The Monte Carlo simulation framework of the ASTRO-H x-ray observatory

Masanobu Ozaki; Masanori Ohno; Yukikatsu Terada; Shin Watanabe; Tsunefumi Mizuno; Tadayuki Takahashi; Motohide Kokubun; Masahiro Tsujimoto; Noriko Y. Yamasaki; Hirokazu Odaka; Yoh Takei; Takayuki Yuasa; Akihiro Furuzawa; Hideyuki Mori; Hironori Matsumoto; Takashi Okajima; Caroline A. Kilbourne; Hiroyasu Tajima; Yoshitaka Ishisaki

doi:10.1117/12.856126

The Monte Carlo simulation framework of the ASTRO-H x-ray observatory

Masanobu Ozaki, Masanori Ohno, Yukikatsu Terada, Shin Watanabe, Tsunefumi Mizuno, Tadayuki Takahashi, Motohide Kokubun, Masahiro Tsujimoto, Noriko Y. Yamasaki, Hirokazu Odaka, Yoh Takei, Takayuki Yuasa, Akihiro Furuzawa, Hideyuki Mori, Hironori Matsumoto, Takashi Okajima, Caroline A. Kilbourne, Hiroyasu Tajima, Yoshitaka Ishisaki

研究成果: 書籍/レポートタイプへの寄稿 › 会議への寄与

4 被引用数 (Scopus)

抄録

We are developing an ASTRO-H data analysis framework with the Geant4-based Monte Carlo simulation core, and numerical models of the on-orbit environmental radiation and full-satellite mass structure. In addition, the framework also includes a mechanism to connect and control data processing modules that are developed independently and data communication channels among them, which has been technically proven by simulations and analysis of the Suzaku HXD, many other detectors and astrophysical issues.

本文言語	英語
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/10.1117/12.856126
出版ステータス	出版済み - 2010
外部発表	はい
イベント	Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray - San Diego, CA, 米国継続期間: 28-06-2010 → 02-07-2010

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

その他

その他	Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray
国/地域	米国
City	San Diego, CA
Period	28-06-10 → 02-07-10

All Science Journal Classification (ASJC) codes

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

10.1117/12.856126

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引用スタイル

Ozaki, M., Ohno, M., Terada, Y., Watanabe, S., Mizuno, T., Takahashi, T., Kokubun, M., Tsujimoto, M., Yamasaki, N. Y., Odaka, H., Takei, Y., Yuasa, T., Furuzawa, A., Mori, H., Matsumoto, H., Okajima, T., Kilbourne, C. A., Tajima, H., & Ishisaki, Y. (2010). The Monte Carlo simulation framework of the ASTRO-H x-ray observatory. In Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray 記事 773239 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 7732). https://doi.org/10.1117/12.856126

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title = "The Monte Carlo simulation framework of the ASTRO-H x-ray observatory",

abstract = "We are developing an ASTRO-H data analysis framework with the Geant4-based Monte Carlo simulation core, and numerical models of the on-orbit environmental radiation and full-satellite mass structure. In addition, the framework also includes a mechanism to connect and control data processing modules that are developed independently and data communication channels among them, which has been technically proven by simulations and analysis of the Suzaku HXD, many other detectors and astrophysical issues.",

author = "Masanobu Ozaki and Masanori Ohno and Yukikatsu Terada and Shin Watanabe and Tsunefumi Mizuno and Tadayuki Takahashi and Motohide Kokubun and Masahiro Tsujimoto and Yamasaki, {Noriko Y.} and Hirokazu Odaka and Yoh Takei and Takayuki Yuasa and Akihiro Furuzawa and Hideyuki Mori and Hironori Matsumoto and Takashi Okajima and Kilbourne, {Caroline A.} and Hiroyasu Tajima and Yoshitaka Ishisaki",

year = "2010",

doi = "10.1117/12.856126",

language = "English",

isbn = "9780819482228",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

booktitle = "Space Telescopes and Instrumentation 2010",

note = "Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray ; Conference date: 28-06-2010 Through 02-07-2010",

}

Ozaki, M, Ohno, M, Terada, Y, Watanabe, S, Mizuno, T, Takahashi, T, Kokubun, M, Tsujimoto, M, Yamasaki, NY, Odaka, H, Takei, Y, Yuasa, T, Furuzawa, A, Mori, H, Matsumoto, H, Okajima, T, Kilbourne, CA, Tajima, H & Ishisaki, Y 2010, The Monte Carlo simulation framework of the ASTRO-H x-ray observatory. in Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray., 773239, Proceedings of SPIE - The International Society for Optical Engineering, vol. 7732, Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray, San Diego, CA, 米国, 28-06-10. https://doi.org/10.1117/12.856126

The Monte Carlo simulation framework of the ASTRO-H x-ray observatory. / Ozaki, Masanobu; Ohno, Masanori; Terada, Yukikatsu その他.
Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray. 2010. 773239 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 7732).

研究成果: 書籍/レポートタイプへの寄稿 › 会議への寄与

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T1 - The Monte Carlo simulation framework of the ASTRO-H x-ray observatory

AU - Ozaki, Masanobu

AU - Ohno, Masanori

AU - Terada, Yukikatsu

AU - Watanabe, Shin

AU - Mizuno, Tsunefumi

AU - Takahashi, Tadayuki

AU - Kokubun, Motohide

AU - Tsujimoto, Masahiro

AU - Yamasaki, Noriko Y.

AU - Odaka, Hirokazu

AU - Takei, Yoh

AU - Yuasa, Takayuki

AU - Furuzawa, Akihiro

AU - Mori, Hideyuki

AU - Matsumoto, Hironori

AU - Okajima, Takashi

AU - Kilbourne, Caroline A.

AU - Tajima, Hiroyasu

AU - Ishisaki, Yoshitaka

PY - 2010

Y1 - 2010

N2 - We are developing an ASTRO-H data analysis framework with the Geant4-based Monte Carlo simulation core, and numerical models of the on-orbit environmental radiation and full-satellite mass structure. In addition, the framework also includes a mechanism to connect and control data processing modules that are developed independently and data communication channels among them, which has been technically proven by simulations and analysis of the Suzaku HXD, many other detectors and astrophysical issues.

AB - We are developing an ASTRO-H data analysis framework with the Geant4-based Monte Carlo simulation core, and numerical models of the on-orbit environmental radiation and full-satellite mass structure. In addition, the framework also includes a mechanism to connect and control data processing modules that are developed independently and data communication channels among them, which has been technically proven by simulations and analysis of the Suzaku HXD, many other detectors and astrophysical issues.

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DO - 10.1117/12.856126

M3 - Conference contribution

AN - SCOPUS:77957876675

SN - 9780819482228

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Space Telescopes and Instrumentation 2010

T2 - Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray

Y2 - 28 June 2010 through 2 July 2010

ER -

The Monte Carlo simulation framework of the ASTRO-H x-ray observatory

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出版物シリーズ

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All Science Journal Classification (ASJC) codes

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