NIAOT OpenIR  > 中国科学院南京天文光学技术研究所  > 期刊论文
Optical design for Antarctic Bright Star Survey Telescope
Zhengyang Li1,2; Haipin Lu1,2; Xiangyan Yuan1,2
2015-10
Source PublicationCHINESE OPTICS LETTERS
Volume13Issue:11Pages:111101-1-5
Abstract
The exoplanet search is one of the most exciting research fields in astrophysics. The Antarctic Bright Star Survey Telescope (BSST), capable of continuous exoplanet observation on polar nights, is a Ritchey–Chretien telescope with a three-lens field corrector, and has a 300 mm aperture, 2.76 focal ratio, and a wavelength coverage ranging from 0.36 to 1.014 μm.
Equipped with a 4 k × 4 k and 12 μm∕pixel CCD camera, the BSST can gain a field of view of 4.8°. This Letter presents the optical design, tolerance analysis, and the alignment plan for the BSST, and the test observation results.
Language英语
Document Type期刊论文
Identifierhttp://ir.niaot.ac.cn/handle/114a32/1183
Collection中国科学院南京天文光学技术研究所_期刊论文
望远镜新技术研究室_期刊论文
南极天文技术中心_期刊论文
Affiliation1.Nanjing Institute of Astronomical Optics and Technology
2.Key Laboratory of Astronomical Optics & Technology,Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Zhengyang Li,Haipin Lu,Xiangyan Yuan. Optical design for Antarctic Bright Star Survey Telescope[J]. CHINESE OPTICS LETTERS,2015,13(11):111101-1-5.
APA Zhengyang Li,Haipin Lu,&Xiangyan Yuan.(2015).Optical design for Antarctic Bright Star Survey Telescope.CHINESE OPTICS LETTERS,13(11),111101-1-5.
MLA Zhengyang Li,et al."Optical design for Antarctic Bright Star Survey Telescope".CHINESE OPTICS LETTERS 13.11(2015):111101-1-5.
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