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Overview of the LAMOST survey in the first decade

文献类型：期刊论文

作者Yan, Hongliang15,16; Li, Haining16; Wang, Song16; Zong, Weikai14; Yuan, Haibo14; Xiang, Maosheng13; Huang, Yang12; Xie, Jiwei10,11; Dong, Subo9; Yuan, Hailong16
刊名INNOVATION
出版日期2022-03-29
卷号3期号:2
ISSN号2666-6758
DOI10.1016/j.xinn.2022.100224
产权排序第12完成单位
文献子类Review
英文摘要

The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST), also known as the Guoshoujing Telescope, is a major national scientific facility for astronomical research located in Xinglong, China. Beginning with a pilot survey in 2011, LAMOST has been surveying the night sky for more than 10 years. The LAMOST survey covers various objects in the Universe, from normal stars to peculiar ones, from the Milky Way to other galaxies, and from stellar black holes and their companions to quasars that ignite ancient galaxies. Until the latest data release 8, the LAMOST survey has released spectra for more than 10 million stars, 220,000 galaxies, and 71,000 quasars. With this largest celestial spectra database ever constructed, LAMOST has helped astronomers to deepen their understanding of the Universe, especially for our Milky Way galaxy and the millions of stars within it. In this article, we briefly review the characteristics, observations, and scientific achievements of LAMOST. In particular, we show how astrophysical knowledge about the Milky Way has been improved by LAMOST data.

学科主题天文学 ; 恒星与银河系 ; 恒星天文学
URL标识查看原文
出版地STE 800, 230 PARK AVE, NEW YORK, NY 10169 USA
WOS关键词RED-GIANT BRANCH ; MILKY-WAY ; SPECTROSCOPIC SURVEY ; ANDROMEDA GALAXY ; METALLICITY GRADIENTS ; SOLAR NEIGHBORHOOD ; PRISTINE SURVEY ; GALACTIC DISK ; MAIN-SEQUENCE ; POOR STARS
资助项目National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11988101] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11973049] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11933004] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11890694] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[12090040] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[12090042] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[12090043] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[12090044] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11833002] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11833006] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[12022304] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11835057] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11973052] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11633005] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[12173007] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11933001] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11703035] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[U2031203] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[U1531244] ; National Key R&D Program of China[2019YFA0405100] ; National Key R&D Program of China[2019YFA0405500] ; National Key R&D Program of China[2019YFA0405502] ; National Key R&D Program of China[2019YFA0405503] ; National Key R&D Program of China[2019YFA0405504] ; National Key R&D Program of China[2016YFA0400804] ; National Key R&D Program of China[2019YFA0405000] ; Strategic Priority Research Program of the Chinese Academy of SciencesChinese Academy of Sciences[XDB34020205] ; Strategic Priority Research Program of the Chinese Academy of SciencesChinese Academy of Sciences[XDB41000000] ; Youth Innovation Promotion Association of the Chinese Academy of Sci-ences[2019060] ; Youth Innovation Promotion Association of the Chinese Academy of Sci-ences[Y202017] ; Youth Innovation Promotion Association of the Chinese Academy of Sci-ences[2019057] ; Youth Innovation Promotion Association of the Chinese Academy of Sci-ences[2020060] ; NAOC Nebula Talents Program ; Guoshoujing Telescope (LAMOST) ; National Major Scientific Project built by the Chinese Academy of Sciences ; Chinese Academy of SciencesChinese Academy of Sciences
WOS研究方向Science & Technology - Other Topics
语种英语
出版者ELSEVIER SCIENCE INC
WOS记录号WOS:000782121000002
资助机构National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11988101, 11973049, 11933004, 11890694, 12090040, 12090042, 12090043, 12090044, 11833002, 11833006, 12022304, 11835057, 11973052, 11633005, 12173007, 11933001, 11703035, U2031203, U1531244] ; National Key R&D Program of China[2019YFA0405100, 2019YFA0405500, 2019YFA0405502, 2019YFA0405503, 2019YFA0405504, 2016YFA0400804, 2019YFA0405000] ; Strategic Priority Research Program of the Chinese Academy of SciencesChinese Academy of Sciences[XDB34020205, XDB41000000] ; Youth Innovation Promotion Association of the Chinese Academy of Sci-ences[2019060, Y202017, 2019057, 2020060] ; NAOC Nebula Talents Program ; Guoshoujing Telescope (LAMOST) ; National Major Scientific Project built by the Chinese Academy of Sciences ; Chinese Academy of SciencesChinese Academy of Sciences
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/25078]  
专题云南天文台_大样本恒星演化研究组
通讯作者Zhao, Yongheng
作者单位1.Department of Astronomy, School of Physics, Peking University, Beijing 100871, China
2.WHU-NAOC Joint Center for Astronomy, Wuhan University, Wuhan 430072, China;
3.Key Laboratory of Space Astronomy and Technology, National Astronomical Observatories, CAS, Beijing 100101, China;
4.Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China;
5.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China;
6.CAS Key Laboratory of Astronomical Optics & Technology, Nanjing Institute of Astronomical Optics & Technology, Nanjing 210042, China;
7.National Astronomical Observatories/Nanjing Institute of Astronomical Optics & Technology, Chinese Academy of Sciences, Nanjing 210042, China;
8.University of Science and Technology of China, Hefei 230026, China;
9.Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, China;
10.Key Laboratory of Modern Astronomy and Astrophysics, Ministry of Education, Nanjing University, Nanjing 210093, China;
推荐引用方式
GB/T 7714		 Yan, Hongliang,Li, Haining,Wang, Song,et al. Overview of the LAMOST survey in the first decade[J]. INNOVATION,2022,3(2).
APA Yan, Hongliang.,Li, Haining.,Wang, Song.,Zong, Weikai.,Yuan, Haibo.,...&Zhao, Yongheng.(2022).Overview of the LAMOST survey in the first decade.INNOVATION,3(2).
MLA Yan, Hongliang,et al."Overview of the LAMOST survey in the first decade".INNOVATION 3.2(2022).

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来源：云南天文台

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