Hostname: page-component-7bb8b95d7b-qxsvm Total loading time: 0 Render date: 2024-09-25T01:18:03.887Z Has data issue: false hasContentIssue false
  • English
  • Français

Several Possible Designs for BFOSC

Published online by Cambridge University Press:  12 April 2016

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

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
Information
International Astronomical Union Colloquium , Volume 149: Tridimensional Optical Spectroscopic Methods in Astrophysics , 1995 , pp. 29 - 32
Copyright
Copyright © Astronomical Society of the Pacific 1995