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观测天体光谱的纤维光学方法及2.16m望远镜实用系统

The Astronomical Fiber Optical Spectroscopy System of the BAO 2.16m Telescope

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【作者】 王顺德冉隆均余宁邹振隆

【Author】 Wang Shunde Ran Longjun Yu Ning Zou Zhenlong(Beijing Astronomical Observatory, Chinese Academy of Sciences) (Joint Laboratory for Optical Astronomy)

【机构】 北京天文台北京天文台 北京 100080 光学天文联合开放实验室北京 100080 光学天文联合开放实验室北京 100080 光学天文联合开放实验室

【摘要】 本文描述了近年来广泛发展起来的天体物理实测技术中的一项重要进展——纤维光学分光技术方法在天体光谱观测中的应用及2.16m望远镜实用系统的特点和初步应用结果

【Abstract】 The advantage of astronomical fiber optical spectroscopy system and its performances of the 2.16m telescope at the Beijing Astronomical Observatory (BAO) as well as some typical results obtained by this fiber system are described in this paper.The working systems include single-object all-fiber-coupler (AFC system) and multi-object fiber system ("Spider" system). The AFC system can found all functions requiring for observations: acquisition, guiding, transmission and calibration. As it is as small as a finger, it can be easily attached onto any focal plane of any telescopes. The "spider" system has 20 fiber probes which are positioned with Blink Comparator according to the original plate taken at the telescoper or a paper target field printed w th laser printer. The fiber probe includes a tiny pristn which is glued with the imput end of the fiber with optical epoxy and assembled inside a button which a small magnet is glued on its bottom. The method positioning fiber on star plate is easier and cheaper than that on dirll-star plate.The fiber systems have been completed in he end of 1989 and operated successfully at the 2.16m telescope.

【基金】 国家自然科学基金;天文基金联合支持项目
  • 【文献出处】 Chinese Journal of Astronomy and Astrophysics ,中国天文和天体物理学报(英文版) , 编辑部邮箱 ,1992年04期
  • 【下载频次】44
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