

Pitts, Kevin

2014-03-01

The APS Conferences for Undergraduate Women in Physics (CUWiP) are a continuation of a grass-roots collaborative effort of physicists from around the country that has provided conferences for undergraduate women annually since 2006. The goals of the CUWiP effort are to increase retention and improve career outcomes of undergraduate women in physics by (i) communicating the breadth of education and career paths open to physics majors; (ii) disseminating information and advice on applying for summer research, graduate school and professional employment; and (iii) providing opportunities to share experiences, advice and ideas with women at different stages of their education or career paths. Since the first conference in 2006, the number of CUWiP locations has grown from one in the first two years to six in 2012 and 2013. The number of participants has shown more than commensurate growth--increasing from 29 students to approximately 650 in the first seven years. Close to 900 women attended the 2013 conferences and almost 300 applicants had to be turned away. The 2014 Conferences again saw record number of applicants and attendees, with 1300 students participated in conferences at eight different sites.

Catalog of Computer Programs Used in Undergraduate Geological Education.

ERIC Educational Resources Information Center

Burger, H. Robert

1983-01-01

Provides list of mineralogy, petrology, and geochemistry computer programs. Each entry includes a brief description, program name and language, availability of program listing, and source and/or reference. (JN)

VizieR Online Data Catalog: Follow-up study of gal. & AGNs in z>1 clusters (Alberts+, 2016)

NASA Astrophysics Data System (ADS)

Alberts, S.; Pope, A.; Brodwin, M.; Chung, S. M.; Cybulski, R.; Dey, A.; Eisenhardt, P. R. M.; Galametz, A.; Gonzalez, A. H.; Jannuzi, B. T.; Stanford, S. A.; Snyder, G. F.; Stern, D.; Zeimann, G. R.

2016-08-01

In this work, we concentrate our analysis on 11 spectroscopically confirmed clusters from the IRAC Shallow/Distant Cluster Survey (ISCS/IDCS) that we observed with Herschel/PACS at 100 and 160um, obtained during Open Time 2 observing (PID: OT2apope3) (summary of imaging in table 6 spanning from June 2012 to January 2013). Given the resolution of PACS (FWHM~6.7" at 100um and 11" at 160um), we expect the majority of sources and all cluster galaxies in our maps to be point sources. See sections 2.1 and 2.3 for further details. The IRAC Shallow Survey (ISS) was followed up with three more observations as part of SDWFS (Ashby et al. 2009, see J/ApJ/716/530), providing a factor of 2 deeper IRAC catalog with an aperture-corrected 5σ limit of 5.2uJy at 4.5um ([4.5]=18.83mag). Spitzer/MIPS observations are available from the MIPS AGM and Galaxy Evolution Survey (MAGES; Jannuzi et al. 2010AAS...21547001J). See section 2.4 for further details. Targeted follow up campaigns by our group have obtained spectroscopic redshifts for galaxies and AGNs in z>1 clusters using multi-object Keck optical spectroscopy and Wide Field Camera 3 (WFC3) slitless NIR grism spectroscopy from the Hubble Space Telescope (HST). The reader is directed to Brodwin et al. (2013ApJ...779..138B), Zeimann et al. (2013, J/ApJ/779/137), and references therein for a detailed description of the targeted spectroscopy. Some spectroscopic redshifts are additionally provided by the AGN and Galaxy Evolution Survey (AGES; Kochanek et al. 2012, J/ApJS/200/8). See section 2.2. (3 data files).

Exploring the Impact of the Increased Tuition Fees on Academic Staffs' Experiences in Post-92 Universities: A Small-Scale Qualitative Study

ERIC Educational Resources Information Center

Bates, Elizabeth A.; Kaye, Linda K.; Blewitt, John

2014-01-01

The introduction of the new tuition fee regime in the UK academic session 2012-2013 has resulted in concerns in the Higher Education (HE) community that students' expectations may become unmanageable. Previous research has explored the expectations and experiences of undergraduate psychology students; the current study extended this by considering…

I Did That Wrong and It Sounded Good: An Ethnographic Study of Vernacular Music Making in Higher Education

ERIC Educational Resources Information Center

Ezquerra, Victor N.

2014-01-01

The purpose of this ethnographic study was to examine vernacular music making in higher education. The participants, undergraduate music education majors (N = 23 for Fall, N = 10 for Spring), were investigated throughout the course of the 2012-2013 academic year. A constructivist philosophical framework was applied and data were collected using…

VizieR Online Data Catalog: WASP-31b:HST/Spitzer transmission spectral survey (Sing+, 2015)

NASA Astrophysics Data System (ADS)

Sing, D. K.; Wakeford, H. R.; Showman, A. P.; Nikolov, N.; Fortney, J. J.; Burrows, A. S.; Ballester, G. E.; Deming, D.; Aigrain, S.; Desert, J.-M.; Gibson, N. P.; Henry, G. W.; Knutson, H.; Lecavelier Des Etangs, A.; Pont, F.; Vidal-Madjar, A.; Williamson, M. W.; Wilson, P. A.

2017-11-01

We observed two transits of WASP-31b with the HST STIS G430L grating during 2012 June 13 and 26, as well as one transit with the STIS G750L during 2012 July 10. In addition to the STIS data, observations of WASP-31b were also conducted in the infrared with WFC3 on the HST. Observations began on 2012 May 13 at 12:53 using the IR G141 grism in forward spatial scan mode over five HST orbits. We analyse two transit observations obtained using the Infrared Array Camera (IRAC) instrument (Programme 90092 with P.I. Desert) on the Spitzer space telescope in the 3.6 μm and 4.5 μm channels in subarray mode (32x32 pixel, or 39 centred on the planets host). The 3.6 μm observation was performed on UT 2013 March 9 (between 06:59 and 11:37) and the 4.5 observation was performed on UT 2013 March 19 (between 12:19 and 16:58). (1 data file).

77 FR 3009 - Knowledge and Abilities Catalog for Nuclear Power Plant Operators: Advanced Boiling Water Reactors

Federal Register 2010, 2011, 2012, 2013, 2014

2012-01-20

... NUCLEAR REGULATORY COMMISSION [NRC-2012-0010] Knowledge and Abilities Catalog for Nuclear Power... comment a draft NUREG, NUREG-2104, Revision 0, ``Knowledge and Abilities Catalog for Nuclear Power Plant... developed using this Catalog along with the Operator Licensing Examination Standards for Power Reactors...

VizieR Online Data Catalog: XMM-Newton and Chandra monitoring of Sgr A* (Ponti+, 2015)

NASA Astrophysics Data System (ADS)

Ponti, G.; de, Marco B.; Morris, M. R.; Merloni, A.; Munoz-Darias, T.; Clavel, M.; Haggard, D.; Zhang, S.; Nandra, K.; Gillessen, S.; Mori, K.; Neilsen, J.; Rea, N.; Degenaar, N.; Terrier, R.; Goldwurm, A.

2018-01-01

As of 2014 November 11 the XMM-Newton archive contains 37 public observations that can be used for our analysis of Sgr A*. In addition, we consider four new observations aimed at monitoring the interaction between the G2 object and Sgr A*, performed in fall 2014 (see Table A4). A total of 41 XMM-Newton data sets are considered in this work. All the 46 Chandra observations accumulated between 1999 and 2011 and analysed here are obtained with the ACIS-I camera without any gratings on (see Table A1). From 2012 onwards, data from the ACIS-S camera were also employed. The 2012 Chandra "X-ray Visionary Project" (XVP) is composed of 38 High-Energy Transmission Grating (HETG) observations with the ACIS-S camera at the focus (Nowak et al. 2012ApJ...759...95N; Neilsen et al. 2013ApJ...774...42N; 2015ApJ...799..199N; Wang et al. 2013Sci...341..981W; see Table A2). The first two observations of the 2013 monitoring campaign were performed with the ACIS-I instrument, while the ACIS-S camera was employed in all the remaining observations, after the outburst of SGR J1745-2900 on 2013 April 25. Three observations between 2013 May and July were performed with the HETG on, while all the remaining ones do not employ any gratings (see Table A2). (4 data files).

VizieR Online Data Catalog: 2FGL sources observed between 5-9GHz (Schinzel+, 2015)

NASA Astrophysics Data System (ADS)

Schinzel, F. K.; Petrov, L.; Taylor, G. B.; Mahony, E. K.; Edwards, P. G.; Kovalev, Yu. Y.

2015-04-01

A list of 216 target fields were observed with the Very Large Array (VLA). The instantaneous bandwidth was split into two parts, with one half centered at 5.0GHz (4.5-5.5GHz) and the other centered at 7.3GHz (6.8-7.8GHz); on 2012 October 26 and 2012 November 3. See section 2.1 During the first campaign with the Australia Telescope Compact Array (ATCA), from 2012 September 19-20, we observed 411 2FGL unassociated sources in a decl. range of [-90°, +10°] at 5.5 and 9GHz. The details of that observing campaign and results have been reported by Petrov et al. (2013, J/MNRAS/432/1294). We detected a total of 424 point sources. In a second ATCA campaign on 2013 September 25-28, we re-observed sources that were detected at 5GHz, but were not detected at 9GHz. See section 2.2. Follow-up observations of 149 targets selected from the VLA and ATCA survey above -30° decl. were conducted with the Very Long Baseline Array (VLBA) between 2013 Feb-Aug (VCS7 project; 4.128-4.608 and 7.392-7.872GHz simultaneously) and in 2013 Jun-Dec (campaign S5272; 7.392-7.872GHz only). See section 2.3. For sources with decl. below -30° we added 21 objects to the on-going LCS campaign (Petrov et al. 2011, J/MNRAS/414/2528) in 2013 Mar-2013 Jun at 8.200-8.520GHz. See section 2.4. (7 data files).

VizieR Online Data Catalog: KiDS-ESO-DR2 multi-band source catalog (de Jong+, 2015)

NASA Astrophysics Data System (ADS)

de Jong, J. T. A.; Verdoes Kleijn, G. A.; Boxhoorn, D. R.; Buddelmeijer, H.; Capaccioli, M.; Getman, F.; Grado, A.; Helmich, E.; Huang, Z.; Irisarri, N.; Kuijken, K.; La Barbera, F.; McFarland, J. P.; Napolitano, N. R.; Radovich, M.; Sikkema, G.; Valentijn, E. A.; Begeman, K. G.; Brescia, M.; Cavuoti, S.; Choi, A.; Cordes, O.-M.; Covone, G.; Dall'Ora, M.; Hildebrandt, H.; Longo, G.; Nakajima, R.; Paolillo, M.; Puddu, E.; Rifatto, A.; Tortora, C.; van Uitert, E.; Buddendiek, A.; Harnois-Deraps, J.; Erben, T.; Eriksen, M. B.; Heymans, C.; Hoekstra, H.; Joachimi, B.; Kitching, T. D.; Klaes, D.; Koopmans, L. V. E.; Koehlinger, F.; Roy, N.; Sifon, C.; Schneider, P.; Sutherland, W. J.; Viola, M.; Vriend, W.-J.

2016-10-01

KiDS data releases consist of ~1 square degree tiles that have been successfully observed in all four survey filters (u,g,r,i). The second data release (KiDS-ESO-DR2) was available in February 2015 and contains imaging data, masks and single-band source lists for all tiles observed in all four filters for which observations were completed during the second year of regular operations (1 October 2012 to 31 September 2013), a total of 98 tiles. Apart from the data products mentioned above, KiDS-ESO-DR2 also provides a multi-band source catalogue based on the combined set of 148 tiles released in the first two data releases. A complete list of all tiles with data quality parameters can be found on the KiDS website: http://kids.strw.leidenuniv.nl/DR2/ (1 data file).

VizieR Online Data Catalog: NIR spectroscopy of 1.5

NASA Astrophysics Data System (ADS)

Shen, Y.

2016-04-01

Our sample of quasars with near-IR spectroscopy consists of the 60 quasars at z~1.5-2.2 from Shen & Liu (2012, J/ApJ/753/125), and 14 additional quasars at z~3.3 for which we have obtained near-IR spectroscopy with the Folded-port InfraRed Echellett (FIRE) on the 6.5m Magellan-Baade telescope during two runs in 2013 May and December. These quasars were selected from the SDSS DR7 (Abazajian et al. 2009, II/294) quasar catalog (Shen et al. 2011, J/ApJS/194/45) with good optical spectra covering the CIV line and in redshift windows of z~1.5,2.1,3.3 such that the Hβ-[OIII] region can be covered in the JHK bands in the near-IR. (2 data files).

41 CFR 101-30.400 - Scope of subpart.

Code of Federal Regulations, 2012 CFR

2012-07-01

... 41 Public Contracts and Property Management 2 2012-07-01 2012-07-01 false Scope of subpart. 101-30... Regulations System FEDERAL PROPERTY MANAGEMENT REGULATIONS SUPPLY AND PROCUREMENT 30-FEDERAL CATALOG SYSTEM 30.4-Use of the Federal Catalog System § 101-30.400 Scope of subpart. This subpart prescribes the...

41 CFR 101-30.500 - Scope of subpart.

Code of Federal Regulations, 2012 CFR

2012-07-01

... 41 Public Contracts and Property Management 2 2012-07-01 2012-07-01 false Scope of subpart. 101-30... Regulations System FEDERAL PROPERTY MANAGEMENT REGULATIONS SUPPLY AND PROCUREMENT 30-FEDERAL CATALOG SYSTEM 30.5-Maintenance of the Federal Catalog System § 101-30.500 Scope of subpart. This subpart prescribes...

41 CFR 101-30.505 - Assistance by Government suppliers.

Code of Federal Regulations, 2012 CFR

2012-07-01

... 41 Public Contracts and Property Management 2 2012-07-01 2012-07-01 false Assistance by Government suppliers. 101-30.505 Section 101-30.505 Public Contracts and Property Management Federal Property... CATALOG SYSTEM 30.5-Maintenance of the Federal Catalog System § 101-30.505 Assistance by Government...

VizieR Online Data Catalog: X-ray AGNs with Subaru/FMOS NIR observations (Suh+, 2015)

NASA Astrophysics Data System (ADS)

Suh, H.; Hasinger, G.; Steinhardt, C.; Silverman, J. D.; Schramm, M.

2016-03-01

We performed NIR spectroscopic observations for the AGN sources with the FMOS high-resolution spectrographs on the Subaru telescope; in J-short (0.92-1.12um), J-long (1.11-1.35um), H-short (1.40-1.60um), and H-long (1.60-1.80um) coverage with a spectral resolution of R~2200. The data span the 2012 Mar 25-2013 Oct 24 period. In addition to NIR spectra, we use existing optical spectroscopy (see section 3.2). (2 data files).

Sleep medicine education and knowledge among undergraduate dental students in Middle East universities.

PubMed

Talaat, Wael; AlRozzi, Balsam; Kawas, Sausan Al

2016-01-02

The aim of this study was to assess the undergraduate dental education in sleep medicine in Middle East universities as well as the students' knowledge in this field. A cross-sectional observational study was carried out during the period from September 2013 to April 2014.Two different questionnaires were used. A self-administered questionnaire and a cover letter were emailed and distributed to 51 randomly selected Middle East dental schools to gather information about their undergraduate sleep medicine education offered in the academic year 2012-2013.The second questionnaire was distributed to the fifth-year dental students in the 2nd Sharjah International Dental Student Conference in April 2014, to assess their knowledge on sleep medicine. A survey to assess knowledge of sleep medicine in medical education (Modified ASKME Survey) was used. Thirty-nine out of 51 (76%) responded to the first questionnaire. Out of the responding schools, only nine schools (23%) reported the inclusion of sleep medicine in their undergraduate curriculum. The total average hours dedicated to teaching sleep medicine in the responding dental schools was 1.2 hours. In the second questionnaire, 29.2% of the respondents were in the high score group, whereas 70.8% scored low in knowledge of sleep-related breathing disorders. Dental students in Middle East universities receive a weak level of sleep medicine education resulting in poor knowledge in this field.

Sleep medicine education and knowledge among undergraduate dental students in Middle East universities.

PubMed

Talaat, Wael; AlRozzi, Balsam; Kawas, Sausan Al

2016-05-01

The aim of this study was to assess the undergraduate dental education in sleep medicine in Middle East universities as well as the students' knowledge in this field. A cross-sectional observational study was carried out during the period from September 2013 to April 2014.Two different questionnaires were used. A self-administered questionnaire and a cover letter were emailed and distributed to 51 randomly selected Middle East dental schools to gather information about their undergraduate sleep medicine education offered in the academic year 2012-2013.The second questionnaire was distributed to the fifth-year dental students in the 2nd Sharjah International Dental Student Conference in April 2014, to assess their knowledge on sleep medicine. A survey to assess knowledge of sleep medicine in medical education (Modified ASKME Survey) was used. Thirty-nine out of 51 (76%) responded to the first questionnaire. Out of the responding schools, only nine schools (23%) reported the inclusion of sleep medicine in their undergraduate curriculum. The total average hours dedicated to teaching sleep medicine in the responding dental schools was 1.2 hours. In the second questionnaire, 29.2% of the respondents were in the high score group, whereas 70.8% scored low in knowledge of sleep-related breathing disorders. Dental students in Middle East universities receive a weak level of sleep medicine education resulting in poor knowledge in this field.

VizieR Online Data Catalog: Vilnius photometry near Sh 2-205 (Straizys+, 2016)

NASA Astrophysics Data System (ADS)

Straizys, V.; Cepas, V.; Boyle, R. P.; Zdanavicius, J.; Maskoliunas, M.; Kazlauskas, A.; Zdanavicius, K.; Cernis, K.

2016-04-01

Table 1 contains the results of photometry of 302 stars down to V=19.5mag in the Vilnius seven-color system in the vicinity of the dark cloud TGU H942 P7 and emission nebula Sh2-205. Photometric data are used to classify stars in spectral and luminosity classes. The identification numbers, coordinates, V magnitudes and six color indices in the Vilnius system, photometric two-dimensional spectral types (spectral and luminosity classes) are given. The identification numbers start from from 1001 to avoid confusion with the catalog of Cepas et al. (2013BaltA..22..243C, Cat. J/BaltA/22/223). The coordinates are from PPMXL catalog (Roeser et al. 2010AJ....139.2440R, Cat. I/317). Table 2 contains the list of 88 YSOs, identified using the Koenig & Leisawitz (2014ApJ...791..131K) classification scheme, which combines the WISE and 2MASS near- and mid-infrared colours. The identification number and W1, W2, W3, J, H, Ks magnitudes are from WISE All-sky Data Release (Cutri et al., 2012yCat.2311....0C, Cat. II/311). The types of identified YSOs are given. (2 data files).

Catalog of Computer Programs Used in Undergraduate Geological Education. Second Edition. Installment 4.

ERIC Educational Resources Information Center

Burger, H. Robert

1984-01-01

Describes 70 computer programs related to (1) structural geology; (2) sedimentology and stratigraphy; and (3) the environment, groundwater, glacial geology, and oceanography. Potential use(s), language, required hardware, and sources are included. (JM)

2011-12 National Postsecondary Student Aid Study (NPSAS:12): Student Financial Aid Estimates for 2011-12. First Look. NCES 2013-165

ERIC Educational Resources Information Center

Radwin, David; Wine, Jennifer; Siegel, Peter; Bryan, Michael

2013-01-01

This brief report presents selected findings about student financial aid during the 2011-12 academic year. These findings are based on data from the 2011-12 National Postsecondary Student Aid Study (NPSAS:12), a nationally representative sample survey of undergraduate and graduate students enrolled any time between July 1, 2011, and June 30, 2012,…

VizieR Online Data Catalog: Differential photometry of the EB* HATS551-027 (Zhou+, 2015)

NASA Astrophysics Data System (ADS)

Zhou, G.; Bayliss, D.; Hartman, J. D.; Rabus, M.; Bakos, G. A.; Jordan, A.; Brahm, R.; Penev, K.; Csubry, Z.; Mancini, L.; Espinoza, N.; de Val-Borro, M.; Bhatti, W.; Ciceri, S.; Henning, T.; Schmidt, B.; Murphy, S. J.; Butler, R. P.; Arriagada, P.; Shectman, S.; Crane, J.; Thompson, I.; Suc, V.; Noyes, R. W.

2017-11-01

The eclipses of HATS551-027 were first identified by observations from the HATSouth survey (Bakos et al. 2013PASP..125..154B). HATSouth is a global network of identical, fully robotic telescopes, providing continuous monitoring of selected 128 deg2 fields of the southern sky. A total of 16622 observations of HATS551-027 were obtained from HATSouth units HS-1, HS-2 in Chile, HS-3, HS-4 in Namibia, and HS-6 in Australia from 2009 September to 2010 September. Two secondary eclipses of HATS551-027 were observed by the Merope camera on 2-m Faulkes Telescope South (FTS), at Siding Spring Observatory, on 2012 December 12 and 2013 March 20. A near-complete primary eclipse of HATS551-027 was observed by the SITe#3 camera on the Swope 1 m telescope at Las Campanas Observatory, Chile, on 2013 February 26. (1 data file).

New GALEX UV Data Products At MAST For Stellar Astrophysics

NASA Astrophysics Data System (ADS)

Shiao, Bernie; Fleming, S. W.; Million, C.; Seibert, M.; Bianchi, L.; Thompson, R.; Tseng, S.; Adler, W. J.; Hubbard, M.; Levay, K.; Madore, B. F.; Martin, C. D.; Nieto-Santisteban, M. A.; Sahai, R.; Schiminovich, D.; White, R. L.; Wyder, T. K.

2014-01-01

The Galaxy Evolution Explorer (GALEX) mission ended in June 2013 after ten years in orbit. Its FUV and NUV microchannel plate detectors were used to conduct a variety of direct imaging and spectroscopic astronomical surveys with various depths and sky coverage, recording individual photon events with a time resolution of five thousandths of a second. Although the mission has ended, MAST is continuing to provide new data products as the mission transitions to a legacy archive. One product is the GCAT (Seibert et al., in prep), a catalog of GALEX sources across the entire GR6 data release that removes duplicate objects found in the GALEX MCAT. The GCAT defines "primary" NUV and FUV fluxes within the AIS and MIS surveys 40 million and 22 million sources, respectively), accounting for tile overlaps, and with visual inspection of every tile to flag artifacts and conduct other quality control checks. Another catalog of unique sources is that of Bianchi et al. (2013). Similar to the GCAT, their catalog produces a list of distinct GALEX sources in both the FUV and NUV from the AIS and MIS surveys, and includes data from GR7 (through the end of 2012). They have also cross-matched their sources with SDSS DR9, GSC-II, PanSTARRS, and 2MASS. We review access options for these catalogs, including updated matches between the GCAT and SDSS / Kepler available at MAST. In addition to these unique GALEX source catalogs, MAST will provide a database and software package that archives each of the ~1.5 trillion photon events detected over the lifetime of the mission. For the first time, users will be able to create calibrated lightcurves, intensity maps, and animated movies from any set of photons selected across any tile, and with specified aperture sizes, coordinates, and time steps. Users can access the data using either a python-based command-line software package, through a web interface at MAST, or (eventually) through CasJobs using direct SQL queries. We present some example GALEX lightcurves and images using this new data product to highlight just some of the possibilities available for users to mine the GALEX photon database, particularly with variable sources.

Extracurricular scientific production among medical students has increased in the past decade.

PubMed

Andersen, Sofie Bech; Østergaard, Lauge; Fosbøl, Philip Loldrup; Fosbøl, Emil Loldrup

2015-09-01

Undergraduate research among medical students is essential in the education of future physicians and scientists. This study aimed to evaluate the scientific yield of extracurricular undergraduate research among medical students. Medical students at the University of Copenhagen who completed an extracurricular research year between January 2004 and June 2013 were evaluated through a manual search in PubMed MEDLINE. The primary focus was the number of peer-reviewed, published articles. Of the 363 included students, 3.1% did their research in 2004-2005 compared with 46.5% in 2012-2013. After three years, 70.4% of the students had published a peer-reviewed article, and of all the 363 students, 36.5%, had published as a first author. In total, 87.7% had a medical specialty as their research area versus a surgical specialty. Most students were involved in cardiology (14.1%). Cardiology was also associated with the greatest scientific yield with a median number of 0.8 publications per year after the students concluded their undergraduate research period. Three or more years after concluding their undergraduate research, 32.8% of the students had continued with research in the context of a PhD programme. Overall, the number of medical students who engaged in extracurricular research followed an increasing trend, and more than two-thirds of these students published a peer-reviewed paper within three years. Cardiology was the most popular specialty and also the specialty with the greatest scientific yield. A third of the undergraduate research students continued doing research in the context of a PhD programme.

VizieR Online Data Catalog: Spitzer-CANDELS catalog within 5 deep fields (Ashby+, 2015)

NASA Astrophysics Data System (ADS)

Ashby, M. L. N.; Willner, S. P.; Fazio, G. G.; Dunlop, J. S.; Egami, E.; Faber, S. M.; Ferguson, H. C.; Grogin, N. A.; Hora, J. L.; Huang, J.-S.; Koekemoer, A. M.; Labbe, I.; Wang, Z.

2015-08-01

We chose to locate S-CANDELS inside the wider and shallower fields already covered by Spitzer Extended Deep Survey (SEDS), in regions that enjoy deep optical and NIR imaging from HST/CANDELS. These S-CANDELS fields are thus the Extended GOODS-south (aka the GEMS field, hereafter ECDFS; Rix et al. 2004ApJS..152..163R; Castellano et al. 2010A&A...511A..20C), the Extended GOODS-north (HDFN; Giavalisco et al. 2004, II/261; Wang et al. 2010, J/ApJS/187/251; Hathi et al. 2012ApJ...757...43H; Lin et al. 2012ApJ...756...71L), the UKIDSS UDS (aka the Subaru/XMM Deep Field, Ouchi et al. 2001ApJ...558L..83O; Lawrence et al. 2007, II/319), a narrow field within the EGS (Davis et al. 2007ApJ...660L...1D; Bielby et al. 2012A&A...545A..23B), and a strip within the UltraVista deep survey of the larger COSMOS field (Scoville et al. 2007ApJS..172...38S; McCracken et al. 2012, J/A+A/544/A156). The S-CANDELS observing strategy was designed to maximize the area covered to full depth within the CANDELS area. Each field was visited twice with six months separating the two visits. Table 1 lists the epochs for each field. All of the IRAC full-depth coverage is within the SEDS area (Ashby et al. 2013, J/ApJ/769/80), and almost all is within the area covered by HST for CANDELS. (6 data files).

VizieR Online Data Catalog: Line list for red giants in open clusters (Reddy+, 2015)

NASA Astrophysics Data System (ADS)

Reddy, A. B. S.; Giridhar, S.; Lambert, D. L.

2017-11-01

Observations were carried out during observing runs in 2011 May and November, 2012 November and 2013 March using the Robert G. Tull echelle spectrograph (Tull et al. 1995PASP..107..251T) at the coude focus of the 2.7m Harlan J. Smith telescope located at the McDonald Observatory. On all occasions we employed a 2048x2048 24μm pixel, backside-illuminated, anti-reflection coated CCD as a detector and the 52.67 grooves/mm echelle grating with exposures centred at 5060Å. (2 data files).

VizieR Online Data Catalog: The Chandra Source Catalog, Release 1.1 (Evans+ 2012)

NASA Astrophysics Data System (ADS)

Evans, I. N.; Primini, F. A.; Glotfelty, C. S.; Anderson, C. S.; Bonaventura, N. R.; Chen, J. C.; Davis, J. E.; Doe, S. M.; Evans, J. D.; Fabbiano, G.; Galle, E. C.; Gibbs, D. G.; Grier, J. D.; Hain, R. M.; Hall, D. M.; Harbo, P. N.; He, X.; Houck, J. C.; Karovska, M.; Kashyap, V. L.; Lauer, J.; McCollough, M. L.; McDowell, J. C.; Miller, J. B.; Mitschang, A. W.; Morgan, D. L.; Mossman, A. E.; Nichols, J. S.; Nowak, M. A.; Plummer, D. A.; Refsdal, B. L.; Rots, A. H.; Siemiginowska, A.; Sundheim, B. A.; Tibbetts, M. S.; van Stone, D. W.; Winkelman, S. L.; Zografou, P.

2014-01-01

This version of the catalog is release 1.1. It includes the information contained in release 1.0.1, plus point and compact source data extracted from HRC imaging observations, and catch-up ACIS observations released publicly prior to the end of 2009. (1 data file).

41 CFR 101-30.504 - Cataloging data from Defense Logistics Services Center (DLSC).

Code of Federal Regulations, 2014 CFR

2014-07-01

... 41 Public Contracts and Property Management 2 2014-07-01 2012-07-01 true Cataloging data from Defense Logistics Services Center (DLSC). 101-30.504 Section 101-30.504 Public Contracts and Property... data from Defense Logistics Services Center (DLSC). Upon receipt of cataloging data from civil agencies...

VizieR Online Data Catalog: Omega Cen candidates RAVE-selected (Fernandez-Trincado+, 2015)

NASA Astrophysics Data System (ADS)

Fernandez-Trincado, J. G.; Robin, A. C.; Vieira, K.; Moreno, E.; Bienayme, O.; Reyle, C.; Valenzuela, O.; Pichardo, B.; Robles-Valdez, F.; Martins, A. M. M.

2015-11-01

The sample was selected from the RAVE DR4 catalog (Kordopatis et al., 2013, Cat. III/272), which provides accurate radial velocities with typical errors of σRV~2km/s, and distances and individual abundances with errors of about 10-20%, determined for approximately 390000 relatively bright stars (9mag20 (algo_conv=0 was required, indicating that the pipeline converges, see Kordopatis et al., 2013, Cat. III/272). This cut allowed us to obtain precise radial velocity measurements, typically σRV<2km/s, in order to constraint the full space motion. The metallicity [Fe/H] distribution for giant stars within Omega Centauri spans more than a magnitude order, from -2.2dex<[Fe/H]<-0.7dex (Johnson & Pilachowski, 2010, Cat. J/ApJ/722/1373), therefore we allowed stars in our sample to be in this range of metallicity. (1 data file).

Compendium of student papers : 2012 undergraduate transportation scholars program.

DOT National Transportation Integrated Search

2013-05-01

This report is a compilation of research papers written by students participating in the 2012 Undergraduate : Transportation Scholars Program. The 10-week summer program, now in its 22nd year, provides : undergraduate students in Civil Engineering th...

VizieR Online Data Catalog: HSTPROMO. III. Dynamical distances (Watkins+, 2015)

NASA Astrophysics Data System (ADS)

Watkins, L. L.; van der Marel, R. P.; Bellini, A.; Anderson, J.

2016-02-01

For our analysis, we use the HST proper-motion (PM) catalogs described in Bellini et al. (Paper I, 2014, J/ApJ/797/115); based on archival HST images spanning 2002 to 2013. We augment these catalogs with line of sight (LOS) velocity data available in the literature. (2 data files).

VizieR Online Data Catalog: BVRI photometry of luminous stars in M31 and M33 (Martin+, 2017)

NASA Astrophysics Data System (ADS)

Martin, J. C.; Humphreys, R. M.

2017-11-01

Images were obtained of M31 and M33 using an Apogee U42 CCD Camera with a back-illuminated E2v CCD42-40 chip on the F/13 20-inch (0.51m) telescope at the University of Illinois Springfield Henry R. Barber Research Observatory near Pleasant Plains, IL. The images are 19.4*19.4 arc minutes squares with a pixel scale of 0.57 arcseconds per pixel. Images were exposed in four high-throughput broad-band filters manufactured by Astrodon: Johnson B and V, and Cousins R and I. The B-filter does not have the red-leak present in most Astrodon B-filers manufactured prior to 2013. Images were taken in V at every epoch except one in 2012. In 2012, many fields were also imaged in R. Imaging in the B-filter started in 2013, and imaging in the I-filter started in 2015. Table 1 gives a record of the 199 images of M31 and 77 images of M33. (5 data files).

English 341: Advanced Composition for Teachers

ERIC Educational Resources Information Center

Duffy, William

2013-01-01

English 341: Advanced Composition for Teachers is a three-credit undergraduate course for pre-service educators at Francis Marion University, a mid-size public university located in northeast South Carolina. According to the university catalog, students enrolled in English 341 "explore connections among writing, teaching, and learning as they…

Workbook for the Introduction to the Library.

ERIC Educational Resources Information Center

Rice, Sheila

To introduce undergraduate students to the library and to familiarize them with the various indexing systems and reference materials, the University of Michigan has produced this workbook designed specifically for their library. The information and exercises included cover physical layout, the card catalog, the Library of Congress Classification…

Compendium of student papers : 2013 undergraduate transportation scholars program.

DOT National Transportation Integrated Search

2013-11-01

This report is a compilation of research papers written by students participating in the 2013 Undergraduate Transportation Scholars Program. The 10-week summer program, now in its 23nd year, provides undergraduate students in Civil Engineering the op...

VizieR Online Data Catalog: Improved multi-band photometry from SERVS (Nyland+, 2017)

NASA Astrophysics Data System (ADS)

Nyland, K.; Lacy, M.; Sajina, A.; Pforr, J.; Farrah, D.; Wilson, G.; Surace, J.; Haussler, B.; Vaccari, M.; Jarvis, M.

2017-07-01

The Spitzer Extragalactic Representative Volume Survey (SERVS) sky footprint includes five well-studied astronomical deep fields with abundant multi-wavelength data spanning an area of ~18deg2 and a co-moving volume of ~0.8Gpc3. The five deep fields included in SERVS are the XMM-LSS field, Lockman Hole (LH), ELAIS-N1 (EN1), ELAIS-S1 (ES1), and Chandra Deep Field South (CDFS). SERVS provides NIR, post-cryogenic imaging in the 3.6 and 4.5um Spitzer/IRAC bands to a depth of ~2uJy. IRAC dual-band source catalogs generated using traditional catalog extraction methods are described in Mauduit+ (2012PASP..124..714M). The Spitzer IRAC data are complemented by ground-based NIR observations from the VISTA Deep Extragalactic Observations (VIDEO; Jarvis+ 2013MNRAS.428.1281J) survey in the south in the Z, Y, J, H, and Ks bands and UKIRT Infrared Deep Sky Survey (UKIDSS; Lawrence+ 2007, see II/319) in the north in the J and K bands. SERVS also provides substantial overlap with infrared data from SWIRE (Lonsdale+ 2003PASP..115..897L) and the Herschel Multitiered Extragalactic Survey (HerMES; Oliver+ 2012, VIII/95). As shown in Figure 1, one square degree of the XMM-LSS field overlaps with ground-based optical data from the Canada-France-Hawaii Telescope Legacy Survey Deep field 1 (CFHTLS-D1). The CFHTLS-D1 region is centered at RAJ2000=02:25:59, DEJ2000=-04:29:40 and includes imaging through the filter set u', g', r', i', and z'. Thus, in combination with the NIR data from SERVS and VIDEO that overlap with the CFHTLS-D1 region, multi-band imaging over a total of 12 bands is available. (2 data files).

VizieR Online Data Catalog: Blazars with γ-ray counterparts. II. (Massaro+, 2013)

NASA Astrophysics Data System (ADS)

Massaro, F.; D'Abrusco, R.; Paggi, A.; Masetti, N.; Giroletti, M.; Tosti, G.; Smith, H. A.; Funk, S.

2013-06-01

Our primary sample of unidentified γ-ray sources (UGSs) consists of all the sources for which no counterpart was assigned at low energies in the 2FGL or in the 2LAC (Nolan et al. 2012, Cat. J/ApJS/199/31; Ackermann et al. 2011, Cat. J/ApJ/743/171, respectively), for a total of 590 γ-ray objects. We considered and analyzed independently two subsamples of UGSs, distinguishing the 299 Fermi sources without any γ-ray analysis flags from the other 291 objects that have a warning in their γ-ray detection. The complete description of our association procedure together with the estimates of its efficiency and its completeness can be found in D'Abrusco et al. (Paper I, 2013, Cat. J/ApJS/206,12). (9 data files).

Stimulant medications for attention-deficit/hyperactivity disorder (ADHD) improve memory of emotional stimuli in ADHD-diagnosed college students.

PubMed

Maul, J; Advokat, C

2013-04-01

Stimulant medications do not improve the academic achievement of ADHD diagnosed undergraduates. One reason may be that stimulant-induced sympathetic arousal might impair memory. To test this hypothesis, we conducted a study between September 2011 and March 2012, to compare medicated (n=12) and non-medicated (n=11) ADHD diagnosed undergraduates, with non-ADHD students (n=12). All participants were presented with an audiovisual narrative that included an emotional segment, and answered questions about the story one week later. All groups remembered the emotional segment significantly better than the neutral segments. Non-medicated ADHD students recalled less of both segments than the medicated ADHD or non-ADHD groups, which did not differ from each other. Stimulants improved memory in ADHD students, and did not impair the relative retention of emotional, as opposed to neutral information. Stimulant-induced arousal cannot explain the academic deficit of ADHD undergraduates. Copyright © 2013 Elsevier Inc. All rights reserved.

The Milky Way Project: A Citizen Science Catalog of Infrared Bow Shock Nebulae

NASA Astrophysics Data System (ADS)

Dixon, Don; Jayasinghe, Tharindu; Povich, Matthew S.

2017-01-01

We present preliminary results from the first citizen-science search for infrared stellar-wind bow shock candidates. This search uses the Milky Way project, hosted by the Zooniverse, an online platform with over 1 million volunteer citizen scientists. Milky Way Project volunteers examine 77,000 randomly-distributed Spitzer image cutouts at varying zoom levels. Volunteers mark the infrared arc of potential bow shock candidates as well as the star likely driving the nebula. We produce lists of candidates from bow shocks flagged by multiple volunteers, which after merging and final visual review form the basis for our catalog. Comparing our new catalog to a recently-published catalog of 709 infrared bow shock candidates identified by a small team of (primarily undergraduate) researchers will allow us to assess the effectiveness of citizen science for this type of search and should yield a more complete catalog. Planned studies using these large catalogs will improve constraints on the mass-loss rates for the massive stars that create these bow shock nebulae. Mass-loss rates are highly uncertain but are a critical component of evolutionary models for massive stars. This work is supported by the National Science Foundation under grants CAREER-1454334, AST-1411851 (RUI) and AST-1412845.

Catalog of Computer Programs Used in Undergraduate Geology Education (Second Edition): Installment 3.

ERIC Educational Resources Information Center

Burger, H. Robert

1983-01-01

Presents annotated list of computer programs related to geophysics, geomorphology, paleontology, economic geology, petroleum geology, and miscellaneous topics. Entries include description, instructional use(s), programing language, and availability. Programs described in previous installments (found in SE 533 635 and 534 182) focused on…

76 FR 93 - Summer Undergraduate Research Fellowships (SURF) NIST Gaithersburg and Boulder Programs...

Federal Register 2010, 2011, 2012, 2013, 2014

2011-01-03

...: Catalog of Federal Domestic Assistance Name and Number: Measurement and Engineering Research and Standards... engineering sciences and, as the lead Federal agency for technology transfer, it provides a strong interface... enables the Center for Nanoscale Science and Technology (CNST), Engineering Laboratory (EL), Information...

"See" References for Authors' Names Revisited.

ERIC Educational Resources Information Center

Baer, Nadine L.; Johnson, Karl E.

The study reported in this paper was conducted to determine the need for "see" references for authors' names in library catalogs. Nine-item patron questionnaires were placed in the University of Rhode Island's main library. Over the course of six years, 160 questionnaires were completed, 47 by undergraduate students, 76 by graduate…

Catalog of earthquake hypocenters at Alaskan volcanoes: January 1 through December 31, 2012

USGS Publications Warehouse

Dixon, James P.; Stihler, Scott D.; Power, John A.; Haney, Matthew M.; Parker, Tom; Searcy, Cheryl; Prejean, Stephanie

2013-01-01

Between January 1 and December 31, 2012, the Alaska Volcano Observatory located 4,787 earthquakes, of which 4,211 occurred within 20 kilometers of the 33 volcanoes monitored by a seismograph network. There was significant seismic activity at Iliamna, Kanaga, and Little Sitkin volcanoes in 2012. Instrumentation highlights for this year include the implementation of the Advanced National Seismic System Quake Monitoring System hardware and software in February 2012 and the continuation of the American Recovery and Reinvestment Act work in the summer of 2012. The operational highlight was the removal of Mount Wrangell from the list of monitored volcanoes. This catalog includes hypocenters, magnitudes, and statistics of the earthquakes located in 2012 with the station parameters, velocity models, and other files used to locate these earthquakes.

VizieR Online Data Catalog: Fermi-LAT flaring gamma-ray sources from FAVA (Ackermann+, 2013)

NASA Astrophysics Data System (ADS)

Ackermann, M.; Ajello, M.; Albert, A.; Allafort, A.; Antolini, E.; Baldini, L.; Ballet, J.; Barbiellini, G.; Bastieri, D.; Bechtol, K.; Bellazzini, R.; Blandford, R. D.; Bloom, E. D.; Bonamente, E.; Bottacini, E.; Bouvier, A.; Brandt, T. J.; Bregeon, J.; Brigida, M.; Bruel, P.; Buehler, R.; Buson, S.; Caliandro, G. A.; Cameron, R. A.; Caraveo, P. A.; Cavazzuti, E.; Cecchi, C.; Charles, E.; Chekhtman, A.; Cheung, C. C.; Chiang, J.; Chiaro, G.; Ciprini, S.; Claus, R.; Cohen-Tanugi, J.; Conrad, J.; Cutini, S.; Dalton, M.; D'Ammando, F.; de Angelis, A.; de Palma, F.; Dermer, C. D.; di Venere, L.; Drell, P. S.; Drlica-Wagner, A.; Favuzzi, C.; Fegan, S. J.; Ferrara, E. C.; Focke, W. B.; Franckowiak, A.; Fukazawa, Y.; Funk, S.; Fusco, P.; Gargano, F.; Gasparrini, D.; Germani, S.; Giglietto, N.; Giordano, F.; Giroletti, M.; Glanzman, T.; Godfrey, G.; Grenier, I. A.; Grondin, M.-H.; Grove, J. E.; Guiriec, S.; Hadasch, D.; Hanabata, Y.; Harding, A. K.; Hayashida, M.; Hays, E.; Hewitt, J.; Hill, A. B.; Horan, D.; Hou, X.; Hughes, R. E.; Inoue, Y.; Jackson, M. S.; Jogler, T.; Johannesson, G.; Johnson, W. N.; Kamae, T.; Kataoka, J.; Kawano, T.; Knodlseder, J.; Kuss, M.; Lande, J.; Larsson, S.; Latronico, L.; Lemoine-Goumard, M.; Longo, F.; Loparco, F.; Lott, B.; Lovellette, M. N.; Lubrano, P.; Mayer, M.; Mazziotta, M. N.; McEnery, J. E.; Michelson, P. F.; Mitthumsiri, W.; Mizuno, T.; Monte, C.; Monzani, M. E.; Morselli, A.; Moskalenko, I. V.; Murgia, S.; Nemmen, R.; Nuss, E.; Ohsugi, T.; Okumura, A.; Omodei, N.; Orienti, M.; Orlando, E.; Ormes, J. F.; Paneque, D.; Panetta, J. H.; Perkins, J. S.; Pesce-Rollins, M.; Piron, F.; Pivato, G.; Porter, T. A.; Raino, S.; Rando, R.; Razzano, M.; Reimer, A.; Reimer, O.; Romoli, C.; Roth, M.; Sanchez-Conde, M.; Scargle, J. D.; Schulz, A.; Sgro, C.; Siskind, E. J.; Spandre, G.; Spinelli, P.; Suson, D. J.; Takahashi, H.; Takeuchi, Y.; Thayer, J. G.; Thayer, J. B.; Thompson, D. J.; Tibaldo, L.; Tinivella, M.; Torres, D. F.; Tosti, G.; Troja, E.; Tronconi, V.; Usher, T. L.; Vandenbroucke, J.; Vasileiou, V.; Vianello, G.; Vitale, V.; Winer, B. L.; Wood, K. S.; Wood, M.; Yang, Z.

2015-01-01

We applied FAVA (Fermi All-sky Variability Analysis) to the first 47 months of Fermi/LAT observations (2008 August 4 to 2012 July 16 UTC), in weekly time intervals. The total number of weeks is 206. We considered two ranges of gamma-ray energy, E>100MeV and E>800MeV, to increase the sensitivity for spectrally soft and hard flares, respectively. We generate measured and expected count maps with a resolution of 0.25deg2 per pixel. We found LAT counterparts for 192 of the 215 FAVA sources. Most of the associated sources, 177, are AGNs. (2 data files).

VizieR Online Data Catalog: Brown dwarf surface gravities with Keck/NIRSPEC (Martin , 2017)

NASA Astrophysics Data System (ADS)

Martin, E. C.; Mace, G. N.; McLean, I. S.; Logsdon, S. E.; Rice, E. L.; Kirkpatrick, J. D.; Burgasser, A. J.; McGovern, M. R.; Prato, L.

2017-10-01

In this paper, we follow up on prior NIR spectroscopy by our group and use a modified Allers & Liu (A13, 2013ApJ...772...79A) method to determine surface gravities for 228 M, L, and T dwarfs. We present medium-resolution (R~20000) J-band spectra of 85 M dwarfs, 92 L dwarfs, and 51 T dwarfs obtained as part of the Keck NIRSPEC Brown Dwarf Spectroscopic Survey (BDSS). Ninety-seven spectra were published previously in McLean+ (2003ApJ...596..561M), Burgasser+ (2003ApJ...592.1186B), McGovern+ (2004ApJ...600.1020M), Rice+ (2010ApJS..186...63R), Kirkpatrick+ (2010, J/ApJS/190/100), Luhman (2012ARA&A..50...65L), Thompson+ (2013PASP..125..809T), Mace+ (2013, J/ApJS/205/6), Mace+ (2013ApJ...777...36M), and Kirkpatrick+ (2014, J/ApJ/783/122), and the remaining 131 are presented here for the first time. Observation information (spanning 1999 Apr to 2015 Mar) for all of the targets in our sample is listed in Table 1. (4 data files).

VizieR Online Data Catalog: Fermi LAT second source catalog (2FGL) (Nolan+, 2012)

NASA Astrophysics Data System (ADS)

Nolan, P. L.; Abdo, A. A.; Ackermann, M.; Ajello, M.; Allafort, A.; Antolini, E.; Atwood, W. B.; Axelsson, M.; Baldini, L.; Ballet, J.; Barbiellini, G.; Bastieri, D.; Bechtol, K.; Belfiore, A.; Bellazzini, R.; Berenji, B.; Bignami, G. F.; Blandford, R. D.; Bloom, E. D.; Bonamente, E.; Bonnell, J.; Borgland, A. W.; Bottacini, E.; Bouvier, A.; Brandt, T. J.; Bregeon, J.; Brigida, M.; Bruel, P.; Buehler, R.; Burnett, T. H.; Buson, S.; Caliandro, G. A.; Cameron, R. A.; Campana, R.; Canadas, B.; Cannon, A.; Caraveo, P. A.; Casandjian, J. M.; Cavazzuti, E.; Ceccanti, M.; Cecchi, C.; Celik, O.; Charles, E.; Chekhtman, A.; Cheung, C. C.; Chiang, J.; Chipaux, R.; Ciprini, S.; Claus, R.; Cohen-Tanugi, J.; Cominsky, L. R.; Conrad, J.; Corbet, R.; Cutini, S.; D'Ammando, F.; Davis, D. S.; de Angelis, A.; Decesar, M. E.; Deklotz, M.; de Luca A.; den Hartog, P. R.; de Palma, F.; Dermer, C. D.; Digel, S. W.; Do Couto, E. Silva E.; Drell, P. S.; Drlica-Wagner, A.; Dubois, R.; Dumora, D.; Enoto, T.; Escande, L.; Fabiani, D.; Falletti, L.; Favuzzi, C.; Fegan, S. J.; Ferrara, E. C.; Focke, W. B.; Fortin, P.; Frailis, M.; Fukazawa, Y.; Funk, S.; Fusco, P.; Gargano, F.; Gasparrini, D.; Gehrels, N.; Germani, S.; Giebels, B.; Giglietto, N.; Giommi, P.; Giordano, F.; Giroletti, M.; Glanzman, T.; Godfrey, G.; Grenier, I. A.; Grondin, M.-H.; Grove, J. E.; Guillemot, L.; Guiriec, S.; Gustafsson, M.; Hadasch, D.; Hanabata, Y.; Harding, A. K.; Hayashida, M.; Hays, E.; Hill, A. B.; Horan, D.; Hou, X.; Hughes, R. E.; Iafrate, G.; Itoh, R.; Johannesson, G.; Johnson, R. P.; Johnson, T. E.; Johnson, A. S.; Johnson, T. J.; Kamae, T.; Katagiri, H.; Kataoka, J.; Katsuta, J.; Kawai, N.; Kerr, M.; Knodlseder, J.; Kocevski, D.; Kuss, M.; Lande, J.; Landriu, D.; Latronico, L.; Lemoine-Goumard, M.; Lionetto, A. M.; Llena Garde, M.; Longo, F.; Loparco, F.; Lott, B.; Lovellette, M. N.; Lubrano, P.; Madejski, G. M.; Marelli, M.; Massaro, E.; Mazziotta, M. N.; McConville, W.; McEnery, J. E.; Mehault, J.; Michelson, P. F.; Minuti, M.; Mitthumsiri, W.; Mizuno, T.; Moiseev, A. A.; Mongelli, M.; Monte, C.; Monzani, M. E.; Morselli, A.; Moskalenko, I. V.; Murgia, S.; Nakamori, T.; Naumann-God, O. M.; Norris, J. P.; Nuss, E.; Nymark, T.; Ohno, M.; Ohsugi, T.; Okumura, A.; Omodei, N.; Orlando, E.; Ormes, J. F.; Ozaki, M.; Paneque, D.; Panetta, J. H.; Parent, D.; Perkins, J. S.; Pesce-Rollins, M.; Pierbattista, M.; Pinchera, M.; Piron, F.; Pivato, G.; Porter, T. A.; Racusin, J. L.; Raino, S.; Rando, R.; Razzano, M.; Razzaque, S.; Reimer, A.; Reimer, O.; Reposeur, T.; Ritz, S.; Rochester, L. S.; Romani, R. W.; Roth, M.; Rousseau, R.; Ryde, F.; Sadrozinski, H. F.-W.; Salvetti, D.; Sanchez, D. A.; Saz Parkinson, P. M.; Sbarra, C.; Scargle, J. D.; Schalk, T. L.; Sgro, C.; Shaw, M. S.; Shrader, C.; Siskind, E. J.; Smith, D. A.; Spandre, G.; Spinelli, P.; Stephens, T. E.; Strickman, M. S.; Suson, D. J.; Tajima, H.; Takahashi, H.; Takahashi, T.; Tanaka, T.; Thayer, J. G.; Thayer, J. B.; Thompson, D. J.; Tibaldo, L.; Tibolla, O.; Tinebra, F.; Tinivella, M.; Torres, D. F.; Tosti, G.; Troja, E.; Uchiyama, Y.; Vandenbroucke, J.; van Etten, A.; van Klaveren, B.; Vasileiou, V.; Vianello, G.; Vitale, V.; Waite, A. P.; Wallace, E.; Wang, P.; Werner, M.; Winer, B. L.; Wood, D. L.; Wood, K. S.; Wood, M.; Yang, Z.; Zimmer, S.

2012-06-01

This paper presents a catalog of high-energy γ-ray sources detected, in the 100MeV-100GeV energy range, in the first two years of the Fermi Gamma-ray Space Telescope mission by the Large Area Telescope (LAT), during the period 2008 August 4 (15:43 UTC)-2010 August 1 (01:17 UTC). (4 data files).

Updating Hawaii Seismicity Catalogs with Systematic Relocations and Subspace Detectors

NASA Astrophysics Data System (ADS)

Okubo, P.; Benz, H.; Matoza, R. S.; Thelen, W. A.

2015-12-01

We continue the systematic relocation of seismicity recorded in Hawai`i by the United States Geological Survey's (USGS) Hawaiian Volcano Observatory (HVO), with interests in adding to the products derived from the relocated seismicity catalogs published by Matoza et al., (2013, 2014). Another goal of this effort is updating the systematically relocated HVO catalog since 2009, when earthquake cataloging at HVO was migrated to the USGS Advanced National Seismic System Quake Management Software (AQMS) systems. To complement the relocation analyses of the catalogs generated from traditional STA/LTA event-triggered and analyst-reviewed approaches, we are also experimenting with subspace detection of events at Kilauea as a means to augment AQMS procedures for cataloging seismicity to lower magnitudes and during episodes of elevated volcanic activity. Our earlier catalog relocations have demonstrated the ability to define correlated or repeating families of earthquakes and provide more detailed definition of seismogenic structures, as well as the capability for improved automatic identification of diverse volcanic seismic sources. Subspace detectors have been successfully applied to cataloging seismicity in situations of low seismic signal-to-noise and have significantly increased catalog sensitivity to lower magnitude thresholds. We anticipate similar improvements using event subspace detections and cataloging of volcanic seismicity that include improved discrimination among not only evolving earthquake sequences but also diverse volcanic seismic source processes. Matoza et al., 2013, Systematic relocation of seismicity on Hawai`i Island from 1992 to 2009 using waveform cross correlation and cluster analysis, J. Geophys. Res., 118, 2275-2288, doi:10.1002/jgrb.580189 Matoza et al., 2014, High-precision relocation of long-period events beneath the summit region of Kīlauea Volcano, Hawai`i, from 1986 to 2009, Geophys. Res. Lett., 41, 3413-3421, doi:10.1002/2014GL059819

VizieR Online Data Catalog: Redshift survey of ALMA-identified SMGs in ECDFS (Danielson+, 2017)

NASA Astrophysics Data System (ADS)

Danielson, A. L. R.; Swinbank, A. M.; Smail, I.; Simpson, J. M.; Casey, C. M.; Chapman, S. C.; da Cunha, E.; Hodge, J. A.; Walter, F.; Wardlow, J. L.; Alexander, D. M.; Brandt, W. N.; De Breuck, C.; Coppin, K. E. K.; Dannerbauer, H.; Dickinson, M.; Edge, A. C.; Gawiser, E.; Ivison, R. J.; Karim, A.; Kovacs, A.; Lutz, D.; Menten, K.; Schinnerer, E.; Weiss, A.; van der Werf, P.

2017-11-01

The 870um LESS survey (Weiss+ 2009, J/ApJ/707/1201) was undertaken using the LABOCA camera on APEX, covering an area of 0.5°x0.5° centered on the ECDFS. Follow-up observations of the LESS sources were carried out with ALMA (Hodge+ 2013, J/ApJ/768/91). In summary, observations for each source were taken between 2011 October and November in the Cycle 0 Project #2011.1.00294.S. To search for spectroscopic redshifts, we initiated an observing campaign using the the FOcal Reducer and low dispersion Spectrograph (FORS2) and VIsible MultiObject Spectrograph (VIMOS) on VLT (program 183.A-0666), but to supplement these observations, we also obtained observations with XSHOOTER on VLT (program 090.A-0927(A) from 2012 December 7-10), the Gemini Near-Infrared Spectrograph (GNIRS; program GN-2012B-Q-90) and the Multi-Object Spectrometer for Infra-Red Exploration (MOSFIRE) on the Keck I telescope (2012B_H251M, 2013BU039M, and 2013BN114M), all of which cover the near-infrared. As part of a spectroscopic campaign targeting Herschel-selected galaxies in the ECDFS, ALESS submillimeter galaxies (SMGs) were included on DEep Imaging Multi-Object Spectrograph (DEIMOS) slit masks on Keck II (program 2012B_H251). In total, we observed 109 out of the 131 ALESS SMGs in the combined main and supp samples. Spectroscopic redshifts for two of our SMGs, ALESS61.1 and ALESS65.1, were determined from serendipitous detections of the [CII]λ158um line in the ALMA band. See section 2.7. (2 data files).

The Ultraviolet Sky: final catalogs of unique UV sources from GALEX, and characterization of the UV-emitting sources across the sky, and of the Milky Way extinction

NASA Astrophysics Data System (ADS)

Bianchi, Luciana; Conti, A.; Shiao, B.; Keller, G. R.; Thilker, D. A.

2014-01-01

The legacy of the Galaxy Evolution Explorer (GALEX), which imaged the sky at Ultraviolet (UV) wavelengths for about 9 years, is its unprecedented database with more than 200 million source measurements in far-UV (FUV) and near-UV (NUV), as well as wide-field imaging of extended objects. GALEX's data, the first substantial sky surveys at UV wavelengths, offer an unprecedented view of the sky and a unique opportunity for an unbiased characterization of several classes of astrophysical objects, such as hot stars, QSOs at red-shift about 1, UV-peculiar QSOs, star-forming galaxies, among others. Bianchi et al. (2013, J. Adv. Space Res. (2013), DOI: http://dx.doi.org/10.1016/j.asr.2013.07.045) have constructed final catalogs of UV sources, with homogeneous quality, eliminating duplicate measurements of the same source ('unique' source catalogs), and excluding rim artifacts and bad photometry. The catalogs are constructed improving on the recipe of Bianchi et al. 2011 (MNRAS, 411, 2770, which presented the earlier version of these catalogs) and include all data for the major surveys, AIS and MIS. Considering the fields where both FUV and NUV detectors were exposed, the catalogs contain about 71 and 16.6 million unique sources respectively. We show several maps illustrating the content of UV sources across the sky, globally, and separately for bright/faint, hot, stellar/extragalactic objects. We matched the UV-source catalogs with optical-IR data from the SDSS, GSC2, 2MASS surveys. We are also in the process of matching the catalogs with preliminary PanSTARRS1 (PS1) 3pi survey photometry which already provides twice the sky coverage of SDSS, at slightly fainter magnitude limits. The sources' SED from FUV to optical wavelengths enables classification, derivation of the object physical parameters, and ultimately also a map of the Milky Way extinction. The catalogs will be available on MAST, Vizier (where the previous version already is), and in reduced form (for agile downloading), with related tools, from the author web site " http://dolomiti.pha.jhu.edu/uvsky "

Catalog of Computer Programs Used in Undergraduate Geological Education, Second Edition: Installment 2.

ERIC Educational Resources Information Center

Burger, H. Robert

1983-01-01

Part 1 (SE 533 635) presented programs for use in mineralogy, petrology, and geochemistry. This part presents an annotated list of 64 additional programs, focusing on introductory geology, mapping, and statistical packages for geological analyses. A brief description, source, suggested use(s), programing language, and other information are…

Discovery of "Escherichia coli" CRISPR Sequences in an Undergraduate Laboratory

ERIC Educational Resources Information Center

Militello, Kevin T.; Lazatin, Justine C.

2017-01-01

Clustered regularly interspaced short palindromic repeats (CRISPRs) represent a novel type of adaptive immune system found in eubacteria and archaebacteria. CRISPRs have recently generated a lot of attention due to their unique ability to catalog foreign nucleic acids, their ability to destroy foreign nucleic acids in a mechanism that shares some…

The Status of Econometrics in the Economics Major: A Survey

ERIC Educational Resources Information Center

Johnson, Bruce K.; Perry, John J.; Petkus, Marie

2012-01-01

In this article, the authors describe the place of econometrics in undergraduate economics curricula in all American colleges and universities that offer economics majors as listed in the "U.S. News & World Report" "Best Colleges 2010" guide ("U.S. News & World Report" 2009). Data come from online catalogs, departmental Web sites, and online…

Expanding Perspectives of Feminism in the Composition Classroom

ERIC Educational Resources Information Center

Masterson, Kelly

2016-01-01

English 3060J: Women and Writing, is designed as a junior-level composition course for both majors and non-majors and is one of four courses from which students may choose to fulfill their junior composition requirement at a medium-sized liberal arts public university with approximately 16,700 undergraduates. The course catalog describes English…

VizieR Online Data Catalog: He abundances in M30 and NGC 6397 (Mucciarelli+, 2014)

NASA Astrophysics Data System (ADS)

Mucciarelli, A.; Lovisi, L.; Lanzoni, B.; Ferraro, F. R.

2017-06-01

In this work we analyzed a set of high-resolution spectra acquired with the multi-object spectrograph FLAMES in the MEDUSA/GIRAFFE mode at the Very Large Telescope of the European Southern Observatory (ESO). The spectra are part of a data set secured within a project aimed at studying the general properties of blue straggler stars (Ferraro et al. 2006ApJ...647L..53F, 2009Natur.462.1028F, 2012Natur.492..393F; Lovisi et al. 2012, J/ApJ/754/91; 2013, J/ApJ/772/148). The employed GIRAFFE grating is HR5A (4340-4587 Å, with a spectral resolution of ~18000), suitable to sample the He I line at 4471.5 Å. Spectra have been reduced with the standard ESO FLAMES pipeline. Six exposures of 45 minutes each have been secured in each cluster. (1 data file).

VizieR Online Data Catalog: LAMOST quasar survey: quasar properties from the DR1 (Ai+, 2016)

NASA Astrophysics Data System (ADS)

Ai, Y. L.; Wu, X.-B.; Yang, J.; Yang, Q.; Wang, F.; Guo, R.; Zuo, W.; Dong, X.; Zhang, Y.-X.; Yuan, H.-L.; Song, Y.-H.; Wang, J.; Dong, X.; Yang, M.; Wu, H.; Shen, S.-Y.; Shi, J.-R.; He, B.-L.; Lei, Y.-J.; Li, Y.-B.; Luo, A.-L.; Zhao, Y.-H.; Zhang, H.-T.

2018-03-01

LAMOST began a pilot survey in 2011 October and a regular survey in 2012 September. The regular survey, carried out over five to six years, has two major components: the LAMOST Experiment for Galactic Understanding and Exploration (LEGUE) and the LAMOST Extragalactic Survey (LEGAS; Zhao et al. 2012RAA....12..723Z). LEGAS only uses a small part of the available observing time due to the limitations of the LAMOST site, especially the bright sky background and poor seeing. The first data release (DR1) contains spectra taken before 2013 June (Luo et al. 2015, Cat. V/146). In this paper we present the results of the quasar survey from LEGAS. LAMOST LEGAS spectroscopic observations are taken in a series of at least three 30 minute exposures. There are 70290 quasar candidates observed, with 82625 spectra in DR1. (2 data files).

VizieR Online Data Catalog: Transition probabilities in TeII + TeIII spectra (Zhang+, 2013)

NASA Astrophysics Data System (ADS)

Zhang, W.; Palmeri, P.; Quinet, P.; Biemont, E.

2013-02-01

Computed weighted oscillator strengths (loggf) and transition probabilities (gA) for Te II (Table 8) and Te III (Table 9). Transitions with wavelengths <1um, loggf>-1 and CF>0.05 are only quoted. Air wavelengths are given above 200 nm. In Table 8 the levels are taken from Kamida et al (Kamida, A., Ralchenko, Yu., Reader, J., and NIST ASD Team (2012). NIST Atomic Spectra Database (ver. 5.0), [Online]. Available: http://physics.nist.gov/asd [2012, September 20]. National Institute of Standards and Technology, Gaithersburg, MD.). In Table 9 the levels are those given in Tauheed & Naz (Tauheed, A., Naz, A. 2011, Journal of the Korean Physical Society 59, 2910) with the exceptions of the 5p6p levels which were taken from Kramida et al. The wavelengths were computed from the experimental levels of Kramida et al and Tauheed & Naz. (2 data files).

VizieR Online Data Catalog: Elemental abundances of solar sibling candidates (Ramirez+, 2014)

NASA Astrophysics Data System (ADS)

Ramirez, I.; Bajkova, A. T.; Bobylev, V. V.; Roederer, I. U.; Lambert, D. L.; Endl, M.; Cochran, W. D.; MacQueen, P. J.; Wittenmyer, R. A.

2017-06-01

We used the Tull coude spectrograph on the 2.7 m Harlan J. Smith Telescope at McDonald Observatory (Tull et al. 1995PASP..107..251T) to observe most of our targets (23). All but three of them were observed in 2012 December; the others were observed in 2013 March. The rest of our targets (seven) have too-low declinations to be observed from McDonald Observatory. Instead, they were observed using the Magellan Inamori Kyocera Echelle (MIKE) spectrograph on the 6.5 m Telescope at Las Campanas Observatory (Bernstein et al. 2003SPIE.4841.1694B) in 2013 April. Slit sizes were chosen so that the spectral resolution of the data is about 60000 in the visible part of the spectrum. We targeted a S/N per pixel of at least 200 at 6000 Å. Only one of our targets (HD 46100) has a significantly lower S/N spectrum. (2 data files).

VizieR Online Data Catalog: BCG high radio-frequency properties (Hogan+, 2015)

NASA Astrophysics Data System (ADS)

Hogan, M. T.; Edge, A. C.; Geach, J. E.; Grainge, K. J. B.; Hlavacek-Larrondo, J.; Hovatta, T.; Karim, A.; McNamara, B. R.; Rumsey, C.; Russell, H. R.; Salome, P.; Aller, H. D.; Aller, M. F.; Benford, D. J.; Fabian, A. C.; Readhead, A. C. S.; Sadler, E. M.; Saunders, R. D. E.

2016-02-01

The sample of sources chosen for this study were selected primarily from Hogan et al. (2015. Cat. J/MNRAS/453/1201) as having the brightest (>10mJy at 5GHz), flat-spectrum cores (α<0.5) so a detection above 100GHz was possible. The H15a sample covers an all-sky, X-ray flux-limited sample of over 700 clusters as outlined above, but the number of sources matching these flux and index cuts is relatively small (<30 or <4 per cent). To increase the target list we added seven bright (>50mJy at 5GHz) sources either in fainter clusters and/or clusters misidentified until now. We obtained data from three epochs, using GISMO to observe 29, 24 and 17 sources in 2012 April, November and 2013 April observing runs, respectively, with as many source overlaps between runs as possible 23 sources were observed at 90GHz using the CARMA interferometer in D-array between 2012 May 21-June 15, of which 20 overlap with our GISMO sources. We used the AMI-LA to observe 17 of our sources, with each target visited either two or three times in 2012. Five of the sources in our sample have been monitored as part of this OVRO monitoring campaign. An additional 11 BCGs that were identified from this work as having strong high radio-frequency emission, have been included within the dynamic queue since 2013 January, allowing regular (typically every 10d) observations for these sources. Observations were made using the SCUBA-2 instrument (Holland et al. 2013) on the James Clerk Maxwell Telescope (JCMT) as part of a poor weather programme (JCMT weather Bands 4 and 5, {tau}225GHz=0.15-0.3) as part of Canadian and UK projects (M12AC15, M12BC18, M12BU38, M13AC16 and M13AU38) between 2012 February and 2013 July. (4 data files).

VizieR Online Data Catalog: Spatial structure of young stellar clusters. I. (Kuhn+, 2014)

NASA Astrophysics Data System (ADS)

Kuhn, M. A.; Feigelson, E. D.; Getman, K. V.; Baddeley, A. J.; Broos, P. S.; Sills, A.; Bate, M. R.; Povich, M. S.; Luhman, K. L.; Busk, H. A.; Naylor, T.; King, R. R.

2015-07-01

The regions included in this study, listed in Table 1, are nearby sites of high-mass star formation that are included in the MYStIX sample (Feigelson et al. 2013ApJS..209...26F). These regions are covered in the near-IR by the UKIRT Infrared Deep Sky Survey (King et al. 2013, J/ApJS/209/28) or Two-Micron All Sky Survey (Skrutskie et al. 2006, VII/233), in the mid-IR by Spitzer IRAC observations (Kuhn et al. 2013, J/ApJS/209/29), and in the X-ray by the ACIS-I array on the Chandra X-Ray Observatory in the 0.5-8.0keV band (Kuhn et al. 2013, J/ApJS/209/27; Townsley et al. 2014, J/ApJS/213/1). Other sources to produce multiwavelength catalogs are described in section 2. The multiwavelength point-source catalogs are combined with a list of spectroscopic OB stars from the literature, and sources are classified probabilistically to obtain a list of MYStIX Probable Complex Members (MPCMs) (Broos et al. 2013, J/ApJS/209/32). (3 data files).

Implementation of a module to promote competency in adverse drug reaction reporting in undergraduate medical students.

PubMed

Tripathi, Raakhi Kaliprasad; Jalgaonkar, Sharmila Vinayak; Sarkate, Pankaj V; Rege, Nirmala Narayan

2016-10-01

Underreporting and poor quality of adverse drug reaction (ADR) reports pose a challenge for the Pharmacovigilance Program of India. A module to impart knowledge and skills of ADR reporting to MBBS students was developed and evaluated. The module consisted of (a) e-mailing an ADR narrative and online filling of the "suspected ADR reporting form" (SARF) and (b) a week later, practical on ADR reporting was conducted followed by online filling of SARF postpractical at 1 and 6 months. SARF was an 18-item form with a total score of 36. The module was implemented in the year 2012-2013. Feedback from students and faculty was taken using 15-item prevalidated feedback questionnaires. The module was modified based on the feedback and implemented for the subsequent batch in the year 2013-2014. The evaluation consisted of recording the number of students responding and the scores achieved. A total of 171 students in 2012-2013 batch and 179 in 2013-2014 batch participated. In the 2012-2013 batch, the number of students filling the SARF decreased from basal: 171; 1 month: 122; 6 months: 17. The average scores showed improvement from basal 16.2 (45%) to 26.4 (73%) at 1 month and to 27.3 (76%) at 6 months. For the 2013-2014 batch, the number ( n = 179) remained constant throughout and the average score progressively increased from basal 10.5 (30%) to 27.8 (77%) at 1 month and 30.3 (84%) at 6 months. This module improved the accuracy of filling SARF by students and this subsequently will led to better ADR reporting. Hence, this module can be used to inculcate better ADR reporting practices in budding physicians.

VizieR Online Data Catalog: Catalog of 316 K giant candidates (Rebull+, 2015)

NASA Astrophysics Data System (ADS)

Rebull, L. M.; Carlberg, J. K.; Gibbs, J. C.; Deeb, J. E.; Larsen, E.; Black, D. V.; Altepeter, S.; Bucksbee, E.; Cashen, S.; Clarke, M.; Datta, A.; Hodgson, E.; Lince, M.

2015-11-01

There are 82 targets published in de la Reza et al. (1997ApJ...482L..77D). There are 86 K giants reported in Carlberg et al. 2012 (cat. J/ApJ/757/109). We compiled 149 additional targets that have been identified either consistently or at one time as confirmed or possible Li-rich K giants, but not included in either the de la Reza et al. (1997ApJ...482L..77D) or the Carlberg et al. 2012 (cat. J/ApJ/757/109) samples. They include targets from Adamow et al. 2014 (cat. J/A+A/569/A55), Anthony-Twarog et al. (2013ApJ...767L..19A), Carney et al. (1998AJ....116.2984C), Carlberg et al. (2015ApJ...802....7C), Castilho et al. 2000 (cat. J/A+A/364/674), Drake et al. (2002AJ....123.2703D), Fekel & Watson (1998AJ....116.2466F), Hill & Pasquini (1999A&A...348L..21H), Jasniewicz et al. (1999A&A...342..831J), Kirby et al. (2012ApJ...752L..16K), Kraft et al. (1999ApJ...518L..53K), Kumar et al. (2011ApJ...730L..12K) and references therein, Liu et al. (2014ApJ...785...94L), Luck & Heiter 2007 (cat. J/AJ/133/2464), Martell & Shetrone (2013MNRAS.430..611M), Monaco et al. (2014A&A...564L...6M), Pilachowski et al. (2003AJ....125..794P), Ruchti et al. (2011ApJ...743..107R), Silva Aguirre et al. (2014ApJ...784L..16A), Smith et al. (1999ApJ...516L..73S), and Torres et al. (2000IAUS..198..320T). Our complete list of 316 targets with position, photometric, and abundance data appears in Table1. We obtained positions for these targets, most of which are quite bright in the optical, primarily from SIMBAD, though literature was consulted for fainter sources as required. Detailed notes on the sources we suspect are subject to source confusion appear in Table4. Table6 contains notes on the entire set of sources. (3 data files).

Jebels Awenat and Arkenu, Libya

NASA Image and Video Library

2018-02-22

In the far southeast corner of Libya, in the Libyan Desert, lie the uplifted massifs of Jebel Awenat and Jebel Arkenu. Both expose ancient Precambrian rocks, intruded by granites, and then overlain with sandstones. Folding and doming have produced these interesting shapes, rising above the surrounding sand sea. Presently, the area receives less than one inch of rain per year. Thousands of years ago, rainfall was more plentiful, and the Jebels were occupied by people, as attested by the numerous rock drawings. The images were acquired July 19, 2012, and July 31, 2013, cover an area of 66 by 67 kilometers, and are located at 22.1 degrees north, 24.8 degrees east. https://photojournal.jpl.nasa.gov/catalog/PIA22283

VizieR Online Data Catalog: Praesepe members masses (Khalaj+, 2013)

NASA Astrophysics Data System (ADS)

Khalaj, P.; Baumgardt, H.

2014-09-01

In this study, we combine data from the PPMXL catalogue (Roser et al., 2010AJ....139.2440R, Cat. I/317) with z magnitudes from SDSS DR9 (Ahn et al., 2012ApJS..203...21A, Cat. V/139). The PPMXL catalogue combines the USNO-B1.0 (Monet et al. 2003AJ....125..984M, Cat. I/284) and 2MASS catalogues (Skrutskie et al. 2006AJ....131.1163S, Cat. VII/233), yielding the largest collection of proper motions in the International Celestial Reference Frame to date (Roser et al., 2010AJ....139.2440R, Cat. I/317). Cat. J/A+A/531/A92). (1 data file).

VizieR Online Data Catalog: Parameters of 529 Kepler eclipsing binaries (Kjurkchieva+, 2017)

NASA Astrophysics Data System (ADS)

Kjurkchieva, D.; Vasileva, D.; Atanasova, T.

2017-11-01

We reviewed the Kepler eclipsing binary catalog (Prsa et al. 2011, Cat. J/AJ/141/83; Slawson et al. 2011, Cat. J/AJ/142/160; Matijevic et al. 2012) to search for detached eclipsing binaries with eccentric orbits. (5 data files).

Use of research in undergraduate nursing students' theses: A mixed methods study.

PubMed

Nordsteien, Anita; Horntvedt, May-Elin T; Syse, Jonn

2017-09-01

Health care personnel are expected to be familiar with evidence-based practice (EBP). Asking clinical questions, conducting systematic literature searches and conducting critical appraisal of research findings have been some of the barriers to EBP. To improve undergraduate nurses' research skills, a collaborative library-faculty teaching intervention was established in 2012. The aim of this study was to evaluate how the collaborative library-faculty teaching intervention affected the nursing students' research skills when writing their final theses. Both quantitative and qualitative data collection and analysis were used. The study focused on a final year undergraduate nurse training programme in Norway. 194 theses submitted between 2013 and 2015 were collected and assessed. The students were exposed to the intervention for respectively one, two and three years during this period. Descriptive statistics were used to compare each year's output over the three-year period and to examine the frequency of the use of various databases, types of information and EBP-tools. Qualitative data was used to capture the students' reasoning behind their selection processes in their research. The research skills with regard to EBP have clearly improved over the three years. There was an increase in employing most EBP-tools and the justifications were connected to important EBP principles. The grades in the upper half of the grading scale increased from 66.7 to 82.1% over the period 2013 to 2015, and a correlation was found between grades and critical appraisal skills. The collaborative library-faculty teaching intervention employed has been successful in the promotion of nursing student research skills as far as the EBP principles are concerned. Writing a thesis in the undergraduate nursing programme is important to develop and practice these research skills. Copyright © 2017 Elsevier Ltd. All rights reserved.

Egyptian women in physics: Progress and challenges

NASA Astrophysics Data System (ADS)

Mohsen, M.; Hosni, Hala; Mohamed, Hadeer; Gadalla, Afaf; Kahil, Heba; Hashem, Hassan

2015-12-01

The present study shows a progressive increase in the number of female physicists as undergraduates and postgraduates in several governmental universities. For instance, in Ain Shams University, the percentage of women who selected physics as a major course of study increased from 7.2% in 2012 to 10.8% in 2013 and 15.7% in 2014. The study also provides the current gender distribution in the various positions among the teaching staff in seven governmental universities. The data supports the fact that female teaching assistants are increasing in these universities.

Integrating Sonography Training Into Undergraduate Medical Education: A Study of the Previous Exposure of One Institution's Incoming Residents.

PubMed

Day, James; Davis, Joshua; Riesenberg, Lee Ann; Heil, Daniel; Berg, Katherine; Davis, Robyn; Berg, Dale

2015-07-01

Sonography is a crucial and versatile tool within the field of medicine. Recent advancements in technology have led to increased use of point-of-care sonography. We designed a survey to assess prior point-of-care sonography training among incoming interns at an academic teaching hospital. In 2012 and 2013, we surveyed incoming interns (n = 154 and 145, respectively) regarding point-of-care sonography training received during medical school. The survey questions included formal didactic sessions, bedside instruction, and the use of simulation technology. One-fourth (26.3% in 2012 and 23.4% in 2013) of responding interns reported having never done an ultrasound scan at the bedside. In 2012 and 2013, 55.0% and 55.6% of respondents reported never having done an ultrasound scan in a simulation center, respectively. Interns agreed that sonography education should be provided during medical school. On average, interns disagreed with the statement that sonography should be taught in residency only. There was no significant difference in the sex or general previous experience with sonography across both intern classes. Point-of-care sonography is inconsistently taught in medical school. The interns in our study also thought that sonography education should begin in medical school, and sonography should be taught by using simulation and at the bedside. © 2015 by the American Institute of Ultrasound in Medicine.

Trends in Undergraduate Economics Degrees, 1991-2012

ERIC Educational Resources Information Center

Siegfried, John J.

2013-01-01

The 2007-10 growth spurt (18 percent over three years) in U.S. undergraduate economics degrees came to an abrupt end in 2011 and 2012. Degrees awarded grew less than one percent over the past two years.

VizieR Online Data Catalog: Catalog of strong MgII absorbers (Lawther+, 2012)

NASA Astrophysics Data System (ADS)

Lawther, D.; Paarup, T.; Schmidt, M.; Vestergaard, M.; Hjorth, J.; Malesani, D.

2012-08-01

Here we present a catalog of strong (rest equivalent width Wr> intervening Mg II absorbers in the SDSS Data Release 7 quasar catalog (2010AJ....139.2360S, Cat. VII/260). The intervening absorbers were found by a semi-automatic algorithm written in IDL - for details of the algorithm see section 2 of our paper. A subset of the absorbers have been visually inspected - see the MAN_OK flag in the catalog. The number of sightlines searched, tabulated by absorber redshift, i.e. g(z), is available as an ASCII table (for S/N>8 and S/N>15). All analysis in our paper is based on the SNR>8 coverage, and considers only sight-lines towards non-BAL quasars. Any questions regarding the catalog should be sent to Daniel Lawther (unclellama(at)gmail.com). (3 data files).

41 CFR 101-30.500 - Scope of subpart.

Code of Federal Regulations, 2014 CFR

2014-07-01

... 41 Public Contracts and Property Management 2 2014-07-01 2012-07-01 true Scope of subpart. 101-30... Regulations System FEDERAL PROPERTY MANAGEMENT REGULATIONS SUPPLY AND PROCUREMENT 30-FEDERAL CATALOG SYSTEM 30.5-Maintenance of the Federal Catalog System § 101-30.500 Scope of subpart. This subpart prescribes...

41 CFR 101-30.400 - Scope of subpart.

Code of Federal Regulations, 2014 CFR

2014-07-01

... 41 Public Contracts and Property Management 2 2014-07-01 2012-07-01 true Scope of subpart. 101-30... Regulations System FEDERAL PROPERTY MANAGEMENT REGULATIONS SUPPLY AND PROCUREMENT 30-FEDERAL CATALOG SYSTEM 30.4-Use of the Federal Catalog System § 101-30.400 Scope of subpart. This subpart prescribes the...

VizieR Online Data Catalog: Swift AGN and Cluster Survey (SACS). I. (Dai+, 2015)

NASA Astrophysics Data System (ADS)

Dai, X.; Griffin, R. D.; Kochanek, C. S.; Nugent, J. M.; Bregman, J. N.

2015-07-01

The Swift XRT observations of GRB fields were downloaded from the HEASARC website. This includes ~9yr of data through 2013 July 27. We matched the sources to the WISE all-sky catalog (see section 3.2). (5 data files).

VizieR Online Data Catalog: S4 1030+61 VLBA observations, 2009-2014 (Kravchenko+, 2016)

NASA Astrophysics Data System (ADS)

Kravchenko, E. V.; Kovalev, Y. Y.; Hovatta, T.; Ramakrishnan, V.

2018-02-01

The source S4 1030+61 was observed (code S2087E) with the VLBA of the National Radio Astronomy Observatory (NRAO) during four sessions: 2010-05-24, 2010-07-09, 2010-08-28 and 2010-10-18 (noted as 'epochs' below). We supplemented our analysis with the data obtained within the MOJAVE programme. Observations are done at 15.4GHz with VLBA at 10 epochs: 2009-06-25, 2009-12-26, 2010-12-24, 2011-04-11, 2011-05-26, 2011-07-15, 2012-01-02, 2012-03-27, 2012-11-11 and 2013-07-08. Public data (http://www.astro.caltech.edu/ovroblazars/) of S4 1030+61 observations within the OVRO 40-m Telescope monitoring programme were used in the analysis. Observations are done at 15GHz in a 3GHz bandwidth from 2008-06-20 to 2014-01-21 about twice per week. The γ-ray fluxes in the range 0.1-200GeV were obtained with the LAT onboard the space Fermi γ-ray observatory from 2008-08-04 to 2014-02-23. (3 data files).

4273π: Bioinformatics education on low cost ARM hardware

PubMed Central

2013-01-01

Background Teaching bioinformatics at universities is complicated by typical computer classroom settings. As well as running software locally and online, students should gain experience of systems administration. For a future career in biology or bioinformatics, the installation of software is a useful skill. We propose that this may be taught by running the course on GNU/Linux running on inexpensive Raspberry Pi computer hardware, for which students may be granted full administrator access. Results We release 4273π, an operating system image for Raspberry Pi based on Raspbian Linux. This includes minor customisations for classroom use and includes our Open Access bioinformatics course, 4273π Bioinformatics for Biologists. This is based on the final-year undergraduate module BL4273, run on Raspberry Pi computers at the University of St Andrews, Semester 1, academic year 2012–2013. Conclusions 4273π is a means to teach bioinformatics, including systems administration tasks, to undergraduates at low cost. PMID:23937194

4273π: bioinformatics education on low cost ARM hardware.

PubMed

Barker, Daniel; Ferrier, David Ek; Holland, Peter Wh; Mitchell, John Bo; Plaisier, Heleen; Ritchie, Michael G; Smart, Steven D

2013-08-12

Teaching bioinformatics at universities is complicated by typical computer classroom settings. As well as running software locally and online, students should gain experience of systems administration. For a future career in biology or bioinformatics, the installation of software is a useful skill. We propose that this may be taught by running the course on GNU/Linux running on inexpensive Raspberry Pi computer hardware, for which students may be granted full administrator access. We release 4273π, an operating system image for Raspberry Pi based on Raspbian Linux. This includes minor customisations for classroom use and includes our Open Access bioinformatics course, 4273π Bioinformatics for Biologists. This is based on the final-year undergraduate module BL4273, run on Raspberry Pi computers at the University of St Andrews, Semester 1, academic year 2012-2013. 4273π is a means to teach bioinformatics, including systems administration tasks, to undergraduates at low cost.

Key science issues in the central and eastern United States for the next version of the USGS National Seismic Hazard Maps

USGS Publications Warehouse

Peterson, M.D.; Mueller, C.S.

2011-01-01

The USGS National Seismic Hazard Maps are updated about every six years by incorporating newly vetted science on earthquakes and ground motions. The 2008 hazard maps for the central and eastern United States region (CEUS) were updated by using revised New Madrid and Charleston source models, an updated seismicity catalog and an estimate of magnitude uncertainties, a distribution of maximum magnitudes, and several new ground-motion prediction equations. The new models resulted in significant ground-motion changes at 5 Hz and 1 Hz spectral acceleration with 5% damping compared to the 2002 version of the hazard maps. The 2008 maps have now been incorporated into the 2009 NEHRP Recommended Provisions, the 2010 ASCE-7 Standard, and the 2012 International Building Code. The USGS is now planning the next update of the seismic hazard maps, which will be provided to the code committees in December 2013. Science issues that will be considered for introduction into the CEUS maps include: 1) updated recurrence models for New Madrid sources, including new geodetic models and magnitude estimates; 2) new earthquake sources and techniques considered in the 2010 model developed by the nuclear industry; 3) new NGA-East ground-motion models (currently under development); and 4) updated earthquake catalogs. We will hold a regional workshop in late 2011 or early 2012 to discuss these and other issues that will affect the seismic hazard evaluation in the CEUS.

VizieR Online Data Catalog: 1H 0323+342 rest frame optical spectrum with GHAO (Leon+, 2014)

NASA Astrophysics Data System (ADS)

Leon Tavares, J.; Kotilainen, J.; Chavushyan, V.; Anorve, C.; Puerari, I.; Cruz-Gonzalez, I.; Patino-Alvarez, V.; Anton, S.; Carraminana, A.; Carrasco, L.; Guichard, J.; Karhunen, K.; Olguin-Iglesias, A.; Sanghvi, J.; Valdes, J.

2017-05-01

Within the framework of a spectrophotometric monitoring program of bright γ-ray sources (Patino-Alvarez et al. 2013, Proc. Fermi Symposium, arXiv:1303.1893), we undertook spectroscopic observations of 1H 0323+342 using the Boller & Chivens long-slit spectrograph on the 2.1 m Guillermo Haro Astrophysical Observatory (GHAO) in Sonora, Mexico. The spectra were obtained under photometric weather conditions (2012 September 17, 2013 January 9, 2013 February 7 and 11) using a slit width of 2.5 arcsec. The spectral resolution was R=15 Å and R=7 Å (FWHM) for the low-resolution and intermediate-resolution spectra, respectively. The wavelength range for the three low-resolution spectra is 3800-7100 Å, and for one intermediate-resolution spectrum the wavelength range is 4300-5900 Å. The signal-to-noise ratio (S/N) was >40 in the continuum near H{Beta}. To enable a wavelength calibration, HeAr lamp spectra were taken after each object exposure. Spectrophotometric standard stars were observed every night (at least two per night) to enable flux calibration. (1 data file).

Trends in basic mathematical competencies of beginning undergraduates in Ireland, 2003-2013

NASA Astrophysics Data System (ADS)

Treacy, Páraic; Faulkner, Fiona

2015-11-01

Deficiencies in beginning undergraduate students' basic mathematical skills has been an issue of concern in higher education, particularly in the past 15 years. This issue has been tracked and analysed in a number of universities in Ireland and internationally through student scores recorded in mathematics diagnostic tests. Students beginning their science-based and technology-based undergraduate courses in the University of Limerick have had their basic mathematics skills tested without any prior warning through a 40 question diagnostic test during their initial service mathematics lecture since 1998. Data gathered through this diagnostic test have been recorded in a database kept at the university and explored to track trends in mathematical competency of these beginning undergraduates. This paper details findings surrounding an analysis of the database between 2003 and 2013, outlining changes in mathematical competencies of these beginning undergraduates in an attempt to determine reasons for such changes. The analysis found that the proportion of students tested through this diagnostic test that are predicted to be at risk of failing their service mathematics end-of-semester examinations has increased significantly between 2003 and 2013. Furthermore, when students' performance in secondary level mathematics was controlled, it was determined that the performance of beginning undergraduates in 2013 was statistically significantly below that of the performance of the beginning undergraduates recorded 10 years previously.

VizieR Online Data Catalog: 231 AGN candidates from the 2FGL catalog (Doert+, 2014)

NASA Astrophysics Data System (ADS)

Doert, M.; Errando, M.

2016-01-01

The second Fermi-LAT source catalog (2FGL; Nolan et al. 2012, cat. J/ApJS/199/31) is the deepest all-sky survey available in the gamma-ray band. It contains 1873 sources, of which 576 remain unassociated. The Large Area Telescope (LAT) on board the Fermi Gamma-ray Space Telescope started operations in 2008. In this work, machine-learning algorithms are used to identify unassociated sources in the 2FGL catalog with properties similar to gamma-ray-emitting Active Galactic Nuclei (AGN). This analysis finds 231 high-confidence AGN candidates (see Table3). (1 data file).

Taking it on the Road: Transferring Knowledge about Rhetoric and Writing across Curricula and Campuses

ERIC Educational Resources Information Center

Fishman, Jenn; Reiff, Mary Jo

2011-01-01

Since Fall 2004, the Undergraduate Catalog at the University of Tennessee-Knoxville has listed a two-part "Communicating through Writing" (WC) requirement, which includes two first-year composition courses and an upper-division course in one of thirty-five majors. Most students fulfill the former by enrolling in English 101 and 102, a…

A Revolution in the Education of Women. Ten Years of Continuing Education at Sarah Lawrence College.

ERIC Educational Resources Information Center

Richter, Melissa Lewis; Whipple, Jane Banks

The Sarah Lawrence Continuing Education Center provides educational opportunities for women who are not now in college, but who wish to continue their educations. This book is a publication about and a catalog for the Continuing Education Center. The Undergraduate Program is explained, as are procedures for admission, financial aid, course work,…

Trends in Undergraduate Economics Degrees, 1991-2016

ERIC Educational Resources Information Center

Siegfried, John J.

2017-01-01

Undergraduate degrees awarded in economics by U.S. colleges and universities were stagnant from 2009-10 through 2012-13, increased rapidly (almost 15 percent) over the two years from 2012-13 through 2014-15, but have again leveled off in 2015-16.

VizieR Online Data Catalog: Low-mass stars in 25 Ori group and Orion OB1a (Suarez+, 2017)

NASA Astrophysics Data System (ADS)

Suarez, G.; Downes, J. J.; Roman-Zuniga, C.; Covey, K. R.; Tapia, M.; Hernandez, J.; Petr-Gotzens, M. G.; Stassun, K. G.; Briceno, C.

2017-09-01

The V, R, and I photometry used in this work was obtained from the Centro de Investigaciones de Astronomia (CIDA) Deep Survey of Orion (CDSO) catalog (Downes et al. 2014, Cat. J/MNRAS/444/1793), which was constructed by coadding the multi-epoch optical observations from the CIDA Variability Survey of Orion (CVSO; Briceno et al. 2005, Cat. J/AJ/129/907). The sensitivity limits of the CDSO covers the Low-Mass Star (LMS) and Brown Dwarf (BD) population of 25 Ori and its surroundings within the region 79.7°<~α<~82.7° and 0.35°<~δ<~3.35°. The limiting magnitude of the CDSO photometry in this region is Ilim=22 and the completeness magnitude is Icom=19.6 (Downes et al. 2014, Cat. J/MNRAS/444/1793), enough to ensure an I-band detection even for the faintest targets of our spectroscopic sample (I{approx}17.0). Additionally, we used the u, g, r, i, and z photometry from the Sloan Digital Sky Survey (SDSS) catalog (Finkbeiner et al. 2004AJ....128.2577F; Ahn et al. 2012, Cat. V/139). These values are listed in Table1. The Z, Y, J, H, and Ks near-infrared photometry used in this study was carried out by Petr-Gotzens et al. (2011Msngr.145...29P) as part of the Visible and Infrared Survey Telescope for Astronomy (VISTA) science verification surveys (Arnaboldi et al. 2010Msngr.139....6A). The 5σ limiting magnitudes of the VISTA survey of the Orion star-forming region are Z=22.5, Y=21.2, J=20.4, H=19.4, and Ks=18.6, which are enough to have VISTA photometry even for the faintest objects in our spectroscopic sample (J{approx}15.0). Additionally, we used near-infrared photometry from the 2MASS catalog (Cutri et al. 2003, Cat. II/246) and mid-infrared photometry from IRAC-Spitzer (Hernandez et al. 2007, Cat. J/ApJ/671/1784) and the AllWISE catalog (Cutri et al. 2013, Cat. II/328). This infrared photometry is listed in Table1. The spectra used in this paper were obtained as part of the Baryon Oscillation Spectroscopic Survey (BOSS; Dawson et al. 2013AJ....145...10D), which is one of the four main surveys of SDSS (York et al. 2000AJ....120.1579Y) in its third phase (SDSS-III; Eisenstein et al. 2011AJ....142...72E). The BOSS spectrograph has plates with 1000 fibers of 2'' diameter spanning a field of view of 3.0° in diameter and covering a wavelength range from 3560Å to 10400Å with a resolution of R=1560 at 3700Å and R=2650 at 9000Å (Gunn et al. 2006AJ....131.2332G; Smee et al. 2013AJ....146...32S). (4 data files).

Do you kiss your mother with that mouth? An authentic large-scale undergraduate research experience in mapping the human oral microbiome.

PubMed

Wang, Jack T H; Daly, Joshua N; Willner, Dana L; Patil, Jayee; Hall, Roy A; Schembri, Mark A; Tyson, Gene W; Hugenholtz, Philip

2015-05-01

Clinical microbiology testing is crucial for the diagnosis and treatment of community and hospital-acquired infections. Laboratory scientists need to utilize technical and problem-solving skills to select from a wide array of microbial identification techniques. The inquiry-driven laboratory training required to prepare microbiology graduates for this professional environment can be difficult to replicate within undergraduate curricula, especially in courses that accommodate large student cohorts. We aimed to improve undergraduate scientific training by engaging hundreds of introductory microbiology students in an Authentic Large-Scale Undergraduate Research Experience (ALURE). The ALURE aimed to characterize the microorganisms that reside in the healthy human oral cavity-the oral microbiome-by analyzing hundreds of samples obtained from student volunteers within the course. Students were able to choose from selective and differential culture media, Gram-staining, microscopy, as well as polymerase chain reaction (PCR) and 16S rRNA gene sequencing techniques, in order to collect, analyze, and interpret novel data to determine the collective oral microbiome of the student cohort. Pre- and postsurvey analysis of student learning gains across two iterations of the course (2012-2013) revealed significantly higher student confidence in laboratory skills following the completion of the ALURE (p < 0.05 using the Mann-Whitney U-test). Learning objectives on effective scientific communication were also met through effective student performance in laboratory reports describing the research outcomes of the project. The integration of undergraduate research in clinical microbiology has the capacity to deliver authentic research experiences and improve scientific training for large cohorts of undergraduate students.

Double Stars in the USNO CCD Astrograpic Catalog

DTIC Science & Technology

2013-10-01

Catalog (UCAC; Zacharias et al. 2013) is a compiled, all-sky star catalog covering mainly the 8 –16 mag range in a single bandpass between V and R...for UCAC were obtained using the USNO’s 1970s vintage 8 inch Twin Astrograph, originally designed for photographic survey work. The astrograph has two...lens was designed for 8 × 10 inch photographic plates and gives a 9◦ field of view, only the∼1 deg2 area covered by the single CCD was used for the

VizieR Online Data Catalog: RESOLVE survey: 21cm obs. with GBT & Arecibo (Stark+, 2016)

NASA Astrophysics Data System (ADS)

Stark, D. V.; Kannappan, S. J.; Eckert, K. D.; Florez, J.; Hall, K. R.; Watson, L. C.; Hoversten, E. A.; Burchett, J. N.; Guynn, D. T.; Baker, A. D.; Moffett, A. J.; Berlind, A. A.; Norris, M. A.; Haynes, M. P.; Giovanelli, R.; Leroy, A. K.; Pisano, D. J.; Wei, L. H.; Gonzalez, R. E.; Calderon, V. F.

2017-02-01

The REsolved Spectroscopy Of a Local VolumE (RESOLVE) survey is a volume-limited census of galaxies in the local universe with the goal of accounting for baryonic and dark matter mass within a statistically complete subset of the z=0 galaxy population. A complete description of the survey design will be presented in S. J. Kannappan et al. (2016, in preparation). This paper presents new 21cm observations, but an optical spectroscopic survey is under way, primarily with the SOAR 4.1m telescope, and also using SALT, Gemini, and the AAT. The blindly detected 21cm sources in the standard ALFALFA catalog (Giovanelli+ 2005AJ....130.2598G) are cross-matched with RESOLVE using a match radius of 2', corresponding to the spatial resolution of the final ALFALFA data cubes. Additionally, we search the ALFALFA data cubes at the positions of all galaxies that lack counterparts within the standard ALFALFA catalogs. To complete the RESOLVE HI census, new 21cm observations were carried out with the Robert C. Byrd New Green Bank Telescope (GBT, programs 11B-056, 13A-276, 13B-246, 14A-441) and Arecibo Observatory (programs a2671, a2812, a2852). GBT data were acquired over a total of 738hr between 2011 August and 2014 July. Arecibo data were acquired over a total of 554hr in 2012 March and again between 2013 July and 2016 May. (2 data files).

77 FR 30350 - Louisiana Disaster #LA-00045

Federal Register 2010, 2011, 2012, 2013, 2014

2012-05-22

..., tornadoes and flooding. Incident Period: 03/20/2012 through 03/22/2012. Effective Date: 05/15/2012. Physical..., Calcasieu, Jefferson Davis, Vernon. Texas Newton. The Interest Rates are: Percent For Physical Damage... States which received an EIDL Declaration are Louisiana and Texas. (Catalog of Federal Domestic...

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

Price, Laura L.; Barela, Amanda Crystal; Walkow, Walter M.

An Evaluation and Screening team supporting the Fuel Cycle Technologies Program Office of the United States Department of Energy, Office of Nuclear Energy is conducting an evaluation and screening of a comprehensive set of fuel cycle options. These options have been assigned to one of 40 evaluation groups, each of which has a representative fuel cycle option [Todosow 2013]. A Fuel Cycle Data Package System Datasheet has been prepared for each representative fuel cycle option to ensure that the technical information used in the evaluation is high-quality and traceable [Kim, et al., 2013]. The information contained in the Fuel Cyclemore » Data Packages has been entered into the Nuclear Fuel Cycle Options Catalog at Sandia National Laboratories so that it is accessible by the evaluation and screening team and other interested parties. In addition, an independent team at Savannah River National Laboratory has verified that the information has been entered into the catalog correctly. This report documents that the 40 representative fuel cycle options have been entered into the Catalog, and that the data entered into the catalog for the 40 representative options has been entered correctly.« less

VizieR Online Data Catalog: SDSS DR7 white dwarf catalog (Kleinman+, 2013)

NASA Astrophysics Data System (ADS)

Kleinman, S. J.; Kepler, S. O.; Koester, D.; Pelisoli, I.; Pecanha, V.; Nitta, A.; Costa, J. E. S.; Krzesinski, J.; Dufour, P.; Lachapelle, F.-R.; Bergeron, P.; Yip, C.-W.; Harris, H. C.; Eisenstein, D. J.; Althaus, L.; Corsico, A.

2013-01-01

Here, we report on the white dwarf catalog built from the SDSS DR7 (Cat. II/294). We have applied automated techniques supplemented by complete, consistent human identifications of each candidate white dwarf spectrum. We make use of the latest SDSS reductions and white dwarf model atmosphere improvements in our spectral fits, providing logg and Teff determinations for each identified clean DA and DB where we use the word "clean" to identify spectra that show only features of non-magnetic, nonmixed, DA or DB stars. Our catalog includes all white dwarf stars from the earlier Kleinman et al. (2004, Cat. J/ApJ/607/426) and Eisenstein et al. (2006, Cat. J/ApJS/167/40) catalogs, although occasionally with different identifications. (1 data file).

VizieR Online Data Catalog: PHAT X. UV-IR photometry of M31 stars (Williams+, 2014)

NASA Astrophysics Data System (ADS)

Williams, B. F.; Lang, D.; Dalcanton, J. J.; Dolphin, A. E.; Weisz, D. R.; Bell, E. F.; Bianchi, L.; Byler, N.; Gilbert, K. M.; Girardi, L.; Gordon, K.; Gregersen, D.; Johnson, L. C.; Kalirai, J.; Lauer, T. R.; Monachesi, A.; Rosenfield, P.; Seth, A.; Skillman, E.

2015-01-01

The data for the Panchromatic Hubble Andromeda Treasury (PHAT) survey were obtained from 2010 July 12 to 2013 October 12 using the Advanced Camera for Surveys (ACS) Wide Field Channel (WFC), the Wide Field Camera 3 (WFC3) IR (infrared) channel, and the WFC3 UVIS (ultraviolet-optical) channel. The observing strategy is described in detail in Dalcanton et al. (2012ApJS..200...18D). A list of the target names, observing dates, coordinates, orientations, instruments, exposure times, and filters is given in Table 1. Using the ACS and WFC3 cameras aboard HST, we have photometered 414 contiguous WFC3/IR footprints covering 0.5deg2 of the M31 star-forming disk. (4 data files).

VizieR Online Data Catalog: 4yr 1.3mm VLBI observations of SgrA* with EHT (Fish+, 2016)

NASA Astrophysics Data System (ADS)

Fish, V. L.; Johnson, M. D.; Doeleman, S. S.; Broderick, A. E.; Psaltis, D.; Lu, R.-S.; Akiyama, K.; Alef, W.; Algaba, J. C.; Asada, K.; Beaudoin, C.; Bertarini, A.; Blackburn, L.; Blundell, R.; Bower, G. C.; Brinkerink, C.; Cappallo, R.; Chael, A. A.; Chamberlin, R.; Chan, C.-K.; Crew, G. B.; Dexter, J.; Dexter, M.; Dzib, S. A.; Falcke, H.; Freund, R.; Friberg, P.; Greer, C. H.; Gurwell, M. A.; Ho, P. T. P.; Honma, M.; Inoue, M.; Johannsen, T.; Kim, J.; Krichbaum, T. P.; Lamb, J.; Leon-Tavares, J.; Loeb, A.; Loinard, L.; MacMahon, D.; Marrone, D. P.; Moran, J. M.; Moscibrodzka, M.; Ortiz-Leon, G. N.; Oyama, T.; Ozel, F.; Plambeck, R. L.; Pradel, N.; Primiani, R. A.; Rogers, A. E. E.; Rosenfeld, K.; Rottmann, H.; Roy, A. L.; Ruszczyk, C.; Smythe, D. L.; Soohoo, J.; Spilker, J.; Stone, J.; Strittmatter, P.; Tilanus, R. P. J.; Titus, M.; Vertatschitsch, L.; Wagner, J.; Wardle, J. F. C.; Weintroub, J.; Woody, D.; Wright, M.; Yamaguchi, P.; Young, A.; Young, K. H.; Zensus, J. A.; Ziurys, L. M.

2016-06-01

The Event Horizon Telescope (EHT) obtained detections of Sgr A* on closed triangles of baselines among stations in Arizona, California, and Hawaii in 2009, 2011, 2012, and 2013. In all cases, two 480MHz bands, centered at 229.089GHz and 229.601GHz (hereafter, low and high bands, respectively), were observed. One or more telescopes from each of three sites in Arizona, California, and Hawaii participated in each set of observations. The Arizona Radio Observatory (ARO) Submillimeter Telescope (SMT) on Mt. Graham, Arizona, was used in all cases. Over the years of data analyzed here, the configuration of VLBI recording at these sites evolved as described in section 2.1. (1 data file).

Misrepresentations of evolutionary psychology in sex and gender textbooks.

PubMed

Winegard, Benjamin M; Winegard, Bo M; Deaner, Robert O

2014-05-20

Evolutionary psychology has provoked controversy, especially when applied to human sex differences. We hypothesize that this is partly due to misunderstandings of evolutionary psychology that are perpetuated by undergraduate sex and gender textbooks. As an initial test of this hypothesis, we develop a catalog of eight types of errors and document their occurrence in 15 widely used sex and gender textbooks. Consistent with our hypothesis, of the 12 textbooks that discussed evolutionary psychology, all contained at least one error, and the median number of errors was five. The most common types of errors were "Straw Man," "Biological Determinism," and "Species Selection." We conclude by suggesting improvements to undergraduate sex and gender textbooks.

Information Competencies for Chemistry Undergraduates and Related Collaborative Endeavors

ERIC Educational Resources Information Center

Peters, Marion C.

2014-01-01

"Information Competencies for Chemistry Undergraduates: The Elements of Information Literacy", (2012-) now in its second edition and available as a Wikibook since 2012, resulted from collaboration by chemistry librarians participating in several professional organizations. Sections covering a) the library and scientific literature and b)…

Science and Technology Undergraduate Students' Use of the Internet, Cell Phones and Social Networking Sites to Access Library Information

ERIC Educational Resources Information Center

Salisbury, Lutishoor; Laincz, Jozef; Smith, Jeremy J.

2012-01-01

Many academic libraries and publishers have developed mobile-optimized versions of their web sites and catalogs. Almost all database vendors and major journal publishers have provided a way to connect to their resources via the Internet and the mobile web. In light of this pervasive use of the Internet, mobile devices and social networking, this…

VizieR Online Data Catalog: SCUBA-2 high-redshift galaxies sample (Barger+, 2014)

NASA Astrophysics Data System (ADS)

Barger, A. J.; Cowie, L. L.; Chen, C.-C.; Owen, F. N.; Wang, W.-H.; Casey, C. M.; Lee, N.; Sanders, D. B.; Williams, J. P.

2017-05-01

We obtained 25.4 hr of observations on the CDF-N with SCUBA-2 on the JCMT during observing runs in 2012 and 2013. The data were obtained using a mixture of scanning modes and under a variety of weather conditions. Using the CV Daisy scanning mode (detailed information about the SCUBA-2 scan patterns can be found in Holland et al. 2013MNRAS.430.2513H), we obtained a 2.2 hr observation in band 1 weather (225 GHz opacity<0.05) and a 16.5 hr observation in band 2 weather (225 GHz opacity ~0.05-0.08). We also obtained a 6.7 hr observation in band 2 weather using the pong-900 scanning mode. While SCUBA-2 observes at both 450 um and 850 um simultaneously, there are too few sources directly detected at 450 um in our data to be interesting. Thus, we only use the 850 um data in our subsequent analysis. (1 data file).

VizieR Online Data Catalog: Young star systems observed with SALT (Riedel+, 2017)

NASA Astrophysics Data System (ADS)

Riedel, A. R.; Alam, M. K.; Rice, E. L.; Cruz, K. L.; Henry, T. J.

2017-11-01

The sample of stars was drawn from the TINYMO survey (Riedel 2012PhDT.......100R). In that survey, nearby low-proper-motion M dwarfs in the southern hemisphere were identified in the SuperCOSMOS Science Archive (Hambly+ 2001MNRAS.326.1279H). We have obtained low-resolution optical spectroscopy from the SALT telescope at the South African Astronomical Observatory in Sutherland, South Africa and the Robert Stoble Spectrograph (RSS), which provides optical spectroscopy between 3200 and 9000Å with a resolving power of up to 6000, depending on slit width. Observations were conducted in semesters 2013A and 2013B. In total, there are 165 spectra of the 79 stars: SCR 2237-2622 was only observed once, two stars (SCR 1816-6305, 2MASS 2004-3356) were observed three times, three stars (2MASS 0510-2340B, 2MASS 1207-3247, SCR 1842-5554A) were observed four times, and the remainder were observed twice. (5 data files).

VizieR Online Data Catalog: Kepler TTVs. IX. The full long-cadence data set (Holczer+, 2016)

NASA Astrophysics Data System (ADS)

Holczer, T.; Mazeh, T.; Nachmani, G.; Jontof-Hutter, D.; Ford, E. B.; Fabrycky, D.; Ragozzine, D.; Kane, M.; Steffen, J. H.

2016-10-01

The Kepler mission in its original mode of operation has been terminated after 17 quarters (May 2009-Apr 2013), and we do not expect any additional Kepler TTVs for the KOIs identified during the original mission. Thus, here we analyze the whole data set of the mission and derive a complete catalog of the transit timings. Following the approach of Mazeh et al. (2013, J/ApJS/208/16), we present here an analysis of 2599 KOIs (from the NASA exoplanet archive), based on all 17 quarters of the Kepler data. (7 data files).

34 CFR 691.6 - Duration of student eligibility-undergraduate course of study.

Code of Federal Regulations, 2012 CFR

2012-07-01

... 34 Education 4 2012-07-01 2012-07-01 false Duration of student eligibility-undergraduate course of study. 691.6 Section 691.6 Education Regulations of the Offices of the Department of Education (Continued) OFFICE OF POSTSECONDARY EDUCATION, DEPARTMENT OF EDUCATION (CONTINUED) ACADEMIC COMPETITIVENESS...

2MASS Catalog Server Kit Version 2.1

NASA Astrophysics Data System (ADS)

Yamauchi, C.

2013-10-01

The 2MASS Catalog Server Kit is open source software for use in easily constructing a high performance search server for important astronomical catalogs. This software utilizes the open source RDBMS PostgreSQL, therefore, any users can setup the database on their local computers by following step-by-step installation guide. The kit provides highly optimized stored functions for positional searchs similar to SDSS SkyServer. Together with these, the powerful SQL environment of PostgreSQL will meet various user's demands. We released 2MASS Catalog Server Kit version 2.1 in 2012 May, which supports the latest WISE All-Sky catalog (563,921,584 rows) and 9 major all-sky catalogs. Local databases are often indispensable for observatories with unstable or narrow-band networks or severe use, such as retrieving large numbers of records within a small period of time. This software is the best for such purposes, and increasing supported catalogs and improvements of version 2.1 can cover a wider range of applications including advanced calibration system, scientific studies using complicated SQL queries, etc. Official page: http://www.ir.isas.jaxa.jp/~cyamauch/2masskit/

Undergraduate Chemistry Education: A Workshop Summary

ERIC Educational Resources Information Center

Sawyer, Keegan; Alper, Joe

2014-01-01

"Undergraduate Chemistry Education" is the summary of a workshop convened in May 2013 by the Chemical Science Roundtable of the National Research Council to explore the current state of undergraduate chemistry education. Research and innovation in undergraduate chemistry education has been done for many years, and one goal of this…

34 CFR 691.6 - Duration of student eligibility-undergraduate course of study.

Code of Federal Regulations, 2013 CFR

2013-07-01

... 34 Education 4 2013-07-01 2013-07-01 false Duration of student eligibility-undergraduate course of study. 691.6 Section 691.6 Education Regulations of the Offices of the Department of Education (Continued) OFFICE OF POSTSECONDARY EDUCATION, DEPARTMENT OF EDUCATION (CONTINUED) ACADEMIC COMPETITIVENESS...

VizieR Online Data Catalog: CANDELS multiwavelength catalog (Galametz+, 2013)

NASA Astrophysics Data System (ADS)

Galametz, A.; Grazian, A.; Fontana, A.; Ferguson, H. C.; Ashby, M. L. N.; Barro, G.; Castellano, M.; Dahlen, T.; Donley, J. L.; Faber, S. M.; Grogin, N.; Guo, Y.; Huang, K.-H.; Kocevski, D. D.; Koekemoer, A. M.; Lee, K.-S.; McGrath, E. J.; Peth, M.; Willner, S. P.; Almaini, O.; Cooper, M.; Cooray, A.; Conselice, C. J.; Dickinson, M.; Dunlop, J. S.; Fazio, G. G.; Foucaud, S.; Gardner, J. P.; Giavalisco, M.; Hathi, N. P.; Hartley, W. G.; Koo, D. C.; Lai, K.; de Mello, D. F.; McLure, R. J.; Lucas, R. A.; Paris, D.; Pentericci, L.; Santini, P.; Simpson, C.; Sommariva, V.; Targett, T.; Weiner, B. J.; Wuyts, S.; CANDELS Team

2013-06-01

The present multiwavelength catalog is based on public data in the CANDELS UDS field (J2000 position: 02:17:37.5-05:12:00) located within the original UDS field. It includes: * CANDELS HST/ACS (F606W, F814W) and HST/WFC3 (F125W, F160W); Grogin et al. 2011ApJS..197...35G, Koekemoer et al. 2011ApJS..197...36K. * CFHT U-band (UKIDSS; Almaini et al. in prep.), * SUBARU B, V, Rc, i', z' (SXDS; Furusawa et al. 2008, Cat. J/ApJS/176/1) * VLT/HAWK-I Y and Ks bands (HUGS; Fontana et al. in prep.) * UKIRT/WFCam J, H, K (UKIDSS DR8; Almaini et al. in prep.) * Spitzer/IRAC SEDS 3.6 and 4.5um (SEDS; Ashby et al. 2013ApJ...769...80A) * Spitzer/IRAC SpUDS 5.8, 8.0um (PI: J. Dunlop). The catalog is F160W-selected and contains 35932 sources over an area of 201.7 square arcmin and includes radio and X-ray detected sources and spectroscopic redshifts available for 210 sources. The full official CANDELS UDS catalog (which contains some extra columns including additional SExtractor parameters derived from the F160W image) can be found on the CANDELS website at: http://candels.ucolick.org/data_access/UDS.html (1 data file).

VizieR Online Data Catalog: M31 PHAT star clusters ages and masses (Fouesneau+, 2014)

NASA Astrophysics Data System (ADS)

Fouesneau, M.; Johnson, L. C.; Weisz, D. R.; Dalcanton, J. J.; Bell, E. F.; Bianchi, L.; Caldwell, N.; Gouliermis, D. A.; Guhathakurta, P.; Kalirai, J.; Larsen, S. S.; Rix, H.-W.; Seth, A. C.; Skillman, E. D.; Williams, B. F.

2017-07-01

For this paper, we use the list of 601 high-probability cluster candidates from the Johnson et al. (2012, J/ApJ/752/95) Year 1 catalog, which contains integrated photometry through six broadband filters from the UV to the near-infrared: F275W (UV), F336W (U), F475W (g), F814W (I), F110W (J), F160W (H). Clusters were detected by eye, primarily based on the F475W images, and visually classified based on their sizes, shapes, and concentrations as explained in Johnson et al. (2012, J/ApJ/752/95). (1 data file).

VizieR Online Data Catalog: Ultra-compact HII regions & methanol masers. I. (Hu+, 2016)

NASA Astrophysics Data System (ADS)

Hu, B.; Menten, K. M.; Wu, Y.; Bartkiewicz, A.; Rygl, K.; Reid, M. J.; Urquhart, J. S.; Zheng, X.

2017-03-01

372 unique targets were selected from the following methanol maser surveys: the Methanol Multi-Beam catalog (MMB; Caswell & Breen 2010MNRAS.407.2599C; Green+ 2010-2012, VIII/96), the Arecibo Methanol Maser Galactic Plane Survey (AMGPS; Pandian+ 2011ApJ...730...55P), the Torun catalog of 6.7GHz methanol masers (Szymczak+ 2012, J/AN/333/634), and other individual observations of known 6.7GHz methanol masers or MSFRs (Caswell+ 1995MNRAS.272...96C; Walsh+ 1997, J/MNRAS/291/261; 1998, J/MNRAS/301/640; Xu+ 2008A&A...485..729X; Caswell 2009, J/other/PASA/26.454). The observations were conducted with the VLA in C-configuration using five sessions from 2012 February 28 to April 16. Spectral line data used 2048 channels across 8MHz, yielding a channel spacing of 3.90625kHz at the central frequency of 6.6685192GHz and a velocity resolution of 0.176km/s. The continuum observations employed two 1GHz sub-bands from 4.9840 to 6.0080GHz (the low band) and from 6.6245 to 7.6485GHz (the high band) and each sub-band was divided into 16 channels. (4 data files).

MAXI/GSC 7-year Source Catalog

NASA Astrophysics Data System (ADS)

Ueda, Y.; Kawamuro, T.; Hori, T.; Shidatsu, M.; Tanimoto, A.; MAXI Team

2017-10-01

Monitor of All-sky X-ray Image (MAXI) on the International Space Station has been continuously observing the X-ray sky since its launch in 2009. The MAXI survey has achieved the best sensitivity in the 4-10 keV band as an all sky X-ray mission, and is complementary to the ROSAT all sky survey (<2 keV) and hard X-ray (>10 keV) surveys performed with Swift and INTEGRAL. Here we present the latest source catalog of MAXI/Gas Slit Camera (GSC) constructed from the first 7-year data, which is an extension of the 37-month catalog of the high Galactic-latitude sky (Hiroi et al. 2013). We summarize statistical properties of the X-ray sources and results of cross identification with other catalogs.

VizieR Online Data Catalog: Flaring gamma-ray sources; LAT 7.4yr (2FAV) (Abdollahi+, 2017)

NASA Astrophysics Data System (ADS)

Abdollahi, S.; Ackermann, M.; Ajello, M.; Albert, A.; Baldini, L.; Ballet, J.; Barbiellini, G.; Bastieri, D.; Becerra Gonzalez, J.; Bellazzini, R.; Bissaldi, E.; Blandford, R. D.; Bloom, E. D.; Bonino, R.; Bottacini, E.; Bregeon, J.; Bruel, P.; Buehler, R.; Buson, S.; Cameron, R. A.; Caragiulo, M.; Caraveo, P. A.; Cavazzuti, E.; Cecchi, C.; Chekhtman, A.; Cheung, C. C.; Chiaro, G.; Ciprini, S.; Conrad, J.; Costantin, D.; Costanza, F.; Cutini, S.; D'Ammando, F.; de Palma, F.; Desai, A.; Desiante, R.; Digel, S. W.; di Lalla, N.; di Mauro, M.; di Venere, L.; Donaggio, B.; Drell, P. S.; Favuzzi, C.; Fegan, S. J.; Ferrara, E. C.; Focke, W. B.; Franckowiak, A.; Fukazawa, Y.; Funk, S.; Fusco, P.; Gargano, F.; Gasparrini, D.; Giglietto, N.; Giomi, M.; Giordano, F.; Giroletti, M.; Glanzman, T.; Green, D.; Grenier, I. A.; Grove, J. E.; Guillemot, L.; Guiriec, S.; Hays, E.; Horan, D.; Jogler, T.; Johannesson, G.; Johnson, A. S.; Kocevski, D.; Kuss, M.; La Mura, G.; Larsson, S.; Latronico, L.; Li, J.; Longo, F.; Loparco, F.; Lovellette, M. N.; Lubrano, P.; Magill, J. D.; Mal! Dera, S.; Manfreda, A.; Mayer, M.; Mazziotta, M. N.; Michelson, P. F.; Mitthumsiri, W.; Mizuno, T.; Monzani, M. E.; Morselli, A.; Moskalenko, I. V.; Negro, M.; Nuss, E.; Ohsugi, T.; Omodei, N.; Orienti, M.; Orlando, E.; Paliya, V. S.; Paneque, D.; Perkins, J. S.; Persic, M.; Pesce-Rollins, M.; Petrosian, V.; Piron, F.; Porter, T. A.; Principe, G.; Raino, S.; Rando, R.; Razzano, M.; Razzaque, S.; Reimer, A.; Reimer, O.; Sgro, C.; Simone, D.; Siskind, E. J.; Spada, F.; Spandre, G.; Spinelli, P.; Stawarz, L.; Suson, D. J.; Takahashi, M.; Tanaka, K.; Thayer, J. B.; Thompson, D. J.; Torres, D. F.; Torresi, E.; Tosti, G.; Troja, E.; Vianello, G.; Wood, K. S.

2018-04-01

To build the second catalog of flaring gamma-ray sources (2FAV) catalog, we apply the Fermi All-sky Variability Analysis (FAVA; Ackermann+ 2013, J/ApJ/771/57) to the first 387 weeks of Fermi observations, from Mission Elapsed Time (MET) 239557418 to 473615018, or Modified Julian Date (MJD) from 54682 (2008 August 4) to 57391 (2016 January 4). In this time range, a total of 7106 seed flares were found, roughly 18 per week. As for the previous catalog, FAVA uses weekly time bins. Two independent energy bands are used, 0.1-0.8GeV and 0.8-300GeV, to enhance the sensitivity to spectrally soft and hard flares, respectively. (2 data files).

VizieR Online Data Catalog: WINERED CN-red band emission in comet C/2013 R1 (Shinnaka+, 2017)

NASA Astrophysics Data System (ADS)

Shinnaka, Y.; Kawakita, H.; Kondo, S.; Ikeda, Y.; Kobayashi, N.; Hamano, S.; Sameshima, H.; Fukue, K.; Matsunaga, N.; Yasui, C.; Izumi, N.; Mizumoto, M.; Otsubo, S.; Takenaka, K.; Watase, A.; Kawanishi, T.; Nakanishi, K.; Nakaoka, T.

2018-05-01

High-resolution spectroscopic observations of comet C/2013 R1 (Lovejoy; hereafter, comet Lovejoy) in the near-infrared wavelength region were performed using the WINERED spectrograph (Ikeda et al. 2016SPIE.9908E..5ZI) mounted on the Nasmyth focus of the 1.3 m Araki telescope (F/10) at Koyama Astronomical Observatory, Japan (Yoshikawa et al. 2012SPIE.8444E..6GY). We used a slit of length 47" and width 1.5". This slit width corresponds to a spectral resolving power of R=28000 (two pixels). The observations of comet Lovejoy were performed on 2013 November 30, from 19:08 UT to 21:04 UT; the total integration time was 6000 s on source. The heliocentric and geocentric distances were 0.91 au and 0.49 au, respectively, and the relative velocities of the comet to the Sun and observer were -14.5 km/s and 25.8 km/s, respectively, at the observations. We put the comet at the center of the slit during the exposures. Other calibration data (darks, flats, and comparison-lamp frames) were also acquired. (1 data file).

Localizing the Transdisciplinary in Practice: A Teaching Account of a Prototype Undergraduate Seminar on Linguistic Landscape

ERIC Educational Resources Information Center

Malinowski, David

2016-01-01

Building upon paradigms of language and languaging practices as "local" phenomena (Canagarajah, 2013; Pennycook, 2010, Pietikäinen & Kelly-Holmes, 2013), this paper narrates a teacher's experience in an undergraduate seminar in applied language studies as an exploration in transdisciplinarity-as-localization. Taught by the author in…

VizieR Online Data Catalog: IR photometry of AGNs in Swift/BAT 70 month cat. (Ichikawa+, 2017)

NASA Astrophysics Data System (ADS)

Ichikawa, K.; Ricci, C.; Ueda, Y.; Matsuoka, K.; Toba, Y.; Kawamuro, T.; Trakhtenbrot, B.; Koss, M. J.

2017-08-01

Our initial sample contains the 834 AGNs reported in the 70 month Swift/BAT catalog (Baumgartner+ 2013, J/ApJS/207/19), 105 of which are blazars. Of the remaining 729 sources, 697 sources have secure redshift information as presented in Ricci et al. (2016, ApJ, submitted). Next, we removed galaxy pairs or interacting galaxies not resolved in the BAT survey. Further, the 606 sources located at higher galactic latitudes with |b|>10° were selected to reduce the contamination in the crowded region through IR catalog matching. (1 data file).

48 CFR 552.238-75 - Price Reductions.

Code of Federal Regulations, 2012 CFR

2012-10-01

... 48 Federal Acquisition Regulations System 4 2012-10-01 2012-10-01 false Price Reductions. 552.238-75 Section 552.238-75 Federal Acquisition Regulations System GENERAL SERVICES ADMINISTRATION CLAUSES... conclude, the Contractor— (i) Revises the commercial catalog, pricelist, schedule or other document upon...

Newly Built Undergraduate Schools Should Place Great Emphasis on Connotation Construction and Quality Promotion: An Analysis Based on the Qualification Evaluation Results for 41 Undergraduate Schools

ERIC Educational Resources Information Center

Binglin, Zhong

2016-01-01

The article presents a quantitative analysis of the evaluation results for 41 newly built undergraduate schools that submitted to the qualification evaluation of undergraduate work by Ministry of Education in 2013. It shows that newly built undergraduate schools should place great emphasis on connotation construction and quality promotion and on…

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.

VizieR Online Data Catalog: Catalog of Earth-Like Exoplanet Survey Targets (Chandler+, 2016)

NASA Astrophysics Data System (ADS)

Chandler, C. O.; McDonald, I.; Kane, S. R.

2016-07-01

We present the Catalog of Earth-Like Exoplanet Survey Targets (CELESTA), a database of habitable zones around 37000 nearby stars. The first step in creating CELESTA was assembling the input data. The Revised Hipparcos Catalog (van Leeuwen 2007, Cat. I/311) is a stellar catalog based on the original Hipparcos mission (Perryman et al. 1997, Cat. I/239) data set. Hipparcos, launched in 1989, recorded with great precision the parallax of nearby stars, ultimately leading to a database of 118218 stars. McDonald et al. 2012 (cat. J/MNRAS/427/343) calculated effective temperatures and luminosities for the Hipparcos stars. The next step was selecting appropriate stars for the construction of CELESTA. The Stellar Parameter Catalog of 103663 stars included many stars that were not suitable for our purposes, especially stars off the Main-Sequence (MS) branch, e.g., giants. Please refer to Section 3.2 in the paper for additional details about the star selection. The final CELESTA catalog contains 37354 stars (see Table2), each with a set of associated attributes, e.g., estimated mass, measured distance. The complete database can also be found online at a dedicated host (http://www.celesta.info/). (2 data files).

Composite Earthquake Catalog of the Yellow Sea for Seismic Hazard Studies

NASA Astrophysics Data System (ADS)

Kang, S. Y.; Kim, K. H.; LI, Z.; Hao, T.

2017-12-01

The Yellow Sea (a.k.a West Sea in Korea) is an epicontinental and semi-closed sea located between Korea and China. Recent earthquakes in the Yellow Sea including, but not limited to, the Seogyuckryulbi-do (1 April 2014, magnitude 5.1), Heuksan-do (21 April 2013, magnitude 4.9), Baekryung-do (18 May 2013, magnitude 4.9) earthquakes, and the earthquake swarm in the Boryung offshore region in 2013, remind us of the seismic hazards affecting east Asia. This series of earthquakes in the Yellow Sea raised numerous questions. Unfortunately, both governments have trouble in monitoring seismicity in the Yellow Sea because earthquakes occur beyond their seismic networks. For example, the epicenters of the magnitude 5.1 earthquake in the Seogyuckryulbi-do region in 2014 reported by the Korea Meteorological Administration and China Earthquake Administration differed by approximately 20 km. This illustrates the difficulty with seismic monitoring and locating earthquakes in the region, despite the huge effort made by both governments. Joint effort is required not only to overcome the limits posed by political boundaries and geographical location but also to study seismicity and the underground structures responsible. Although the well-established and developing seismic networks in Korea and China have provided unprecedented amount and quality of seismic data, high quality catalog is limited to the recent 10s of years, which is far from major earthquake cycle. It is also noticed the earthquake catalog from either country is biased to its own and cannot provide complete picture of seismicity in the Yellow Sea. In order to understand seismic hazard and tectonics in the Yellow Sea, a composite earthquake catalog has been developed. We gathered earthquake information during last 5,000 years from various sources. There are good reasons to believe that some listings account for same earthquake, but in different source parameters. We established criteria in order to provide consistent information in the Yellow Sea composite earthquake catalog (YComCat). Since earthquake catalog plays critical role in the seismic hazard assessment, YComCat provides improved input to reduce uncertainties in the seismic hazard estimations.

Catalog of Training and Education Sources in Concurrent Engineering

DTIC Science & Technology

1989-11-01

Undergraduate degree in engineering or hard science. TOEFL (Test of English as a Foreign Language) of 550 or better for international students and GMAT (Graduate...Graduate Record Examination)of 1000 0 (Verbal + Quantitative); TOEFL (Test of English as a Foreign Language) of 550 for students whose first language...Graduate Record Examination) and TOEFL (Test of English as a Foreign Language) 0 scores. Comments: Recipient of the CASA/SME 1988 University LEAD

New Americans in Postsecondary Education: A Profile of Immigrant and Second-Generation American Undergraduates. Stats in Brief. NCES 2012-213

ERIC Educational Resources Information Center

Staklis, Sandra; Horn, Laura

2012-01-01

This Statistics in Brief describes the undergraduate experiences of students who immigrated to the United States or who had at least one immigrant parent (second-generation Americans). The analysis compares these two groups with all undergraduates (excluding foreign students) and with third-or higher generation American undergraduates whose…

VizieR Online Data Catalog: Hubble Source Catalog (V1 and V2) (Whitmore+, 2016)

NASA Astrophysics Data System (ADS)

Whitmore, B. C.; Allam, S. S.; Budavari, T.; Casertano, S.; Downes, R. A.; Donaldson, T.; Fall, S. M.; Lubow, S. H.; Quick, L.; Strolger, L.-G.; Wallace, G.; White, R. L.

2016-10-01

The HSC v1 contains members of the WFPC2, ACS/WFC, WFC3/UVIS and WFC3/IR Source Extractor source lists from HLA version DR8 (data release 8). The crossmatching process involves adjusting the relative astrometry of overlapping images so as to minimize positional offsets between closely aligned sources in different images. After correction, the astrometric residuals of crossmatched sources are significantly reduced, to typically less than 10mas. The relative astrometry is supported by using Pan-STARRS, SDSS, and 2MASS as the astrometric backbone for initial corrections. In addition, the catalog includes source nondetections. The crossmatching algorithms and the properties of the initial (Beta 0.1) catalog are described in Budavari & Lubow (2012ApJ...761..188B). The HSC v2 contains members of the WFPC2, ACS/WFC, WFC3/UVIS and WFC3/IR Source Extractor source lists from HLA version DR9.1 (data release 9.1). The crossmatching process involves adjusting the relative astrometry of overlapping images so as to minimize positional offsets between closely aligned sources in different images. After correction, the astrometric residuals of crossmatched sources are significantly reduced, to typically less than 10mas. The relative astrometry is supported by using Pan-STARRS, SDSS, and 2MASS as the astrometric backbone for initial corrections. In addition, the catalog includes source nondetections. The crossmatching algorithms and the properties of the initial (Beta 0.1) catalog are described in Budavari & Lubow (2012ApJ...761..188B). Hubble Source Catalog Acknowledgement: Based on observations made with the NASA/ESA Hubble Space Telescope, and obtained from the Hubble Legacy Archive, which is a collaboration between the Space Telescope Science Institute (STScI/NASA), the Space Telescope European Coordinating Facility (ST-ECF/ESAC/ESA) and the Canadian Astronomy Data Centre (CADC/NRC/CSA). (2 data files).

Assessing Undergraduates' Understanding of Diversity Using Concept Maps

ERIC Educational Resources Information Center

Golightly, Amy F.; Nottis, Katharyn E. K.

2017-01-01

Many undergraduates in privileged positions mistakenly feel that we live in a post-racial society (e.g. Goodman, 1995; Osborne, Kriese, & Davis, 2013). Their prior knowledge about diversity can be limited and they can be unaware of what they do not know about cultural competence and intercultural sensitivity (e.g., Osborne et al., 2013;…

41 CFR 101-30.704 - Agency responsibilities.

Code of Federal Regulations, 2012 CFR

2012-07-01

... 41 Public Contracts and Property Management 2 2012-07-01 2012-07-01 false Agency responsibilities. 101-30.704 Section 101-30.704 Public Contracts and Property Management Federal Property Management Regulations System FEDERAL PROPERTY MANAGEMENT REGULATIONS SUPPLY AND PROCUREMENT 30-FEDERAL CATALOG SYSTEM 30...

The male of the orb-weaving spider Plebs mitratus (Simon, 1895) and a redescription of the female (Araneae, Araneidae).

PubMed

Paul, Jimmy; Sankaran, Pradeep M; Joseph, Mathew M; Sebastian, Pothalil A

2016-10-28

The orb-weaving spider genus Plebs Joseph & Framenau, 2012 currently has only two representatives in India: Plebs himalayaensis (Tikader, 1975) from the Himalayas and Plebs mitratus (Simon, 1895) from the Nilgiris and Anamudi Shola National Park (World Spider Catalog 2016), both are found in high altitude mountainous habitats (Joseph & Framenau 2012). Both species were known only from females (World Spider Catalog 2016), although Sherriffs (1918, 1919) provided a description of an immature male of P. mitratus. In the present paper, we provide the first description of the adult male of P. mitratus, together with the detailed redescription of its female demonstrating considerable intraspecific variation.

48 CFR 552.238-75 - Price Reductions.

Code of Federal Regulations, 2013 CFR

2013-10-01

... 48 Federal Acquisition Regulations System 4 2013-10-01 2013-10-01 false Price Reductions. 552.238-75 Section 552.238-75 Federal Acquisition Regulations System GENERAL SERVICES ADMINISTRATION CLAUSES... conclude, the Contractor— (i) Revises the commercial catalog, pricelist, schedule or other document upon...

Investigations of Martian Impact Crater Morphologies and Morphometries

NASA Technical Reports Server (NTRS)

Barlow, Nadine G.

2002-01-01

We have made substantial progress towards completion of the original objectives and are continuing to include new data from the Mars Global Surveyor MOC and TES instruments as they become available (the MOLA instrument has ceased operation as of 2002). The project funding has been used to provide salary support to the PI and several undergraduate students, cover publication charges for two papers, reimburse travel expenses to conferences and workshops incurred by the PI and students, and cover a number of other expenses such as software upgrades and production costs of slides and color prints. This study is revising the PI's Catalog of Large Martian Impact Craters with information obtained from MGS and is utilizing data in the revised Catalog to investigate which planetary factors (such as location, elevation, terrain type, etc.) primarily affect the formation of specific ejecta morphologies and morphometries.

Comprehensive Cross-Training among STEM Disciplines in Geothermal Energy

NASA Astrophysics Data System (ADS)

Nunn, J. A.; Dutrow, B. L.

2012-12-01

One of the foremost areas of sustainability is society's need for energy. The US uses more energy per capita than any other country in the world with most of this energy coming from fossil fuels. With its link to climate change coupled with declining resources, renewable alternatives are being pursued. Given the high demand for energy, it is not a question of if these alternatives will be utilized but when and where. One of the "greenest" of the green technologies is geothermal energy. It is a renewable resource with a small environmental footprint. To educate advanced undergraduate and graduate students from across STEM disciplines in geothermal energy, a series of three distinct but linked and related courses are being developed and taught. Courses are focused on one of the STEM disciplines to provide students with essential discipline-specific knowledge and taught by different faculty members in the departments of geology, petroleum engineering and mathematics. These courses provide the foundation necessary for interdisciplinary research projects. The first course on Geologic Properties and Processes of Geothermal Energy was developed and taught in 2012. The class had an enrollment of 27 students including: 5 undergraduates and 4 graduate students in Geology, 12 undergraduates and two graduate students in Petroleum Engineering, and 4 non-matriculated undergraduate students. The course began with the essentials of heat and mass transfer, a common deficiency for all students, then progressed to the geologic materials of these systems: minerals, rocks and fluids. To provide students with first hand experience, two short research projects were embedded into the course. The first project involved analyses of cuttings from a well-studied geothermal system (Salton Sea, CA). Students were in teams consisting of both engineers and geologists. The first assignment was to identify minerals in the cuttings. They were then provided with XRD patterns for their cuttings to more precisely identify the mineralogy of the cuttings. Based on this data with depth, they were asked to predict an approximate temperature range and calculate various fluid parameters for these conditions. The second research project was completed individually, each student covered aspects of heat transport and geologic materials on a specific geothermal field of their choice, created a poster, and gave a brief oral presentation of the poster similar to what is done at scientific meetings. This not only helped students develop communication skills it also provide the class and the instructors information on the breath and diversity of geothermal projects already underway throughout the world and helped to improve critical thinking skills. Continued integration of our research and graduate training programs in Geology and Geophysics, Petroleum Engineering, and Mathematics will occur in 2012-2013. The Petroleum Engineering course will be offered in the fall semester of 2012 and the Mathematics class in the spring semester of 2013. Providing this three semester sequence of courses across the STEM disciplines promotes comprehensive cross-training among disciplines and provides a template for future directions of teaching sustainability across the disciplines.

Undergraduate Medical Education Research in Malaysia: Time for a Change

PubMed Central

Salam, Abdus; Hamzah, Jemaima Che; Chin, Tan Geok; Siraj, Harlina Halizah; Idrus, Ruszymah; Mohamad, Nabishah; Raymond, Azman Ali

2015-01-01

Objective: Special Study Module (SSM) is a mandatory research module implemented in Universiti Kebangsaan Malaysia (UKM). The objective of this paper is to provide a brief overview on the student research activities and to find out the outcome measures in terms of publication. Methods: It was a retrospective study done on SSM research projects at UKM. The SSM research is conducted from beginning of year-4 until 1st seven weeks of year-5. In year-4, students are assigned to a faculty-supervisor in small groups and spend every Thursday afternoon to plan and carry the research. Whole first seven weeks of year-5, students are placed with their supervisor continuously to collect data, do analysis, write report and present in the scientific conference. Outcomes of 5-years SSM research-projects starting from 2008/2009 to 2012/2013 academic session were analyzed. Results: Total 257 projects were completed and presented in annual scientific meetings from which 57 (22.2%) articles were published in peer reviewed journals. Conclusion: Mandatory undergraduate student research project brings an opportunity to develop students’ capacity building from conception to final report writing and thereby narrowing the gap between education and practice. Medical schools should implement research module to bring changes in research and publication culture of undergraduate medical education. PMID:26150832

The construction and validation of an instrument for the assessment of graduates of undergraduate nursing courses 1

PubMed Central

Vieira, Maria Aparecida; Ohara, Conceição Vieira da Silva; de Domenico, Edvane Birelo Lopes

2016-01-01

Abstract Objective: to construct an instrument for the assessment of graduates of undergraduate nursing courses and to validate this instrument through the consensus of specialists. Method: methodological study. In order to elaborate the instrument, documental analysis and a literature review were undertaken. Validation took place through use of the Delphi Conference, between September 2012 and September 2013, in which 36 specialists from Brazilian Nursing participated. In order to analyze reliability, the Cronbach alpha coefficient, the item/total correlation, and the Pearson correlation coefficient were calculated. Results: the instrument was constructed with the participation of specialist nurses representing all regions of Brazil, with experience in lecturing and research. The first Delphi round led to changes in the first instrument, which was restructured and submitted to another round, with a response rate of 94.44%. In the second round, the instrument was validated with a Cronbach alpha of 0.75. Conclusion: the final instrument possessed three dimensions related to the characterization of the graduate, insertion in the job market, and evaluation of the professional training process. This instrument may be used across the territory of Brazil as it is based on the curricular guidelines and contributes to the process of regulation of the quality of the undergraduate courses in Nursing. PMID:27305184

41 CFR 101-30.100 - Scope of subpart.

Code of Federal Regulations, 2012 CFR

2012-07-01

... 41 Public Contracts and Property Management 2 2012-07-01 2012-07-01 false Scope of subpart. 101-30.100 Section 101-30.100 Public Contracts and Property Management Federal Property Management Regulations System FEDERAL PROPERTY MANAGEMENT REGULATIONS SUPPLY AND PROCUREMENT 30-FEDERAL CATALOG SYSTEM 30...

41 CFR 101-30.300 - Scope of subpart.

Code of Federal Regulations, 2012 CFR

2012-07-01

... 41 Public Contracts and Property Management 2 2012-07-01 2012-07-01 false Scope of subpart. 101-30.300 Section 101-30.300 Public Contracts and Property Management Federal Property Management Regulations System FEDERAL PROPERTY MANAGEMENT REGULATIONS SUPPLY AND PROCUREMENT 30-FEDERAL CATALOG SYSTEM 30...

40 CFR 35.936-19 - Small purchases.

Code of Federal Regulations, 2012 CFR

2012-07-01

... 40 Protection of Environment 1 2012-07-01 2012-07-01 false Small purchases. 35.936-19 Section 35.936-19 Protection of Environment ENVIRONMENTAL PROTECTION AGENCY GRANTS AND OTHER FEDERAL ASSISTANCE... these documents and of written quotations received, or references to catalogs or printed price lists...

48 CFR 945.608-2 - Standard screening.

Code of Federal Regulations, 2012 CFR

2012-10-01

... System (REAPS). Agency screening will begin when the item is first included in the REAPS monthly catalog... 48 Federal Acquisition Regulations System 5 2012-10-01 2012-10-01 false Standard screening. 945.608-2 Section 945.608-2 Federal Acquisition Regulations System DEPARTMENT OF ENERGY CONTRACT...

VizieR Online Data Catalog: Hα observations of LSI+61 303 (Zamanov+, 2013)

NASA Astrophysics Data System (ADS)

Zamanov, R.; Stoyanov, K.; Marti, J.; Tomov, N. A.; Belcheva, G.; Luque-Escamilla, P. L.; Latev, G.

2013-09-01

Optical spectroscopic observations of the Hα emission line (137 spectra obtained during the period of September 1998 - January 2013) are presented for the the radio- and gamma-ray-emitting Be/X-ray binary LSI+61 303. (2 data files).

VizieR Online Data Catalog: ATLASGAL clumps with IRAS flux and MALT90 data (Stephens+, 2016)

NASA Astrophysics Data System (ADS)

Stephens, I. W.; Jackson, J. M.; Whitaker, J. S.; Contreras, Y.; Guzman, A. E.; Sanhueza, P.; Foster, J. B.; Rathborne, J. M.

2016-08-01

The Millimetre Astronomy Legacy Team 90GHz (MALT90) survey (Foster+ 2011, J/ApJS/197/25; 2013PASA...30...38F; Jackson+ 2013PASA...30...57J) mapped 16 lines for 3246 clumps, primarily high-mass star-forming clumps that are >200M⊙, as identified from the ATLASGAL 870um survey (Schuller et al. 2009A&A...504..415S). In order to compare luminosities derived from IRAS (LIR) to molecular line luminosities from MALT90 (Lmolecule), we first matched the MALT90 clumps to the IRAS Point Source Catalog v2.1 (PSC; see Cat. II/125). See section 2.1 for further explanations. (1 data file).

The Third Fermi LAT Catalog of High-Energy Gamma-ray Sources

NASA Astrophysics Data System (ADS)

Thompson, David J.; Ballet, J.; Burnett, T.; Fermi Large Area Telescope Collaboration

2014-01-01

The Fermi Gamma-ray Space Telescope Large Area Telescope (LAT) has been gathering science data since August 2008, surveying the full sky every three hours. The second source catalog (2FGL, Nolan et al 2012, ApJS 199, 31) was based on 2 years of data. We are preparing a third source catalog (3FGL) based on 4 years of reprocessed data. The reprocessing introduced a more accurate description of the instrument, which resulted in a narrower point spread function. Both the localization and the detection threshold for hard-spectrum sources have been improved. The new catalog also relies on a refined model of Galactic diffuse emission, particularly important for low-latitude soft-spectrum sources. The process for associating LAT sources with those at other wavelengths has also improved, thanks to dedicated multiwavelength follow-up, new surveys and better ways to extract sources likely to be gamma-ray counterparts. We describe the construction of this new catalog, its characteristics, and its remaining limitations.

The Third Fermi-LAT Catalog of High-Energy Gamma-ray Sources

NASA Astrophysics Data System (ADS)

Burnett, Toby

2014-03-01

The Fermi Gamma-ray Space Telescope Large Area Telescope (LAT) has been gathering science data since August 2008, surveying the full sky every three hours. The second source catalog (2FGL, Nolan et al. 2012, ApJS 199, 31) was based on 2 years of data. We are preparing a third source catalog (3FGL) based on 4 years of reprocessed data. The reprocessing introduced a more accurate description of the instrument, which resulted in a narrower point spread function. Both the localization and the detection threshold for hard-spectrum sources have been improved. The new catalog also relies on a refined model of Galactic diffuse emission, particularly important for low-latitude soft-spectrum sources. The process for associating LAT sources with those at other wavelengths has also improved, thanks to dedicated multiwavelength follow-up, new surveys and better ways to extract sources likely to be gamma-ray counterparts. We describe the construction of this new catalog, its characteristics, and its remaining limitations.

VizieR Online Data Catalog: JCMT Gould Belt Survey: Southern Orion A (Mairs+, 2016)

NASA Astrophysics Data System (ADS)

Mairs, S.; Johnstone, D.; Kirk, H.; Buckle, J.; Berry, D. S.; Broekhoven-Fiene, H.; Currie, M. J.; Fich, M.; Graves, S.; Hatchell, J.; Jenness, T.; Mottram, J. C.; Nutter, D.; Pattle, K.; Pineda, J. E.; Salji, C.; di, Francesco J.; Hogerheijde, M. R.; Ward-Thompson, D.; Bastien, P.; Bresnahan, D.; Butner, H.; Chen, M.; Chrysostomou, A.; Coude, S.; Davis, C. J.; Drabek-Maunder, E.; Duarte-Cabral, A.; Fiege, J.; Friberg, P.; Friesen, R.; Fuller, G. A.; Greaves, J.; Gregson, J.; Holland, W.; Joncas, G.; Kirk, J. M.; Knee, L. B. G.; Marsh, K.; Matthews, B. C.; Moriarty-Schieven, G.; Mowat, C.; Rawlings, J.; Richer, J.; Robertson, D.; Rosolowsky, E.; Rumble, D.; Sadavoy, S.; Thomas, H.; Tothill, N.; Viti, S.; White, G. J.; Wouterloot, J.; Yates, J.; Zhu, M.

2017-11-01

The observations presented throughout this paper were performed using the SCUBA-2 instrument (Holland et al., 2013MNRAS.430.2513H) as part of the JCMT Gould Belt Survey (Ward-Thompson et al., 2007PASP..119..855W). This instrument has provided continuum coverage at both 850um and 450um simultaneously at effective beam sizes of 14.1-arcsec and 9.6-arcsec, respectively (Dempsey et al., 2013MNRAS.430.2534D). In this work, we present Southern Orion A in both wavelengths, but focus mainly on the 850um data for analysis. All of the observations were taken in the PONG1800 mapping mode, yielding circular maps ('PONGs') of 0.5° in diameter. There are 17 0.5° subregions across the Orion A Molecular Cloud, 13 of which cover Southern Orion A. These locations were individually observed four to six times throughout 2012 February to 2015 January, and were then co-added (once co-added, these structures are referred to as 'tiles') and mosaicked to form the final map. (3 data files).

VizieR Online Data Catalog: Near-infrared observations of 84 KOI systems (Atkinson+, 2017)

NASA Astrophysics Data System (ADS)

Atkinson, D.; Baranec, C.; Ziegler, C.; Law, N.; Riddle, R.; Morton, T.

2017-06-01

The initial observations identifying companion candidates are from multiple Robo-AO observing runs on the Palomar Observatory 1.5m telescope, spanning 2012 July to September, 2013 April to October, 2014 June to September, and 2015 June. Observations were in either Sloan-i or a long-pass 600nm (LP600) filter, the latter being similar to the Kepler-bandpass when combined with the EMCCD's quantum efficiency curve for red/cool stars. The near-infrared observations are from the Near-InfraRed Camera 2 (NIRC2) instrument on the 10m Keck II telescope, conducted on 2013 June 24, August 24 and 25, 2014 August 17, 2015 July 25, and August 4 in the J, H, K, and/or Kp filters in the narrow mode of NIRC2 (9.952mas/pixel). The relative positions and raw contrast measurements of imaged companions are presented in Table4. The reduced apparent magnitudes, which use both measured contrasts and canonical apparent magnitudes of combined systems in Kepler literature, are presented in Table5. (5 data files).

41 CFR 101-30.000 - Scope of part.

Code of Federal Regulations, 2012 CFR

2012-07-01

... Regulations System FEDERAL PROPERTY MANAGEMENT REGULATIONS SUPPLY AND PROCUREMENT 30-FEDERAL CATALOG SYSTEM... personnel in managing these items of supply, a prerequisite for integrated item management under the Federal... 41 Public Contracts and Property Management 2 2012-07-01 2012-07-01 false Scope of part. 101-30...

40 CFR 35.6585 - Cost and price analysis.

Code of Federal Regulations, 2012 CFR

2012-07-01

... 40 Protection of Environment 1 2012-07-01 2012-07-01 false Cost and price analysis. 35.6585 Section 35.6585 Protection of Environment ENVIRONMENTAL PROTECTION AGENCY GRANTS AND OTHER FEDERAL... determination of price reasonableness on a catalog or market price of a commercial product sold in substantial...

48 CFR 46.203 - Criteria for use of contract quality requirements.

Code of Federal Regulations, 2012 CFR

2012-10-01

... 48 Federal Acquisition Regulations System 1 2012-10-01 2012-10-01 false Criteria for use of contract quality requirements. 46.203 Section 46.203 Federal Acquisition Regulations System FEDERAL...) Commercial (described in commercial catalogs, drawings, or industrial standards; see part 2); or (2) Military...

40 CFR 30.12 - Forms for applying for Federal assistance.

Code of Federal Regulations, 2012 CFR

2012-07-01

... particular State can be obtained from EPA or the Catalog of Federal Domestic Assistance. The SPOC shall... 40 Protection of Environment 1 2012-07-01 2012-07-01 false Forms for applying for Federal assistance. 30.12 Section 30.12 Protection of Environment ENVIRONMENTAL PROTECTION AGENCY GRANTS AND OTHER...

41 CFR 101-30.704-2 - Other agencies.

Code of Federal Regulations, 2012 CFR

2012-07-01

... Regulations System FEDERAL PROPERTY MANAGEMENT REGULATIONS SUPPLY AND PROCUREMENT 30-FEDERAL CATALOG SYSTEM 30.7-Item Reduction Program § 101-30.704-2 Other agencies. Civil agencies participating in the Federal... 41 Public Contracts and Property Management 2 2012-07-01 2012-07-01 false Other agencies. 101-30...

22 CFR 145.12 - Forms for applying for Federal assistance.

Code of Federal Regulations, 2012 CFR

2012-04-01

... Catalog of Federal Domestic Assistance. The SPOC shall advise the applicant whether the program for which... 22 Foreign Relations 1 2012-04-01 2012-04-01 false Forms for applying for Federal assistance. 145... Forms for applying for Federal assistance. (a) Department Grants Officers shall comply with the...

41 CFR 101-30.101-1 - Civil agency item.

Code of Federal Regulations, 2012 CFR

2012-07-01

... 41 Public Contracts and Property Management 2 2012-07-01 2012-07-01 false Civil agency item. 101-30.101-1 Section 101-30.101-1 Public Contracts and Property Management Federal Property Management Regulations System FEDERAL PROPERTY MANAGEMENT REGULATIONS SUPPLY AND PROCUREMENT 30-FEDERAL CATALOG SYSTEM 30...

32 CFR 32.12 - Forms for applying for Federal assistance.

Code of Federal Regulations, 2012 CFR

2012-07-01

... or the Catalog of Federal Domestic Assistance. The SPOC shall advise the applicant whether the... 32 National Defense 1 2012-07-01 2012-07-01 false Forms for applying for Federal assistance. 32.12... for Federal assistance. (a) DoD Components shall comply with the applicable report clearance...

77 FR 41195 - Oklahoma; Major Disaster and Related Determinations

Federal Register 2010, 2011, 2012, 2013, 2014

2012-07-12

... eligible to apply for assistance under the Hazard Mitigation Grant Program. The following Catalog of... declaration of a major disaster for the State of Oklahoma (FEMA-4064-DR), dated June 14, 2012, and related determinations. DATES: Effective Date: June 14, 2012. FOR FURTHER INFORMATION CONTACT: Peggy Miller, Office of...

The XCatDB, a Rich 3XMM Catalogue Interface

NASA Astrophysics Data System (ADS)

Michel, L.; Grisé, F.; Motch, C.; Gomez-Moran, A. N.

2015-09-01

The last release of the XMM catalog, the 3XMM-DR4 published in July 2013, is the largest X-ray catalog ever built. It includes lots of data products such as spectra, time series, images, previews, and extractions of archival catalogs matching the position of X-ray sources. The Strasbourg Observatory built an original interface called XCatDB. It was designed to make the best of this wide set of related products with an emphasis on the images. Besides, it offers an easy access to all other catalog parameters. Users can select data with very elaborate queries and can process them with online services such as an X-ray spectral fitting routine. The combination of all these features allows the users to select data of interest to the naked eye as well as to filter catalog parameters. Data selections can be picked out for further scientific analysis thanks to an interface operating external VO clients. The XcatDB has been developed with Saada.

VizieR Online Data Catalog: UV spectra of classical T Tauri stars (France+, 2014)

NASA Astrophysics Data System (ADS)

France, K.; Schindhelm, E.; Bergin, E. A.; Roueff, E.; Abgrall, H.

2017-06-01

We present 16 objects from the larger GTO + DAO T Tauri star samples described by Ardila et al. (2013ApJS..207....1A; focusing on the hot gas emission lines) and France et al. (2012, J/ApJ/756/171; focusing on the molecular circumstellar environment). Eleven of the 16 sources were observed as part of the DAO of Tau guest observing program (PID 11616; PI: G. Herczeg), four were part of the COS Guaranteed Time Observing program on protoplanetary disks (PIDs 11533 and 12036; PI: J. Green), and we have included archival STIS observations of the well-studied CTTS TW Hya (Herczeg et al. 2002ApJ...572..310H, 2004ApJ...607..369H), obtained through StarCAT (Ayres 2010, J/ApJS/187/149). The targets were selected by the availability of reconstructed Lyα spectra, as this emission line is a critical component to the intrinsic CTTS UV radiation field (Schindhelm et al. 2012ApJ...756L..23S) and has not been uniformly included in recent studies of the CTTS radiation field (e.g., Ingleby et al. 2011AJ....141..127I; Yang et al. 2012, J/ApJ/744/121). Most of the targets were observed with the medium-resolution FUV modes of COS (G130M and G160M; Green et al. 2012ApJ...744...60G). (2 data files).

Student Perceptions on Live-Case Projects: Undergraduate Marketing Research

ERIC Educational Resources Information Center

Gundala, Raghava Rao; Singh, Mandeep; Baldwin, Andrew

2014-01-01

This paper is an investigation into undergraduate students' perceptions on use of live projects as a teaching pedagogy in marketing research courses. Students in undergraduate marketing research courses from fall 2009 to spring 2013 completed an online questionnaire consisting of 17 items. The results suggested that student understanding of…

40 CFR 35.936-19 - Small purchases.

Code of Federal Regulations, 2013 CFR

2013-07-01

... 40 Protection of Environment 1 2013-07-01 2013-07-01 false Small purchases. 35.936-19 Section 35.936-19 Protection of Environment ENVIRONMENTAL PROTECTION AGENCY GRANTS AND OTHER FEDERAL ASSISTANCE... these documents and of written quotations received, or references to catalogs or printed price lists...

40 CFR 35.6585 - Cost and price analysis.

Code of Federal Regulations, 2013 CFR

2013-07-01

... 40 Protection of Environment 1 2013-07-01 2013-07-01 false Cost and price analysis. 35.6585 Section 35.6585 Protection of Environment ENVIRONMENTAL PROTECTION AGENCY GRANTS AND OTHER FEDERAL... determination of price reasonableness on a catalog or market price of a commercial product sold in substantial...

48 CFR 46.203 - Criteria for use of contract quality requirements.

Code of Federal Regulations, 2013 CFR

2013-10-01

... 48 Federal Acquisition Regulations System 1 2013-10-01 2013-10-01 false Criteria for use of contract quality requirements. 46.203 Section 46.203 Federal Acquisition Regulations System FEDERAL...) Commercial (described in commercial catalogs, drawings, or industrial standards; see part 2); or (2) Military...

32 CFR 32.12 - Forms for applying for Federal assistance.

Code of Federal Regulations, 2013 CFR

2013-07-01

... or the Catalog of Federal Domestic Assistance. The SPOC shall advise the applicant whether the... 32 National Defense 1 2013-07-01 2013-07-01 false Forms for applying for Federal assistance. 32.12... for Federal assistance. (a) DoD Components shall comply with the applicable report clearance...

22 CFR 145.12 - Forms for applying for Federal assistance.

Code of Federal Regulations, 2013 CFR

2013-04-01

... Catalog of Federal Domestic Assistance. The SPOC shall advise the applicant whether the program for which... 22 Foreign Relations 1 2013-04-01 2013-04-01 false Forms for applying for Federal assistance. 145... Forms for applying for Federal assistance. (a) Department Grants Officers shall comply with the...

40 CFR 30.12 - Forms for applying for Federal assistance.

Code of Federal Regulations, 2013 CFR

2013-07-01

... particular State can be obtained from EPA or the Catalog of Federal Domestic Assistance. The SPOC shall... 40 Protection of Environment 1 2013-07-01 2013-07-01 false Forms for applying for Federal assistance. 30.12 Section 30.12 Protection of Environment ENVIRONMENTAL PROTECTION AGENCY GRANTS AND OTHER...

VizieR Online Data Catalog: 89 Her interferometric study (Hillen+, 2013)

NASA Astrophysics Data System (ADS)

Hillen, M.; Verhoelst, T.; van Winckel, H.; Chesneau, O.; Hummel, C. A.; Monnier, J. D.; Farrington, C.; Tycner, C.; Mourard, D.; Ten Brummelaar, T.; Banerjee, D. P. K.; Zavala, R. T.

2013-08-01

89 Herculis was observed with the AMBER instrument on the VLTI using the Auxiliary Telescopes (ATs) in 2007, 2008, and 2012, all in the low-spectral-resolution (R=30) mode covering the H and K bands with detector integration times (DITs) of 25 and 50ms and without the use of the fringe tracker FINITO. Both the CLASSIC and CLIMB beam combiners on the Georgia State University CHARA Array interferometer were used to conduct observations in the H and K bands.In May 2012 observations were performed with the sensitive two-beam CLASSIC beam combiner in both H and K band. Three-beam CLIMB observations, in H and K band, were also obtained during three nights in July 2012. We retrieved and calibrated observations from the PTI archive. 89 Her was observed during 30 nights between 1999 and 2003, equally spread over the H and K bands. Eight and 15 observations of 89 Her were obtained at the IOTA interferometer on 2003 June 15 and 16, respectively. Observations of 89 Her were carried out in October 2011 with the NPOI. Two observations were performed in June and August 2011 with the Visible spEctroGraph And Polarimeter (VEGA instrument) integrated within the CHARA Array. (2 data files).

“Real-Time” Cosmology with Extragalactic Proper Motions: the Secular Aberration Drift and Evolution of Large-Scale Structure

NASA Astrophysics Data System (ADS)

Truebenbach, Alexandra; Darling, Jeremy

2018-01-01

We present the VLBA Extragalactic Proper Motion Catalog, a catalog of extragalactic proper motions created using archival VLBI data and our own VLBA astrometry. The catalog contains 713 proper motions, with average uncertainties of ~ 24 microarcsec/yr, including 40 new or improved proper motion measurements using relative astrometry with the VLBA. We detect the secular aberration drift – the apparent motion of extragalactic objects caused by the solar system's acceleration around the Galactic Center – at 6.3 sigma significance with an amplitude of 1.69 +/- 0.27 microarcsec/yr and an apex consistent with the Galactic Center (275.2 +/- 10.0 deg, -29.4 +/- 8.8 deg). Our dipole model detects the aberration drift at a higher significance than some previous studies (e.g., Titov & Lambert 2013), but at a lower amplitude than expected or previously measured. We then use the correlated relative proper motions of extragalactic objects to place upper limits on the rate of large-scale structure collapse (e.g., Quercellini et al. 2009; Darling 2013). Pairs of small separation objects that are in gravitationally interacting structures such as filaments of large-scale structure will show a net decrease in angular separation (> - 15.5 microarcsec/yr) as they move towards each other, while pairs of large separation objects that are gravitationally unbound and move with the Hubble expansion will show no net change in angular separation. With our catalog, we place a 3 sigma limit on the rate of convergence of large-scale structure of -11.4 microarcsec/yr for extragalactic objects within 100 comoving Mpc of each other. We also confirm that large separation objects (> 800 comoving Mpc) move with the Hubble flow to within ~ 2.2 microarcsec/yr. In the future, we plan to incorporate the upcoming Gaia proper motions into our catalog to achieve a higher precision measurement of the average relative proper motion of gravitationally interacting extragalactic objects and to refine our measurement of the collapse of large-scale structure. This research was performed with support from the NSF grant AST-1411605.Darling, J. 2013, AJ, 777, L21; Quercellini et al. 2009. Phys. Rev. Lett., 102, 151302; Titov, O. & Lambert, S. 2013, A&A, 559, A95

Creativity, Diversity, and Integration: Radical Change in the Bachelor of Music Curriculum

ERIC Educational Resources Information Center

Myers, David E.

2016-01-01

During 2013-2014, the Task Force on the Undergraduate Music Major of the USA's College Music Society prepared a report entitled "Transforming Music Study from its Foundations: A Manifesto for Progressive Change in the Undergraduate Preparation of Music Majors." The report is a call for increased relevance in undergraduate music studies…

Insights for Academic Developers from Three International Undergraduate Research Program Resources

ERIC Educational Resources Information Center

Allison, Meredith; Miller, Paul

2018-01-01

Undergraduate research is recognized as a high-impact educational practice (Kuh & O'Donnell, 2013), and increasingly it occurs world-wide in higher education, in particular in the United States, United Kingdom, and Australia. In each of these countries, undergraduate research is delivered through a variety of pedagogical approaches that…

22 CFR 226.12 - Forms for applying for Federal assistance.

Code of Federal Regulations, 2012 CFR

2012-04-01

... from the Federal awarding agency or the Catalog of Federal Domestic Assistance. The SPOC shall advise... review. (d) Federal awarding agencies that do not use the SF-424 form should indicate whether the... 22 Foreign Relations 1 2012-04-01 2012-04-01 false Forms for applying for Federal assistance. 226...

31 CFR 205.1 - What Federal assistance programs are covered by this part?

Code of Federal Regulations, 2012 CFR

2012-07-01

...; and (2) All Federal program agencies, except the Tennessee Valley Authority (TVA) and its Federal assistance programs. (b) Only programs listed in the Catalog of Federal Domestic Assistance, as established... 31 Money and Finance:Treasury 2 2012-07-01 2012-07-01 false What Federal assistance programs are...

Evaluation of the Seismic Hazard in Venezuela with a revised seismic catalog that seeks for harmonization along the country borders

NASA Astrophysics Data System (ADS)

Rendon, H.; Alvarado, L.; Paolini, M.; Olbrich, F.; González, J.; Ascanio, W.

2013-05-01

Probabilistic Seismic Hazard Assessment is a complex endeavor that relies on the quality of the information that comes from different sources: the seismic catalog, active faults parameters, strain rates, etc. Having this in mind, during the last several months, the FUNVISIS seismic hazard group has been working on a review and update of the local data base that form the basis for a reliable PSHA calculation. In particular, the seismic catalog, which provides the necessary information that allows the evaluation of the critical b-value, which controls how seismic occurrence distributes with magnitude, has received particular attention. The seismic catalog is the result of the effort of several generations of researchers along the years; therefore, the catalog necessarily suffers from the lack of consistency, homogeneity and completeness for all ranges of magnitude over any seismic study area. Merging the FUNVISIS instrumental catalog with the ones obtained from international agencies, we present the work that we have been doing to produce a consistent seismic catalog that covers Venezuela entirely, with seismic events starting from 1910 until 2012, and report the magnitude of completeness for the different periods. Also, we present preliminary results on the Seismic Hazard evaluation that takes into account such instrumental catalog, the historical catalog, updated known fault geometries and its correspondent parameters, and the new seismic sources that have been defined accordingly. Within the spirit of the Global Earthquake Model (GEM), all these efforts look for possible bridges with neighboring countries to establish consistent hazard maps across the borders.

Engaging actively with issues in the responsible conduct of science: lessons from international efforts are relevant for undergraduate education in the United States.

PubMed

Clements, John D; Connell, Nancy D; Dirks, Clarissa; El-Faham, Mohamed; Hay, Alastair; Heitman, Elizabeth; Stith, James H; Bond, Enriqueta C; Colwell, Rita R; Anestidou, Lida; Husbands, Jo L; Labov, Jay B

2013-01-01

Numerous studies are demonstrating that engaging undergraduate students in original research can improve their achievement in the science, technology, engineering, and mathematics (STEM) fields and increase the likelihood that some of them will decide to pursue careers in these disciplines. Associated with this increased prominence of research in the undergraduate curriculum are greater expectations from funders, colleges, and universities that faculty mentors will help those students, along with their graduate students and postdoctoral fellows, develop an understanding and sense of personal and collective obligation for responsible conduct of science (RCS). This Feature describes an ongoing National Research Council (NRC) project and a recent report about educating faculty members in culturally diverse settings (Middle East/North Africa and Asia) to employ active-learning strategies to engage their students and colleagues deeply in issues related to RCS. The NRC report describes the first phase of this project, which took place in Aqaba and Amman, Jordan, in September 2012 and April 2013, respectively. Here we highlight the findings from that report and our subsequent experience with a similar interactive institute in Kuala Lumpur, Malaysia. Our work provides insights and perspectives for faculty members in the United States as they engage undergraduate and graduate students, as well as postdoctoral fellows, to help them better understand the intricacies of and connections among various components of RCS. Further, our experiences can provide insights for those who may wish to establish "train-the-trainer" programs at their home institutions.

Engaging Actively with Issues in the Responsible Conduct of Science: Lessons from International Efforts Are Relevant for Undergraduate Education in the United States

PubMed Central

Clements, John D.; Connell, Nancy D.; Dirks, Clarissa; El-Faham, Mohamed; Hay, Alastair; Heitman, Elizabeth; Stith, James H.; Bond, Enriqueta C.; Colwell, Rita R.; Anestidou, Lida; Husbands, Jo L.; Labov, Jay B.

2013-01-01

Numerous studies are demonstrating that engaging undergraduate students in original research can improve their achievement in the science, technology, engineering, and mathematics (STEM) fields and increase the likelihood that some of them will decide to pursue careers in these disciplines. Associated with this increased prominence of research in the undergraduate curriculum are greater expectations from funders, colleges, and universities that faculty mentors will help those students, along with their graduate students and postdoctoral fellows, develop an understanding and sense of personal and collective obligation for responsible conduct of science (RCS). This Feature describes an ongoing National Research Council (NRC) project and a recent report about educating faculty members in culturally diverse settings (Middle East/North Africa and Asia) to employ active-learning strategies to engage their students and colleagues deeply in issues related to RCS. The NRC report describes the first phase of this project, which took place in Aqaba and Amman, Jordan, in September 2012 and April 2013, respectively. Here we highlight the findings from that report and our subsequent experience with a similar interactive institute in Kuala Lumpur, Malaysia. Our work provides insights and perspectives for faculty members in the United States as they engage undergraduate and graduate students, as well as postdoctoral fellows, to help them better understand the intricacies of and connections among various components of RCS. Further, our experiences can provide insights for those who may wish to establish “train-the-trainer” programs at their home institutions. PMID:24297287

The first AGILE low-energy (< 30 MeV) Terrestrial Gamma-ray Flashes catalog

NASA Astrophysics Data System (ADS)

Marisaldi, Martino; Fuschino, Fabio; Pittori, Carlotta; Verrecchia, Francesco; Giommi, Paolo; Tavani, Marco; Dietrich, Stefano; Price, Colin; Argan, Andrea; Labanti, Claudio; Galli, Marcello; Longo, Francesco; Del Monte, Ettore; Barbiellini, Guido; Giuliani, Andrea; Bulgarelli, Andrea; Gianotti, Fulvio; Trifoglio, Massimo; Trois, Alessio

2014-05-01

We present the first catalog of Terrestrial Gamma-ray Flashes (TGFs) detected by the Minicalorimeter (MCAL) instrument on-board the AGILE satellite. The catalog includes 308 TGFs detected during the period March 2009 - July 2012 in the +/- 2.5° latitude band and selected to have the maximum photon energy up to 30 MeV. The characteristics of the AGILE events are analysed and compared to the observational framework established by the two other currently active missions capable of detecting TGFs from space, RHESSI and Fermi. A detailed model of the MCAL dead time is presented, which is fundamental to properly interpret our observations, particularly concerning duration, intensity and correlation with lightning sferics detected by the World Wide Lightning Location Network. The TGFs cumulative spectrum supports a low production altitude, in agreement with previous measurements. The AGILE TGF catalog below 30 MeV is publicly accessible online at the website of the ASI Science Data Center (ASDC) http://www.asdc.asi.it/mcaltgfcat/ In addition to the TGF sample properties we also present the catalog website functionalities available to users.

78 FR 24395 - Applications for New Awards; Training and Information for Parents of Children With Disabilities...

Federal Register 2010, 2011, 2012, 2013, 2014

2013-04-25

... DEPARTMENT OF EDUCATION Applications for New Awards; Training and Information for Parents of... applications for new awards for fiscal year (FY) 2013. Catalog of Federal Domestic Assistance (CFDA) Number: 84... Individuals with Disabilities Education Act (IDEA)). Absolute Priority: For FY 2013 and any subsequent year in...

31 CFR 205.1 - What Federal assistance programs are covered by this part?

Code of Federal Regulations, 2013 CFR

2013-07-01

...; and (2) All Federal program agencies, except the Tennessee Valley Authority (TVA) and its Federal assistance programs. (b) Only programs listed in the Catalog of Federal Domestic Assistance, as established... 31 Money and Finance:Treasury 2 2013-07-01 2013-07-01 false What Federal assistance programs are...

22 CFR 226.12 - Forms for applying for Federal assistance.

Code of Federal Regulations, 2013 CFR

2013-04-01

... from the Federal awarding agency or the Catalog of Federal Domestic Assistance. The SPOC shall advise... review. (d) Federal awarding agencies that do not use the SF-424 form should indicate whether the... 22 Foreign Relations 1 2013-04-01 2013-04-01 false Forms for applying for Federal assistance. 226...

Aircraft Measurements for Understanding Air-Sea Coupling and Improving Coupled Model Predictions Over the Indian Ocean

DTIC Science & Technology

2012-09-30

briefing for aircraft operations in Diego Garcia, reports posted on EOL field catalog in realtime (http://catalog.eol.ucar.edu/cgi- bin/dynamo/report...index); • Dropsonde data processing on all P3 flights and realtime QC/reporting to GTS; and • Science summary of aircraft missions posted on EOL ...data analysis, worked with EOL on data quality control (QC), participated in the DYNAMO Sounding Workshop at EOL /NCAR from 6-7 February 2012

Comparing Foreshock Characteristics and Foreshock Forecasting in Observed and Simulated Earthquake Catalogs

NASA Astrophysics Data System (ADS)

Ogata, Y.

2014-12-01

In our previous papers (Ogata et al., 1995, 1996, 2012; GJI), we characterized foreshock activity in Japan, and then presented a model that forecasts the probability that one or more earthquakes form a foreshock sequence; then we tested prospectively foreshock probabilities in the JMA catalog. In this talk, I compare the empirical results with results for synthetic catalogs in order to clarify whether or not these results are consistent with the description of the seismicity by a superposition of background activity and epidemic-type aftershock sequences (ETAS models). This question is important, because it is still controversially discussed whether the nucleation process of large earthquakes is driven by seismically cascading (ETAS-type) or by aseismic accelerating processes. To explore the foreshock characteristics, I firstly applied the same clustering algorithms to real and synthetic catalogs and analyzed the temporal, spatial and magnitude distributions of the selected foreshocks, to find significant differences particularly in the temporal acceleration and magnitude dependence. Finally, I calculated forecast scores based on a single-link cluster algorithm which could be appropriate for real-time applications. I find that the JMA catalog yields higher scores than all synthetic catalogs and that the ETAS models having the same magnitude sequence as the original catalog performs significantly better (more close to the reality) than ETAS-models with randomly picked magnitudes.

The Pan-STARRS data server and integrated data query tool

NASA Astrophysics Data System (ADS)

Guo, Jhen-Kuei; Chen, Wen-Ping; Lin, Chien-Cheng; Chen, Ying-Tung; Lin, Hsing-Wen

2013-06-01

The Pan-STARRS project is operated by an international consortium. Located in Haleakala, Hawaii, the Pan-STARRS telescope system patrols the entire visible sky several times a month, with an aim to identify and characterize varying celestial objects of phenomena or in brightness (supernovae, novae, variable stars, etc) or in position (comets, asteroids, near-earth objects, X-planet etc.) PS1 science mission has started officially from May, 2010 and expects to end in the end of 2013. As of early 2012, every patch of sky observable from Hawaii has been observed in at least 5 bands (g', r', i', z', y') for 5 to 40 epochs. We have set up a data depository at NCU to serve the users in Taiwan. The massive amounts of Pan-STARRS data are downloaded via Internet from the Institute for Astronomy, University of Hawaii whenever new observations are obtained and processed. So far we have stored a total of 200 TB worth of data. In addition to star/galaxy catalogs, a postage stamp server provides access to FITS images. The Pan-STARRS Published Science Products Subsystem (PSPS) has recently passed its operational readiness, that provides users to query individual PS1 measurements. Here we present the data query tool to interface with the PS1 catalogs and postage stamp images, together with other complementary databases such as 2MASS and other data at IRSA (NASA/IPAC Infrared Science Archive).

VizieR Online Data Catalog: SNLS and SDSS SN surveys photometric calibration (Betoule+, 2013)

NASA Astrophysics Data System (ADS)

Betoule, M.; Marriner, J.; Regnault, N.; Cuillandre, J.-C.; Astier, P.; Guy, J.; Balland, C.; El, Hage P.; Hardin, D.; Kessler, R.; Le Guillou, L.; Mosher, J.; Pain, R.; Rocci, P.-F.; Sako, M.; Schahmaneche, K.

2012-11-01

We present a joined photometric calibration for the SNLS and the SDSS supernova surveys. Our main delivery are catalogs of natural AB magnitudes for a large set of selected tertiary standard stars covering the science field of both surveys. Those catalogs are calibrated to the AB flux scale through observations of 5 primary spectrophotometric standard stars, for which HST-STIS spectra are available in the CALSPEC database. The estimate of the uncertainties associated to this calibration are delivered as a single covariance matrix. We also provide a model of the transmission efficiency of the SNLS photometric instrument MegaCam. Those transmission functions are required for the interpretation of MegaCam natural magnitudes in term of physical fluxes. Similar curves for the SDSS photometric instrument have been published in Doi et al. (2010AJ....139.1628D). Last, we release the measured magnitudes of the five CALSPEC standard stars in the magnitude system of the tertiary catalogs. This makes it possible to update the calibration of the tertiary catalogs if CALSPEC spectra for the primary standards are revised. (11 data files).

31 CFR 205.3 - What Federal assistance programs are subject to this subpart A?

Code of Federal Regulations, 2012 CFR

2012-07-01

... programs which: (1) Are listed in the Catalog of Federal Domestic Assistance; (2) Meet the funding... Federal assistance programs subject to subpart A if a State or Federal Program Agency fails to comply with... 31 Money and Finance:Treasury 2 2012-07-01 2012-07-01 false What Federal assistance programs are...

Discovery of Very High Energy Gamma-Ray Emission from Rbs 0723 with the Magic Telescopes

NASA Astrophysics Data System (ADS)

Mirzoyan, Razmik

2014-01-01

The MAGIC collaboration reports the discovery of very high energy (VHE; E>100 GeV) gamma-ray emission from RBS 0723 (RA: 08:47:12.9 DEC: +11:33:50, J2000.0) RBS 0723 is a BL Lac object at redshift z=0.198. The source has been detected by Fermi-LAT, in the Second Fermi-LAT source Catalogue (2FGL; Nolan et al. 2012) with F(>1 GeV) = (5.3+-1.2)e-10 cm^-2 s^-1 and with photon index 1.48+-0.16. It also belongs to the first Fermi-LAT catalog of >10 GeV sources (1FHL; Ackermann et al, 2013), showing a hard (photon index = 1.4 +- 0.4) and bright (photon flux = 9.6e-11 ph cm^-2 s^-1) emission above 10 GeV, and identified as a good candidate for VHE detection.

VizieR Online Data Catalog: Giant molecular clouds in nearby galaxies (Donovan Meyer+, 2013)

NASA Astrophysics Data System (ADS)

Donovan Meyer, J.; Koda, J.; Momose, R.; Mooney, T.; Egusa, F.; Carty, M.; Kennicutt, R.; Kuno, N.; Rebolledo, D.; Sawada, T.; Scoville, N.; Wong, T.

2015-02-01

The CO(J=1-0) observations presented in this paper were taken as part of the CANON CO(1-0) Survey, in which data from the Combined Array for Research in Millimeter Astronomy (CARMA) and Nobeyama Radio Observatory 45m (NRO45) single dish telescope are combined to image the central regions of nearby spiral galaxies (J. Koda et al., in preparation). We observe all galaxies in the (J=1-0) transition of 12CO with CARMA in the C and D configurations. The observations presented in this paper were taken from early 2007 through 2012 March. To achieve accurate total flux measurements, we also observe the galaxies using the Beam Array Receiver System (BEARS) instrument on the NRO45 single dish telescope. The total bandwidth is 265MHz, and we smooth the 500kHz velocity resolution to 5.08km/s to match the CARMA data. (2 data files).

VizieR Online Data Catalog: Extrasolar planet HD 189733b whitelight curve (Crouzet+, 2014)

NASA Astrophysics Data System (ADS)

Crouzet, N.; McCullough, P. R.; Deming, D.; Madhusudhan, N.

2017-05-01

We used HST WFC3 with the newly implemented spatial scanning mode, developed in part to enable observations such as these (McCullough & MacKenty, 2012wfc..rept....8M). In this mode, a controlled scan is applied to the telescope during the exposure in a direction perpendicular to the wavelength dispersion direction (Figure 1). This technique is particularly efficient for bright stars such as HD 189733 (see McCullough et al. 2014ApJ...791...55M, for more details). One eclipse of HD 189733b was observed on 2013 June 24. The observations are divided into five HST orbits, the planetary eclipse occurring during the fourth orbit. In total, 159 exposures of 5.97 s each were acquired, corresponding to 32 exposures per orbit (except for the first orbit in which the first image is a direct image). (1 data file).

VizieR Online Data Catalog: Transits of HAT-P-16 and WASP-21 (Ciceri+, 2013)

NASA Astrophysics Data System (ADS)

Ciceri, S.; Mancini, L.; Southworth, J.; Nikolov, N.; Bozza, V.; Bruni, I.; Calchi Novati, S.; D'Ago, G.; Henning, T.

2013-07-01

For both planetary systems, we observed one transit event simultaneously with two telescopes (Figs. 1 and 2). These observations were carried out between September and October 2012 with the 1.52m Cassini telescope from the Loiano observatory and with the 1.23m Calar Alto telescope. An additional transit of HAT-P-16 was observed on October 29th 2010 from Loiano during the PLAN microlensing campaign towards M31 (Calchi Novati et al. 2009ApJ...695..442N, 2010ApJ...717..987C). Another transit of HAT-P-16 was observed in Calar Alto on August 22th 2011. In total we present six new light curves, five of them being from defocussed 1.2-1.5m telescopes (see table 1). File contain the data used to plot the lightcurves in Fig. 3 and 4 in the paper. (7 data files).

An Analysis of the FY-1C, Iridium 33, and Cosmos 2251 Fragments

NASA Technical Reports Server (NTRS)

Liou, J.-C.

2014-01-01

The beginning of the year 2013 marks the sixth anniversary of the destruction of the Fengyun-1C (FY-1C) weather satellite as the result of an anti-satellite test conducted by China in January 2007 and the fourth anniversary of the accidental collision between Cosmos 2251 and the operational Iridium 33 in February 2009. These two events represent the worst satellite breakups in history. A total of 5579 fragments have been cataloged by the U.S. Space Surveillance Network (SSN), and almost 5000 of them were still in orbit in January 2013. In addition to these cataloged objects, hundreds of thousands (or more) of fragments down to the millimeter size regime were also generated during the breakups. These fragments are too small to be tracked by the SSN, but are large enough to be a safety concern for human space activities and robotic missions in low Earth orbit (LEO, the region below 2000 km altitude). Like their cataloged siblings, many of them remain in orbit today. These two breakup events dramatically changed the landscape of the orbital debris environment in LEO. The spatial density of the cataloged population in January 2013 is shown as the top blue curve. The combined FY-1C, Iridium 33, and Cosmos 2251 fragments (black curve) account for about 50 percent of the cataloged population below an altitude of 1000 km. They are also responsible for the concentrations at 770 km and 850 km, altitudes at which the collisions occurred. The effects of the FY-1C, Iridium 33, and Cosmos 2251 fragments will continue to be felt for decades to come. For example, approximately half of the generated FY-1C fragments will remain in orbit 20 years from now. In general, the Iridium 33 and Cosmos 2251 fragments will decay faster than the FY-1C fragments because of their lower altitudes. Of the Iridium 33 and Cosmos 2251 fragments, the former have much shorter orbital lifetimes than the latter, because lightweight composite materials were heavily used in the construction of the Iridium vehicle, leading to the higher area-to-mass ratios of the fragments.

Japan unified hIgh-resolution relocated catalog for earthquakes (JUICE): Crustal seismicity beneath the Japanese Islands

NASA Astrophysics Data System (ADS)

Yano, Tomoko E.; Takeda, Tetsuya; Matsubara, Makoto; Shiomi, Katsuhiko

2017-04-01

We have generated a high-resolution catalog called the ;Japan Unified hIgh-resolution relocated Catalog for Earthquakes; (JUICE), which can be used to evaluate the geometry and seismogenic depth of active faults in Japan. We relocated > 1.1 million hypocenters from the NIED Hi-net catalog for events which occurred between January 2001 and December 2012, to a depth of 40 km. We apply a relative hypocenter determination method to the data in each grid square, in which entire Japan is divided into 1257 grid squares to parallelize the relocation procedure. We used a double-difference method, incorporating cross-correlating differential times as well as catalog differential times. This allows us to resolve, in detail, a seismicity distribution for the entire Japanese Islands. We estimated location uncertainty by a statistical resampling method, using Jackknife samples, and show that the uncertainty can be within 0.37 km in the horizontal and 0.85 km in the vertical direction with a 90% confidence interval for areas with good station coverage. Our seismogenic depth estimate agrees with the lower limit of the hypocenter distribution for a recent earthquake on the Kamishiro fault (2014, Mj 6.7), which suggests that the new catalog should be useful for estimating the size of future earthquakes for inland active faults.

31 CFR 205.3 - What Federal assistance programs are subject to this subpart A?

Code of Federal Regulations, 2013 CFR

2013-07-01

... programs which: (1) Are listed in the Catalog of Federal Domestic Assistance; (2) Meet the funding... Federal assistance programs subject to subpart A if a State or Federal Program Agency fails to comply with... 31 Money and Finance:Treasury 2 2013-07-01 2013-07-01 false What Federal assistance programs are...

Version 1 of the Hubble Source Catalog

DOE PAGES

Whitmore, Bradley C.; Allam, Sahar S.; Budavari, Tamas; ...

2016-05-11

The Hubble Source Catalog is designed to help optimize science from the Hubble Space Telescope by combining the tens of thousands of visit-based source lists in the Hubble Legacy Archive into a single master catalog. Version 1 of the Hubble Source Catalog includes WFPC2, ACS/WFC, WFC3/UVIS, and WFC3/IR photometric data generated using SExtractor software to produce the individual source lists. The catalog includes roughly 80 million detections of 30 million objects involving 112 different detector/filter combinations, and about 160 thousand HST exposures. Source lists from Data Release 8 of the Hubble Legacy Archive are matched using an algorithm developed by Budavari & Lubow (2012). The mean photometric accuracy for the catalog as a whole is better than 0.10 mag, with relative accuracy as good as 0.02 mag in certain circumstances (e.g., bright isolated stars). The relative astrometric residuals are typically within 10 mas, with a value for the mode (i.e., most common value) of 2.3 mas. The absolute astrometric accuracy is better thanmore » $$\\sim$$0.1 arcsec for most sources, but can be much larger for a fraction of fields that could not be matched to the PanSTARRS, SDSS, or 2MASS reference systems. In this paper we describe the database design with emphasis on those aspects that enable the users to fully exploit the catalog while avoiding common misunderstandings and potential pitfalls. Here, we provide usage examples to illustrate some of the science capabilities and data quality characteristics, and briefly discuss plans for future improvements to the Hubble Source Catalog.« less

VizieR Online Data Catalog: List of Telescope Array events with E > 57EeV (Abbasi+, 2014)

NASA Astrophysics Data System (ADS)

Abbasi, R. U.; Abe, M.; Abu-Zayyad, T.; Allen, M.; Anderson, R.; Azuma, R.; Barcikowski, E.; Belz, J. W.; Bergman, D. R.; Blake, S. A.; Cady, R.; Chae, M. J.; Cheon, B. G.; Chiba, J.; Chikawa, M.; Cho, W. R.; Fujii, T.; Fukushima, M.; Goto, T.; Hanlon, W.; Hayashi, Y.; Hayashida, N.; Hibino, K.; Honda, K.; Ikeda, D.; Inoue, N.; Ishii, T.; Ishimori, R.; Ito, H.; Ivanov, D.; Jui, C. C. H.; Kadota, K.; Kakimoto, F.; Kalashev, O.; Kasahara, K.; Kawai, H.; Kawakami, S.; Kawana, S.; Kawata, K.; Kido, E.; Kim, H. B.; Kim, J. H.; Kitamura, S.; Kitamura, Y.; Kuzmin, V.; Kwon, Y. J.; Lan, J.; Lim, S. I.; Lundquist, J. P.; Machida, K.; Martens, K.; Matsuda, T.; Matsuyama, T.; Matthews, J. N.; Minamino, M.; Mukai, K.; Myers, I.; Nagasawa, K.; Nagataki, S.; Nakamura, T.; Nonaka, T.; Nozato, A.; Ogio, S.; Ogura, J.; Ohnishi, M.; Ohoka, H.; Oki, K.; Okuda, T.; Ono, M.; Oshima, A.; Ozawa, S.; Park, I. H.; Pshirkov, M. S.; Rodriguez, D. C.; Rubtsov, G.; Ryu, D.; Sagawa, H.; Sakurai, N.; Sampson, A. L.; Scott, L. M.; Shah, P. D.; Shibata, F.; Shibata, T.; Shimodaira, H.; Shin, B. K.; Smith, J. D.!; Sokolsk, Y. P.; Springer, R. W.; Stokes, B. T.; Stratton, S. R.; Stroman, T. A.; Suzawa, T.; Takamura, M.; Takeda, M.; Takeishi, R.; Taketa, A.; Takita, M.; Tameda, Y.; Tanaka, H.; Tanaka, K.; Tanaka, M.; Thomas, S. B.; Thomson, G. B.; Tinyakov, P.; Tkachev, I.; Tokuno, H.; Tomida, T.; Troitsky, S.; Tsunesada, Y.; Tsutsumi, K.; Uchihori, Y.; Udo, S.; Urban, F.; Vasiloff, G.; Wong, T.; Yamane, R.; Yamaoka, H.; Yamazaki, K.; Yang, J.; Yashiro, K.; Yoneda, Y.; Yoshida, S.; Yoshii, H.; Zollinger, R.; Zundel, Z.

2017-03-01

The TA is the largest cosmic-ray detector in the northern hemisphere. It consists of a scintillator SD array (Abu-Zayyad et al. 2012NIMPA.689...87A) and three fluorescence detector (FD) stations (Tokuno et al. 2012NIMPA.676...54T). The observatory has been in full operation in Millard Country, Utah, USA (39fdg30N, 112fdg91W; about 1400 m above sea level) since 2008. The TA SD array consists of 507 plastic scintillation detectors each 3 m2 in area and located on a 1.2 km square grid. The array has an area of ~700 km2. The TA SD array observes cosmic-ray-induced extensive air showers with E > ~1 EeV, regardless of weather conditions with a duty cycle near 100% and a wide field of view (FoV). These capabilities ensure a very stable and large geometrical exposure over the northern sky survey in comparison with FD observations that have a duty cycle of ~10%. In this analysis, we used SD data recorded between 2008 May 11 and 2013 May 4. (1 data file).

Detailed spatiotemporal evolution of microseismicity and repeating earthquakes following the 2012 Mw 7.6 Nicoya earthquake

NASA Astrophysics Data System (ADS)

Yao, Dongdong; Walter, Jacob I.; Meng, Xiaofeng; Hobbs, Tiegan E.; Peng, Zhigang; Newman, Andrew V.; Schwartz, Susan Y.; Protti, Marino

2017-01-01

We apply a waveform matching technique to obtain a detailed earthquake catalog around the rupture zone of the 5 September 2012 moment magnitude 7.6 Nicoya earthquake, with emphasis on its aftershock sequence. Starting from a preliminary catalog, we relocate 7900 events using TomoDD to better quantify their spatiotemporal behavior. Relocated aftershocks are mostly clustered in two groups. The first is immediately above the major coseismic slip patch, partially overlapping with shallow afterslip. The second one is 50 km SE to the main shock nucleation point and near the terminus of coseismic rupture, in a zone that exhibited little resolvable afterslip. Using the relocated events as templates, we scan through the continuous recording from 29 June 2012 to 30 December 2012, detecting approximately 17 times more than template events. We find 190 aftershocks in the first half hour following the main shock, mostly along the plate interface. Later events become more scattered in location, showing moderate expansion in both along-trench and downdip directions. From the detected catalog we identify 53 repeating aftershock clusters with mean cross-correlation values larger than 0.9, and indistinguishably intracluster event locations, suggesting slip on the same fault patch. Most repeating clusters occurred within the first major aftershock group. Very few repeating clusters were found in the aftershock grouping along the southern edge of the Peninsula, which is not associated with substantial afterslip. Our observations suggest that loading from nearby afterslip along the plate interface drives spatiotemporal evolution of aftershocks just above the main shock rupture patch, while aftershocks in the SE group are to the SE of the observed updip afterslip and poorly constrained.

Status of personal health requirement for graduation at institutions of higher education in the United States.

PubMed

Henry, Dayna S; Aydt Klein, Nicole; Kempland, Monica; Rose Oswalt, Sarah; Rexilius, Molly A

2017-01-01

The purpose of this study was to examine the proportion of higher education institutions in the United States that require a personal health course (PHC) for graduation and to describe the nature of such requirements. Participants: This study included a random sample of public and private institutions of higher education (IHE) with undergraduate programs within the United States (N = 310). Data were collected between September 2014 and May 2015. University catalogs were accessed from the institutions' public Web sites to determine whether a PHC was offered, and whether it was exclusively or optionally required for graduation. The majority (55.8%) of the sample offered at least 1 PHC, with only 10% exclusively requiring the course and an additional 10% optionally required the course. Although the utility of undergraduate students completing a PHC is clear, the majority of institutions do not require such a course for degree conferral.

VizieR Online Data Catalog: i filter photometry for HATS-25 through HATS-30 (Espinoza+, 2016)

NASA Astrophysics Data System (ADS)

Espinoza, N.; Bayliss, D.; Hartman, J. D.; Bakos, G. A.; Jordan, A.; Zhou, G.; Mancini, L.; Brahm, R.; Ciceri, S.; Bhatti, W.; Csubry, Z.; Rabus, M.; Penev, K.; Bento, J.; de Val-Borro, M.; Henning, T.; Schmidt, B.; Suc, V.; Wright, D. J.; Tinney, C. G.; Tan, T. G.; Noyes, R.

2017-05-01

The photometric detection data of the six exoplanets come from the three HATSouth sites, namely, the site at Las Campanas Observatory in Chile (LCO, whose stations are designated HS-1 and HS-2), the site at of the High Energy Spectroscopic Survey (HESS) in Namibia (whose stations are designated HS-3 and HS-4) and the site at the Siding Spring Observatory (SSO) in Australia whose stations are designated HS-5 and HS-6). HATS-25 was observed with an r SDSS filter on 2011 Mar-2011 Aug using HS-2.1, on 2011 Jul-2011 Aug using HS-4.1, and on 2011 May with HS-6.1. HATS-26 was observed with an r SDSS filter on 2012 Feb-2012 Jun using HS-2.3, HS-4.3, and HS-6.3. HATS-27 was observed with an r SDSS filter on 2011 Apr-2012 Jul using HS-2.1, on 2011 Jul-2012 Jul using HS-4.1, and on 2011 May-2012 Jul using HS-6.1. HATS-28 was observed with an r SDSS filter on 2013 Mar-2013 Oct using HS-1.2, on 2013 Sep-2013 Oct using HS-2.2, on 2013 Apr-2013 Nov using HS-3.2, on 2013 Sep-2013 Nov using HS-4.2 and HS-6.2, and 2013 Mar-2013 Nov using HS-5.2. HATS-29 was observed with an r SDSS filter on 2013 Apr-2013 May using HS-1.1, on 2013 Sep-2013 Oct using HS-2.1, on 2013 Apr-2013 Nov using HS-3.1, on 2013 Sep-2013 Nov using HS-4.1 and HS-6.1, and on 2013 Mar-2013 Nov using HS-5.1. HATS-30 was observed using an r SDSS filter on 2012 Sep-2012 Dec using HS-2.3, HS-6.3 and HS-2.4, on 2012 Sep-2013 Jan using HS-4.4, on 2012 Sep-2012 Dec using HS-6.4, and on 2011 Jul-2012 Oct using HS-1.1, HS-3.1 and HS-5.1. Photometric follow-up for the six systems was obtained mainly from 1m-class telescopes at different sites of the Las Cumbres Observatory Global Telescope (LCOGT) network, using the i filter. In particular, one partial transit and a full transit was observed for HATS-25b on 2015 February 23 at Cerro Tololo Inter-American Observatory (CTIO) and 2015 March 16 at SSO, respectively; three partial transits were observed for HATS-26b on 2015 April 19 and 2015 May 21 at CTIO, and 2015 June 04 at SSO; one full transit was observed for HATS-27b on 2015 April 09 at SSO; two partial transits were observed for HATS-28b on 2015 August 31 and 2015 September 03 at CTIO; one full transit and a partial transit were observed for HATS-29b on 2015 and 2014 June, respectively, at CTIO; and two partial transits were observed for HATS-30b on 2014 October 19 at South African Astronomical Observatory (SAAO) and on 2014 Oct 23 at CTIO. In addition, one full transit of HATS-27b was observed using the 0.3m Perth Exoplanet Survey Telescope (PEST) on 2015 March 12 using a RC filter. The reconnaissance spectroscopy of our candidates was made using the Wide Field Spectrograph (WiFeS), located on the Australian National University (ANU) 2.3m telescope. The observing strategy usually consists of taking data with two resolutions: R=λ/Δλ=7000 (medium) and R=3000 (low). For HATS-25, four medium resolution spectra (2014 Jun-Aug) and one low resolution spectrum (2014 Aug 5) were obtained. For HATS-26, two medium resolution spectra (2014 Jun 3-5) and one low resolution spectrum (2014 Jun 4) were obtained. For HATS-27, three medium resolution (2014 Jun 3-5) and one low resolution (2014 Jun 2) spectra were obtained. For HATS-28, only one low resolution spectrum (2015 Jun 1) was obtained. For HATS-29, four medium resolution spectra (2014 Dec-2015 Mar) and one low resolution spectrum (2015 Mar 2) were obtained. For HATS-30, three medium resolution spectra (2014 Oct 4-10) and one low resolution spectrum (2014 Oct 4) were obtained. High-precision spectroscopy was obtained for our targets with different instruments. Several R=115000 spectra were taken with the High Accuracy Radial Velocity Planet Searcher (HARPS) on the ESO 3.6m telescope at La Silla Observatory (LSO) between 2015 February and 2016 March in order to obtain high-precision radial velocities for HATS-25, HATS-26, HATS-27, and HATS-29. Spectra with R=48000 were also taken with the Fiber-fed Extended Range Optical Spectrograph (FEROS) mounted on the Max Planck Gesellschaft (MPG) 2.2m telescope at La Silla Observatory (LSO) between 2014 July and 2015 July in order to both extract precise spectroscopic parameters of the host stars and obtain precise radial velocities for all of our targets. In addition, R=60000 spectra were also taken with the CORALIE spectrograph mounted on the 1.2m Euler telescope at LSO between 2014 June and November for HATS-26, HATS-27, HATS-29, and HATS-30. Finally, eight R=70000 spectra were obtained for HATS-29 on 2015 May to measure radial velocities, using the CYCLOPS2 fiber feed with the University College London Echelle Spectrograph (UCLES) on the 3.9m Anglo-Australian Telescope (AAT). (3 data files).

VizieR Online Data Catalog: Candidate strong lens systems from DES obs. (Diehl+, 2017)

NASA Astrophysics Data System (ADS)

Diehl, H. T.; Buckley-Geer, E. J.; Lindgren, K. A.; Nord, B.; Gaitsch, H.; Gaitsch, S.; Lin, H.; Allam, S.; Collett, T. E.; Furlanetto, C.; Gill, M. S. S.; More, A.; Nightingale, J.; Odden, C.; Pellico, A.; Tucker, D. L.; da Costa, L. N.; Neto, A. F.; Kuropatkin, N.; Soares-Santos, M.; Welch, B.; Zhang, Y.; Frieman, J. A.; Abdalla, F. B.; Annis, J.; Benoit-Levy, A.; Bertin, E.; Brooks, D.; Burke, D. L.; Rosell, A. C.; Kind, M. C.; Carretero, J.; Cunha, C. E.; D'Andrea, C. B.; Desai, S.; Dietrich, J. P.; Drlica-Wagner, A.; Evrard, A. E.; Finley, D. A.; Flaugher, B.; Garcia-Bellido, J.; Gerdes, D. W.; Goldstein, D. A.; Gruen, D.; Gruendl, R. A.; Gschwend, J.; Gutierrez, G.; James, D. J.; Kuehn, K.; Kuhlmann, S.; Lahav, O.; Li, T. S.; Lima, M.; Maia, M. A. G.; Marshall, J. L.; Menanteau, F.; Miquel, R.; Nichol, R. C.; Nugent, P.; Ogando, R. L. C.; Plazas, A. A.; Reil, K.; Romer, A. K.; Sako, M.; Sanchez, E.; Santiago, B.; Scarpine, V.; Schindler, R.; Schubnell, M.; Sevilla-Noarbe, I.; Sheldon, E.; Smith, M.; Sobreira, F.; Suchyta, E.; Swanson, M. E. C.; Tarle, G.; Thomas, D.; Walker, A. R.; DES Collaboration

2017-10-01

The Dark Energy Survey (DES) is in the midst of imaging 5000°2 of the southern galactic cap using the Dark Energy Camera (DECam), which is operated on the 4m Victor M. Blanco Telescope at Cerro Tololo Interamerican Observatory (CTIO) near La Serena, Chile. Science verification (SV) spanned 79 nights or half-nights from 2012 November 1, to 2013 February 22. The main SV wide-field (WF) survey areas amounted to ~250°2 at non-uniform depth and data quality. The first full observing season, Year 1 (Y1), spanned 119 nights or half-nights from 2013 August 31 to 2014 February 9. The Y1 wide-field (WF) survey observations were concentrated in two areas: one of about 150°2 near the celestial equator that included a part of SDSS Stripe 82 (Annis+ 2014ApJ...794..120A), and a much larger region of roughly 1800°2 from -60° to -40° decl. that overlapped the area mapped in microwaves by the South Pole Telescope (SPT). Generally, we observed those fields four times in each of the five filters: the g, r, i, z, and Y-bands. (2 data files).

VizieR Online Data Catalog: Activity and rotation in Praesepe and the Hyades (Douglas+, 2014)

NASA Astrophysics Data System (ADS)

Douglas, S. T.; Agueros, M. A.; Covey, K. R.; Bowsher, E. C.; Bochanski, J. J.; Cargile, P. A.; Kraus, A.; Law, N. M.; Lemonias, J. J.; Arce, H. G.; Fierroz, D. F.; Kundert, A.

2017-05-01

Kraus & Hillenbrand (2007, J/AJ/134/2340) calculated proper motions and photometry for several million objects within 7° of the center of Praesepe. The resulting catalog includes 1128 candidate cluster members with membership probabilities Pmem>50%. As in Paper I (Agueros et al. 2011ApJ...740..110A), we supplement this catalog with 41 known members that are too bright to be identified as members by Kraus & Hillenbrand (2007, J/AJ/134/2340). For the Hyades, we adopt the Roser et al. (2011, J/A+A/531/A92) membership catalog. These authors identified candidate Hyades members via the convergent point method and confirmed membership using photometry. We used the MDM Observatory Modular Spectrograph (ModSpec) on the Hiltner 2.4 m telescope to obtain spectra of stars in Praesepe and the Hyades over the course of five multi-night runs between 2010 December 2 and 2012 November 14. (2 data files).

Roster of Astronomy Departments with Enrollment and Degree Data, 2014: Results from the 2014 Survey of Enrollments and Degrees. Focus On

ERIC Educational Resources Information Center

Nicholson, Starr; Mulvey, Patrick J.

2015-01-01

Undergraduate astronomy enrollments in the US continue to rise with junior and senior level enrollments exceeding the previous year's all-time high. The increasing undergraduate enrollments have produced 428 bachelor's in the 2013-14 academic year, also an all-time high. Undergraduate astronomy degree production will continue to rise given the…

"I don't want to grow up, I'm a [Gen X, Y, Me] kid": Increasing maturity fears across the decades.

PubMed

Smith, April R; Bodell, Lindsay P; Holm-Denoma, Jill; Joiner, Thomas E; Gordon, Kathryn H; Perez, Marisol; Keel, Pamela K

2017-11-01

The current studies examined the hypothesis that maturity fears are increasing among undergraduate men and women from the United States over time. Study 1 used a time-lag method to assess generational effects of maturity fears among a large sample (n = 3,291) of undergraduate men and women assessed in 1982, 1992, 2002, and 2012. Results revealed that both men and women reported significantly higher rates of maturity fears across time. Study 2 replicated these findings, and used a more restricted time frame to more closely examine the rate of change. Undergraduate women (n = 554) were assessed in 2001, 2003, 2009, and 2012. Maturity fears were again found to increase from 2001 to 2012. Recent cohorts of emerging adults seem more reluctant to mature than previous cohorts. Many contributing factors may be at play, including challenging economic times, social pressures to remain youthful, and/or internal fears of assuming increased responsibility.

VizieR Online Data Catalog: SDSS-DR8 galaxies classified by WND-CHARM (Kuminski+, 2016)

NASA Astrophysics Data System (ADS)

Kuminski, E.; Shamir, L.

2016-06-01

The image analysis method used to classify the images is WND-CHARM (wndchrm; Shamir et al. 2008, BMC Source Code for Biology and Medicine, 3: 13; 2010PLSCB...6E0974S; 2013ascl.soft12002S), which first computes 2885 numerical descriptors from each SDSS image such as textures, edges, shapes), the statistical distribution of the pixel intensities, the polynomial decomposition of the image, and fractal features. These features are extracted from the raw pixels, as well as the image transforms and multi-order image transforms. See section 2 for further explanations. In a similar way than the catalog we also compiled a catalog of all objects with spectra in DR8. For each object, that catalog contains the spec ObjID, the R.A., the decl., the z, z error, the certainty of classification as elliptical, the certainty of classification as spiral, and the certainty of classification as a star. See section 3.1 for further explanations. (2 data files).

VizieR Online Data Catalog: An ALMA survey of ECDFS submillimeter galaxies (Simpson+, 2014)

NASA Astrophysics Data System (ADS)

Simpson, J. M.; Swinbank, A. M.; Smail, I.; Alexander, D. M.; Brandt, W. N.; Bertoldi, F.; De Breuck, C.; Chapman, S. C.; Coppin, K. E. K.; da Cunha, E.; Danielson, A. L. R.; Dannerbauer, H.; Greve, T. R.; Hodge, J. A.; Ivison, R. J.; Karim, A.; Knudsen, K. K.; Poggianti, B. M.; Schinnerer, E.; Thomson, A. P.; Walter, F.; Wardlow, J. L.; Weiss, A.; van der Werf, P. P.

2017-07-01

In this study we undertake a multi-wavelength analysis of the ALMA-detected submm galaxies from the catalog presented by Hodge et al. (2013, J/ApJ/768/91) (see also Karim et al. 2013MNRAS.432....2K). To briefly summarize the observations, we obtained 120 s integrations of 122 of the original 126 LESS submm sources, initially identified using the LABOCA camera on the APEX telescope (Weiss et al. 2009, J/ApJ/707/1201). These Cycle 0 observations used the compact configuration, yielding a median synthesized beam of ~1.6"x1.2". The observing frequency was matched to the original LESS survey, 344 GHz (Band 7), and we reach a typical rms across our velocity-integrated maps of 0.4 mJy/beam. (3 data files).

Adapting biomarker technologies to adverse outcome ...

EPA Pesticide Factsheets

Adverse outcome pathways (AOP) research is a relatively new concept in human systems biology for assessing the molecular level linkage from an initiating (chemical) event that could lead to a disease state. Although most implementations of AOPs are based on liquids analyses, there are now new technologies being considered derived from the broad field of breath research, especially in applications of gas-phase analysis and instrumentation. The ultimate goal is to discover disease progressions in human or animal systems, identify them at the molecular or cellular level, and then choose analytes that can distinctly define the presence of a particular path (Ankley et al. 2010, Villeneuve et al. 2014). Once such in vivo pathways are identified, then in vitro assays can be developed for streamlined testing of chemical effects without additional human or animal based studies (Pleil et al. 2012). Recent work has focused on discovery analysis in breath, or other biological media, wherein as many as possible compounds are cataloged and then linked to their biochemical source as exogenous (external), endogenous (internal) or from the microbiome (Pleil et al. 2013a, de Lacy Costello 2014, Pleil et al. 2013b, Trefz et al. 2013, Pleil et al. 2014). Such research lays the groundwork for identifying compounds from systems biology that might be relevant for developing AOPs for in vitro research. The National Exposure Research Laboratory’s (NERL’s) Human Exposure and Atm

VizieR Online Data Catalog: NGC 5548 43 year-long monitoring in Hβ (Bon+, 2016)

NASA Astrophysics Data System (ADS)

Bon, E.; Zucker, S.; Netzer, H.; Marziani, P.; Bon, N.; Jovanovic, P.; Shapovalova, A. I.; Komossa, S.; Gaskell, C. M.; Popovic, L. C.; Britzen, S.; Chavushyan, V. H.; Burenkov, A. N.; Sergeev, S.; La Mura, G.; Valdes, J. R.; Stalevski, M.

2016-10-01

We analyzed 1600 spectra of NGC 5548 in the Hβ spectral interval, covering 43 years. We used: (a) archival spectra obtained by K.K. Chuvaev from 1972-1988 (Sergeev+ 2007ApJ...668..708S) prior to the International AGN Watch (IAW) campaigns. These early spectra were recorded on photographic plates acquired with an image tube at the 2.6m Shajn Telescope of the Crimean Astrophysical Observatory. (b) The 13 year study (from 1988 to 2002) of the IAW program (Peterson+ 2002ApJ...581..197P), which provided 1530 optical continuum measurements and 1248 Hβ measurements. (c) A spectral monitoring program with the 6 and 1m telescopes of the Special Astrophysical Observatory (SAO) in Russia from 1996 to 2002, and the 2.1m telescope of Guillermo Haro Observatory (GHO) in Cananea, Mexico, from 1996 to 2003 (S04; Shapovalova+ 2004, J/A+A/422/925). (d) More recent, unpublished observations of the same program covering 2003-2013 observed at SAO (see Table 1), and a continuation of the monitoring campaign presented in S04. (e) Spectra from the new IAW campaign obtained at Asiago observatory in 2012, 2013, and 2015. (f) New unpublished observations from 2013 from the Asiago observatory (also given in Table 1). See section 2 for further details. (2 data files).

The Society of Astronomy Students: From the Ground Up

NASA Astrophysics Data System (ADS)

Rees, Shannon; Maldonado, M.; Beasley, D.; Campos, A.; Medina, A.; Chanover, N. J.

2014-01-01

The Society of Astronomy Students (SAS) at New Mexico State University (NMSU) was founded in October of 2012 and chartered in January 2013. New Mexico State University is located in Las Cruces, New Mexico, which is a small city with a population of just over 100,000. The main campus at NMSU has an enrollment of approximately 14,300 undergraduate students and 3,375 graduate students. The NMSU Astronomy Department is a vibrant research environment that offers Ph.D. and M.S. Graduate degrees and serves the undergraduate population through a large number of general education courses. Although there is no undergraduate major in Astronomy at NMSU, students can earn an undergraduate Astronomy Minor. The SAS was conceived as a way to provide undergraduates with an interest in astronomy a way to communicate, network, and provide mutual support. Currently, the SAS is in its second year of being a chartered organization and has about 18 active members, about half of whom are planning on pursuing an Astronomy Minor. The SAS is striving to become one of the most active clubs on the NMSU campus in order to raise awareness about Astronomy and encourage the option of pursuing the Astronomy Minor. One of the main focus areas of the SAS is to be involved in both astronomy-related and non-astronomy-related public outreach and community service events. Since the clubs inception, the SAS members have contributed a total of over 120 volunteer hours. We do many outreach events with the elementary and middle schools around the community; these events are done jointly with the Astronomy Graduate Student Organization at NMSU. In the near future, the SAS is also planning a wide range of activities, including a guest speaker series at weekly club meetings, tours of the Apache Point Observatory, full moon outings, and participation in amateur astronomy events such as the Messier Marathon. This presentation will include an overview of the club's history, accomplishments, and future activities.

VizieR Online Data Catalog: Stellar activity and kinematics of FGK stars (Murgas+, 2013)

NASA Astrophysics Data System (ADS)

Murgas, F.; Jenkins, J. S.; Rojo, P.; Jones, H. R. A.; Pinfield, D. J.

2013-02-01

We present a compilation of stellar activity catalogs combined with galactic velocity information of 2529 F, G, and K stars. The stellar activity catalogs use in this work are: Jenkins et al. 2011 (Cat. J/A+A/531/A8); Gray et al. 2003 (Cat. J/AJ/126/2048), 2006 (Cat. J/AJ/132/161); Henry et al 1996 (Cat. J/A+A/111/439); Wright et al. 2004 (Cat. J/ApJS/152/261); Duncan et al. (1991ApJS...76..383D, Cat. III/159). The galactic velocities are taken from the Jenkins et al. 2011 (Cat. J/A+A/531/A8) and the Geneva-Copenhaguen Survey (GCS) Nordstrom et al. (2004A&A...418..989N, Cat. V/117). (1 data file).

Selections from the ABC 2013 Annual Convention, New Orleans, Louisiana: A Gumbo of Favorite Assignments: Global, Communicating Complex Information, Short-Message Packaging

ERIC Educational Resources Information Center

Whalen, D. Joel

2014-01-01

This article, the first of a two-part series, catalogs teaching innovations presented at the 2013 Association for Business Communication (ABC) Annual Convention, New Orleans. They were presented during the My Favorite Assignment session. The 11 Favorite Assignments featured here offer the reader a variety of learning experiences including…

Fractals for Geoengineering

NASA Astrophysics Data System (ADS)

Oleshko, Klaudia; de Jesús Correa López, María; Romero, Alejandro; Ramírez, Victor; Pérez, Olga

2016-04-01

The effectiveness of fractal toolbox to capture the scaling or fractal probability distribution, and simply fractal statistics of main hydrocarbon reservoir attributes, was highlighted by Mandelbrot (1995) and confirmed by several researchers (Zhao et al., 2015). Notwithstanding, after more than twenty years, it's still common the opinion that fractals are not useful for the petroleum engineers and especially for Geoengineering (Corbett, 2012). In spite of this negative background, we have successfully applied the fractal and multifractal techniques to our project entitled "Petroleum Reservoir as a Fractal Reactor" (2013 up to now). The distinguishable feature of Fractal Reservoir is the irregular shapes and rough pore/solid distributions (Siler, 2007), observed across a broad range of scales (from SEM to seismic). At the beginning, we have accomplished the detailed analysis of Nelson and Kibler (2003) Catalog of Porosity and Permeability, created for the core plugs of siliciclastic rocks (around ten thousand data were compared). We enriched this Catalog by more than two thousand data extracted from the last ten years publications on PoroPerm (Corbett, 2012) in carbonates deposits, as well as by our own data from one of the PEMEX, Mexico, oil fields. The strong power law scaling behavior was documented for the major part of these data from the geological deposits of contrasting genesis. Based on these results and taking into account the basic principles and models of the Physics of Fractals, introduced by Per Back and Kan Chen (1989), we have developed new software (Muukíl Kaab), useful to process the multiscale geological and geophysical information and to integrate the static geological and petrophysical reservoir models to dynamic ones. The new type of fractal numerical model with dynamical power law relations among the shapes and sizes of mesh' cells was designed and calibrated in the studied area. The statistically sound power law relations were established for the reservoir' hydraulic units distribution in space and time, as well as for the corresponding well testing data. References: 1. Mandelbrot, B., 1995. Foreword to Fractals in Petroleum Geology and Earth Processes, Edited by: Christopher C. Barton and Paul R. La Pointe, Plenum Press, New York: vii-xii. 2. Jin-Zhou Zhao, Cui-Cui Sheng, Yong_Ming Li, and Shun-Chu Li, 2015. A Mathematical Model for the Analysis of the Pressure Transient Response of Fluid Flow in Fractal Reservoir. J. of Chemistry, ID 596597, 8p. 3. Siler, T. , 2007. Fractal Reactor. International Conference Series on Emerging Nuclear Energy Systems 4. Corbett, P. W. M., 2012. The Role of Geoengineering in field development. INTECH, Chapter 8: 181- 198. 5. Nelson, P.H. and J. Kibler, 2003. A Catalog of Porosity and Permeability from core plugs in siliciclastic rocks. U.S. Geological Survey. 6. Per Bak and Kan Chen, 1989. The Physics of Fractals. Physica D 38: 5-12.

75 FR 65527 - Agency Information Collection Activities: Proposed Collection; Comment Request

Federal Register 2010, 2011, 2012, 2013, 2014

2010-10-25

... Education Program Evaluation. OMB Number: 3145-0211. Expiration Date of Approval: March 31, 2013. Title of collection: Revitalizing Computing Pathways (CPATH) in Undergraduate Education Program Evaluation. Type of... organizations) to formulate and implement plans to revitalize undergraduate computing education in the United...

VizieR Online Data Catalog: EC 01541-1409 pulsations frequencies (Reed+, 2012)

NASA Astrophysics Data System (ADS)

Reed, M. D.; Kilkenny, D.; O'Toole, S.; Ostensen, R. H.; Honer, C.; Gilker, J. T.; Quint, A. C.; Doennig, A. M.; Hicks, L. H.; Thompson, M. A.; McCart, P. A., II; Zietsman, E.; Chen, W.-P.; Chen, C.-W.; Lin, C.-C.; Beck, P.; Degroote, P.; Barlow, B. N.; Reichart, D. E.; Nysewander, M. C.; Lacluyze, A. P.; Ivarsen, K. M.; Haislip, J. B.; Baran, A.; Winiarski, M.; Drozdz, M.

2012-10-01

Data were obtained from six different observatories, each with a somewhat different CCD setup. South African Astronomical Observatory's (SAAO's) 1.0-m telescope observed during both 2008 and 2009. (1 data file).

The WISE AGN Catalog

NASA Astrophysics Data System (ADS)

Assef, R. J.; Stern, D.; Noirot, G.; Jun, H. D.; Cutri, R. M.; Eisenhardt, P. R. M.

2018-02-01

We present two large catalogs of active galactic nucleus (AGN) candidates identified across 30,093 deg2 of extragalactic sky from the Wide-field Infrared Survey Explorer’s AllWISE Data Release. Both catalogs are selected purely using the Wide-field Infrared Survey Explorer (WISE) W1 and W2 bands. The R90 catalog consists of 4,543,530 AGN candidates with 90% reliability, while the C75 catalog consists of 20,907,127 AGN candidates with 75% completeness. These reliability and completeness figures were determined from a detailed analysis of UV- to near-IR spectral energy distributions of ∼ {10}5 sources in the 9 deg2 Boötes field. The AGN selection criteria are based on those of Assef et al. (2013) recalibrated to the AllWISE data release. We provide a detailed discussion of potential artifacts and excise portions of the sky close to the Galactic Center, Galactic Plane, nearby galaxies, and other expected contaminating sources. These catalogs are expected to enable a broad range of science, and we present a few illustrative cases. From the R90 sample, we identify 45 highly variable AGNs lacking radio counterparts in the FIRST survey. One of these sources, WISEA J142846.71+172353.1, is a changing-look quasar at z = 0.104, which has changed from having broad Hα to being a narrow-lined AGN. We characterize our catalogs by comparing them to large, wide-area AGN catalogs in the literature. We identify four ROSAT X-ray sources that are each matched to three WISE-selected AGNs in the R90 sample within 30″. Spectroscopy reveals that one of these systems, 2RXS J150158.6+691029, consists of a triplet of quasars at z = 1.133 ± 0.004, suggestive of a rich group or forming galaxy cluster.

VizieR Online Data Catalog: Northern bright planet host stars parameters (Sousa+, 2015)

NASA Astrophysics Data System (ADS)

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

2015-03-01

The spectroscopic data were collected between 16 April 2013 and 20 August 2013 with the NARVAL spectrograph located at the 2-meter Bernard Lyot Telescope (@ Pic du Midi). The data was obtained through the Opticon proposal (OPTI- CON2013A027). Table 1 contains the spectroscopic parameters derived with ARES+MOOG for the sample of planet hosts analysed in this work. Table 2 contains the stellar mass and radius estimated for the planet hosts analysed in this work. (2 data files).

Tracking a Very Near Earth Asteroid

NASA Astrophysics Data System (ADS)

Bruck, R.; Rashid, S.; Peppard, T.

2013-09-01

The potential effects of an asteroid passing within close proximity to the Earth were recently realized. During the February 16, 2013 event, Asteroid 2012 DA14 passed within an estimated 27,700 kilometers of the earth, well within the geosynchronous (GEO) orbital belt. This was the closest known approach of a planetoid of this size, in modern history. The GEO belt is a region that is filled with critical communications satellites which provide relays for essential government, business and private datum. On the day of the event, optical instruments at Detachment 3, 21OG, Maui GEODSS were able to open in marginal atmospheric conditions, locate and collect metric and raw video data on the asteroid as it passed a point of near heliocentric orbital propinquity to the Earth. Prior to the event, the Joint Space Operations Center (JSpOC) used propagated trajectory data from NASA's Near Earth Object Program Office at the Jet Propulsion Laboratory to assess potential collisions with man-made objects in Earth orbit. However, the ability to actively track this asteroid through the populated satellite belt not only allowed surveillance for possible late orbital perturbations of the asteroid, but, afforded the ability to monitor possible strikes on all other orbiting bodies of anthropogenic origin either not in orbital catalogs or not recently updated in those catalogs. Although programmed only for tracking satellites in geocentric orbits, GEODSS was able to compensate and maintain track on DA14, collecting one hundred and fifty four metric observations during the event.

77 FR 33496 - Agency Information Collection Activities: Proposed Collection, Comment Request

Federal Register 2010, 2011, 2012, 2013, 2014

2012-06-06

...: August 31, 2012. Abstract: The Division of Undergraduate Education (DUE) Project Data Form is a component of all grant proposals submitted to NSF's Division of Undergraduate Education. This form collects...) that the project would target (e.g., women, minorities, persons with disabilities), strategic foci (if...

Effects of Professorial Tenure on Undergraduate Ratings of Teaching Performance

ERIC Educational Resources Information Center

Cheng, Dorothy A.

2015-01-01

This study estimates the effect of professorial tenure on undergraduate ratings of learning, instructor quality, and course quality at the University of California, San Diego from Summer 2004 to Spring 2012. During this eight-year period, 120 assistant professors received tenure and 83 associate professors attained full rank. A…

VizieR Online Data Catalog: Extinction law in the Cep OB3b young cluster (Allen+, 2014)

NASA Astrophysics Data System (ADS)

Allen, T. S.; Prchlik, J. J.; Megeath, S. T.; Gutermuth, R. A.; Pipher, J. L.; Naylor, T.; Jeffries, R. D.

2017-06-01

We use Johnson V and Cousins Rc (hereafter called VR) band phot from the Isaac Newton Telescope (INT), compiled in the catalog of Littlefair et al. (2010, J/MNRAS/403/545). The R-band photometry was obtained using the Sloan r filter. It was calibrated against photometric standard stars measured in the Cousins Rc filter with an arbitrary zero point. Moderate resolution ((λ/Δλ)~1000-2000, FWHM resolution of about 6 Å) optical spectra (covering 4000-9000 Å) were obtained for ~1700 sources toward Cep OB3b using the multi-fiber spectrograph Hectospec on the MMT telescope. About 600 sources were selected for observation because they were determined to be possible cluster members (Allen et al. 2012, J/ApJ/750/125), based on indicators of youth, such as IR emission due to circumstellar dusty material and heightened X-ray activity. We use an extinction map from Allen et al. (2012, J/ApJ/750/125) to initially estimate the extinction toward each source. This map is derived using the 2MASS Point Source Catalog (Skrutskie et al. 2006AJ....131.1163S, Cat. VII/233) H and Ks band photometry of background stars. (1 data file).

Evaluating the Effectiveness of an Undergraduate Multicultural Course

ERIC Educational Resources Information Center

Chappell, Charisse

2014-01-01

The American Psychological Association (APA) recently revised their "Guidelines for the undergraduate psychology major" in 2013. In this updated version diversity is included in the broad goal of ethical and social responsibility in a diverse world. Indicators associated with this goal include student awareness of prejudice within…

Rethinking Undergraduate Physical Chemistry Curricula

ERIC Educational Resources Information Center

Miller, Stephen R.

2016-01-01

A summary of fundamental changes made to the undergraduate physical chemistry curriculum in the Chemistry Department at Gustavus Adolphus College (beginning in the 2013-2014 academic year) is presented. The yearlong sequence now consists of an introductory semester covering both quantum mechanics and thermodynamics/kinetics, followed by a second…

Long-Term Seismic Quiescences and Great Earthquakes in and Around the Japan Subduction Zone Between 1975 and 2012

NASA Astrophysics Data System (ADS)

Katsumata, Kei

2017-06-01

An earthquake catalog created by the International Seismological Center (ISC) was analyzed, including 3898 earthquakes located in and around Japan between January 1964 and June 2012 shallower than 60 km with the body wave magnitude of 5.0 or larger. Clustered events such as earthquake swarms and aftershocks were removed from the ISC catalog by using a stochastic declustering method based on Epidemic-Type Aftershock Sequence (ETAS) model. A detailed analysis of the earthquake catalog using a simple scanning technique (ZMAP) shows that the long-term seismic quiescences lasting more than 9 years were recognized ten times along the subduction zone in and around Japan. The three seismic quiescences among them were followed by three great earthquakes: the 1994 Hokkaido-toho-oki earthquake ( M w 8.3), the 2003 Tokachi-oki earthquake ( M w 8.3), and the 2011 Tohoku earthquake ( M w 9.0). The remaining seven seismic quiescences were followed by no earthquake with the seismic moment M 0 ≥ 3.0 × 1021 Nm ( M w 8.25), which are candidates of the false alarm. The 2006 Kurile Islands earthquake ( M w 8.3) was not preceded by the significant seismic quiescence, which is a case of the surprise occurrence. As a result, when limited to earthquakes with the seismic moment of M 0 ≥ 3.0 × 1021 Nm, four earthquakes occurred between 1976 and 2012 in and around Japan, and three of them were preceded by the long-term seismic quiescence lasting more than 9 years.

Achieved Competencies and Satisfaction in Temporomandibular Disorders and Orofacial Pain Education.

PubMed

Nordin, Sara; Dawson, Andreas; Ekberg, Ewa Carin

2016-01-01

To assess dental students' achieved competencies and perceived satisfaction with their temporomandibular disorders (TMD) and orofacial pain education and to compare these with the results of their final examination in TMD and orofacial pain. Dental students from two consecutive classes (2011/2012 and 2012/2013) at the Department of Orofacial Pain and Jaw Function at the dental school in Malmö, Sweden completed two self-evaluations, one at the beginning of semester seven and one at the end of semester eight. The questionnaire that they were given concerned achieved competencies and satisfaction with education in TMD and orofacial pain. Items focused on anatomy, physiology, and clinical training. Students estimated their competence and satisfaction on a numeric rating scale and described their idea of treating TMD and orofacial pain patients on a verbal rating scale. Outcome variables were tested with paired samples t test for differences over time and independent samples t test for between-class comparisons; both were adjusted for multiple testing with Bonferroni correction. Significant improvement in all items was observed for achieved competencies and satisfaction in both classes between semester seven and semester eight (P < .05). No differences in competencies or satisfaction occurred between classes at the end of the clinical course in semester eight (P > .05). This study has shown that expansion in undergraduate TMD and orofacial pain education at the dental school in Malmö has allowed all students to develop the same level of competence, independent of prior experience. The study also pointed out that continuous evaluation and enhancement of TMD and orofacial pain education in undergraduate dental education is beneficial.

THEMIS Art #127

NASA Image and Video Library

2017-06-16

In this image, NASA's 2001 Mars Odyssey spacecraft spies what looks like a deep water fish yelling. Orbit Number: 52146 Latitude: 31.751 Longitude: 306.831 Instrument: VIS Captured: 2013-09-15 16:11 https://photojournal.jpl.nasa.gov/catalog/PIA21685

Clinical Sequencing Uncovers Origins and Evolution of Lassa Virus.

PubMed

Andersen, Kristian G; Shapiro, B Jesse; Matranga, Christian B; Sealfon, Rachel; Lin, Aaron E; Moses, Lina M; Folarin, Onikepe A; Goba, Augustine; Odia, Ikponmwonsa; Ehiane, Philomena E; Momoh, Mambu; England, Eleina M; Winnicki, Sarah; Branco, Luis M; Gire, Stephen K; Phelan, Eric; Tariyal, Ridhi; Tewhey, Ryan; Omoniwa, Omowunmi; Fullah, Mohammed; Fonnie, Richard; Fonnie, Mbalu; Kanneh, Lansana; Jalloh, Simbirie; Gbakie, Michael; Saffa, Sidiki; Karbo, Kandeh; Gladden, Adrianne D; Qu, James; Stremlau, Matthew; Nekoui, Mahan; Finucane, Hilary K; Tabrizi, Shervin; Vitti, Joseph J; Birren, Bruce; Fitzgerald, Michael; McCowan, Caryn; Ireland, Andrea; Berlin, Aaron M; Bochicchio, James; Tazon-Vega, Barbara; Lennon, Niall J; Ryan, Elizabeth M; Bjornson, Zach; Milner, Danny A; Lukens, Amanda K; Broodie, Nisha; Rowland, Megan; Heinrich, Megan; Akdag, Marjan; Schieffelin, John S; Levy, Danielle; Akpan, Henry; Bausch, Daniel G; Rubins, Kathleen; McCormick, Joseph B; Lander, Eric S; Günther, Stephan; Hensley, Lisa; Okogbenin, Sylvanus; Schaffner, Stephen F; Okokhere, Peter O; Khan, S Humarr; Grant, Donald S; Akpede, George O; Asogun, Danny A; Gnirke, Andreas; Levin, Joshua Z; Happi, Christian T; Garry, Robert F; Sabeti, Pardis C

2015-08-13

The 2013-2015 West African epidemic of Ebola virus disease (EVD) reminds us of how little is known about biosafety level 4 viruses. Like Ebola virus, Lassa virus (LASV) can cause hemorrhagic fever with high case fatality rates. We generated a genomic catalog of almost 200 LASV sequences from clinical and rodent reservoir samples. We show that whereas the 2013-2015 EVD epidemic is fueled by human-to-human transmissions, LASV infections mainly result from reservoir-to-human infections. We elucidated the spread of LASV across West Africa and show that this migration was accompanied by changes in LASV genome abundance, fatality rates, codon adaptation, and translational efficiency. By investigating intrahost evolution, we found that mutations accumulate in epitopes of viral surface proteins, suggesting selection for immune escape. This catalog will serve as a foundation for the development of vaccines and diagnostics. VIDEO ABSTRACT. Copyright © 2015 Elsevier Inc. All rights reserved.

Clinical sequencing uncovers origins and evolution of Lassa virus

PubMed Central

Andersen, Kristian G.; Shapiro, B. Jesse; Matranga, Christian B.; Sealfon, Rachel; Lin, Aaron E.; Moses, Lina M.; Folarin, Onikepe A.; Goba, Augustine; Odia, Ikponmwonsa; Ehiane, Philomena E.; Momoh, Mambu; England, Eleina M.; Winnicki, Sarah; Branco, Luis M.; Gire, Stephen K.; Phelan, Eric; Tariyal, Ridhi; Tewhey, Ryan; Omoniwa, Omowunmi; Fullah, Mohammed; Fonnie, Richard; Fonnie, Mbalu; Kanneh, Lansana; Jalloh, Simbirie; Gbakie, Michael; Saffa, Sidiki; Karbo, Kandeh; Gladden, Adrianne D.; Qu, James; Stremlau, Matthew; Nekoui, Mahan; Finucane, Hilary K.; Tabrizi, Shervin; Vitti, Joseph J.; Birren, Bruce; Fitzgerald, Michael; McCowan, Caryn; Ireland, Andrea; Berlin, Aaron M.; Bochicchio, James; Tazon-Vega, Barbara; Lennon, Niall J.; Ryan, Elizabeth M.; Bjornson, Zach; Milner, Danny A.; Lukens, Amanda K.; Broodie, Nisha; Rowland, Megan; Heinrich, Megan; Akdag, Marjan; Schieffelin, John S.; Levy, Danielle; Akpan, Henry; Bausch, Daniel G.; Rubins, Kathleen; McCormick, Joseph B.; Lander, Eric S.; Günther, Stephan; Hensley, Lisa; Okogbenin, Sylvanus; Schaffner, Stephen F.; Okokhere, Peter O.; Khan, S. Humarr; Grant, Donald S.; Akpede, George O.; Asogun, Danny A.; Gnirke, Andreas; Levin, Joshua Z.; Happi, Christian T.; Garry, Robert F.; Sabeti, Pardis C.

2015-01-01

Summary The 2013-2015 West African epidemic of Ebola virus disease (EVD) reminds us how little is known about biosafety level-4 viruses. Like Ebola virus, Lassa virus (LASV) can cause hemorrhagic fever with high case fatality rates. We generated a genomic catalog of almost 200 LASV sequences from clinical and rodent reservoir samples. We show that whereas the 2013-2015 EVD epidemic is fueled by human-to-human transmissions, LASV infections mainly result from reservoir-to-human infections. We elucidated the spread of LASV across West Africa and show that this migration was accompanied by changes in LASV genome abundance, fatality rates, codon adaptation, and translational efficiency. By investigating intrahost evolution, we found that mutations accumulate in epitopes of viral surface proteins, suggesting selection for immune escape. This catalog will serve as a foundation for the development of vaccines and diagnostics. PMID:26276630

Mode switching in volcanic seismicity: El Hierro 2011-2013

NASA Astrophysics Data System (ADS)

Roberts, Nick S.; Bell, Andrew F.; Main, Ian G.

2016-05-01

The Gutenberg-Richter b value is commonly used in volcanic eruption forecasting to infer material or mechanical properties from earthquake distributions. Such studies typically analyze discrete time windows or phases, but the choice of such windows is subjective and can introduce significant bias. Here we minimize this sample bias by iteratively sampling catalogs with randomly chosen windows and then stack the resulting probability density functions for the estimated b>˜ value to determine a net probability density function. We examine data from the El Hierro seismic catalog during a period of unrest in 2011-2013 and demonstrate clear multimodal behavior. Individual modes are relatively stable in time, but the most probable b>˜ value intermittently switches between modes, one of which is similar to that of tectonic seismicity. Multimodality is primarily associated with intermittent activation and cessation of activity in different parts of the volcanic system rather than with respect to any systematic inferred underlying process.

VizieR Online Data Catalog: Candidate X-ray OB stars in MYStIX regions (Povich+, 2017)

NASA Astrophysics Data System (ADS)

Povich, M. S.; Busk, H. A.; Feigelson, E. D.; Townsley, L. K.; Kuhn, M. A.

2017-10-01

X-ray point source catalogs for the 18 Massive Young Star-forming Complex Study in Infrared and X-Rays (MYStIX) regions studied here were produced by Kuhn+ (2010, J/ApJ/725/2485 and 2013, J/ApJS/209/27) and Townsley (2014+, J/ApJS/213/1) from archival Chandra Advanced CCD Imaging Camera (ACIS) observations. MYStIX JHKs NIR photometry was obtained from images taken with the United Kingdom Infrared Telescope (UKIRT) Wide-field Camera or from the Two-Micron All-Sky Survey (2MASS). See section 2 for further details. Spitzer MIR photometry at 3.6, 4.5, 5.8, and 8.0um was provided either by the Galactic Legacy Mid-Plane Survey Extraordinaire (GLIMPSE; Benjamin+ 2003PASP..115..953B) or by Kuhn+ (2013, J/ApJS/209/29). (4 data files).

Using Social Cognitive Theory to Explain the Intention of Final-year Pharmacy Students to Undertake a Higher Degree in Pharmacy Practice Research.

PubMed

Carter, Stephen R; Moles, Rebekah J; Krass, Ines; Kritikos, Vicki S

2016-08-25

Objective. To develop and test a conceptual model that hypothesized student intention to undertake a higher degree in pharmacy practice research (PPR) would be increased by self-efficacy, outcome expectancy, and the social influence of faculty members. Methods. Cross-sectional surveys were completed by 387 final-year pharmacy undergraduates enrolled in 2012 and 2013. Structural equation modeling was used to explore relationships between variables and intention. Results. Fit indices were good. The model explained 55% of the variation in intention. As hypothesized, faculty social influence increased self-efficacy and indirectly increased outcome expectancy and intention. Conclusion. To increase pharmacy students' orientation towards a career in PPR, faculty members could use their social influence by highlighting PPR in their teaching.

VizieR Online Data Catalog: IRAS 22023+5249 spectroscopy (Sarkar+, 2012)

NASA Astrophysics Data System (ADS)

Sarkar, G.; Garcia-Hernandez, D. A.; Parthasarathy, M.; Manchado, A.; Garcia-Lario, P.; Takeda, Y.

2012-10-01

IRAS 22023+5249 was observed on 14 July 2001 using the Utrecht Echelle Spectrograph on the 4.2m William Herschel Telescope at the Roque de los Muchachos Observatory in La Palma (Spain). (3 data files).

The Fermi Large Area Telescope Thrid Gamma-ray Source Catalog

NASA Astrophysics Data System (ADS)

Stephens, Thomas E.; Ballet, Jean; Burnett, Toby; Cavazzuti, Elisabetta; Digel, Seth William; Fermi LAT Collaboration

2015-01-01

We present an overview of the third Fermi Large Area Telescope source catalog (3FGL) of sources in the 100 MeV - 300 GeV range. Based on the first four years of science data from the Fermi Gamma-ray Space Telescope mission, it is the deepest yet in this energy range. Relative to the 2FGL catalog (Nolan et al. 2012, ApJS 199, 31), the 3FGL catalog incorporates twice as much data as well as a number of analysis improvements, including improved calibrations at the event reconstruction level, an updated model for Galactic diffuse gamma-ray emission, a refined procedure for source detection, and improved methods for associating LAT sources with potential counterparts at other wavelengths. The 3FGL catalog includes 3033 sources, with source location regions, spectral properties, and monthly light curves for each. For approximately one-third of the sources we have not found counterparts at other wavelengths. More than 1100 of the identified or associated sources are active galaxies of the blazar class; several other classes of non-blazar active galaxies are also represented in the 3FGL. Pulsars represent the largest Galactic source class. From source counts of Galactic sources we estimate the contribution of unresolved sources to the Galactic diffuse emission.

VizieR Online Data Catalog: The magnetic field of L1544. I. NIR data (Clemens+, 2016)

NASA Astrophysics Data System (ADS)

Clemens, D. P.; Tassis, K.; Goldsmith, P. F.

2017-04-01

NIR imaging polarimetric observations of L1544 were conducted on the UT nights of 2013 January 20, 2015 October 27 and 31, 2015 November 1 and 2, and 2016 January 27 and 31 using the Mimir instrument on the 1.83m Perkins Telescope, located outside Flagstaff, Arizona. Six pointing centers ("fields") were selected toward a Center direction (RAJ200=05:04:16.6, DEJ2000=+25:10:48), the four equatorial NSEW directions offset by 6 arcmin from the Center, and one field to the NW offset mostly diagonally by about 10.9 arcmin. In addition, the AllWISE (Cutri+ 2013, II/328) catalog entries for the field shown in Figure 1 were fetched, resulting in 3616 stars with a detection in at least the WISE W1 (3.6um) band or W2 (4.5um) band. These were positionally matched to the H-band catalog, yielding 1262 matches. The properties of the 450 H-band stars without WISE star matches and the WISE stars without H-band star matches were similar in being fainter than the subset of stars with H-to-WISE matches. The combined data set of 1712 stars is listed in Table 1. (1 data file).

Reliability and Validity of the Research Methods Skills Assessment

ERIC Educational Resources Information Center

Smith, Tamarah; Smith, Samantha

2018-01-01

The Research Methods Skills Assessment (RMSA) was created to measure psychology majors' statistics knowledge and skills. The American Psychological Association's Guidelines for the Undergraduate Major in Psychology (APA, 2007, 2013) served as a framework for development. Results from a Rasch analysis with data from n = 330 undergraduates showed…

Ethics as an Undergraduate Psychology Outcome: When, Where, and How to Teach It

ERIC Educational Resources Information Center

Ruiz, Ana; Warchal, Judith

2014-01-01

The American Psychological Association (APA) recently approved a new set of "Guidelines for the undergraduate psychology major, version 2.0" (APA, 2013a) which addressed ethics specifically. Yet the teaching of ethics receives little attention in publications, national and international institutes, and conferences. Few guidelines for…

Generational Perceptions of Campus Climate among LGBTQ Undergraduates

ERIC Educational Resources Information Center

Garvey, Jason C.; Sanders, Laura A.; Flint, Maureen A.

2017-01-01

Using data from the National LGBT Alumni Survey, we examined generational perceptions of campus climate for LGBTQ undergraduate students who graduated from 1944 through 2013 (N = 3,121) with Renn and Arnold's (2003) reconceptualized ecological model as a framework. Results demonstrate differences in LGBTQ student campus climate perceptions across…

40 CFR 86.1811-10 - Emission standards for light-duty vehicles, light-duty trucks and medium-duty passenger vehicles.

Code of Federal Regulations, 2010 CFR

2010-07-01

... 25 2013 50 2014 75 2015 and subsequent 100 (4) Alternate phase-in schedules for cold temperature NMHC... 2012 2013 2009 2010 2011 2012 2013 2014 2010 2011 2012 2013 2014 2011 2012 2013 Table S10-5—In-Use Standards for Applicable Phase-In HLDT/MDPVs Model Year of Introduction 2010 2011 2012 2013 2014 2015 Models...

A Catalog of Distances to Molecular Clouds from Pan-STARRS1

NASA Astrophysics Data System (ADS)

Schlafly, Eddie; Green, G.; Finkbeiner, D. P.; Rix, H.

2014-01-01

We present a catalog of distances to molecular clouds, derived from PanSTARRS-1 photometry. We simultaneously infer the full probability distribution function of reddening and distance of the stars towards these clouds using the technique of Green et al. (2013) (see neighboring poster). We fit the resulting measurements using a simple dust screen model to infer the distance to each cloud. The result is a large, homogeneous catalog of distances to molecular clouds. For clouds with heliocentric distances greater than about 200 pc, typical statistical uncertainties in the distances are 5%, with systematic uncertainty stemming from the quality of our stellar models of about 10%. We have applied this analysis to many of the most well-studied clouds in the δ > -30° sky, including Orion, California, Taurus, Perseus, and Cepheus. We have also studied the entire catalog of Magnani, Blitz, and Mundy (1985; MBM), though for about half of those clouds we can provide only upper limits on the distances. We compare our distances with distances from the literature, when available, and find good agreement.

VizieR Online Data Catalog: VISTA Magellanic Survey (VMC) catalog (Cioni+, 2011)

NASA Astrophysics Data System (ADS)

Cioni, M.-R. L.; Clementini, G.; Girardi, L.; Guandalini, R.; Gullieuszik, M.; Miszalski, B.; Moretti, M.-I.; Ripepi, V.; Rubele, S.; Bagheri, G.; Bekki, K.; Cross, N.; de Blok, W. J. G.; de Grijs, R.; Emerson, J. P.; Evans, C. J.; Gibson, B.; Gonzales-Solares, E.; Groenewegen, M. A. T.; Irwin, M.; Ivanov, V. D.; Lewis, J.; Marconi, M.; Marquette, J.-B.; Mastropietro, C.; Moore, B.; Napiwotzki, R.; Naylor, T.; Oliveira, J. M.; Read, M.; Sutorius, E.; van Loon, J. Th.; Wilkinson, M. I.; Wood, P. R.

2017-11-01

The VISTA survey of the Magellanic Clouds system (VMC) survey is a homogeneous and uniform YJKs survey of ~184deg2 across the Magellanic system. Observations were obtained with the VISTA telescope as part of the VISTA survey of the Magellanic Cloud system (VMC; ESO program 179.B-2003). This data release is based on the observa tions of twelve new VMC survey tiles LMC 35, 42, 43, 73, 93, SMC 43, 52, 54, BRI 28, 35, and STR 11, 21. Observations were acquired between November 2009 and August 2013. (1 data file).

VizieR Online Data Catalog: Kepler planetary candidates. VII. 48-month (Coughlin+, 2016)

NASA Astrophysics Data System (ADS)

Coughlin, J. L.; Mullally, F.; Thompson, S. E.; Rowe, J. F.; Burke, C. J.; Latham, D. W.; Batalha, N. M.; Ofir, A.; Quarles, B. L.; Henze, C. E.; Wolfgang, A.; Caldwell, D. A.; Bryson, S. T.; Shporer, A.; Catanzarite, J.; Akeson, R.; Barclay, T.; Borucki, W. J.; Boyajian, T. S.; Campbell, J. R.; Christiansen, J. L.; Girouard, F. R.; Haas, M. R.; Howell, S. B.; Huber, D.; Jenkins, J. M.; Li, J.; Patil-Sabale, A.; Quintana, E. V.; Ramirez, S.; Seader, S.; Smith, J. C.; Tenenbaum, P.; Twicken, J. D.; Zamudio, K. A.

2016-07-01

This catalog is based on Kepler's 24th data release (DR24), which includes the processing of all data utilizing version 9.2 of the Kepler pipeline (Jenkins et al. 2010ApJ...724.1108J). This marks the first time that all of the Kepler mission data have been processed consistently with the same version of the Kepler pipeline. Over a period of 48 months (2009 May 13 to 2013 May 11), subdivided into 17 quarters (Q1-Q17), a total of 198646 targets were observed. (7 data files).

78 FR 31535 - Assistive Technology Alternative Financing Program

Federal Register 2010, 2011, 2012, 2013, 2014

2013-05-24

... DEPARTMENT OF EDUCATION Assistive Technology Alternative Financing Program AGENCY: Office of Special Education and Rehabilitative Services, Department of Education. ACTION: Notice. Catalog of Federal... developed for the Assistive Technology (AT) Alternative Financing Program (AFP) in fiscal year (FY) 2012 to...

Interview with Christine Franklin

ERIC Educational Resources Information Center

Rossman, Allan; Franklin, Christine

2013-01-01

Chris Franklin is Senior Lecturer, Undergraduate Coordinator, and Lothar Tresp Honoratus Honors Professor of Statistics at the University of Georgia. She is a Fellow of the American Statistical Association and received the USCOTS Lifetime Achievement Award in 2013. This interview took place via email on August 16, 2013-October 9, 2013. Franklin…

The University of West Florida Annual Accountability Report, 2013-14

ERIC Educational Resources Information Center

Board of Governors, State University System of Florida, 2014

2014-01-01

This statistical report provides data tables on the University of West Florida's (UWF's) financial resources, personnel, enrollment, undergraduate education, graduate education, and research & economic development. Highlights of UWF's achievements in the 2013-2014 academic year include: (1) In 2013-2014, UWF was Designated as a "Best…

Older Undergraduate English Majors and Their Self-Described Value of English

ERIC Educational Resources Information Center

Price, Joseph W.

2013-01-01

The purpose of this multiple case study was to develop an understanding of what older nontraditional undergraduate English majors voiced as the challenges, attributes, and promises concerning their choice of that academic major. Ten participants took part in this study; these were students enrolled during the Spring 2012 semester as English majors…

The Difficulties That the Undergraduate Students Face about Inner Product Space

ERIC Educational Resources Information Center

Burhanzade, Hülya; Aygör, Nilgün

2016-01-01

In this qualitative research, we studied difficulties that undergraduate students face while learning the concept of inner product space. Participants were 35 first-year mathematics students from Yildiz Technical University in the 2011 and 2012 academic years. We asked participants to solve 5 inner product space questions. Data were jointly…

Selections from the ABC 2013 Annual Convention, New Orleans, Louisiana. Part II: All That Favorite Assignment Jazz--Message Packaging and Delivery, Job Interviews, and On-the-Job Communication

ERIC Educational Resources Information Center

Whalen, D. Joel

2014-01-01

This article, the second in a two-part series, catalogs teaching innovations presented at the 2013 Association for Business Communication Annual Convention, New Orleans. They were presented during the My Favorite Assignment session. The 11 Favorite Assignments featured here offer the reader a variety of learning experiences, including…

Statistical Approach to the Operational Testing of Space Fence

DTIC Science & Technology

2015-07-01

detect, track, and catalog space objects, including the growing population of space debris (“ space junk ”). The new system will consist of two S-Band...Statistical Association Volume 64, pages 610-620, June 1969. [26] L. Hutchinson, “How NASA steers the Internaional Space Station around space junk ...Arstechnica, (2013,July) [Online]. Available: http://arstechnica.com/science/2013/07/how-nasa-steers-the-international- space -station-around- space - junk

VizieR Online Data Catalog: Radial velocities of 51 Peg (Martins+, 2015)

NASA Astrophysics Data System (ADS)

Martins, J. H. C.; Santos, N. C.; Figueira, P.; Faria, J. P.; Montalto, M.; Boisse, I.; Ehrenreich, D.; Lovis, C.; Mayor, M.; Melo, C.; Pepe, F.; Sousa, S.; Udry, S.; Cunha, D.

2015-04-01

The table contains the radial velocity data for HARPS observations of 51 Peg. This data was collected with the HARPS spectrograph at ESO's 3.6-m Telescope at La Silla-Paranal Observatory, as part of ESO programme 091.C-0271. It consists of 91 spectra observed in seven different nights (2013-06-08, 2013-06-25, 2013-08-02, 2013-08-04, 2013-09-05, 2013-09-09 and 2013-09-30) totalling around 12.5h of observing time. The obtained spectra have a S/N on the 50th order (~5560Å) that varies between 122 and 388. The spectra cover the wavelengths range from roughly 3781Å to 6910Å. (1 data file).

VizieR Online Data Catalog: Five years of blazar observations with VERITAS (Archambault+, 2016)

NASA Astrophysics Data System (ADS)

Archambault, S.; Archer, A.; Benbow, W.; Bird, R.; Biteau, J.; Buchovecky, M.; Buckley, J. H.; Bugaev, V.; Byrum, K.; Cerruti, M.; Chen, X.; Ciupik, L.; Connolly, M. P.; Cui, W.; Eisch, J. D.; Errando, M.; Falcone, A.; Feng, Q.; Finley, J. P.; Fleischhack, H.; Fortin, P.; Fortson, L.; Furniss, A.; Gillanders, G. H.; Griffin, S.; Grube, J.; Gyuk, G.; Hutten, M.; Hakansson, N.; Hanna, D.; Holder, J.; Humensky, T. B.; Johnson, C. A.; Kaaret, P.; Kar, P.; Kelley-Hoskins, N.; Kertzman, M.; Kieda, D.; Krause, M.; Krennrich, F.; Kumar, S.; Lang, M. J.; Maier, G.; McArthur, S.; McCann, A.; Meagher, K.; Moriarty, P.; Mukherjee, R.; Nguyen, T.; Nieto, D.; O'Faolain de Bhroithe, A.; Ong, R. A.; Otte, A. N.; Park, N.; Perkins, J. S.; Pichel, A.; Pohl, M.; Popkow, A.; Pueschel, E.; Quinn, J.; Ragan, K.; Reynolds, P. T.; Richards, G. T.; Roache, E.; Rovero, A. C.; Santander, M.; Sembroski, G. H.; Shahinyan, K.; Smith, A. W.; Staszak, D.; Telezhinsky, I.; Tucci, J. V.; Tyler, J.; Vincent, S.; Wakely, S. P.; Weiner, O. M.; Weinstein, A.; Williams, D. A.; Zitzer, B.

2018-04-01

In this paper, we present the results of the analysis of most of the non-detected blazars observed by VERITAS from 2007 (the beginning of full-scale scientific operations) to 2012 August (before the upgrade of the VERITAS array, see Kieda 2013arXiv1308.4849D). The VERITAS (Very Energetic Radiation Imaging Telescope Array System) telescope array is composed of four IACTs of 12 m diameter each, located at the Fred Lawrence Whipple Observatory, on the slopes of Mount Hopkins, in southern Arizona (31°40'N, 110°57'W). Each telescope has a segmented mirror that focuses light onto a camera composed of 499 photomultipliers located at the focal plane. The instrument FOV is 3.5°. For further details on the VERITAS instrument, see Holder et al. (2006APh....25..391H) and Holder (2011ICRC...12..137H). The VERITAS observations here have an average length of 20 minutes (referred to as a run), before switching targets or wobble directions. (7 data files).

Mushroom Flora of Ulleung-gun and a Newly Recorded Bovista Species in the Republic of Korea

PubMed Central

Kim, Chang Sun; Jo, Jong Won; Kwag, Young-Nam; Sung, Gi-Ho; Lee, Sle-gee; Kim, Sang-Yong; Shin, Chang-Ho

2015-01-01

We conducted five times surveys, in June, September and October in 2012; June and September 2013, to catalog the mushroom flora in Ulleung-gun, Republic of Korea. More than 400 specimens were collected, and 317 of the specimens were successfully sequenced using the ribosomal DNA internal transcribed spacer barcode marker. We also surveyed the morphological characteristics of the sequenced specimens. The specimens were classified into 2 phyla, 7 classes, 21 orders, 59 families, 122 genera, and 221 species, and were deposited in the herbarium of Korea National Arboretum. Among the collected species, 72% were saprophytic, 25% were symbiotic, and 3% were parasitic. The most common order was Agaricales (189 specimens, 132 species), followed by Polyporales (47 specimens, 27 species), Russulales (31 specimens, 22 species), Boletales (10 specimens, 7 species), and so on. Herein, we also reported the first Bovista species in Korea, which was collected from Dokdo, the far-eastern island of Korea. PMID:26539040

VizieR Online Data Catalog: 27 pulsating DA WDs follow-up observations (Hermes+, 2017)

NASA Astrophysics Data System (ADS)

Hermes, J. J.; Gansicke, B. T.; Kawaler, S. D.; Greiss, S.; Tremblay, P.-E.; Gentile Fusillo, N. P.; Raddi, R.; Fanale, S. M.; Bell, K. J.; Dennihy, E.; Fuchs, J. T.; Dunlap, B. H.; Clemens, J. C.; Montgomery, M. H.; Winget, D. E.; Chote, P.; Marsh, T. R.; Redfield, S.

2017-11-01

All observations analyzed here were collected by the Kepler spacecraft with short-cadence exposures from 2012 to 2016. Full details of the raw and processed Kepler and K2 observations are summarized in Table2. We complemented our space-based photometry of these 27 pulsating hydrogen-atmosphere white dwarfs (DAVs) by determining their atmospheric parameters based on model-atmosphere fits to follow-up spectroscopy obtained from two 4m class, ground-based facilities. Spectra taken with the 4.2m William Herschel Telescope (WHT) on the island of La Palma cover roughly 3800-5100Å at roughly 2.0Å resolution; spanning 2013 Jun 06 to 2014 Jul 25. Spectra taken with the 4.1m Southern Astrophysical Research (SOAR) telescope on Cerro Pachon in Chile cover roughly 3600-5200Å; spanning 2014 Oct 13 to 2017 Apr 21. We detail these spectroscopic observations and their resultant fits in Table 3. (4 data files).

VizieR Online Data Catalog: SPT-SZ survey galaxy clusters optical spectroscopy (Ruel+, 2014)

NASA Astrophysics Data System (ADS)

Ruel, J.; Bazin, G.; Bayliss, M.; Brodwin, M.; Foley, R. J.; Stalder, B.; Aird, K. A.; Armstrong, R.; Ashby, M. L. N.; Bautz, M.; Benson, B. A.; Bleem, L. E.; Bocquet, S.; Carlstrom, J. E.; Chang, C. L.; Chapman, S. C.; Cho, H. M.; Clocchiatti, A.; Crawford, T. M.; Crites, A. T.; de Haan, T.; Desai, S.; Dobbs, M. A.; Dudley, J. P.; Forman, W. R.; George, E. M.; Gladders, M. D.; Gonzalez, A. H.; Halverson, N. W.; Harrington, N. L.; High, F. W.; Holder, G. P.; Holzapfel, W. L.; Hrubes, J. D.; Jones, C.; Joy, M.; Keisler, R.; Knox, L.; Lee, A. T.; Leitch, E. M.; Liu, J.; Lueker, M.; Luong-van, D.; Mantz, A.; Marrone, D. P.; McDonald, M.; McMahon, J. J.; Mehl, J.; Meyer, S. S.; Mocanu, L.; Mohr, J. J.; Montroy, T. E.; Murray, S. S.; Natoli, T.; Nurgaliev, D.; Padin, S.; Plagge, T.; Pryke, C.; Reichardt, C. L.; Rest, A.; Ruhl, J. E.; Saliwanchik, B. R.; Saro, A.; Sayre, J. T.; Schaffer, K. K.; Shaw, L.; Shirokoff, E.; Song, J.; Suhada, R.; Spieler, H. G.; Stanford, S. A.; Staniszewski, Z.; Starsk, A. A.; Story, K.; Stubbs, C. W.; van Engelen, A.; Vanderlinde, K.; Vieira, J. D.; Vikhlinin, A.; Williamson, R.; Zahn, O.; Zenteno, A.

2017-04-01

Most of the galaxy clusters for which we report spectroscopic observations were published as SPT cluster detections (and new discoveries) in Vanderlinde et al. (2010ApJ...722.1180V), Williamson et al. (2011ApJ...738..139W), and Reichardt et al. (2013, J/ApJ/763/127); we refer the reader to those publications for details of the SPT observations. The spectroscopic observations presented in this work are the first of our ongoing follow-up program. The data were taken from 2008 to 2012 using the Gemini Multi Object Spectrograph (GMOS; Hook et al. 2004PASP..116..425H) on Gemini South, the Focal Reducer and low dispersion Spectrograph (FORS2; Appenzeller et al. 1998Msngr..94....1A) on VLT Antu, the Inamori Magellan Areal Camera and Spectrograph (IMACS; Dressler et al. 2006SPIE.6269E..0FD) on Magellan Baade, and the Low Dispersion Survey Spectrograph (LDSS339; Allington-Smith et al. 1994PASP..106..983A) on Magellan Clay. (2 data files).

VizieR Online Data Catalog: H2O + CH3OH maser survey of Orion protostar

NASA Astrophysics Data System (ADS)

Kang, M.; Lee, J.-E.; Choi, M.; Choi, Y.; Kim, K.-T.; di Francesco, J.; Park, Y.-S.

2015-04-01

Out of the protostars listed in the Herschel Orion Protostar Survey (HOPS) catalogue (Fischer et al. 2010A&A...518L.122F; Stutz et al. 2013, J/ApJ/767/36), we selected protostars showing line wings in the CO(J=2->1) line spectra obtained with the Seoul Radio Astronomy Observatory 6m telescope. In the Orion molecular cloud complex 99 protostars were observed using the KVN 21m radio antennas in the single-dish telescope mode during the 2010 Mar-2010 Jun and 2011-2012 observing seasons. The observations were carried out with the KVN Yonsei telescope at Seoul, the KVN Ulsan telescope at Ulsan, and the KVN Tamna telescope at Seogwipo, Korea. The target lines were the H2O(616->523) (22.23508GHz) line and the CH3OH (70->61 A+), (80->71A+), and (6-1->50E) lines at 44.06943, 95.169516, and 132.890800GHz, respectively. (6 data files).

VizieR Online Data Catalog: Positions and distances of RR Lyrae stars (Sesar+, 2014)

NASA Astrophysics Data System (ADS)

Sesar, B.; Banholzer, S. R.; Cohen, J. G.; Martin, N. F.; Grillmair, C. J.; Levitan, D.; Laher, R. R.; Ofek, E. O.; Surace, J. A.; Kulkarni, S. R.; Prince, T. A.; Rix, H.-W.

2017-04-01

RRab stars used in this work were selected by an automated classification algorithm that uses imaging data provided by the Palomar Transient Factory survey (PTF). The PTF (Law et al. 2009PASP..121.1395L; Rau et al. 2009PASP..121.1334R) is a synoptic survey designed to explore the transient sky. The project utilizes the 48-inch Samuel Oschin Schmidt Telescope on Mount Palomar. Each PTF image covers 7.26 deg2 with a pixel scale of 1.01''. The typical PTF cadence consists of two 60 s exposures separated by ~1 hr and repeated every one to five days. By 2013 June, PTF observed ~11000 deg2 of sky at least 25 times in the Mould-R filter (hereafter the R-band filter), and about 2200 deg2 in the SDSS g' filter. PTF photometry is calibrated to an accuracy of about 0.02 mag (Ofek et al. 2012PASP..124...62O, 2012PASP..124..854O) and light curves have relative precision of better than 10 mmag at the bright end, and about 0.2 mag at the survey limiting magnitude of R=20.6 mag. The relative photometry algorithm is described in Ofek et al. (2011, J/ApJ/740/65, see their Appendix A). (1 data file).

The third catalog of active galactic nuclei detected by the Fermi large area telescope

DOE PAGES

Ackermann, M.; Ajello, M.; Atwood, W. B.; ...

2015-08-25

We present the third catalog of active galactic nuclei (AGNs) detected by the Fermi-LAT (3LAC). It is based on the third Fermi-LAT catalog (3FGL) of sources detected between 100 MeV and 300 GeV with a Test Statistic greater than 25, between 2008 August 4 and 2012 July 31. The 3LAC includes 1591 AGNs located at high Galactic latitudes (more » $$| b| \\gt 10^\\circ $$), a 71% increase over the second catalog based on 2 years of data. There are 28 duplicate associations, thus 1563 of the 2192 high-latitude gamma-ray sources of the 3FGL catalog are AGNs. Most of them (98%) are blazars. About half of the newly detected blazars are of unknown type, i.e., they lack spectroscopic information of sufficient quality to determine the strength of their emission lines. Based on their gamma-ray spectral properties, these sources are evenly split between flat-spectrum radio quasars (FSRQs) and BL Lacs. The most abundant detected BL Lacs are of the high-synchrotron-peaked (HSP) type. There were about 50% of the BL Lacs that had no measured redshifts. A few new rare outliers (HSP-FSRQs and high-luminosity HSP BL Lacs) are reported. The general properties of the 3LAC sample confirm previous findings from earlier catalogs. The fraction of 3LAC blazars in the total population of blazars listed in BZCAT remains non-negligible even at the faint ends of the BZCAT-blazar radio, optical, and X-ray flux distributions, which hints that even the faintest known blazars could eventually shine in gamma-rays at LAT-detection levels. Furthermore, the energy-flux distributions of the different blazar populations are in good agreement with extrapolation from earlier catalogs.« less

A Lithium Abundance Study of Solar-type Stars in Blanco 1 using the 2.1m McDonald Telescope: Developing Undergraduate Research Experiences.

NASA Astrophysics Data System (ADS)

Cargile, Phillip; James, D. J.; Villalon, K.; Girgenti, S.; Mermilliod, J.

2007-12-01

We present a new catalog of lithium equivalent widths for 20 solar-type stars in the young (60-100 Myr), nearby (250 pc) open cluster Blanco 1, measured from high-resolution spectra (R 30,000), taken during an observing run on the 2.1m telescope at McDonald Observatory. These new lithium data, coupled with the 20 or so extant measurements in the literature, are used in combination with the results of a recently completed standardized BVIc CCD survey, and corresponding 2MASS near-infrared colors, to derive precise lithium abundances for solar-type stars in Blanco 1. Comparing these new results with the existing lithium dataset for other open clusters, we investigate the mass- and age-dependent lithium depletion distribution among early-epoch (< 1Gyr) solar-type stars, and specifically, the lithium abundance scatter as a function of mass in Blanco 1. Our scientific project is highly synergystic with a pedagogical philosophy. We have instituted a program whereby undergraduate students - typically majoring in Liberal Arts and performing an independent study in Astronomy - receive hands-on research experience observing with the 2.1m telescope at the McDonald Observatory. After their observing run, these undergraduates take part in the reduction and analysis of the acquired spectra, and their research experience typically culminates in writing an undergraduate thesis and/or giving a professional seminar to the Astronomy group at Vanderbilt University.

Trends in Basic Mathematical Competencies of Beginning Undergraduates in Ireland, 2003-2013

ERIC Educational Resources Information Center

Treacy, Páraic; Faulkner, Fiona

2015-01-01

Deficiencies in beginning undergraduate students' basic mathematical skills has been an issue of concern in higher education, particularly in the past 15 years. This issue has been tracked and analysed in a number of universities in Ireland and internationally through student scores recorded in mathematics diagnostic tests. Students beginning…

The Five Year Fermi/GBM Magnetar Burst Catalog

NASA Astrophysics Data System (ADS)

Collazzi, A. C.; Kouveliotou, C.; van der Horst, A. J.; Younes, G. A.; Kaneko, Y.; Göğüş, E.; Lin, L.; Granot, J.; Finger, M. H.; Chaplin, V. L.; Huppenkothen, D.; Watts, A. L.; von Kienlin, A.; Baring, M. G.; Gruber, D.; Bhat, P. N.; Gibby, M. H.; Gehrels, N.; McEnery, J.; van der Klis, M.; Wijers, R. A. M. J.

2015-05-01

Since launch in 2008, the Fermi Gamma-ray Burst Monitor (GBM) has detected many hundreds of bursts from magnetar sources. While the vast majority of these bursts have been attributed to several known magnetars, there is also a small sample of magnetar-like bursts of unknown origin. Here, we present the Fermi/GBM magnetar catalog, providing the results of the temporal and spectral analyses of 440 magnetar bursts with high temporal and spectral resolution. This catalog covers the first five years of GBM magnetar observations, from 2008 July to 2013 June. We provide durations, spectral parameters for various models, fluences, and peak fluxes for all the bursts, as well as a detailed temporal analysis for SGR J1550-5418 bursts. Finally, we suggest that some of the bursts of unknown origin are associated with the newly discovered magnetar 3XMM J185246.6+0033.7.

VizieR Online Data Catalog: The Red MSX Source Survey: massive protostars (Lumsden+, 2013)

NASA Astrophysics Data System (ADS)

Lumsden, S. L.; Hoare, M. G.; Urquhart, J. S.; Oudmaijer, R. D.; Davies, B.; Mottram, J. C.; Cooper, H. D. B.; Moore, T. J. T.

2013-10-01

The Midcourse Space Experiment (MSX) satellite mission included an astronomy experiment (SPIRIT III) designed to acquire mid-infrared photometry of sources in the Galactic plane (b<5°). MSX had a raw resolution of 18.3", a beam size 50 times smaller than that of IRAS at 12 and 25um. MSX observed six bands between 4 and 21um, of which the four between 8 and 21um are sensitive to astronomical sources. We used v2.3 of the MSX PSC (Egan et al. 2003, Cat. V/114) as our basic input, restricting ourselves to the main Galactic plane catalog, which excludes sources seen in only a single observing pass and those seen in multiple passes but with low significance. We restricted our catalog to 10

77 FR 77085 - Changes in Flood Hazard Determinations

Federal Register 2010, 2011, 2012, 2013, 2014

2012-12-31

... Docket Town of Tea (11-08- The Honorable John City Hall, 600 East June 18, 2012 460143 No.: B-1252). 0969P). Lawler, Mayor, Town 1st Street, Tea, SD of Tea, P.O. Box 57064. 128, Tea, SD 57064. (Catalog of...

A catalog of video records of the 2013 Chelyabinsk superbolide

NASA Astrophysics Data System (ADS)

Borovička, J.; Shrbený, L.; Kalenda, P.; Loskutov, N.; Brown, P.; Spurný, P.; Cooke, W.; Blaauw, R.; Moser, D. E.; Kingery, A.

2016-01-01

The Chelyabinsk superbolide of February 15, 2013, was caused by the atmospheric entry of a ~19 m asteroid with a kinetic energy of 500 kT TNT just south of the city of Chelyabinsk, Russia. It was a rare event; impacts of similar energy occur on the Earth only a few times per century. Impacts of this energy near such a large urban area are expected only a few times per 10 000 years. A number of video records obtained by casual eyewitnesses, dashboard cameras in cars, security, and traffic cameras were made publicly available by their authors on the Internet. These represent a rich repository for future scientific studies of this unique event. To aid researchers in the archival study of this airburst, we provide and document a catalog of 960 videos showing various aspects of the event. Among the video records are 400 distinct videos showing the bolide itself and 108 videos showing the illumination caused by the bolide. Other videos show the dust trail left in the atmosphere, the arrival of the blast wave on the ground, or the damage caused by the blast wave. As these video recordings have high scientific, historical, and archival value for future studies of this airburst, a systematic documentation and description of records is desirable. Many have already been used for scientific analyses. We give the exact locations where 715 videos were taken as well as details of the visible/audible phenomena in each video recording. An online version of the published catalog has been developed and will be regularly updated to provide a long-term database for investigators. An online version of the catalog is available at http://meteor.asu.cas.cz/Chelyabinsk/

Possible slow periglacial mass wasting at the Southern Hemisphere on Mars.

NASA Astrophysics Data System (ADS)

Johnsson, Andreas; Reiss, Dennis; Hauber, Ernst; Hiesinger, Harald

2014-05-01

Small-scale lobate landforms which are strikingly similar to terrestrial solifluction lobes are cataloged at the Southern Hemisphere on Mars. Terrestrial periglacial solifluction lobes are formed by frost creep, a combination of repeated frost heave and thaw consolidation, and gelifluction (visco-plastic deformation of near saturated soil) in the active layer on top of the permafrost table (e.g., Matsuoka, 2001). All publically available HiRISE images between latitudes 40°S and 80°S on Mars are being used in this study. Compared to previous studies of small-scale lobes in the northern mid and high latitudes (e.g., Gallagher et al., 2011; Johnsson et al., 2012; Barrett et al., 2013), these landforms also occur, in most cases, in close spatial proximity to fluvial gullies and polygonal terrain. This study aims to investigate whether the southern small-scale lobes differ from the northern counterparts in terms of morphology and distribution. Furthermore, spatio-temporal relationships to landforms with ground-ice affinity, such as gullies and polygonal terrain, are investigated. Solifluction-like small-scale lobes have been studied in detail at the northern hemisphere on Mars (Gallagher et al., 2011), where they are widely distributed at high latitudes between 59°N and 80°N (Johnsson et al., 2012). Small-scale lobes are proposed to represent freeze-thaw activity late in Martian climate history (Gallagher et al., 2011; Balme and Gallagher, 2011; Johnsson et al, 2012; Balme et al., 2013). Small-scale lobes differ from permafrost creep (i.e. rock glaciers) in having low fronts, decimeters to less than <5 m meters in height. They also lack compression ridges and furrows and are not confined to topographic niches (i.e. valley confinement). The presence of small-scale lobes raises the question whether they have formed by a warmer-than-thought-climate, or by the influence of soil salts (i.e. perchlorates) under sub-freezing conditions (e.g., Gallagher et al., 2011). Preliminary results indicate that the small-scale lobes are distributed more equatorward than in the north. Morphometry and morphology suggest that they are distinct from permafrost creep. Even though the southern hemisphere have more impact crater slopes fewer lobes have been observed so far in this study. The project is on-going and more work is required to firmly establish their distribution and their association to gullies and polygonal terrain. Though landforms indicative of freeze-thaw activity may be rare on flat terrain on Mars, there is growing evidence that freeze-thaw conditions may have been met on mid and high latitude slopes in recent climate history on Mars. References: Matsuoka, 2001. Earth Sci. Rev. Gallagher et al., 2011. Icarus 211, Balme and Gallagher, 2011. GSL. Johnsson et al., 2012. Icarus 218, Balme et al., 2013. Prog. Phys. Geogr. 1-36. Barrett et al., 2013. EPSC2013-159.

The Perceived Readiness of the Graduates of Delaware State University to Transition into the Workforce

ERIC Educational Resources Information Center

Scott-Cheatham, Lawita Germaine

2013-01-01

This study was designed to explore the perceived readiness of the graduating seniors at Delaware State University to transition from the classroom into the workforce. Delaware State University's undergraduate graduating class of 2012, 547 undergraduate seniors, were invited to participate in an online survey comprised of 23 items--derived from the…

A Structured Approach to Honours Undergraduate Research Course, Evaluation Rubrics and Assessment

ERIC Educational Resources Information Center

Khoukhi, Amar

2013-01-01

This paper presents a new approach to the Honours Undergraduate Research Course design and implementation. The course design process, assessment and evaluation rubrics are provided. Lessons learned and the experience of the faced challenges and opportunities for two cohort offerings of the course during the winter terms of 2011 and 2012 are…

No Point Worrying? Potential Undergraduates, Study-Related Debt, and the Financial Allure of Higher Education

ERIC Educational Resources Information Center

Esson, James; Ertl, Hubert

2016-01-01

As of September 2012, the undergraduate tuition fee cap at English universities was raised from £3375 to £9000 per annum. This article explores the rationales underpinning prospective students' decision whether or not to apply to higher education following the fee increase, specifically, how this decision is influenced by perceptions of…

The Expansion of Private Loans in Postsecondary Education. Stats in Brief. NCES 2012-184

ERIC Educational Resources Information Center

Woo, Jennie H.

2011-01-01

This Statistics in Brief examines private loans by institution sector, tuition amount, student characteristics, and level. This study attempts to answer the following questions: (1) How did undergraduate borrowing from private sources change from 2003-04 to 2007-08 and who obtained private loans?; (2) To what extent did undergraduates combine…

VizieR Online Data Catalog: Merging galaxies with tidal tails in COSMOS to z=1 (Wen+, 2016)

NASA Astrophysics Data System (ADS)

Wen, Z. Z.; Zheng, X. Z.

2017-02-01

Our study utilizes the public data and catalogs from multi-band deep surveys of the COSMOS field. The UltraVISTA survey (McCracken+ 2012, J/A+A/544/A156) provides ultra-deep near-IR imaging observations of this field in the Y,J,H, and Ks-band, as well as a narrow band (NB118). The HST/ACS I-band imaging data are publicly available, allowing us to measure morphologies in the rest-frame optical for galaxies at z<=1. The HST/ACS I-band images reach a 5σ depth of 27.2 magnitude for point sources. (1 data file).

VizieR Online Data Catalog: NGC5897 red giant abundances (Koch+, 2014)

NASA Astrophysics Data System (ADS)

Koch, A.; McWilliam, A.

2014-03-01

Our observations were performed with the Magellan Inamori Kyocera Echelle (MIKE) spectrograph at the 6.5-m Magellan2/Clay Telescope at Las Campanas Observatory, Chile. The data were gathered over four nights in May 2013. (2 data files).

VizieR Online Data Catalog: Near-infrared variability in RCW 38 (Doerr+, 2013)

NASA Astrophysics Data System (ADS)

Doerr, M.; Chini, R.; Haas, M.; Lemke, R.; Nuernberger, D.

2013-03-01

Observations were carried out using the 80cm IRIS telescope of the Universitaetssternwarte Bochum near Cerro Armazones, Chile at an altitude of 2817m. The monitoring campaign was scheduled from January to March 2011. (2 data files).

Naming Collections of Solar Physics Data

NASA Astrophysics Data System (ADS)

Hourcle, Joseph

2014-06-01

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" [1] and it was followed last year by the CODATA-ICSTI report "Out of Cite, Out of Mind".[2]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.[3] 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.Unfortunately, to implement these principles, we first need to come up with appropriate groupings of data such that they can be easily cited.[4] From this, we can determine appropriate names/titles to unambiguously identify them. The Virtual Solar Observatory will need to work with PI teams to determine these groupings and document them using the DataCite schema.[5]We will present the Joint Declaration of Data Citation Principles and the DataCite schema, discuss the implication of them for solar physics data, and recommend steps towards implementation.References:[1] National Research Council, 2012. http://www.nap.edu/catalog.php?record_id=13564[2] CODATA, 2013. http://dx.doi.org/10.2481/dsj.OSOM13-043[3] FORCE11, 2014. http://www.force11.org/datacitation[4] Wynholds, 2011. http://dx.doi.org/10.2218/ijdc.v6i1.183[5] DataCite, 2013. http://dx.doi.org/10.5438/0008

VizieR Online Data Catalog: 44 SZ-selected galaxy clusters ACT observations (Sifon+, 2016)

NASA Astrophysics Data System (ADS)

Sifon, C.; Battaglia, N.; Hasselfield, M.; Menanteau, F.; Barrientos, L. F.; Bond, J. R.; Crichton, D.; Devlin, M. J.; Dunner, R.; Hilton, M.; Hincks, A. D.; Hlozek, R.; Huffenberger, K. M.; Hughes, J. P.; Infante, L.; Kosowsky, A.; Marsden, D.; Marriage, T. A.; Moodley, K.; Niemack, M. D.; Page, L. A.; Spergel, D. N.; Staggs, S. T.; Trac, H.; Wollack, E. J.

2017-11-01

ACT is a 6-metre off-axis Gregorian telescope located at an altitude of 5200um in the Atacama desert in Chile, designed to observe the CMB at arcminute resolution. Galaxy clusters were detected in the 148GHz band by matched-filtering the maps with the pressure profile suggested by Arnaud et al. (2010A&A...517A..92A), fit to X-ray selected local (z<0.2) clusters, with varying cluster sizes,θ500, from 1.18 to 27-arcmin. Because of the complete overlap of ACT equatorial observations with Sloan Digital Sky Survey Data Release 8 (SDSS DR8; Aihara et al., 2011ApJS..193...29A) imaging, all cluster candidates were assessed with optical data (Menanteau et al., 2013ApJ...765...67M). We observed 20 clusters from the equatorial sample with the Gemini Multi-Object Spectrograph (GMOS) on the Gemini-South telescope, split in semesters 2011B (ObsID:GS-2011B-C-1, PI:Barrientos/Menanteau) and 2012A (ObsID:GS-2012A-C-1, PI:Menanteau), prioritizing clusters in the cosmological sample at 0.3

NOAA's Data Catalog and the Federal Open Data Policy

NASA Astrophysics Data System (ADS)

Wengren, M. J.; de la Beaujardiere, J.

2014-12-01

The 2013 Open Data Policy Presidential Directive requires Federal agencies to create and maintain a 'public data listing' that includes all agency data that is currently or will be made publicly-available in the future. The directive requires the use of machine-readable and open formats that make use of 'common core' and extensible metadata formats according to the best practices published in an online repository called 'Project Open Data', to use open licenses where possible, and to adhere to existing metadata and other technology standards to promote interoperability. In order to meet the requirements of the Open Data Policy, the National Oceanic and Atmospheric Administration (NOAA) has implemented an online data catalog that combines metadata from all subsidiary NOAA metadata catalogs into a single master inventory. The NOAA Data Catalog is available to the public for search and discovery, providing access to the NOAA master data inventory through multiple means, including web-based text search, OGC CS-W endpoint, as well as a native Application Programming Interface (API) for programmatic query. It generates on a daily basis the Project Open Data JavaScript Object Notation (JSON) file required for compliance with the Presidential directive. The Data Catalog is based on the open source Comprehensive Knowledge Archive Network (CKAN) software and runs on the Amazon Federal GeoCloud. This presentation will cover topics including mappings of existing metadata in standard formats (FGDC-CSDGM and ISO 19115 XML ) to the Project Open Data JSON metadata schema, representation of metadata elements within the catalog, and compatible metadata sources used to feed the catalog to include Web Accessible Folder (WAF), Catalog Services for the Web (CS-W), and Esri ArcGIS.com. It will also discuss related open source technologies that can be used together to build a spatial data infrastructure compliant with the Open Data Policy.

VizieR Online Data Catalog: LX-T relation in galaxy clusters (Hilton+, 2012)

NASA Astrophysics Data System (ADS)

Hilton, M.; Romer, A. K.; Kay, S. T.; Mehrtens, N.; Lloyd-Davies, E. J.; Thomas, P. A.; Short, C. J.; Mayers, J. A.; Rooney, P. J.; Stott, J. P.; Collins, C. A.; Harrison, C. D.; Hoyle, B.; Liddle, A. R.; Mann, R. G.; Miller, C. J.; Sahlen, M.; Viana, P. T. P.; Davidson, M.; Hosmer, M.; Nichol, R. C.; Sabirli, K.; Stanford, S. A.; West, M. J.

2013-05-01

XCS-DR1 (http://www.xcs-home.org/datareleases) is constructed from 5776 XMM observations, publicly available before 2010 July. In this work, we use only the subsample of 211 XCS-DR1 clusters with spectroscopic redshifts. (1 data file).

41 CFR 101-30.704 - Agency responsibilities.

Code of Federal Regulations, 2014 CFR

2014-07-01

... 41 Public Contracts and Property Management 2 2014-07-01 2012-07-01 true Agency responsibilities. 101-30.704 Section 101-30.704 Public Contracts and Property Management Federal Property Management Regulations System FEDERAL PROPERTY MANAGEMENT REGULATIONS SUPPLY AND PROCUREMENT 30-FEDERAL CATALOG SYSTEM 30...

VizieR Online Data Catalog: OGLE-III. Magellanic Clouds stellar proper motions (Poleski+, 2012)

NASA Astrophysics Data System (ADS)

Poleski, R.; Soszynski, I.; Udalski, A.; Szymanski, M. K.; Kubiak, M.; Pietrzynski, G.; Wyrzykowski, L.; Ulaczyk, K.

2012-06-01

The OGLE-III project observed the MCs between 2001 and 2009 with 1.3-m Warsaw telescope, which is situated at the Las Campanas Observatory, Chile. The observatory is operated by the Carnegie Institution for Science. (4 data files).

Leveraging Long-term Seismic Catalogs for Automated Real-time Event Classification

NASA Astrophysics Data System (ADS)

Linville, L.; Draelos, T.; Pankow, K. L.; Young, C. J.; Alvarez, S.

2017-12-01

We investigate the use of labeled event types available through reviewed seismic catalogs to produce automated event labels on new incoming data from the crustal region spanned by the cataloged events. Using events cataloged by the University of Utah Seismograph Stations between October, 2012 and June, 2017, we calculate the spectrogram for a time window that spans the duration of each event as seen on individual stations, resulting in 110k event spectrograms (50% local earthquakes examples, 50% quarry blasts examples). Using 80% of the randomized example events ( 90k), a classifier is trained to distinguish between local earthquakes and quarry blasts. We explore variations of deep learning classifiers, incorporating elements of convolutional and recurrent neural networks. Using a single-layer Long Short Term Memory recurrent neural network, we achieve 92% accuracy on the classification task on the remaining 20K test examples. Leveraging the decisions from a group of stations that detected the same event by using the median of all classifications in the group increases the model accuracy to 96%. Additional data with equivalent processing from 500 more recently cataloged events (July, 2017), achieves the same accuracy as our test data on both single-station examples and multi-station medians, suggesting that the model can maintain accurate and stable classification rates on real-time automated events local to the University of Utah Seismograph Stations, with potentially minimal levels of re-training through time.

A dynamical study of the multiple system 17 Cygni ABFG

NASA Astrophysics Data System (ADS)

Romanenko, L. G.

2017-03-01

Adynamical study of the relative motions of the components of the inner pairs AB (ADS 12913) and FG (ADS 12889) of the quadruple heirarchical system 17 Cygni (WDS 19464+3344) is presented, as well as analysis of themotions of the outer pair AB-FG. The study is based on CCD observations obtained on the 26-inch refractor of the Pulkovo Observatory (2003-2013), position observations from the WDS catalog, Hipparcos parallaxes, and radial velocities of the components from literature data. A family of orbits for 17 Cyg AB is obtained for the first time, and has a most probable period of 6200 yrs. The apparent motion parameters (AMP) method is used, since the entire visible arc of the orbit over 1832-2013 is only 4°. The AMP method is also used to calculate the orbit of the 17 Cyg FG pair, which has a period of 238 yrs, yielding results in good agreement with the orbits derived in other studies. The ephemerides of the obtained AMP orbits, the position data for the AF pair from the WDS catalog (11 positions during 1893-2002), and Pulkovo CCD observations for 2007-2013 are used to calculate the apparent motion parameters of AB-FG outer pair, as well as a family of close-to-parabolic orbits with periods of 3.7 million years ormore. All the orbits (for both the inner and the outer pairs) are steeply inclined to theGalactic plane. Monte Carlo simulations are used to compute the probability that the outer pair is gravitationally bound, which is 47%. The similarity of the proper motions and radial velocities of all the components provides evidence that they all belong to a single stellar stream. Data from the CNS3 catalog are used to compose a list of candidate members of this stream.

Student Financing of Undergraduate Education: 2011-12. Web Tables. NCES 2015-173

ERIC Educational Resources Information Center

National Center for Education Statistics, 2014

2014-01-01

Approximately 23 million students enrolled in undergraduate postsecondary education in the United States during the 2011-12 academic year (Simone et al. 2013). The Web Tables in this report provide a comprehensive source (2011-12 National Postsecondary Student Aid Study [NPSAS:12]) of information on the financial aid that was awarded to these…

Analysis of Computer Self-Efficacy of Turkish Undergraduate Students in the Sport Management Departments

ERIC Educational Resources Information Center

Çoknaz, Dilsad; Aktag, Isil

2017-01-01

In this study computer self-efficacy of Turkish undergraduate sport management students was investigated. There were a total of 295 sport management students from three universities. Data were collected by survey which was developed by Compeau and Higgins, 1995, translated to Turkish and adapted for students by Aktag, 2013. The results showed that…

Guidelines for the undergraduate psychology major: Version 2.0.

PubMed

2016-01-01

The APA Guidelines for the Undergraduate Psychology Major: Version 2.0 (henceforth Guidelines 2.0; APA, 2013) represents a national effort to describe and develop high-quality undergraduate programs in psychology. The task force charged with the revision of the original guidelines for the undergraduate major examined the success of the document's implementation and made changes to reflect emerging best practices and to integrate psychology's work with benchmarking scholarship in higher education. Guidelines 2.0 abandoned the original distinction drawn between psychology-focused skills and psychology skills that enhance liberal arts development. Instead, Guidelines 2.0 describes five inclusive goals for the undergraduate psychology major and two developmental levels of student learning outcomes. Suggestions for assessment planning are provided for each of the five learning goals. (c) 2016 APA, all rights reserved).

The InterPlanetary Network Supplement to the Second Fermi GBM Catalog of Cosmic Gamma-Ray Bursts

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

Hurley, K.; Aptekar, R. L.; Golenetskii, S. V.

InterPlanetary Network (IPN) data are presented for the gamma-ray bursts in the second Fermi Gamma-Ray Burst Monitor (GBM) catalog. Of the 462 bursts in that catalog between 2010 July 12 and 2012 July 11, 428, or 93%, were observed by at least 1 other instrument in the 9-spacecraft IPN. Of the 428, the localizations of 165 could be improved by triangulation. For these bursts, triangulation gives one or more annuli whose half-widths vary between about 2.′3° and 16°, depending on the peak flux, fluence, time history, arrival direction, and the distance between the spacecraft. We compare the IPN localizations withmore » the GBM 1 σ , 2 σ , and 3 σ error contours and find good agreement between them. The IPN 3 σ error boxes have areas between about 8 square arcminutes and 380 square degrees, and are an average of 2500 times smaller than the corresponding GBM 3 σ localizations. We identify four bursts in the IPN/GBM sample whose origins were given as “uncertain,” but may in fact be cosmic. This leads to an estimate of over 99% completeness for the GBM catalog.« less

Development, Implementation, and Assessment of Climate Curricular Materials for Introductory Undergraduates: Lessons Learned from the InTeGrate Project's Climate of Change Module

NASA Astrophysics Data System (ADS)

Walker, B.; Fadem, C. M.; Shellito, L. J.

2014-12-01

Designing climate change curricular materials suitable for wide adoption across institutions and academic disciplines (including those outside of the geosciences) requires collaboration among faculty at different types of institutions and consideration of a variety of student populations, learning styles, and course formats. The Interdisciplinary Teaching of Geoscience for a Sustainable Future (InTeGrate) project, an NSF STEP Center program, provides opportunities for faculty to develop 2-3 week teaching modules to engage students in understanding the intersections between geoscience topics and societal issues. From 2012-2014, a team of 3 faculty from a liberal arts college, comprehensive university, and community college developed, implemented, assessed, and revised a 2-3 week module for introductory undergraduates entitled "Climate of change: interactions and feedbacks between water, air, and ice". The module uses authentic atmosphere, ocean, and cryosphere data from several regions to illustrate how climate impacts human societies and that the climate system has interacting components complicated by feedbacks, uncertainties, and human behavioral decisions. Students also consider past and present human adaptations to climate fluctuations. The module was piloted in introductory geology, meteorology, and oceanography courses during the 2012-2013 academic year, during which time formative and summative assessments were administered and used to modify the curricular materials. We will provide an overview of the module's content, instructional strategies involved in implementing the module, and methods of formative and summative assessment. We will also report on lessons learned during the development, piloting, revision, and publishing process, the importance of fostering partnerships between faculty from different institution types, and design approaches that promote widespread adoption of climate curricular materials.

The influence of MCAT and GPA preadmission academic metrics on interview scores.

PubMed

Gay, Steven E; Santen, Sally A; Mangrulkar, Rajesh S; Sisson, Thomas H; Ross, Paula T; Zaidi, Nikki L Bibler

2018-03-01

Medical school admissions interviews are used to assess applicants' nonacademic characteristics as advocated by the Association of American Medical Colleges' Advancing Holistic Review Initiative. The objective of this study is to determine whether academic metrics continue to significantly influence interviewers' scores in holistic processes by blinding interviewers to applicants' undergraduate grade point averages (uGPA) and Medical College Admission Test (MCAT). This study examines academic and demographic predictors of interview scores for two applicant cohorts at the University of Michigan Medical School. In 2012, interviewers were provided applicants' uGPA and MCAT scores; in 2013, these academic metrics were withheld from interviewers' files. Hierarchical regression analysis was conducted to examine the influence of academic and demographic variables on overall cohort interview scores. When interviewers were provided uGPA and MCAT scores, academic metrics explained more variation in interview scores (7.9%) than when interviewers were blinded to these metrics (4.1%). Further analysis showed a statistically significant interaction between cohort and uGPA, indicating that the association between uGPA and interview scores was significantly stronger for the 2012 unblinded cohort compared to the 2013 blinded cohort (β = .573, P < .05). By contrast, MCAT scores had no interactive effects on interviewer scores. While MCAT scores accounted for some variation in interview scores for both cohorts, only access to uGPA significantly influenced interviewers' scores when looking at interaction effects. Withholding academic metrics from interviewers' files may promote assessment of nonacademic characteristics independently from academic metrics.

Kepler Planet Detection Metrics: Automatic Detection of Background Objects Using the Centroid Robovetter

NASA Technical Reports Server (NTRS)

Mullally, Fergal

2017-01-01

We present an automated method of identifying background eclipsing binaries masquerading as planet candidates in the Kepler planet candidate catalogs. We codify the manual vetting process for Kepler Objects of Interest (KOIs) described in Bryson et al. (2013) with a series of measurements and tests that can be performed algorithmically. We compare our automated results with a sample of manually vetted KOIs from the catalog of Burke et al. (2014) and find excellent agreement. We test the performance on a set of simulated transits and find our algorithm correctly identifies simulated false positives approximately 50 of the time, and correctly identifies 99 of simulated planet candidates.

VizieR Online Data Catalog: Australian Dark Energy Survey (OzDES) quasar catalog (Tie+, 2017)

NASA Astrophysics Data System (ADS)

Tie, S. S.; Martini, P.; Mudd, D.; Ostrovski, F.; Reed, S. L.; Lidman, C.; Kochanek, C.; Davis, T. M.; Sharp, R.; Uddin, S.; King, A.; Wester, W.; Tucker, B. E.; Tucker, D. L.; Buckley-Geer, E.; Carollo, D.; Childress, M.; Glazebrook, K.; Hinton, S. R.; Lewis, G.; Macaulay, E.; O'Neill, C. R.; Abbott, T. M. C.; Abdalla, F. B.; Annis, J.; Benoit-Levy, A.; Bertin, E.; Brooks, D.; Carnero Rosell, A.; Carrasco Kind, M.; Carretero, J.; Cunha, C. E.; da Costa, L. N.; Depoy, D. L.; Desai, S.; Doel, P.; Eifler, T. F.; Evrard, A. E.; Finley, D. A.; Flaugher, B.; Fosalba, P.; Frieman, J.; Garcia-Bellido, J.; Gaztanaga, E.; Gerdes, D. W.; Goldstein, D. A.; Gruen, D.; Gruendl, R. A.; Gutierrez, G.; Honscheid, K.; James, D. J.; Kuehn, K.; Kuropatkin, N.; Lima, M.; Maia, M. A. G.; Marshall, J. L.; Menanteau, F.; Miller, C. J.; Miquel, R.; Nichol, R. C.; Nord, B.; Ogando, R.; Plazas, A. A.; Romer, A. K.; Sanchez, E.; Santiago, B.; Scarpine, V.; Schubnell, M.; Sevilla-Noarbe, I.; Smith, R. C.; Soares-Santos, M.; Sobreira, F.; Suchyta, E.; Swanson, M. E. C.; Tarle, G.; Thomas, D.; Walker, A. R.; DES Collaboration

2017-07-01

The Australian Dark Energy Survey (OzDES; Yuan et al. 2015MNRAS.452.3047Y) is a spectroscopic survey of the DES supernova fields using the AAOmega spectrograph (Smith et al. 2004SPIE.5492..410S) on the Anglo-Australian Telescope (AAT). The field of view of the AAT multi-object fiber-positioning system (Lewis et al. 2002MNRAS.333..279L) is well matched to DECam, making the AAT a well-suited spectroscopic follow-up instrument for DES. OzDES commenced observations at the same time as DES in 2013B and aims to measure redshifts for thousands of host galaxies of Type Ia supernovae and black hole masses for hundreds of AGNs and quasars (King et al. 2015MNRAS.453.1701K) using reverberation mapping (Blandford & McKee 1982ApJ...255..419B; Peterson 1993PASP..105..247P). The observing targets and results of OzDES observations are compiled into a spectroscopic catalog known as the Global Redshift Catalog (GRC). The GRC is updated after every OzDES observing season. In this work, we used the 2016 February version of the OzDES GRC. Here we present the OzDES Quasar Catalog of 1263 OzDES sources with Mi<-22 mag and i<22 mag that are spectroscopically confirmed quasars. (1 data file).

Barriers to human papillomavirus vaccine acceptability in Israel.

PubMed

Fisher, William A; Laniado, Hila; Shoval, Hila; Hakim, Marwan; Bornstein, Jacob

2013-11-22

Barriers to human papillomavirus (HPV) vaccine acceptability in Israel include Israel's relatively low incidence of cervical cancer; the religiously-based 80% circumcision rate in Israel, which is regarded as contributing to the lower incidence of HPV infection in the country; the fact that HPV vaccine provides immunity against only few virus types; the vaccine's high cost; and the perception that HPV transmission is associated with unacceptable sexual relations. A recent survey has demonstrated that, following media two campaigns, Israeli's level of awareness of the vaccine increased but the actual vaccination rate remained low, at approximately 10%. Survey findings also indicated that an enduring barrier to HPV vaccination is the vaccine's high cost. Recent research on a convenience sample of Israeli undergraduate women 21 to 24 years of age showed that intentions to receive HPV vaccination in the coming year were a function of women's attitudes towards getting vaccinated and their perceptions of social support for doing so. Undergraduate women who intended to be vaccinated perceived the prevention of cervical cancer, avoidance of personal health threat, and avoidance of HPV infection per se to be the advantages of undergoing HPV vaccination. Disadvantages of getting vaccinated included fear of vaccine side effects, cost of the vaccine, and newness of the vaccine, doubts about vaccines, time required to undergo multiple vaccinations, and dislike of injections. Friends', mothers' and physicians' recommendations influenced women's intentions to be vaccinated in the coming year as well. This article forms part of a regional report entitled "Comprehensive Control of HPV Infections and Related Diseases in Israel" Vaccine Volume 31, Supplement 8, 2013. Updates of the progress in the field are presented in a separate monograph entitled "Comprehensive Control of HPV Infections and Related Diseases" Vaccine Volume 30, Supplement 5, 2012. Copyright © 2013 Elsevier Ltd. All rights reserved.

Cooperative learning in 'Special Needs in Dentistry' for undergraduate students using the Jigsaw approach.

PubMed

Suárez-Cunqueiro, M M; Gándara-Lorenzo, D; Mariño-Pérez, R; Piñeiro-Abalo, S; Pérez-López, D; Tomás, I

2017-11-01

The goals of this study were to (i) describe the use of the Jigsaw approach for the resolution of clinical cases by undergraduate students in the subject 'Special Needs in Dentistry' and (ii) assess the impact of its implementation on academic performance and the students' perception. The Jigsaw approach was applied to the fifth-year in the subject 'Special Needs in Dentistry', as part of the Dentistry degree curriculum of the University of Santiago de Compostela, during the academic years 2012/2013 and 2013/2014. A total of 109 dental students were enrolled in the study, and the final marks of the Jigsaw (n = 55) and the non-Jigsaw groups (n = 54) were compared. Students' perceptions on the Jigsaw technique were assessed using a 13-question questionnaire. Academic performance based on the final examination mark for the Jigsaw and non-Jigsaw groups was 6.45 ± 1.49 and 6.13 ± 1.50, respectively. There were not students in the Jigsaw group who failed to attend the mandatory examination (0% vs. 12.96% in the non-Jigsaw group, P = 0.006). The questionnaire's internal consistency was 0.90. The mean value for all the questionnaire items was 3.80, with the highest response score of 4.35 for the statement 'I have seen the complexity that the resolution of a clinical case can involve'. Based on the students' perceptions, the Jigsaw approach could contribute to a better understanding of the complexity of solving clinical cases in the subject 'Special Needs in Dentistry'. However, further investigations should be conducted to analyse the influence of this technique on students' academic performance in the field of clinical dentistry. © 2016 John Wiley & Sons A/S. Published by John Wiley & Sons Ltd.

VizieR Online Data Catalog: Optical transit light curves of WASP-57 (Southworth+, 2015)

NASA Astrophysics Data System (ADS)

Southworth, J.; Mancini, L.; Tregloan-Reed, J.; Calchi Novati, S.; Ciceri, S.; D'Ago, G.; Delrez, L.; Dominik, M.; Evans, D. F.; Gillon, M.; Jehin, E.; Jorgensen, U. G.; Haugbolle, T.; Lendl, M.; Arena, C.; Barbieri, L.; Barbieri, M.; Corfini, G.; Lopresti, C.; Marchini, A.; Marino, G.; Alsubai, K. A.; Bozza, V.; Bramich, D. M.; Figuera Jaimes, R.; Hinse, T. C.; Henning, Th.; Hundertmark, M.; Juncher, D.; Korhonen, H.; Popovas, A.; Rabus, M.; Rahvar, S.; Schmidt, R. W.; Skottfelt, J.; Snodgrass, C.; Starkey, D.; Surdej, J.; Wertz, O.

2018-01-01

Two complete transits of WASP-57 were observed using the 1.54 m Danish Telescope and DFOSC instrument at ESO La Silla, Chile (see Dominik et al. 2010AN....331..671D), on the dates 2014/05/18 and 2014/06/24. Both transits were obtained through a Bessell R filter. The transit on 2014/06/24 observed with DFOSC was also monitored using GROND (Greiner et al. 2008PASP..120..405G) mounted on the MPG 2.2 m telescope at La Silla, Chile. GROND was used to obtain light curves simultaneously in four passbands, which approximate the SDSS g, r, i and z bands. We observed WASP-57 on the night of 2012/05/10 using the BUSCA instrument on the 2.2 m telescope at Calar Alto Astronomical Observatory. BUSCA is capable of observing simultaneously in four passbands, for which we chose Gunn u, g, r and z. One transit of WASP-57 was observed on 2012/04/01 with EulerCam, using the same methods as for the EulerCam transit in Faedi et al. (2013, J/A+A/551/A73). We obtained 212 images through a Gunn r filter, without applying a defocus to the instrument. Two transits of WASP-57 were observed on 2012/03/15 and 2012/04/01 using the 0.6 m TRAPPIST robotic telescope located at La Silla (Gillon et al. 2011EPJWC..1106002G; Jehin et al. 2011Msngr.145....2J). Images were obtained with a slight defocus and through a blue-blocking filter that has a transmittance greater than 90 per cent from 500 nm to beyond 1000 nm. (1 data file).

78 FR 4966 - Puerto Rico Disaster #PR-00018

Federal Register 2010, 2011, 2012, 2013, 2014

2013-01-23

... SMALL BUSINESS ADMINISTRATION [Disaster Declaration 13445 and 13446] Puerto Rico Disaster PR-00018... Administrative declaration of a disaster for the Commonwealth of Puerto Rico dated 01/10/2013. Incident: Tropical... which received an EIDL Declaration is Puerto Rico. (Catalog of Federal Domestic Assistance Numbers 59002...

What if a State Required Civic Learning for All Its Undergraduates?

ERIC Educational Resources Information Center

Reiff, John D.

2016-01-01

This article tells the story of the first state in the U.S. to set the expectation that every undergraduate in public higher education would be involved in civic learning. In 2012, the Massachusetts Board of Higher Education made "Preparing Citizens" one of seven key outcomes of its Vision Project for public higher education. In 2014,…

Borrowing at the Maximum: Undergraduate Stafford Loan Borrowers in 2007-08. Stats in Brief. NCES 2012-161

ERIC Educational Resources Information Center

Wei, Christina Chang; Skomsvold, Paul

2011-01-01

Using data from the 2007-08 National Postsecondary Student Aid Study (NPSAS:08), this Statistics in Brief examines the extent to which undergraduate students borrow the maximum possible within the limits of the Stafford loan program (the program maximum) and their own financial need and student budgets (the individual maximum). Students who…

41 CFR 101-30.100 - Scope of subpart.

Code of Federal Regulations, 2014 CFR

2014-07-01

... 41 Public Contracts and Property Management 2 2014-07-01 2012-07-01 true Scope of subpart. 101-30.100 Section 101-30.100 Public Contracts and Property Management Federal Property Management Regulations System FEDERAL PROPERTY MANAGEMENT REGULATIONS SUPPLY AND PROCUREMENT 30-FEDERAL CATALOG SYSTEM 30...

41 CFR 101-30.600 - Scope of subpart.

Code of Federal Regulations, 2014 CFR

2014-07-01

... 41 Public Contracts and Property Management 2 2014-07-01 2012-07-01 true Scope of subpart. 101-30.600 Section 101-30.600 Public Contracts and Property Management Federal Property Management Regulations System FEDERAL PROPERTY MANAGEMENT REGULATIONS SUPPLY AND PROCUREMENT 30-FEDERAL CATALOG SYSTEM 30...

41 CFR 101-30.700 - Scope of subpart.

Code of Federal Regulations, 2014 CFR

2014-07-01

... 41 Public Contracts and Property Management 2 2014-07-01 2012-07-01 true Scope of subpart. 101-30.700 Section 101-30.700 Public Contracts and Property Management Federal Property Management Regulations System FEDERAL PROPERTY MANAGEMENT REGULATIONS SUPPLY AND PROCUREMENT 30-FEDERAL CATALOG SYSTEM 30...

41 CFR 101-30.4900 - Scope of subpart.

Code of Federal Regulations, 2014 CFR

2014-07-01

... 41 Public Contracts and Property Management 2 2014-07-01 2012-07-01 true Scope of subpart. 101-30.4900 Section 101-30.4900 Public Contracts and Property Management Federal Property Management Regulations System FEDERAL PROPERTY MANAGEMENT REGULATIONS SUPPLY AND PROCUREMENT 30-FEDERAL CATALOG SYSTEM 30...

41 CFR 101-30.300 - Scope of subpart.

Code of Federal Regulations, 2014 CFR

2014-07-01

... 41 Public Contracts and Property Management 2 2014-07-01 2012-07-01 true Scope of subpart. 101-30.300 Section 101-30.300 Public Contracts and Property Management Federal Property Management Regulations System FEDERAL PROPERTY MANAGEMENT REGULATIONS SUPPLY AND PROCUREMENT 30-FEDERAL CATALOG SYSTEM 30...

77 FR 8228 - Applications for New Awards; Developing Hispanic-Serving Institutions Program

Federal Register 2010, 2011, 2012, 2013, 2014

2012-02-14

... DEPARTMENT OF EDUCATION Applications for New Awards; Developing Hispanic-Serving Institutions Program AGENCY: Office of Postsecondary Education, Department of Education. ACTION: Notice. Overview Information: Developing Hispanic-Serving Institutions (HSI) Program Notice inviting applications for new awards for fiscal year (FY) 2012. Catalog of...

Value of Undergraduate Internship Experiences at NOAA: Analysis of Survey Results

NASA Astrophysics Data System (ADS)

Kaplan, M.

2014-12-01

This presentation will examine survey data from over 500 undergraduates who participated in summer internships at NOAA facilities as Ernest F. Hollings Scholars and Educational Partnership Program (EPP) Undergraduate Scholars. NOAA selects over 100 students per year to receive academic support in their junior and senior years and a paid summer internship at any NOAA facility in the country. Scholars are hosted by NOAA mentors who actively oversee summer research activities. Analysis of survey results identified six thematic impacts from the internship experience (McIntosh and Baek, 2013).

Health assessment of French university students and risk factors associated with mental health disorders

PubMed Central

Geghre, Nicolas; Darmon, David; Rampal, Marion; Brandone, Diane; Gozzo, Jean-Michel; Haas, Hervé; Rebouillat-Savy, Karine; Caci, Hervé; Avillach, Paul

2017-01-01

Objective The first year of university is a particularly stressful period and can impact academic performance and students’ health. The aim of this study was to evaluate the health and lifestyle of undergraduates and assess risk factors associated with psychiatric symptoms. Materials and methods Between September 2012 and June 2013, we included all undergraduate students who underwent compulsory a medical visit at the university medical service in Nice (France) during which they were screened for potential diseases during a diagnostic interview. Data were collected prospectively in the CALCIUM database (Consultations Assistés par Logiciel pour les Centres Inter-Universitaire de Médecine) and included information about the students’ lifestyle (living conditions, dietary behavior, physical activity, use of recreational drugs). The prevalence of psychiatric symptoms related to depression, anxiety and panic attacks was assessed and risk factors for these symptoms were analyzed using logistic regression. Results A total of 4,184 undergraduates were included. Prevalence for depression, anxiety and panic attacks were 12.6%, 7.6% and 1.0%, respectively. During the 30 days preceding the evaluation, 0.6% of the students regularly drank alcohol, 6.3% were frequent-to-heavy tobacco smokers, and 10.0% smoked marijuana. Dealing with financial difficulties and having learning disabilities were associated with psychiatric symptoms. Students who were dissatisfied with their living conditions and those with poor dietary behavior were at risk of depression. Being a woman and living alone were associated with anxiety. Students who screened positively for any psychiatric disorder assessed were at a higher risk of having another psychiatric disorder concomitantly. Conclusion The prevalence of psychiatric disorders in undergraduate students is low but the rate of students at risk of developing chronic disease is far from being negligible. Understanding predictors for these symptoms may improve students’ health by implementing targeted prevention campaigns. Further research in other French universities is necessary to confirm our results. PMID:29176864

Health assessment of French university students and risk factors associated with mental health disorders.

PubMed

Tran, Antoine; Tran, Laurie; Geghre, Nicolas; Darmon, David; Rampal, Marion; Brandone, Diane; Gozzo, Jean-Michel; Haas, Hervé; Rebouillat-Savy, Karine; Caci, Hervé; Avillach, Paul

2017-01-01

The first year of university is a particularly stressful period and can impact academic performance and students' health. The aim of this study was to evaluate the health and lifestyle of undergraduates and assess risk factors associated with psychiatric symptoms. Between September 2012 and June 2013, we included all undergraduate students who underwent compulsory a medical visit at the university medical service in Nice (France) during which they were screened for potential diseases during a diagnostic interview. Data were collected prospectively in the CALCIUM database (Consultations Assistés par Logiciel pour les Centres Inter-Universitaire de Médecine) and included information about the students' lifestyle (living conditions, dietary behavior, physical activity, use of recreational drugs). The prevalence of psychiatric symptoms related to depression, anxiety and panic attacks was assessed and risk factors for these symptoms were analyzed using logistic regression. A total of 4,184 undergraduates were included. Prevalence for depression, anxiety and panic attacks were 12.6%, 7.6% and 1.0%, respectively. During the 30 days preceding the evaluation, 0.6% of the students regularly drank alcohol, 6.3% were frequent-to-heavy tobacco smokers, and 10.0% smoked marijuana. Dealing with financial difficulties and having learning disabilities were associated with psychiatric symptoms. Students who were dissatisfied with their living conditions and those with poor dietary behavior were at risk of depression. Being a woman and living alone were associated with anxiety. Students who screened positively for any psychiatric disorder assessed were at a higher risk of having another psychiatric disorder concomitantly. The prevalence of psychiatric disorders in undergraduate students is low but the rate of students at risk of developing chronic disease is far from being negligible. Understanding predictors for these symptoms may improve students' health by implementing targeted prevention campaigns. Further research in other French universities is necessary to confirm our results.

Florida Gulf Coast University Annual Accountability Report, 2013-14

ERIC Educational Resources Information Center

Board of Governors, State University System of Florida, 2014

2014-01-01

This statistical report provides data tables on Florida Gulf Coast University's (FGCU's) financial resources, personnel, enrollment, undergraduate education, graduate education, and research & economic development. Highlighted data include: (1) Recent results (fall 2013) of FGCU's participation in the National Survey of Student Engagement…

VizieR Online Data Catalog: Photometry for HATS-31 through HATS-35 (de Val-Borro+, 2016)

NASA Astrophysics Data System (ADS)

de Val-Borro, M.; Bakos, G. A.; Brahm, R.; Hartman, J. D.; Espinoza, N.; Penev, K.; Ciceri, S.; Jordan, A.; Bhatti, W.; Csubry, Z.; Bayliss, D.; Bento, J.; Zhou, G.; Rabus, M.; Mancini, L.; Henning, T.; Schmidt, B.; Tan, T. G.; Tinney, C. G.; Wright, D. J.; Kedziora-Chudczer, L.; Bailey, J.; Suc, V.; Durkan, S.; Lazar, J.; Papp, I.; Sari, P.

2017-05-01

The HATSouth survey is a global network of homogeneous, completely automated wide-field telescopes located at three sites in the Southern Hemisphere: HS-1 and -2 are located at Las Campanas Observatory (LCO) in Chile, HS-3 and -4 are located at the High Energy Stereoscopic Survey (H.E.S.S.) site in Namibia, and HS-5 and -6 are located at Siding Spring Observatory (SSO) in Australia. Observations are performed using a Sloan-r filter with four-minute exposures. The HATSouth network was commissioned in 2009 and since then has proved to be a robust system for the monitoring of time-variable phenomena. Each HATSouth unit consists of four Takahashi E180 astrographs with an aperture of 18cm and an f/2.8 focal ratio on a common mount, equipped with Apogee 4096*4096 U16M ALTA cameras. HATS-31 was observed with the HS-1.4/G565 on 2012 Dec-2013 Jun, with the HS-3.4/G565 on 2012 Dec-2013 Jul, and with the HS-5.4/G565 on 2012 Dec-2013 Jul. HATS-32 was observed with the HS-2.3/G586 on 2010 Aug-2011 Nov, with the HS-4.3/G586 on 2010 Aug-2011 Nov, and with the HS-6.3/G586 on 2010 Aug-2011 Nov. HATS-33 was observed with the HS-1.4/G747 on 2013 Mar-2013 Oct, with the HS-2.4/G747 on 2013 Sep-2013 Oct, with the HS-3.4/G747 on 2013 Apr-2013 Nov, with the HS-4.4/G747 on 2013 Sep-2013 Nov, with the HS-5.4/G747 on 2013 Mar-2013 Nov, and with the HS-6.4/G747 on 2013 Sep-2013 Nov. HATS-34 was observed with the HS-2.4/G754 on 2012 Sep-2012 Dec, with the HS-4.4/G754 on 2012 Sep-2013 Jan, and with the HS-6.4/G754 on 2012 Sep-2012 Dec. HATS-35 was observed with the HS-2.4/G778 on 2011 May-2012 Nov, with the HS-4.4/G778 on 2011 Jul-2012 Nov, with the HS-6.4/G778 on 2011 Apr-2012 Oct. The egress of HATS-31b was observed on 2015 February 28 and 2015 April 02 with the Las Cumbres Observatory Global Telescope (LCOGT) 1m+Cerro Tololo Inter-American Observatory (CTIO) telescope network and the Swope 1m telescopes, respectively. Additionally, an almost full transit of HATS-31b was observed with LCOGT 1m+South African Astronomical Observatory/Santa Barbara Instrument Group (LCOGT 1 m+SAAO/SBIG) on 2015 March 6. Another three partial transits of HATS-32b were observed with the Perth Exoplanet Survey Telescope (PEST) 0.3m, DK 1.54m, and the Swope 1m telescopes on 2014 Jul 09, 2014 Nov 04, and 2015 May 28, respectively. The egress of HATS-33 was measured with the 1m LCOGT at CTIO on 2015 May 20. Both ingress and egress of HATS-34b were observed by the PEST 0.3m on 2014 Oct 26 and by the Danish Faint Object Spectrograph and Camera (DFOSC) on the DK 1.54m telescope on 2014 Nov 03. HATS-34b was also observed using Anglo-Australian Telescope 3.9m/InfraRed Imaging Spectrograph 2 (AAT 3.9m/IRIS2) on 2015 Sep 25 but This light curve covers a predicted secondary eclipse event, it is not included in the analysis carried out to determine the system parameters for HATS-34 (however, it is included in the analysis carried out to exclude blend scenarios). Finally, five partial transit events of HATS-35b were obtained between 2015 June 12 and 2015 July 24 using the LCOGT network at CTIO on 2015 Jun 12, 2015 Jul 15 and 2015 Jul 24, at SAAO on 2015 Jul 14, and at SSO on 2015 Jul 18. Reconnaissance spectroscopy was carried out using the Wide Field Spectrograph (WiFeS) on the Australian National University (ANU) 2.3m telescope at SSO on 2014 Dec 30-31 and 2015 Jan 1 for HATS-31, on 2014 Jun 3-5 and 2014 Jun 4 for HATS-32, on 2014 Dec-2015 Mar and 2015 Mar 4 for HATS-33, on 2014 Oct 4 and 2014 Oct 4-10 for HATS-34, and on 2014 Oct 5 and 2014 Oct 11 for HATS-35. Medium-resolution WiFeS observations spectral resolution was R=λ/Δλ=7000. We obtained 11 spectra using CYCLOPS2+University College London Echelle Spectrograph (CYCLOPS2+UCLES; Δλ/λ/1000=70) at the 3.9m AAT on 2015 May 7-13 for HATS-33, 11 spectra using the High-Accuracy Radial velocity Planetary Searcher (HARPS; Δλ/λ/1000=115) on the European Southern Observatory (ESO) 3.6m telescope (6 spectra on 2015 Feb 14-19 for HATS-31; 3 spectra on 2015 Apr 6-8 for HATS-33; 2 spectra on 2015 Apr 7-8 for HATS-35), 10 spectra using CORALIE (Δλ/λ/1000=60) on the Euler 1.2m telescope (5 spectra on 2015 Mar-Jun for HATS-33; 5 spectra on 2014 Nov-2015 Jun for HATS-35), and 32 spectra with Fiber-fed Extended Range Optical Spectrograph (FEROS; Δλ/λ/1000=48) at the Max Planck Gesellschaft (MPG) 2.2m telescope (8 spectra on 2014 Jul-2015 Jun for HATS-32; 4 spectra on 2015 May-Jul for HATS-33; 10 spectra on 2015 Jun-Jul for HATS-34; 10 spectra on 2015 Jun-Jul for HATS-35). The photometric data are available in Table3. The high-resolution spectroscopic data are provided in Table8. (3 data files).

Social Connectedness and Life Satisfaction: Comparing Mean Levels for 2 Undergraduate Samples and Testing for Improvement Based on Brief Counseling

ERIC Educational Resources Information Center

Blau, Gary; DiMino, John; DeMaria, Peter A.; Beverly, Clyde; Chessler, Marcy; Drennan, Rob

2016-01-01

Objectives: Comparing the mean levels of social connectedness and life satisfaction, and analyzing their relationship for 2 undergraduate samples, and testing for an increase in their means for a brief counseling sample. Participants: Between October 2013 and May 2015, 3 samples were collected: not-in-counseling (NIC; n = 941), initial counseling…

A Curricular Analysis of Undergraduate Technology & Engineering Teacher Preparation Programs in the United States

ERIC Educational Resources Information Center

Litowitz, Len S.

2014-01-01

Technology & engineering teacher preparation programs at colleges and universities in the United States have been in a state of decline since the 1970's. In the fall of 2013 a study was conducted to compare the required curricula of the 24 undergraduate programs that maintain enrollment of 20 students or more in order to determine what a…

Development of a Blended Instructional Model via Weblog to Enhance English Summary Writing Ability of Thai Undergraduate Students

ERIC Educational Resources Information Center

Termsinsuk, Saisunee

2015-01-01

The objective of this research and development was to develop an effective blended instructional model via weblog to enhance English summary writing ability of Thai undergraduate students. A sample group in the English program of Nakhon Ratchasima Rajabhat University was studied in academic year 2010-2013. The research instruments were an…

VizieR Online Data Catalog: NGC 300 giant dust clouds (Riener+, 2018)

NASA Astrophysics Data System (ADS)

Riener, M.; Faesi, C. M.; Forbrich, J.; Lada, C. J.

2017-11-01

We obtained photometric observations of NGC 300 with the Herschel Space Observatory (PI: Jan Forbrich) with two of its instruments,the Spectral and Photometric Imaging Receiver (SPIRE) and the Photodetector Array Camera and Spectrometer (PACS). The SPIRE observations took place on 2012 May 11 with a total exposure time of 4558s. The two PACS observations were carried out on 2012 June 25 with a total exposure time of 3245 and 3803s. (2 data files).

VizieR Online Data Catalog: L and T dwarfs from UKIDSS LAS (Marocco+, 2015)

NASA Astrophysics Data System (ADS)

Marocco, F.; Jones, H. R. A.; Day-Jones, A. C.; Pinfield, D. J.; Lucas, P. W.; Burningham, B.; Zhang, Z. H.; Smart, R. L.; Gomes, J. I.; Smith, L.

2015-11-01

The objects presented here have been selected from the UKIDSS LAS 7th Data Release. The details of the selection criteria can be found in Day-Jones et al. (2013, Cat. J/MNRAS/430/1171, hereafter ADJ13). (5 data files).

VizieR Online Data Catalog: Hard X-ray survey from Swift-BAT 2004-2010 (Baumgartner+, 2013)

NASA Astrophysics Data System (ADS)

Baumgartner, W. H.; Tueller, J.; Markwardt, C. B.; Skinner, G. K.; Barthelmy, S.; Mushotzky, R. F.; Evans, P. A.; Gehrels, N.

2013-09-01

This paper extends the BAT 22 month paper (Tueller et al. 2010, Cat. J/ApJS/186/378) to include all sources detected in the first 70 months of data between 2004 December and 2010 September. (2 data files).

Introducing the Japan Unified HIgh-Resolution Relocated Catalog for Earthquakes (JUICE) Project

NASA Astrophysics Data System (ADS)

Yano, T. E.; Takeda, T.; Shiomi, K.

2013-12-01

To understand the tectonic processes, seismogenic zones, and active fault evaluations, the precise location of earthquake hypocenters is necessary. Routinely determined hypocenters typically have uncertainties that can make seismically active areas appear more diffuse. These uncertainties influence the interpretation of what are active faults. Objective of this Japan Unified HIgh-resolution Relocated Catalog for Earthquakes (JUICE) project is to create a high-resolution earthquake relocated catalog for all of Japan. To initiate the project, we relocate hypocenters around Kanto-Tokai region. The network geometry, available phases, arrival-time reading accuracy, and knowledge of crustal structure control the accuracy of absolute hypocenter locations (Pavlis, 1986; Gomberg et al., 1990). We take advantage of having an excellent network operated by NIED Hi-net team. We use the high-quality data from this network for events from 2001 to the present. To initiate the JUICE project, we utilize more than 5,500,000 and 5,300,000 P and S phase arrival-time readings (catalog data) and waveforms for about 120,000 events between M0 and M6.5 from 2001 through 2012 in the Kanto and Tokai region. To reduce uncertainties, we apply the double-difference algorithm (hypoDD) by Waldhauser and Ellsworth (2000) to the data. To obtain the travel time differences for the pairs of earthquakes, we cross correlate the seismograms at the stations, which produces another data set -- cross-correlation data. In addition to the catalog phase data, we add 800,000 and 1,000,000 of P and S phase cross-correlations that are used to relocate hypocenters. We use Hi-net routine velocity structure (Ukawa et al., 1984) to estimate theoretical differential travel times. The newly relocated hypocenters show tighter clusters and lineaments compared to the routinely generated hypocenters. Figure 1 (a) shows the hypocenters in the Shizuoka region before relocation and (b) shows the hypocenters after relocation. Particularly, more compact clusters and lineaments clearly appear in the Shizuoka region after relocation. Significant changes are indicated in red circles and arrows for clusters and lineaments, respectively This relocated catalog will contribute to a better understanding of the depth of seismogenic zone and the mechanism for earthquakes. Because relocated hypocenters reflect the thickness of the seismogenic zone more accurately (Hauksson et al., 2012), they are more easily related to other data sets, such as geodetic, geological, gravity, and stress field measurements. We will continue expanding the area of study to relocate events all over Japan. We will apply 3D velocity model in future updated JUICE catalog to complete this project. Figure 1 (a): Map of hypocenters routinely determined by NIED Hi-net. (b): An example of hypocenters after relocations. Significant changes are indicated in red circles/arrows for clusters/lineaments.

VizieR Online Data Catalog: HD20794 HARPS radial velocities (Feng+, 2017)

NASA Astrophysics Data System (ADS)

Feng, F.; Tuomi, M.; Jones, H. R. A.

2017-05-01

HARPS radial velocities, activity indices and differential radial velocities for HD 20794. The HARPS spectra are available in the European Southern Observatory archive, and are processed using the TERRA algorithm (Anglada-Escude and Butler, 2012, Cat. J/ApJS/200/15). (1 data file).

41 CFR 101-30.000 - Scope of part.

Code of Federal Regulations, 2014 CFR

2014-07-01

... 41 Public Contracts and Property Management 2 2014-07-01 2012-07-01 true Scope of part. 101-30.000 Section 101-30.000 Public Contracts and Property Management Federal Property Management Regulations System FEDERAL PROPERTY MANAGEMENT REGULATIONS SUPPLY AND PROCUREMENT 30-FEDERAL CATALOG SYSTEM § 101-30.000...

Teaching Moments: Opening the Pipeline to Teaching Innovations

ERIC Educational Resources Information Center

Tanner, John F.; Whalen, D. Joel

2013-01-01

This paper demonstrates a strategy to speed teaching innovation transfer between marketing educators. Nine teaching innovations presented at the Society for Marketing Advances 2012 Annual Conference are offered in a brief catalog form. The reader can also download support materials at www.salesleadershipcenter.com/research.html#mer-tm13/.…

A Catalog of Architectural Tactics for Cyber-Foraging

DTIC Science & Technology

2015-01-06

Grid Access for Mobile Devices. PhD thesis, University of Southampton, 2008. [12] S.-H. Hung, J.-P. Shieh, and C.-P. Lee. Migrating android applications...computing. International Journal of Interactive Multimedia and Artificial Intelligence, 1(7):6–15, 2012. [17] K. Kumar and Y.-H. Lu. Cloud computing

VizieR Online Data Catalog: RR Lyraes in NGC 6101 (Fitzgerald+, 2012)

NASA Astrophysics Data System (ADS)

Fitzgerald, M.; Criss, J.; Lukaszewicz, T.; Frew, D. J.; Catelan, M.; Woodward, S.; Danaia, L.; McKinnon, D. H.

2012-04-01

V- and I-band observations of cluster NGC 6101 were taken over 31 nights between June 2010 and April 2011 using the Merope CCD camera attached to the robotically controlled 2-metre Faulkes Telescope South at Siding Spring Observatory, NSW, Australia. (2 data files).

77 FR 46077 - Applications for New Awards: Personnel Development To Improve Services and Results for Children...

Federal Register 2010, 2011, 2012, 2013, 2014

2012-08-02

... DEPARTMENT OF EDUCATION Applications for New Awards: Personnel Development To Improve Services and... Disabilities. Notice inviting applications for new awards for fiscal year (FY) 2012. Catalog of Federal... scientifically based research and experience, to be successful in serving those children. Priority: In accordance...

41 CFR 101-30.101-1 - Civil agency item.

Code of Federal Regulations, 2014 CFR

2014-07-01

... 41 Public Contracts and Property Management 2 2014-07-01 2012-07-01 true Civil agency item. 101-30.101-1 Section 101-30.101-1 Public Contracts and Property Management Federal Property Management Regulations System FEDERAL PROPERTY MANAGEMENT REGULATIONS SUPPLY AND PROCUREMENT 30-FEDERAL CATALOG SYSTEM 30...

41 CFR 101-30.704-2 - Other agencies.

Code of Federal Regulations, 2014 CFR

2014-07-01

... Regulations System FEDERAL PROPERTY MANAGEMENT REGULATIONS SUPPLY AND PROCUREMENT 30-FEDERAL CATALOG SYSTEM 30.7-Item Reduction Program § 101-30.704-2 Other agencies. Civil agencies participating in the Federal... 41 Public Contracts and Property Management 2 2014-07-01 2012-07-01 true Other agencies. 101-30...

VizieR Online Data Catalog: Molecular clumps in W51 giant molecular cloud (Parsons+, 2012)

NASA Astrophysics Data System (ADS)

Parsons, H.; Thompson, M. A.; Clark, J. S.; Chrysostomou, A.

2013-04-01

The W51 GMC was mapped using the Heterodyne Array Receiver Programme (HARP) receiver with the back-end digital autocorrelator spectrometer Auto-Correlation Spectral Imaging System (ACSIS) on the James Clerk Maxwell Telescope (JCMT). Data were taken in 2008 May. (2 data files).

78 FR 5755 - Change in Terminology: “Mental Retardation” to “Intellectual Disability”

Federal Register 2010, 2011, 2012, 2013, 2014

2013-01-28

... SOCIAL SECURITY ADMINISTRATION 20 CFR Parts 404 and 416 [Docket No. SSA-2012-0066] RIN 0960-AH52 Change in Terminology: ``Mental Retardation'' to ``Intellectual Disability'' AGENCY: Social Security... non- substantive change requests. (Catalog of Federal Domestic Program Nos. 96.001, Social Security...

University of Florida Annual Accountability Report, 2013-14

ERIC Educational Resources Information Center

Board of Governors, State University System of Florida, 2014

2014-01-01

This statistical report provides data tables on the University of Florida (UF's) financial resources, personnel, enrollment, undergraduate education, graduate education, and research & economic development. Highlights of UF's achievements in the 2013-2014 academic year include: (1) Upon being named the state's highest-achieving preeminent…

Undergraduate Research as a Process for STEM Teaching and Learning Systemic Change: Lessons Learned from the Council on Undergraduate Research NSF CCLI and TUES Projects

NASA Astrophysics Data System (ADS)

Ambos, E. L.; Havholm, K. G.; Malachowski, M.; Osborn, J.; Karukstis, K.

2013-12-01

For more than seven years, the Council on Undergraduate Research (CUR), the primary organization supporting programs, services, and advocacy for undergraduate research, has been working with support from the NSF's Division of Undergraduate Education (DUE) to enhance, sustain, and institutionalize undergraduate research in diverse STEM disciplines and higher education settings. The Council on Undergraduate Research comprises more than 9000 individual and 670 institutional members within a divisional structure that includes geosciences, as well as 11 other thematic areas. Through its most recent grant: 'Transformational Learning through Undergraduate Research: Comprehensive Support for Faculty, Institutions, State Systems and Consortia' (NSF DUE CCLI III Award #09-20275), CUR has been collaborating with six higher education systems, each selected after a rigorous national application process in 2010 and 2011. These six systems, which collectively represent 79 individual institutions, are the Council of Public Liberal Arts Colleges (COPLAC), University of Wisconsin System (UWS), California State University System (CSU), City University of New York (CUNY), Great Lakes Colleges Association (GLCA), and Pennsylvania State System of Higher Education (PASSHE). The more than 350 participants of faculty and senior-level administrators from the six systems are engaged in shared multi-faceted and multi-year professional development experiences. Teams from each system attended customized institutes facilitated by CUR experts in 2011-2012, during which the teams developed specific action plans focused on institutionalizing undergraduate research on their campus and within their system. The systems were reconvened as a group a year after the first institute, to chart progress toward achieving their goals. Based on interviews and surveys with participants, campus teams are making substantial progress toward implementation of robust undergraduate research programs, and are making concerted efforts to affect policy, workload, tenure and promotion and resource issues, which are often core factors in any STEM education change process. Several systems are now connecting individual campus-based undergraduate research efforts more effectively, and tying undergraduate research to regional workforce and economic development programs. Many campus teams are moving their department and colleges toward curricular innovations that emphasize scaffolding undergraduate research throughout the undergraduate curriculum. An NSF EAGER/WIDER supplement to the CUR CCLI III award was received in October 2012 and expanded the scope of the project to include deeper study of the changes processes underway at each of the six systems and to tease out the factors that can either promote or retard expansion of undergraduate research as a teaching and learning paradigm. Lessons learned from one of the six systems, the University of Wisconsin, will be highlighted.

The HEASARC Swift Gamma-Ray Burst Archive: The Pipeline and the Catalog

NASA Technical Reports Server (NTRS)

Donato, Davide; Angelini, Lorella; Padgett, C.A.; Reichard, T.; Gehrels, Neil; Marshall, Francis E.; Sakamoto, Takanori

2012-01-01

Since its launch in late 2004, the Swift satellite triggered or observed an average of one gamma-ray burst (GRB) every 3 days, for a total of 771 GRBs by 2012 January. Here, we report the development of a pipeline that semi automatically performs the data-reduction and data-analysis processes for the three instruments on board Swift (BAT, XRT, UVOT). The pipeline is written in Perl, and it uses only HEAsoft tools and can be used to perform the analysis of a majority of the point-like objects (e.g., GRBs, active galactic nuclei, pulsars) observed by Swift. We run the pipeline on the GRBs, and we present a database containing the screened data, the output products, and the results of our ongoing analysis. Furthermore, we created a catalog summarizing some GRB information, collected either by running the pipeline or from the literature. The Perl script, the database, and the catalog are available for downloading and querying at the HEASARC Web site.

The HEASARC Swift Gamma-Ray Burst Archive: The Pipeline and the Catalog

NASA Astrophysics Data System (ADS)

Donato, D.; Angelini, L.; Padgett, C. A.; Reichard, T.; Gehrels, N.; Marshall, F. E.; Sakamoto, T.

2012-11-01

Since its launch in late 2004, the Swift satellite triggered or observed an average of one gamma-ray burst (GRB) every 3 days, for a total of 771 GRBs by 2012 January. Here, we report the development of a pipeline that semi-automatically performs the data-reduction and data-analysis processes for the three instruments on board Swift (BAT, XRT, UVOT). The pipeline is written in Perl, and it uses only HEAsoft tools and can be used to perform the analysis of a majority of the point-like objects (e.g., GRBs, active galactic nuclei, pulsars) observed by Swift. We run the pipeline on the GRBs, and we present a database containing the screened data, the output products, and the results of our ongoing analysis. Furthermore, we created a catalog summarizing some GRB information, collected either by running the pipeline or from the literature. The Perl script, the database, and the catalog are available for downloading and querying at the HEASARC Web site.

Physics Enrollments in Two-Year Colleges: Results from the 2012 Survey of Physics in Two-Year Colleges. Focus On

ERIC Educational Resources Information Center

White, Susan; Chu, Raymond

2013-01-01

This "Focus On" first considers the role two-year colleges (TYCs) play in post-secondary physics education. In their 2007 Survey of Undergraduate Seniors in degree-granting physics departments, the authors asked students if they had begun their post-secondary education at a TYC. Nine percent of the physics undergraduate seniors in 2007…

Selection Methods for Undergraduate Admissions in Australia. Does the Australian Predominate Entry Scheme the Australian Tertiary Admissions Rank (ATAR) Have a Future?

ERIC Educational Resources Information Center

Blyth, Kathryn

2014-01-01

This article considers the Australian entry score system, the Australian Tertiary Admissions Rank (ATAR), and its usage as a selection mechanism for undergraduate places in Australian higher education institutions and asks whether its role as the main selection criterion will continue with the introduction of demand driven funding in 2012.…

EnviroAtlas One Meter Resolution Urban Land Cover Data (2008-2012) Web Service

EPA Pesticide Factsheets

This EnviroAtlas web service supports research and online mapping activities related to EnviroAtlas (https://www.epa.gov/enviroatlas ). The EnviroAtlas One Meter-scale Urban Land Cover (MULC) Data were generated individually for each EnviroAtlas community. Source imagery varies by community. Land cover classes mapped also vary by community and include the following: water, impervious surfaces, soil and barren land, trees, shrub, grass and herbaceous, agriculture, orchards, woody wetlands, and emergent wetlands. Accuracy assessments were completed for each community's classification. For specific information about methods and accuracy of each community's land cover classification, consult their individual metadata records: Austin, TX (https://edg.epa.gov/metadata/catalog/search/resource/details.page?uuid=%7B91A32A9D-96F5-4FA0-BC97-73BAD5D1F158%7D); Cleveland, OH (https://edg.epa.gov/metadata/catalog/search/resource/details.page?uuid=%7B82ab1edf-8fc8-4667-9c52-5a5acffffa34%7D); Des Moines, IA (https://edg.epa.gov/metadata/catalog/search/resource/details.page?uuid=%7BA4152198-978D-4C0B-959F-42EABA9C4E1B%7D); Durham, NC (https://edg.epa.gov/metadata/catalog/search/resource/details.page?uuid=%7B2FF66877-A037-4693-9718-D1870AA3F084%7D); Fresno, CA (https://edg.epa.gov/metadata/catalog/search/resource/details.page?uuid=%7B87041CF3-05BC-43C3-82DA-F066267C9871%7D); Green Bay, WI (https://edg.epa.gov/metadata/catalog/search/resource/details.page?uuid=%7BD602E7C9-7F53-4C24

Insights from a Convocation: Integrating Discovery-Based Research into the Undergraduate Curriculum

ERIC Educational Resources Information Center

Elgin, Sarah C. R.; Bangera, Gita; Decatur, Sean M.; Dolan, Erin L.; Guertin, Laura; Newstetter, Wendy C.; San Juan, Elvyra F.; Smith, Mary A.; Weaver, Gabriela C.; Wessler, Susan R.; Brenner, Kerry A.; Labov, Jay B.

2016-01-01

Recommendation 2 of the February 2012 report "Engage to Excel" from the President's Council of Advisors on Science and Technology (PCAST 2012) urges the science, technology, engineering, and mathematics (STEM) education community and funding agencies to "advocate and provide support for replacing standard laboratory courses with…

2012: A Brave New World

ERIC Educational Resources Information Center

Jeffreys, Andrea

2012-01-01

The Australian Government decision in response to the Bradley review to introduce a demand-driven funding model for undergraduate university places from 2012 was met with mixed reaction across the higher education sector. The removal of caps without subsequent fee deregulation is considered by some to be unsustainable. Opinions suggest that…

VizieR Online Data Catalog: Abundances for all seven stars in Latham 1 (O'Connell+, 2016)

NASA Astrophysics Data System (ADS)

O'Connell, J. E.; Martens, K.; Frinchaboy, P. M.

2017-03-01

Observations for all target stars were obtained at McDonald Observatory with the Otto Struve 2.1m telescope instrumented with the Sandiford Cass Echelle Spectrometer (SES; R=λ/Δλ~60000) in 2013 and 2014 June. The spectrograph setup was centered near 6175Å in 2013 and 6375Å in 2014 with wavelength coverage spanning from ~5350-6560Å and ~5560-6750Å, respectively (see Table2 for observation dates and exposure times). (3 data files).

VizieR Online Data Catalog: Optical to NIR spectra of nova V2676 Oph 2012 (Raj+, 2017)

NASA Astrophysics Data System (ADS)

Raj, A.; Das, R. K.; Walter, F. M.

2017-09-01

Near-infrared observations were obtained using the 1.2m telescope of Mt.Abu Infrared Observatory from 2012 March 29 to June 18 and the SMARTS/CTIO 1.3m telescope. The SMARTS photometry is available on the SMARTS atlas (Walter+, 2012PASP..124.1057W). Optical spectra were obtained with the Asiago 1.22m telescope + B&C spectrograph. Further low-dispersion spectra and photometry were obtained using the SMARTS 1.5m facilities. We obtained 19 spectra on an irregular cadence and with various sky conditions from 2012 April 5 through 2012 June 24. The target was observed using the COSMOS long slit spectrograph at CTIO on 2015 May 8, some three years after the outburst. (3 data files).

Prospects for asteroid mass determination from close encounters between asteroids: ESA's Gaia space mission and beyond

NASA Astrophysics Data System (ADS)

Ivantsov, Anatoliy; Hestroffer, Daniel; Eggl, Siegfried

2018-04-01

We present a catalog of potential candidates for asteroid mass determination based on mutual close encounters of numbered asteroids with massive perturbers (D>20 km). Using a novel geometric approach tuned to optimize observability, we predict optimal epochs for mass determination observations. In contrast to previous studies that often used simplified dynamical models, we have numerically propagated the trajectories of all numbered asteroids over the time interval from 2013 to 2023 using relativistic equations of motion including planetary perturbations, J2 of the Sun, the 16 major asteroid perturbers and the perturbations due to non-sphericities of the planets. We compiled a catalog of close encounters between asteroids where the observable perturbation of the sky plane trajectory is greater than 0.5 mas so that astrometric measurements of the perturbed asteroids in the Gaia data can be leveraged. The catalog v1.0 is available at ftp://dosya.akdeniz.edu.tr/ivantsov.

VizieR Online Data Catalog: The Washington Visual Double Star Catalog (Mason+ 2001-2012)

NASA Astrophysics Data System (ADS)

Mason, B. D.; Wycoff, G. L.; Hartkopf, W. I.; Douglass, G. G.; Worley, C. E.

2012-11-01

The Washington Visual Double Star Catalog (WDS) is the successor to the Index Catalogue of Visual Double Stars, 1961.0 (IDS; Jeffers and van den Bos, Publ. Lick Obs. 21). Three earlier double star catalogs in XXth century, those by Burnham (BDS, 1906, "General Catalogue of Double Stars within 121 degrees of the North Pole", Carnegie Institution of Washington), Innes (SDS, 1927, "Southern Double Star Catalogue -19 to -90 degrees", Union Observatory, Johannesburg, South Africa), and Aitken (ADS, 1932 "New General Catalogue of Double Stars within 121 degrees of the North Pole", Carnegie Institution of Washington), each covered only a portion of the sky. Both the IDS and the WDS cover the entire sky, and the WDS is intended to contain all known visual double stars for which at least one differential measure has been published. The WDS is continually updated as published data become available. Prior to this, three major updates have been published (Worley and Douglass 1984, "Washington Visual Double Star Catalog, 1984.0", U.S. Naval Observatory, Washington; Worley and Douglass 1997A&AS..125..523W, Cat. I/237; Mason, Wycoff, Hartkopf, Douglass and Worley 2001AJ....122.3466M; and Mason et al. 2006.5). The Washington Double Star Catalog (WDS) has seen numerous changes since the last major release of the catalog. The application of many techniques and considerable industry over the past few years has yielded significant gains in both the number of systems and the number of measures. Is is maintained by the US Naval Observatory, and represents the world's principal database of astrometric double and multiple star information. The WDS contains positions (J2000), discoverer designations, epochs, position angles, separations, magnitudes, spectral types, proper motions, and, when available, Durchmusterung numbers and notes for the components of the systems. (3 data files).

78 FR 64522 - Pennsylvania; Major Disaster and Related Determinations

Federal Register 2010, 2011, 2012, 2013, 2014

2013-10-29

... provided under the Stafford Act for Hazard Mitigation will be limited to 75 percent of the total eligible... eligible to apply for assistance under the Hazard Mitigation Grant Program. The following Catalog of... declaration of a major disaster for the Commonwealth of Pennsylvania (FEMA-4149-DR), dated October 1, 2013...

78 FR 14806 - Louisiana; Major Disaster and Related Determinations

Federal Register 2010, 2011, 2012, 2013, 2014

2013-03-07

... Stafford Act for Public Assistance and Hazard Mitigation will be limited to 75 percent of the total... eligible to apply for assistance under the Hazard Mitigation Grant Program. (The following Catalog of... declaration of a major disaster for the State of Louisiana (FEMA-4102-DR), dated February 22, 2013, and...

VizieR Online Data Catalog: Transiting planet WASP-19b (Tregloan-Reed+, 2013)

NASA Astrophysics Data System (ADS)

Tregloan-Reed, J.; Southworth, J.; Tappert, C.

2018-05-01

Defocussed photometry for the transiting extrasolar planetary system WASP-19. The data were obtained in the Gunn r passband using the EFOSC CCD imager on the 3.6m New Technology Telescope at ESO La Silla. The observer was Claus Tappert. (1 data file).

VizieR Online Data Catalog: VIc photometry of IR-excess stars in NGC6611 (De Marchi+ 2013)

NASA Astrophysics Data System (ADS)

de Marchi, G.; Panagia, N.; Guarcello, M. G.; Bonito, R.

2014-10-01

The data analysed in this work were extracted from the multiband photometric catalogue of NGC 6611 and of the surrounding M 16 cloud compiled by Guarcello et al. (2010, Cat. J/A+A/521/A61). (1 data file).

Study: Third of Big Groundwater Basins in Distress

NASA Image and Video Library

2015-06-16

Groundwater storage trends for Earth's 37 largest aquifers from UCI-led study using NASA GRACE data (2003-2013). Of these, 21 have exceeded sustainability tipping points and are being depleted, with 13 considered significantly distressed, threatening regional water security and resilience. http://photojournal.jpl.nasa.gov/catalog/PIA19685

VizieR Online Data Catalog: Molecular clouds in the dwarf galaxy NGC6822 (Schruba+, 2017)

NASA Astrophysics Data System (ADS)

Schruba, A.; Leroy, A. K.; Kruijssen, J. M. D.; Bigiel, F.; Bolatto, A. D.; de Blok, W. J. G.; Tacconi, L.; van Dishoeck, E. F.; Walter, F.

2017-09-01

We observed five fields in NGC 6822 with the Atacama Large Millimeter/submillimeter Array (ALMA) in Cycle 1 using the 1.3mm Band 6 receivers (project code: 2013.1.00351.S; PI. A. Schruba) in 2014 Mar 23-25. (1 data file).

University of South Florida System Annual Accountability Report, 2013-14

ERIC Educational Resources Information Center

Board of Governors, State University System of Florida, 2014

2014-01-01

This statistical report provides data tables on the University of South Florida System's (USF's) financial resources, personnel, enrollment, undergraduate education, graduate education, and research & economic development. Highlights of USF's achievements in the 2013-2014 academic year include: (1) In Tampa, USF celebrated its strongest…

EPA Interim Evaluation of 2012-2013 Milestone Progress in the Chesapeake Bay Watershed

EPA Pesticide Factsheets

This page provides the EPA interim evaluations of the 2012-2013 milestones for the Chesapeake Bay TMDL. These interim assessments provide a mid-point check on the progress made on the 2012-2013 milestones, recognizing the achievements made in 2012.

Development of a measure of college students' adherence to religious doctrine concerning sexual behavior.

PubMed

Victor, Elizabeth C; Bowman, Hilary; Thompson, Robert J

2015-01-01

The authors developed a 14-item measure of adherence to religious doctrine concerning sexual behavior (ARDSB). The ARDSB psychometric properties were investigated to better understand religious motivations associated with changes in sexual behavior that may provide support for sexual health promotion and prevention programs. Four hundred eighty-three undergraduates aged 18 to 26. Data were collected from an online survey during the 2012-2013 academic school year. Principle components factor analysis identified 2 factors: reasons to break religious doctrine and reasons to adhere to religious doctrine concerning sexual behavior. The subscales had good internal consistency. Correlations, t tests, and analyses of variance of the subscales with measures of intrinsic and extrinsic religiosity and self-reported sexual behavior and risk provide support for concurrent validity. The ARDSB could be employed as a measure to better understand sexual behavior; it is inexpensive and relatively easy to employ in both research and campus ministry settings.

6th Annual Midwest Conference for Undergraduate Women in Physics, January 18-20, 2013, Urbana, Illinois

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

Pitts, Kevin T.

This document is the program for the 6th Annual Midwest Conference for Undergraduate Women in Physics, which was held at the University of Illinois at Urbana-Champaign on January 18-20, 2013. The goals of the conference were to foster a culture in which undergraduate women are encouraged and supported to pursue, and also to succeed in, higher education in physics; to provide career information to students in physics and related fields; to give women the resources, motivation, and confidence to apply to graduate school and successfully complete a Ph.D. program in Physics; to provide information and dispel misconceptions about the applicationmore » process for graduate school and the diverse employment opportunities in physics and related fields, enabling women to make more informed decisions about their goals and attain them; and to connect female physics students with successful female physicists to whom they can relate and who can act as inspirational role models and mentors.« less

Foreshock search over a long duration using a method of setting appropriate criteria

NASA Astrophysics Data System (ADS)

Toyomoto, Y.; Kawakata, H.; Hirano, S.; Doi, I.

2016-12-01

Recently, small foreshocks have been detected using cross-correlation techniques (e.g., Bouchon et al., 2011) in which the foreshocks are identified when the cross-correlation coefficient (CC) exceeded a certain threshold. For some shallow intraplate earthquakes, foreshocks whose hypocenters were estimated to be adjacent to the main shock hypocenter were detected from several tens of minutes before the main shock occurrence (Doi and Kawakata, 2012; 2013). At least two problems remain in the cross-correlation techniques employed. First, previous studies on foreshocks used data whose durations are at most a month (Kato et al., 2013); this is insufficient to check if such events occurred only before the main shock occurrence or not. Second, CC is used for detection criteria without considering validity of the threshold. In this study, we search for foreshocks of an M 5.4 earthquake in central Nagano prefecture in Japan on June 30, 2011 with a vertical-component waveform at N.MWDH (Hi-net) station due to one of the cataloged foreshocks (M 1) as a template to calculate CC. We calculate CC between the template and continuous waveforms of the same component at the same station for two years before the main shock occurrence, and we try to overcome the problems mentioned above. We find that histogram of CC is well modeled with the normal distribution, which is similar to previous studies on tremors (e.g., Ohta and Ide, 2008). According to the model, the expected number of misdetection is less than 1 when CC > 0.63. Therefore, we regard that the waveform is due to a foreshock when CC > 0.63. As a result, foreshocks are detected only within thirteen hours immediately before the main shock occurrence for the two years. By setting an appropriate threshold, we conclude that foreshocks just before the main shock occurrence are not stationary events. Acknowledgments: We use continuous waveform records of NIED high sensitivity seismograph network in Japan (Hi-net) and the JMA unified hypocenter catalogs. This work is supported by MEXT of Japan, under its Earthquake and Volcano Hazards Observation and Research Program.

Optics and communication technology major of physics undergraduate degree at King Mongkut's Institute of Technology Ladkrabang

NASA Astrophysics Data System (ADS)

Buranasiri, Prathan

2014-09-01

A physics undergraduate degree major in optics and communication technology has been offered at King Mongkut's Institute of Technology Ladkrabang (KMITL), Bangkok, Thailand. There are nine required three credit hour courses including two laboratory courses plus a number of selections in optics and communication based technology courses. For independent thinking and industrial working skills, nine credit hours of research project, practical training or overseas studies are included for selection in the final semester. Students are encouraged to participate in international conferences and professional organizations. Recently the program, with support from SPIE and OSA, has organized its first international conference on photonic solutions 2013 (ICPS 2013).

Increasing Research Productivity in Undergraduate Research Experiences: Exploring Predictors of Collaborative Faculty–Student Publications

PubMed Central

Morales, Danielle X.; Grineski, Sara E.; Collins, Timothy W.

2017-01-01

Little attention has been paid to understanding faculty–student productivity via undergraduate research from the faculty member’s perspective. This study examines predictors of faculty–student publications resulting from mentored undergraduate research, including measures of faculty–student collaboration, faculty commitment to undergraduate students, and faculty characteristics. Generalized estimating equations were used to analyze data from 468 faculty members across 13 research-intensive institutions, collected by a cross-sectional survey in 2013/2014. Results show that biomedical faculty mentors were more productive in publishing collaboratively with undergraduate students when they worked with students for more than 1 year on average, enjoyed teaching students about research, had mentored Black students, had received more funding from the National Institutes of Health, had a higher H-index scores, and had more years of experience working in higher education. This study suggests that college administrators and research program directors should strive to create incentives for faculty members to collaborate with undergraduate students and promote faculty awareness that undergraduates can contribute to their research. PMID:28747352

The Education and Public Engagement (EPE) Component of the Ocean Observatories Initiative (OOI): Enabling Near Real-Time Data Use in Undergraduate Classrooms

NASA Astrophysics Data System (ADS)

Glenn, S. M.; Companion, C.; Crowley, M.; deCharon, A.; Fundis, A. T.; Kilb, D. L.; Levenson, S.; Lichtenwalner, C. S.; McCurdy, A.; McDonnell, J. D.; Overoye, D.; Risien, C. M.; Rude, A.; Wieclawek, J., III

2011-12-01

The National Science Foundation's Ocean Observatories Initiative (OOI) is constructing observational and computer infrastructure that will provide sustained ocean measurements to study climate variability, ocean circulation, ecosystem dynamics, air-sea exchange, seafloor processes, and plate-scale geodynamics over the next ~25-30 years. To accomplish this, the Consortium for Ocean Leadership established four Implementing Organizations: (1) Regional Scale Nodes; (2) Coastal and Global Scale Nodes; (3) Cyberinfrastructure (CI); and (4) Education and Public Engagement (EPE). The EPE, which we represent, was just recently established to provide a new layer of cyber-interactivity for educators to bring near real-time data, images and videos of our Earth's oceans into their learning environments. Our focus over the next four years is engaging educators of undergraduates and free-choice learners. Demonstration projects of the OOI capabilities will use an Integrated Education Toolkit to access OOI data through the Cyberinfrastructure's On Demand Measurement Processing capability. We will present our plans to develop six education infrastructure software modules: Education Web Services (middleware), Visualization Tools, Concept Map and Lab/Lesson Builders, Collaboration Tools, and an Education Resources Database. The software release of these tools is staggered to coincide with other major OOI releases. The first release will include stand-alone versions of the first four EPE modules (Fall 2012). Next, all six EPE modules will be integrated within the OOI cyber-framework (Fall 2013). The last release will include advanced capabilities for all six modules within a collaborative network that leverages the CI's Integrated Observatory Network (Fall 2014). We are looking for undergraduate and informal science educators to provide feedback and guidance on the project, please contact us if you are interested in partnering with us.

VizieR Online Data Catalog: The Washington Visual Double Star Catalog (Mason+ 2001-2013)

NASA Astrophysics Data System (ADS)

Mason, B. D.; Wycoff, G. L.; Hartkopf, W. I.; Douglass, G. G.; Worley, C. E.

2013-11-01

The Washington Visual Double Star Catalog (WDS) is the successor to the Index Catalogue of Visual Double Stars, 1961.0 (IDS; Jeffers and van den Bos, Publ. Lick Obs. 21). Three earlier double star catalogs in XXth century, those by Burnham (BDS, 1906, "General Catalogue of Double Stars within 121 degrees of the North Pole", Carnegie Institution of Washington), Innes (SDS, 1927, "Southern Double Star Catalogue -19 to -90 degrees", Union Observatory, Johannesburg, South Africa), and Aitken (ADS, 1932 "New General Catalogue of Double Stars within 121 degrees of the North Pole", Carnegie Institution of Washington), each covered only a portion of the sky. Both the IDS and the WDS cover the entire sky, and the WDS is intended to contain all known visual double stars for which at least one differential measure has been published. The WDS is continually updated as published data become available. Prior to this, three major updates have been published (Worley and Douglass 1984, "Washington Visual Double Star Catalog, 1984.0", U.S. Naval Observatory, Washington; Worley and Douglass 1997A&AS..125..523W, Cat. I/237; Mason, Wycoff, Hartkopf, Douglass and Worley 2001AJ....122.3466M; and Mason et al. 2006.5). The Washington Double Star Catalog (WDS) has seen numerous changes since the last major release of the catalog. The application of many techniques and considerable industry over the past few years has yielded significant gains in both the number of systems and the number of measures. Is is maintained by the US Naval Observatory, and represents the world's principal database of astrometric double and multiple star information. The WDS contains positions (J2000), discoverer designations, epochs, position angles, separations, magnitudes, spectral types, proper motions, and, when available, Durchmusterung numbers and notes for the components of the systems. (3 data files).

VizieR Online Data Catalog: SFiNCs: X-ray, IR and membership catalogs (Getman+, 2017)

NASA Astrophysics Data System (ADS)

Getman, K. V.; Broos, P. S.; Kuhn, M. A.; Feigelson, E. D.; Richert, A. J. W.; Ota, Y.; Bate, M. R.; Garmire, G. P.

2017-06-01

Sixty five X-ray observations for the 22 Star Formation in Nearby Clouds (SFiNCs) star-forming regions (SFRs) (see tables 1 and 2), made with the imaging array on the Advanced CCD Imaging Spectrometer (ACIS), were pulled from the Chandra archive (spanning 2000 Jan to 2015 Apr; see table 2). Our final Chandra-ACIS catalog for the 22 SFiNCs SFRs comprises 15364 X-ray sources (Tables 3 and 4 and section 3.2). To obtain MIR photometry for X-ray objects and to identify and measure MIR photometry for additional non-Chandra disky stars that were missed in previous studies of the SFiNCs regions (typically faint YSOs), we have reduced the archived Spitzer-IRAC data by homogeneously applying the MYStIX-based Spitzer-IRAC data reduction methods of Kuhn+ (2013, J/ApJS/209/29) to the 423 Astronomical Object Request (AORs) data sets for the 22 SFiNCs SFRs (Table 5). As in MYStIX, here the SFiNCs IRAC source catalog retains all point sources with the photometric signal-to-noise ratio >5 in both [3.6] and [4.5] channels. This catalog covers the 22 SFiNCs SFRs and their vicinities on the sky and comprises 1638654 IRAC sources with available photometric measurements for 100%, 100%, 29%, and 23% of these sources in the 3.6, 4.5, 5.8, and 8.0um bands, respectively (see table 6 and section 3.4). Source position cross correlations between the SFiNCs Chandra X-ray source catalog and an IR catalog, either the "cut-out" IRAC or 2MASS, were made using the steps described in section 3.5. Tables 7 and 8 provide the list of 8492 SFiNCs probable cluster members (SPCMs) and their main IR and X-ray properties (see section 4). (9 data files).

Data reduction and calibration for LAMOST survey

NASA Astrophysics Data System (ADS)

Luo, Ali; Zhang, Jiannan; Chen, Jianjun; Song, Yihan; Wu, Yue; Bai, Zhongrui; Wang, Fengfei; Du, Bing; Zhang, Haotong

2014-01-01

There are three data pipelines for LAMOST survey. The raw data is reduced to one dimension spectra by the data reduction pipeline(2D pipeline), the extracted spectra are classified and measured by the spectral analysis pipeline(1D pipeline), while stellar parameters are measured by LASP pipeline. (a) The data reduction pipeline. The main tasks of the data reduction pipeline include bias calibration, flat field, spectra extraction, sky subtraction, wavelength calibration, exposure merging and wavelength band connection. (b) The spectra analysis pipeline. This pipeline is designed to classify and identify objects from the extracted spectra and to measure their redshift (or radial velocity). The PCAZ (Glazebrook et al. 1998) method is applied to do the classification and redshift measurement. (c) Stellar parameters LASP. Stellar parameters pipeline (LASP) is to estimate stellar atmospheric parameters, e.g. effective temperature Teff, surface gravity log g, and metallicity [Fe/H], for F, G and K type stars. To effectively determine those fundamental stellar measurements, three steps with different methods are employed. The first step utilizes the line indices to approximately define the effective temperature range of the analyzed star. Secondly, a set of the initial approximate values of the three parameters are given based on template fitting method. Finally, we exploit ULySS (Koleva et al. 2009) to give the final values of parameters through minimizing the χ 2 value between the observed spectrum and a multidimensional grid of model spectra which is generated by an interpolating of ELODIE library. There are two other classification for A type star and M type star. For A type star, standard MK system is employed (Gray et al. 2009) to give each object temperature class and luminosity type. For M type star, they are classified into subclasses by an improved Hammer method, and metallicity of each objects is also given. During the pilot survey, algorithms were improved and the pipelines were tested. The products of LAMOST survey will include extracted and calibrated spectra in FITS format, a catalog of FGK stars with stellar parameters, a catalog of M dwarf with subclass and metallicity, and a catalog of A type star with MK classification. A part of the pilot survey data, including about 319 000 high quality spectra with SNR > 10, a catalog of stellar parameters of FGK stars and another catalog of a subclass of M type stars have been released to the public in August 2012 (Luo et al. 2012). The general survey started from October 2012, and completed the first year survey. The formal data release one (DR1) is being prepared, which will include both pilot survey and first year general survey, and planed to be released under the LAMOST data policy.

Clinical audit training improves undergraduates' performance in root canal therapy.

PubMed

Fong, J Y M; Tan, V J H; Lee, J R; Tong, Z G M; Foong, Y K; Tan, J M E; Parolia, A; Pau, A

2017-12-20

To evaluate the effectiveness of clinical audit-feedback cycle as an educational tool in improving the technical quality of root canal therapy (RCT) and compliance with record keeping performed by dental undergraduates. Clinical audit learning was introduced in Year 3 of a 5-year curriculum for dental undergraduates. During classroom activities, students were briefed on clinical audit, selected their audit topics in groups of 5 or 6 students, and prepared and presented their audit protocols. One chosen topic was RCT, in which 3 different cohorts of Year 3 students conducted retrospective audits of patients' records in 2012, 2014 and 2015 for their compliance with recommended record keeping criteria and their performance in RCT. Students were trained by and calibrated against an endodontist (κ ≥ 0.8). After each audit, the findings were reported in class, and recommendations were made for improvement in performance of RCT and record keeping. Students' compliance with published guidelines was presented and their RCT performances in each year were compared using the chi-square test. Overall compliance with of record keeping guidelines was 44.1% in 2012, 79.6% in 2014 and 94.6% in 2015 (P = .001). In the 2012 audit, acceptable extension, condensation and the absence of mishap were observed in 72.4, 75.7% and 91.5%; in the 2014 audit, 95.1%, 64.8% and 51.4%; and in 2015 audit, 96.4%, 82.1% and 92.8% of cases, respectively. In 2015, 76.8% of root canal fillings met all 3 technical quality criteria when compared to 48.6% in 2014 and 44.7% in 2012 (P = .001). Clinical audit-feedback cycle is an effective educational tool for improving dental undergraduates' compliance with record keeping and performance in the technical quality of RCT. © 2017 John Wiley & Sons A/S. Published by John Wiley & Sons Ltd.

VizieR Online Data Catalog: Differential photometry of the F-subgiant HAT-P-67 (Zhou+, 2017)

NASA Astrophysics Data System (ADS)

Zhou, G.; Bakos, G. A.; Hartman, J. D.; Latham, D. W.; Torres, G.; Bhatti, W.; Penev, K.; Buchhave, L.; Kovacs, G.; Bieryla, A.; Quinn, S.; Isaacson, H.; Fulton, B. J.; Falco, E.; Csubry, Z.; Everett, M.; Szklenar, T.; Esquerdo, G.; Berlind, P.; Calkins, M. L.; Beky, B.; Knox, R. P.; Hinz, P.; Horch, E. P.; Hirsch, L.; Howell, S. B.; Noyes, R. W.; Marcy, G.; de Val-Borro, M.; Lazar, J.; Papp, I.; Sari, P.

2018-04-01

The transits of HAT-P-67b were first detected with the HATNet survey (Bakos et al. 2004PASP..116..266B). HATNet employs a network of small, wide field telescopes, located at the Fred Lawrence Whipple Observatory (FLWO) in Arizona and at the Mauna Kea Observatory (MKO) in Hawaii, to photometrically monitor selected 8x8° fields of the sky. A total of 4050 I band observations were taken by HAT-5 and HAT-8 from 2005 January to July, and an additional 4518 observations were obtained in the Cousins R band using HAT-5, HAT-7, and HAT-8 telescopes between 2008 February and August. To better characterize the planetary properties, follow-up photometry of the transits were obtained using the KeplerCam on the FWLO 1.2 m telescope. KeplerCam is a 4Kx4K CCD camera with a pixel scale of 0.672"/pixel at 2x2 pixel binning. The photometry was reduced as per Bakos et al. (2010, J/ApJ/710/1724). A full transit was observed in the Sloan-i band on 2012 May 28, and five partial transits were observed on 2011 April 15, May 19, June 07, and 2013 April 25 in the Sloan-i band, and 2013 May 24 in the Sloan-z band. (1 data file).

Thickness and Lower Limit Seismogenic Layer within the Crust beneath Japanese Islands on the Japan Sea Side

NASA Astrophysics Data System (ADS)

Matsubara, M.; Sato, H.

2015-12-01

1. Introduction I investigate the depth of the seismogenic layer in order to estimate the lower limit of the seismogenic fault plane since this depth is related to the size of the earthquake caused by the active fault. I have indexes D10 and D90 as the upper and lower limits of the seismogenic layer defined as the depth above which 10 % and 90 % of the whole crustal earthquakes occurred from the surface, respectively. The difference between the D10 and D90 is the thickness of the seismogenic layer. 2. Data and method The NIED Hi-net has a catalog of hypocenters determined with one-dimensional　velocity (1D) structure (Ukawa et al., 1984) and I estimated the D10 and D90 with this catalog at first. I construct the system to relocate the hypocenters from 2001 to 2013 with magnitude greater than 1.5 on the Japan Sea side shallower than 50 km depth with the three-dimensional velocity (3D) structure (Matsubara and Obara, 2011) obtained by seismic tomography. I estimate the D10 and D90 from the hypocenter catalog with 3D structure. 3. Result Many earthquakes shallower than 5 km with 1D structure are relocated to deeper with 3D structure and the earthquakes deeper than 15 km are relocated to about 5 km shallower. With 3D structure D10 deepens and D90 shallows from 1D structure. D90 beneath the northern Honshu is deeper than the other area and D90 beneath the Japan Sea is much deeper than the inland area. The thickness of the seismogenic layer beneath the Japan Sea is also thick from 8-16 km. D90 on the Japan Sea side of the southwestern Japan on the west side of the Itoigawa Shizuoka Tectonic Line is very shallow as 11-16 km and the thickness of the seismogenic layer is also thin as 2-7 km. 4. Discussion Omuralieva et al. (2012) relocated the JMA unified hypocenters with 3D structure and estimated shallower D90 than that from the JMA catalog. Very deep D90 beneath the northern Hokkaido and northern Honshu is consistent with our result. 5. Conclusion Using 3D velocity structure D10 deepens, D90 shallows, and the thickness of the seismogenic layer becomes thinner. The thickness of the seismogenic layer is thick beneath the northern Honshu, however, that is very thin beneath southwestern Japan on the Japan Sea side.

Factors affecting the number and type of student research products for chemistry and physics students at primarily undergraduate institutions: A case study.

PubMed

Mellis, Birgit; Soto, Patricia; Bruce, Chrystal D; Lacueva, Graciela; Wilson, Anne M; Jayasekare, Rasitha

2018-01-01

For undergraduate students, involvement in authentic research represents scholarship that is consistent with disciplinary quality standards and provides an integrative learning experience. In conjunction with performing research, the communication of the results via presentations or publications is a measure of the level of scientific engagement. The empirical study presented here uses generalized linear mixed models with hierarchical bootstrapping to examine the factors that impact the means of dissemination of undergraduate research results. Focusing on the research experiences in physics and chemistry of undergraduates at four Primarily Undergraduate Institutions (PUIs) from 2004-2013, statistical analysis indicates that the gender of the student does not impact the number and type of research products. However, in chemistry, the rank of the faculty advisor and the venue of the presentation do impact the number of research products by undergraduate student, whereas in physics, gender match between student and advisor has an effect on the number of undergraduate research products. This study provides a baseline for future studies of discipline-based bibliometrics and factors that affect the number of research products of undergraduate students.

Factors affecting the number and type of student research products for chemistry and physics students at primarily undergraduate institutions: A case study

PubMed Central

Soto, Patricia; Bruce, Chrystal D.; Lacueva, Graciela; Wilson, Anne M.; Jayasekare, Rasitha

2018-01-01

For undergraduate students, involvement in authentic research represents scholarship that is consistent with disciplinary quality standards and provides an integrative learning experience. In conjunction with performing research, the communication of the results via presentations or publications is a measure of the level of scientific engagement. The empirical study presented here uses generalized linear mixed models with hierarchical bootstrapping to examine the factors that impact the means of dissemination of undergraduate research results. Focusing on the research experiences in physics and chemistry of undergraduates at four Primarily Undergraduate Institutions (PUIs) from 2004–2013, statistical analysis indicates that the gender of the student does not impact the number and type of research products. However, in chemistry, the rank of the faculty advisor and the venue of the presentation do impact the number of research products by undergraduate student, whereas in physics, gender match between student and advisor has an effect on the number of undergraduate research products. This study provides a baseline for future studies of discipline-based bibliometrics and factors that affect the number of research products of undergraduate students. PMID:29698502

Examining seismicity patterns in the 2010 M 8.8 Maule rupture zone.

NASA Astrophysics Data System (ADS)

Diniakos, R. S.; Bilek, S. L.; Rowe, C. A.; Draganov, D.

2016-12-01

The subduction of the Nazca Plate beneath the South American Plate along Chile has produced some of the largest earthquakes recorded on modern seismic instrumentation. These include the 1960 M 9.5 Valdivia, 2010 M 8.8 Maule, 2014 M 8.1 Iquique, and more recently the 2015 M 8.3 Illapel earthquakes. Slip heterogeneity in the 2010 Maule earthquake has been noted in various studies, with bilateral slip and peak slip of 15 m north of the epicenter. For other great subduction zone earthquakes, such as the 2004 M 9.1 Sumatra, 2010 M 8.8 Maule, and 2011 M 9.0 Tohoku, there was an increase in normal-faulting earthquakes in regions of high slip. In order to understand aftershock behavior of the 2010 Maule event, we are expanding the catalog of small magnitude earthquakes using a template-matching algorithm to find other small earthquakes in the rupture area. We use a starting earthquake catalog (magnitudes between 2.5-4.0) developed from regional and local array seismic data; these comprise our template catalog from Jan. - Dec. 2012 that we use to search through seismic waveforms recorded by a 2012 temporary seismic array in Malargüe, Argentina located 300 km east of the Maule rupture area. We use waveform cross correlation techniques in order to detect new events, and then we use HYPOINVERSE2000 (Klein, 2002) and a velocity model designed for the south-central Chilean region (Haberland et al., 2006) to locate new detections. We also determine focal mechanisms to further analyze aftershock behavior for the region. To date, over 2400 unique detections have been found, of which we have located 133 events with an RMS <1. Many of these events are located in the region of greatest coseismic slip, north of the 2010 epicenter, whereas catalog events are located north and south of the epicenter, along the regions of bilateral slip. Focal mechanisms for the new locations will also be presented.

A Fresh Look at Student Engagement. Annual Results 2013

ERIC Educational Resources Information Center

National Survey of Student Engagement, 2013

2013-01-01

The National Survey of Student Engagement (NSSE), launched in 2000 and updated in 2013, documents dimensions of quality in undergraduate education and provides information and assistance to colleges, universities, and other organizations to improve student learning. Its primary activity is annually surveying college students to assess the extent…

"I Don't Want to Grow Up, I'm a [Gen X, Y, Me] Kid": Increasing Maturity Fears across the Decades

ERIC Educational Resources Information Center

Smith, April; Bodell, Lindsay P.; Holm-Denoma, Jill; Joiner, Thomas; Gordon, Kathryn; Perez, Marisol; Keel, Pamela

2017-01-01

The current studies examined the hypothesis that maturity fears are increasing among undergraduate men and women from the United States over time. Study 1 used a time-lag method to assess generational effects of maturity fears among a large sample (n = 3291) of undergraduate men and women assessed in 1982, 1992, 2002, and 2012. Results revealed…

A Profile of the Enrollment Patterns and Demographic Characteristics of Undergraduates at For-Profit Institutions. Stats in Brief. NCES 2017-416

ERIC Educational Resources Information Center

Arbeit, Caren A.; Horn, Laura

2017-01-01

In 2012, more than 13 percent of undergraduates attended for-profit postsecondary institutions, up from 9 percent in 2009. The rapid growth of the for-profit sector has renewed public scrutiny and concern about the historically poor labor market outcomes of students at many of these institutions and the amount of debt students in these…

77 FR 11505 - Applications for New Awards; Training and Information for Parents of Children With Disabilities

Federal Register 2010, 2011, 2012, 2013, 2014

2012-02-27

... activities under section 663 of IDEA and the Department's Institute of Education Sciences, and with other... DEPARTMENT OF EDUCATION Applications for New Awards; Training and Information for Parents of... Disabilities. Notice inviting applications for new awards for fiscal year (FY) 2012. Catalog of Federal...

77 FR 36501 - Applications for New Awards: Technical Assistance and Dissemination To Improve Services and...

Federal Register 2010, 2011, 2012, 2013, 2014

2012-06-19

... outcome data for program improvement; and meeting new requirements in the IDEA Part C regulations issued... DEPARTMENT OF EDUCATION Applications for New Awards: Technical Assistance and Dissemination To... applications for new awards for fiscal year (FY) 2012. Catalog of Federal Domestic Assistance (CFDA) Number: 84...

77 FR 37915 - Kansas; Major Disaster Declaration and Related Determinations

Federal Register 2010, 2011, 2012, 2013, 2014

2012-06-25

... to apply for assistance under the Hazard Mitigation Grant Program. The following Catalog of Federal... Presidential declaration of a major disaster for the State of Kansas (FEMA-4063-DR), dated May 24, 2012, and... have determined that the damage in certain areas of the State of Kansas resulting from severe storms...

VizieR Online Data Catalog: Infrared excesses of Hipparcos stars (McDonald+, 2012)

NASA Astrophysics Data System (ADS)

McDonald, I.; Zijlstra, A. A.; Boyer, M. L.

2013-08-01

The new Hipparcos (Hp)/Tycho (BT, VT) reduction (van Leeuwen 2007. Cat. I/311) was used as the primary astrometric and photometric catalogue, to which the other catalogues were matched. Additional data were sourced from SDSS DR8, DENIS, 2MASS, MSX, AKARI, IRAS and Wide surveys. (1 data file).

VizieR Online Data Catalog: NGC 225 CCD UBV photometry (Bilir+, 2016)

NASA Astrophysics Data System (ADS)

Bilir, S.; Bostanci, Z. F.; Yontan, T.; Guver, T.; Bakis, V.; Ak, T.; Ak, S.; Paunzen, E.; Eker, Z.

2016-11-01

CCD UBVRI images of the open cluster NGC 225 and standard stars selected from Landolt (2009, Cat. J/AJ/137/4186) were acquired on 2012 July 18 using a 1-m Ritchey-Chretien telescope (T100) located at the TUBITAK National Observatory (TUG) in Bakirlitepe, Antalya/Turkey. (1 data file).

77 FR 41190 - Office of Clinical and Preventive Services Funding Opportunity: National HIV Program for Enhanced...

Federal Register 2010, 2011, 2012, 2013, 2014

2012-07-12

... DEPARTMENT OF HEALTH AND HUMAN SERVICES Indian Health Service Office of Clinical and Preventive Services Funding Opportunity: National HIV Program for Enhanced HIV/AIDS Screening and Engagement in Care... Announcement Number: HHS-2012-IHS-OCPS-HIV-0001. Catalog of Federal Domestic Assistance Number: 93.933. The...

VizieR Online Data Catalog: New gamma-ray blazar candidates in the 3PBC (Maselli+, 2013)

NASA Astrophysics Data System (ADS)

Maselli, A.; Massaro, F.; Cusumano, G.; D'Abrusco, R.; La Parola, V.; Paggi, A.; Segreto, A.; Smith, H. A.; Tosti, G.

2013-06-01

We searched for γ-ray blazar candidates among the 382 unidentified hard X-ray sources of the third Palermo BAT Catalog (3PBC) obtained from the analysis of 66 months of Swift Burst Alert Telescope (BAT) survey data and listing 1586 sources. We adopted a recently developed association method based on the peculiar infrared colors that characterize the γ-ray blazars included in the second catalog of active galactic nuclei detected by the Fermi Large Area Telescope. We used this method exploiting the data of the all-sky survey performed by the Wide-field Infrared Survey Explorer (WISE) to establish correspondences between unidentified 3PBC sources and WISE γ-ray blazar candidates located within the BAT positional uncertainty region at a 99% confidence level. We obtained a preliminary list of candidates for which we analyzed all the available data in the Swift archive to complement the information in the literature and in the radio, infrared, and optical catalogs with the information on their optical-UV and soft X-ray emission. Requiring the presence of radio and soft X-ray counterparts consistent with the infrared positions of the selected WISE sources, as well as a blazar-like radio morphology, we finally obtained a list of 24 γ-ray blazar candidates. (2 data files).

VizieR Online Data Catalog: UV and optical photometric data for SN 2013by (Valenti+, 2015)

NASA Astrophysics Data System (ADS)

Valenti, S.; Sand, D.; Stritzinger, M.; Howell, D. A.; Arcavi, I.; McCully, C.; Childress, M. J.; Hsiao, E. Y.; Contreras, C.; Morrell, N.; Phillips, M. M.; Gromadzki, M.; Kirshner, R. P.; Marion, G. H.

2017-11-01

Photometric monitoring in BVgri of SN 2013by with the LCOGT 1 m telescope network began on 2013 April 24 (UT), and continued every two to three nights (52 epochs of data were collected) for more than 150 d, well after the light curve settled on to the 56Co decay tail. Additional imaging was obtained from Swift and the CSP. The CSP obtained 17 epochs of science images using the SITe3 CCD camera along with a set of ugriBV filters attached to the Swope 1 m telescope located at Las Campanas Observatory (LCO). (1 data file).

VizieR Online Data Catalog: MOJAVE. XIII. New 15GHz observations on 1994-2013 (Lister+, 2016)

NASA Astrophysics Data System (ADS)

Lister, M. L.; Aller, M. F.; Aller, H. D.; Homan, D. C.; Kellermann, K. I.; Kovalev, Y. Y.; Pushkarev, A. B.; Richards, J. L.; Ros, E.; Savolainen, T.

2016-09-01

Starting with the 2cm Very Long Baseline Array (VLBA) survey in 1994 (Kellermann et al. 1998AJ....115.1295K), and continuing with the MOJAVE (Monitoring of Jets in Active Galactic Nuclei with VLBA Experiments) program (Lister et al. 2009, Cat. J/AJ/137/3718), we have carried out multi-epoch VLBA observations of several hundred of the brightest, most compact radio sources in the northern sky. In this paper, we present 1625 VLBA 15GHz contour maps of 295 AGNs for epochs between 1994 August 31 and 2013 August 20 that have not previously appeared in any paper from the MOJAVE (Lister & Homan 2005, Cat. J/AJ/130/1389; Lister et al. 2009, Cat. J/AJ/137/3718; Lister et al. 2013, Cat. J/AJ/146/120) or 2cm VLBA surveys (Kellermann et al. 1998AJ....115.1295K; Zensus et al. 2002AJ....124..662Z). These AGNs (see Table1) are from one or more of the following: the MOJAVE low-luminosity sample (Lister et al. 2013, Cat. J/AJ/146/120), the complete flux density-limited MOJAVE 1.5Jy sample (Lister et al. 2015, Cat. J/ApJ/810/L9), the VLBA 2cm survey (Kellermann et al. 1998AJ....115.1295K), the third EGRET gamma-ray catalog (Hartman et al. 1999, Cat. J/ApJS/123/79), or the 3FGL Fermi gamma-ray catalog (Acero et al. 2015, Cat. J/ApJS/218/23). Also included are some AGNs that were originally candidates for these samples, but did not meet the final selection criteria. We list the parameters of the contour maps in Table2. We modeled the (u, v) visibility data in Difmap (Shepherd 1997ASPC..125...77S) using a set of Gaussian features, which we list in Table3. We analyzed the kinematics of the robust Gaussian jet features in our sample using two methods. The results of these analyses are listed separately in Tables 4 and 5, respectively. (6 data files).

VizieR Online Data Catalog: SAMI Galaxy Survey: rotators classification (van de Sande+, 2017)

NASA Astrophysics Data System (ADS)

van de Sande, J.; Bland-Hawthorn, J.; Fogarty, L. M. R.; Cortese, L.; D'Eugenio, F.; Croom, S. M.; Scott, N.; Allen, J. T.; Brough, S.; Bryant, J. J.; Cecil, G.; Colless, M.; Couch, W. J.; Davies, R.; Elahi, P. J.; Foster, C.; Goldstein, G.; Goodwin, M.; Groves, B.; Ho, I.-T.; Jeong, H.; Jones, D. H.; Konstantopoulos, I. S.; Lawrence, J. S.; Leslie, S. K.; Lopez-Sanchez, A. R.; McDermid, R. M.; McElroy, R.; Medling, A. M.; Oh, S.; Owers, M. S.; Richards, S. N.; Schaefer, A. L.; Sharp, R.; Sweet, S. M.; Taranu, D.; Tonini, C.; Walcher, C. J.; Yi, S. K.

2017-08-01

The SAMI instrument and Galaxy Survey is described in detail in Croom+ (2012MNRAS.421..872C) and Bryant+ (2015MNRAS.447.2857B). SAMI is a multi-object integral field spectrograph on the 3.9m Anglo Australian Telescope (AAT). For the SAMI Galaxy Survey, the 580V grating is used in the blue arm of the spectrograph, which results in a resolution of R~1700 with wavelength coverage of 3700-5700Å. In the red arm, the higher resolution grating 1000R is used, which gives an R~4500 over the range 6300-7400Å. We use 24 unsaturated, unblended CuAr arc lines in the blue arm, and 12 lines in the red arm, from 16 frames between 2013 March 05 and 2015 August 17, for all 819 fibers. The survey has four volume-limited galaxy samples derived from cuts in stellar mass in the Galaxy and Mass Assembly (GAMA) G09, G12, and G15 regions (Driver+ 2011, J/MNRAS/413/971). (2 data files).

VizieR Online Data Catalog: XMM-Newton point-source catalogue of the SMC (Sturm+, 2013)

NASA Astrophysics Data System (ADS)

Sturm, R.; Haberl, F.; Pietsch, W.; Ballet, J.; Hatzidimitriou, D.; Buckley, D. A. H.; Coe, M.; Ehle, M.; Filipovic, M. D.; La Palombara, N.; Tiengo, A.

2013-07-01

The XMM-Newton survey of the Small Magellanic Cloud (SMC) yields a complete coverage of the bar and eastern wing in the 0.2-12.0keV band. This catalogue comprises 3053 unique X-ray point sources and sources with moderate extent that have been reduced from 5236 individual detections found in observations between April 2000 and April 2010. Sources have a median position uncertainty of 1.3" (1σ) and limiting fluxes down to ~1*10-14erg/s/cm2 in the 0.2-4.5keV band, corresponding to 5*1033erg/s for sources in the SMC. Sources have been classified using hardness ratios, X-ray variability, and their multi-wavelength properties. In addition to the main-field (5.58deg2) available outer fields have been included in the catalogue, yielding a total field area of 6.32deg2. X-ray sources with high extent (>40", e.g. supernova remnants and galaxy cluster) have been presented by Haberl et al. (2012, Cat. J/A+A/545/A128) (2 data files).

VizieR Online Data Catalog: Main-sequence A, F, G, and K stars photometry (Boyajian+, 2013)

NASA Astrophysics Data System (ADS)

Boyajian, T. S.; von Braun, K.; van Belle, G.; Farrington, C.; Schaefer, G.; Jones, J.; White, R.; McAlister, H. A.; Ten Brummelaar, T. A.; Ridgway, S.; Gies, D.; Sturmann, L.; Sturmann, J.; Turner, N. H.; Goldfinger, P. J.; Vargas, N.

2016-07-01

Akin to the observing outlined in DT1 and DT2, observations for this project were made with the CHARA Array, a long-baseline optical/infrared interferometer located on Mount Wilson Observatory in southern California. The target stars were selected based on their approximate angular size (a function of their intrinsic linear size and distance to the observer). We limit the selection to stars with angular sizes >0.45mas, in order to adequately resolve their sizes to a few percent precision with the selected instrument setup. Note that all stars that meet this requirement are brighter than the instrumental limits of our detector by several magnitudes. The stars also have no known stellar companion within 3-arcsec to avoid contamination of incoherent light in the interferometers' field of view. From 2008 to 2012, we used the CHARA Classic beam combiner operating in the H band (λH=1.67um) and the K' band (λK'=2.14um) to collect observations of 23 stars using CHARA's longest baseline combinations. (5 data files).

VizieR Online Data Catalog: NuSTAR hard X-ray survey of the Galactic Center. II. (Hong+, 2016)

NASA Astrophysics Data System (ADS)

Hong, J.; Mori, K.; Hailey, C. J.; Nynka, M.; Zhang, S.; Gotthelf, E.; Fornasini, F. M.; Krivonos, R.; Bauer, F.; Perez, K.; Tomsick, J. A.; Bodaghee, A.; Chiu, J.-L.; Clavel, M.; Stern, D.; Grindlay, J. E.; Alexander, D. M.; Aramaki, T.; Baganoff, F. K.; Barret, D.; Barriere, N.; Boggs, S. E.; Canipe, A. M.; Christensen, F. E.; Craig, W. W.; Desai, M. A.; Forster, K.; Giommi, P.; Grefenstette, B. W.; Harrison, F. A.; Hong, D.; Hornstrup, A.; Kitaguchi, T.; Koglin, J. E.; Madsen, K. K.; Mao, P. H.; Miyasaka, H.; Perri, M.; Pivovaroff, M. J.; Puccetti, S.; Rana, V.; Westergaard, N. J.; Zhang, W. W.; Zoglauer, A.

2018-02-01

Observations of the GC region with NuSTAR began in 2012 July, shortly after launch. The original survey strategy for the GC region was to match the central 2°x0.7° region covered by the Chandra X-ray Observatory (Wang et al. 2002Natur.415..148W; Muno et al. 2009, J/ApJS/181/110). The field of views (FOVs) of neighboring NuSTAR observations in the survey were designed to overlap with each other by ~40%. Multiple observations of the same region with relatively large FOV offsets tend to average out the vignetting effects of each observation, enabling a more uniform coverage of the region. Multiple observations are also suitable for monitoring long term X-ray variability of sources in the region. Even when observing a single target, the NuSTAR observation is often broken up into two or more segments with relatively large pointing offsets to allow an efficient subtraction of a detector coordinate-dependent background component (e.g., Mori et al. 2013ApJ...770L..23M). (4 data files).

VizieR Online Data Catalog: Minima of 41 binaries from entire Kepler mission (Gies+, 2015)

NASA Astrophysics Data System (ADS)

Gies, D. R.; Matson, R. A.; Guo, Z.; Lester, K. V.; Orosz, J. A.; Peters, G. J.

2016-06-01

We embarked on a search for eclipse timing variations among a subset of 41 eclipsing binaries that were identified prior to the start of Kepler observations (see our first paper, Gies et al. 2012, cat. J/AJ/143/137). Our first paper documented the eclipse times in observations made over quarters Q0-Q9 (2009.3-2011.5). Now with the Kepler mission complete with observations through Q17 (ending 2013.4), we present here the eclipse timings for our sample of 41 binaries over the entire duration of the mission. The associated times given in our first paper were based upon UTC (Coordinated Universal Time) while the current set uses TDB (Barycentric Dynamical Time), and here we report the times in reduced Barycentric Julian Date (BJD-2400000 days). We used the Simple Aperture Photometry (SAP) flux except in the case of KIC04678873. The list of targets appears in Table1. The eclipse timing measurements were made in almost the same way as described in our first paper. Our measurements appear in Table2. (2 data files).

Characterizing radio continuum sources in a sample of Hi-GAL massive cores

NASA Astrophysics Data System (ADS)

Armstrong, Jason

In 2012 and 2013, Olmi and collaborators conducted a survey for 6.7GHz methanol masers with the Arecibo Telescope toward far infrared sources selected from the Hi-GAL catalog of massive cores. They reported a number of sources with weak 6.7GHz methanol masers, possibly indicating regions in early stages of star formation. Follow-up observations were conducted with the Karl G. Jansky Very Large Array (VLA) in New Mexico to characterize the sources. This thesis presents the results of radio continuum observations of nine of the Arecibo regions. A total of 33 radio continuum sources were detected. The nature of the radio continuum sources was analyzed based on their spectral indices. Most of the sources have negative spectral indices, which is indicative of synchrotron radiation. Many of the synchrotron sources are associated with a supernova remnant in our Galaxy, while the rest are likely background radio galaxies and quasars. Evidence for thermal bremsstrahlung radiation was found toward six sources associated with the Arecibo regions, which is consistent with the interpretation of gas ionized by young high-mass stellar objects.

VizieR Online Data Catalog: WISE W1/W2 Tully-Fisher relation calibrator data (Neill+, 2014)

NASA Astrophysics Data System (ADS)

Neill, J. D.; Seibert, M.; Tully, R. B.; Courtois, H.; Sorce, J. G.; Jarrett, T. H.; Scowcroft, V.; Masci, F. J.

2017-04-01

We have instigated a separate project to provide high-quality surface photometry of all WISE galaxies larger than 0.8' on the sky. The WISE Nearby Galaxy Atlas (WNGA; M. Seibert et al., in preparation) will provide photometry that is quality controlled for over 20000 galaxies. This photometry, optimized for extended sources, significantly reduces the resulting scatter in the Tully-Fisher relation (here after TFR) calibration and thus improves the resulting distances. Having an accurate calibration of the TFR for these two WISE passbands will allow the use of this large sample to explore the structure and dynamics of local galaxy bulk flows. With the current tally, there are 310 cluster calibrators with WISE W1 and W2 photometry, compared with 213 available to Sorce et al. (2013, J/ApJ/765/94) for the Spitzer calibration, and 291 of the 310 WISE calibrators have I-band photometry, compared with the 267 available to Tully & Courtois (2012ApJ...749...78T) for the previous I-band calibration. (1 data file).

Undergraduate teaching on biological weapons and bioterrorism at medical schools in the UK and the Republic of Ireland: results of a cross-sectional study.

PubMed

Green, Stephen T; Cladi, Lorenzo; Morris, Paul; Forde, Donall

2013-06-20

To determine if individual undergraduate schools of medicine in the UK and the Republic of Ireland provide any teaching to medical students about biological weapons, bioterrorism, chemical weapons and weaponised radiation, if they perceive them to be relevant issues and if they figure them in their future plans. A cross-sectional study utilising an internet-based questionnaire sent to key figures responsible for leading on the planning and delivery of undergraduate medical teaching at all schools of medicine in the UK and Ireland. All identified undergraduate schools of medicine in the UK and Ireland between August 2012 and December 2012. Numerical data and free text feedback about relevant aspects of undergraduate teaching. Of the 38 medical schools approached, 34 (28 in UK, 6 in Ireland) completed the questionnaire (89.47%). 4 (all in UK) chose not to complete it. 6/34 (17.65%) included some specific teaching on biological weapons and bioterrorism. 7/34 (20.59%) had staff with bioterrorism expertise (mainly in microbiological and syndromic aspects). 4/34 (11.76%) had plans to introduce some specific teaching on bioterrorism. Free text responses revealed that some felt that because key bodies (eg, UK's General Medical Council) did not request teaching on bioterrorism, then it should not be included, while others regarded this field of study as a postgraduate subject and not appropriate for undergraduates, or argued that the curriculum was too congested already. 4/34 (11.76%) included some specific teaching on chemical weapons, and 3/34 (8.82%) on weaponised radiation. This study provides evidence that at the present time there is little teaching at the undergraduate level in the UK and Ireland on the subjects of biological weapons and bioterrorism, chemical weapons and weaponised radiation and signals that this situation is unlikely to change unless there were to be high-level policy guidance.

Undergraduate teaching on biological weapons and bioterrorism at medical schools in the UK and the Republic of Ireland: results of a cross-sectional study

PubMed Central

Green, Stephen T; Cladi, Lorenzo; Morris, Paul; Forde, Donall

2013-01-01

Objective To determine if individual undergraduate schools of medicine in the UK and the Republic of Ireland provide any teaching to medical students about biological weapons, bioterrorism, chemical weapons and weaponised radiation, if they perceive them to be relevant issues and if they figure them in their future plans. Design A cross-sectional study utilising an internet-based questionnaire sent to key figures responsible for leading on the planning and delivery of undergraduate medical teaching at all schools of medicine in the UK and Ireland. Setting All identified undergraduate schools of medicine in the UK and Ireland between August 2012 and December 2012. Outcome measures Numerical data and free text feedback about relevant aspects of undergraduate teaching. Results Of the 38 medical schools approached, 34 (28 in UK, 6 in Ireland) completed the questionnaire (89.47%). 4 (all in UK) chose not to complete it. 6/34 (17.65%) included some specific teaching on biological weapons and bioterrorism. 7/34 (20.59%) had staff with bioterrorism expertise (mainly in microbiological and syndromic aspects). 4/34 (11.76%) had plans to introduce some specific teaching on bioterrorism. Free text responses revealed that some felt that because key bodies (eg, UK's General Medical Council) did not request teaching on bioterrorism, then it should not be included, while others regarded this field of study as a postgraduate subject and not appropriate for undergraduates, or argued that the curriculum was too congested already. 4/34 (11.76%) included some specific teaching on chemical weapons, and 3/34 (8.82%) on weaponised radiation. Conclusions This study provides evidence that at the present time there is little teaching at the undergraduate level in the UK and Ireland on the subjects of biological weapons and bioterrorism, chemical weapons and weaponised radiation and signals that this situation is unlikely to change unless there were to be high-level policy guidance. PMID:23794539

Engineering Students at Typically Invisible Transition Points: A Focus on Admissions and the Sophomore Year

ERIC Educational Resources Information Center

Holloway, Elizabeth M.

2013-01-01

As of 2012, women are approximately 19% of all engineering undergraduate students nationally (American Society for Engineering Education, 2012). Women's representation in engineering has not changed significantly over the last 20 years, despite increased attention, increased funding, and increased programmatic activities intended to encourage more…

34 CFR 648.61 - How must the academic department supervise the training of fellows?

Code of Federal Regulations, 2012 CFR

2012-07-01

... 34 Education 3 2012-07-01 2012-07-01 false How must the academic department supervise the training... academic department supervise the training of fellows? The institution shall provide to fellows at least one academic year of supervised training in instruction at the graduate or undergraduate level at the...

Evaluating the Use of Declustering for Induced Seismicity Hazard Assessment

NASA Astrophysics Data System (ADS)

Llenos, A. L.; Michael, A. J.

2016-12-01

The recent dramatic seismicity rate increase in the central and eastern US (CEUS) has motivated the development of seismic hazard assessments for induced seismicity (e.g., Petersen et al., 2016). Standard probabilistic seismic hazard assessment (PSHA) relies fundamentally on the assumption that seismicity is Poissonian (Cornell, BSSA, 1968); therefore, the earthquake catalogs used in PSHA are typically declustered (e.g., Petersen et al., 2014) even though this may remove earthquakes that may cause damage or concern (Petersen et al., 2015; 2016). In some induced earthquake sequences in the CEUS, the standard declustering can remove up to 90% of the sequence, reducing the estimated seismicity rate by a factor of 10 compared to estimates from the complete catalog. In tectonic regions the reduction is often only about a factor of 2. We investigate how three declustering methods treat induced seismicity: the window-based Gardner-Knopoff (GK) algorithm, often used for PSHA (Gardner and Knopoff, BSSA, 1974); the link-based Reasenberg algorithm (Reasenberg, JGR,1985); and a stochastic declustering method based on a space-time Epidemic-Type Aftershock Sequence model (Ogata, JASA, 1988; Zhuang et al., JASA, 2002). We apply these methods to three catalogs that likely contain some induced seismicity. For the Guy-Greenbrier, AR earthquake swarm from 2010-2013, declustering reduces the seismicity rate by factors of 6-14, depending on the algorithm. In northern Oklahoma and southern Kansas from 2010-2015, the reduction varies from factors of 1.5-20. In the Salton Trough of southern California from 1975-2013, the rate is reduced by factors of 3-20. Stochastic declustering tends to remove the most events, followed by the GK method, while the Reasenberg method removes the fewest. Given that declustering and choice of algorithm have such a large impact on the resulting seismicity rate estimates, we suggest that more accurate hazard assessments may be found using the complete catalog.

Space-Time Earthquake Rate Models for One-Year Hazard Forecasts in Oklahoma

NASA Astrophysics Data System (ADS)

Llenos, A. L.; Michael, A. J.

2017-12-01

The recent one-year seismic hazard assessments for natural and induced seismicity in the central and eastern US (CEUS) (Petersen et al., 2016, 2017) rely on earthquake rate models based on declustered catalogs (i.e., catalogs with foreshocks and aftershocks removed), as is common practice in probabilistic seismic hazard analysis. However, standard declustering can remove over 90% of some induced sequences in the CEUS. Some of these earthquakes may still be capable of causing damage or concern (Petersen et al., 2015, 2016). The choices of whether and how to decluster can lead to seismicity rate estimates that vary by up to factors of 10-20 (Llenos and Michael, AGU, 2016). Therefore, in order to improve the accuracy of hazard assessments, we are exploring ways to make forecasts based on full, rather than declustered, catalogs. We focus on Oklahoma, where earthquake rates began increasing in late 2009 mainly in central Oklahoma and ramped up substantially in 2013 with the expansion of seismicity into northern Oklahoma and southern Kansas. We develop earthquake rate models using the space-time Epidemic-Type Aftershock Sequence (ETAS) model (Ogata, JASA, 1988; Ogata, AISM, 1998; Zhuang et al., JASA, 2002), which characterizes both the background seismicity rate as well as aftershock triggering. We examine changes in the model parameters over time, focusing particularly on background rate, which reflects earthquakes that are triggered by external driving forces such as fluid injection rather than other earthquakes. After the model parameters are fit to the seismicity data from a given year, forecasts of the full catalog for the following year can then be made using a suite of 100,000 ETAS model simulations based on those parameters. To evaluate this approach, we develop pseudo-prospective yearly forecasts for Oklahoma from 2013-2016 and compare them with the observations using standard Collaboratory for the Study of Earthquake Predictability tests for consistency.

77 FR 76569 - Sunshine Act Meetings

Federal Register 2010, 2011, 2012, 2013, 2014

2012-12-28

... Regulatory Commission [NRC-2012- 0002]. DATE: Weeks of December 24, 31, 2012, January 7, 14, 21, 28, 2013... Closed. Week of December 24, 2012 There are no meetings scheduled for the week of December 24, 2012. Week.... Week of January 7, 2013--Tentative Tuesday, January 8, 2013 9:00 a.m. Briefing on Fort Calhoun (Public...

2012-2013 Delaware Valley Household Travel Survey | Transportation Secure

Science.gov Websites

Data Center | NREL 12-2013 Delaware Valley Household Travel Survey 2012-2013 Delaware Valley Household Travel Survey The 2012-2013 Delaware Valley Household Travel Survey collected data for multiple ) sponsored the survey in collaboration with AbtSRBI. Methodology A sampling strategy was designed to recruit

78 FR 52759 - Brass Sheet and Strip from Germany: Rescission of Antidumping Duty Administrative Review; 2012-2013

Federal Register 2010, 2011, 2012, 2013, 2014

2013-08-26

... Germany: Rescission of Antidumping Duty Administrative Review; 2012-2013 AGENCY: Import Administration... from Germany for the period March 1, 2012, through February 28, 2013. DATES: Effective Date: August 26... 1, 2013, the Department initiated an administrative review of brass sheet and strip from Germany...

AKARI Infrared Camera Survey of the Large Magellanic Cloud

NASA Astrophysics Data System (ADS)

Shimonishi, Takashi; Kato, Daisuke; Ita, Yoshifusa; Onaka, Takashi

2015-08-01

The Large Magellanic Cloud (LMC) is one of the closest external galaxies to the Milky Way and has been playing a central role in various fields of modern astronomy and astrophysics. We conducted an unbiased near- to mid-infrared imaging and spectroscopic survey of the LMC with the infrared satellite AKARI. An area of about 10 square degrees of the LMC was observed by five imaging bands (each centered at 3.2, 7, 11, 15, and 24 micron) and the low-resolution slitless prism spectroscopy mode (2--5 micron, R~20) equipped with the Infrared Camera on board AKARI. Based on the data obtained in the survey, we constructed the photometric and spectroscopic catalogues of point sources in the LMC. The photometric catalogue includes about 650,000, 90,000, 49,000, 17,000, 7,000 sources at 3.2, 7, 11, 15, and 24 micron, respectively (Ita et al. 2008, PASJ, 60, 435; Kato et al. 2012, AJ, 144, 179), while the spectroscopic catalogue includes 1,757 sources (Shimonishi et al. 2013, AJ, 145, 32). Both catalogs are publicly released and available through a website (AKARI Observers Page, http://www.ir.isas.ac.jp/AKARI/Observation/). The catalog includes various infrared sources such as young stellar objects, asymptotic giant branch stars, giants/supergiants, and many other cool or dust-enshrouded stars. A large number of near-infrared spectral data, coupled with complementary broadband photometric data, allow us to investigate infrared spectral features of sources by comparison with their spectral energy distributions. Combined use of the present AKARI LMC catalogues with other infrared catalogues such as SAGE and HERITAGE possesses scientific potential that can be applied to various astronomical studies. In this presentation, we report the details of the AKARI photometric and spectroscopic catalogues of the LMC.

VizieR Online Data Catalog: New OB star candidates in Carina Arm (Mohr-Smith+, 2015)

NASA Astrophysics Data System (ADS)

Mohr-Smith, M.; Drew, J. E.; Barentsen, G.; Wright, N. J.; Napiwotzki, R.; Corradi, R. L. M.; Eisloffel, J.; Groot, P.; Kalari, V.; Parker, Q. A.; Raddi, R.; Sale, S. E.; Unruh, Y. C.; Vink, J. S.; Wesson, R.

2017-08-01

We make use of the photometry from two VPHAS+ fields, numbered 1678 and 1679, that are, respectively, centred on RA=10:18:10.91, DE=-58:03:52.3 (J2000) and on RA=10:25:27.27, DE=-58:03:52.3 (J2000). These were observed in succession in the u, g and r filters on the night of 2012 January 22. The red filter data in Hα, r and i were obtained on 2012 April 29. (2 data files).

78 FR 32412 - Illinois; Amendment No. 1 to Notice of a Major Disaster Declaration

Federal Register 2010, 2011, 2012, 2013, 2014

2013-05-30

... Island, Schuyler, Stark, Tazewell, and Woodford Counties for Individual Assistance. The following Catalog... Declaration AGENCY: Federal Emergency Management Agency, DHS. ACTION: Notice. SUMMARY: This notice amends the notice of a major disaster declaration for the State of Illinois (FEMA-4116-DR), dated May 10, 2013, and...

Juno: Morse code "HI" received from Earth

NASA Image and Video Library

2017-03-22

During its close flyby of Earth in 2013, NASA's Jupiter-bound Juno spacecraft listened for -- and heard -- a coordinated, global transmission from amateur radio operators using its radio and plasma wave science instrument. The message said "HI" in Morse code. More details about this sound can be found here: photojournal.jpl.nasa.gov/catalog/PIA17744

A Study of Faculty Approaches to Teaching Undergraduate Physical Chemistry Courses

NASA Astrophysics Data System (ADS)

Mack, Michael Ryan

Chemistry education researchers have not adequately studied teaching and learning experiences at all levels in the undergraduate chemistry curriculum leaving gaps in discipline-based STEM education communities understanding about how the upper- division curricula works (National Research Council, 2012b; Towns, 2013). This study explored faculty approaches to teaching in upper-division physical chemistry course settings using an interview-based methodology. Two conceptualizations of approaches to teaching emerged from a phenomenographic analysis of interview transcripts: (1) faculty beliefs about the purposes for teaching physical chemistry and (2) their conceptions of their role as an instructor in these course settings. Faculty who reported beliefs predominantly centered on helping students develop conceptual knowledge and problem-solving skills in physical chemistry often worked with didactic models of teaching, which emphasized the transfer of expert knowledge to students. When faculty expressed beliefs that were more inclusive of conceptual, epistemic, and social learning goals in science education they often described more student-centered models of teaching and learning, which put more responsibilities on them to facilitate students' interactive engagement with the material and peers during regularly scheduled class time. Knowledge of faculty thinking, as evinced in a rich description of their accounts of their experience, provides researchers and professional developers with useful information about the potential opportunities or barriers that exist for helping faculty align their beliefs and goals for teaching with research-based instructional strategies.

Federal Education Tax Benefits: Who Receives Them and to What Extent Do They Shape the Price of College Attendance? Stats in Brief. NCES 2012-212

ERIC Educational Resources Information Center

Radford, Alexandria Walton; Berkner, Lutz

2011-01-01

This Statistics in Brief applies IRS rules and data to a nationally representative sample of 2007-08 undergraduates to estimate who received education tax benefits and looks at the extent to which these benefits shaped their price of college attendance. Key findings include: (1) Nearly one-half of all 2007-08 undergraduates were estimated to have…

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

Massaro, F.; D’Abrusco, R.; Paggi, A.

The Fermi-Large Area Telescope (LAT) First Source Catalog (1FGL) was released in 2010 February and the Fermi-LAT 2-Year Source Catalog (2FGL) appeared in 2012 April, based on data from 24 months of operation. Since they were released, many follow up observations of unidentified γ-ray sources have been performed and new procedures for associating γ-ray sources with potential counterparts at other wavelengths have been developed. Here we review and characterize all of the associations as published in the 1FGL and 2FGL catalogs on the basis of multifrequency archival observations. In particular, we located 177 spectra for the low-energy counterparts that weremore » not listed in the previous Fermi catalogs, and in addition we present new spectroscopic observations of eight γ-ray blazar candidates. Based on our investigations, we introduce a new counterpart category of “candidate associations” and propose a refined classification for the candidate low-energy counterparts of the Fermi sources. We compare the 1FGL-assigned counterparts with those listed in 2FGL to determine which unassociated sources became associated in later releases of the Fermi catalogs. We also search for potential counterparts to all of the remaining unassociated Fermi sources. Finally, we prepare a refined and merged list of all of the associations of 1FGL plus 2FGL that includes 2219 unique Fermi objects. This is the most comprehensive and systematic study of all the associations collected for the γ-ray sources available to date. We conclude that 80% of the Fermi sources have at least one known plausible γ-ray emitter within their positional uncertainty regions.« less

VizieR Online Data Catalog: Multiwavelength catalog in the SEP field (Baronchelli+, 2016)

NASA Astrophysics Data System (ADS)

Baronchelli, I.; Scarlata, C.; Rodighiero, G.; Franceschini, A.; Capak, P. L.; Mei, S.; Vaccari, M.; Marchetti, L.; Hibon, P.; Sedgwick, C.; Pearson, C.; Serjeant, S.; Menendez-Delmestre, K.; Salvato, M.; Malkan, M.; Teplitz, H. I.; Hayes, M.; Colbert, J.; Papovich, C.; Devlin, M.; Kovacs, A.; Scott, K. S.; Surace, J.; Kirkpatrick, J. D.; Atek, H.; Urrutia, T.; Scoville, N. Z.; Takeuchi, T. T.

2016-04-01

Spitzer-IRAC/MIPS Extragalactic survey (SIMES) is a Spitzer Cycle 8 General Observer program (PID 80039, P.I.: Scarlata) observed during the warm mission phase. The survey covers an area of 7.74deg2 to a depth of ~5.80μJy (3σ) at 3.6μm and 5.25μJy at 4.5μm. The field was covered in two visits, between 2011 November 16 and 23, in order to facilitate identification and removal of asteroids. The MIPS 24μm catalog is described in Clements et al. (2011, J/MNRAS/411/373). This catalog covers an area of ~12deg2 in the South Ecliptic Pole (SEP) region and includes counterparts at 70um of the 24um detected sources, and so we limit the analysis to the cross-correlation between IRAC and MIPS 24 and report the 70um association identified in the original MIPS catalog. The SIMES field was observed as part of the Herschel Multi-tiered Extragalactic Survey (HerMES, Oliver et al. 2012, VIII/95; Wang et al. 2014MNRAS.444.2870W). Here, we keep only those sources with fluxes above 3σ in at least one SPIRE band (250, 350 or 500um). A central area of approximately one square degree was observed at the MPG/ESO 2.2m telescope at La Silla with the Wide Field Imager (WFI) during 2010 October (P.I.: T. Takeuchi). Four pointings with the Rc broadband filter (λc=6517.25Å) were obtained, covering a total area of 1.13deg2. (1 data file).

The Milky Way Project: Mapping star formation in our home Galaxy, one click at a time

NASA Astrophysics Data System (ADS)

Jayasinghe, Tharindu K.; Povich, Matthew S.; Dixon, Don; Velasco, Jose; Milky Way Project Team

2017-01-01

In the recent years, citizen science has helped astronomers comb through large data sets to identify patterns and objects that are not easily found through automated processes. The Milky Way Project (MWP), a popular citizen science initiative, presents internet users with images from the GLIMPSE, MIPSGAL, SMOG and CYGNUS-X surveys of the Galactic plane using the Spitzer Space Telescope. These citizen scientists are directed to make "classification" drawings on the images to identify targeted classes of astronomical objects. We present an updated data reduction pipeline for the MWP. Written from the ground up in Python, this data reduction pipeline allows for the aggregation of classifications made by MWP users into catalogs of infrared (IR) bubbles, IR bow shocks and “yellowballs” (which may be the early precursors of IR bubbles). Coupled with the more accurate bubble classification tool used in the latest iterations of the MWP, this pipeline enables for better accuracy in the shapes and sizes of the bubbles when compared with those listed in the first MWP data release (DR1). We obtain an initial catalog of over 4000 bubbles using 2 million user classifications made between 2012 and 2015. Combined with the classifications from the latest MWP iteration (2016-2017), we will use a database of over 4 million classifications to produce a MWP DR2 bubble catalog. We will also create the first catalog of candidate IR bow shocks identified through citizen science and an updated “yellowball” catalog. This work is supported by the National Science Foundation under grants CAREER-1454334 and AST-1411851.

34 CFR 648.61 - How must the academic department supervise the training of fellows?

Code of Federal Regulations, 2013 CFR

2013-07-01

... 34 Education 3 2013-07-01 2013-07-01 false How must the academic department supervise the training... academic department supervise the training of fellows? The institution shall provide to fellows at least one academic year of supervised training in instruction at the graduate or undergraduate level at the...

Two Undergraduate Projects for Data Acquisition and Control

NASA Astrophysics Data System (ADS)

Hiersche, Kelly; Pena, Tara; Grogan, Tanner; Wright, Matthew

We are designing two separate instruments for use in our undergraduate laboratory. In the first project, a Raspberry Pi is used to simultaneously monitor a large number of current and voltage readings and store them in a database. In our second project, we are constructing our own microcontrollers to work as a general-purpose interface based off work carried out in Review of Scientific Instruments 84, 103101 (2013). It was designed for low cost and simple construction, making it ideal for undergraduate level work. This circuit has room for two interchangeable daughter boards, giving it the capability to work as a general lab interface, lock-in detector, or waveform generator.

The design of a medical school social justice curriculum.

PubMed

Coria, Alexandra; McKelvey, T Greg; Charlton, Paul; Woodworth, Michael; Lahey, Timothy

2013-10-01

The acquisition of skills to recognize and redress adverse social determinants of disease is an important component of undergraduate medical education. In this article, the authors justify and define "social justice curriculum" and then describe the medical school social justice curriculum designed by the multidisciplinary Social Justice Vertical Integration Group (SJVIG) at the Geisel School of Medicine at Dartmouth. The SJVIG addressed five goals: (1) to define core competencies in social justice education, (2) to identify key topics that a social justice curriculum should cover, (3) to assess social justice curricula at other institutions, (4) to catalog institutionally affiliated community outreach sites at which teaching could be paired with hands-on service work, and (5) to provide examples of the integration of social justice teaching into the core (i.e., basic science) curriculum. The SJVIG felt a social justice curriculum should cover the scope of health disparities, reasons to address health disparities, and means of addressing these disparities. The group recommended competency-based student evaluations and advocated assessing the impact of medical students' social justice work on communities. The group identified the use of class discussion of physicians' obligation to participate in social justice work as an educational tool, and they emphasized the importance of a mandatory, longitudinal, immersive, mentored community outreach practicum. Faculty and administrators are implementing these changes as part of an overall curriculum redesign (2012-2015). A well-designed medical school social justice curriculum should improve student recognition and rectification of adverse social determinants of disease.

VizieR Online Data Catalog: Astro-photometric catalog of the core of NGC 5139 (Bellini+, 2017)

NASA Astrophysics Data System (ADS)

Bellini, A.; Anderson, J.; Bedin, L. R.; King, I. R.; van der Marel, R. P.; Piotto, G.; Cool, A.

2018-01-01

The core of ω Cen (NGC 5139) has been observed through many of the WFC3 filters since 2009 for calibration purposes, and new observations continue to be scheduled. Table 1 summarizes the massive archive of data, organized in a camera/filter fashion. We downloaded from the archive a total of 655 exposures (~205Ks) taken through 26 HST different bands: 18 for WFC3/UVIS (385 exposures) and 8 for WFC3/IR (270 exposures); spanning 2009 July to 2013 March. This data set can be accessed at MAST via this link: http://archive.stsci.edu/doi/resolve/resolve.html?doi=10.17909/T9WG6S (5 data files).

Domestic violence education for UK and Ireland undergraduate dental students: a five-year perspective.

PubMed

Patel, Neil; Bailey, Edmund; Mahdmina, Ayeh; Lomax, Alastair; Coulthard, Paul

2014-08-01

The purpose of this cross-sectional study was to ascertain whether undergraduate dental students in the United Kingdom and Ireland are receiving formal teaching on recognizing and managing domestic violence (DV) as part of their curricula. A questionnaire was sent to all dental schools in the UK and Ireland in 2007 and again in 2012, requesting information on whether the subject was taught, by which specialty it was taught, and whether schools felt it was important to include in the curriculum. In 2007, twelve of the fifteen dental schools completed and returned the questionnaire, for a response rate of 80 percent; in 2012, eleven of the sixteen dental schools responded, for a response rate of 69 percent. The main findings were that, in 2007, 50 percent of the responding schools were providing teaching about DV and the majority of this teaching was delivered by oral surgery and pediatric dentistry departments. In 2012, only 45 percent of the responding schools were teaching DV, with 60 percent of this teaching being delivered by pediatric dentists. This study's findings suggest that DV is an undertaught area in UK and Irish undergraduate dental curricula. Some schools recognized the importance of DV teaching; however, they have been unable to implement it because of a full curriculum and lack of appropriately trained staff amongst other reasons.

VizieR Online Data Catalog: 2 new candidate luminous blue variables (Gvaramadze+ 2012)

NASA Astrophysics Data System (ADS)

Gvaramadze, V. V.; Kniazev, A. Y.; Miroshnichenko, A. S.; Berdnikov, L. N.; Langer, N.; Stringfellow, G. S.; Todt, H.; Hamann, W.-R.; Grebel, E. K.; Buckley, D.; Crause, L.; Crawford, S.; Gulbis, A.; Hettlage, C.; Hooper, E.; Husser, T.-O.; Kotze, P.; Loaring, N.; Nordsieck, K. H.; O'Donoghue, D.; Pickering, T.; Potter, S.; Romero Colmenero, E.; Vaisanen, P.; Williams, T.; Wolf, M.; Reichart, D. E.; Ivarsen, K. M.; Haislip, J. B.; Nysewander, M. C.; Lacluyze, A. P.

2013-03-01

Two circular shells, which are the main subject of this paper, were discovered using the WISE 22-um archival data. Spectral observations of WS1 and WS2 were conducted with SALT on 2011 June 12 and 13 during the performance verification phase of the Robert Stobie Spectrograph. (3 data files).

VizieR Online Data Catalog: WISE All-Sky Data Release (Cutri+ 2012)

NASA Astrophysics Data System (ADS)

Cutri, R. M.; et al.

2012-04-01

The Wide-field Infrared Survey Explorer (WISE; see Wright et al. 2010AJ....140.1868W) is a NASA Medium Class Explorer mission that conducted a digital imaging survey of the entire sky in the 3.4, 4.6, 12 and 22um mid-infrared bandpasses (hereafter W1, W2, W3 and W4). WISE will produce and release to the world astronomical and educational communities and general public a digital Image Atlas covering the sky in the four survey bands, and a reliable Source Catalog containing accurate photometry and astrometry for over 300 million objects. The WISE Catalog and Atlas will enable a broad variety of research efforts ranging from the search for the closest stars and brown dwarfs to the most luminous galaxies in the Universe. WISE science data products will serve as an important reference data set for planning observations and interpreting data obtained with future ground and space-borne observatories, such as JWST. WISE was launched on 2009-12-14 from Vandenberg SLC2W. (1 data file).

VizieR Online Data Catalog: Orbits based on SOAR speckle interferometry. II. (Tokovinin, 2017)

NASA Astrophysics Data System (ADS)

Tokovinin, A.

2018-01-01

We present new or updated orbits of 44 binary systems or subsystems. It is based on speckle interferometric measurements made at the 4.1m Southern Astrophysical Research (SOAR) telescope (Tokovinin et al. 2010, Cat. J/AJ/139/743; 2014, Cat. J/AJ/147/123; 2015, Cat. J/AJ/150/50; 2016, Cat. J/AJ/151/153; 2010PASP..122.1483T; Tokovinin 2012, Cat. J/AJ/144/56) combined with archival data collected in the Washington Double Star Catalog (WDS; Mason et al. 2001-2014, Cat. B/wds). It continues previous work on binary orbits resulting from the SOAR speckle program and follows the template of the Paper I (Tokovinin 2016, Cat. J/AJ/152/138), where the motivation is discussed. Briefly, the calculation of binary orbits is part of the astronomical infrastructure, and visual orbital elements are used in many areas. The state of the art is reflected in the Sixth Catalog of Visual Binary Orbits (VB6; Hartkopf et al. 2001AJ....122.3472H; http://www.usno.navy.mil/USNO/astrometry/optical-IR-prod/wds/orb6.html). (5 data files).

47 CFR 73.1020 - Station license period.

Code of Federal Regulations, 2011 CFR

2011-10-01

..., 2013. (4) Alabama and Georgia: (i) Radio stations, April 1, 2012. (ii) Television stations, April 1, 2013. (5) Arkansas, Louisiana and Mississippi: (i) Radio stations, June 1, 2012. (ii) Television stations, June 1, 2013. (6) Tennessee, Kentucky and Indiana: (i) Radio stations, August 1, 2012. (ii...

Pediatric Online Evidence-Based Medicine Assignment Is a Novel Effective Enjoyable Undergraduate Medical Teaching Tool

PubMed Central

Kotb, Magd A.; Elmahdy, Hesham Nabeh; Khalifa, Nour El Deen Mahmoud; El-Deen, Mohamed Hamed Nasr; Lotfi, Mohamed Amr N.

2015-01-01

Abstract Evidence-based medicine (EBM) is delivered through a didactic, blended learning, and mixed models. Students are supposed to construct an answerable question in PICO (patient, intervention, comparison, and outcome) framework, acquire evidence through search of literature, appraise evidence, apply it to the clinical case scenario, and assess the evidence in relation to clinical context. Yet these teaching models have limitations especially those related to group work, for example, handling uncooperative students, students who fail to contribute, students who domineer, students who have personal conflict, their impact upon progress of their groups, and inconsistent individual acquisition of required skills. At Pediatrics Department, Faculty of Medicine, Cairo University, we designed a novel undergraduate pediatric EBM assignment online system to overcome shortcomings of previous didactic method and aimed to assess its effectiveness by prospective follow-up during academic years 2012 to 2013 and 2013 to 2014. The novel web-based online interactive system was tailored to provide sequential single and group assignments for each student. Single assignment addressed a specific case scenario question, while group assignment was teamwork that addressed different questions of same case scenario. Assignment comprised scholar content and skills. We objectively analyzed students’ performance by criterion-based assessment and subjectively by anonymous student questionnaire. A total of 2879 were enrolled in 5th year Pediatrics Course consecutively, of them 2779 (96.5%) logged in and 2554 (88.7%) submitted their work. They were randomly assigned to 292 groups. A total of 2277 (89.15%) achieved ≥80% of total mark (4/5), of them 717 (28.1%) achieved a full mark. A total of 2178 (85.27%) and 2359 (92.36%) made evidence-based conclusions and recommendations in single and group assignment, respectively (P < 0.001). A total of 1102 (43.1%) answered student questionnaire, of them 898 (81.48%) found e-educational experience satisfactory, 175 (15.88%) disagreed, and 29 (2.6%) could not decide. A total of 964 (87.47%) found single assignment educational, 913 (82.84%) found group assignment educational, and 794 (72.3%) enjoyed it. Web-based online interactive undergraduate EBM assignment was found effective in teaching medical students and assured individual student acquisition of concepts and skills of pediatric EMB. It was effective in mass education, data collection, and storage essential for system and student assessment. PMID:26200621

Pediatric Online Evidence-Based Medicine Assignment Is a Novel Effective Enjoyable Undergraduate Medical Teaching Tool: A SQUIRE Compliant Study.

PubMed

Kotb, Magd A; Elmahdy, Hesham Nabeh; Khalifa, Nour El Deen Mahmoud; El-Deen, Mohamed Hamed Nasr; Lotfi, Mohamed Amr N

2015-07-01

Evidence-based medicine (EBM) is delivered through a didactic, blended learning, and mixed models. Students are supposed to construct an answerable question in PICO (patient, intervention, comparison, and outcome) framework, acquire evidence through search of literature, appraise evidence, apply it to the clinical case scenario, and assess the evidence in relation to clinical context. Yet these teaching models have limitations especially those related to group work, for example, handling uncooperative students, students who fail to contribute, students who domineer, students who have personal conflict, their impact upon progress of their groups, and inconsistent individual acquisition of required skills. At Pediatrics Department, Faculty of Medicine, Cairo University, we designed a novel undergraduate pediatric EBM assignment online system to overcome shortcomings of previous didactic method and aimed to assess its effectiveness by prospective follow-up during academic years 2012 to 2013 and 2013 to 2014. The novel web-based online interactive system was tailored to provide sequential single and group assignments for each student. Single assignment addressed a specific case scenario question, while group assignment was teamwork that addressed different questions of same case scenario. Assignment comprised scholar content and skills. We objectively analyzed students' performance by criterion-based assessment and subjectively by anonymous student questionnaire. A total of 2879 were enrolled in 5th year Pediatrics Course consecutively, of them 2779 (96.5%) logged in and 2554 (88.7%) submitted their work. They were randomly assigned to 292 groups. A total of 2277 (89.15%) achieved ≥ 80% of total mark (4/5), of them 717 (28.1%) achieved a full mark. A total of 2178 (85.27%) and 2359 (92.36%) made evidence-based conclusions and recommendations in single and group assignment, respectively (P < 0.001). A total of 1102 (43.1%) answered student questionnaire, of them 898 (81.48%) found e-educational experience satisfactory, 175 (15.88%) disagreed, and 29 (2.6%) could not decide. A total of 964 (87.47%) found single assignment educational, 913 (82.84%) found group assignment educational, and 794 (72.3%) enjoyed it. Web-based online interactive undergraduate EBM assignment was found effective in teaching medical students and assured individual student acquisition of concepts and skills of pediatric EMB. It was effective in mass education, data collection, and storage essential for system and student assessment.

Enhancing undergraduate nursing students' global health competencies in South Korea.

PubMed

Kim, Yoonseo; Han, Kihye; Yoo, Hae Young

2017-09-01

As the need for greater global health competency increases for health care professionals in South Korea, educational efforts for nursing students have begun. This study examined the effectiveness of two educational courses for freshmen and sophomores that were designed to improve students' global health competencies. A trend study was conducted for all undergraduate nursing students enrolled in a 4-year undergraduate nursing program in 2013 and 2014. We assessed students' global health competencies (1-knowledge and interests in global health and health equity, 2-global health skills, and 3-learning needs) in 2013 and 2014 and analyzed variance between mean scores by year and by course exposure, using 95% confidence intervals. Students who took both global health courses (sophomores in both years) reported higher global health-related knowledge and interests than did freshmen (p < .01); these scores were not sustained a year later. The two courses may have improved students' global health competencies. Reinforcement of knowledge in later courses may be needed to build on the global competencies. © 2017 Wiley Periodicals, Inc.

VizieR Online Data Catalog: SNR G18.8+0.3 data cubes (Paron+, 2015)

NASA Astrophysics Data System (ADS)

Paron, S.; Celis Pena, M.; Ortega, M. E.; Petriella, A.; Rubio, M.; Dubner, G.; Giacani, E.

2015-07-01

The observations of the molecular lines were carried out between September 7 and 13, 2013 with the 10m Atacama Submillimeter Telescope Experiment (ASTE). We used the CATS345 receiver, which is a two-single band SIS receiver remotely tunable in the LO frequency range of 324-372GHz. (2 data files).

VizieR Online Data Catalog: SDSS-RM project: velocity dispersions of QSOs (Shen+, 2015)

NASA Astrophysics Data System (ADS)

Shen, Y.; Greene, J. E.; Ho, L. C.; Brandt, W. N.; Denney, K. D.; Horne, K.; Jiang, L.; Kochanek, C. S.; McGreer, I. D.; Merloni, A.; Peterson, B. M.; Petitjean, P.; Schneider, D. P.; Schulze, A.; Strauss, M. A.; Tao, C.; Trump, J. R.; Pan, K.; Bizyaev, D.

2015-09-01

The spectra were taken as part of the SDSS-III BOSS survey (Eisenstein et al. 2011AJ....142...72E; Dawson et al. 2013AJ....145...10D) from 2014 January to July. The wavelength coverage of BOSS spectroscopy is 3650-10400Å, with a spectral resolution of R~2000. (2 data files).

A Compendium of Social-Behavioral Research Funded by NCER and NCSER: 2002-2013. NCER 2016-2002

ERIC Educational Resources Information Center

Yamaguchi, Ryoko; Hall, Adam; Stapleton, Katina; Doolittle, Emily; Buckley, Jacquelyn

2016-01-01

The purpose of this compendium is to catalog NCER's and NCSER's contributions to social-behavioral research. Research undertaken as part of these projects is contributing to a knowledge base that ultimately aims to improve academic outcomes for students via improvements in students' social-behavioral competencies, teachers' practices, and the…

VizieR Online Data Catalog: KIC star parallaxes from asteroseismology vs Gaia (Huber+, 2017)

NASA Astrophysics Data System (ADS)

Huber, D.; Zinn, J.; Bojsen-Hansen, M.; Pinsonneault, M.; Sahlholdt, C.; Serenelli, A.; Aguirre, V. S.; Stassun, K.; Stello, D.; Tayar, J.; Bastien, F.; Bedding, T. R.; Buchhave, L. A.; Chaplin, W. J.; Davies, G. R.; Garcia, R. A.; Latham, D. W.; Mathur, S.; Mosser, B.; Sharma, S.

2018-03-01

Our sample consists of dwarfs, subgiants, and red giants from the APOGEE-Kepler Asteroseismic Science Consortium (APOKASC, Pinsonneault+ J/ApJS/215/19), supplemented with seismic detections using Kepler short-cadence data from Chaplin+ (2014MNRAS.445..946C) and Huber+ (2013, J/ApJ/767/127). (2 data files).

VizieR Online Data Catalog: The Seven Sisters DANCe. II. Pleiades (Barrado+, 2016)

NASA Astrophysics Data System (ADS)

Barrado, D.; Bouy, H.; Bouvier, J.; Moraux, E.; Sarro, L. M.; Bertin, E.; Cuillandre, J. C.; Stauffer, J. R.; Lillo-Box, J.; Pollock, A.

2016-08-01

Lithium equivalent widths (Table 1), Proper motions (Table 2), and general properties (Table 3) for bona fide members of the Pleiades clusters, based on the literature and the DANCe membership analysis (Bouy et al. 2013A&A...554A.101B, 2015, Cat. J/A+A/577/A148). (3 data files).

A Structured Approach to Honours Undergraduate Research Course, Evaluation Rubrics and Assessment

NASA Astrophysics Data System (ADS)

Khoukhi, Amar

2013-10-01

This paper presents a new approach to the Honours Undergraduate Research Course design and implementation. The course design process, assessment and evaluation rubrics are provided. Lessons learned and the experience of the faced challenges and opportunities for two cohort offerings of the course during the winter terms of 2011 and 2012 are highlighted. Assessments show that major benefits include increasing interaction with the faculty and increasing intellectual maturity, skills, knowledge and confidence for the students and for the faculty, the furthering of research projects by the participation of undergraduate students. The course can serve as a model that can be easily adapted for use across the disciplines of science, technology, engineering and mathematics.

Tuition and Fees in the West 2013-14. Policy Insights

ERIC Educational Resources Information Center

Bransberger, Peace

2014-01-01

Average resident undergraduate tuition and fees for the academic year 2013-14 at public two-year institutions in the Western Interstate Commission for Higher Education (WICHE) region (excluding California) increased by 3.2 percent ($106) from the previous year, while published prices at public four-year institutions grew by 3.1 percent ($231). By…

76 FR 30139 - Federal Need Analysis Methodology for the 2012-2013 Award Year

Federal Register 2010, 2011, 2012, 2013, 2014

2011-05-24

... DEPARTMENT OF EDUCATION Federal Need Analysis Methodology for the 2012-2013 Award Year AGENCY: Federal Student Aid, Department of Education. ACTION: Notice of revision of the Federal Need Analysis...; 84.268; 84.379]. Federal Need Analysis Methodology for the 2012-2013 award year; Federal Pell Grant...

The role of tablets in accessing information throughout undergraduate medical education in Botswana.

PubMed

Witt, Rachel E; Kebaetse, Masego B; Holmes, John H; Littman-Quinn, Ryan; Ketshogileng, Dineo; Antwi, Cynthia; Kovarik, Carrie; Nkomazana, Oathokwa

2016-04-01

Mobile learning (mLearning) uses wireless networks and mobile devices to expand physician trainees' and healthcare providers' access to and exchange of medical information. Opportunities to increase implementation and expand use of mobile devices to support health care information access and delivery in Africa are vast, but the rapid growth of mLearning has caused project implementation to outpace objective measurement of impact. This study makes a contribution to the existing body of literature regarding mLearning implementation in Africa through its focus on the use of smart devices (tablets) in undergraduate medical education and medical students' perceptions of the effects on their learning environment. The population of this prospective mixed-methods study consisted of 82 undergraduate medical students (45 third year and 37 fourth year) at the University of Botswana Faculty of Medicine. They received tablets in the earliest phase of the mLearning project implementation (between November 2012 and January 2013), when they were in the third and fourth year of their medical training. Usage of the tablets was assessed both quantitatively and qualitatively, through both application usage tracking and focus groups. Based on application usage data and coding and analysis of focus group discussions, undergraduate medical students indicated that tablets were useful in their medical education, allowing them continual access to information and opportunities for communication. Participants noted that the primary barrier to use of tablets was the lack of mobile cellular Internet beyond the Wi-Fi zones at the training sites. Moreover, participants offered suggestions for improvements to the implementation process. Even in resource-limited settings where Internet access can be unreliable and intermittent, the adoption of tablets can have benefits to medical education by providing consistent access to extensive and current medical information resources. This study highlights the value of clinical resources with offline functionality, with or without consistent access to the Internet. There is also the potential for optimizing the use of tablets through improved training and technical support. Copyright © 2016 Elsevier Ireland Ltd. All rights reserved.

Clinical pharmacokinetics: perceptions of hospital pharmacists in Qatar about how it was taught and how it is applied.

PubMed

Kheir, Nadir; Awaisu, Ahmed; Gad, Hoda; Elazzazy, Shereen; Jibril, Farah; Gajam, Mawadda

2015-12-01

The application of clinical pharmacokinetics (PK) is essential when providing pharmaceutical care. Appropriate application of PK monitoring results in improved patient outcomes including decreased mortality, length of treatment, length of hospital stay, and adverse effects of drug therapy. Despite the well-documented evidence of benefits of clinical PK services, many pharmacists find it challenging to apply PK in clinical practice. To evaluate pharmacists' training backgrounds, attitude, practices, and perceived barriers pertaining to the application of PK in clinical practice in Qatar. All hospitals under Hamad Medical Corporation, the main healthcare provider in Qatar. This was a cross-sectional, descriptive study that was conducted between October 2012 and January 2013, using a self-administered web-based survey. Pharmacists were eligible to participate if they: (1) were working as full-time hospital pharmacists and; (2) have been in practice for at least 1 year. PK contents learned in undergraduate curriculum; perception towards the PK contents and instructions received in the undergraduate curriculum and; application of PK in current clinical practice. A total of 112 pharmacists responded to the questionnaire. The majority of the respondents (n = 91; 81.3 %) reported that they had received PK course(s) in their undergraduate curriculum. Similarly, the majority (70-80 %) of them agreed that the undergraduate PK courses or contents they received were important and relevant to their current practice. The pharmacists identified spending more time on dispensing and inventory issues rather than clinical practice, scarce resources, and manual rather than computerized PK calculations as some of the barriers they encountered in learning about PK and its application. The characteristics of the surveyed pharmacists such as gender, age, highest academic degree, and country of graduation did not influence the pharmacists' perception and attitudes towards PK teaching and application (p > 0.05). PK course contents were perceived to lack depth and relevance to practice, and pharmacist had no experiential training that included aspects of PK. These, and other issues, result in poor application of PK in practice.

The Effective of Using 5 Simple Steps (QSCCS) Learning Activities on Facebook to Promote Self-Learning in the 21st Century in Technology Printing and Advertising Course for Undergraduate Students in Education Technology and Communications

ERIC Educational Resources Information Center

Sittiwong, Tipparat; Wongnam, Thanet

2015-01-01

The objectives of this study were to: 1) study the result of implementing QSCCS with Facebook; 2) study students' opinions concerning the implementation of QSCCS with Facebook. The samples were 38 Technology and Communications undergraduates who attended Printing and Advertising Technology course in academic year of 2013. The information was…

3 CFR 8844 - Proclamation 8844 of July 27, 2012. National Korean War Veterans Armistice Day, 2012

Code of Federal Regulations, 2013 CFR

2013-01-01

... 3 The President 1 2013-01-01 2013-01-01 false Proclamation 8844 of July 27, 2012. National Korean War Veterans Armistice Day, 2012 8844 Proclamation 8844 Presidential Documents Proclamations Proclamation 8844 of July 27, 2012 Proc. 8844 National Korean War Veterans Armistice Day, 2012By the President...

VizieR Online Data Catalog: MEarth mid-to-late M dwarfs rotation & kinematics (West+, 2015)

NASA Astrophysics Data System (ADS)

West, A. A.; Weisenburger, K. L.; Irwin, J.; Berta-Thompson, Z. K.; Charbonneau, D.; Dittmann, J.; Pineda, J. S.

2016-02-01

To measure M dwarf rotation periods, we use photometric observations from the MEarth survey for transiting exoplanets (see Nutzman & Charbonneau 2008PASP..120..317N; Berta et al. 2012AJ....144..145B). All of the data in this paper come from the MEarth-north array at the Fred Lawrence Whipple Observatory (FLWO) at Mt. Hopkins, AZ, which has been gathering data since 2008. FAST spectrograph (1.5m Tillinghast Telescope at FLWO, R=3000; 5550-7550Å) observations were acquired over 30 nights from 2010 December to 2012 July. (1 data file).

VizieR Online Data Catalog: WASP-103b radial velocities and light curves (Gillon+, 2014)

NASA Astrophysics Data System (ADS)

Gillon, M.; Anderson, D. R.; Collier-Cameron, A.; Delrez, L.; Hellier, C.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Segransan, D.; Smith, A. M. S.; Smalley, B.; Southworth, J.; Triaud, A. H. M. J.; Udry, S.; Van Grootel, V.; West, R. G.

2014-01-01

The host star WASP-103 (1SWASPJ163715.59+071100.0 = 2MASS16371556+0711000; V=12.1, K=10.8) was observed by the southern station of the WASP survey during the 2010, 2011, and 2012 observing seasons, covering the intervals 2010 May 15 to Aug. 16, 2011 Mar. 26 to Aug. 20, and 2012 Mar. 25 to Jun. 28. Files wasp.dat, trappist.dat, euler.dat contain the photometric time-series presented in the paper. File rv.dat contains the radial velocity time-series presented in the paper. (4 data files).

77 FR 37007 - Applications for New Awards: National Institute on Disability and Rehabilitation Research...

Federal Register 2010, 2011, 2012, 2013, 2014

2012-06-20

... Robotics; Notice Inviting Applications for New Awards for Fiscal Year (FY) 2012 Catalog of Federal Domestic... Robotics. Note: The full text of these priorities is included in the notice of final priorities published... Disabilities (CFDA No. 84.133E-1) and 1 for Rehabilitation Robotics (CFDA No. 84.133E-3). Note: The Department...

Statistical Methods for Protecting Personally Identifiable Information in the Disclosure of Graduation Rates of First-Time, Full-Time Degree- or Certificate-Seeking Undergraduate Students by 2-Year Degree-Granting Institutions of Higher Education. Technical Brief. NCES 2012-151

ERIC Educational Resources Information Center

Chen, Xianglei; Bersudskaya, Vera; Cubarrubi, Archie

2011-01-01

The Higher Education Opportunity Act of 2008 (HEOA) requires that Title IV degree-granting institutions disclose annually the graduation rates of first-time, full-time degree- or certificate-seeking undergraduate students, disaggregated by gender, each major racial/ethnic subgroup, and receipt or non-receipt of a federal Pell grant or subsidized…

River-Based Experiential Learning: the Bear River Fellows Program

NASA Astrophysics Data System (ADS)

Rosenberg, D. E.; Shirley, B.; Roark, M. F.

2012-12-01

The Department of Civil and Environmental Engineering, Outdoor Recreation, and Parks and Recreation programs at Utah State University (USU) have partnered to offer a new, unique river-based experiential learning opportunity for undergraduates called the Bear River Fellows Program. The program allows incoming freshmen Fellows to experience a river first hand during a 5-day/4-night river trip on the nearby Bear River two weeks before the start of their first Fall semester. As part of the program, Fellows will navigate the Bear River in canoes, camp along the banks, interact with local water and environmental managers, collect channel cross section, stream flow, vegetation cover, and topological complexity data, meet other incoming freshmen, interact with faculty and graduate students, develop boating and leadership skills, problem solve, and participate as full members of the trip team. Subsequently, Fellows will get paid as undergraduate researchers during their Fall and Spring Freshman semesters to analyze, synthesize, and present the field data they collect. The program is a collaborative effort between two USU academic units and the (non-academic) division of Student Services and supports a larger National Science Foundation funded environmental modelling and management project for the lower Bear River, Utah watershed. We have advertised the program via Facebook and emails to incoming USU freshmen, received 35 applications (60% women), and accepted 5 Fellows into the program (3 female and 2 male). The river trip departs August 14, 2012. The poster will overview the Bear River Fellows Program and present qualitative and preliminary outcomes emerging from the trip and Fellows' work through the Fall semester with the field data they collect. We will also undertake more rigorous and longer longitudinal quantitative evaluation of Program outcomes (for example, in problem-solving and leadership) both in Spring 2013 and in subsequent 2013 and 2014 offerings of the program.

VizieR Online Data Catalog: Astrometry and photometry of nearby white dwarfs (Limoges+, 2013)

NASA Astrophysics Data System (ADS)

Limoges, M.-M.; Lepine, S.; Bergeron, P.

2014-06-01

Optical spectra have been obtained with the Steward Observatory 2.3m telescope and the B&C spectrograph on 2009 May, 2009 Nov, 2010 July, with the NOAO Mayall 4m telescope and the RC spectrograph on 2009 Aug, 2010 Mar, 2010 Oct, and with the NOAO 2.1m and the Goldcam spectrograph on 2009 Dec, 2010 May. The adopted configurations allow a spectral coverage of λλ3800-5600 and λλ3800-6700, at an intermediate resolution of ~6ÅFWHM. Spectra were first obtained at low signal-to-noise ratio (S/N ~25). As a result of our spectroscopic observations, 193 newly identified white dwarfs from the SUPERBLINK catalog have been spectroscopically confirmed (Tables 3 and 4). (3 data files).

VizieR Online Data Catalog: Spectroscopic binary population of ONC and NGC2264 (Kounkel+, 2016)

NASA Astrophysics Data System (ADS)

Kounkel, M.; Hartmann, L.; Tobin, J. J.; Mateo, M.; Bailey, J. I., III; Spencer, M.

2016-06-01

We reanalyzed all of the spectra previously obtained by T09 (Tobin et al. 2009, J/ApJ/697/1103) for the ONC region and by T15 (Tobin et al. 2015, J/AJ/149/119) for the NGC 2264 region (including several stars observed but not included in their published catalog) using Hectochelle and MIKE fibers. In addition to these data, we include new observations from these instruments (spanning 2008 Oct to 2009 Dec) and from the Michigan/Magellan Fiber System (M2FS). We observed a total of four fields toward the ONC and two fields toward NGC 2264 in 2013 November and 2014 February using M2FS. The MgI filter was used covering a wavelength range of ~5100-5210Å. (4 data files).

78 FR 27249 - Announcement of Funding Awards for Fiscal Year 2012/2013; Strong Cities, Strong Communities...

Federal Register 2010, 2011, 2012, 2013, 2014

2013-05-09

... Awards for Fiscal Year 2012/2013; Strong Cities, Strong Communities National Resource Network AGENCY... 2012/2013 Strong Cities, Strong Communities National Resource Network (SC2 Network). The purpose of... SC2 Network is a capacity building program targeted to assisting the nation's most distressed...

New paradigm in training of undergraduate clinical skills: the NEPTUNE-CS project at the Split University School of Medicine.

PubMed

Simunovic, Vladimir J; Hozo, Izet; Rakic, Mladen; Jukic, Marko; Tomic, Snjezana; Kokic, Slaven; Ljutic, Dragan; Druzijanic, Nikica; Grkovic, Ivica; Simunovic, Filip; Marasovic, Dujomir

2010-10-01

Clinical skills' training is arguably the weakest point in medical schools' curriculum. This study briefly describes how we at the Split University School of Medicine cope with this problem. We consider that, over the last decades, a considerable advancement in teaching methodologies, tools, and assessment of students has been made. However, there are many unresolved issues, most notably: (i) the institutional value system, impeding the motivation of the teaching staff; (ii) lack of a strong mentoring system; (iii) organization, timing, and placement of training in the curriculum; (iv) lack of publications pertinent to training; and (v) unwillingness of patients to participate in student training. To improve the existing training models we suggest increased institutional awareness of obstacles, as well as willingness to develop mechanisms for increasing the motivation of faculty. It is necessary to introduce changes in the structure and timing of training and to complement it with a catalog, practicum, and portfolio of clinical skills. At Split University School of Medicine, we developed a new paradigm aimed to improve the teaching of clinical skills called "Neptune-CSS," which stands for New Paradigm in Training of Undergraduate Clinical Skills in Split.

Progress toward poliomyelitis eradication - Afghanistan, January 2012-September 2013.

PubMed

2013-11-22

Since 2012, transmission of indigenous wild poliovirus (WPV) has been limited to three countries: Afghanistan, Pakistan, and Nigeria. This report describes polio eradication activities and progress in Afghanistan during January 2012-September 2013 and updates previous reports. During 2012, 37 WPV type 1 (WPV1) cases were confirmed in Afghanistan, compared with 80 cases in 2011; nine WPV1 cases were confirmed during January-September, 2013, compared with 26 WPV1 cases during the same period in 2012. Since November 2012, no WPV1 cases have been reported from the Southern Region, previously the main WPV reservoir in Afghanistan; all nine polio cases in 2013 were in the Eastern Region and caused by WPV1 that originated in Pakistan. From October 2012 to March 2013, 14 polio cases caused by circulating vaccine-derived poliovirus type 2 (cVDPV2) were detected in the Southern Region. During 2012-2013, strategies to improve supplemental immunization activity (SIA)§ effectiveness in 11 low-performing districts (LPDs) in the Southern Region included increasing staff and supervisory training, implementing short-interval-additional-dose (SIAD) campaigns, placing transit vaccination teams at the borders of districts inaccessible because of insecurity, and establishing permanent polio vaccination teams to vaccinate children quarterly. From March 2012 to August 2013, the percentage of children unreached during SIAs declined by 43% in the Southern Region but increased by 122% in the Eastern Region. Despite ongoing challenges, the government of Afghanistan continues to expand the application of innovative solutions to reach unvaccinated children in accessible and inaccessible districts.

VizieR Online Data Catalog: Herschel protocluster survey (Kato+, 2016)

NASA Astrophysics Data System (ADS)

Kato, Y.; Matsuda, Y.; Smail, I.; Swinbank, A. M.; Hatsukade, B.; Umehata, H.; Tanaka, I.; Saito, T.; Iono, D.; Tamura, Y.; Kohno, K.; Erb, D. K.; Lehmer, B. D.; Geach, J. E.; Steidel, C. C.; Alexander, D. M.; Yamada, T.; Hayashino, T.

2017-11-01

The observations were executed in Large Map mode with a scan rate of 30arcsec/s, repeated 14 times for each field (Nrep=14). The dates of observations are 2012 June 22 (2QZCluster), 2012 March 4 (HS1700), and 2012 May 10 (SSA22). The coverage of the maps are ~23-arcminx23-arcmin (2QZCluster), ~22-arcminx22-arcmin (HS1700), and ~33-arcminx33-arcmin (SSA22) corresponding to ~40-60 comoving Mpc at the protocluster redshifts, which are sufficient to search for concentration of DSFGs around the density peak of protocluster members. The integration times are 1.8, 1.5, and 3.7h for 2QZCluster, HS1700, and SSA22, respectively. (5 data files).

Influences on Faculty Willingness to Mentor Undergraduate Students from Another University as Part of an Interinstitutional Research Training Program

PubMed Central

Morales, Danielle X.; Grineski, Sara E.; Collins, Timothy W.

2016-01-01

In 2014, the National Institutes of Health invested $31 million in 10 primary institutions across the United States through the Building Undergraduate Infrastructure Leading to Diversity (BUILD) program; one requirement of BUILD is sending undergraduate trainees from those primary institutions to partner institutions for research experiences. Mechanisms like BUILD are designed to broaden research opportunities for students, especially those from underrepresented backgrounds. However, to our knowledge, no studies have examined faculty willingness to mentor undergraduates from other institutions through structured training programs. Survey data from 536 faculty members at 13 institutions were collected in Fall 2013 and analyzed using multiple statistical techniques. Results show that faculty who valued the opportunity to increase diversity in the academy and those who believed that mentoring undergraduates benefited their own research expressed greater willingness to serve as research mentors to visiting undergraduates, and faculty who perceived that they did not have the ability to accommodate additional students expressed less willingness to do so. Most respondents viewed student and faculty incentives as motivating factors in their willingness to mentor, but their perspectives on different types of incentives varied based on faculty career stage, discipline, and research funding status. Results have important implications for designing multi-institutional undergraduate research training programs. PMID:27521237

3 CFR 8774 - Proclamation 8774 of January 13, 2012. Religious Freedom Day, 2012

Code of Federal Regulations, 2013 CFR

2013-01-01

... 3 The President 1 2013-01-01 2013-01-01 false Proclamation 8774 of January 13, 2012. Religious... 13, 2012 Proc. 8774 Religious Freedom Day, 2012By the President of the United States of America A... religious freedom. Hailing from diverse backgrounds and faiths, countless settlers have shared a simple...

77 FR 73694 - Sunshine Federal Register Notice

Federal Register 2010, 2011, 2012, 2013, 2014

2012-12-11

...: Nuclear Regulatory Commission [NRC-2012- 0002]. DATES: Weeks of December 10, 17, 24, 31, 2012, January 7..., 2012. Week of December 24, 2012--Tentative There are no meetings scheduled for the week of December 24..., 2012. Week of January 7, 2013--Tentative Tuesday, January 8, 2013 9:00 a.m. Briefing on Fort Calhoun...

Physics Bachelors: Initial Employment. Data from the Degree Recipient Follow-Up Survey for the Classes of 2013 and 2014. Focus On

ERIC Educational Resources Information Center

Mulvey, Patrick; Pold, Jack

2017-01-01

New physics bachelors entering the workforce receive some of the highest starting salaries of any undergraduate majors. Bachelors accepting STEM (science, technology, engineering, mathematics) positions in the private sector had a median starting salary of $55,000. Physics bachelors from 2013 and 2014 were contacted in the winter following the…

VizieR Online Data Catalog: Spatial deconvolution code (Quintero Noda+, 2015)

NASA Astrophysics Data System (ADS)

Quintero Noda, C.; Asensio Ramos, A.; Orozco Suarez, D.; Ruiz Cobo, B.

2015-05-01

This deconvolution method follows the scheme presented in Ruiz Cobo & Asensio Ramos (2013A&A...549L...4R) The Stokes parameters are projected onto a few spectral eigenvectors and the ensuing maps of coefficients are deconvolved using a standard Lucy-Richardson algorithm. This introduces a stabilization because the PCA filtering reduces the amount of noise. (1 data file).

VizieR Online Data Catalog: LMC OGLE-III Shallow Survey variable stars (Ulaczyk+, 2013)

NASA Astrophysics Data System (ADS)

Ulaczyk, K.; Szymanski, M. K.; Udalski, A.; Kubiak, M.; Pietrzynski, G.; Soszynski, I.; Wyrzykowski, L.; Poleski, R.; Gieren, W.; Walker, A. R.; Garcia-Varela, A.

2017-07-01

Photometric data were collected using the 1.3-m Warsaw Telescope located at Las Campanas Observatory, operated by the Carnegie Institution for Science. We used exactly the same photometric system as in the OGLE-III main survey. Detailed information about whole instrumentation can be found in Udalski (2003AcA....53..291U). (5 data files).

VizieR Online Data Catalog: RMS survey: NIR spectroscopy of massive YSOs (Cooper+, 2013)

NASA Astrophysics Data System (ADS)

Cooper, H. D. B.; Lumsden, S. L.; Oudmaijer, R. D.; Hoare, M. G.; Clarke, A. J.; Urquhart, J. S.; Mottram, J. C.; Moore, T. J. T.; Davies, B.

2014-04-01

Spectroscopic observations of the YSO candidates were made using the UIST instrument at the United Kingdom Infra-Red Telescope (UKIRT) observatory from 2002 to 2008. 247 objects were successfully observed over 84 nights. Sources were selected from the ~2000 candidate MYSOs found using the MSX catalogue in the preceding stages of the RMS survey. (6 data files).

VizieR Online Data Catalog: Energy levels & transition rates for F-like ions (Si+, 2016)

NASA Astrophysics Data System (ADS)

Si, R.; Li, S.; Guo, X. L.; Chen, Z. B.; Brage, T.; Jonsson, P.; Wang, K.; Yan, J.; Chen, C. Y.; Zou, Y. M.

2017-01-01

For the multiconfiguration Dirac-Hartree-Fock (MCDHF) calculation we use the latest version of the GRASP2K code (Jonsson+ 2013CoPhC.184.2197J), while the many-body perturbation theory (MBPT) calculation is performed using the Flexible Atomic Code (FAC; Gu 2008CaJPh..86..675G). (2 data files).

VizieR Online Data Catalog: GJ 1214b optical and near-IR transit phot. (Angerhausen+, 2017)

NASA Astrophysics Data System (ADS)

Angerhausen, D.; Dreyer, C.; Placek, B.; Csizmadia, Sz.; Eigmueller, P.; Godolt, M.; Kitzmann, D.; Mallonn, M.; Becklin, E.; Collins, P.; Dunham, E. W.; Grenfell, J. L.; Hamilton, R. T.; Kabath, P.; Logsdon, S. E.; Mandell, A.; Mandushev, G.; McElwain, M.; McLean, I. S.; Pfueller, E.; Rauer, H.; Savage, M.; Shenoy, S.; Vacca, W. D.; van Cleve, J. E.; Wiedemann, M.; Wolf, J.

2017-11-01

The joint US-German Cycle 2 Guest Investigator (GI) programme - US-proposal: Angerhausen (2013); Germanproposal: Dreyer (2013) - was performed on SOFIAs flight number 149 on UT February 27, 2014. Observations were simultaneously conducted in two optical HIPO channels: open blue at 0.3-0.6um and Sloan z' at 0.9-m; and one infrared FLITECAM fiter: Paschen-α cont. at 1.9um. Complementary data were also obtained with the optical focal plane guiding camera FPI+ in the Sloan i' band (0.8um). (5 data files).

VizieR Online Data Catalog: Study of protostars in the Perseus molecular cloud (Tobin+, 2016)

NASA Astrophysics Data System (ADS)

Tobin, J. J.; Looney, L. W.; Li, Z.-Y.; Chandler, C. J.; Dunham, M. M.; Segura-Cox, D.; Sadavoy, S. I.; Melis, C.; Harris, R. J.; Kratter, K.; Perez, L.

2018-01-01

We conducted observations with the VLA in B-configuration between 2013 September 28 and 2013 November 20 and in A-configuration during 2014 February 24 to 2014 May 31 and 2015 June 19 to 2015 September 21. The B-configuration (also referred to as B-array) has a maximum baseline (antenna separation) of 11.1 km and at 8 mm provides a resolution of ~0.2" (46 au). The A-configuration (A-array) has a maximum baseline of 36.4 km, providing a resolution of ~0.065" (15 au). (2 data files).

A cross-sectional study of the beliefs and attitudes towards menstruation of Chinese undergraduate males and females in Hong Kong.

PubMed

Wong, Wing Chi; Li, Mei Kuen; Chan, Wai Ying Veronica; Choi, Yuen Yu; Fong, Chi Hung Sandra; Lam, Ka Wah Kara; Sham, Wun Chi; So, Ping Ping; Wong, Kit; Yeung, Kuen Ha; Yeung, Tsz Yan

2013-12-01

To explore the beliefs and attitudes towards menstruation of Chinese undergraduates in Hong Kong and to compare those of (1) male and female undergraduates with those of (2) undergraduates studying health-related vs. nonhealth-related programmes. Menstruation is typically viewed as a forbidden topic or a troublesome experience. These negative beliefs and attitudes result from existing myths and taboos associated with cultural factors and health education levels. A cross-sectional survey was conducted in all universities in Hong Kong. Undergraduates were invited through convenience sampling to complete a questionnaire assessing their attitudes and beliefs towards menstruation. A questionnaire on 'beliefs about and attitudes towards menstruation' was adopted. Questionnaires were self-administered by the respondents. A total of 450 questionnaires were distributed, and a response rate of 96.6% was obtained; 416 completed questionnaires were collected and analysed. Many Chinese undergraduates agreed that menstruation is annoying, causes disability, involves prescription and proscription and is not pleasant. When comparing the beliefs and attitudes towards menstruation of Chinese male undergraduates with those of female undergraduates, females tended to disagree that menstruation should be maintained secret, but tended to agree that it was annoying. When comparing the beliefs and attitudes towards menstruation of Chinese undergraduates studying health-related programmes with those under nonhealth-related programmes, the latter group exhibited a higher level of belief in prescription and proscription for menstruation than the former group. Chinese undergraduates in Hong Kong were influenced by the traditional Chinese culture and social environment, resulting in negative attitudes towards menstruation. This study recommends that sex education, especially reproductive health education, be extended to tertiary education. This study provides relevant information on planning the content of sex education or reproductive health education for Chinese undergraduates. © 2013 John Wiley & Sons Ltd.

Teaching of Psychology: Ideas and Innovations. Proceedings of the Annual Conference (26th, Tarrytown, New York, March 23-24, 2012)

ERIC Educational Resources Information Center

Howell-Carter, Marya, Ed.; Gonder, Jennifer, Ed.; Mushtaq, Zahra, Ed.

2012-01-01

Included herein is the conference proceedings of the 26th Annual Conference on the Teaching of Psychology: Ideas and Innovations, sponsored by the Psychology Department of the State University of New York at Farmingdale. The conference theme for 2012 was: The value of an undergraduate degree in psychology: Why psychology--Why now?. The Conference…

Probabilistic Seismic Hazard Assessment for Northeast India Region

NASA Astrophysics Data System (ADS)

Das, Ranjit; Sharma, M. L.; Wason, H. R.

2016-08-01

Northeast India bounded by latitudes 20°-30°N and longitudes 87°-98°E is one of the most seismically active areas in the world. This region has experienced several moderate-to-large-sized earthquakes, including the 12 June, 1897 Shillong earthquake ( M w 8.1) and the 15 August, 1950 Assam earthquake ( M w 8.7) which caused loss of human lives and significant damages to buildings highlighting the importance of seismic hazard assessment for the region. Probabilistic seismic hazard assessment of the region has been carried out using a unified moment magnitude catalog prepared by an improved General Orthogonal Regression methodology (Geophys J Int, 190:1091-1096, 2012; Probabilistic seismic hazard assessment of Northeast India region, Ph.D. Thesis, Department of Earthquake Engineering, IIT Roorkee, Roorkee, 2013) with events compiled from various databases (ISC, NEIC,GCMT, IMD) and other available catalogs. The study area has been subdivided into nine seismogenic source zones to account for local variation in tectonics and seismicity characteristics. The seismicity parameters are estimated for each of these source zones, which are input variables into seismic hazard estimation of a region. The seismic hazard analysis of the study region has been performed by dividing the area into grids of size 0.1° × 0.1°. Peak ground acceleration (PGA) and spectral acceleration ( S a) values (for periods of 0.2 and 1 s) have been evaluated at bedrock level corresponding to probability of exceedance (PE) of 50, 20, 10, 2 and 0.5 % in 50 years. These exceedance values correspond to return periods of 100, 225, 475, 2475, and 10,000 years, respectively. The seismic hazard maps have been prepared at the bedrock level, and it is observed that the seismic hazard estimates show a significant local variation in contrast to the uniform hazard value suggested by the Indian standard seismic code [Indian standard, criteria for earthquake-resistant design of structures, fifth edition, Part-I. Bureau of Indian Standards, New Delhi, 2002]. Not only holistic treatment of earthquake catalog and seismogenic zones has been performed, but also higher resolution in spatial distribution could be achieved. The COV maps have been provided with the strong ground-motion maps under various conditions to show the confidence in the results obtained. Results obtained in the present study would be helpful for risk assessment and other disaster mitigation-related studies.

Earthquake Hazard and Risk in Alaska

NASA Astrophysics Data System (ADS)

Black Porto, N.; Nyst, M.

2014-12-01

Alaska is one of the most seismically active and tectonically diverse regions in the United States. To examine risk, we have updated the seismic hazard model in Alaska. The current RMS Alaska hazard model is based on the 2007 probabilistic seismic hazard maps for Alaska (Wesson et al., 2007; Boyd et al., 2007). The 2015 RMS model will update several key source parameters, including: extending the earthquake catalog, implementing a new set of crustal faults, updating the subduction zone geometry and reoccurrence rate. First, we extend the earthquake catalog to 2013; decluster the catalog, and compute new background rates. We then create a crustal fault model, based on the Alaska 2012 fault and fold database. This new model increased the number of crustal faults from ten in 2007, to 91 faults in the 2015 model. This includes the addition of: the western Denali, Cook Inlet folds near Anchorage, and thrust faults near Fairbanks. Previously the subduction zone was modeled at a uniform depth. In this update, we model the intraslab as a series of deep stepping events. We also use the best available data, such as Slab 1.0, to update the geometry of the subduction zone. The city of Anchorage represents 80% of the risk exposure in Alaska. In the 2007 model, the hazard in Alaska was dominated by the frequent rate of magnitude 7 to 8 events (Gutenberg-Richter distribution), and large magnitude 8+ events had a low reoccurrence rate (Characteristic) and therefore didn't contribute as highly to the overall risk. We will review these reoccurrence rates, and will present the results and impact to Anchorage. We will compare our hazard update to the 2007 USGS hazard map, and discuss the changes and drivers for these changes. Finally, we will examine the impact model changes have on Alaska earthquake risk. Consider risk metrics include average annual loss, an annualized expected loss level used by insurers to determine the costs of earthquake insurance (and premium levels), and the loss exceedance probability curve used by insurers to address their solvency and manage their portfolio risk. We analyze risk profile changes in areas with large population density and for structures of economic and financial importance: the Trans-Alaska pipeline, industrial facilities in Valdez, and typical residential wood buildings in Anchorage, Fairbanks and Juneau.

Mapping the Future: Towards Oncology Curriculum Reform in Undergraduate Medical Education at a Canadian Medical School

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

Kwan, Jennifer Y.Y.; Nyhof-Young, Joyce; Catton, Pamela

Purpose: To evaluate (1) the quantity and quality of current undergraduate oncology teaching at a major Canadian medical school; and (2) curricular changes over the past decade, to enhance local oncology education and provide insight for other educators. Methods and Materials: Relevant 2011-2012 undergraduate curricular sessions were extracted from the University of Toronto curriculum mapping database using keywords and database identifiers. Educational sessions were analyzed according to Medical Council of Canada objectives, discussion topics, instructor qualifications, teaching format, program year, and course subject. Course-related oncology research projects performed by students during 2000 to 2012 were extracted from another internal database.more » Elective choices of clerks during 2008-2014 were retrieved from the institution. The 2011-2012 and 2000-2001 curricula were compared using common criteria. Results: The 2011-2012 curriculum covers 5 major themes (public health, cancer biology, diagnosis, principles of care, and therapy), which highlight 286 oncology teaching topics within 80 sessions. Genitourinary (10, 12.5%), gynecologic (8, 10.0%), and gastrointestinal cancers (7.9, 9.8%) were the most commonly taught cancers. A minority of sessions were taught by surgical oncologists (6.5, 8.1%), medical oncologists (2.5, 3.1%), and radiation oncologists (1, 1.2%). During 2000-2012, 9.0% of students (233 of 2578) opted to complete an oncology research project. During 2008-2014, oncology electives constituted 2.2% of all clerkship elective choices (209 of 9596). Compared with pre-2001 curricula, the 2012 oncology curriculum shows notable expansion in the coverage of epidemiology (6:1 increase), prevention (4:1), screening (3:1), and molecular biology (6:1). Conclusions: The scope of the oncology curriculum has grown over the past decade. Nevertheless, further work is needed to improve medical student knowledge of cancers, particularly those relevant to public health needs. Defining minimum curricular content, emphasizing content based on population needs, and ensuring educational delivery with the support and expertise of oncologists and non-oncologists will be essential next steps.« less

Correlates of Stress and Coping among Jordanian Nursing Students during Clinical Practice in Psychiatric/Mental Health Course.

PubMed

Alzayyat, Abdulkarim; Al-Gamal, Ekhlas

2016-10-01

Training in psychiatric settings is stressful for nursing students. The purpose of this study was to examine the correlations between the students' characteristics, their stress degrees, stressors and types of coping strategies they experience during training in psychiatric course. A descriptive, correlational, longitudinal design was used. Sixty-five undergraduate nursing students were recruited randomly from five Jordanian universities. Self-report questionnaires were administered at the second semester of the 2012-2013 academic year. The findings showed that students who utilized avoidance or transference strategies reported high stress degrees. Moreover, the results showed that those students who were in the fourth year, with a low family income, who avoid extracurricular activities, with a low academic grade or who registered in other clinical course(s) reported high stress degrees. These findings present a worthy data for the clinical instructors that facilitate students training in psychiatric settings and promote their psychosocial well-being. Copyright © 2014 John Wiley & Sons, Ltd. Copyright © 2014 John Wiley & Sons, Ltd.

[Childhood Traumas and Attachment Style-Associated Depression Symptoms: The Mediator Role of Alexithymia].

PubMed

Şenkal, İpek; Işıklı, Sedat

2015-01-01

The aim of this study was to investigate the mediator role of alexithymia and its relationship with childhood traumas (sexual abuse, physical abuse, emotional abuse, emotional neglect, physical neglect) and attachment style (anxiety and avoidance dimensions of attachment) associated depression symptoms in adulthood. The sample of this study included 417 undergraduate university students from different departments that studied at Hacettepe University during the 2012-2013 school years with a final analysis done over 369 participants. The Demographic Information Form, Experiences in Close Relationship Inventory-II (ECR-R), Childhood Trauma Questionnaire (CTQ), Toronto Alexithymia Scale (TAS-20), and Beck Depression Inventory (BDI) were administered to the undergraduate students who participated in this study. Mediator analyses were applied to the data. The results revealed that the total score of the Toronto Alexithymia Scale had a partial mediating role in the relationship of childhood traumas (the total score of Childhood Trauma Questionnaire), childhood emotional abuse and emotional neglect with depressive symptom levels in university students. Besides, the total score of the Toronto Alexithymia Scale had a full mediating role in the relationship between childhood physical neglect and depressive symptom levels in adulthood. Additionally, it was found that the total score of the Toronto Alexithymia Scale had a partial mediating role between the anxiety dimension of the attachment and the depressive symptom levels. This study revealed that alexithymia should be considered as a significant variable in the relationship of childhood traumas and attachment patterns with depression symptoms in adulthood.

Learning styles of medical students at Taibah University: Trends and implications

PubMed Central

Guraya, Shaista Salman; Guraya, Salman Yousuf; Habib, Fawzia A.; Khoshhal, Khalid I.

2014-01-01

Background: Understanding the learning styles of medical students can drive the institutions to adapt instructional materials to enhance students’ learning of knowledge and skills. This study explored the learning styles of undergraduate medical students, comparing gender variations in terms of their significant preferences. Materials and Methods: A cross-sectional observational study was performed in 2012-2013, incorporating 1st-5th year undergraduate medical students of Taibah University. The instrument used was a Learning Style Questionnaire, with four learning styles (activist, reflector, theorist and pragmatist) and 40 items. Results: Of 450 students, 384 responded (response rate; 85%). No single learning style predominated; 96 (25%) reflectors, 78 (20%) theorists, 68 (17%) pragmatists, and 37 (9%) activists. Combined reflector and theorist was the predominant dual learning style in 27 (7%) students. Among genders, theorist style had a significant result (P = 0.071) indicating that theorists varied among genders due to their different opinions. Learning style preferences of theorists and pragmatists also showed a significant result (P = 0.000 each), depicting that both genders had unique preferences. Males had fewer variations of preferences, when compared with females who showed a significant difference of opinions (P < 0.05). Conclusion: The students in the study preferred diverse learning styles, which were unevenly distributed, reflectors being the most common and activists as the least common. The results reflect the need to promote self-directed learning and modifications of instructional strategies, with expectant tilt in the students’ learning styles towards activists and pragmatists. PMID:25709657

Emotional intelligence score and performance of dental undergraduates.

PubMed

Hasegawa, Yuh; Ninomiya, Kazunori; Fujii, Kazuyuki; Sekimoto, Tsuneo

2016-09-01

The purpose of this study was to investigate the relationship between emotional intelligence (EI) and undergraduate dental students' ability to deal with different situations of communication in a clinical dentistry practical training course of communication skills. Fourth-year students in 2012 and in 2013 at the Nippon Dental University School of Life Dentistry at Niigata participated in the survey. The total number of participating students was 129 (88 males and 41 females). The students were asked to complete the Japanese version of the Mayer-Salovey-Caruso Emotional Intelligence Test in communication skills. Female students tended to have significantly higher EI score than males. The EI score in the group with high-grade academic performers was higher than in the low-grade group. The influence of EI on academic performance appeared to be mainly due to the students' ability to accurately perceiving emotions and to their ability to understand emotional issues. The importance of EI may also lie in its ability to parse out personality factors from more changeable aspects of a person's behavior. Although further studies are required, we believe that dental educators need to assume the responsibility to help students develop their emotional competencies that they will need to prosper in their chosen careers. In our conclusion, dental educators should support low achievers to increase their levels of self-confidence instead of concentrating mainly on improving their technical skill and academic performance. This may lead to upgrading their skills for managing emotions and to changing their learning approach.

3 CFR 8796 - Proclamation 8796 of April 3, 2012. Education and Sharing Day, U.S.A., 2012

Code of Federal Regulations, 2013 CFR

2013-01-01

... 3 The President 1 2013-01-01 2013-01-01 false Proclamation 8796 of April 3, 2012. Education and Sharing Day, U.S.A., 2012 8796 Proclamation 8796 Presidential Documents Proclamations Proclamation 8796 of April 3, 2012 Proc. 8796 Education and Sharing Day, U.S.A., 2012By the President of the United States of...

3 CFR 8795 - Proclamation 8795 of April 2, 2012. World Autism Awareness Day, 2012

Code of Federal Regulations, 2013 CFR

2013-01-01

... 3 The President 1 2013-01-01 2013-01-01 false Proclamation 8795 of April 2, 2012. World Autism..., 2012 Proc. 8795 World Autism Awareness Day, 2012By the President of the United States of America A Proclamation Autism spectrum disorders (ASDs) affect young people and adults of every background, and millions...

3 CFR 8845 - Proclamation 8845 of July 27, 2012. World Hepatitis Day, 2012

Code of Federal Regulations, 2013 CFR

2013-01-01

... 3 The President 1 2013-01-01 2013-01-01 false Proclamation 8845 of July 27, 2012. World Hepatitis..., 2012 Proc. 8845 World Hepatitis Day, 2012By the President of the United States of America A Proclamation Worldwide, one in twelve people is living with viral hepatitis—a disease that threatens the health...

3 CFR 8895 - Proclamation 8895 of November 1, 2012. Military Family Month, 2012

Code of Federal Regulations, 2013 CFR

2013-01-01

... November 1, 2012 Proc. 8895 Military Family Month, 2012By the President of the United States of America A Proclamation Since our Nation's earliest days, courageous men and women of all backgrounds and beliefs have... 3 The President 1 2013-01-01 2013-01-01 false Proclamation 8895 of November 1, 2012. Military...

Assessment of Course-Based Undergraduate Research Experiences: A Meeting Report

PubMed Central

Auchincloss, Lisa Corwin; Laursen, Sandra L.; Branchaw, Janet L.; Eagan, Kevin; Graham, Mark; Hanauer, David I.; Lawrie, Gwendolyn; McLinn, Colleen M.; Pelaez, Nancy; Rowland, Susan; Towns, Marcy; Trautmann, Nancy M.; Varma-Nelson, Pratibha; Weston, Timothy J.; Dolan, Erin L.

2014-01-01

The Course-Based Undergraduate Research Experiences Network (CUREnet) was initiated in 2012 with funding from the National Science Foundation program for Research Coordination Networks in Undergraduate Biology Education. CUREnet aims to address topics, problems, and opportunities inherent to integrating research experiences into undergraduate courses. During CUREnet meetings and discussions, it became apparent that there is need for a clear definition of what constitutes a CURE and systematic exploration of what makes CUREs meaningful in terms of student learning. Thus, we assembled a small working group of people with expertise in CURE instruction and assessment to: 1) draft an operational definition of a CURE, with the aim of defining what makes a laboratory course or project a “research experience”; 2) summarize research on CUREs, as well as findings from studies of undergraduate research internships that would be useful for thinking about how students are influenced by participating in CUREs; and 3) identify areas of greatest need with respect to CURE assessment, and directions for future research on and evaluation of CUREs. This report summarizes the outcomes and recommendations of this meeting. PMID:24591501

Seismicity in Oklahoma Before Prague

NASA Astrophysics Data System (ADS)

Delorey, A. A.; Johnson, P. A.

2017-12-01

The 2011 M5.7 Prague earthquake was the first large anthropogenically induced earthquake in Oklahoma. Since then, three more M5+ earthquakes followed it near Fairview, Pawnee, and Cushing. Oklahoma induced seismicity has garnered a lot of attention from both the media and the scientific community. But, little is known about seismicity in Oklahoma prior to the Prague earthquake due to a lack of instrumentation. We ask the question, "Was there any indication in the geophysical record prior to the Prague earthquake that bigger earthquakes were becoming more likely?" Fortunately, stations from Earthscope's Transportable Array were in Oklahoma during 2010 and 2011 providing a sparse, but still useful data set. Using our microseismicity detector called Interstation Seismic Coherence, we were able to catalog over 3000 earthquakes with a magnitude of completeness around 2.0 in northeastern Oklahoma over 17 months between June 2010 and the Prague earthquake in November 2011. During this period of time there are less than 200 earthquakes in the ANSS Comprehensive Catalog and 900 in the catalog produced by the Array Network Facility at the UCSD using Transportable Array stations. The M>5 earthquakes occurred in a region where stress conditions and seismicity rates were evolving much faster than they do in many natural systems presenting an opportunity to study the time dependence of upper crustal behavior. A clustering analysis shows that earthquakes occurring in northeastern Oklahoma during 2010-2011 are highly correlated with the magnitude of solid earth tides. Although some aftershocks and clusters were recorded following the Prague earthquake using temporary arrays, regional seismicity is not well recorded again until later in 2013. Of note, after 2013, we no longer observe tidal correlation suggesting the ensemble of fault criticality has evolved. One explanation for this change in earthquake behavior is a change in poroelastic conditions.

Biotechnology essay competition: biotechnology and sustainable food practices.

PubMed

Peng, Judy; Schoeb, Helena; Lee, Gina

2013-06-01

Biotechnology Journal announces our second biotechnology essay competition with the theme "biotechnology and sustainable food practices", open to all undergraduate students. Copyright © 2013 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.

Mm-Wave Spectroscopic Sensors, Catalogs, and Uncatalogued Lines

NASA Astrophysics Data System (ADS)

Medvedev, Ivan; Neese, Christopher F.; De Lucia, Frank C.

2014-06-01

Analytical chemical sensing based on high resolution rotational molecular spectra has been recognized as a viable technique for decades. We recently demonstrated a compact implementation of such a sensor. Future generations of these sensors will rely on automated algorithms for quantification of chemical dilutions based on their spectral libraries, as well as identification of spectral features not present in spectral catalogs. Here we present an algorithm aimed at detection of unidentified lines in complex molecular species based on spectroscopic libraries developed in our previous projects. We will discuss the approaches suitable for data mining in feature-rich rotational molecular spectra. Neese, C.F., I.R. Medvedev, G.M. Plummer, A.J. Frank, C.D. Ball, and F.C. De Lucia, "A Compact Submillimeter/Terahertz Gas Sensor with Efficient Gas Collection, Preconcentration, and ppt Sensitivity." Sensors Journal, IEEE, 2012. 12(8): p. 2565-2574

77 FR 76584 - Alaska Disaster #AK-00025

Federal Register 2010, 2011, 2012, 2013, 2014

2012-12-28

... Administrative declaration of a disaster for the State of Alaska dated 12/18/2012. Incident: High Winds and Flooding. Incident Period: 09/15/2012 through 09/30/2012. Effective Date: 12/18/2012. Physical Loan Application Deadline Date: 02/18/2013. Economic Injury (EIDL) Loan Application Deadline Date: 09/18/2013...

47 CFR 201.3 - Policy.

Code of Federal Regulations, 2012 CFR

2012-10-01

... 47 Telecommunication 5 2012-10-01 2012-10-01 false Policy. 201.3 Section 201.3 Telecommunication OFFICE OF SCIENCE AND TECHNOLOGY POLICY AND NATIONAL SECURITY COUNCIL EXECUTIVE POLICY § 201.3 Policy. (a... and recovery. (g) The Director of the Office of Science and Technology Policy will serve as the...

Seasonal Temperature Pattern Indicating Martian Dust Storms

NASA Image and Video Library

2016-06-09

This graphic shows Martian atmospheric temperature data related to seasonal patterns in occurrence of large regional dust storms. The data shown here were collected by the Mars Climate Sounder instrument on NASA's Mars Reconnaissance Orbiter over the course of one-half of a Martian year, during 2012 and 2013. The color coding indicates daytime temperatures of a layer of the atmosphere centered about 16 miles (25 kilometers) above ground level, corresponding to the color-key bar at the bottom of the graphic. Three regional dust storms indicated by increased temperatures are labeled A, B and C. A similar sequence of three large regional dust storms has been seen in atmosphere-temperature data from five other Martian years. The vertical axis is latitude on Mars, from the north pole at the top to south pole at the bottom. Each graphed data point is an average for all Martian longitudes around the planet. The horizontal axis is the time of year, spanning from the beginning of Mars' southern-hemisphere spring (on the left) to the end of southern-hemisphere summer. This is the half of the year when large Martian dust storms are most active. http://photojournal.jpl.nasa.gov/catalog/PIA20746

The 2008 M7.9 Wenchuan earthquake - a human-caused event

NASA Astrophysics Data System (ADS)

Klose, C. D.

2013-12-01

A catalog of global human-caused earthquakes shows statistical evidence that the triggering of earthquakes by large-scale geoengineering activities depends on geological and tectonic constrains (in Klose 2013). Such geoengineering activities also include the filling of water reservoirs. This presentation illuminates mechanical and statistical aspects of the 2008 M7.9 Wenchuan earthquake in light of the hypothesis of being NOT human-caused. However, available data suggest that the Wenchuan earthquake was triggered by the filling of the Zipungpu water reservoir 30 months prior to the mainshock. The reservoir spatially extended parallel and near to the main Beichuan fault zone in a highly stressed reverse fault regime. It is mechanically evident that reverse faults tend to be very trigger-sensitive due to mass shifts (static loads) that occur on the surface of the Earth's crust. These circumstances made a triggering of a seismic event of this magnitude at this location possible (in Klose 2008, 2012). The data show that the Wenchuan earthquake is not an outlier. From a statistical view point, the earthquake falls into the upper range of the family of reverse fault earthquakes that were caused by humans worldwide.