| Autor: |
Genrong Liu, Yong-Hui Hou, Zhi-Gang Liu, Dan Wang, A-Li Luo, Li Men, Haotong Zhang, Guohua Zhou, Hong-Zhuan Hu, Yin-Dun Mao, J. N. Zhang, Hongjun Su, Jianling Wang, Zhongwen Hu, Yao-Quan Chu, Li Xinnan, Fang-Hua Jiang, Yongtian Zhu, Zhaoxiang Qi, L. P. Zhang, Hai-Yuan Chen, Ming Zhao, Xiao-Zheng Xing, Jia-Ning Wang, Ying Chen, Ya-nan Wang, Shu-Yun Cao, Shihai Yang, Xin-Qi Xu, Yue-Fei Wang, Bozhong Gu, Lei Jia, Yong-Heng Zhao, Yan Xu, Jia-Ru Chu, Ge Jin, Jie Zhu, Zheng-Qiu Yao, Hai Wang, H.-L. Yuan, Xuefei Gong, Jian-Ping Wang, Xiangqun Cui, Kunxin Chen, Fang Zhou, Yong Zhang, Lingzhe Xu, Z. B. Jiang, Qi Li, Yanxia Zhang, Xiangyan Yuan, Gang Wang, D. Wang, Lei Feng, Xiang Jiang, Wen-Zhi Lu, Zhenchao Zhang, Ning-Sheng Hu, Yong-Jun Qi, Dehua Yang, Qing-Sheng Tao, Aihua Li, Huo-Ming Shi, Lei Wang, Yan Li, Jian-Jun Chen, Guan-Qun Liu, Jian Wang, Guoping Li, Shu-Qing Wang, Si-Cheng Zou, Chao Zhai, Yong Yu, Zheng-Hong Tang, Guo-Min Wang, You Wang, Ye-Ping Li |
| Rok vydání: |
2012 |
| Předmět: |
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| Zdroj: |
ResearcherID |
| ISSN: |
1674-4527 |
| Popis: |
The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST, also called the Guo Shou Jing Telescope) is a special reflecting Schmidt telescope. LAMOST's special design allows both a large aperture (effective aperture of 3.6 m–4.9 m) and a wide field of view (FOV) (5°). It has an innovative active reflecting Schmidt configuration which continuously changes the mirror's surface that adjusts during the observation process and combines thin deformable mirror active optics with segmented active optics. Its primary mirror (6.67 m × 6.05 m) and active Schmidt mirror (5.74m × 4.40m) are both segmented, and composed of 37 and 24 hexagonal sub-mirrors respectively. By using a parallel controllable fiber positioning technique, the focal surface of 1.75 m in diameter can accommodate 4000 optical fibers. Also, LAMOST has 16 spectrographs with 32 CCD cameras. LAMOST will be the telescope with the highest rate of spectral acquisition. As a national large scientific project, the LAMOST project was formally proposed in 1996, and approved by the Chinese government in 1997. The construction started in 2001, was completed in 2008 and passed the official acceptance in June 2009. The LAMOST pilot survey was started in October 2011 and the spectroscopic survey will launch in September 2012. Up to now, LAMOST has released more than 480000 spectra of objects. LAMOST will make an important contribution to the study of the large-scale structure of the Universe, structure and evolution of the Galaxy, and cross-identification of multi-waveband properties in celestial objects. |
| Databáze: |
OpenAIRE |
| Externí odkaz: |
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