LAMOST project and its current status | |
Hongjun Su; Xiangqun Cui![]() | |
2003-02-01 | |
Source Publication | Large Ground-based Telescopes |
Volume | 4837 |
Issue | 4837 |
Pages | Vol.4837 26-35 |
Conference Date | 2002-8-22 |
Conference Place | Hawaii USA |
Funding Organization | The International Society for Optical Engineering |
Publisher | SPIE |
Abstract |
The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) is a quasi-meridian reflecting Schmidt telescope with a clear aperture of 4-meter, a focal length of 20-meter and a field of view of 5-degree, dedicated for spectroscopic sky survey. The telescope will be located at the Xinglong Station of National Astronomical Observatory,
China, as a national facility open to the astronomical community. The project was planned to be completed in 2004,with its budget of RMB 235 millions yuan (about 28 M$). The project is well in progress, with various sub-systems and their parts in critical reviews or kick-out for manufacturing early or late. Here we report the current status of the project generally. Other authors in this conference will describe details for individual parts of the project. |
Keyword | Astronomical Telescope Active Optics Multi-fiber Spectroscopy |
Subject Area | 郭守敬望远镜(lamost) |
Document Type | 会议论文 |
Identifier | http://ir.niaot.ac.cn/handle/114a32/359 |
Collection | 会议论文 |
Recommended Citation GB/T 7714 | Hongjun Su,Xiangqun Cui. LAMOST project and its current status[C]:SPIE,2003:Vol.4837 26-35. |
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