New Statistics of the Dimmest BATSE GRBs for Testing Cosmological Models

Details New Statistics of the Dimmest BATSE GRBs for Testing Cosmological Models New Statistics of the Dimmest BATSE GRBs for Testing Cosmological Models

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..312...35m&link_type=abstract

Third Rome Workshop on Gamma-Ray Bursts in the Afterglow Era ASP Conference Series, Volume 312, Proceedings of the conference he

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Cosmological models of the sources of gamma-ray bursts can be tested by comparing the model predictions with the observed burst intensity distribution. Strong testing of these models requires data on the intensity distribution of bursts over a wide intensity range, extending down to the dimmest bursts in the flux range <0.2 ph cm-2 s-1, which is well below the BATSE triggering threshold. We present new statistics of the dimmest gamma-ray bursts in this intensity range, which were obtained from 500 days of DISCLA data by a special project of post-flight detection.

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