NIAOT OpenIR  > 会议论文
Preparing first light of LAMOST
Xiangqun Cui
2008-08-27
会议录名称Ground-based and Airborne Telescopes II
卷号7012
期号7012
页码Vol.7012 04-1-7
会议日期2008-6-23
会议地点Marseille, France
会议主办者The International Society for Optical Engineering
出版者SPIE
摘要
Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) is an innovative telescope project with both large aperture (effective in 4 meters) and wide field of view (5 degrees) to achieve the large scale spectroscopic survey observation. It is a horizontal meridian reflecting Schmidt configuration realized by an active deformable Schmidt plate. For achieving such an ambitious project with limited budget, both its primary mirror (6.67m X 6.05m) and Schmidt plate (5.74m X 4.4m) are segmented. LAMOST project is expected to be completed before the end of 2008. The assembly and test of whole telescope and 16 spectrographs with 4000 optical fibers in its focal plane is going to be finished in August of 2008. With just its partial aperture, more than 200 optical fibers and one spectrograph, the scientific commissioning has been done and some preliminary results have been obtained. This paper introduces the progress of LAMOST project during 2007 and 2008, and presents the achievement in its technology which is also useful for the future extremely large telescopes.
关键词Large Astronomical Telescope Wide Field Of View Active Optics Segmented Mirror Multi-fiber Spectroscopy Survey
学科领域郭守敬望远镜(lamost)
文献类型会议论文
条目标识符http://ir.niaot.ac.cn/handle/114a32/562
专题会议论文
推荐引用方式
GB/T 7714
Xiangqun Cui. Preparing first light of LAMOST[C]:SPIE,2008:Vol.7012 04-1-7.
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
Preparing first ligh(732KB) 开放获取CC BY-NC-ND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
百度学术
百度学术中相似的文章
[Xiangqun Cui]的文章
必应学术
必应学术中相似的文章
[Xiangqun Cui]的文章
相关权益政策
暂无数据
收藏/分享
文件名: Preparing first light of LAMOST.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。