The i-band Sky brightness and Transparency at Dome A, Antarctica
Based on the observations of the Chinese Small Telescope ARray (CSTAR), the i band observing conditions at Antarctic Dome A have been investigated. The over all variations of sky brightness and transparency are calculated and subsequently cloud cover, contributions to the sky background from various...
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ftdatacite:10.48550/arxiv.1101.2362 2023-05-15T13:52:32+02:00 The i-band Sky brightness and Transparency at Dome A, Antarctica Zou, Hu Zhou, Xu 2011 https://dx.doi.org/10.48550/arxiv.1101.2362 https://arxiv.org/abs/1101.2362 unknown arXiv arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Instrumentation and Methods for Astrophysics astro-ph.IM FOS Physical sciences Preprint Article article CreativeWork 2011 ftdatacite https://doi.org/10.48550/arxiv.1101.2362 2022-04-01T14:29:24Z Based on the observations of the Chinese Small Telescope ARray (CSTAR), the i band observing conditions at Antarctic Dome A have been investigated. The over all variations of sky brightness and transparency are calculated and subsequently cloud cover, contributions to the sky background from various factors including aurorae are derived. The median sky brightness of moonless clear nights is about 20.5 mag arcsec$^{-2}$ in the SDSS i band at the South Celestial Pole, which contains the diffused Galactic light of about 0.06 mag. There are no thick clouds in the year of 2008. Relatively strong aurorae are detected by their brightening the normal sky, which contribute up to about 2 of the observed images. : Contribution in conference "Comprehensive characterization of astronomical sites", held October 4-10, 2010, in Kislovodsk, Russia Report Antarc* Antarctic Antarctica DataCite Metadata Store (German National Library of Science and Technology) Antarctic |
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DataCite Metadata Store (German National Library of Science and Technology) |
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ftdatacite |
language |
unknown |
topic |
Instrumentation and Methods for Astrophysics astro-ph.IM FOS Physical sciences |
spellingShingle |
Instrumentation and Methods for Astrophysics astro-ph.IM FOS Physical sciences Zou, Hu Zhou, Xu The i-band Sky brightness and Transparency at Dome A, Antarctica |
topic_facet |
Instrumentation and Methods for Astrophysics astro-ph.IM FOS Physical sciences |
description |
Based on the observations of the Chinese Small Telescope ARray (CSTAR), the i band observing conditions at Antarctic Dome A have been investigated. The over all variations of sky brightness and transparency are calculated and subsequently cloud cover, contributions to the sky background from various factors including aurorae are derived. The median sky brightness of moonless clear nights is about 20.5 mag arcsec$^{-2}$ in the SDSS i band at the South Celestial Pole, which contains the diffused Galactic light of about 0.06 mag. There are no thick clouds in the year of 2008. Relatively strong aurorae are detected by their brightening the normal sky, which contribute up to about 2 of the observed images. : Contribution in conference "Comprehensive characterization of astronomical sites", held October 4-10, 2010, in Kislovodsk, Russia |
format |
Report |
author |
Zou, Hu Zhou, Xu |
author_facet |
Zou, Hu Zhou, Xu |
author_sort |
Zou, Hu |
title |
The i-band Sky brightness and Transparency at Dome A, Antarctica |
title_short |
The i-band Sky brightness and Transparency at Dome A, Antarctica |
title_full |
The i-band Sky brightness and Transparency at Dome A, Antarctica |
title_fullStr |
The i-band Sky brightness and Transparency at Dome A, Antarctica |
title_full_unstemmed |
The i-band Sky brightness and Transparency at Dome A, Antarctica |
title_sort |
i-band sky brightness and transparency at dome a, antarctica |
publisher |
arXiv |
publishDate |
2011 |
url |
https://dx.doi.org/10.48550/arxiv.1101.2362 https://arxiv.org/abs/1101.2362 |
geographic |
Antarctic |
geographic_facet |
Antarctic |
genre |
Antarc* Antarctic Antarctica |
genre_facet |
Antarc* Antarctic Antarctica |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.1101.2362 |
_version_ |
1766256931395076096 |