Physics
Scientific paper
Aug 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....7.2751p&link_type=abstract
Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int
Physics
Scientific paper
In recent years much progress has been achieved in understanding the Gamma-Ray Burst phenomenon by means of the prompt observation of GRB afterglows and the identification of some GRB host galaxies. The number of events for which such observations were possible is however still small and does not allow statistical studies , which are instead possible on large numbers of events, such as the BATSE catalog. I shall show the results of a search for correlations betweeen spectral hardness, intensity, duration and spatial distribution of events. Events with low spectral hardness show evidence of belonging to a different class.
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