A Coudé Echelle Spectrograph with a Large Mosaic Grating but with Small Corrector Lenses

  • E. Harvey Richardson
  • Christopher L. Morbey
Conference paper
Part of the Santa Cruz Summer Workshops in Astronomy and Astrophysics book series (SANTA CRUZ)


A spectrograph is described which uses a 30 cm by 60 cm mosaic echelle grating with 316 g/mm. The large free spectral region permits removal of overlapping orders with a filter or a small grism but is not suitable for the stacking of many orders. It is not a survey instrument. The camera mirror is made paraboloidal to avoid the need for large refractive correctors such as a Schmidt plate or a Maksutov lens. Instead, a small triplet lens is located near the focus, and can be made of fused silica at low cost to permit good transmission in the ultraviolet down to the atmospheric cut-off. The collimator mirror is spherical.


Fuse Silica Spherical Aberration Entrance Aperture Optical Layout Corrector Lens 
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  1. 1.
    E. H. Richardson: SPIE, 445, 530 (1983).ADSGoogle Scholar
  2. 2.
    G. A. Brealey, J. M. Fletcher, W. A. Grundmann, and E. H. Richardson: SPIE, 240, (1980).Google Scholar
  3. 3.
    E. H. Richardson, J. M. Fletcher, and W. A. Grundmann: Proc. IAU Colloquium 79, 496 (1984).Google Scholar

Copyright information

© Springer-Verlag New York Inc. 1988

Authors and Affiliations

  • E. Harvey Richardson
  • Christopher L. Morbey

There are no affiliations available

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