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
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Journal ArticleDOI
High precision gamma-ray spectrometer PGS for Russian interplanetary mission to Mars
I. G. Mitrofanov,D.S. Anfimov,A. M. Chernenko,V. Sh. Dolidze,V. I. Kostenko,O. E. Isupov,Alexei Pozanenko,A. K. Ton'shev,D. A. Ushakov,G.F. Auchampaugh,Maureen M. Cafferty,D. M. Drake,E. E. Fenimore,R. W. Klebesadel,J. L. Longmire,C. E. Moss,Robert C. Reedy +16 more
TL;DR: The high precision gamma-ray spectrometer (PGS) is scheduled to be launched on the Russian MARS mission in 1996, and to go into an elliptical polar orbit around Mars as discussed by the authors.
Journal Article
GRB 130603B: Swift-BAT refined analysis.
S. D. Barthelmy,W. H. Baumgartner,J. R. Cummings,E. E. Fenimore,N. Gehrels,H. A. Krimm,A. Y. Lien,C. B. Markwardt,A. Melandri,D. M. Palmer,T. Sakamoto,G. Sato,M. Stamatikos,J. Tueller,T. N. Ukwatta +14 more
Journal ArticleDOI
Constraints on the fraction of repeating gamma-ray burst sources from batse measurements
The high-energy transient experiment (HETE) - An international multiwavelength mission
George Ricker,John P. Doty,Saul Rappaport,Roland Vanderspek,M. Matsuoka,Nobuyuki Kawai,Atsumasa Yoshida,E. E. Fenimore,Cheng Ho,Diane Roussel-Dupre +9 more
TL;DR: The High Energy Transient Experiment (HETE) as mentioned in this paper was the first multi-wavelength study of gamma-ray bursts with UV, X-ray, and gamma-rays instruments mounted on a single, compact spacecraft.
Journal ArticleDOI
Swift and XMM observations of the dark GRB 050326
Alberto Moretti,A. De Luca,D. Malesani,Sergio Campana,Andrea Tiengo,A. Cucchiara,James Reeves,G. Chincarini,C. Pagani,P. Romano,G. Tagliaferri,P. Banat,M. Capalbi,M. Perri,G. Cusumano,V. Mangano,Teresa Mineo,V. La Parola,A. P. Beardmore,M. R. Goad,J. P. Osborne,Joanne E. Hill,Lorella Angelini,David N. Burrows,Shiho Kobayashi,Peter Mészáros,Bing Zhang,S. D. Barthelmy,L. M. Barbier,N. E. White,E. E. Fenimore,L. R. Cominsky,N. Gehrels +32 more
TL;DR: In this article, the afterglow light curve did not show any break nor flares between ~1 hr and ~6 d after the burst, and decayed with a slope 1.70.