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

S. Nakahira; K. Yamaoka; A. Yoshida; T. Doshida; K. Suzuki; S. Sugita; T. Oyama; Y. E. Nakagawa; H. Tomida; Shoji Torii

doi:10.1063/1.2943546

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

S. Nakahira, K. Yamaoka, A. Yoshida, T. Doshida, K. Suzuki, S. Sugita, T. Oyama, Y. E. Nakagawa, H. Tomida, Shoji Torii

研究成果: Conference contribution

1 引用（Scopus）

抜粋

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.

元の言語	English
ホスト出版物のタイトル	AIP Conference Proceedings
ページ	616-619
ページ数	4
巻	1000
DOI	https://doi.org/10.1063/1.2943546
出版物ステータス	Published - 2008
イベント	Santa Fe Conference on Gamma-Ray Bursts 2007, GRB 2007 - Santa Fe, NM 継続期間: 2007 11 5 → 2007 11 9

Other

Other	Santa Fe Conference on Gamma-Ray Bursts 2007, GRB 2007
市	Santa Fe, NM
期間	07/11/5 → 07/11/9

フィンガープリント

ASJC Scopus subject areas

Physics and Astronomy(all)

これを引用

Nakahira, S., Yamaoka, K., Yoshida, A., Doshida, T., Suzuki, K., Sugita, S., Oyama, T., Nakagawa, Y. E., Tomida, H., & Torii, S. (2008). Design and development of Gamma-ray Burst Monitor for the CALET Mission. ： AIP Conference Proceedings (巻 1000, pp. 616-619) https://doi.org/10.1063/1.2943546

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abstract = "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.",

author = "S. Nakahira and K. Yamaoka and A. Yoshida and T. Doshida and K. Suzuki and S. Sugita and T. Oyama and Nakagawa, {Y. E.} and H. Tomida and Shoji Torii",

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T1 - Design and development of Gamma-ray Burst Monitor for the CALET Mission

AU - Nakahira, S.

AU - Yamaoka, K.

AU - Yoshida, A.

AU - Doshida, T.

AU - Suzuki, K.

AU - Sugita, S.

AU - Oyama, T.

AU - Nakagawa, Y. E.

AU - Tomida, H.

AU - Torii, Shoji

PY - 2008

Y1 - 2008

N2 - 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.

AB - 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.

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M3 - Conference contribution

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BT - AIP Conference Proceedings

T2 - Santa Fe Conference on Gamma-Ray Bursts 2007, GRB 2007

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ER -

文献にアクセス

10.1063/1.2943546