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Relative Fluxes by Spectrophotometry with RUBIKON

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Abstract

By means of the RUBIKON multi-channel detector system with integrated grism spectrograph, attached to the Bochum 61cm telescope, five primary standars stars have been intercompared and an additional secondary standard star (HD 37027 in the center field of the LMC) has been set up in the wavelength range of 326–777 nm.

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Authors and Affiliations

  1. Astronomisches Institut Ruhr-Universität Bochum, Universitätsstrasse 150, D-44780, Bochum, Germany and

    Th. Schmidt-Kaler

  2. D-97276, Margetshöchheim, Georg-Büchner-Str.37, Germany, Fax

    Th. Schmidt-Kaler

  3. Centro de Investigaciones de Astronomia, Apartado Postal 264, Merida, 5101-A, Venezuela

    M. O. Oestreicher

Authors
  1. Th. Schmidt-Kaler
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  2. M. O. Oestreicher
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Correspondence to M. O. Oestreicher.

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Schmidt-Kaler, T., Oestreicher, M.O. Relative Fluxes by Spectrophotometry with RUBIKON. Experimental Astronomy 9, 213–236 (1999). https://doi.org/10.1023/A:1008126909771

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  • DOI: https://doi.org/10.1023/A:1008126909771

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