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Paper: Two Years of GRB Observations with HETE-2/FREGATE
Volume: 312, Third Rome Workshop on Gamma-Ray Bursts in the Afterglow Era
Page: 12
Authors: Atteia, J.-L.; Barraud, C.; Lestrade, J. P.; Olive, J.-F.; Dezalay, J.-P.; Boer, M.; Hurley, K.; Jernigan, G.; Ricker, G.; Vanderspek, R.; Crew, G.; Doty, J.; Monnelly, G.; Villasenor, J.; Butler, N.; Levine, A.; Kawai, N.; Yoshida, A.; Sakamoto, T.; Tamagawa, T.; Torii, K.; Matsuoka, M.; Lamb, D.Q.; Donaghy, T.Q.; Graziani, C.; Pizzichini, G.; Fenimore, E.E.; Galassi, M.; Tavenner, T.
Abstract: 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 in 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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