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Fermi-LAT Observations of the Gamma-Ray Burst GRB 130427AThe observations of the exceptionally bright gamma-ray burst (GRB) 130427A by the Large Area Telescope aboard the Fermi Gamma-ray Space Telescope provide constraints on the nature of these unique astrophysical sources. GRB 130427A had the largest fluence, highest-energy photon (95 GeV), longest gamma-ray duration (20 hours), and one of the largest isotropic energy releases ever observed from a GRB. Temporal and spectral analyses of GRB 130427A challenge the widely accepted model that the nonthermal high-energy emission in the afterglow phase of GRBs is synchrotron emission radiated by electrons accelerated at an external shock.
Document ID
20150007900
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Ackermann, M.
(Deutsches Elektronen-Synchrotron Zeuthen, Germany)
Ajello, M.
(California Univ. Berkeley, CA, United States)
Asano, K.
(Tokyo Univ. Chiba, Japan)
Atwood, W. B.
(California Univ. Santa Cruz, CA, United States)
Axelsson, M.
(Stockholm Univ. Sweden)
Baldini, L.
(Pisa Univ. Italy)
Ballet, J.
(CEA Saclay, Service d'Astrophysique Gif-sur-Yvette, France)
Barbiellini, G.
(Istituto Nazionale di Fisica Nucleare Trieste, Italy)
Baring, M. G.
(Rice Univ. Houston, TX, United States)
Bastieri, D.
(Istituto Nazionale di Fisica Nucleare Padova, Italy)
Gehrels, Cornelis
(NASA Goddard Space Flight Center Greenbelt, MD United States)
Date Acquired
May 12, 2015
Publication Date
November 21, 2013
Publication Information
Publication: Science
Publisher: Science
Volume: 343
Issue: 6166
Subject Category
Astrophysics
Report/Patent Number
GSFC-E-DAA-TN22618
Distribution Limits
Public
Copyright
Public Use Permitted.
Keywords
Observations
fermi
Gamma
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