Zobrazeno 1 - 10
of 49
pro vyhledávání: '"Ding-qiang Su"'
Publikováno v:
Research in Astronomy and Astrophysics. 21:132
In the first part of this paper, four different Cassegrain optical systems with their correctors are designed and studied for multi-object fiber slit spectroscopic survey. The aperture in 6.5 m and field of view 3° are taken for these optical system
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 469:3792-3801
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 460:2286-2295
This is an optical/infrared telescope. It is a general purpose telescope. A segmented primary mirror is adopted with diameter 12 m and f-ratio 1.6. This telescope has prime focus, Cassegrain, Nasmyth and coud´e systems. The prime focus system has a
Publikováno v:
Research in Astronomy and Astrophysics. 20:001
FAST, the largest single-dish radio telescope in the world, has a 500-meter diameter main reflector and a 300-meter diameter illumination area. It has a shape variable main reflector, which changes the shape of the illuminated area in the main reflec
Autor:
Zhongwen Hu, Xiangyan Yuan, Ming Liang, Yongtian Zhu, Hua Bai, Ding-qiang Su, Xiangqun Cui, Bozhong Gu
Publikováno v:
Ground-based and Airborne Telescopes VII.
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 clas
Autor:
Ding-qiang Su, Xiangqun Cui
Publikováno v:
Research in Astronomy and Astrophysics. 14:1055-1060
China will establish a 2-meter space-based astronomical telescope. Its main science goals are performing a sky survey for research about dark matter and dark energy, and high resolution observations. Some experts suggest that this space telescope sho
Autor:
Yongtian Zhu, Genrong Liu, Lin He, Xiao-Zheng Xing, Kunxin Chen, Wen-Zhi Lu, Peng Du, Yong-Hui Hou, Ning-Sheng Hu, Wei Zhang, Ya-nan Wang, Xiang-Xiang Xue, Jian Li, Wen Hou, Jianrong Shi, Hailong Yuan, Ge Jin, M. Zhao, Haotong Zhang, A-Li Luo, Gang Wang, Hongjun Su, Zhi-Gang Liu, Xin-Nan Li, Ye-Ping Li, Yan Xu, Xiang Jiang, Xiangqun Cui, Hui-Qin Yang, Yong-Jun Qi, Yu Luo, En-Peng Zhang, Zheng-Hong Tang, Guan-Qun Liu, Dan Wang, Hong-Zhuan Hu, Zheng-Qiu Yao, Guang-Wei Li, Ding-qiang Su, J. Song, Yao-Quan Chu, Shu-Yun Cao, Yong Zhang, Yue Wu, Y. Yu, Liang-Ping Tu, J. N. Zhang, Xuefei Gong, Yuan Tian, Shou-Guan Wang, Aihua Li, Yin-Dun Mao, Fang Zhou, Guo-Min Wang, Lingzhe Xu, Yin-Bi Li, Zhongwen Hu, Bing Du, Z. B. Jiang, Qi Li, Yanxia Zhang, L. P. Zhang, You Wang, Li Men, Zhaoxiang Qi, Yue-Fei Wang, Xiao Kong, Shi-Wei Sun, Fengfei Wang, Ying Chen, Meng-Xin Wang, Huo-Ming Shi, Lei Wang, Gang Zhao, Qi-Shuai Lu, Xin-Qi Xu, Jia-Ru Chu, Guoping Li, Jian-Ping Wang, Shu-Qing Wang, Yi-Han Song, Lei Jia, Si-Cheng Zou, Chao Zhai, Fang-Hua Jiang, Jian-Nan Zhang, Jian Wang, Yan Li, Jian-Jun Chen, Ji-Jun Ni, Jie Zhu, Yong-Heng Zhao, Zhong-Rui Bai, Zhenchao Zhang, Lei Feng, Qing-Sheng Tao, Yajuan Lei, Dehua Yang, Xin-Lin Zhou, Jia-Ning Wang, Hai-Yuan Chen, Yi-Qiao Dong, H.-L. Yuan, Ming-Zhi Wei, Shi-Hai Yang, Hai Wang, Shuang Li, Da-Qing Wang, Zhi-Ying Huo, Ke-Fei Wu, Yan-Xin Guo, Bozhong Gu, Jianling Wang, Fang Zuo, Xiao-Yan Chen
Publikováno v:
ResearcherID
This paper describes the data release of the LAMOST pilot survey, which includes data reduction, calibration, spectral analysis, data products and data access. The accuracy of the released data and the information about the FITS headers of spectra ar
Autor:
Xiangqun Cui, Xuefei Gong, Xiangyan Yuan, Ding-qiang Su, Yongtian Zhu, Bozhong Gu, Li Xinnan, Lifan Wang
Publikováno v:
Proceedings of the International Astronomical Union. 8:271-274
From theoretical analysis and site testing work for 4 years on Dome A, Antarctica, we can reasonably predict that it is a very good astronomical site, as good as or even better than Dome C and suitable for observations ranging from optical to infrare
Autor:
Xiangyan Yuan, Ding-qiang Su
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 424:23-30
Dome A is the highest point on the Antarctic Plateau, and the Chinese Expedition Team first arrived here in 2005 January. It is an excellent site for astronomical observations. The first-generation Chinese Antarctic optical telescope CSTAR has been o
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 419:3406-3413
The Large Sky Area Multi–object Fibre Spectroscopic Telescope (LAMOST) is the largest (aperture 4 m) wide field of view (FOV) telescope and is equipped with the largest amount (4000) of optical fibres in the world. For the LAMOST North and the LAMO