中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Focal surface attitude detection for LAMOST

文献类型:期刊论文

作者Hu TZ(胡天柱); Zhang Y(张勇); Cui XQ(崔向群); Li YP(李烨平); Pan XS(潘秀山); Fu Y(傅莹)
刊名Research in Astronomy and Astrophysics
出版日期2020-11
卷号20期号:11页码:181-191
关键词Methods: Data Analysis Techniques: High Angular Resolution Techniques: Image Processing
英文摘要
With telescope apertures becoming larger and larger, the deployment of large-field telescopes is becoming increasingly popular. However, optical path calibration is necessary to ensure the image quality of large-field and large-diameter telescopes. In particular, focal plane attitude calibration is an essential optical path calibration technique that has a direct impact on image quality. In this paper, a focal plane attitude detection method using eight acquisition cameras is proposed based on the calibration requirements of the wide-field telescope, LAMOST (Large Sky AreaMulti-Object Fiber Spectroscopic Telescope). Comparisonof simulation and experimental results shows that the detection accuracy of the proposed method can reach
30 arcsec.With additional testing and verification, this method could be used to facilitate regular focal plane attitude calibration for LAMOST as well as other large-field telescopes.
学科主题天文技术与方法
语种英语
源URL[http://ir.niaot.ac.cn/handle/114a32/1767]  
专题期刊论文
作者单位南京天文光学技术研究所
推荐引用方式
GB/T 7714
Hu TZ,Zhang Y,Cui XQ,et al. Focal surface attitude detection for LAMOST[J]. Research in Astronomy and Astrophysics,2020,20(11):181-191.
APA Hu TZ,Zhang Y,Cui XQ,Li YP,Pan XS,&Fu Y.(2020).Focal surface attitude detection for LAMOST.Research in Astronomy and Astrophysics,20(11),181-191.
MLA Hu TZ,et al."Focal surface attitude detection for LAMOST".Research in Astronomy and Astrophysics 20.11(2020):181-191.

入库方式: OAI收割

来源:南京天文光学技术研究所

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