Engineering solution for the high-resolution optical spectrograph on Gemini South

Details Engineering solution for the high-resolution optical spectrograph on Gemini South Engineering solution for the high-resolution optical spectrograph on Gemini South

Jul 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998spie.3355..315c&link_type=abstract

Proc. SPIE Vol. 3355, p. 315-323, Optical Astronomical Instrumentation, Sandro D'Odorico; Ed.

Computer Science

Performance

Scientific paper

The High Resolution Optical Spectrograph (HROS) will operate at the Cassegrain focus of the Gemini South telescope, at a resolving power of R equals 50,000. It will use an immersed echelle for dispersion, and fused-silica prisms for cross- dispersion. The instrument will weigh two tonnes and will need to meet stringent engineering performance requirements. This paper describes these requirements and the engineering approach used in the HROS design.

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