Astronomical data reduction: LAMOST 2D pipeline, LAMOST survey strategy software
Binary star
stellar steams

The wavelength calibration accuracy of LAMOST 2D pipeline is about 4.5km/s which is about 3% of resolution unit (2.5？), and our sky subtraction accuracy  is better than SDSS.

With measuring flux of fiber at 3 positions around bright stars, we have measured the accuracy of fiber positioner and adjust the system error of fiber positioners to within 1" .

Sky Subtraction for LAMOST, Zhong-Rui Bai, Hao-Tong Zhang, Hai-Long Yuan, Guang-Wei Li, Jian-Jun Chen, Ya-Juan Lei, Hui-Qin Yang, Yi-Qiao Dong, Gang Wang  and Yong-Heng Zhao,2017,RAA, in press(arXiv:1705.02079).

Cosmic Ray Removal in Fiber Spectroscopic Image, Zhongrui Bai, Haotong Zhang, Hailong Yuan, et al. 2017, PASP, 129,024004

The effects of spectrograph slit modes on the accuracy of stellar radial velocity measurement and atmospheric parameter estimation, WANG FengFei, ZHANG HaoTong, LUO ALi1, BAI ZhongRui1, DU Bing & ZHAO YongHeng, 2013, Science China, Physics, Mechanics & Astronomy, 56, 1833

Moon night sky brightness simulation for the Xinglong station, Song Yao, Hao-Tong Zhang, Hai-Long Yuan, Yong-Heng Zhao, Yi-Qiao Dong, Zhong-Rui Bai1, Li-Cai Deng1 and Ya-Juan Lei1,2013,RAA, 13,1255