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The First Release of the CSTAR Point Source Catalog from Dome A, Antarctica
Zhou, Xu1; Fan, Zhou1; Jiang, Zhaoji1; Ashley, M. C. B.2; Cui, Xiangqun3; Feng, Longlong4; Gong, Xuefei3; Hu, Jingyao1; Kulesa, C. A.5; Lawrence, J. S.2,6; Liu, Genrong3; Luong-Van, D. M.2; Ma, Jun1; Moore, A. M.7; Qin, Weijia8; Shang, Zhaohui9; Storey, J. W. V.2; Sun, Bo; Travouillon, T.7; Walker, C. K.5; Wang, Jiali1; Wang, Lifan4; Wu, Jianghua1; Wu, Zhenyu1; Xia, Lirong3; Yan, Jun1; Yang, Ji4; Yang, Huigen8; Yuan, Xiangyan3; York, D.10,11; Zhang, Zhanhai8; Zhu, Zhenxi4
2010-03-01
发表期刊PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC
卷号122期号:889页码:347-353
摘要In 2008 January the twenty-fourth Chinese expedition team successfully deployed the Chinese Small Telescope ARray (CSTAR) to Dome A, the highest point on the Antarctic plateau. CSTAR consists of four 14.5 cm optical telescopes, each with a different filter (g, r, i, and open) and has a 4.5 degrees x 4.5 degrees field of view (FOV). It operates robotically as part of the Plateau Observatory, PLATO, with each telescope taking an image every similar to 30 s throughout the year whenever it is dark. During 2008, CSTAR 1 performed almost flawlessly, acquiring more than 0.3 million i-band images for a total integration time of 1728 hr during 158 days of observations. For each image taken under good sky conditions, more than 10,000 sources down to similar to 16(th) magnitude could be detected. We performed aperture photometry on all the sources in the field to create the catalog described herein. Since CSTAR has a fixed pointing centered on the south celestial pole (decl. = -90 degrees), all the sources within the FOV of CSTAR were monitored continuously for several months. The photometric catalog can be used for studying any variability in these sources, and for the discovery of transient sources such as supernovae, gamma-ray bursts, and minor planets.
收录类别SCI
语种英语
WOS记录号WOS:000275129700008
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文献类型期刊论文
条目标识符http://ir.bao.ac.cn/handle/114a11/7714
专题光学天文研究部
作者单位1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
2.Univ New S Wales, Sch Phys, Sydney, NSW 2052, Australia
3.Nanjing Inst Astron Opt & Technol, Nanjing 210042, Peoples R China
4.Purple Mt Observ, Nanjing 210008, Peoples R China
5.Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
6.Anglo Australian Observ, Epping, NSW 2121, Australia
7.CALTECH, Dept Astron, Pasadena, CA 91125 USA
8.Polar Res Inst China, Shanghai 200136, Peoples R China
9.Tianjin Normal Univ, Tianjin 300074, Peoples R China
10.Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
11.Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA
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Zhou, Xu,Fan, Zhou,Jiang, Zhaoji,et al. The First Release of the CSTAR Point Source Catalog from Dome A, Antarctica[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC,2010,122(889):347-353.
APA Zhou, Xu.,Fan, Zhou.,Jiang, Zhaoji.,Ashley, M. C. B..,Cui, Xiangqun.,...&Zhu, Zhenxi.(2010).The First Release of the CSTAR Point Source Catalog from Dome A, Antarctica.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC,122(889),347-353.
MLA Zhou, Xu,et al."The First Release of the CSTAR Point Source Catalog from Dome A, Antarctica".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC 122.889(2010):347-353.
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