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Statistical study of evolution of gamma-ray bursts detected by Apex/Phobos and BATSE/COMPTON instrumentsThe new method of statistical studying of cosmic gamma-ray bursts is presented based on the averaging of time profiles. The comparison is done between bright and dim events: while no differences were found between average flux curves, the hardness ratios pointed out the effect of hardness/brightness correlation.
Document ID
19950044483
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1016/0273-1177(94)00052-3
Authors
Mitrofanov, I. G. (Institute for Space Research Moscow, Russia)
Chernenko, A. M. (Institute for Space Research Moscow, Russia)
Pozanenko, A. S. (Institute for Space Research Moscow, Russia)
Fishman, G. J. (NASA Marshall Space Flight Center Huntsville, AL, US, United States)
Meegan, C. A. (NASA Marshall Space Flight Center Huntsville, AL, US, United States)
Briggs, M. S. (Univ. of Alabama, Huntsville, AL US, United States)
Paciesas, W. S. (Univ. of Alabama, Huntsville, AL US, United States)
Sagdeev, R. Z. (Univ. of Maryland, College Park, MD US, United States)
Date Acquired
August 16, 2013
Publication Date
May 1, 1995
Publication Information
Publication: Advances in Space Research
Volume: 15
Issue: 5
ISSN: 0273-1177
Subject Category
Astrophysics
Accession Number
95A76082
Distribution Limits
Public
Copyright
Other

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IDRelationTitle19950044457Collected WorksGamma Ray Astronomy; E2 Symposium of COSPAR Scientific Commission E, COSPAR Scientific Assembly, 30th, Hamburg, Germany, July 11-21, 1994
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