Winter sky brightness and cloud cover at Dome A, Antarctica

• 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
• Other Authors: Burton, M. G., Cui, X., Tothill, N. F. H.
• Format: Article in Journal/Newspaper
• Language: English
• Published: 2012
• Subjects: Antarctic; Plato; The Antarctic; Antarc*; Antarctica
• Online Access: https://researchers.mq.edu.au/en/publications/e0ff592a-20de-4d38-a9f0-de7433aa3f3b; https://doi.org/10.1017/S174392131201664X; https://research-management.mq.edu.au/ws/files/62412354/Author%20final%20version.pdf; http://www.scopus.com/inward/record.url?scp=84873333595&partnerID=8YFLogxK

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.