activity
20152021
most citedLAMOST Medium-Resolution Spectroscopic Survey (LAMOST-MRS): Scientific goals and survey plan

45 citations · 137 across the 6 of their papers we have counts for

collaborators

15 papers

astro-ph.SR20214 cited

Study on Outliers in the Big Stellar Spectral Dataset of the Fifth Data Release (DR5) of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST)

Yan Lu, A-Li Luo, Li-Li Wang +10

To study the quality of stellar spectra of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) and the correctness of the corresponding stellar parameters derive…

astro-ph.SR2021

Rotational Velocities of Am and Non-CP Stars based on Kepler and LAMOST DR5

Li Qin, A-Li Luo, Wen Hou +9

Rotation is a critical physical process operating in the formation of Am stars. There is a strong correlation between low-velocity rotation and chemical peculiarity. However, the e…

astro-ph.SR202011 cited

M Subdwarf Research. II. Atmospheric Parameters and Kinematics

Shuo Zhang, A-Li Luo, Georges Comte +12

Applying the revised M subdwarf classification criteria discussed in Paper I to LAMOST DR7, combining the M subdwarf sample from Savcheva et al, a new M subdwarf sample was constru…

astro-ph.SR202045 cited

LAMOST Medium-Resolution Spectroscopic Survey (LAMOST-MRS): Scientific goals and survey plan

Chao Liu, Jianning Fu, Jianrong Shi +38

Since September 2018, LAMOST starts a new 5-year medium-resolution spectroscopic survey (MRS) using bright/gray nights. We present the scientific goals of LAMOST-MRS and propose a…

astro-ph.SR2019

Properties of Radial Velocities measurement based on LAMOST-II Medium-Resolution Spectroscopic Observations

R. Wang, A. -L. Luo, J. -J. Chen +28

The radial velocity (RV) is a basic physical quantity which can be determined through Doppler shift of the spectrum of a star. The precision of RV measurement depends on the resolu…

astro-ph.GA2019

Bivariate Luminosity Function of Galaxy Pairs

Shuai Feng, Shi-Yin Shen, Fang-Ting Yuan +8

We measure the bivariate luminosity function (BLF) of galaxy pairs and use it to probe and characterize the galaxy-galaxy interaction between pair members. The galaxy pair sample i…