Astro-E hard x-ray detector

Tsuneyoshi Kamae; Hajime Ezawa; Yasushi Fukazawa; Masaharu Hirayama; Eriko Idesawa; Naoko Iyomoto; Hidehiro Kaneda; G. Kawaguti; M. Kokubun; Hidetoshi Kubo; A. Kubota; Kyoko Matsushita; Keiichi Matsuzaki; Kazuo Makishima

Astro-E hard x-ray detector

Tsuneyoshi Kamae, Hajime Ezawa, Yasushi Fukazawa, Masaharu Hirayama, Eriko Idesawa, Naoko Iyomoto, Hidehiro Kaneda, G. Kawaguti, M. Kokubun, Hidetoshi Kubo, A. Kubota, Kyoko Matsushita, Keiichi Matsuzaki, Kazuo Makishima

研究成果: Conference contribution

13 被引用数 (Scopus)

抄録

Astro-E is the x-ray satellite to be launched in the year 2000 by Inst. of Space & Astronautical Science. This report deals with the design and expected performance of the hard x-ray detector (HXD), one of the 3 experiments aboard Astro-E. The HXD is a combination of GSO/BGO well-type phoswich counters and silicon PIN diodes: the two combined will cover a wide energy band of 10-700 keV. The detector is characterized by its low background of approximately 10 ^-5/s/cm ²/keV and its sensitivity higher than any past missions between a few 10 keV and several 100 keV. Combined with the other 2 experiments, a micro-calorimeter array (XRS) and 4 CCD arrays (XIS), both with x-ray mirrors, the mission will cover the soft and hard x-ray range at a highest sensitivity.

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
編集者	Brian D. Ramsey, Thomas A. Parnell
ページ	314-328
ページ数	15
出版ステータス	Published - 1996 12月 1
外部発表	はい
イベント	Gamma-Ray and Cosmic-Ray Detectors, Techniques, and Missions - Denver, CO, USA 継続期間: 1996 8月 5 → 1996 8月 7

出版物シリーズ

名前	Proceedings of SPIE - The International Society for Optical Engineering
巻	2806

Other

Other	Gamma-Ray and Cosmic-Ray Detectors, Techniques, and Missions
City	Denver, CO, USA
Period	96/8/5 → 96/8/7

ASJC Scopus subject areas

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

他のファイルとリンク

引用スタイル

Kamae, T., Ezawa, H., Fukazawa, Y., Hirayama, M., Idesawa, E., Iyomoto, N., Kaneda, H., Kawaguti, G., Kokubun, M., Kubo, H., Kubota, A., Matsushita, K., Matsuzaki, K., & Makishima, K. (1996). Astro-E hard x-ray detector. In B. D. Ramsey, & T. A. Parnell (Eds.), Proceedings of SPIE - The International Society for Optical Engineering (pp. 314-328). (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 2806).

Kamae, T, Ezawa, H, Fukazawa, Y, Hirayama, M, Idesawa, E, Iyomoto, N, Kaneda, H, Kawaguti, G, Kokubun, M, Kubo, H, Kubota, A, Matsushita, K, Matsuzaki, K & Makishima, K 1996, Astro-E hard x-ray detector. in BD Ramsey & TA Parnell (eds), Proceedings of SPIE - The International Society for Optical Engineering. Proceedings of SPIE - The International Society for Optical Engineering, vol. 2806, pp. 314-328, Gamma-Ray and Cosmic-Ray Detectors, Techniques, and Missions, Denver, CO, USA, 96/8/5.

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author = "Tsuneyoshi Kamae and Hajime Ezawa and Yasushi Fukazawa and Masaharu Hirayama and Eriko Idesawa and Naoko Iyomoto and Hidehiro Kaneda and G. Kawaguti and M. Kokubun and Hidetoshi Kubo and A. Kubota and Kyoko Matsushita and Keiichi Matsuzaki and Kazuo Makishima",

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AU - Ezawa, Hajime

AU - Fukazawa, Yasushi

AU - Hirayama, Masaharu

AU - Idesawa, Eriko

AU - Iyomoto, Naoko

AU - Kaneda, Hidehiro

AU - Kawaguti, G.

AU - Kokubun, M.

AU - Kubo, Hidetoshi

AU - Kubota, A.

AU - Matsushita, Kyoko

AU - Matsuzaki, Keiichi

AU - Makishima, Kazuo

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AB - Astro-E is the x-ray satellite to be launched in the year 2000 by Inst. of Space & Astronautical Science. This report deals with the design and expected performance of the hard x-ray detector (HXD), one of the 3 experiments aboard Astro-E. The HXD is a combination of GSO/BGO well-type phoswich counters and silicon PIN diodes: the two combined will cover a wide energy band of 10-700 keV. The detector is characterized by its low background of approximately 10 -5/s/cm 2/keV and its sensitivity higher than any past missions between a few 10 keV and several 100 keV. Combined with the other 2 experiments, a micro-calorimeter array (XRS) and 4 CCD arrays (XIS), both with x-ray mirrors, the mission will cover the soft and hard x-ray range at a highest sensitivity.

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M3 - Conference contribution

AN - SCOPUS:0030374669

SN - 0819421944

SN - 9780819421944

T3 - Proceedings of SPIE - The International Society for Optical Engineering

SP - 314

EP - 328

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

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T2 - Gamma-Ray and Cosmic-Ray Detectors, Techniques, and Missions

Y2 - 5 August 1996 through 7 August 1996

ER -

Astro-E hard x-ray detector

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ASJC Scopus subject areas

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