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EUVITA - an extreme UV imaging telescope array with spectral capability

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Abstract

EUVITA is a set of 8 extreme UV and soft X-ray normal incidence imaging telescopes, each of them sensitive in a narrow band (λ/Δλ=15 to 80), centered at wavelengths between 50 and 175 Å. Each telescope has an effective area of a few cm2, a field of view of 1.2° and an angular resolution of 10 arcseconds. EUVITA will be Sown on the Russian mission SPECTRUM X-G. This satellite will be launched in a highly eccentric orbit with a period of 4 days, allowing long, uninterrupted observations (e.g. 105 seconds). The present paper includes an overview of EUVITA's scientific capabilities and a short description of the instrument. Simulations of various types of sources show EUVITA's capability to detect galactic and extragalactic EUV sources. EUVITA's narrow spectral bands allow the measurement of source parameters such as temperature or power law index as well as interstellar absorption, and will resolve groups of strong lines emitted by optically thin hot plasmas.

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References

  • C. Allen, Astrophysical Quantities (3rd edition; Athlone, London), 1973

    Google Scholar 

  • K. A. Arnaud, in Cooling Flows in Clusters and Galaxies, A. C. Fabian ed., NATO ASI Series, p. 31, 1988

  • J. Bechtold et. al., Ap. J., 314:699, 1987

    Google Scholar 

  • T. Belloni et al., Astron. Astrophys., 246, L44, 1991

  • S. Bowyer, in Extreme Ultraviolet Astronomy, R. Malina, S. Bowyer eds., Pergammon Press, p. 120, 1991

  • S. Bowyer, R. Malina, in Extreme Ultraviolet Astronomy, R. Malina, S. Bowyer eds., Pergammon Press, p. 397, 1991a

  • S. Bowyer, R. Malina, Adv. Space Research, Vol. 11, p. 205, 1991

    Google Scholar 

  • A. Comastri et. al., Ap. J., 384:62, 1991

    Google Scholar 

  • T. Courvoisier et. al., Astron. Astrophys., 176:197, 1987

    Google Scholar 

  • T. Courvoisier, J. Clavel, Astron. Astrophys., 248: 389, 1991

    Google Scholar 

  • P. De Korte et al, Space Science Review, 30, 495, 1981

    Google Scholar 

  • M. Elvis et al., Astron. J., 97:777, 1989

    Google Scholar 

  • EUVE Guest Observer Program Handbook, NASA NRA 92-OSSA-5, Appendix G, 1992

  • A. C. Fabian, P.E.J. Nulsen and C.R. Canizares, Astron. & Astrophys. Rev., 2:191,1992

    Google Scholar 

  • W. Forman, C. Jones, in Clusters of Galaxies, W. Oegerle et al. eds., Cambridge University Press, p. 257, 1990

  • D. Frail, J. Weisberg, Astron. J., 100:743, 1990

    Google Scholar 

  • J. Heise et al., Ap. J., 334:958, 1988

    Google Scholar 

  • K. Jahoda et al., Ap. J., 354:184, 1990

    Google Scholar 

  • R.-P. Kudritzki et al., in Extreme Ultraviolet Astronomy, R. Malina, S. Bowyer eds., Pergammon Press, p. 130, 1991

  • R. Mewe et al., Astron. & Astrophys. Suppl. Ser., 62: 197, 1985

    Google Scholar 

  • R. Mewe et al., Astron. & Astrophys. Suppl. Ser., 65: 511, 1986

    Google Scholar 

  • R. Morrison, D. Mc Cammon, Ap. J., 270:119, 1983

    Google Scholar 

  • H. Ögelman, in Neutron stars: Theory and Observation, J. Ventura, D. Pines eds., Kluwer Academ. Publ., 1991

  • R. Pallavicini, Astron. Astrophys. Rev., 1:177, 1989

    Google Scholar 

  • R. Polidan et al., Ap. J., 356:211, 1990

    Google Scholar 

  • K. Pounds et al., submitted to M.N.R.A.S., 1992

  • W. Priedhorsky et al., in Extreme Ultraviolet Astronomy, R. Malina, S. Bowyer eds., Pergammon Press, p. 464, 1991

  • C. L. Sarazin, R.W. O'Connell and B.R. McNamara, Ap. J., 389, L59, 1992

  • F. Seward, Z. Wang, Ap. J., 332:199, 1988

    Google Scholar 

  • O. Siegmund et al., Journal of the Opt. Soc. of America A, vol.3, p. 2139, 1986

    Google Scholar 

  • M. Sims et al., Optical Engineering, 26, 649, 1990

    Google Scholar 

  • R. Staubert et al., in AIP Conf. Proced. on ‘Testing the AGN Paradigm ’, S. Holt, S. Neff, C. Urry eds., p. 366, 1992

  • T. Turner, K. Pounds, M.N.R.A.S., 240:833, 1989

    Google Scholar 

  • P. Vedder et al., in Extreme Ultraviolet Astronomy, R. Malina, S. Bowyer eds., Pergammon Press, p. 120, 1991

  • R. Wade, M. Ward, in Interacting Binary Stars, J. Pringle, R. Wade eds., Cambridge University Press, 1985

  • R. Wade, in Extreme Ultraviolet Astronomy, R. Malina, S. Bowyer eds., Pergammon Press, p. 186, 1991

  • N. White, in Extreme Ultraviolet Astronomy, R. Malina, S. Bowyer eds., Pergammon Press, p. 15, 1991

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Courvoisier, J.L., Orr, A., Bühler, P. et al. EUVITA - an extreme UV imaging telescope array with spectral capability. Exp Astron 4, 117–135 (1993). https://doi.org/10.1007/BF01588349

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  • DOI: https://doi.org/10.1007/BF01588349

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