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The LEGUE high latitude bright survey design for the LAMOST pilot survey
Zhang, YY1,2; Carlin, JL3; Yang, F1,2; Liu, C1; Deng, LC1; Newberg, HJ3; Zhang, HT1; Lepine, S4; Xu, Y1; Gao, S1; Christlieb, N5; Han ZW(韩占文)6; Hou, JL7; Lee, HT8; Liu, XW9; Pan, KK10; Wang, HC11; Zhang, YY (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:792-804
DOI10.1088/1674-4527/12/7/007
产权排序第6完成单位
收录类别SCI
关键词Surveys: Lamost Techniques: Spectroscopic Galaxy: Stellar Content
摘要We describe the footprint and input catalog for bright nights in the LAMOST Pilot Survey, which began in October 2011. Targets are selected from two stripes in the north and south Galactic Cap regions, centered at delta = 29 degrees, with 10 degrees width in declination, covering right ascensions of 135 degrees to 290 degrees and -30 degrees to 30 degrees respectively. We selected spectroscopic targets from a combination of the SDSS and 2MASS point source catalogs. The catalog of stars defining the field centers (as required by the Shack-Hartmann wavefront sensor at the center of the LAMOST field) consists of all V < 8(m) stars from the Hipparcos catalog. We employ a statistical selection algorithm that assigns priorities to targets based on their positions in multidimensional color/magnitude space. This scheme overemphasizes rare objects and de-emphasizes more populated regions of magnitude and color phase space, while ensuring a smooth, well-understood selection function. A demonstration of plate design is presented based on the Shack-Hartmann star catalog and an input catalog that was generated by our target selection routines.
项目资助者National Natural Science Foundation of China [10573022, 10973015, 11061120454] ; Chinese Academy of Sciences [GJHZ 20081] ; US National Science Foundation [AST-09-37523]
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:000306892600007
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]DIGITAL SKY SURVEY ; CATALOG ; TARGETS
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被引频次:28[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/114a53/4532
专题大样本恒星演化研究组
通讯作者Zhang, YY (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 Astrophysics, Division of Physical Sciences, American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024, USA
4.Department of Physics, Applied Physics and Astronomy, Rensselaer Polytechnic Institute, 110 8th Street, Troy, NY 12180, USA
5.University of Heidelberg, Landessternwarte, Königstuhl 12, D-69117 Heidelberg, Germany
6.Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming 650011, China
7.Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China
8.Institute of Astronomy and Astrophysics, Academia Sinica, P.O. Box 23-141, Taipei 106, China
9.Department of Astronomy & Kavli Institute of Astronomy and Astrophysics, Peking University, Beijing 100871, China
10.Apache Point Observatory, PO Box 59, Sunspot, NM 88349, USA
11.Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China
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Zhang, YY,Carlin, JL,Yang, F,et al. The LEGUE high latitude bright survey design for the LAMOST pilot survey[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2012,12(7):792-804.
APA Zhang, YY.,Carlin, JL.,Yang, F.,Liu, C.,Deng, LC.,...&Zhang, YY .(2012).The LEGUE high latitude bright survey design for the LAMOST pilot survey.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,12(7),792-804.
MLA Zhang, YY,et al."The LEGUE high latitude bright survey design for the LAMOST pilot survey".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 12.7(2012):792-804.
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