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. KawaiJun Kataoka, H. Negoro

Research output: Chapter in Book/Report/Conference proceedingConference contribution

1 Citation (Scopus)

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.

Original languageEnglish
Title of host publicationProceedings of SPIE - The International Society for Optical Engineering
EditorsO.H.W. Siegmund
Pages1-10
Number of pages10
Volume5898
DOIs
Publication statusPublished - 2005
Externally publishedYes
EventUV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XIV - San Diego, CA, United States
Duration: 2005 Aug 12005 Aug 3

Other

OtherUV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XIV
CountryUnited States
CitySan Diego, CA
Period05/8/105/8/3

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Keywords

  • All sky monitor
  • MAXI
  • X-ray

ASJC Scopus subject areas

  • Electrical and Electronic Engineering
  • Condensed Matter Physics

Cite this

Tsuchiya, Y., Yoshida, A., Yamaoka, K., Arakuni, T., Miyakawa, T., Matsuoka, M., Ueno, S., Tomida, H., Yokota, T., Kawasaki, K., Kuramata, N., Katayama, H., Morii, M., Mihara, T., Nakajima, M., Isobe, N., Kohama, M., Tsunemi, H., Miyata, E., ... Negoro, H. (2005). Detector response of GSC/MAXI and its expected performance in orbit. In O. H. W. Siegmund (Ed.), Proceedings of SPIE - The International Society for Optical Engineering (Vol. 5898, pp. 1-10). [58981F] https://doi.org/10.1117/12.616434