Development status and simulation study of monitor of all-sky x-ray image (MAXI) mission

Hiroshi Tomida; Masaru Matsuoka; Kazuyoshi Kawasaki; Shiro Ueno; Yasuki Adachi; Mitsuhiro Kohama; Motoko Suzuki; Masaki Ishikawa; Haruyoshi Katayama; Tatehiro Mihara; Mutsumi Sugizaki; Naoki Isobe; Hiroshi Tsunemi; Emi Miyata; Nobuyuki Kawai; Jun Kataoka; Atsumasa Yoshida; Kazutaka Yamaoka; Hitoshi Negoro; Motoki Nakajima; Yoshihiro Ueda; Satochi Eguchi; Mikio Morii

doi:10.1117/12.788833

Development status and simulation study of monitor of all-sky x-ray image (MAXI) mission

Hiroshi Tomida, Masaru Matsuoka, Kazuyoshi Kawasaki, Shiro Ueno, Yasuki Adachi, Mitsuhiro Kohama, Motoko Suzuki, Masaki Ishikawa, Haruyoshi Katayama, Tatehiro Mihara, Mutsumi Sugizaki, Naoki Isobe, Hiroshi Tsunemi, Emi Miyata, Nobuyuki Kawai, Jun Kataoka, Atsumasa Yoshida, Kazutaka Yamaoka, Hitoshi Negoro, Motoki NakajimaYoshihiro Ueda, Satochi Eguchi, Mikio Morii

先進理工学部

研究成果: Conference contribution

抜粋

MAXI (Monitor of All-sky X-ray Image) is a payload on board the International Space Station, and will be launched on April 2009. We report on the current development status on MAXI, in particular on the two types of X-ray camera (GSC and SSC), and the simulation results of the MAXI observation. SSC is a CCD camera. The moderate energy resolution enables us to detect the various emission peak including 0.5 keV oxygen line. The averaged energy resolution at the CCD temperature of -70 deg is 144.5 eV (FWHM) for 5.9 keV X-ray. GSC includes proportional gas counters, which have large X-ray detection area (5350cm²). The averaged position resolution of 1.1mm at 8 keV enable us to determined the celestial position of bright sources within the accuracy of 0.1 degree. The simulation study involving the results of performance test exhibits the high sensitivity of MAXI as designed.

元の言語	English
ホスト出版物のタイトル	Space Telescopes and Instrumentation 2008
ホスト出版物のサブタイトル	Ultraviolet to Gamma Ray
DOI	https://doi.org/10.1117/12.788833
出版物ステータス	Published - 2008 12 1
イベント	Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray - Marseille, France 継続期間: 2008 6 23 → 2008 6 28

出版物シリーズ

名前	Proceedings of SPIE - The International Society for Optical Engineering
巻	7011
ISSN（印刷物）	0277-786X

Conference

Conference	Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray
国	France
市	Marseille
期間	08/6/23 → 08/6/28

ASJC Scopus subject areas

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

文献にアクセス

10.1117/12.788833

フィンガープリント Development status and simulation study of monitor of all-sky x-ray image (MAXI) mission' の研究トピックを掘り下げます。これらはともに一意のフィンガープリントを構成します。

これを引用

Tomida, H., Matsuoka, M., Kawasaki, K., Ueno, S., Adachi, Y., Kohama, M., Suzuki, M., Ishikawa, M., Katayama, H., Mihara, T., Sugizaki, M., Isobe, N., Tsunemi, H., Miyata, E., Kawai, N., Kataoka, J., Yoshida, A., Yamaoka, K., Negoro, H., ... Morii, M. (2008). Development status and simulation study of monitor of all-sky x-ray image (MAXI) mission. ： Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray [70112R] (Proceedings of SPIE - The International Society for Optical Engineering; 巻数 7011). https://doi.org/10.1117/12.788833

Development status and simulation study of monitor of all-sky x-ray image (MAXI) mission. / Tomida, Hiroshi; Matsuoka, Masaru; Kawasaki, Kazuyoshi; Ueno, Shiro; Adachi, Yasuki; Kohama, Mitsuhiro; Suzuki, Motoko; Ishikawa, Masaki; Katayama, Haruyoshi; Mihara, Tatehiro; Sugizaki, Mutsumi; Isobe, Naoki; Tsunemi, Hiroshi; Miyata, Emi; Kawai, Nobuyuki; Kataoka, Jun; Yoshida, Atsumasa; Yamaoka, Kazutaka; Negoro, Hitoshi; Nakajima, Motoki; Ueda, Yoshihiro; Eguchi, Satochi; Morii, Mikio.

Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray. 2008. 70112R (Proceedings of SPIE - The International Society for Optical Engineering; 巻 7011).

研究成果: Conference contribution

Tomida, H, Matsuoka, M, Kawasaki, K, Ueno, S, Adachi, Y, Kohama, M, Suzuki, M, Ishikawa, M, Katayama, H, Mihara, T, Sugizaki, M, Isobe, N, Tsunemi, H, Miyata, E, Kawai, N, Kataoka, J, Yoshida, A, Yamaoka, K, Negoro, H, Nakajima, M, Ueda, Y, Eguchi, S & Morii, M 2008, Development status and simulation study of monitor of all-sky x-ray image (MAXI) mission. ： Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray., 70112R, Proceedings of SPIE - The International Society for Optical Engineering, 巻. 7011, Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray, Marseille, France, 08/6/23. https://doi.org/10.1117/12.788833

Tomida, Hiroshi ; Matsuoka, Masaru ; Kawasaki, Kazuyoshi ; Ueno, Shiro ; Adachi, Yasuki ; Kohama, Mitsuhiro ; Suzuki, Motoko ; Ishikawa, Masaki ; Katayama, Haruyoshi ; Mihara, Tatehiro ; Sugizaki, Mutsumi ; Isobe, Naoki ; Tsunemi, Hiroshi ; Miyata, Emi ; Kawai, Nobuyuki ; Kataoka, Jun ; Yoshida, Atsumasa ; Yamaoka, Kazutaka ; Negoro, Hitoshi ; Nakajima, Motoki ; Ueda, Yoshihiro ; Eguchi, Satochi ; Morii, Mikio. / Development status and simulation study of monitor of all-sky x-ray image (MAXI) mission. Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray. 2008. (Proceedings of SPIE - The International Society for Optical Engineering).

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abstract = "MAXI (Monitor of All-sky X-ray Image) is a payload on board the International Space Station, and will be launched on April 2009. We report on the current development status on MAXI, in particular on the two types of X-ray camera (GSC and SSC), and the simulation results of the MAXI observation. SSC is a CCD camera. The moderate energy resolution enables us to detect the various emission peak including 0.5 keV oxygen line. The averaged energy resolution at the CCD temperature of -70 deg is 144.5 eV (FWHM) for 5.9 keV X-ray. GSC includes proportional gas counters, which have large X-ray detection area (5350cm2). The averaged position resolution of 1.1mm at 8 keV enable us to determined the celestial position of bright sources within the accuracy of 0.1 degree. The simulation study involving the results of performance test exhibits the high sensitivity of MAXI as designed.",

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AU - Tomida, Hiroshi

AU - Matsuoka, Masaru

AU - Kawasaki, Kazuyoshi

AU - Ueno, Shiro

AU - Adachi, Yasuki

AU - Kohama, Mitsuhiro

AU - Suzuki, Motoko

AU - Ishikawa, Masaki

AU - Katayama, Haruyoshi

AU - Mihara, Tatehiro

AU - Sugizaki, Mutsumi

AU - Isobe, Naoki

AU - Tsunemi, Hiroshi

AU - Miyata, Emi

AU - Kawai, Nobuyuki

AU - Kataoka, Jun

AU - Yoshida, Atsumasa

AU - Yamaoka, Kazutaka

AU - Negoro, Hitoshi

AU - Nakajima, Motoki

AU - Ueda, Yoshihiro

AU - Eguchi, Satochi

AU - Morii, Mikio

PY - 2008/12/1

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AB - MAXI (Monitor of All-sky X-ray Image) is a payload on board the International Space Station, and will be launched on April 2009. We report on the current development status on MAXI, in particular on the two types of X-ray camera (GSC and SSC), and the simulation results of the MAXI observation. SSC is a CCD camera. The moderate energy resolution enables us to detect the various emission peak including 0.5 keV oxygen line. The averaged energy resolution at the CCD temperature of -70 deg is 144.5 eV (FWHM) for 5.9 keV X-ray. GSC includes proportional gas counters, which have large X-ray detection area (5350cm2). The averaged position resolution of 1.1mm at 8 keV enable us to determined the celestial position of bright sources within the accuracy of 0.1 degree. The simulation study involving the results of performance test exhibits the high sensitivity of MAXI as designed.

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