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XSPECT: A Telescope/Spectrometer System on SPECTRUM RÖNTGEN GAMMA

Published online by Cambridge University Press:  12 April 2016

Herbert W. Schnopper
Herbert W. Schnopper*
Affiliation:
Danish Space Research Institute, DK-2800 Lyngby, Denmark

Abstract

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The SPECTRUM RÖNTGEN-GAMMA mission is being developed by the Babakin Center (BC) together with the Space Research Institute (IKI) of the Academy of Sciences, USSR and is scheduled for launch in 1993. Mission objectives include broad and narrow band imaging spectroscopy over a wide range of energies from the EUV through gamma rays with particular emphasis on the study of extragalactic objects. The Danish Space Research Institute (DSRI) BC and IKI share the responsibility for the preparation of the XSPECT system. Two thin foil telescopes which are conical shell approximations to Wolter 1 geometry, each with an aperture of 60 cm and a focal length of 8 m, are designed to have a half-power width of less than 2 arcmin and will have collecting areas of 1700 and 1200 cm at 2 and 8 keV, respectively. Images and spectra will be recorded with position sensitive proportional counters with good spectral resolution. An objective Bragg crystal panel, placed in front of one of the telescopes, will make high resolution spectroscopic studies (E/ΔE ~103) of point- and extended sources. Other instruments are under consideration.

Information

Type
8. Future X-ray Observatories
Information
International Astronomical Union Colloquium , Volume 115: High Resolution X-ray Spectroscopy of Cosmic Plasmas , 1990, pp. 307 - 317
Copyright
Copyright © Cambridge University Press 1990

References

Aschenbach, B. 1985, Rep. Prog. Phys., 48, 579–629.Google Scholar
Budtz-Jorgensen, C., Madsen, M.M., Jonasson, P., Schnopper, H.W., and Oed, A. 1989, SPIE Proc., 982, in press.Google Scholar
Hamilton, T.T., and Helfand, D.J. 1987, Ap. J., 318, 93–102.Google Scholar
Hudec, R., and Valnicek, B. 1985, SPIE Proc., 597, 111–118.Google Scholar
Hudec, R. 1988, private communication.Google Scholar
Kunieda, , and Serlemitsos, P.J. 1988, SPIE Proc., 830, 12–15.Google Scholar
Madsen, M.M., Jonasson, P., Jensen, P.L., Rasmussen, H.E., Ørup, P., and Schnopper, H.W. 1985, SPIE Proc, 597, 199–205.Google Scholar
Oed, A. 1988, Nucl. Instr. Meth., A263, 351–359.Google Scholar
Schnopper, H.W., and Brynak, B.P. 1987, Appl. Opt., 26, 2871–2876.Google Scholar
Serlemitsos, P.J., Petre, R., Glasser, C., and Birsa, F. 1984, IEEE Trans. Nuc. Sci., NS-31, 786–790.Google Scholar
Sipilä, H. 1988, private communication.Google Scholar
Tanaka, Y., and Makino, F., 1988, SPIE Proc, 830, 242–244.Google Scholar
Wolter, H. 1952a, Ann. Phys., 10, 94.Google Scholar
Wolter, H. 1952b, Ann. Phys., 10, 286.Google Scholar