Observation of high-energy electron, gamma ray, and dark matter with CALET

K. Yoshida; S. Torii; T. Tamura; K. Kasahara; J. Chang; H. Fuke; K. Hibino; M. Ichimura; T. Kashiwagi; Y. Katayose; H. Kitamura; T. Kobayashi; Y. Komori; S. Kuramata; F. Makino; K. Mizutani; H. Murakami; J. Nishimura; S. Okuno; Y. Saito; M. Shibata; M. Takayanagi; N. Tateyama; T. Terasawa; S. Tomida; Y. Uchihori; S. Ueno; T. Yamagami; T. Yuda

Observation of high-energy electron, gamma ray, and dark matter with CALET

K. Yoshida, S. Torii, T. Tamura, K. Kasahara, J. Chang, H. Fuke, K. Hibino, M. Ichimura, T. Kashiwagi, Y. Katayose, H. Kitamura, T. Kobayashi, Y. Komori, S. Kuramata, F. Makino, K. Mizutani, H. Murakami, J. Nishimura, S. Okuno, Y. SaitoM. Shibata, M. Takayanagi, N. Tateyama, T. Terasawa, S. Tomida, Y. Uchihori, S. Ueno, T. Yamagami, T. Yuda

研究成果: Paper › 査読

抄録

We are proposing the CALET (CALorimetric Electron Telescope) for the observation of high-energy electrons and gamma rays at the Exposed Facility of the Japanese Experiment Module on the International Space Station. The CALET has a capability to observe electrons (+positrons) in 1GeV-10TeV and gamma rays in 20MeV- 10TeV with a high energy resolution of 2%@100GeV, an angular resolution of 0.06deg@100GeV, and a high proton rejection power of 10. CALET has the geometrical factor of nearly 1m-sr and three-years observation is expected. Precise electron observation of CALET enables us to identify cosmic-ray electron sources by the detection of distinctive features in the energy spectrum and anisotropy toward nearby sources. The ISS orbit enables CALET to survey all of the sky in a wide field of view of 2 sr without attitude control of the instrument. In addition, by the hybrid observations of high-energy electrons and gamma rays, the CALET can search for WIMP dark matter.

本文言語	English
ページ	337-340
ページ数	4
出版ステータス	Published - 2005 1月 1
イベント	29th International Cosmic Ray Conference, ICRC 2005 - Pune, India 継続期間: 2005 8月 3 → 2005 8月 10

Conference

Conference	29th International Cosmic Ray Conference, ICRC 2005
国/地域	India
City	Pune
Period	05/8/3 → 05/8/10

ASJC Scopus subject areas

核物理学および高エネルギー物理学

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引用スタイル

Yoshida, K., Torii, S., Tamura, T., Kasahara, K., Chang, J., Fuke, H., Hibino, K., Ichimura, M., Kashiwagi, T., Katayose, Y., Kitamura, H., Kobayashi, T., Komori, Y., Kuramata, S., Makino, F., Mizutani, K., Murakami, H., Nishimura, J., Okuno, S., ... Yuda, T. (2005). Observation of high-energy electron, gamma ray, and dark matter with CALET. 337-340. Paper presented at 29th International Cosmic Ray Conference, ICRC 2005, Pune, India.

Yoshida, K, Torii, S, Tamura, T, Kasahara, K, Chang, J, Fuke, H, Hibino, K, Ichimura, M, Kashiwagi, T, Katayose, Y, Kitamura, H, Kobayashi, T, Komori, Y, Kuramata, S, Makino, F, Mizutani, K, Murakami, H, Nishimura, J, Okuno, S, Saito, Y, Shibata, M, Takayanagi, M, Tateyama, N, Terasawa, T, Tomida, S, Uchihori, Y, Ueno, S, Yamagami, T & Yuda, T 2005, 'Observation of high-energy electron, gamma ray, and dark matter with CALET', Paper presented at 29th International Cosmic Ray Conference, ICRC 2005, Pune, India, 05/8/3 - 05/8/10 pp. 337-340.

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title = "Observation of high-energy electron, gamma ray, and dark matter with CALET",

abstract = "We are proposing the CALET (CALorimetric Electron Telescope) for the observation of high-energy electrons and gamma rays at the Exposed Facility of the Japanese Experiment Module on the International Space Station. The CALET has a capability to observe electrons (+positrons) in 1GeV-10TeV and gamma rays in 20MeV- 10TeV with a high energy resolution of 2%@100GeV, an angular resolution of 0.06deg@100GeV, and a high proton rejection power of 10. CALET has the geometrical factor of nearly 1m-sr and three-years observation is expected. Precise electron observation of CALET enables us to identify cosmic-ray electron sources by the detection of distinctive features in the energy spectrum and anisotropy toward nearby sources. The ISS orbit enables CALET to survey all of the sky in a wide field of view of 2 sr without attitude control of the instrument. In addition, by the hybrid observations of high-energy electrons and gamma rays, the CALET can search for WIMP dark matter.",

author = "K. Yoshida and S. Torii and T. Tamura and K. Kasahara and J. Chang and H. Fuke and K. Hibino and M. Ichimura and T. Kashiwagi and Y. Katayose and H. Kitamura and T. Kobayashi and Y. Komori and S. Kuramata and F. Makino and K. Mizutani and H. Murakami and J. Nishimura and S. Okuno and Y. Saito and M. Shibata and M. Takayanagi and N. Tateyama and T. Terasawa and S. Tomida and Y. Uchihori and S. Ueno and T. Yamagami and T. Yuda",

year = "2005",

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language = "English",

pages = "337--340",

note = "29th International Cosmic Ray Conference, ICRC 2005 ; Conference date: 03-08-2005 Through 10-08-2005",

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TY - CONF

T1 - Observation of high-energy electron, gamma ray, and dark matter with CALET

AU - Yoshida, K.

AU - Torii, S.

AU - Tamura, T.

AU - Kasahara, K.

AU - Chang, J.

AU - Fuke, H.

AU - Hibino, K.

AU - Ichimura, M.

AU - Kashiwagi, T.

AU - Katayose, Y.

AU - Kitamura, H.

AU - Kobayashi, T.

AU - Komori, Y.

AU - Kuramata, S.

AU - Makino, F.

AU - Mizutani, K.

AU - Murakami, H.

AU - Nishimura, J.

AU - Okuno, S.

AU - Saito, Y.

AU - Shibata, M.

AU - Takayanagi, M.

AU - Tateyama, N.

AU - Terasawa, T.

AU - Tomida, S.

AU - Uchihori, Y.

AU - Ueno, S.

AU - Yamagami, T.

AU - Yuda, T.

PY - 2005/1/1

Y1 - 2005/1/1

N2 - We are proposing the CALET (CALorimetric Electron Telescope) for the observation of high-energy electrons and gamma rays at the Exposed Facility of the Japanese Experiment Module on the International Space Station. The CALET has a capability to observe electrons (+positrons) in 1GeV-10TeV and gamma rays in 20MeV- 10TeV with a high energy resolution of 2%@100GeV, an angular resolution of 0.06deg@100GeV, and a high proton rejection power of 10. CALET has the geometrical factor of nearly 1m-sr and three-years observation is expected. Precise electron observation of CALET enables us to identify cosmic-ray electron sources by the detection of distinctive features in the energy spectrum and anisotropy toward nearby sources. The ISS orbit enables CALET to survey all of the sky in a wide field of view of 2 sr without attitude control of the instrument. In addition, by the hybrid observations of high-energy electrons and gamma rays, the CALET can search for WIMP dark matter.

AB - We are proposing the CALET (CALorimetric Electron Telescope) for the observation of high-energy electrons and gamma rays at the Exposed Facility of the Japanese Experiment Module on the International Space Station. The CALET has a capability to observe electrons (+positrons) in 1GeV-10TeV and gamma rays in 20MeV- 10TeV with a high energy resolution of 2%@100GeV, an angular resolution of 0.06deg@100GeV, and a high proton rejection power of 10. CALET has the geometrical factor of nearly 1m-sr and three-years observation is expected. Precise electron observation of CALET enables us to identify cosmic-ray electron sources by the detection of distinctive features in the energy spectrum and anisotropy toward nearby sources. The ISS orbit enables CALET to survey all of the sky in a wide field of view of 2 sr without attitude control of the instrument. In addition, by the hybrid observations of high-energy electrons and gamma rays, the CALET can search for WIMP dark matter.

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M3 - Paper

AN - SCOPUS:84898978578

SP - 337

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T2 - 29th International Cosmic Ray Conference, ICRC 2005

Y2 - 3 August 2005 through 10 August 2005

ER -

Observation of high-energy electron, gamma ray, and dark matter with CALET

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Conference

ASJC Scopus subject areas

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