Hard X-ray imager for the NeXT mission

Kazuhiro Nakazawa; Yasushi Fukazawa; Tuneyoshi Kamae; Jun Kataoka; Motohide Kokubun; Kazuo Makishima; Tsunefumi Mizuno; Toshio Murakami; Masaharu Nomachi; Hiroyasu Tajima; Tadayuki Takahashi; Makoto Tashiro; Toru Tamagawa; Yukikatsu Terada; Shin Watanabe; Kazutaka Yamaoka; Daisuke Yonetoku

doi:10.1117/12.670674

Hard X-ray imager for the NeXT mission

Kazuhiro Nakazawa, Yasushi Fukazawa, Tuneyoshi Kamae, Jun Kataoka, Motohide Kokubun, Kazuo Makishima, Tsunefumi Mizuno, Toshio Murakami, Masaharu Nomachi, Hiroyasu Tajima, Tadayuki Takahashi, Makoto Tashiro, Toru Tamagawa, Yukikatsu Terada, Shin Watanabe, Kazutaka Yamaoka, Daisuke Yonetoku

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

15 Citations (Scopus)

Abstract

The hard X-ray imager (HXI) is the primary detector of the NeXT mission, proposed to explore high-energy non-thermal phenomena in the universe. Combined with a novel hard X-ray mirror optics, the HXI is designed to provide better than arc-minutes imaging capability with 1 keV level spectroscopy, and more than 30 times higher sensitivity compared with any existing hard X-ray instruments. The base-line design of the HXI is improving to secure high sensitivity. The key is to reduce the detector background as far as possible. Based on the experience of the Suzaku satellite launched in July 2005, the current design has a well-type tight active shield and multi layered, multi material imaging detector made of Si and CdTe. Technology has been under development for a few years so that we have reached the level where a basic detector performance is satisfied. Design tuning to further improve the sensitivity and reliability is on-going.

Original language	English
Title of host publication	Space Telescopes and Instrumentation II
Subtitle of host publication	Ultraviolet to Gamma Ray
DOIs	https://doi.org/10.1117/12.670674
Publication status	Published - 2006 Oct 2
Externally published	Yes
Event	Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray - Orlando, FL, United States Duration: 2006 May 24 → 2006 May 31

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	6266 II
ISSN (Print)	0277-786X

Conference

Conference	Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray
Country	United States
City	Orlando, FL
Period	06/5/24 → 06/5/31

Keywords

CdTe
DSSD
Hard X-ray
X-ray Astronomy

ASJC Scopus subject areas

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

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10.1117/12.670674

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Nakazawa, K., Fukazawa, Y., Kamae, T., Kataoka, J., Kokubun, M., Makishima, K., Mizuno, T., Murakami, T., Nomachi, M., Tajima, H., Takahashi, T., Tashiro, M., Tamagawa, T., Terada, Y., Watanabe, S., Yamaoka, K., & Yonetoku, D. (2006). Hard X-ray imager for the NeXT mission. In Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray [62662H] (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 6266 II). https://doi.org/10.1117/12.670674

Hard X-ray imager for the NeXT mission. / Nakazawa, Kazuhiro; Fukazawa, Yasushi; Kamae, Tuneyoshi; Kataoka, Jun; Kokubun, Motohide; Makishima, Kazuo; Mizuno, Tsunefumi; Murakami, Toshio; Nomachi, Masaharu; Tajima, Hiroyasu; Takahashi, Tadayuki; Tashiro, Makoto; Tamagawa, Toru; Terada, Yukikatsu; Watanabe, Shin; Yamaoka, Kazutaka; Yonetoku, Daisuke.

Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray. 2006. 62662H (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 6266 II).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Nakazawa, K, Fukazawa, Y, Kamae, T, Kataoka, J, Kokubun, M, Makishima, K, Mizuno, T, Murakami, T, Nomachi, M, Tajima, H, Takahashi, T, Tashiro, M, Tamagawa, T, Terada, Y, Watanabe, S, Yamaoka, K & Yonetoku, D 2006, Hard X-ray imager for the NeXT mission. in Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray., 62662H, Proceedings of SPIE - The International Society for Optical Engineering, vol. 6266 II, Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray, Orlando, FL, United States, 06/5/24. https://doi.org/10.1117/12.670674

Nakazawa, Kazuhiro ; Fukazawa, Yasushi ; Kamae, Tuneyoshi ; Kataoka, Jun ; Kokubun, Motohide ; Makishima, Kazuo ; Mizuno, Tsunefumi ; Murakami, Toshio ; Nomachi, Masaharu ; Tajima, Hiroyasu ; Takahashi, Tadayuki ; Tashiro, Makoto ; Tamagawa, Toru ; Terada, Yukikatsu ; Watanabe, Shin ; Yamaoka, Kazutaka ; Yonetoku, Daisuke. / Hard X-ray imager for the NeXT mission. Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray. 2006. (Proceedings of SPIE - The International Society for Optical Engineering).

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abstract = "The hard X-ray imager (HXI) is the primary detector of the NeXT mission, proposed to explore high-energy non-thermal phenomena in the universe. Combined with a novel hard X-ray mirror optics, the HXI is designed to provide better than arc-minutes imaging capability with 1 keV level spectroscopy, and more than 30 times higher sensitivity compared with any existing hard X-ray instruments. The base-line design of the HXI is improving to secure high sensitivity. The key is to reduce the detector background as far as possible. Based on the experience of the Suzaku satellite launched in July 2005, the current design has a well-type tight active shield and multi layered, multi material imaging detector made of Si and CdTe. Technology has been under development for a few years so that we have reached the level where a basic detector performance is satisfied. Design tuning to further improve the sensitivity and reliability is on-going.",

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author = "Kazuhiro Nakazawa and Yasushi Fukazawa and Tuneyoshi Kamae and Jun Kataoka and Motohide Kokubun and Kazuo Makishima and Tsunefumi Mizuno and Toshio Murakami and Masaharu Nomachi and Hiroyasu Tajima and Tadayuki Takahashi and Makoto Tashiro and Toru Tamagawa and Yukikatsu Terada and Shin Watanabe and Kazutaka Yamaoka and Daisuke Yonetoku",

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AU - Nakazawa, Kazuhiro

AU - Fukazawa, Yasushi

AU - Kamae, Tuneyoshi

AU - Kataoka, Jun

AU - Kokubun, Motohide

AU - Makishima, Kazuo

AU - Mizuno, Tsunefumi

AU - Murakami, Toshio

AU - Nomachi, Masaharu

AU - Tajima, Hiroyasu

AU - Takahashi, Tadayuki

AU - Tashiro, Makoto

AU - Tamagawa, Toru

AU - Terada, Yukikatsu

AU - Watanabe, Shin

AU - Yamaoka, Kazutaka

AU - Yonetoku, Daisuke

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N2 - The hard X-ray imager (HXI) is the primary detector of the NeXT mission, proposed to explore high-energy non-thermal phenomena in the universe. Combined with a novel hard X-ray mirror optics, the HXI is designed to provide better than arc-minutes imaging capability with 1 keV level spectroscopy, and more than 30 times higher sensitivity compared with any existing hard X-ray instruments. The base-line design of the HXI is improving to secure high sensitivity. The key is to reduce the detector background as far as possible. Based on the experience of the Suzaku satellite launched in July 2005, the current design has a well-type tight active shield and multi layered, multi material imaging detector made of Si and CdTe. Technology has been under development for a few years so that we have reached the level where a basic detector performance is satisfied. Design tuning to further improve the sensitivity and reliability is on-going.

AB - The hard X-ray imager (HXI) is the primary detector of the NeXT mission, proposed to explore high-energy non-thermal phenomena in the universe. Combined with a novel hard X-ray mirror optics, the HXI is designed to provide better than arc-minutes imaging capability with 1 keV level spectroscopy, and more than 30 times higher sensitivity compared with any existing hard X-ray instruments. The base-line design of the HXI is improving to secure high sensitivity. The key is to reduce the detector background as far as possible. Based on the experience of the Suzaku satellite launched in July 2005, the current design has a well-type tight active shield and multi layered, multi material imaging detector made of Si and CdTe. Technology has been under development for a few years so that we have reached the level where a basic detector performance is satisfied. Design tuning to further improve the sensitivity and reliability is on-going.

KW - CdTe

KW - DSSD

KW - Hard X-ray

KW - X-ray Astronomy

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ER -

Hard X-ray imager for the NeXT mission

Abstract

Publication series

Conference

Keywords

ASJC Scopus subject areas

Access to Document

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