Paper
1 June 1994 Upgrade of the McMath-Pierce stellar spectrograph
Mark S. Giampapa, Jorge E. Simmons, David B. Jaksha, E. L. Perkins
Author Affiliations +
Abstract
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.
© (1994) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Mark S. Giampapa, Jorge E. Simmons, David B. Jaksha, and E. L. Perkins "Upgrade of the McMath-Pierce stellar spectrograph", Proc. SPIE 2198, Instrumentation in Astronomy VIII, (1 June 1994); https://doi.org/10.1117/12.176706
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KEYWORDS
Prisms

Spectrographs

Charge-coupled devices

Optical components

Spectroscopy

Sensors

Observatories

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