scholarly journals Broadband Spectral Properties of Bright High‐Energy Gamma‐Ray Bursts Observed with BATSE and EGRET

2008 ◽  
Vol 677 (2) ◽  
pp. 1168-1183 ◽  
Author(s):  
Yuki Kaneko ◽  
M. Magdalena González ◽  
Robert D. Preece ◽  
Brenda L. Dingus ◽  
Michael S. Briggs
Author(s):  
M. Merck ◽  
D. L. Bertsch ◽  
B. L. Dingus ◽  
C. E. Fichtel ◽  
R. C. Hartman ◽  
...  

2009 ◽  
Vol 706 (2) ◽  
pp. 1152-1162 ◽  
Author(s):  
Hao-Ning He ◽  
Xiang-Yu Wang ◽  
Yun-Wei Yu ◽  
Peter Mészáros

2008 ◽  
Vol 34 (8) ◽  
pp. 509-514 ◽  
Author(s):  
V. B. Petkov ◽  
E. V. Bugaev ◽  
P. A. Klimai ◽  
M. V. Andreev ◽  
V. I. Volchenko ◽  
...  

2014 ◽  
Vol 28 ◽  
pp. 1460174
Author(s):  
PAK-HIN THOMAS TAM

The extended high-energy gamma-ray (>100 MeV) emission occurring after the prompt gamma-ray bursts (GRBs) is usually characterized by a single power-law spectrum, which has been explained as the afterglow synchrotron radiation. We report on the Fermi Large Area Telescope (LAT) observations of the >100 MeV emission from the very bright and nearby GRB 130427A, up to ~100 GeV. By performing time-resolved spectral fits of GRB 130427A, we found a strong evidence of an extra hard spectral component above a few GeV that exists in the extended high-energy emission of this GRB. This extra spectral component may represent the first clear evidence of the long sought-after afterglow inverse Compton emission. Prospects for observations at the very high-energy gamma-rays, i.e., above 100 GeV, are described.


1982 ◽  
Vol 83 (1-2) ◽  
pp. 279-286 ◽  
Author(s):  
R. W. Clay ◽  
P. R. Gerhardy ◽  
A. G. Gregory

2008 ◽  
Author(s):  
Kohta Murase ◽  
Kunihito Ioka ◽  
Shigehiro Nagataki ◽  
M. Galassi ◽  
David Palmer ◽  
...  

2005 ◽  
Vol 630 (2) ◽  
pp. 996-1002 ◽  
Author(s):  
R. Atkins ◽  
W. Benbow ◽  
D. Berley ◽  
E. Blaufuss ◽  
D. G. Coyne ◽  
...  

2000 ◽  
Vol 529 (2) ◽  
pp. 675-681 ◽  
Author(s):  
S. D. Bloom ◽  
J. Hallum ◽  
H. Terasranta ◽  
M. Tornikoski

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