Hostname: page-component-cd9895bd7-gxg78 Total loading time: 0 Render date: 2024-12-12T18:29:45.886Z Has data issue: false hasContentIssue false

An X-Ray All Sky Monitor for a Japanese Experimental Module on the Space Station

Published online by Cambridge University Press:  12 April 2016

M. Matsuoka
Affiliation:
The Institute of Physical and Chemical Research, 2-1 Hirosawa, Wako, Saitama 351-01, Japan
N. Kawai
Affiliation:
The Institute of Physical and Chemical Research, 2-1 Hirosawa, Wako, Saitama 351-01, Japan
T. Imai
Affiliation:
The Institute of Physical and Chemical Research, 2-1 Hirosawa, Wako, Saitama 351-01, Japan
M. Yamauchi
Affiliation:
The Institute of Physical and Chemical Research, 2-1 Hirosawa, Wako, Saitama 351-01, Japan
A. Yoshida
Affiliation:
The Institute of Physical and Chemical Research, 2-1 Hirosawa, Wako, Saitama 351-01, Japan
T. Kohno
Affiliation:
The Institute of Physical and Chemical Research, 2-1 Hirosawa, Wako, Saitama 351-01, Japan
A. Yoneda
Affiliation:
The Institute of Physical and Chemical Research, 2-1 Hirosawa, Wako, Saitama 351-01, Japan
H. Tsunemi
Affiliation:
Department of Physics, Faculty of Science, Osaka University, 1-1 Machikaneyama-cho, Toyonaka, Osaka 560, Japan

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We propose an X-ray all sky monitor for Japanese Experimental Module (JEM) on the space station. Considering practical circumstances, we show as a case study that the all sky monitor with slit hole cameras is most promising for monitoring the short-term and long-term X-ray transients. We call this all sky monitor as MAXI (Monitor of All-sky X-ray Image). Position determination of gamma-ray bursts could be achieved with accuracy less than one degree observing the X-ray component of the burst. Weak X-ray sources such as active galactic nuclei could be also monitored with time resolution less than one day. The X-ray all sky monitor will work to discover X-ray novae and transient phenomena and give us the alarm for further detailed observations. The obtained data will be also used for archival study.

Type
V. Long Term Future Issues
Copyright
Copyright © Kluwer 1990

References

Caroli, E. et al.: 1987, Space Sci. Rev. 45, 349 Google Scholar
Doi, K.: 1988, LxR Report “Intrinsic ambiguity in the X-ray image data obtained with the rotating modulation collimator system”, No.8801 Google Scholar
Holt, S.S. and Priedhorsky, W.: 1987, Space Sci. Rev. 45, 269 Google Scholar
Kondo, I. et al.: 1981, Space Sci. Instr. 5, 211 Google Scholar
Lund, N.: 1985, SPIE Proc. of X-ray Instrumentation in Astronomy, 597, 95 Google Scholar
Matsuoka, M., Kawai, N., and Tsunemi, H.: 1988, IPCR CR-13 prepared for a reference mission to be attached to the JEM on the space station,Google Scholar
Nishimura, J., et al.: 1978, Nature 272, 337 Google Scholar
Priedhorsky, W.C. and Holt, S.S.: 1987, Space Sci. Rev. 45, 291 Google Scholar