Upgrade of the McMath-Pierce stellar spectrograph

Details Upgrade of the McMath-Pierce stellar spectrograph Upgrade of the McMath-Pierce stellar spectrograph

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994spie.2198..302g&link_type=abstract

Proc. SPIE Vol. 2198, p. 302-308, Instrumentation in Astronomy VIII, David L. Crawford; Eric R. Craine; Eds.

Astronomy and Astrophysics

Astronomy

Scientific paper

We discuss a design for an echelle spectrograph based on three prisms as the cross-dispersing optical elements. Since high throughput in our particular system is achieved using an image slicer, obtaining adequate order separation is a challenge. We find that the design described herein yields good efficiencies throughout the visible wavelength range while also providing adequate order separation in the red.

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