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arXiv · astro-ph/0109144

The GLAST Burst Monitor (GBM)

G. G. Lichti·M. S. Briggs·R. Diehl·G. Fishman·R. Georgii·R. M. Kippen·C. Kouveliotou·C. Meegan·W. Paciesas·R. Preece·V. Schoenfelder·A. von Kienlin
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Abstract

The selection of the GLAST burst monitor (GBM) by NASA will allow the investigation of the relation between the keV and the MeV-GeV emission from gamma-ray bursts. The GBM consists of 12 NaI and 2 BGO crystals allowing a continuous measurement of the energy spectra of gamma-ray bursts from ~5 keV to \~30 MeV. One feature of the GBM is its high time resolution for time-resolved gamma-ray spectroscopy. Moreover the arrangement of the NaI crystals allows a rapid on-board location (<15 degrees) of a gamma-ray burst within a FoV of ~8.6 sr. This position will be communicated to the main instrument of GLAST making follow-up observations at high energies possible.

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G. G. Lichti, M. S. Briggs, R. Diehl, G. Fishman, R. Georgii, R. M. Kippen, C. Kouveliotou, C. Meegan, W. Paciesas, R. Preece, V. Schoenfelder, A. von Kienlin. 2001-09-10. The GLAST Burst Monitor (GBM). https://arxiv.org/abs/astro-ph/0109144

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