The observational response of MAXI onboard ISS

Naoki Isobe; Masaru Matsuoka; Shiro Ueno; Hiroshi Tomida; Kazuyoshi Kawasaki; Haruyoshi Katayama; Tatehiro Mihara; Mitsuhiro Kohama; Ikuya Sakurai; Motoki Nakajima; Nobuyuki Kawai; Jun Kataoka; Atsumasa Yoshida; Daiki Takahashi; Masami Uzawa; Hiroshi Tsunemi; Emi Miyata; Isao Tanaka

doi:10.1117/12.505315

The observational response of MAXI onboard ISS

Naoki Isobe^*, Masaru Matsuoka, Shiro Ueno, Hiroshi Tomida, Kazuyoshi Kawasaki, Haruyoshi Katayama, Tatehiro Mihara, Mitsuhiro Kohama, Ikuya Sakurai, Motoki Nakajima, Nobuyuki Kawai, Jun Kataoka, Atsumasa Yoshida, Daiki Takahashi, Masami Uzawa, Hiroshi Tsunemi, Emi Miyata, Isao Tanaka

^*この研究の対応する著者

研究成果 › 査読

9 被引用数 (Scopus)

抄録

The current status is reported of the development of Monitor of All-sky X-ray Image and the measurement of its observational response. MAXI is a scanning X-ray camera to be attached to the Japanese Experiment Module of the International Space Station in 2008. MAXI is mainly composed of two kinds of instruments, GSC which is sensitive to the 2 - 30 keV photons, and SSC to the 0.5 - 10 keV ones. As an X-ray all-sky monitor, MAXI has an unprecedented sensitivity of 7 mCrab in one orbit scan, and 1 mCrab in one week. Using the engineering mode of the proportional counter and of the collimator for GSC, the observational response of GSC is extensively measured. The acceptable performances are obtained as a whole for both the collimator and the counter. The engineering models of the other part of MAXI are also constructed and the measurement of their performance is ongoing.

本文言語	English
ページ（範囲）	354-365
ページ数	12
ジャーナル	Proceedings of SPIE - The International Society for Optical Engineering
巻	5165
DOI	https://doi.org/10.1117/12.505315
出版ステータス	Published - 2004
外部発表	はい
イベント	X-Ray and Gamma-Ray Instrumentation for Astronomy XIII - San Diego, CA, United States 継続期間: 2003 8 3 → 2003 8 5

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

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10.1117/12.505315

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引用スタイル

Isobe, N., Matsuoka, M., Ueno, S., Tomida, H., Kawasaki, K., Katayama, H., Mihara, T., Kohama, M., Sakurai, I., Nakajima, M., Kawai, N., Kataoka, J., Yoshida, A., Takahashi, D., Uzawa, M., Tsunemi, H., Miyata, E., & Tanaka, I. (2004). The observational response of MAXI onboard ISS. Proceedings of SPIE - The International Society for Optical Engineering, 5165, 354-365. https://doi.org/10.1117/12.505315

The observational response of MAXI onboard ISS. / Isobe, Naoki; Matsuoka, Masaru; Ueno, Shiro; Tomida, Hiroshi; Kawasaki, Kazuyoshi; Katayama, Haruyoshi; Mihara, Tatehiro; Kohama, Mitsuhiro; Sakurai, Ikuya; Nakajima, Motoki; Kawai, Nobuyuki; Kataoka, Jun; Yoshida, Atsumasa; Takahashi, Daiki; Uzawa, Masami; Tsunemi, Hiroshi; Miyata, Emi; Tanaka, Isao.

In: Proceedings of SPIE - The International Society for Optical Engineering, Vol. 5165, 2004, p. 354-365.

研究成果 › 査読

Isobe, N, Matsuoka, M, Ueno, S, Tomida, H, Kawasaki, K, Katayama, H, Mihara, T, Kohama, M, Sakurai, I, Nakajima, M, Kawai, N, Kataoka, J, Yoshida, A, Takahashi, D, Uzawa, M, Tsunemi, H, Miyata, E & Tanaka, I 2004, 'The observational response of MAXI onboard ISS', Proceedings of SPIE - The International Society for Optical Engineering, vol. 5165, pp. 354-365. https://doi.org/10.1117/12.505315

Isobe, Naoki ; Matsuoka, Masaru ; Ueno, Shiro ; Tomida, Hiroshi ; Kawasaki, Kazuyoshi ; Katayama, Haruyoshi ; Mihara, Tatehiro ; Kohama, Mitsuhiro ; Sakurai, Ikuya ; Nakajima, Motoki ; Kawai, Nobuyuki ; Kataoka, Jun ; Yoshida, Atsumasa ; Takahashi, Daiki ; Uzawa, Masami ; Tsunemi, Hiroshi ; Miyata, Emi ; Tanaka, Isao. / The observational response of MAXI onboard ISS. In: Proceedings of SPIE - The International Society for Optical Engineering. 2004 ; Vol. 5165. pp. 354-365.

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abstract = "The current status is reported of the development of Monitor of All-sky X-ray Image and the measurement of its observational response. MAXI is a scanning X-ray camera to be attached to the Japanese Experiment Module of the International Space Station in 2008. MAXI is mainly composed of two kinds of instruments, GSC which is sensitive to the 2 - 30 keV photons, and SSC to the 0.5 - 10 keV ones. As an X-ray all-sky monitor, MAXI has an unprecedented sensitivity of 7 mCrab in one orbit scan, and 1 mCrab in one week. Using the engineering mode of the proportional counter and of the collimator for GSC, the observational response of GSC is extensively measured. The acceptable performances are obtained as a whole for both the collimator and the counter. The engineering models of the other part of MAXI are also constructed and the measurement of their performance is ongoing.",

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AU - Isobe, Naoki

AU - Matsuoka, Masaru

AU - Ueno, Shiro

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AU - Kawasaki, Kazuyoshi

AU - Katayama, Haruyoshi

AU - Mihara, Tatehiro

AU - Kohama, Mitsuhiro

AU - Sakurai, Ikuya

AU - Nakajima, Motoki

AU - Kawai, Nobuyuki

AU - Kataoka, Jun

AU - Yoshida, Atsumasa

AU - Takahashi, Daiki

AU - Uzawa, Masami

AU - Tsunemi, Hiroshi

AU - Miyata, Emi

AU - Tanaka, Isao

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N2 - The current status is reported of the development of Monitor of All-sky X-ray Image and the measurement of its observational response. MAXI is a scanning X-ray camera to be attached to the Japanese Experiment Module of the International Space Station in 2008. MAXI is mainly composed of two kinds of instruments, GSC which is sensitive to the 2 - 30 keV photons, and SSC to the 0.5 - 10 keV ones. As an X-ray all-sky monitor, MAXI has an unprecedented sensitivity of 7 mCrab in one orbit scan, and 1 mCrab in one week. Using the engineering mode of the proportional counter and of the collimator for GSC, the observational response of GSC is extensively measured. The acceptable performances are obtained as a whole for both the collimator and the counter. The engineering models of the other part of MAXI are also constructed and the measurement of their performance is ongoing.

AB - The current status is reported of the development of Monitor of All-sky X-ray Image and the measurement of its observational response. MAXI is a scanning X-ray camera to be attached to the Japanese Experiment Module of the International Space Station in 2008. MAXI is mainly composed of two kinds of instruments, GSC which is sensitive to the 2 - 30 keV photons, and SSC to the 0.5 - 10 keV ones. As an X-ray all-sky monitor, MAXI has an unprecedented sensitivity of 7 mCrab in one orbit scan, and 1 mCrab in one week. Using the engineering mode of the proportional counter and of the collimator for GSC, the observational response of GSC is extensively measured. The acceptable performances are obtained as a whole for both the collimator and the counter. The engineering models of the other part of MAXI are also constructed and the measurement of their performance is ongoing.

KW - All sky monitor

KW - GSC

KW - International Space Station

KW - MAXI

KW - Observational response

KW - SSC

KW - X-Ray

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The observational response of MAXI onboard ISS

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