SKY BRIGHTNESS AND TRANSPARENCY IN THE i-BAND AT DOME A, ANTARCTICA
文献类型：期刊论文
| 作者 | 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
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| 刊名 | ASTRONOMICAL JOURNAL
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| 出版日期 | 2010-08-01 |
| 卷号 | 140期号:2页码:602-611 |
| ISSN号 | 0004-6256 |
| 关键词 | methods: data analysis methods: statistical techniques: photometric telescopes |
| 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 |
| 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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来源：紫金山天文台
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