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.
Statistical study of evolution of gamma-ray bursts detected by Apex/Phobos and BATSE/COMPTON instruments
Advances in Space Research ; 15 , 5
1995-05-01
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Englisch
British Library Conference Proceedings | 1995
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