Monitoring of high energy X-ray sources with the BeppoSAX GRBM

Details Monitoring of high energy X-ray sources with the BeppoSAX GRBM Monitoring of high energy X-ray sources with the BeppoSAX GRBM

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999nuphs..69..664g&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 69, Issue 1-3, p. 664-667.

Physics

Nuclear Physics

Scientific paper

The Gamma-Ray Burst Monitor (GRBM) aboard the BeppoSAX satellite has already shown good capabilities in the detection of Gamma-Ray Bursts (GRB). We have also tested its performance as monitor of the hard X-ray flux from strong celestial sources, using the Earth Occultation Technique. A verification of the on-ground calibrations of the instrument was performed deriving the flux of the Crab Nebula. In this paper we report results on Crab and light curves of other sources detected.

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