Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...203.8001b&link_type=abstract
American Astronomical Society Meeting 203, #80.01; Bulletin of the American Astronomical Society, Vol. 35, p.1330
Astronomy and Astrophysics
Astronomy
Scientific paper
The spectral and temporal correlations between gamma-ray bursts' hard X-ray ( ˜100 keV) and gamma-ray ( ˜1 GeV) emission will probe particle acceleration in different emitting regimes. GLAST's primary instrument, the Large Area Telescope (LAT) will be a pair-conversion detector sensitive in the 0.2-300 GeV energy band. The GLAST Burst Monitor (GBM) will be an array of 12 NaI and 2 BGO detectors covering the >10 keV to 25 MeV band; the GBM's purpose is to detect bursts and extend GLAST's energy coverage to bursts. We describe GLAST's burst operations, and present predictions for the burst detection rate.
Band David L.
GLAST GRB Team
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