27 July 2016 Progress of Antarctic survey telescopes
Author Affiliations +
The Antarctic Survey Telescope-AST3 consists of three optical telescopes with 680mm primary mirror and 8 square degree field of view, mainly for observations of supernovas and extrasolar planets searching from Antarctic Dome A. The first two AST3 telescopes (AST3-1 and AST3-2) were successfully installed on Dome A by Chinese expedition team in Jan. 2012 and Jan. 2015 separately. Multi-anti-frost methods were designed for AST3-2 and the automatic observations are keeping on from March 2016. The best limited magnitude is 19.4m with exposure time 60s in G band. The third AST3 will have switchable interface for both optical camera and near infrared camera optimized for k dark band survey. Now the telescope is under development in NIAOT and the K-band camera is under development in AAO.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Xiangyan Yuan, Xiangyan Yuan, Shihai Yang, Shihai Yang, Bozhong Gu, Bozhong Gu, Xiaoyan Li, Xiaoyan Li, Fujjia Du, Fujjia Du, Zhengyang Li, Zhengyang Li, Haikun Wen, Haikun Wen, Haiping Lu, Haiping Lu, Lingzhe Xu, Lingzhe Xu, Ru Zhang, Ru Zhang, Yi Zhang, Yi Zhang, Xiangqun Cui, Xiangqun Cui, Lifan Wang, Lifan Wang, Zhaohui Shang, Zhaohui Shang, Ce Yu, Ce Yu, Bin Ma, Bin Ma, Yi Hu, Yi Hu, "Progress of Antarctic survey telescopes", Proc. SPIE 9906, Ground-based and Airborne Telescopes VI, 99061O (27 July 2016); doi: 10.1117/12.2232282; https://doi.org/10.1117/12.2232282


Introduction of Chinese SONG Telescope
Proceedings of SPIE (September 16 2012)
Introduction of a 2.5m telescope mount and its performance
Proceedings of SPIE (August 05 2010)
Atmospheric seeing measurements in the near infrared
Proceedings of SPIE (May 31 1994)

Back to Top