Luo A-Li1, Zhang Hao-Tong1, Zhao Yong-Heng1, Zhao Gang1, Cui Xiang-Qun2, Li Guo-Ping2, Chu Yao-Quan3, Shi Jian-Rong1, Wang Gang1, Zhang Jian-Nan1, Bai Zhong-Rui1, Chen Xiao-Yan1, Wang Feng-Fei1, Guo Yan-Xin1, Chen Jian-Jun1, Du Bing1, Kong Xiao1, Lei Ya-Juan1, Li Yin-Bi1, Song Yi-Han1, Wu Yue1, Zhang Yan-Xia1, Zhou Xin-Lin1, Zuo Fang1, Du Peng1, He Lin1, Hou Wen1, Dong Yi-Qiao1, Li Jian1, Li Guang-Wei1, Li Shuang1, Song Jing1, Tian Yuan1, Wang Meng-Xin1, Wu Ke-Fei1, Yang Hui-Qin1, Yuan Hai-Long1, Cao Shu-Yun1, Chen Hai-Yuan2, Chen Kun-Xin2, Chen Ying1, Chu Jia-Ru3, Feng Lei1, Gong Xue-Fei2, Gu Bo-Zhong2, Hou Yong-Hui2, Huo Zhi-Ying1, Hu Hong-Zhuan3, Hu Ning-Sheng2, Hu Zhong-Wen2, Jia Lei1, Jiang Fang-Hua2, Jiang Xiang2, Jiang Zi-Bo2, Jin Ge3, Li Ai-Hua2, Li Qi1, Li Xin-Nan2, Li Yan4, Li Ye-Ping2, Liu Gen-Rong2, Liu Guan-Qun2, Liu Zhi-Gang3, Lu Qi-Shuai2, Lu Wen-Zhi2, Luo Yu1, Mao Yin-Dun4, Men Li1, Ni Ji-Jun2, Qi Yong-Jun2, Qi Zhao-Xiang4, Shi Huo-Ming1, Su Ding-Qiang2, Sun Shi-Wei1, Su Hong-Jun1, Tang Zheng-Hong4, Tao Qing-Sheng2, Tu Liang-Ping1, Wang Da-Qing1, Wang Dan1, Wang Guo-Min2, Wang Hai2, Wang Jia-Ning2, Wang Jian3, Wang Jian-Ling1, Wang Jian-Ping3, Wang Lei2, Wang Shou-Guan1, Wang Shu-Qing1, Wang Ya-Nan2, Wang You2, Wang Yue-Fei2, Wei Ming-Zhi1, Xue Xiang-Xiang1, Xing Xiao-Zheng3, Xu Ling-Zhe2, Xu Xin-Qi2, Xu Yan1, Yang De-Hua2, Yang Shi-Hai2, Yao Zheng-Qiu2, Yu Yong4, Yuan Hui1, Zhai Chao3, Zhang En-Peng1, Zhang Jing5, Zhang Li-Ping2, Zhang Wei1, Zhang Yong2, Zhang Zhen-Chao2, Zhao Ming4, Zhou Fang2, Zhu Yong-Tian2, Zhu Jie2 and Zou Si-Cheng1
2012 National Astronomical Observatories of Chinese Academy of Sciences and IOP Publishing Ltd.
Research in Astronomy and Astrophysics,
Volume 12,
Number 9
Citation Luo A-Li et al 2012 Res. Astron. Astrophys.12 1243DOI 10.1088/1674-4527/12/9/004
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 are also introduced. The released data set includes 319 000 spectra and a catalog of these objects.