On-Orbit Performance of the Fermi Gamma-Ray Burst Monitoi
- Universities Space Research Association 320 Sparkman Drive, Huntsville, AL 35805 (United States)
- University of Alabama Huntsville 320 Sparkman Drive, Huntsville, AL 35805 (United States)
- Max Planck Institute for Extraterrestrial Physics Garching (Germany)
- Marshall Space Flight Center, Mail Code VP62, 320 Sparkman Drive, Huntsville, AL 35805 (United States)
- Los Alamos National Laboratory Los Alamos, NM 87545 (United States)
The Fermi Gamma Ray Burst Monitor (GBM) enhances the science return from the Fermi mission by providing observations of GRBs in the energy range 8 keV to 40 MeV, thereby extending GRB spectra three decades below the Large Area Telescope (LAT) threshold of {approx}20 MeV. GBM employs twelve sodium iodide scintillation detectors and two bismuth germinate scintillation detectors to observe the full unocculted sky. The flight software localizes GRBs and can generate a request to autonomously repoint the spacecraft to place a burst within the LAT field of view. GBM has a trigger threshold of 0.74 photons-cm{sup -2}-s{sup -1} and triggers on {approx}260 bursts per year, as well as a variety of other gamma-ray transients.
- OSTI ID:
- 21308683
- Journal Information:
- AIP Conference Proceedings, Vol. 1133, Issue 1; Conference: 6. Huntsville symposium on gamma-ray burst, Huntsville, AL (United States), 20-23 Oct 2008; Other Information: DOI: 10.1063/1.3155975; (c) 2009 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
- Country of Publication:
- United States
- Language:
- English
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