Winter sky brightness and cloud cover at Dome A, Antarctica

Abstract 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 Ant...

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Bibliographic Details
Published in:Proceedings of the International Astronomical Union
Main Authors: Moore, Anna M., Yang, Yi, Fu, Jianning, Ashley, Michael C. B., Cui, Xiangqun, Feng, Long Long, 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
Format: Article in Journal/Newspaper
Language:English
Published: Cambridge University Press (CUP) 2012
Subjects:
Astronomy and Astrophysics
Space and Planetary Science
Antarctic
Plato
The Antarctic
Antarc*
Antarctica
Online Access:http://dx.doi.org/10.1017/s174392131201664x
https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S174392131201664X
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Summary:Abstract 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.

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