GLAST's Sensitivity to Gamma-Ray Bursts

Details GLAST's Sensitivity to Gamma-Ray Bursts GLAST's Sensitivity to Gamma-Ray Bursts

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006head....9.1318b&link_type=abstract

American Astronomical Society, HEAD meeting #9, #13.18; Bulletin of the American Astronomical Society, Vol. 38, p.369

Astronomy and Astrophysics

Astronomy

Scientific paper

The Gamma-ray Large Area Space Telescope (GLAST) will advance the study of gamma-ray bursts. The spectral coverage of more than 7 energy decades and large fields-of-view of the Large Area Telescope (LAT; 20 MeV to >300 GeV) and the GLAST Burst Monitor (GBM; 10 keV to 30 GeV) will result in unprecedented spectral and temporal coverage of a large number of bursts. In addition, both detectors will localize the bursts. Semi-analytic calculations can characterize the burst populations to which each instrument will be sensitive.

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