A statistical study of high-energy emission of BATSE GRBs with COMPTEL and EGRET data
Journal Article
·
· AIP Conference Proceedings
- Space Research Institute, Profsojuznaya str. 84/32, 117810 Moscow (Russian Federation)
- Department of Physics, University of Alabama in Huntsville, Huntsville, Alabama 35899 (United States)
- NASA/Marshall Space Flight Center, Huntsville, Alabama 35812 (United States)
- Physics Department, University of Utah, Salt Lake City, Utah 84112 (United States)
- Space Science Center, University of New Hampshire, Durham, New Hampshire 03824 (United States)
- Space Sciences Laboratory, University of California, Berkeley, California 94720 (United States)
Using the peak aligned averaging method we analyze a subset of BATSE gamma-ray bursts (GRBs) with positions within the fields of view of the COMPTEL and EGRET instruments. We consider GRBs detected by the two telescopes as well as those individually undetected. With this averaging method we make a collective detection of GRBs that were undetected individually at high energies. The average temporal and spectral properties of bursts above 1 MeV are determined.
- OSTI ID:
- 21185790
- Journal Information:
- AIP Conference Proceedings, Vol. 428, Issue 1; Conference: 4. Huntsville gamma-ray burst symposium, Huntsville, AL (United States), 15-20 Sep 1997; Other Information: DOI: 10.1063/1.55341; (c) 1998 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
- Country of Publication:
- United States
- Language:
- English
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