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Fermi-LAT observations of the gamma-ray burst GRB 130427A

The 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 γ-ra... Full description

Journal Title: Science (New York N.Y.), 03 January 2014, Vol.343(6166), pp.42-7
Main Author: Ackermann, M
Other Authors: Ajello, M , Asano, K , Atwood, W B , Axelsson, M , Baldini, L , Ballet, J , Barbiellini, G , Baring, M G , Bastieri, D , Bechtol, K , Bellazzini, R , Bissaldi, E , Bonamente, E , Bregeon, J , Brigida, M , Bruel, P , Buehler, R , Burgess, J Michael , Buson
Format: Electronic Article Electronic Article
Language: English
Subjects:
ID: E-ISSN: 1095-9203 ; PMID: 24263133 Version:1 ; DOI: 10.1126/science.1242353
Link: http://pubmed.gov/24263133
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recordid: medline24263133
title: Fermi-LAT observations of the gamma-ray burst GRB 130427A
format: Article
creator:
  • Ackermann, M
  • Ajello, M
  • Asano, K
  • Atwood, W B
  • Axelsson, M
  • Baldini, L
  • Ballet, J
  • Barbiellini, G
  • Baring, M G
  • Bastieri, D
  • Bechtol, K
  • Bellazzini, R
  • Bissaldi, E
  • Bonamente, E
  • Bregeon, J
  • Brigida, M
  • Bruel, P
  • Buehler, R
  • Burgess, J Michael
  • Buson
subjects:
  • Gamma Rays -- Properties
  • Wave Motion -- Research
  • Luminosity (Astronomy) -- Research
ispartof: Science (New York, N.Y.), 03 January 2014, Vol.343(6166), pp.42-7
description: The 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 γ-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.
language: eng
source:
identifier: E-ISSN: 1095-9203 ; PMID: 24263133 Version:1 ; DOI: 10.1126/science.1242353
fulltext: no_fulltext
issn:
  • 10959203
  • 1095-9203
url: Link


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titleFermi-LAT observations of the gamma-ray burst GRB 130427A
creatorAckermann, M ; Ajello, M ; Asano, K ; Atwood, W B ; Axelsson, M ; Baldini, L ; Ballet, J ; Barbiellini, G ; Baring, M G ; Bastieri, D ; Bechtol, K ; Bellazzini, R ; Bissaldi, E ; Bonamente, E ; Bregeon, J ; Brigida, M ; Bruel, P ; Buehler, R ; Burgess, J Michael ; Buson
ispartofScience (New York, N.Y.), 03 January 2014, Vol.343(6166), pp.42-7
identifier
descriptionThe 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 γ-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.
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71Gruber, D
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titleFermi-LAT observations of the gamma-ray burst GRB 130427A
descriptionThe 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 γ-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.
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9Bastieri, D
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11Bellazzini, R
12Bissaldi, E
13Bonamente, E
14Bregeon, J
15Brigida, M
16Bruel, P
17Buehler, R
18Burgess, J Michael
19Buson, S
20Caliandro, G A
21Cameron, R A
22Caraveo, P A
23Cecchi, C
24Chaplin, V
25Charles, E
26Chekhtman, A
27Cheung, C C
28Chiang, J
29Chiaro, G
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32Cleveland, W
33Cohen-Tanugi, J
34Collazzi, A
35Cominsky, L R
36Connaughton, V
37Conrad, J
38Cutini, S
39D'Ammando, F
40De Angelis, A
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71Gruber, D
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79Hughes, R E
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82Jóhannesson, G
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85Knödlseder, J
86Kocevski, D
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89Larsson, S
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91Longo, F
92Loparco, F
93Lovellette, M N
94Lubrano, P
95Mayer, M
96Mazziotta, M N
97Mcenery, J E
98Michelson, P F
99Mizuno, T
100...
atitleFermi-LAT observations of the gamma-ray burst GRB 130427A
jtitleScience (New York, N.Y.)
risdate20140103
volume343
issue6166
spage42
pages42-47
issn0036-8075
eissn1095-9203
formatjournal
genrearticle
ristypeJOUR
abstractThe 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 γ-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.
doi10.1126/science.1242353
pmid24263133
date2014-01-03