The Coude Echelle Spectrograph for the Lijiang 1.8m telescope

被引:4
|
作者
Wang, Xiao-Li [1 ,2 ]
Chang, Liang [1 ,2 ,5 ,6 ]
Wang, Lei [3 ]
Ji, Hang-Xin [3 ]
Xian, Hao [4 ]
Tang, Zhen [3 ]
Xin, Yu-Xin [1 ,2 ]
Wang, Chuan-Jun [1 ,2 ]
He, Shou-Sheng [1 ,2 ]
Zhang, Ju-Jia [1 ,2 ]
Lun, Bao-Li [1 ,2 ]
Wei, Kai [4 ]
Li, Xi-Qi [4 ]
Jiang, Xiao-Jun [5 ,6 ]
Wang, Hui-Juan [5 ,6 ]
Li, Hong-Bin [5 ]
Mao, Ji-Rong [1 ,2 ]
机构
[1] Chinese Acad Sci, Yunnan Observ, Kunming 650216, Yunnan, Peoples R China
[2] Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Kunming 650216, Yunnan, Peoples R China
[3] Chinese Acad Sci, Natl Astron Observ, Nanjing Inst Astron Opt & Technol, Nanjing 210042, Peoples R China
[4] Chinese Acad Sci, Inst Opt & Elect, Chengdu 610209, Peoples R China
[5] Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100101, Peoples R China
[6] Univ Chinese Acad Sci, Beijing 100049, Peoples R China
基金
美国国家科学基金会; 中国国家自然科学基金;
关键词
Instrumentation; spectrographs; methods; observational; techniques; spectroscopic;
D O I
10.1088/1674-4527/20/3/32
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Coude Echelle Spectrograph (CES) was originally mounted on Xinglong 2.16 m telescope in 1994. When the High Resolution Fiber-fed Spectrograph (HRS) was commissioned at Xinglong 2.16 m telescope, the red path of CES was moved to Lijiang 1.8 m telescope, following some redesign and reinstallation. The CES of Lijiang 1.8 m telescope has the spectral resolution (R = lambda/Delta lambda) ranging from 20000 to 50000 corresponding to different slit widths. With a 2k x 2k PI CCD, CES has a wavelength coverage between 570 nm to 1030 nm. In particular, the resolution of 37000 at 0.5 mm slit corresponds to 1.3 '' on the sky. The limiting magnitude is V = 11.5 with the use of the tip-tilt feedback system, and the S/N is about 40 for 1 hour exposure at 600 nm (R = 37000). During the installation of CES, the tip-tilt mirror technology had successfully fulfilled high precision guiding and tracking for high resolution spectral observation and significantly improved the observation efficiency.
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页数:8
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