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30m级光学/红外望远镜的宽视场多目标光谱仪
引用本文:季杭馨,胡中文,朱永田,许明明,戴松新,章华涛,汤振,王晋峰.30m级光学/红外望远镜的宽视场多目标光谱仪[J].天文学报,2019,60(4):67-86.
作者姓名:季杭馨  胡中文  朱永田  许明明  戴松新  章华涛  汤振  王晋峰
作者单位:中国科学院国家天文台南京天文光学技术研究所;中国科学院天文光学技术重点实验室(南京天文光学技术研究所);中国科学院大学
基金项目:国家自然科学基金项目(11503059、11603054、U1831108、11603053、11503061)资助
摘    要:宽视场多目标光谱仪具有宽波段、多分辨率模式和高通光效率的特点,是极大望远镜终端仪器使用率最高的通用型仪器. 30 m级望远镜的宽视场多目标光谱仪因体量和成本急剧增加而面临重要挑战,同时天文学的不断发展对天文新技术的发展提出了更高的要求,尤其是多个巡天项目对于多目标光谱后随观测的迫切需求.综述了几类宽视场多目标光谱仪的发展现状,介绍了国际3架30 m望远镜宽视场多目标光谱仪概念设计的最新进展和仪器特点,着重介绍了中国参与研制的30 m望远镜(TMT)中的宽视场多目标光谱仪的相关进展.

关 键 词:仪器:  光谱仪    望远镜    技术:  成像光谱技术    技术:  光谱学    方法:  分析
收稿时间:2019/2/12 0:00:00
修稿时间:2019/4/9 0:00:00

Wide Field Multi-object Spectrograph for 30 m Class Optical/Near Infrared Telescope
JI Hang-xin,HU Zhong-wen,ZHU Yong-tian,XU Ming-ming,DAI Song-xin,ZHANG Hua-tao,TANG Zhen and WANG Jin-feng.Wide Field Multi-object Spectrograph for 30 m Class Optical/Near Infrared Telescope[J].Acta Astronomica Sinica,2019,60(4):67-86.
Authors:JI Hang-xin  HU Zhong-wen  ZHU Yong-tian  XU Ming-ming  DAI Song-xin  ZHANG Hua-tao  TANG Zhen and WANG Jin-feng
Institution:National Astronomical Observatories/Nanjing Institute of Astronomical Optics & Technology, Chinese Academy of Sciences, Nanjing 210042;CAS Key Laboratory of Astronomical Optics & Technology, Nanjing Institute of Astronomical Optics & Technology, Nanjing 210042;University of Chinese Academy of Sciences, Beijing 100049,National Astronomical Observatories/Nanjing Institute of Astronomical Optics & Technology, Chinese Academy of Sciences, Nanjing 210042;CAS Key Laboratory of Astronomical Optics & Technology, Nanjing Institute of Astronomical Optics & Technology, Nanjing 210042,National Astronomical Observatories/Nanjing Institute of Astronomical Optics & Technology, Chinese Academy of Sciences, Nanjing 210042;CAS Key Laboratory of Astronomical Optics & Technology, Nanjing Institute of Astronomical Optics & Technology, Nanjing 210042,National Astronomical Observatories/Nanjing Institute of Astronomical Optics & Technology, Chinese Academy of Sciences, Nanjing 210042;CAS Key Laboratory of Astronomical Optics & Technology, Nanjing Institute of Astronomical Optics & Technology, Nanjing 210042,National Astronomical Observatories/Nanjing Institute of Astronomical Optics & Technology, Chinese Academy of Sciences, Nanjing 210042;CAS Key Laboratory of Astronomical Optics & Technology, Nanjing Institute of Astronomical Optics & Technology, Nanjing 210042,National Astronomical Observatories/Nanjing Institute of Astronomical Optics & Technology, Chinese Academy of Sciences, Nanjing 210042;CAS Key Laboratory of Astronomical Optics & Technology, Nanjing Institute of Astronomical Optics & Technology, Nanjing 210042,National Astronomical Observatories/Nanjing Institute of Astronomical Optics & Technology, Chinese Academy of Sciences, Nanjing 210042;CAS Key Laboratory of Astronomical Optics & Technology, Nanjing Institute of Astronomical Optics & Technology, Nanjing 210042 and National Astronomical Observatories/Nanjing Institute of Astronomical Optics & Technology, Chinese Academy of Sciences, Nanjing 210042;CAS Key Laboratory of Astronomical Optics & Technology, Nanjing Institute of Astronomical Optics & Technology, Nanjing 210042
Abstract:Due to its wide wavelength coverage, multi-resolution mode, and high efficiency, wide field multi-object spectrograph become the work-horse general purpose instrument for the extremely large telescope. It''s still a great challenge to build wide field multi-object spectrograph for a 30 m class telescope with sharply increasing volume and budget. With the great development of astronomy and astrophysics, new astronomical technology is essentially required. In this paper, the research progress of different wide field multi-object spectrographs is illustrated and reviewed, especially with the introduction about the recent status of conceptual design and their instrument features from three 30 m class telescope international projects. It also introduces the current effort made by the China''s team to the TMT (Thirty Meter Telescope)-WFOS (Wide Field multi-Object Spectrograph).
Keywords:instrumentation: spectrographs  telescope  techniques: imaging spectroscopy  techniques: spectroscopic  methods: analytical
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