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

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

doi:10.1117/12.857933

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

Motohide Kokubun^*, Kazuhiro Nakazawa, Teruaki Enoto, Yasushi Fukazawa, Kirk Gilmore, Jun Kataoka, Madoka Kawaharada, Philippe Laurent, Francois Lebrun, Olivier Limousin, Kazuo Makishima, Tsunefumi Mizuno, Kunishiro Mori, Takeshi Nakamori, Masanori Ohno, Masayuki Ohta, Goro Sato, Hiroyasu Tajima, Hiromitsu Takahashi, Tadayuki TakahashiTakaaki Tanaka, Yukikatsu Terada, Hideki Uchiyama, Yasunobu Uchiyama, Shin Watanabe, Yoichi Yatsu, Kazutaka Yamaoka

^*この研究の対応する著者

先進理工学部

研究成果: Conference contribution

37 被引用数 (Scopus)

抄録

The Hard X-ray Imager (HXI) is one of 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, the instrument fully covers the energy range of photons collected with the hard X-ray telescope up to 80 keV with a high quantum efficiency. High spatial resolution of 250 μm and an energy resolution of 1-2 keV (FWHM) are both achieved with 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 high background reduction 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 2010
ホスト出版物のサブタイトル	Ultraviolet to Gamma Ray
DOI	https://doi.org/10.1117/12.857933
出版ステータス	Published - 2010
イベント	Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray - San Diego, CA, United States 継続期間: 2010 6月 28 → 2010 7月 2

出版物シリーズ

名前	Proceedings of SPIE - The International Society for Optical Engineering
巻	7732
ISSN（印刷版）	0277-786X

Conference

Conference	Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray
国/地域	United States
City	San Diego, CA
Period	10/6/28 → 10/7/2

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

10.1117/12.857933

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引用スタイル

Kokubun, M., Nakazawa, K., Enoto, T., Fukazawa, Y., Gilmore, K., Kataoka, J., Kawaharada, M., Laurent, P., Lebrun, F., Limousin, O., Makishima, K., Mizuno, T., Mori, K., Nakamori, T., Ohno, M., Ohta, M., Sato, G., Tajima, H., Takahashi, H., ... Yamaoka, K. (2010). Hard X-ray Imager (HXI) for the ASTRO-H mission. In Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray [773215] (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 7732). https://doi.org/10.1117/12.857933

Kokubun, M, Nakazawa, K, Enoto, T, Fukazawa, Y, Gilmore, K, Kataoka, J, Kawaharada, M, Laurent, P, Lebrun, F, Limousin, O, Makishima, K, Mizuno, T, Mori, K, Nakamori, T, Ohno, M, Ohta, M, Sato, G, Tajima, H, Takahashi, H, Takahashi, T, Tanaka, T, Terada, Y, Uchiyama, H, Uchiyama, Y, Watanabe, S, Yatsu, Y & Yamaoka, K 2010, Hard X-ray Imager (HXI) for the ASTRO-H mission. in Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray., 773215, Proceedings of SPIE - The International Society for Optical Engineering, vol. 7732, Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray, San Diego, CA, United States, 10/6/28. https://doi.org/10.1117/12.857933

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title = "Hard X-ray Imager (HXI) for the ASTRO-H mission",

abstract = "The Hard X-ray Imager (HXI) is one of 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, the instrument fully covers the energy range of photons collected with the hard X-ray telescope up to 80 keV with a high quantum efficiency. High spatial resolution of 250 μm and an energy resolution of 1-2 keV (FWHM) are both achieved with 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 high background reduction 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 - Kokubun, Motohide

AU - Nakazawa, Kazuhiro

AU - Enoto, Teruaki

AU - Fukazawa, Yasushi

AU - Gilmore, Kirk

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 - Ohno, Masanori

AU - Ohta, Masayuki

AU - Sato, Goro

AU - Tajima, Hiroyasu

AU - Takahashi, Hiromitsu

AU - Takahashi, Tadayuki

AU - Tanaka, Takaaki

AU - Terada, Yukikatsu

AU - Uchiyama, Hideki

AU - Uchiyama, Yasunobu

AU - Watanabe, Shin

AU - Yatsu, Yoichi

AU - Yamaoka, Kazutaka

PY - 2010

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N2 - The Hard X-ray Imager (HXI) is one of 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, the instrument fully covers the energy range of photons collected with the hard X-ray telescope up to 80 keV with a high quantum efficiency. High spatial resolution of 250 μm and an energy resolution of 1-2 keV (FWHM) are both achieved with 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 high background reduction 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.

AB - The Hard X-ray Imager (HXI) is one of 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, the instrument fully covers the energy range of photons collected with the hard X-ray telescope up to 80 keV with a high quantum efficiency. High spatial resolution of 250 μm and an energy resolution of 1-2 keV (FWHM) are both achieved with 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 high background reduction 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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T2 - Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray

Y2 - 28 June 2010 through 2 July 2010

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

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Conference

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