NIAOT OpenIR  > 中国科学院南京天文光学技术研究所  > 会议论文
Kunlun Dark Universe Survey Telescope
Yongtian Zhu; Lifan Wang; Xiangyan Yuan; Bozhong Gu; Xinnan Li; Shihai Yang; Xuefei Gong; Fujia Du; Yongjun Qi; Linzhe Xu
2014-07-22
Source PublicationGround-based and Airborne Telescopes V
Volume9145
PagesVol.9145 0E-1-17
Conference Date2014-6-22
Conference PlaceMontréal, Quebec, Canada
Funding OrganizationSPIE
PublisherSPIE
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.
KeywordGround-based Telescopes Optics/ir Antarctic
Subject Area南极望远镜
Document Type会议论文
Identifierhttp://ir.niaot.ac.cn/handle/114a32/799
Collection中国科学院南京天文光学技术研究所_会议论文
望远镜新技术研究室_会议论文
大口径光学技术研究室_会议论文
望远镜工程中心_会议论文
南极天文技术中心_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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