D
D. Hinshaw
Researcher at Goddard Space Flight Center
Publications - 4
Citations - 756
D. Hinshaw is an academic researcher from Goddard Space Flight Center. The author has contributed to research in topics: Galaxy & Gamma-ray burst. The author has an hindex of 4, co-authored 4 publications receiving 741 citations.
Papers
More filters
Journal ArticleDOI
A short γ-ray burst apparently associated with an elliptical galaxy at redshift z = 0.225
Neil Gehrels,Craig L. Sarazin,P. T. O'Brien,Bing Zhang,L. M. Barbier,Scott Barthelmy,A. J. Blustin,David N. Burrows,J. K. Cannizzo,J. K. Cannizzo,Jay Cummings,Jay Cummings,Michael R. Goad,Stephen T. Holland,Stephen T. Holland,Cheryl Hurkett,J. A. Kennea,Andrew J. Levan,C. B. Markwardt,C. B. Markwardt,Keith O. Mason,Peter Mészáros,M. J. Page,David Palmer,Evert Rol,T. Sakamoto,T. Sakamoto,Richard Willingale,Lorella Angelini,Lorella Angelini,Andrew P. Beardmore,Patricia T. Boyd,Patricia T. Boyd,A. A. Breeveld,Sergio Campana,M. M. Chester,Guido Chincarini,Guido Chincarini,L. R. Cominsky,Giancarlo Cusumano,M. de Pasquale,Edward E. Fenimore,Paolo Giommi,Caryl Gronwall,Dirk Grupe,Joanne E. Hill,D. Hinshaw,Jens Hjorth,D. Hullinger,D. Hullinger,Kevin Hurley,Sylvio Klose,Shiho Kobayashi,Chryssa Kouveliotou,Hans A. Krimm,Hans A. Krimm,Vanessa Mangano,F. E. Marshall,Katherine E. McGowan,A. Moretti,Richard Mushotzky,Kazuhiro Nakazawa,Jay P. Norris,John A. Nousek,J. P. Osborne,K. L. Page,A. M. Parsons,Sandeep K. Patel,M. Perri,T. S. Poole,P. Romano,P. W. A. Roming,Stuart Rosen,G. Sato,Patricia Schady,Alan P. Smale,Jesper Sollerman,R. L. C. Starling,Martin Still,Martin Still,Masaya Suzuki,Gianpiero Tagliaferri,Tadayuki Takahashi,Makoto Tashiro,Jack Tueller,Alan A. Wells,Nicholas E. White,Ralph A. M. J. Wijers +87 more
TL;DR: In this article, the authors reported the detection of the X-ray afterglow from the short burst GRB 050509B and its location on the sky is near a luminous, non-star-forming elliptical galaxy at a redshift of 0.225.
Journal ArticleDOI
Swift panchromatic observations of the bright gamma-ray burst GRB 050525a
A. J. Blustin,Scott Barthelmy,P. T. Boyd,M. Capalbi,Stephen T. Holland,F. E. Marshall,Keith O. Mason,M. Perri,T. S. Poole,P. W. A. Roming,Stuart Rosen,Patricia Schady,Patricia Schady,Martin Still,Bing Zhang,Lorella Angelini,L. M. Barbier,A. P. Beardmore,A. A. Breeveld,David N. Burrows,Jay Cummings,J. Canizzo,Sergio Campana,M. M. Chester,G. Chincarini,L. R. Cominsky,A. Cucchiara,M. de Pasquale,E. E. Fenimore,N. Gehrels,P. Giommi,M. R. Goad,Caryl Gronwall,Dirk Grupe,Joanne E. Hill,D. Hinshaw,S. D. Hunsberger,Kevin Hurley,M. Ivanushkina,J. A. Kennea,Hans A. Krimm,Pawan Kumar,W. B. Landsman,V. La Parola,C. B. Markwardt,Katherine E. McGowan,Peter Mészáros,Teresa Mineo,A. Moretti,Adam N. Morgan,J. A. Nousek,P. T. O'Brien,J. P. Osborne,K. L. Page,M. J. Page,David Palmer,A. M. Parsons,James E. Rhoads,P. Romano,T. Sakamoto,G. Sato,Gianpiero Tagliaferri,Jack Tueller,Alan A. Wells,Nicholas E. White +64 more
TL;DR: In this paper, the authors derived an empirical timelag redshift from the BAT data of (z) over bar z 0: 69 +/- 0: 02, in good agreement with the spectroscopic redshift of 0.61.
Journal ArticleDOI
Ultraviolet number counts of galaxies from Swift UV/Optical Telescope deep imaging of the Chandra Deep Field South
E. A. Hoversten,C. Gronwall,D. E. vanden Berk,T. S. Koch,A. A. Breeveld,P. A. Curran,D. Hinshaw,F. E. Marshall,P. W. A. Roming,M. H. Siegel,Martin Still +10 more
TL;DR: In this article, the authors used deep Swift UV/Optical Telescope (UVOT) imaging of the Chandra Deep Field South to measure galaxy number counts in three near ultraviolet (NUV) filters.
Journal ArticleDOI
Ultraviolet number counts of galaxies from swift ultraviolet/optical telescope deep imaging of the chandra deep field south
E. A. Hoversten,Caryl Gronwall,D. E. vanden Berk,T. S. Koch,A. A. Breeveld,P. A. Curran,D. Hinshaw,F. E. Marshall,P. W. A. Roming,M. H. Siegel,Martin Still +10 more
TL;DR: In this article, the authors used deep Swift UV/Optical Telescope (UVOT) imaging of the Chandra Deep Field South is used to measure galaxy number counts in three near-ultraviolet (NUV) filters (uvw2: 1928 A, uvm2: 2246 A, and uvw1: 2600 A).