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Several Possible Designs for BFOSC

Published online by Cambridge University Press:  12 April 2016

Jiang Shi-Yang*
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100080, China

Abstract

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Various optical solutions are presented for the Beijing Faint Object Spectrograph and Camera of Beijing Astrophysical Observatory 2.16 m telescope. They are based either on dioptric or catoptric designs including an adaptation of the existing Cassegrain spectrograph.

Type
1. Basic Principles, Focal Reducers
Copyright
Copyright © Astronomical Society of the Pacific 1995