| Optical design for Antarctic Bright Star Survey Telescope | |
Zhengyang Li1,2 ; Haipin Lu1,2; Xiangyan Yuan1,2
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| 2015-10 | |
| Source Publication | CHINESE OPTICS LETTERS
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| Volume | 13Issue: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 |
| Identifier | http://ir.niaot.ac.cn/handle/114a32/1183 |
| Collection | 期刊论文 |
| Affiliation | 1.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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| Optical design for A（781KB） | 期刊论文 | 作者接受稿 | 开放获取 | CC BY-NC-SA | View Download | |
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