NIAOT OpenIR  > 会议论文
Introduction on Chinese 12-m optical/infrared telescope(LOT)
Xiangqun Cui1,2; Yongtian Zhu1,2; Ding-qiang Su1,3; Xiangyan Yuan1,2; Zhongwen Hu1,2; Hua Bai1,2; Bozhong Gu1,2
2018-07-06
会议名称SPIE Ground-based and Airborne Telescopes VII(Vol.10700)
会议录名称Ground-based and Airborne Telescopes VII
会议日期2018-6-10
会议地点Austin, Texas, United States
其他摘要
Except for the spectroscopic survey telescope LAMOST, there are only two 2m class general purpose telescopes for precision observation in China (2.16m in Xinglong and 2.4m in Lijiang). Chinese astronomical community unanimously agrees that a 10m class large diameter general purpose optical/infrared telescope is urgently needed in China for a wide
range of scientific research. The configuration for LOT with primary aperture 12m has been selected by Chinese government for the Thirteen-five-years plan in July, 2016. The concept design introduced here has been approved by Chinese astronomical community and Chinese Academy of Sciences in Dec. 2017, and submitted into the formal funding procedure of Chinese government. For quite a long time, China will very likely have only one 10m class telescope, therefore LOT should be a general-purpose telescope including multi-foci. The Nasmyth focus, prime focus, Cassegrain focus and coudé focus have been considered or reserved. Also, LOT will closely combine with the development of new technologies, such as AO、GLAO、fiber and instrument related new technologies, to make it has powerful capability for the frontier sciences. The four-mirror Nasmyth system, optimized according to the GLAO requirements, has a f-ratio about 14 and field of view 14 arecmin with excellent image quality. Some off-axis four-mirror Nasmyth optical systems are also presented in this paper. The primary focus system has a f-ratio 2 and 1.5degree field of
view with 80% light energy encircled in 0.5 arecsec, which will let LOT complementary with the coming 30m-class telescopes. A double–layer Nasmyth platforms are proposed to accommodate more instruments, such as the wide field imaging spectrograph, broad band medium resolution spectrograph, high resolution spectrograph and multi-object fiber spectrographs and so on. Not all optical systems will be constructed in the same time,which will be in stages depending on the science and funding situation.
关键词Telescope High Angular Resolution Spectrograph Survey Glao
学科领域天文技术与方法
语种英语
文献类型会议论文
条目标识符http://ir.niaot.ac.cn/handle/114a32/1554
专题会议论文
作者单位1.南京天文光学技术研究所
2.天文光学技术重点实验室
3.南京大学
推荐引用方式
GB/T 7714
Xiangqun Cui,Yongtian Zhu,Ding-qiang Su,等. Introduction on Chinese 12-m optical/infrared telescope(LOT)[C],2018.
条目包含的文件 下载所有文件
文件名称/大小 文献类型 版本类型 开放类型 使用许可
Introduction on Chin(1397KB)会议论文 开放获取CC BY-NC-SA浏览 下载
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[Xiangqun Cui]的文章
[Yongtian Zhu]的文章
[Ding-qiang Su]的文章
百度学术
百度学术中相似的文章
[Xiangqun Cui]的文章
[Yongtian Zhu]的文章
[Ding-qiang Su]的文章
必应学术
必应学术中相似的文章
[Xiangqun Cui]的文章
[Yongtian Zhu]的文章
[Ding-qiang Su]的文章
相关权益政策
暂无数据
收藏/分享
文件名: Introduction on Chinese 12m optical_infrared telescope (LOT).pdf
格式: Adobe PDF
所有评论 (0)
暂无评论
 

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。