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.
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Journal ArticleDOI
GRB 221009A: The BOAT
Eric Burns,Dmitry S. Svinkin,E. E. Fenimore,D. A. Kann,J. F. Agüí Fernández,D. D. Frederiks,Rachel Hamburg,Stephen Lesage,Yu R Temiraev,A. Tsvetkova,Elisabetta Bissaldi,Michael S. Briggs,Rachel Dunwoody,C. Fletcher,Adam Goldstein,C. M. Hui,Boyan Hristov,Daniel Kocevski,A. Lysenko,Bagrat Mailyan,Joseph Mangan,Sheila McBreen,Judith Racusin,A. Ridnaia,Oliver J. Roberts,M. Ulanov,Péter Veres,Colleen A. Wilson-Hodge,Joshua D. Wood +28 more
TL;DR: In this article , the authors investigated the veracity of the BOAT claim by comparing it with a half century of prompt gamma-ray burst observations and found that the burst of GRB 221009A appears to be a once-in-10,000-year event.
Journal ArticleDOI
Gamma-burst observations from the Pioneer Venus Orbiter
TL;DR: The LASL Pioneer Venus Orbiter Gamma Burst Detector (OGBD) is a vital element in the long base-line array of similar instruments intended to precisely locate sources of gamma-ray bursts as discussed by the authors.
Proceedings ArticleDOI
Performance of the wide-field x-ray monitor on board the High-Energy Transient Explorer 2
Yuji Shirasaki,Nobuyuki Kawai,Atsumasa Yoshida,Masaru Matsuoka,Masaaki Namiki,Ikuya Sakurai,Makoto Yamauchi,K. Takagishi,Isamu Hatsukade,E. E. Fenimore,M. Galassi +10 more
TL;DR: The Wide-field X-ray Monitor (WFXM) is one of the scientific instruments carried on the High Energy Transient Explorer 2 (HETE-2) satellite planned to be launched in May, 2000 as discussed by the authors.
Journal ArticleDOI
Cyclotron lines in γ-ray burst spectra: Absorption in a radiation-driven wind
TL;DR: It is shown that the observed absorption lines may in fact form in a radiation-diriven plasma wind expelled at relativistic velocities from the surface of a neutron star.