Measurements of Gamma-Ray Bursts (GRBs) with Glast
G. G. Lichti, M. Briggs, R. Diehl, G. Fishman, J. Greiner, R. M. Kippen, C. Kouveliotou, C. Meegan, W. Paciesas, R. Preece, V. Schoenfelder, A. von Kienlin
Abstract
One of the scientific goals of the main instrument of GLAST is the study of Gamma-Ray Bursts (GRBs) in the energy range from ~20 MeV to ~300 GeV. In order to extend the energy measurement towards lower energies a secondary instrument, the GLAST Burst Monitor (GBM), will measure GRBs from ~10 keV to ~25 MeV and will therefore allow the investigation of the relation between the keV and the MeV-GeV emission from GRBs over six energy decades. These unprecedented measurements will permit the exploration of the unknown aspects of the high-energy burst emission and the investigation of their connection with the well-studied low-energy emission. They will also provide ne insights into the physics of GRBs in general. In addition the excellent localization of GRBs by the LAT will stimulate follow-up observations at other wavelengths which may yield clues about the nature of the burst sources.
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