Zobrazeno 1 - 10
of 5 359
pro vyhledávání: '"Welsh W"'
We have carried out a systematic analysis of the nearby (z=0.0279) active galaxy Zw 229.015 using multi-epoch, multi-instrument and deep pointed observations with XMM-Newton, Suzaku, Swift and NuSTAR. Spectral and temporal variability are examined in
Externí odkaz:
http://arxiv.org/abs/1907.07048
Autor:
Gregg Barak
Publikováno v:
Criminal Justice Review. 34:570-572
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a2a8106564468b2814b84aa7be8a01fe
https://doi.org/10.1177/0734016808328802
https://doi.org/10.1177/0734016808328802
Autor:
Sperling J; Social Science Research Institute, Duke University, Durham, NC 27708, United States.; Clinical and Translational Science Institute, Duke University School of Medicine, Durham, NC 27701, United States.; Department of Medicine, Duke University School of Medicine, Durham, NC 27708, United States., Welsh W; Social Science Research Institute, Duke University, Durham, NC 27708, United States., Haseley E; Social Science Research Institute, Duke University, Durham, NC 27708, United States., Quenstedt S; Clinical and Translational Science Institute, Duke University School of Medicine, Durham, NC 27701, United States., Muhigaba PB; Clinical and Translational Science Institute, Duke University School of Medicine, Durham, NC 27701, United States., Brown A; Social Science Research Institute, Duke University, Durham, NC 27708, United States., Ephraim P; Institute of Health System Science, Feinstein Institutes for Medical Research, Northwell Health, Manhasset, NY 11030, United States., Shafi T; Department of Medicine, Houston Methodist, Houston, TX 77030, United States., Waitzkin M; Science & Society, Duke University, Durham, NC 27708, United States., Casarett D; Department of Medicine, Duke University School of Medicine, Durham, NC 27708, United States., Goldstein BA; Department of Biostatistics and Bioinformatics, Duke University School of Medicine, Durham, NC 27708, United States.
Publikováno v:
Journal of the American Medical Informatics Association : JAMIA [J Am Med Inform Assoc] 2025 Jan 01; Vol. 32 (1), pp. 51-62.
Autor:
Borucki, W. J., Agol, E., Fressin, F., Kaltenegger, L., Rowe, J., Isaacson, H., Fischer, D., Batalha, N., Lissauer, J. J., Marcy, G. W., Fabrycky, D., Désert, J. -M., Bryson, S. T., Barclay, T., Bastien, F., Boss, A., Brugamyer, E., Buchhave, L. A., Burke, Chris, Caldwell, D. A., Carter, J., Charbonneau, D., Crepp, J. R., Christensen-Dalsgaard, J., Christiansen, J. L., Ciardi, D., Cochran, W. D., DeVore, E., Doyle, L., Dupree, A. K., Endl, M., Everett, M. E., Ford, E. B., Fortney, J., Gautier III, T. N., Geary, J. C., Gould, A., Haas, M., Henze, C., Howard, A. W., Howell, S. B., Huber, D., Jenkins, J. M., Kjeldsen, H., Kolbl, R., Kolodziejczak, J., Latham, D. W., Lee, B. L., Lopez, E., Mullally, F., Orosz, J. A., Prsa, A., Quintana, E. V., Sanchez-Ojeda, R., Sasselov, D., Seader, S., Shporer, A., Steffen, J. H., Still, M., Tenenbaum, P., Thompson, S. E., Torres, G., Twicken, J. D., Welsh, W. F., Winn, J. N.
Publikováno v:
Science Express / http://www.sciencemag.org/content/early/recent / 18 April 2013 / Page 1/ 10.1126/science.1234702
We present the detection of five planets -- Kepler-62b, c, d, e, and f -- of size 1.31, 0.54, 1.95, 1.61 and 1.41 Earth radii, orbiting a K2V star at periods of 5.7, 12.4, 18.2, 122.4 and 267.3 days, respectively. The outermost planets (Kepler-62e &
Externí odkaz:
http://arxiv.org/abs/1304.7387
Autor:
Mauche, C. W., Abada-Simon, M., Desmurs, J. -F., Dulude, M. J., Ioannou, Z., Neill, J. D., Price, A., Sidro, N., Welsh, W. F., Astrophysics, the Center for Backyard, Observers, the American Association of Variable Star
We provide a summary of results, obtained from a multiwavelength (TeV gamma-ray, X-ray, UV, optical, and radio) campaign of observations of AE Aqr conducted in 2005 August 28-September 2, on the nature and correlation of the flux variations in the va
Externí odkaz:
http://arxiv.org/abs/1111.1190
Autor:
Steffen, J. H., Quinn, S. N., Borucki, W. J., Brugamyer, E., Bryson, S. T., Buchhave, L. A., Cochran, W. D., Endl, M., Fabrycky, D. C., Ford, E. B., Holman, M. J., Jenkins, J., Koch, D., Latham, D. W., MacQueen, P., Mullally, F., Prsa, A., Ragozzine, D., Rowe, J. F., Sanderfer, D. T., Seader, S. E., Short, D., Shporer, A., Thompson, S. E., Torres, G., Twicken, J. D., Welsh, W. F., Windmiller, G.
We present a hierarchical triple star system (KIC 9140402) where a low mass eclipsing binary orbits a more massive third star. The orbital period of the binary (4.98829 Days) is determined by the eclipse times seen in photometry from NASA's Kepler sp
Externí odkaz:
http://arxiv.org/abs/1106.4530
Autor:
Shporer, A., Winn, J. N., Dreizler, S., Colon, K. D., Wood-Vasey, W. M., Choi, P. I., Morley, C., Moutou, C., Welsh, W. F., Pollaco, D., Starkey, D., Adams, E., Barros, S. C. C., Bouchy, F., Cabrera-Lavers, A., Cerutti, S., Coban, L., Costello, K., Deeg, H., Diaz, R. F., Esquerdo, G. A., Fernandez, J., Fleming, S. W., Ford, E. B., Fulton, B. J., Good, M., Hebrard, G., Holman, M. J., Hunt, M., Kadakia, S., Lander, G., Lockhart, M., Mazeh, T., Morehead, R. C., Nelson, B. E., Nortmann, L., Reyes, F., Roebuck, E., Rudy, A. R., Ruth, R., Simpson, E., Vincent, C., Weaver, G., Xie, J. -W.
We present ground-based optical observations of the September 2009 and January 2010 transits of HD 80606b. Based on 3 partial light curves of the September 2009 event, we derive a midtransit time of T_c [HJD] = 2455099.196 +- 0.026, which is about 1
Externí odkaz:
http://arxiv.org/abs/1008.4129
Autor:
Welsh, W. F., Orosz, J. A.
Publikováno v:
ASP Conf.Ser.366:176,2007
We explore the possibility that the transit signature of an Earth-size planet can be detected in spectroscopic velocity shifts via the Rossiter effect. Under optimistic but not unrealistic conditions, it should be possible to detect a large terrestri
Externí odkaz:
http://arxiv.org/abs/0707.2407
We present phase-resolved spectroscopy of the short period cataclysmic variable WZ Sge obtained with the Hubble Space Telescope. We were able to resolve the orbital motion of a number of absorption lines that likely probe the environment near the acc
Externí odkaz:
http://arxiv.org/abs/0706.0987
Autor:
Gallo, L. C., Edwards, P. G., Ferrero, E., Kataoka, J., Lewis, D. R., Ellingsen, S. P., Misanovic, Z., Welsh, W. F., Whiting, M., Boller, Th., Brinkmann, W., Greenhill, J., Oshlack, A.
Publikováno v:
Mon.Not.Roy.Astron.Soc.370:245-254,2006
(abridged) The spectral energy distribution (SED) of the compact steep spectrum (CSS) source and possible radio-loud narrow-line Seyfert 1 galaxy (NLS1), PKS2004-447, is presented. Five out of six well studied RL NLS1 share this dual classification (
Externí odkaz:
http://arxiv.org/abs/astro-ph/0604480