Two years of GRB observations with HETE-2/FREGATE

Details Two years of GRB observations with HETE-2/FREGATE Two years of GRB observations with HETE-2/FREGATE

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..312...12a&link_type=abstract

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

Astronomy and Astrophysics

Astronomy

Scientific paper

We briefly describe the main parameters of the GRBs detected by FREGATE within its field of view during the first two years of its operation (October 2000 - November 2002). This sample includes classical GRBs, X-ray rich GRBs and Short/Hard GRBs. Thanks to the extensive follow-up of HETE-2 GRBs, these observations will allow on the long term to connect the properties of the prompt gamma-ray emission with those of the afterglow for all three types of GRBs.

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