The first data release (DR1) of the LAMOST regular survey

By A. Luo, Yongheng Zhao, Gang Zhao, Licai Deng, Xiaowei Liu, Yipeng Jing, Gang Wang, Hao-Tong Zhang, Jian-rong Shi, X. Cui and 135 more. 2015

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The GALAH Survey: Second Data Release (2018, background): “LAMOST is a lower spectral resolution (R ∼ 1800) survey but has observed a far greater number of stars than other surveys, with over 1.5 million stellar spectra collected to date (Luo et al. 2015).”
The Pristine survey - I. Mining the Galaxy for the most metal-poor stars (2017, background): “In addition to the SDSS/SEGUE sample, 21,969 Pristine stars are also present with measurements for their velocities and metallicities in the DR2 of the LAMOST survey (Cui et al. 2012; Xiang et al. 2015; Luo et al. 2015).”
The biggest splash (2019, background): “In order to increase our sample size, we now explore a larger catalogue of K-giants from the LAMOST survey (Luo et al. 2015).”
Mapping the Milky Way with LAMOST– III. Complicated spatial structure in the outer disc (2018, methodology): “We select the RGB stars from the LAMOST DR3 catalogue, which contains about 3.2 million stellar spectra with stellar parameter estimates based on the pipeline described by Luo et al. (2015).”