CAET Mission on the ISS

Shoji Torii; M. Hareyama; Nobuyuki Hasebe; K. Kasahara; S. Kobayashi; S. Kodaira; H. Murakami; Shunsuke Ozawa; S. Udo; N. Yamashita; K. Ebisawa; H. Fuke; J. Nishimura; Y. Saito; M. Takayanagi; H. Tomida; S. Ueno; T. Yamagami; K. Hibino; S. Okuno; T. Tamura; N. Tateyama; T. Kobayashi; T. Kotani; K. Yamaoka; A. Yoshida; Y. Shimizu; M. Takita; T. Yuda; Y. Katayose; M. Shibata; E. Kamioka; A. Kubota; K. Yoshida; M. Ichimura; S. Kuramata; Y. Tunesada; T. Terasawai; H. Kitamura; Y. Uchihori; Y. Komori; K. Mizutani; K. Munakata; A. Shiomi; J. W. Michell; A. J. Ericsson; T. Hams; J. F. Krizmanic; A. A. Moissev; M. Sasaki; J. F. Ormes; M. L. Cherry; T. G. Guzik; J. P. Wefel; W. R. Binns; M. H. Israel; H. Krawzczynski; P. S. Marrocchesi; M. G. Gagliesi; G. Bigongiari; A. Caldarone; M. Y. Kim; R. Cecchi; P. Maestro; V. Millucci; R. Zei; C. Avanzini; T. Avanzini; A. Messine; F. Morsani; O. Adriani; L. Bonechi; P. Papini; E. Vannuccini; J. Chan; W. Gan; T. Lu; Y. Ma; H. Wang; G. Chen

doi:10.1117/12.788524

CAET Mission on the ISS

Shoji Torii^*, M. Hareyama, Nobuyuki Hasebe, K. Kasahara, S. Kobayashi, S. Kodaira, H. Murakami, Shunsuke Ozawa, S. Udo, N. Yamashita, K. Ebisawa, H. Fuke, J. Nishimura, Y. Saito, M. Takayanagi, H. Tomida, S. Ueno, T. Yamagami, K. Hibino, S. OkunoT. Tamura, N. Tateyama, T. Kobayashi, T. Kotani, K. Yamaoka, A. Yoshida, Y. Shimizu, M. Takita, T. Yuda, Y. Katayose, M. Shibata, E. Kamioka, A. Kubota, K. Yoshida, M. Ichimura, S. Kuramata, Y. Tunesada, T. Terasawai, H. Kitamura, Y. Uchihori, Y. Komori, K. Mizutani, K. Munakata, A. Shiomi, J. W. Michell, A. J. Ericsson, T. Hams, J. F. Krizmanic, A. A. Moissev, M. Sasaki, J. F. Ormes, M. L. Cherry, T. G. Guzik, J. P. Wefel, W. R. Binns, M. H. Israel, H. Krawzczynski, P. S. Marrocchesi, M. G. Gagliesi, G. Bigongiari, A. Caldarone, M. Y. Kim, R. Cecchi, P. Maestro, V. Millucci, R. Zei, C. Avanzini, T. Avanzini, A. Messine, F. Morsani, O. Adriani, L. Bonechi, P. Papini, E. Vannuccini, J. Chan, W. Gan, T. Lu, Y. Ma, H. Wang, G. Chen

^*この研究の対応する著者

理工学術院総合研究所

研究成果: Conference contribution

9 被引用数 (Scopus)

抄録

We are developing the CALorimetric Electron Telescope, CALET, mission for the Japanese Experiment Module Exposed Facility, JEM-EF, of the International Space Station. Major scientific objectives are to search for the nearby cosmic ray sources and dark matter by carrying out a precise measurement of the electrons in 1 GeV - 20 TeV and gamma rays in 20 MeV - several 10 TeV. CALET has a unique capability to observe electrons and gamma rays over 1 TeV since the hadron rejection power can be larger than 105 and the energy resolution better than a few % over 100 GeV. The detector consists of an imaging calorimeter with scintillating fibers and tungsten plates and a total absorption calorimeter with BGO scintillators. CALET has also a capability to measure cosmic ray H, He and heavy ions up to 1000 TeV. It also will have a function to monitor solar activity and gamma ray transients. The phase A study has started on a schedule of launch in 2013 by H-II Transfer Vehicle (HTV) for 5 year observation.

本文言語	English
ホスト出版物のタイトル	Proceedings of SPIE - The International Society for Optical Engineering
巻	7021
DOI	https://doi.org/10.1117/12.788524
出版ステータス	Published - 2008
イベント	High Energy, Optical, and Infrared Detectors for Astronomy III - Marseille 継続期間: 2008 6月 23 → 2008 6月 26

Other

Other	High Energy, Optical, and Infrared Detectors for Astronomy III
City	Marseille
Period	08/6/23 → 08/6/26

ASJC Scopus subject areas

応用数学
コンピュータサイエンスの応用
電子工学および電気工学
電子材料、光学材料、および磁性材料
凝縮系物理学

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10.1117/12.788524

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Torii, S., Hareyama, M., Hasebe, N., Kasahara, K., Kobayashi, S., Kodaira, S., Murakami, H., Ozawa, S., Udo, S., Yamashita, N., Ebisawa, K., Fuke, H., Nishimura, J., Saito, Y., Takayanagi, M., Tomida, H., Ueno, S., Yamagami, T., Hibino, K., ... Chen, G. (2008). CAET Mission on the ISS. In Proceedings of SPIE - The International Society for Optical Engineering (Vol. 7021). [702114] https://doi.org/10.1117/12.788524

Torii, S, Hareyama, M, Hasebe, N, Kasahara, K, Kobayashi, S, Kodaira, S, Murakami, H, Ozawa, S, Udo, S, Yamashita, N, Ebisawa, K, Fuke, H, Nishimura, J, Saito, Y, Takayanagi, M, Tomida, H, Ueno, S, Yamagami, T, Hibino, K, Okuno, S, Tamura, T, Tateyama, N, Kobayashi, T, Kotani, T, Yamaoka, K, Yoshida, A, Shimizu, Y, Takita, M, Yuda, T, Katayose, Y, Shibata, M, Kamioka, E, Kubota, A, Yoshida, K, Ichimura, M, Kuramata, S, Tunesada, Y, Terasawai, T, Kitamura, H, Uchihori, Y, Komori, Y, Mizutani, K, Munakata, K, Shiomi, A, Michell, JW, Ericsson, AJ, Hams, T, Krizmanic, JF, Moissev, AA, Sasaki, M, Ormes, JF, Cherry, ML, Guzik, TG, Wefel, JP, Binns, WR, Israel, MH, Krawzczynski, H, Marrocchesi, PS, Gagliesi, MG, Bigongiari, G, Caldarone, A, Kim, MY, Cecchi, R, Maestro, P, Millucci, V, Zei, R, Avanzini, C, Avanzini, T, Messine, A, Morsani, F, Adriani, O, Bonechi, L, Papini, P, Vannuccini, E, Chan, J, Gan, W, Lu, T, Ma, Y, Wang, H & Chen, G 2008, CAET Mission on the ISS. in Proceedings of SPIE - The International Society for Optical Engineering. vol. 7021, 702114, High Energy, Optical, and Infrared Detectors for Astronomy III, Marseille, 08/6/23. https://doi.org/10.1117/12.788524

@inproceedings{6dfb4767cde64054875c4cd8686b15f1,

title = "CAET Mission on the ISS",

abstract = "We are developing the CALorimetric Electron Telescope, CALET, mission for the Japanese Experiment Module Exposed Facility, JEM-EF, of the International Space Station. Major scientific objectives are to search for the nearby cosmic ray sources and dark matter by carrying out a precise measurement of the electrons in 1 GeV - 20 TeV and gamma rays in 20 MeV - several 10 TeV. CALET has a unique capability to observe electrons and gamma rays over 1 TeV since the hadron rejection power can be larger than 105 and the energy resolution better than a few % over 100 GeV. The detector consists of an imaging calorimeter with scintillating fibers and tungsten plates and a total absorption calorimeter with BGO scintillators. CALET has also a capability to measure cosmic ray H, He and heavy ions up to 1000 TeV. It also will have a function to monitor solar activity and gamma ray transients. The phase A study has started on a schedule of launch in 2013 by H-II Transfer Vehicle (HTV) for 5 year observation.",

keywords = "Calorimeter, cosmic ray, Dark matter, Diffuse gamma ray, Gamma ray burst, High energy, ISS, Solar modulation",

author = "Shoji Torii and M. Hareyama and Nobuyuki Hasebe and K. Kasahara and S. Kobayashi and S. Kodaira and H. Murakami and Shunsuke Ozawa and S. Udo and N. Yamashita and K. Ebisawa and H. Fuke and J. Nishimura and Y. Saito and M. Takayanagi and H. Tomida and S. Ueno and T. Yamagami and K. Hibino and S. Okuno and T. Tamura and N. Tateyama and T. Kobayashi and T. Kotani and K. Yamaoka and A. Yoshida and Y. Shimizu and M. Takita and T. Yuda and Y. Katayose and M. Shibata and E. Kamioka and A. Kubota and K. Yoshida and M. Ichimura and S. Kuramata and Y. Tunesada and T. Terasawai and H. Kitamura and Y. Uchihori and Y. Komori and K. Mizutani and K. Munakata and A. Shiomi and Michell, {J. W.} and Ericsson, {A. J.} and T. Hams and Krizmanic, {J. F.} and Moissev, {A. A.} and M. Sasaki and Ormes, {J. F.} and Cherry, {M. L.} and Guzik, {T. G.} and Wefel, {J. P.} and Binns, {W. R.} and Israel, {M. H.} and H. Krawzczynski and Marrocchesi, {P. S.} and Gagliesi, {M. G.} and G. Bigongiari and A. Caldarone and Kim, {M. Y.} and R. Cecchi and P. Maestro and V. Millucci and R. Zei and C. Avanzini and T. Avanzini and A. Messine and F. Morsani and O. Adriani and L. Bonechi and P. Papini and E. Vannuccini and J. Chan and W. Gan and T. Lu and Y. Ma and H. Wang and G. Chen",

year = "2008",

doi = "10.1117/12.788524",

language = "English",

isbn = "9780819472311",

volume = "7021",

booktitle = "Proceedings of SPIE - The International Society for Optical Engineering",

note = "High Energy, Optical, and Infrared Detectors for Astronomy III ; Conference date: 23-06-2008 Through 26-06-2008",

}

TY - GEN

T1 - CAET Mission on the ISS

AU - Torii, Shoji

AU - Hareyama, M.

AU - Hasebe, Nobuyuki

AU - Kasahara, K.

AU - Kobayashi, S.

AU - Kodaira, S.

AU - Murakami, H.

AU - Ozawa, Shunsuke

AU - Udo, S.

AU - Yamashita, N.

AU - Ebisawa, K.

AU - Fuke, H.

AU - Nishimura, J.

AU - Saito, Y.

AU - Takayanagi, M.

AU - Tomida, H.

AU - Ueno, S.

AU - Yamagami, T.

AU - Hibino, K.

AU - Okuno, S.

AU - Tamura, T.

AU - Tateyama, N.

AU - Kobayashi, T.

AU - Kotani, T.

AU - Yamaoka, K.

AU - Yoshida, A.

AU - Shimizu, Y.

AU - Takita, M.

AU - Yuda, T.

AU - Katayose, Y.

AU - Shibata, M.

AU - Kamioka, E.

AU - Kubota, A.

AU - Yoshida, K.

AU - Ichimura, M.

AU - Kuramata, S.

AU - Tunesada, Y.

AU - Terasawai, T.

AU - Kitamura, H.

AU - Uchihori, Y.

AU - Komori, Y.

AU - Mizutani, K.

AU - Munakata, K.

AU - Shiomi, A.

AU - Michell, J. W.

AU - Ericsson, A. J.

AU - Hams, T.

AU - Krizmanic, J. F.

AU - Moissev, A. A.

AU - Sasaki, M.

AU - Ormes, J. F.

AU - Cherry, M. L.

AU - Guzik, T. G.

AU - Wefel, J. P.

AU - Binns, W. R.

AU - Israel, M. H.

AU - Krawzczynski, H.

AU - Marrocchesi, P. S.

AU - Gagliesi, M. G.

AU - Bigongiari, G.

AU - Caldarone, A.

AU - Kim, M. Y.

AU - Cecchi, R.

AU - Maestro, P.

AU - Millucci, V.

AU - Zei, R.

AU - Avanzini, C.

AU - Avanzini, T.

AU - Messine, A.

AU - Morsani, F.

AU - Adriani, O.

AU - Bonechi, L.

AU - Papini, P.

AU - Vannuccini, E.

AU - Chan, J.

AU - Gan, W.

AU - Lu, T.

AU - Ma, Y.

AU - Wang, H.

AU - Chen, G.

PY - 2008

Y1 - 2008

N2 - We are developing the CALorimetric Electron Telescope, CALET, mission for the Japanese Experiment Module Exposed Facility, JEM-EF, of the International Space Station. Major scientific objectives are to search for the nearby cosmic ray sources and dark matter by carrying out a precise measurement of the electrons in 1 GeV - 20 TeV and gamma rays in 20 MeV - several 10 TeV. CALET has a unique capability to observe electrons and gamma rays over 1 TeV since the hadron rejection power can be larger than 105 and the energy resolution better than a few % over 100 GeV. The detector consists of an imaging calorimeter with scintillating fibers and tungsten plates and a total absorption calorimeter with BGO scintillators. CALET has also a capability to measure cosmic ray H, He and heavy ions up to 1000 TeV. It also will have a function to monitor solar activity and gamma ray transients. The phase A study has started on a schedule of launch in 2013 by H-II Transfer Vehicle (HTV) for 5 year observation.

AB - We are developing the CALorimetric Electron Telescope, CALET, mission for the Japanese Experiment Module Exposed Facility, JEM-EF, of the International Space Station. Major scientific objectives are to search for the nearby cosmic ray sources and dark matter by carrying out a precise measurement of the electrons in 1 GeV - 20 TeV and gamma rays in 20 MeV - several 10 TeV. CALET has a unique capability to observe electrons and gamma rays over 1 TeV since the hadron rejection power can be larger than 105 and the energy resolution better than a few % over 100 GeV. The detector consists of an imaging calorimeter with scintillating fibers and tungsten plates and a total absorption calorimeter with BGO scintillators. CALET has also a capability to measure cosmic ray H, He and heavy ions up to 1000 TeV. It also will have a function to monitor solar activity and gamma ray transients. The phase A study has started on a schedule of launch in 2013 by H-II Transfer Vehicle (HTV) for 5 year observation.

KW - Calorimeter

KW - cosmic ray

KW - Dark matter

KW - Diffuse gamma ray

KW - Gamma ray burst

KW - High energy

KW - ISS

KW - Solar modulation

UR - http://www.scopus.com/inward/record.url?scp=66749125327&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=66749125327&partnerID=8YFLogxK

U2 - 10.1117/12.788524

DO - 10.1117/12.788524

M3 - Conference contribution

AN - SCOPUS:66749125327

SN - 9780819472311

VL - 7021

BT - Proceedings of SPIE - The International Society for Optical Engineering

T2 - High Energy, Optical, and Infrared Detectors for Astronomy III

Y2 - 23 June 2008 through 26 June 2008

ER -

CAET Mission on the ISS

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