Statistical study of evolution of gamma-ray bursts detected by Apex/Phobos and BATSE/COMPTON instruments

Details Statistical study of evolution of gamma-ray bursts detected by Apex/Phobos and BATSE/COMPTON instruments Statistical study of evolution of gamma-ray bursts detected by Apex/Phobos and BATSE/COMPTON instruments

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995adspr..15q.131m&link_type=abstract

Advances in Space Research (ISSN 0273-1177), vol. 15, no. 5, p. (5)131-(5)134

Astronomy and Astrophysics

Astronomy

Brightness, Correlation, Gamma Ray Astronomy, Gamma Ray Bursts, Hardness, Ratios, Statistical Analysis, Temporal Distribution, Time Dependence, Astronomical Models, Energy Spectra, Gamma Ray Observatory, Interplanetary Spacecraft, Light Curve, Spaceborne Astronomy

Scientific paper

The 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.

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