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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
刊名ASTRONOMICAL JOURNAL
2010-08-01
卷号140期号:2页码:602-611
关键词methods: data analysis methods: statistical techniques: photometric telescopes
ISSN号0004-6256
英文摘要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.
学科主题Astronomy & Astrophysics
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]2-M CLASS TELESCOPE ; SITE ; PILOT ; PHOTOMETRY ; CATALOG ; CSTAR
收录类别SCI
语种英语
WOS记录号WOS:000279958000026
公开日期2011-11-23
内容类型期刊论文
源URL[http://159.226.72.40/handle/332002/1195]  
专题紫金山天文台_南极天文中心
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
推荐引用方式
GB/T 7714
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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