Real-time atmospheric extinction variation analysis with the Photometric Telescope at Xinglong Observatory
文献类型:期刊论文
作者 | Zhao, Yong1,2; Fan, Zhou2![]() |
刊名 | ASTROPHYSICS AND SPACE SCIENCE
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出版日期 | 2020-01-15 |
卷号 | 365期号:1页码:9 |
关键词 | Astronomical instrumentation Methods and techniques Techniques photometric |
ISSN号 | 0004-640X |
DOI | 10.1007/s10509-020-3726-6 |
英文摘要 | We present the Photometric Auxiliary System (PAS) attached to the 25-cm Photometric Telescope (PT) at Xinglong Observatory of National Astronomical Observatories, Chinese Academy of Sciences (NAOC). This PAS can provide real-time atmospheric extinction for other telescopes at the same station for flux calibration via observing standard stars, e.g. the 2.16-m reflector and 1-m telescope. Moreover, the real-time atmospheric extinction could act as a useful reference for other local telescopes regarding the adjustment of observing strategies, such as changing the exposure time, which is important for the observers. This PAS has been operated since February 2012, and we have obtained the r-band atmospheric extinction of Xinglong Observatory from February 2012 to March 2018. With these data, we have analyzed the atmospheric extinction of Xinglong Observatory in detail. |
WOS关键词 | ASTRONOMICAL OBSERVING CONDITIONS ; BRIGHTNESS |
资助项目 | Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Joint Research Fund in Astronomy National Natural Science Foundation of China[U1831209] ; National Program on Key Research and Development Project[2016YFA0400804] ; National Key Basic Research Program of China (973 Program)[2015CB857002] ; National Natural Science Foundation of China (NFSC)[11503045] ; National Natural Science Foundation of China (NFSC)[11373003] |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:000519588400002 |
出版者 | SPRINGER |
资助机构 | Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Joint Research Fund in Astronomy National Natural Science Foundation of China ; Joint Research Fund in Astronomy National Natural Science Foundation of China ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; National Key Basic Research Program of China (973 Program) ; National Key Basic Research Program of China (973 Program) ; National Natural Science Foundation of China (NFSC) ; National Natural Science Foundation of China (NFSC) ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Joint Research Fund in Astronomy National Natural Science Foundation of China ; Joint Research Fund in Astronomy National Natural Science Foundation of China ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; National Key Basic Research Program of China (973 Program) ; National Key Basic Research Program of China (973 Program) ; National Natural Science Foundation of China (NFSC) ; National Natural Science Foundation of China (NFSC) ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Joint Research Fund in Astronomy National Natural Science Foundation of China ; Joint Research Fund in Astronomy National Natural Science Foundation of China ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; National Key Basic Research Program of China (973 Program) ; National Key Basic Research Program of China (973 Program) ; National Natural Science Foundation of China (NFSC) ; National Natural Science Foundation of China (NFSC) ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Joint Research Fund in Astronomy National Natural Science Foundation of China ; Joint Research Fund in Astronomy National Natural Science Foundation of China ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; National Key Basic Research Program of China (973 Program) ; National Key Basic Research Program of China (973 Program) ; National Natural Science Foundation of China (NFSC) ; National Natural Science Foundation of China (NFSC) |
源URL | [http://ir.bao.ac.cn/handle/114a11/56211] ![]() |
专题 | 中国科学院国家天文台 |
通讯作者 | Zhao, Yong |
作者单位 | 1.Univ Chinese Acad Sci, Beijing 100049, Peoples R China 2.Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China 3.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China |
推荐引用方式 GB/T 7714 | Zhao, Yong,Fan, Zhou,Ge, Liang,et al. Real-time atmospheric extinction variation analysis with the Photometric Telescope at Xinglong Observatory[J]. ASTROPHYSICS AND SPACE SCIENCE,2020,365(1):9. |
APA | Zhao, Yong.,Fan, Zhou.,Ge, Liang.,Ren, Juanjuan.,Tian, Jianfeng.,...&Jiang, Xiaojun.(2020).Real-time atmospheric extinction variation analysis with the Photometric Telescope at Xinglong Observatory.ASTROPHYSICS AND SPACE SCIENCE,365(1),9. |
MLA | Zhao, Yong,et al."Real-time atmospheric extinction variation analysis with the Photometric Telescope at Xinglong Observatory".ASTROPHYSICS AND SPACE SCIENCE 365.1(2020):9. |
入库方式: OAI收割
来源:国家天文台
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