Achievements of the ASTRO-E hard X-ray detector development

M. Tashiro; K. Makishima; T. Kamae; T. Murakami; T. Takahashi; Y. Fukazawa; M. Kokubun; K. Nakazawa; M. Nomachi; A. Yoshida; Y. Ezoe; N. Isobe; N. Iyomoto; J. Kataoka; J. Kotoku; M. Kouda; S. Kubo; A. Kubota; Y. Matsumoto; T. Mizuno; Y. Okada; N. Ota; H. Ozawa; G. Sato; M. Sugiho; M. Sugizaki; I. Takahashi; H. Takahashi; T. Tamura; C. Tanihata; Y. Terada; Y. Uchiyama; S. Watanabe; K. Yamaoka; D. Yonetoku

Achievements of the ASTRO-E hard X-ray detector development

M. Tashiro, K. Makishima, T. Kamae, T. Murakami, T. Takahashi, Y. Fukazawa, M. Kokubun, K. Nakazawa, M. Nomachi, A. Yoshida, Y. Ezoe, N. Isobe, N. Iyomoto, J. Kataoka, J. Kotoku, M. Kouda, S. Kubo, A. Kubota, Y. Matsumoto, T. MizunoY. Okada, N. Ota, H. Ozawa, G. Sato, M. Sugiho, M. Sugizaki, I. Takahashi, H. Takahashi, T. Tamura, C. Tanihata, Y. Terada, Y. Uchiyama, S. Watanabe, K. Yamaoka, D. Yonetoku

研究成果: Paper › 査読

抄録

The ASTRO-E Hard X-ray Detector utilized GSO/BGO well-type phoswich counters in compound-eye configuration [1], to achieve an extremely low background level of a few ×10^-5 counts s^-1cm^-2keV^-1. The GSO scintillators installed in the BGO active shield wells observes 30-600 keV photons, while silicon PIN diodes of 2 mm thick placed in front of each GSO crystal covers 10 - 60 keV photons with energy resolution of ∼3.5 keV FWHM. The design goals both of low background and high energy resolution in the hard X-ray bands were confirmed to be achieved through the preflight calibration experiments.

本文言語	English
ページ	483-486
ページ数	4
出版ステータス	Published - 2001
外部発表	はい
イベント	2001 IEEE Nuclear Science Symposium Conference Record - San Diege, CA, United States 継続期間: 2001 11月 4 → 2001 11月 10

Conference

Conference	2001 IEEE Nuclear Science Symposium Conference Record
国/地域	United States
City	San Diege, CA
Period	01/11/4 → 01/11/10

ASJC Scopus subject areas

放射線
核物理学および高エネルギー物理学
放射線学、核医学およびイメージング

他のファイルとリンク

引用スタイル

Tashiro, M., Makishima, K., Kamae, T., Murakami, T., Takahashi, T., Fukazawa, Y., Kokubun, M., Nakazawa, K., Nomachi, M., Yoshida, A., Ezoe, Y., Isobe, N., Iyomoto, N., Kataoka, J., Kotoku, J., Kouda, M., Kubo, S., Kubota, A., Matsumoto, Y., ... Yonetoku, D. (2001). Achievements of the ASTRO-E hard X-ray detector development. 483-486. Paper presented at 2001 IEEE Nuclear Science Symposium Conference Record, San Diege, CA, United States.

Tashiro, M, Makishima, K, Kamae, T, Murakami, T, Takahashi, T, Fukazawa, Y, Kokubun, M, Nakazawa, K, Nomachi, M, Yoshida, A, Ezoe, Y, Isobe, N, Iyomoto, N, Kataoka, J, Kotoku, J, Kouda, M, Kubo, S, Kubota, A, Matsumoto, Y, Mizuno, T, Okada, Y, Ota, N, Ozawa, H, Sato, G, Sugiho, M, Sugizaki, M, Takahashi, I, Takahashi, H, Tamura, T, Tanihata, C, Terada, Y, Uchiyama, Y, Watanabe, S, Yamaoka, K & Yonetoku, D 2001, 'Achievements of the ASTRO-E hard X-ray detector development', Paper presented at 2001 IEEE Nuclear Science Symposium Conference Record, San Diege, CA, United States, 01/11/4 - 01/11/10 pp. 483-486.

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abstract = "The ASTRO-E Hard X-ray Detector utilized GSO/BGO well-type phoswich counters in compound-eye configuration [1], to achieve an extremely low background level of a few ×10-5 counts s-1cm-2keV-1. The GSO scintillators installed in the BGO active shield wells observes 30-600 keV photons, while silicon PIN diodes of 2 mm thick placed in front of each GSO crystal covers 10 - 60 keV photons with energy resolution of ∼3.5 keV FWHM. The design goals both of low background and high energy resolution in the hard X-ray bands were confirmed to be achieved through the preflight calibration experiments.",

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author = "M. Tashiro and K. Makishima and T. Kamae and T. Murakami and T. Takahashi and Y. Fukazawa and M. Kokubun and K. Nakazawa and M. Nomachi and A. Yoshida and Y. Ezoe and N. Isobe and N. Iyomoto and J. Kataoka and J. Kotoku and M. Kouda and S. Kubo and A. Kubota and Y. Matsumoto and T. Mizuno and Y. Okada and N. Ota and H. Ozawa and G. Sato and M. Sugiho and M. Sugizaki and I. Takahashi and H. Takahashi and T. Tamura and C. Tanihata and Y. Terada and Y. Uchiyama and S. Watanabe and K. Yamaoka and D. Yonetoku",

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language = "English",

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AU - Tashiro, M.

AU - Makishima, K.

AU - Kamae, T.

AU - Murakami, T.

AU - Takahashi, T.

AU - Fukazawa, Y.

AU - Kokubun, M.

AU - Nakazawa, K.

AU - Nomachi, M.

AU - Yoshida, A.

AU - Ezoe, Y.

AU - Isobe, N.

AU - Iyomoto, N.

AU - Kataoka, J.

AU - Kotoku, J.

AU - Kouda, M.

AU - Kubo, S.

AU - Kubota, A.

AU - Matsumoto, Y.

AU - Mizuno, T.

AU - Okada, Y.

AU - Ota, N.

AU - Ozawa, H.

AU - Sato, G.

AU - Sugiho, M.

AU - Sugizaki, M.

AU - Takahashi, I.

AU - Takahashi, H.

AU - Tamura, T.

AU - Tanihata, C.

AU - Terada, Y.

AU - Uchiyama, Y.

AU - Watanabe, S.

AU - Yamaoka, K.

AU - Yonetoku, D.

PY - 2001

Y1 - 2001

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AB - The ASTRO-E Hard X-ray Detector utilized GSO/BGO well-type phoswich counters in compound-eye configuration [1], to achieve an extremely low background level of a few ×10-5 counts s-1cm-2keV-1. The GSO scintillators installed in the BGO active shield wells observes 30-600 keV photons, while silicon PIN diodes of 2 mm thick placed in front of each GSO crystal covers 10 - 60 keV photons with energy resolution of ∼3.5 keV FWHM. The design goals both of low background and high energy resolution in the hard X-ray bands were confirmed to be achieved through the preflight calibration experiments.

KW - ASTRO-E

KW - Hard X-ray detector

KW - Sensitivity

KW - Spectral response

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T2 - 2001 IEEE Nuclear Science Symposium Conference Record

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Achievements of the ASTRO-E hard X-ray detector development

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Conference

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