Published May 22, 2008 | Version v1
Journal article

Design and development of Gamma-ray Burst Monitor for the CALET Mission

  • 1. Department of Physics and Mathematics, Aoyama Gakuin University (Japan)
  • 2. ISS Science Project Team, Institute of Space and Astronautional Science (ISAS), Japan Aerospace Exploration Agency (JAXA) (Japan)
  • 3. Research Institute for Science and Engineering, Waseda University (Japan)

Description

We propose to provide a gamma-ray burst monitor (GBM) for the CALET mission to monitor gamma-ray bursts (GRBs) together with the CALET Imaging Calorimeter detector. The major purpose is to derive a wide-band energy spectrum of GRBs over an unprecedented 9 decades of energy (from a few keV to a few TeV) in combination with the CALET tower detector. Hence it is desirable to have the CALET-GBM covering an energy range from a few keV to about 20 MeV to avoid a gap in the observational energy bands. The design of GBM is underway to fulfill this requirement. The current detector candidate is BGO, and a LaBr (Ce) scintillator which has a superior energy resolution to that of NaI(Tl). In this paper, design and expected performance of the CALET-GBM is shown

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1000
Journal Issue
1
Journal Page Range
p. 616-619
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
Santa Fe conference on gamma-ray bursts 2007
Dates
5-9 Nov 2007
Place
Santa Fe, NM (United States)

Optional Information

Notes
(c) 2008 American Institute of Physics