Kunlun Dark Universe Survey Telescope | |
Yongtian Zhu![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() | |
2014-07-22 | |
Source Publication | Ground-based and Airborne Telescopes V |
Volume | 9145 |
Pages | Vol.9145 0E-1-17 |
Conference Date | 2014-6-22 |
Conference Place | Montréal, Quebec, Canada |
Funding Organization | SPIE |
Publisher | SPIE |
Abstract |
Chinese Antarctic Observatory has been listed as National large research infrastructure during twelfth five-year plan. Kunlun Dark Universe Survey Telescope, one of two major facility of Chinese Antarctic Observatory, is a 2.5-meter optic/infrared telescope and will be built at the Chinese Antarctic Kunlun Station. It is intended to take advantage of the exceptional seeing conditions, as well as the low temperature reducing background for infrared observations. KDUST will adopt an innovative optical system, which can deliver very good image quality over a 2 square degree flat field of view. All of parts of it have been designed carefully to endure the extremely harsh environment. KDUST will be perched on a 14.5-meter-high tower to lift it above the turbulence layer. In this paper, preliminary design and key technology pre-research of KDUST will be introduced. |
Keyword | Ground-based Telescopes Optics/ir Antarctic |
Subject Area | 南极望远镜 |
Document Type | 会议论文 |
Identifier | http://ir.niaot.ac.cn/handle/114a32/799 |
Collection | 会议论文 |
Recommended Citation GB/T 7714 | Yongtian Zhu,Lifan Wang,Xiangyan Yuan,et al. Kunlun Dark Universe Survey Telescope[C]:SPIE,2014:Vol.9145 0E-1-17. |
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Kunlun Dark Universe(984KB) | 开放获取 | CC BY-NC-SA | View Download |
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