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Fibre optics at the 4.2 m telescope (WHT)

  • Session 6 Astronomical Instrumentation
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Abstract

We summarize some of the work on optical fibres carried out at the 4.2 m (WHT) telescope. We will briefly describe the Fibre Linked Experimental spectrograph.

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References

  • Barden, S.: 1988,Fiber Optics in Astronomy, PSA, Conference Series.

  • Rasilla, J. L., Arribas, S., Mediavilla, E., and Sebastian, J. L.: 1990,Astrophys. Space Sci. 171, 301 (this issue).

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  • Unger, S., Brinks, E., Laing, R. A., Tritton, K. P., and Gray, P. M.: 1988,Observer Guide, Isaac Newton Group, La Palma.

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Authors and Affiliations

  1. Instituto de Astrofisica de Canarias, Spain

    S. Arribas, J. L. Rasilla & J. L. Sebastian

  2. Royal Greenwich Observatory, U.K.

    P. M. Gray, R. Terlevich & D. Carter

  3. Anglo-Australian Observatory, Australia

    P. M. Gray

Authors
  1. S. Arribas
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  2. P. M. Gray
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  3. R. Terlevich
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  4. D. Carter
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  5. J. L. Rasilla
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  6. J. L. Sebastian
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Arribas, S., Gray, P.M., Terlevich, R. et al. Fibre optics at the 4.2 m telescope (WHT). Astrophys Space Sci 171, 293–296 (1990). https://doi.org/10.1007/BF00646866

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  • DOI: https://doi.org/10.1007/BF00646866

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