Optical design for Antarctic Bright Star Survey Telescope

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	Optical design for Antarctic Bright Star Survey Telescope
	Zhengyang Li1,2 ; Haipin Lu1,2 ; Xiangyan Yuan1,2
	2015-10
发表期刊	CHINESE OPTICS LETTERS
卷号	13 期号:11 页码:111101-1-5
摘要	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.
语种	英语
文献类型	期刊论文
条目标识符	http://ir.niaot.ac.cn/handle/114a32/1183
专题	期刊论文
作者单位	1.Nanjing Institute of Astronomical Optics and Technology 2.Key Laboratory of Astronomical Optics & Technology,Chinese Academy of Sciences
推荐引用方式 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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