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.
引用
收藏
页数:8
相关论文
共 50 条
  • [21] Steel maker fined £1.8m
    不详
    PROFESSIONAL ENGINEERING, 1998, 11 (02) : 5 - 5
  • [22] φ1.8m磨机节能改造
    邱国潮
    福建能源开发与节约, 1997, (02) : 47 - 48
  • [23] The high-resolution Echelle Spectrograph of the 6-m telescope of the special astrophysical observatory
    V. E. Panchuk
    V. G. Klochkova
    M. V. Yushkin
    Astronomy Reports, 2017, 61 : 820 - 831
  • [24] FIDEOS: a high resolution echelle spectrograph for the ESO 1m telescope at La Silla
    Tala, M.
    Berdja, A.
    Jones, M.
    Vanzi, L.
    Ropert, S.
    Flores, M.
    Viscasillas Vazquez, Carlos
    GROUND-BASED AND AIRBORNE INSTRUMENTATION FOR ASTRONOMY V, 2014, 9147
  • [25] Fabrication of 1.8M Standard Spherical Mirror
    Yu, Jun
    Shen, Shidong
    Pan, Junhe
    Mao, Yijiang
    Mu, Yongji
    Hu, Mingyong
    6TH INTERNATIONAL SYMPOSIUM ON ADVANCED OPTICAL MANUFACTURING AND TESTING TECHNOLOGIES: LARGE MIRRORS AND TELESCOPES, 2012, 8415
  • [26] FEROS, the new fiber-linked echelle spectrograph for the ESO 1.52-m telescope
    Kaufer, A
    Pasquini, L
    OPTICAL ASTRONOMICAL INSTRUMENTATION, PTS 1 AND 2, 1998, 3355 : 844 - 854
  • [27] The high-resolution Echelle Spectrograph of the 6-m telescope of the special astrophysical observatory
    Panchuk, V. E.
    Klochkova, V. G.
    Yushkin, M. V.
    ASTRONOMY REPORTS, 2017, 61 (09) : 820 - 831
  • [28] First light of the deformable secondary mirror-based adaptive optics system on 1.8m telescope
    Guo, Youming
    Zhang, Ang
    Fan, Xinlong
    Rao, Changhui
    Wei, Ling
    Xian, Hao
    Wei, Kai
    Zhang, Xiaojun
    Guan, Chunlin
    Li, Min
    Zhou, Luchun
    Jin, Kai
    Zhang, Junbo
    Zhou, Longfeng
    Zhang, Xuejun
    Zhang, Yudong
    ADAPTIVE OPTICS SYSTEMS V, 2016, 9909
  • [29] Performance and results with the NIRSPEC echelle spectrograph on the Keck II Telescope
    McLean, IS
    Graham, JR
    Becklin, EE
    Figer, DF
    Larkin, J
    Levenson, N
    Teplitz, HI
    OPTICAL AND IR TELESCOPE INSTRUMENTATION AND DETECTORS, PTS 1 AND 2, 2000, 4008 : 1048 - 1055
  • [30] First light for the sodium laser guide star adaptive optics system on the Lijiang 1.8 m telescope
    Wei, Kai
    Li, Min
    Chen, Shan-Qiu
    Bo, Yong
    Chen, Feng
    Zuo, Jun-Wei
    Bian, Qi
    Yao, Ji
    Zhou, Lu-Chun
    Wei, Lin
    Chen', Dong-Hong
    Gao, Yang
    Jin, Kai
    Dai, Xiao-Lin
    Fu, Han-Chu
    Xu, Chang
    Wang, Zhi-Chao
    Xue, Xiang -Hui
    Chen, Xue-Wu
    Qian, Xian-Mei
    Zhou, Yu
    Xian, Hao
    Peng, Qin-Jun
    Rao, Chang-Hui
    Xu, Zu-Yan
    Zhang, Yu-Dong
    RESEARCH IN ASTRONOMY AND ASTROPHYSICS, 2016, 16 (12)