The CALET Gamma-ray Burst Monitor (CGBM)

@inproceedings{Yamaoka2011TheCG,
  title={The CALET Gamma-ray Burst Monitor (CGBM)},
  author={K. Yamaoka and A. Yoshida and T. Sakamoto and I. Takahashi and T. Hara and Tatsuma Yamamoto and Y. Kawakubo and R. Inoue and S. Terazawa and R. Fujioka and Kazumasa Senuma and S. Nakahira and H. Tomida and S. Ueno and S. Torii and M. Cherry and S. Ricciarini and The Calet Collaboration},
  year={2011}
}
The CALET Gamma-ray Burst Monitor (CGBM) is the secondary scientific instrument of the CALET mission to be attached to the ISS, sensitive to X and gamma-rays from 7 keV to 20 MeV. The scientific goal of the CGBM is to search out a clue to radiation mechanisms of gamma-ray bursts (GRBs) by obtaining very broadband spectra from optical to TeV gamma-rays together with the primary instrument, the calorimeter (CAL) sensitive to GeV-TeV gamma-rays, and the star camera (ASC). The CGBM sensor consists… Expand

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61(SP1): p.S35-S53 Figure 4: 137Cs spectra for LaBr3 (lower panel) and BGO (bottom panel) crystals with similar shape to the flight model. The energy resolution at 662 keV is 2.9±0.1
  • ApJ,
  • 2011