Hardness Ratio and the Log N - Log P distribution of Gamma-Ray Bursts

Details Hardness Ratio and the Log N - Log P distribution of Gamma-Ray Bursts Hardness Ratio and the Log N - Log P distribution of Gamma-Ray Bursts

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...192.8505p&link_type=abstract

American Astronomical Society, 192nd AAS Meeting, #85.05; Bulletin of the American Astronomical Society, Vol. 30, p.1158

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The distribution of peak intensities in Gamma-Ray Bursts in the BATSE/CGRO catalog is different for events with different hardness ratios, namely for events with different ratios of 100 to 300 KeV to 50 to 100 KeV fluences. The much larger number of events available after years of continuous BATSE operation makes it now possible to use only bursts having reasonably small measurement errors for the quantities considered and to show that the change in the Log N - Log P curve for bursts with low hardness ratios is indeed more evident.

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