Statistical Properties of Gamma-Ray Bursts

Details Statistical Properties of Gamma-Ray Bursts Statistical Properties of Gamma-Ray Bursts

Apr 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999head....4.1402p&link_type=abstract

American Astronomical Society, HEAD meeting #4, #14.02; Bulletin of the American Astronomical Society, Vol. 31, p.711

Astronomy and Astrophysics

Astronomy

Scientific paper

Gamma-Ray Bursts from the BATSE catalog, available at www.batse.msfc.nasa.gov, have been divided into "classes" according to duration, hardness ratio and galactic latitude. Some selection criteria have been adopted, in order to avoid data affected by very large measurement errors and/or strong detection biases. The well known "bimodal" distribution in burst duration is quite evident, as well as differences in the intensity distributions of bursts with different hardness ratios and a weak indication of anisotropy both for the softer and harder events.

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