Expected Performance of the GLAST Burst Monitor
Autor: | Charles Meegan, Narayana Bhat, Elisabetta Bissaldi, Michael Briggs, Valerie Connaughton, Roland Diehl, Gerald Fishman, Jochen Greiner, Andreas von Kienlin, R. Marc Kippen, Chryssa Kouveliotou, Giselher Lichti, William Paciesas, Robert Preece, Helmut Steinle, Colleen Wilson-Hodge, M. Galassi, David Palmer, Ed Fenimore |
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Přispěvatelé: | M. Galassi , David Palmer and Ed Fenimore, Meegan, C., Bhat, N., Bissaldi, Elisabetta, Briggs, M., Connaughton, V., Diehl, R., Fishman, G., Greiner, J., von Kienlin, A., Kippen, R. M., Kouveliotou, C., Lichti, G., Paciesas, W., Preece, R., Steinle, H., Wilson Hodge, C. |
Rok vydání: | 2008 |
Předmět: |
Physics
Scintillation Photon Spacecraft Physics::Instrumentation and Detectors business.industry gamma-ray sources gamma-ray bursts Scintillation detectors X- and gamma-ray telescopes and instrumentation Astrophysics::High Energy Astrophysical Phenomena gamma-ray bursts Detector Field of view Astrophysics gamma-ray detectors Physics and Astronomy (all) Scintillation detector Optics Scintillation counter Measuring instrument Gamma-ray bursts business Gamma-ray burst gamma-ray sources gamma-ray sources gamma-ray burst |
Zdroj: | AIP Conference Proceedings. |
ISSN: | 0094-243X |
DOI: | 10.1063/1.2943535 |
Popis: | The GLAST Burst Monitor (GBM) will enhance LAT observations of GRBs by extending the spectral coverage from the LAT threshold down to 8 keV, and will provide a trigger for re-orienting the spacecraft to observe delayed emission from selected bursts outside the LAT field of view. GBM consists of twelve NaI scintillation detectors operating in the 8 keV to 1 MeV energy range and two BGO scintillation detectors operating in the 150 keV to 30 MeV energy range. Detector resolution, effective area, and angular response have been determined by calibrations. Analyses indicate that the on-board burst threshold will be 0.7 photons cm-2s-1 and the on-board burst localization accuracy will typically be better than 8deg. |
Databáze: | OpenAIRE |
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