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Max-Planck-Institut für extraterrestrische Physik
- High-Energy Astrophysics -
Project: Fermi Gamma-ray Burst Monitor (GBM) |
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InstrumentThe GBM detector system consists of twelve single NaI detectors mounted in bunches of three detectors on each corner of the Fermi satellite and of two BGO detectors mounted on opposite sides of the spacecraft. The energy range covered by the NaI detectors is 10 keV to 1 MeV, and the range of the BGO is 150 keV to ∼30 MeV.
Last update: 2010-03-11 / 2022-01-29 by H. Steinle |
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© H. Steinle |