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The LEGUE input catalog for dark night observing in the LAMOST pilot survey
Yang, F1,2; Carlin, JL3; Liu, C1; Zhang, YY1,2; Gao, S1; Xu, Y1; Deng, LC1; Newberg, HJ3; Lepine, S4; Hou, JL5; Liu, XW6; Christlieb, N7; Zhang, HT1; Lee, HT8; Pan, KK9; Han ZW(韩占文)10; Wang, HC11; Yang, F (reprint author), Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China.
发表期刊RESEARCH IN ASTRONOMY AND ASTROPHYSICS
2012-07
卷号12期号:7页码:781-791
DOI10.1088/1674-4527/12/7/006
产权排序第10完成单位
收录类别SCI
关键词Surveys: Lamost Galaxy: Halo Techniques: Spectroscopic
摘要We outline the design of the dark nights portion of the LAMOST Pilot Survey, which began observations in 2011 October. In particular, we focus on Milky Way stellar candidates that are targeted for the LEGUE (LAMOST Experiment for Galactic Understanding and Exploration) survey. We discuss the regions of sky in which spectroscopic candidates were selected, and the motivations for selecting each of these sky areas. Some limitations due to the unique design of the telescope are discussed, including the requirement that a bright (V < 8) star be placed at the center of each plate for wavefront sensing and active optics corrections. The target selection categories and scientific goals motivating them are briefly discussed, followed by a detailed overview of how these selection functions were implemented. We illustrate the difference between the overall input catalog - Sloan Digital Sky Survey (SDSS) photometry and the final targets selected for LAMOST observations.
项目资助者National Natural Science Foundation of China [10573022, 10973015, 11061120454] ; US National Science Foundation through AST [09-37523] ; Chinese Academy of Sciences [GJHZ 200812]
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN1674-4527
URL查看原文
WOS记录号WOS:000306892600006
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]COLD STELLAR STREAM ; DIGITAL SKY SURVEY ; GALACTIC HALO ; DATA RELEASE ; 1ST DATA ; SDSS ; TARGETS ; DEBRIS
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被引频次:26[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/4531
专题大样本恒星演化研究组
通讯作者Yang, F (reprint author), Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China.
作者单位1.Key Lab for Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
2.Graduate University of Chinese Academy of Sciences, Beijing 100049, China
3.Department of Physics, Applied Physics and Astronomy, Rensselaer Polytechnic Institute, 110 8th Street, Troy, NY 12180, USA
4.American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024, USA
5.Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China
6.Department of Astronomy & Kavli Institute of Astronomy and Astrophysics, Peking University, Beijing 100871, China
7.University of Heidelberg, Landessternwarte, Königstuhl 12, D-69117 Heidelberg, Germany
8.Institute of Astronomy and Astrophysics, Academia Sinica, P.O. Box 23-141, Taipei 106, China
9.Apache Point Observatory, P.O. Box 59, Sunspot, NM 88349, USA
10.Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming 650011, China
11.Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China
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Yang, F,Carlin, JL,Liu, C,et al. The LEGUE input catalog for dark night observing in the LAMOST pilot survey[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2012,12(7):781-791.
APA Yang, F.,Carlin, JL.,Liu, C.,Zhang, YY.,Gao, S.,...&Yang, F .(2012).The LEGUE input catalog for dark night observing in the LAMOST pilot survey.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,12(7),781-791.
MLA Yang, F,et al."The LEGUE input catalog for dark night observing in the LAMOST pilot survey".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 12.7(2012):781-791.
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