The Hard X-ray Imager (HXI) for the ASTRO-H mission

Motohide Kokubun; Kazuhiro Nakazawa; Teruaki Enoto; Yasushi Fukazawa; Jun Kataoka; Madoka Kawaharada; Philippe Laurent; Francois Lebrun; Olivier Limousin; Kazuo Makishima; Tsunefumi Mizuno; Kunishiro Mori; Takeshi Nakamori; Hirokazu Odaka; Masanori Ohno; Masayuki Ohta; Goro Sato; Rie Sato; Hiroyasu Tajima; Hiromitsu Takahashi; Tadayuki Takahashi; Takaaki Tanaka; Yukikatsu Terada; Hideki Uchiyama; Yasunobu Uchiyama; Shin Watanabe; Yoichi Yatsu; Takayuki Yuasa

doi:10.1117/12.925648

The Hard X-ray Imager (HXI) for the ASTRO-H mission

Motohide Kokubun^*, Kazuhiro Nakazawa, Teruaki Enoto, Yasushi Fukazawa, Jun Kataoka, Madoka Kawaharada, Philippe Laurent, Francois Lebrun, Olivier Limousin, Kazuo Makishima, Tsunefumi Mizuno, Kunishiro Mori, Takeshi Nakamori, Hirokazu Odaka, Masanori Ohno, Masayuki Ohta, Goro Sato, Rie Sato, Hiroyasu Tajima, Hiromitsu TakahashiTadayuki Takahashi, Takaaki Tanaka, Yukikatsu Terada, Hideki Uchiyama, Yasunobu Uchiyama, Shin Watanabe, Yoichi Yatsu, Takayuki Yuasa

^*この研究の対応する著者

先進理工学部

研究成果: Conference contribution

28 被引用数 (Scopus)

抄録

The Hard X-ray Imager (HXI) is one of the four detectors on board the ASTRO-H mission (6th Japanese X-ray satellite), which is scheduled to be launched in 2014. Using the hybrid structure composed of double-sided silicon strip detectors and a cadmium telluride double-sided strip detector, both with a high spatial resolution of 250 μm. Combined with the hard X-ray telescope (HXT), it consists a hard X-ray imaging spectroscopic instrument covering the energy range from 5 to 80 keV with an effective area of >300 cm² in total at 30 keV. An energy resolution of 1-2 keV (FWHM) and lower threshold of 5 keV are both achieved with using a low noise front-end ASICs. In addition, the thick BGO active shields surrounding the main detector package is a heritage of the successful performance of the Hard X-ray Detector on board the Suzaku satellite. This feature enables the instrument to achieve an extremely good reduction of background caused by cosmic-ray particles, cosmic X-ray background, and in-orbit radiation activation. In this paper, we present the detector concept, design, latest results of the detector development, and the current status of the hardware.

本文言語	English
ホスト出版物のタイトル	Space Telescopes and Instrumentation 2012
ホスト出版物のサブタイトル	Ultraviolet to Gamma Ray
DOI	https://doi.org/10.1117/12.925648
出版ステータス	Published - 2012
イベント	Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray - Amsterdam, Netherlands 継続期間: 2012 7 1 → 2012 7 6

出版物シリーズ

名前	Proceedings of SPIE - The International Society for Optical Engineering
巻	8443
ISSN（印刷版）	0277-786X

Conference

Conference	Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray
国/地域	Netherlands
City	Amsterdam
Period	12/7/1 → 12/7/6

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

文献へのアクセス

10.1117/12.925648

他のファイルとリンク

引用スタイル

Kokubun, M., Nakazawa, K., Enoto, T., Fukazawa, Y., Kataoka, J., Kawaharada, M., Laurent, P., Lebrun, F., Limousin, O., Makishima, K., Mizuno, T., Mori, K., Nakamori, T., Odaka, H., Ohno, M., Ohta, M., Sato, G., Sato, R., Tajima, H., ... Yuasa, T. (2012). The Hard X-ray Imager (HXI) for the ASTRO-H mission. In Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray [844325] (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 8443). https://doi.org/10.1117/12.925648

The Hard X-ray Imager (HXI) for the ASTRO-H mission. / Kokubun, Motohide; Nakazawa, Kazuhiro; Enoto, Teruaki; Fukazawa, Yasushi; Kataoka, Jun; Kawaharada, Madoka; Laurent, Philippe; Lebrun, Francois; Limousin, Olivier; Makishima, Kazuo; Mizuno, Tsunefumi; Mori, Kunishiro; Nakamori, Takeshi; Odaka, Hirokazu; Ohno, Masanori; Ohta, Masayuki; Sato, Goro; Sato, Rie; Tajima, Hiroyasu; Takahashi, Hiromitsu; Takahashi, Tadayuki; Tanaka, Takaaki; Terada, Yukikatsu; Uchiyama, Hideki; Uchiyama, Yasunobu; Watanabe, Shin; Yatsu, Yoichi; Yuasa, Takayuki.

Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray. 2012. 844325 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 8443).

研究成果: Conference contribution

Kokubun, M, Nakazawa, K, Enoto, T, Fukazawa, Y, Kataoka, J, Kawaharada, M, Laurent, P, Lebrun, F, Limousin, O, Makishima, K, Mizuno, T, Mori, K, Nakamori, T, Odaka, H, Ohno, M, Ohta, M, Sato, G, Sato, R, Tajima, H, Takahashi, H, Takahashi, T, Tanaka, T, Terada, Y, Uchiyama, H, Uchiyama, Y, Watanabe, S, Yatsu, Y & Yuasa, T 2012, The Hard X-ray Imager (HXI) for the ASTRO-H mission. in Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray., 844325, Proceedings of SPIE - The International Society for Optical Engineering, vol. 8443, Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray, Amsterdam, Netherlands, 12/7/1. https://doi.org/10.1117/12.925648

Kokubun, Motohide ; Nakazawa, Kazuhiro ; Enoto, Teruaki ; Fukazawa, Yasushi ; Kataoka, Jun ; Kawaharada, Madoka ; Laurent, Philippe ; Lebrun, Francois ; Limousin, Olivier ; Makishima, Kazuo ; Mizuno, Tsunefumi ; Mori, Kunishiro ; Nakamori, Takeshi ; Odaka, Hirokazu ; Ohno, Masanori ; Ohta, Masayuki ; Sato, Goro ; Sato, Rie ; Tajima, Hiroyasu ; Takahashi, Hiromitsu ; Takahashi, Tadayuki ; Tanaka, Takaaki ; Terada, Yukikatsu ; Uchiyama, Hideki ; Uchiyama, Yasunobu ; Watanabe, Shin ; Yatsu, Yoichi ; Yuasa, Takayuki. / The Hard X-ray Imager (HXI) for the ASTRO-H mission. Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray. 2012. (Proceedings of SPIE - The International Society for Optical Engineering).

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abstract = "The Hard X-ray Imager (HXI) is one of the four detectors on board the ASTRO-H mission (6th Japanese X-ray satellite), which is scheduled to be launched in 2014. Using the hybrid structure composed of double-sided silicon strip detectors and a cadmium telluride double-sided strip detector, both with a high spatial resolution of 250 μm. Combined with the hard X-ray telescope (HXT), it consists a hard X-ray imaging spectroscopic instrument covering the energy range from 5 to 80 keV with an effective area of >300 cm2 in total at 30 keV. An energy resolution of 1-2 keV (FWHM) and lower threshold of 5 keV are both achieved with using a low noise front-end ASICs. In addition, the thick BGO active shields surrounding the main detector package is a heritage of the successful performance of the Hard X-ray Detector on board the Suzaku satellite. This feature enables the instrument to achieve an extremely good reduction of background caused by cosmic-ray particles, cosmic X-ray background, and in-orbit radiation activation. In this paper, we present the detector concept, design, latest results of the detector development, and the current status of the hardware.",

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AU - Kataoka, Jun

AU - Kawaharada, Madoka

AU - Laurent, Philippe

AU - Lebrun, Francois

AU - Limousin, Olivier

AU - Makishima, Kazuo

AU - Mizuno, Tsunefumi

AU - Mori, Kunishiro

AU - Nakamori, Takeshi

AU - Odaka, Hirokazu

AU - Ohno, Masanori

AU - Ohta, Masayuki

AU - Sato, Goro

AU - Sato, Rie

AU - Tajima, Hiroyasu

AU - Takahashi, Hiromitsu

AU - Takahashi, Tadayuki

AU - Tanaka, Takaaki

AU - Terada, Yukikatsu

AU - Uchiyama, Hideki

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The Hard X-ray Imager (HXI) for the ASTRO-H mission

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Conference

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