Detector response of GSC/MAXI and its expected performance in orbit

Y. Tsuchiya*, A. Yoshida, K. Yamaoka, T. Arakuni, T. Miyakawa, M. Matsuoka, S. Ueno, H. Tomida, T. Yokota, K. Kawasaki, N. Kuramata, H. Katayama, M. Morii, T. Mihara, M. Nakajima, N. Isobe, M. Kohama, H. Tsunemi, E. Miyata, N. KawaiJ. Kataoka, H. Negoro

*この研究の対応する著者

研究成果: Conference article査読

1 被引用数 (Scopus)

抄録

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.

本文言語English
論文番号58981F
ページ(範囲)1-10
ページ数10
ジャーナルProceedings of SPIE - The International Society for Optical Engineering
5898
DOI
出版ステータスPublished - 2005
外部発表はい
イベントUV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XIV - San Diego, CA, United States
継続期間: 2005 8 12005 8 3

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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