Winter sky brightness and cloud cover at Dome A, Antarctica
At the summit of the Antarctic plateau, Dome A offers an intriguing location for future large scale optical astronomical observatories. The Gattini Dome A project was created to measure the optical sky brightness and large area cloud cover of the winter-time sky above this high altitude Antarctic si...
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ftcaltechauth:oai:authors.library.caltech.edu:rd7b4-e1e70 2024-06-23T07:46:42+00:00 Winter sky brightness and cloud cover at Dome A, Antarctica Moore, Anna M. Yang, Yi Fu, Jianning Ashley, Michael C. B. Cui, Xiangqun Feng, LongLong Gong, Xuefei Hu, Zhongwen Lawrence, Jon S. Luong-van, Daniel M. Riddle, Reed Shang, Zhaohui Sims, Geoff Storey, John W. V. Tothill, Nicholas F. H. Travouillon, Tony Wang, Lifan Yang, Huigen Yang, Ji Zhou, Xu Zhu, Zhenxi Burton, Michael G. Cui, Xiangqun Tothill, Nicholas F. H. 2013 https://doi.org/10.1017/S174392131201664X unknown Cambridge University Press https://doi.org/10.1017/S174392131201664X oai:authors.library.caltech.edu:rd7b4-e1e70 eprintid:41618 resolverid:CaltechAUTHORS:20131002-131453985 info:eu-repo/semantics/openAccess Other 288th symposium of the International Astronomical Union, Beijing, China, August 20-24, 2012 site testing surveys info:eu-repo/semantics/bookPart 2013 ftcaltechauth https://doi.org/10.1017/S174392131201664X 2024-06-12T05:10:56Z At the summit of the Antarctic plateau, Dome A offers an intriguing location for future large scale optical astronomical observatories. The Gattini Dome A project was created to measure the optical sky brightness and large area cloud cover of the winter-time sky above this high altitude Antarctic site. The wide field camera and multi-filter system was installed on the PLATO instrument module as part of the Chinese-led traverse to Dome A in January 2008. This automated wide field camera consists of an Apogee U4000 interline CCD coupled to a Nikon fisheye lens enclosed in a heated container with glass window. The system contains a filter mechanism providing a suite of standard astronomical photometric filters (Bessell B, V, R) and a long-pass red filter for the detection and monitoring of airglow emission. The system operated continuously throughout the 2009, and 2011 winter seasons and part-way through the 2010 season, recording long exposure images sequentially for each filter. We have in hand one complete winter-time dataset (2009) returned via a manned traverse. We present here the first measurements of sky brightness in the photometric V band, cloud cover statistics measured so far and an estimate of the extinction. © 2013 International Astronomical Union. Published online: 30 January 2013. The research is supported by the Chinese PANDA International Polar Year project and the Polar Research Institute of China. The project was funded by the following awards from the National Science Foundation Office of Polar Programs: ANT 0836571, ANT 0909664 and ANT 1043282. We thank Shri Kulkarni and Caltech Optical Observatories, Gerard Van Belle and Chas Beichman for financial contribution to this project. The operation of PLATO at Dome A is supported by the Australian Research Council, the Australian Antarctic Division, and the University of New South Wales. The authors wish to thank all the members of the 2008/2009/2010 PRIC Dome A heroic expeditions. Published - Moore_2012p34.pdf Book Part Antarc* Antarctic Antarctica Australian Antarctic Division International Polar Year National Science Foundation Office of Polar Programs Polar Research Institute of China Caltech Authors (California Institute of Technology) Antarctic Plato ENVELOPE(-54.674,-54.674,-63.433,-63.433) The Antarctic Proceedings of the International Astronomical Union 8 S288 34 37 |
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Caltech Authors (California Institute of Technology) |
op_collection_id |
ftcaltechauth |
language |
unknown |
topic |
site testing surveys |
spellingShingle |
site testing surveys Moore, Anna M. Yang, Yi Fu, Jianning Ashley, Michael C. B. Cui, Xiangqun Feng, LongLong Gong, Xuefei Hu, Zhongwen Lawrence, Jon S. Luong-van, Daniel M. Riddle, Reed Shang, Zhaohui Sims, Geoff Storey, John W. V. Tothill, Nicholas F. H. Travouillon, Tony Wang, Lifan Yang, Huigen Yang, Ji Zhou, Xu Zhu, Zhenxi Winter sky brightness and cloud cover at Dome A, Antarctica |
topic_facet |
site testing surveys |
description |
At the summit of the Antarctic plateau, Dome A offers an intriguing location for future large scale optical astronomical observatories. The Gattini Dome A project was created to measure the optical sky brightness and large area cloud cover of the winter-time sky above this high altitude Antarctic site. The wide field camera and multi-filter system was installed on the PLATO instrument module as part of the Chinese-led traverse to Dome A in January 2008. This automated wide field camera consists of an Apogee U4000 interline CCD coupled to a Nikon fisheye lens enclosed in a heated container with glass window. The system contains a filter mechanism providing a suite of standard astronomical photometric filters (Bessell B, V, R) and a long-pass red filter for the detection and monitoring of airglow emission. The system operated continuously throughout the 2009, and 2011 winter seasons and part-way through the 2010 season, recording long exposure images sequentially for each filter. We have in hand one complete winter-time dataset (2009) returned via a manned traverse. We present here the first measurements of sky brightness in the photometric V band, cloud cover statistics measured so far and an estimate of the extinction. © 2013 International Astronomical Union. Published online: 30 January 2013. The research is supported by the Chinese PANDA International Polar Year project and the Polar Research Institute of China. The project was funded by the following awards from the National Science Foundation Office of Polar Programs: ANT 0836571, ANT 0909664 and ANT 1043282. We thank Shri Kulkarni and Caltech Optical Observatories, Gerard Van Belle and Chas Beichman for financial contribution to this project. The operation of PLATO at Dome A is supported by the Australian Research Council, the Australian Antarctic Division, and the University of New South Wales. The authors wish to thank all the members of the 2008/2009/2010 PRIC Dome A heroic expeditions. Published - Moore_2012p34.pdf |
author2 |
Burton, Michael G. Cui, Xiangqun Tothill, Nicholas F. H. |
format |
Book Part |
author |
Moore, Anna M. Yang, Yi Fu, Jianning Ashley, Michael C. B. Cui, Xiangqun Feng, LongLong Gong, Xuefei Hu, Zhongwen Lawrence, Jon S. Luong-van, Daniel M. Riddle, Reed Shang, Zhaohui Sims, Geoff Storey, John W. V. Tothill, Nicholas F. H. Travouillon, Tony Wang, Lifan Yang, Huigen Yang, Ji Zhou, Xu Zhu, Zhenxi |
author_facet |
Moore, Anna M. Yang, Yi Fu, Jianning Ashley, Michael C. B. Cui, Xiangqun Feng, LongLong Gong, Xuefei Hu, Zhongwen Lawrence, Jon S. Luong-van, Daniel M. Riddle, Reed Shang, Zhaohui Sims, Geoff Storey, John W. V. Tothill, Nicholas F. H. Travouillon, Tony Wang, Lifan Yang, Huigen Yang, Ji Zhou, Xu Zhu, Zhenxi |
author_sort |
Moore, Anna M. |
title |
Winter sky brightness and cloud cover at Dome A, Antarctica |
title_short |
Winter sky brightness and cloud cover at Dome A, Antarctica |
title_full |
Winter sky brightness and cloud cover at Dome A, Antarctica |
title_fullStr |
Winter sky brightness and cloud cover at Dome A, Antarctica |
title_full_unstemmed |
Winter sky brightness and cloud cover at Dome A, Antarctica |
title_sort |
winter sky brightness and cloud cover at dome a, antarctica |
publisher |
Cambridge University Press |
publishDate |
2013 |
url |
https://doi.org/10.1017/S174392131201664X |
long_lat |
ENVELOPE(-54.674,-54.674,-63.433,-63.433) |
geographic |
Antarctic Plato The Antarctic |
geographic_facet |
Antarctic Plato The Antarctic |
genre |
Antarc* Antarctic Antarctica Australian Antarctic Division International Polar Year National Science Foundation Office of Polar Programs Polar Research Institute of China |
genre_facet |
Antarc* Antarctic Antarctica Australian Antarctic Division International Polar Year National Science Foundation Office of Polar Programs Polar Research Institute of China |
op_source |
288th symposium of the International Astronomical Union, Beijing, China, August 20-24, 2012 |
op_relation |
https://doi.org/10.1017/S174392131201664X oai:authors.library.caltech.edu:rd7b4-e1e70 eprintid:41618 resolverid:CaltechAUTHORS:20131002-131453985 |
op_rights |
info:eu-repo/semantics/openAccess Other |
op_doi |
https://doi.org/10.1017/S174392131201664X |
container_title |
Proceedings of the International Astronomical Union |
container_volume |
8 |
container_issue |
S288 |
container_start_page |
34 |
op_container_end_page |
37 |
_version_ |
1802647579339522048 |