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THEFERMIGAMMA-RAY BURST MONITOR
2009
Astrophysical Journal
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The Gamma-Ray Burst Monitor (GBM) will significantly augment the science return from the Fermi Observatory in the study of Gamma-Ray Bursts (GRBs). The primary objective of GBM is to extend the energy range over which bursts are observed downward from the energy range of the Large Area Telescope (LAT) on Fermi into the hard X-ray range where extensive previous data exist. A secondary objective is to compute burst locations on-board to allow re-orientiong the spacecraft so that the LAT can
doi:10.1088/0004-637x/702/1/791
fatcat:afwvrersnraoflk25lzkz5vwl4