Paper
30 July 2010 The Monte Carlo simulation framework of the ASTRO-H X-ray Observatory
Author Affiliations +
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.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
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, and Yoshitaka Ishisaki "The Monte Carlo simulation framework of the ASTRO-H X-ray Observatory", Proc. SPIE 7732, Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray, 773239 (30 July 2010); https://doi.org/10.1117/12.856126
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CITATIONS
Cited by 3 scholarly publications.
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KEYWORDS
Monte Carlo methods

Sensors

Satellites

Particles

X-rays

Absorption

Computer aided design

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