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A Low Energy Gas Scintillation Proportional Counter for the SAX-X-Ray Astronomy Satellite

Published online by Cambridge University Press:  12 April 2016

A.N. Parmar ,
A. Smith  and
M. Bavdaz
A.N. Parmar
Affiliation:
Space Science Department, European Space Agency, ESTEC, Noordwijk, The Netherlands
A. Smith
Affiliation:
Space Science Department, European Space Agency, ESTEC, Noordwijk, The Netherlands
M. Bavdaz
Affiliation:
Space Science Department, European Space Agency, ESTEC, Noordwijk, The Netherlands

Abstract

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The payload of the italian/Dutch satellite SAX will include a set of four concentrators each with a geometric area of 90 cm2. Imaging GSPCs will be located at the focal planes of the concetrators. The Space Science Department of ESA will provide one of these GSPCs which will be sensitive to X-rays with energies between 0.1-10 keV. In order to achieve such a low-energy energy response, a driftless configuration and a thin plastic window have been adopted. At 6 keV the collecting area will be 50 cm2 and the energy and angular resolutions 8% and 1.6′ FWHM, respectively.

Type
V. Long Term Future Issues
Information
International Astronomical Union Colloquium , Volume 123: Observatories in Earth Orbit and Beyond , 1990 , pp. 457 - 461
Copyright
Copyright © Kluwer 1990

References

Favata, F., and Smith, A.: 1989, SPIE Proceedings of EUV, X-Ray and Gamma-Ray Instrumentation for Astronomy and Atomic Physics, SPIE, Bellingham, 1159, 488 Google Scholar
Favata, F., Smith, A., Bavdaz, M. and Kowalski, T.Z.: 1990, Submitted to Nucl, Instr. Meth. Google Scholar
Holland, A.D., Lumb, D.H., and Castelli, C.M.: 1989, SPIE Proceedings of EUV, X-ray, and Gamma-Ray Instrumentation for Astronomy and Atomic Physics, SPIE, Bellingham, 1159, 113 Google Scholar
Inoue, H., Koyama, K., Matsuoka, M., Ohashi, T. and Tanaka, Y.: 1979, Nucl. Instr. Meth. 157, 295 Google Scholar
Kowalsky, T.Z., Smith, A. and Peacock, A.: 1989, Nucl. Instr. Meth. A279, 567 CrossRefGoogle Scholar
Peacock, A., etal.: 1981, Space Sci. Rev. 30, 479 CrossRefGoogle Scholar
Perola, G. C.: 1983, Proceedings of the Workshop on Non-thermal and Very High Temperature Phenomena in X-ray Astronomy, Rome, 175 Google Scholar
Scarsi, L.: 1983, Proceedings of the Workshop on Non-thermal and Very High Temperature Phenomena in X-ray Astronomy, Rome, 171 Google Scholar
Simons, D.G., de Korte, P.A.J., Peacock, A., and Bleeker, J.A.M.: 1985, SPIE Proceedings of X-ray Instrumentation in Astronomy, SPIE, Bellingham, 597, 190 Google Scholar
Smith, A., Favata, F. and Kowalsky, T.Z.: 1989, Nucl. Instr. Meth. A284, 375 CrossRefGoogle Scholar
Smith, A, Peacock, A., and Kowalski, T.Z.: 1987, IEEE Trans. Nucl. Sci. NS-34, 57 Google Scholar
Spada, G.F.L.: 1983, Proceedings of the Workshop on Non-thermal and Very High Temperature Phenomena in X-ray Astronomy, Rome, 217 Google Scholar