E
E. E. Fenimore
Researcher at Los Alamos National Laboratory
Publications - 360
Citations - 14390
E. E. Fenimore is an academic researcher from Los Alamos National Laboratory. The author has contributed to research in topics: Gamma-ray burst & Neutron star. The author has an hindex of 51, co-authored 358 publications receiving 13692 citations. Previous affiliations of E. E. Fenimore include University of Maryland, Baltimore County.
Papers
More filters
Journal ArticleDOI
HETE Observations of the Gamma-Ray Burst GRB 030329: Evidence for an Underlying Soft X-Ray Component
Roland Vanderspek,Takanori Sakamoto,Takanori Sakamoto,C. Barraud,T. Tamagawa,Carlo Graziani,Motoko Suzuki,Y. Shirasaki,Gregory Y. Prigozhin,J. Villasenor,J. G. Jernigan,Geoffrey B. Crew,J. L. Atteia,Kevin Hurley,Nobuyuki Kawai,D. Q. Lamb,George R. Ricker,S. E. Woosley,N. Butler,John P. Doty,A. Dullighan,T. Q. Donaghy,E. E. Fenimore,M. Galassi,Masaru Matsuoka,K. Takagishi,Ken'ichi Torii,Atsumasa Yoshida,M. Boer,J. P. Dezalay,J-F. Olive,João Braga,R. K. Manchanda,G. Pizzichini +33 more
TL;DR: An exceptionally intense gamma-ray burst, GRB 030329, was detected and localized by the instruments on board the High Energy Transient Explorer satellite (HETE) at 11:37:14 UT on 2003 March 29 as discussed by the authors.
Posted Content
Redshifts For 220 BATSE Gamma-Ray Bursts Determined by Variability and the Cosmological Consequences
TL;DR: In this article, the time variability of a gamma-ray burst (GRB) appears to be correlated with the absolute luminosity of the burst: smooth bursts are intrinsically less luminous.
Journal ArticleDOI
Confirmation of the E(sup src)(sub Peak)-E(sub iso) (Amati) relation from the x-ray flash XRF 050416A observed by the Swift burst alert telescope
T. Sakamoto,T. Sakamoto,L. M. Barbier,Scott Barthelmy,Jay Cummings,Jay Cummings,E. E. Fenimore,N. Gehrels,D. Hullinger,Hans A. Krimm,Hans A. Krimm,C. B. Markwardt,C. B. Markwardt,David Palmer,A. M. Parsons,G. Sato,J. Tueller +16 more
TL;DR: In this article, the fluence ratio between the 15-25 and 25-50 keV energy bands of the X-ray flash (XRF) XRF 050416A is 1.5, thus making it the softest gamma-ray burst observed by BAT so far.
Journal ArticleDOI
Confirmation of the $\eps$ -- $\eiso$ (Amati) relation from the X-ray flash XRF 050416A observed by Swift/BAT
T. Sakamoto,L. M. Barbier,S. D. Barthelmy,J. R. Cummings,E. E. Fenimore,N. Gehrels,D. Hullinger,H. A. Krimm,C. B. Markwardt,D. M. Palmer,A. M. Parsons,G. Sato,J. Tueller +12 more
TL;DR: In this article, the authors reported the Swift Burst Alert Telescope (BAT) observations of the X-ray Flash (XRF) XRF 050416A, which is the softest gamma-ray burst (GRB) observed by BAT so far.
Journal ArticleDOI
GRB 010921: Discovery of the First High Energy Transient Explorer Afterglow
P. A. Price,P. A. Price,Shrinivas R. Kulkarni,Edo Berger,S. G. Djorgovski,Dale A. Frail,Dale A. Frail,Ashish Mahabal,D. W. Fox,Fiona A. Harrison,Joshua S. Bloom,S. A. Yost,Daniel E. Reichart,Arne Henden,George R. Ricker,R. van der Spek,Kevin Hurley,J-L. Atteia,Nobuyuki Kawai,E. E. Fenimore,Carlo Graziani +20 more
TL;DR: In this article, the authors reported the discovery of the optical and radio afterglow of GRB 010921, the first gamma-ray burst afterglove to be found from a localization by the High Energy Transient Explorer satellite.