Astrophysics and Space Science

, Volume 31, Issue 2, pp 417–425 | Cite as

An all-sky camera battery for x-ray astronomy

  • Cornelis De Jager
Article
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Abstract

The increasing number of interesting variable X-ray sources asks for an instrument for continuously monitoring the brightness of the most important X-ray sources over the whole sky. We describe a system consisting of a set of identical large position-sensitive detectors, mounted on the sides of a polyhedral satellite. Each counter is illuminated through a large diaphragm, with binary shadow characteristics. By holographic methods the X-ray image of the observed part of the sky could be derived from the illumination of each detector by multiplex analysing methods. The satellite should have fairly coarse (half a degree accuracy) three-axial stabilization, and an on-board computersteered data accumulation system.

A relation is derived between the number of transparent holes in the diaphragm, the total count rate, and the flux of the faintest observable source. It appears that for a diaphragm with a few hundred transparent holes (detector geometrical area ≈103 cm2) an integration time of approximately 6 min is needed in order that sources with a count rate of 0.01 cm−2 s−1 should still be observable with a confidence limit of 99%.

Keywords

Count Rate Data Accumulation Accumulation System Geometrical Area Degree Accuracy 

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References

  1. Dicke, R. H.: 1968,Astrophys. J. 153, L101.Google Scholar
  2. Gilland, J. R. and Emming, J. G.: 1972,Nucl. Instr. Methods 104, 241.Google Scholar
  3. Van Beek, H. F.: 1974, in preparation.Google Scholar

Copyright information

© D. Reidel Publishing Company 1974

Authors and Affiliations

  • Cornelis De Jager
    • 1
  1. 1.The Astronomical InstituteUtrechtHolland

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