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The High Resolution Spectrograph for Spectrum UV

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Abstract

The Spectrum-UV mission, a general purpose ultraviolet observatory equipped with a 170-cm aperture telescope for imaging and spectroscopy in the 912 to 3600 Å range, will be launched in a seven days, high elliptical orbit in the late '90s by a Proton booster. The German contribution to the focal plane instrument complex is described: HIRDES, a High Resolution Double Echelle Spectrograph.

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References

  1. Becker-Ross, H., SPACE OPTICS 1994, Earth Observation and Astronomy, SPIE, Vol. 2209

  2. Boyarchuk, A.A, Tanzi, E.G, Mem. S.A.It., Vol. 64,No.2

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Authors and Affiliations

  1. Institut für Astronomie und Astrophysik, Abtl. Astronomie, Universität, Waldhäuser 64, D-72076, Tübingen

    N. Kappelmann, J. Barnstedt, M. Grewing & G. Krämer

  2. Institut für Spektrochemie, ISAS/LSMU, Rudower Chaussee 5, D-12489, Berlin-Adlershof

    H. Becker-Ross & S. Florek

  3. Astrophysikalisches Institut Potsdam, Telegrafenberg, D-14482, Potsdam

    D. Schönberner

Authors
  1. N. Kappelmann
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  2. J. Barnstedt
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  3. H. Becker-Ross
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  4. S. Florek
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  5. M. Grewing
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  6. G. Krämer
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  7. D. Schönberner
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Kappelmann, N., Barnstedt, J., Becker-Ross, H. et al. The High Resolution Spectrograph for Spectrum UV. Experimental Astronomy 7, 361–367 (1997). https://doi.org/10.1023/A:1007993321627

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  • DOI: https://doi.org/10.1023/A:1007993321627

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