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Proceedings Paper

Detector response of GSC/MAXI and its expected performance in orbit
Author(s): Yuichiro Tsuchiya; Atsumasa Yoshida; Kazutaka Yamaoka; Tomomichi Arakuni; T. Miyakawa; Masaru Matsuoka; Shiro Ueno; Hiroshi Tomida; Takao Yokota; Kazuyoshi Kawasaki; Naoyuki Kuramata; Haruyoshi Katayama; Mikio Morii; Tatehiro Mihara; Motoki Nakajima; Naoki Isobe; Mitsuhiro Kohama; Hiroshi Tsunemi; Emi Miyata; Nobuyuki Kawai; Jun Kataoka; Hitoshi Negoro
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Paper Abstract

Monitor of All-sky X-ray Image(MAXI) is an X-ray all sky monitor, which will be attached to the Japanese Experiment Module (JEM) on the International Space Station (ISS) around the year 2008. MAXI carries two types of scientific instruments. The Gas Slit Camera(GSC) consists of twelve Xe filled one-dimensional position sensitive gas proportional counters sensitive to X-ray in 2-30 keV band. The Solid-state Slit Camera (SSC) is a set of X-ray CCD arrays sensitive to 0.5-10 keV photons. Both detectors are utilized in combination with a slit and orthogonally arranged collimator plates to produce one-dimensional X-ray images along sky great circles. The instruments are now under fabrication and preflight testing. A detector response matrix (DRM) of GSC is also under development phase based on flight model calibration tests for counters and collimators. MAXI's overall performance depends on not only hardware characteristics but on the fact that the field-of-view changes in time even during observations. To study this complicated situation, we are developing a software, DRM builder, and also a simulation software to evaluate "realistic" performance of GSC in ISS orbits.

Paper Details

Date Published: 18 August 2005
PDF: 10 pages
Proc. SPIE 5898, UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XIV, 58981F (18 August 2005); doi: 10.1117/12.616434
Show Author Affiliations
Yuichiro Tsuchiya, Aoyama Gakuin Univ. (Japan)
Atsumasa Yoshida, Aoyama Gakuin Univ. (Japan)
Kazutaka Yamaoka, Aoyama Gakuin Univ. (Japan)
Tomomichi Arakuni, Aoyama Gakuin Univ. (Japan)
T. Miyakawa, Aoyama Gakuin Univ. (Japan)
Masaru Matsuoka, Japan Aerospace Exploration Agency (Japan)
Shiro Ueno, Japan Aerospace Exploration Agency (Japan)
Hiroshi Tomida, Japan Aerospace Exploration Agency (Japan)
Takao Yokota, Japan Aerospace Exploration Agency (Japan)
Kazuyoshi Kawasaki, Japan Aerospace Exploration Agency (Japan)
Naoyuki Kuramata, Japan Aerospace Exploration Agency (Japan)
Haruyoshi Katayama, Japan Aerospace Exploration Agency (Japan)
Mikio Morii, Japan Aerospace Exploration Agency (Japan)
Tatehiro Mihara, The Institute of Physical and Chemical Research (RIKEN) (Japan)
Motoki Nakajima, The Institute of Physical and Chemical Research (RIKEN) (Japan)
Naoki Isobe, The Institute of Physical and Chemical Research (RIKEN) (Japan)
Mitsuhiro Kohama, The Institute of Physical and Chemical Research (RIKEN) (Japan)
Hiroshi Tsunemi, Osaka Univ. (Japan)
Emi Miyata, Osaka Univ. (Japan)
Nobuyuki Kawai, Tokyo Institute of Technology (Japan)
Jun Kataoka, Tokyo Institute of Technology (Japan)
Hitoshi Negoro, Nihon Univ. (Japan)


Published in SPIE Proceedings Vol. 5898:
UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XIV
Oswald H. W. Siegmund, Editor(s)

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