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SKY BRIGHTNESS AND TRANSPARENCY IN THE i-BAND AT DOME A, ANTARCTICA
Zou, Hu1,2; Zhou, Xu1,3; Jiang, Zhaoji1,3; Ashley, M. C. B.4; Cui, Xiangqun3,5; Feng, Longlong3; Gong, Xuefei3,5; Hu, Jingyao1,3; Kulesa, C. A.6; Lawrence, J. S.7; Liu, Genrong5; Luong-Van, D. M.4; Ma, Jun1; Moore, A. M.8; Pennypacker, C. R.9; Qin, Weijia10; Shang, Zhaohui11; Storey, J. W. V.4; Sun, Bo10; Travouillon, T.9; Walker, C. K.6; Wang, Jiali1,3; Wang, Lifan3; Wu, Jianghua1; Wu, Zhenyu1; Xia, Lirong5; Yan, Jun1,3; Yang, Ji3; Yang, Huigen10; Yao, Yongqiang1; Yuan, Xiangyan3,5; York, D. G.12,13; Zhang, Zhanhai10; Zhu, Zhenxi3
2010-08-01
发表期刊ASTRONOMICAL JOURNAL
卷号140期号:2页码:602-611
摘要The i-band observing conditions at Dome A on the Antarctic plateau have been investigated using data acquired during 2008 with the Chinese Small Telescope Array. The sky brightness, variations in atmospheric transparency, cloud cover, and the presence of aurorae are obtained from these images. The median sky brightness of moonless clear nights is 20.5 mag arcsec(-2) in the SDSS i band at the south celestial pole (which includes a contribution of about 0.06 mag from diffuse Galactic light). The median over all Moon phases in the Antarctic winter is about 19.8 mag arcsec(-2). There were no thick clouds in 2008. We model contributions of the Sun and the Moon to the sky background to obtain the relationship between the sky brightness and transparency. Aurorae are identified by comparing the observed sky brightness to the sky brightness expected from this model. About 2% of the images are affected by relatively strong aurorae.
关键词Methods: Data Analysis Methods: Statistical Techniques: Photometric Telescopes
DOI10.1088/0004-6256/140/2/602
收录类别SCI
语种英语
WOS记录号WOS:000279958000026
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文献类型期刊论文
条目标识符http://ir.bao.ac.cn/handle/114a11/7822
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.Chinese Acad Sci, Grad Univ, Beijing 100049, Peoples R China
3.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
4.Univ New S Wales, Sch Phys, Sydney, NSW 2052, Australia
5.Nanjing Inst Astron Opt & Technol, Nanjing 210042, Peoples R China
6.Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
7.Macquarie Univ, Dept Phys, N Ryde, NSW 2109, Australia
8.CALTECH, Dept Astron, Pasadena, CA 91125 USA
9.Univ Calif Berkeley, Lawrence Berkeley Lab, Berkeley, CA 94720 USA
10.Polar Res Inst China, Shanghai 200136, Peoples R China
11.Tianjin Normal Univ, Tianjin 300074, Peoples R China
12.Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA
13.Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
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Zou, Hu,Zhou, Xu,Jiang, Zhaoji,et al. SKY BRIGHTNESS AND TRANSPARENCY IN THE i-BAND AT DOME A, ANTARCTICA[J]. ASTRONOMICAL JOURNAL,2010,140(2):602-611.
APA Zou, Hu.,Zhou, Xu.,Jiang, Zhaoji.,Ashley, M. C. B..,Cui, Xiangqun.,...&Zhu, Zhenxi.(2010).SKY BRIGHTNESS AND TRANSPARENCY IN THE i-BAND AT DOME A, ANTARCTICA.ASTRONOMICAL JOURNAL,140(2),602-611.
MLA Zou, Hu,et al."SKY BRIGHTNESS AND TRANSPARENCY IN THE i-BAND AT DOME A, ANTARCTICA".ASTRONOMICAL JOURNAL 140.2(2010):602-611.
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