Paper
27 July 2016 Progress of Antarctic survey telescopes
Author Affiliations +
Abstract
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, Shihai Yang, Bozhong Gu, Xiaoyan Li, Fujjia Du, Zhengyang Li, Haikun Wen, Haiping Lu, Lingzhe Xu, Ru Zhang, Yi Zhang, Xiangqun Cui, Lifan Wang, Zhaohui Shang, Ce Yu, Bin Ma, and Yi Hu "Progress of Antarctic survey telescopes", Proc. SPIE 9906, Ground-based and Airborne Telescopes VI, 99061O (27 July 2016); https://doi.org/10.1117/12.2232282
Lens.org Logo
CITATIONS
Cited by 1 scholarly publication.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Telescopes

Cameras

Domes

Astronomy

Computer programming

K band

K band

RELATED CONTENT

A 2.5m astronomical telescope project
Proceedings of SPIE (July 25 2008)
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 (June 01 1994)
The ELT situation in China
Proceedings of SPIE (April 22 2008)

Back to Top