activity
20132018
most citedExoplanet Orbital Eccentricities Derived From LAMOST-Kepler Analysis

243 citations · 1.1k across the 36 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

12 papers · 1 filter

astro-ph.SR2018★ 11 cited

Misclassified B stars in the Kepler field

Chunguang Zhang, Chao Liu, Yue Wu +7

Stellar fundamental parameters are important in the asteroseismic study of Kepler light curves. However, the most used estimates in the Kepler Input Catalog (KIC) are not accurate…

astro-ph.SR2018★ 66 cited

Carbon stars identified from LAMOST DR4 using Machine Learning

Yin-Bi Li, A-Li Luo, Chang-De Du +27

In this work, we present a catalog of 2651 carbon stars from the fourth Data Release (DR4) of the Large Sky Area Multi-Object Fiber Spectroscopy Telescope (LAMOST). Using an effici…

astro-ph.SR2016★ 99 cited

Estimating stellar atmospheric parameters, absolute magnitudes and elemental abundances from the LAMOST spectra with Kernel-based Principal Component Analysis

Maosheng Xiang, Xiaowei Liu, Jianrong Shi +16

Accurate determination of stellar atmospheric parameters and elemental abundances is crucial for Galactic archeology via large-scale spectroscopic surveys. In this paper, we estima…

astro-ph.SR2016★ 44 cited

LAMOST observations in the Kepler field. Analysis of the stellar parameters measured with the LASP based on the low-resolution spectra

Anbing Ren, Jianning Fu, Peter De Cat +12

All of the 14 subfields of the Kepler field have been observed at least once with the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST, Xinglong Observatory, China…

astro-ph.SR2016★ 25 cited

The LAMOST spectroscopic survey of star clusters in M31. II. Metallicities, ages and masses

Chen Bingqiu, Liu Xiaowei, Xiang Maosheng +14

We select from Paper I a sample of 306 massive star clusters observed with the Large Sky Area Multi-Object Fibre Spectroscopic Telescope (LAMOST) in the vicinity fields of M31 and…

astro-ph.SR2016★ 16 cited

A catalogue of early-type emission-line stars and Hα line profiles from LAMOST DR2

Wen Hou, ALi Luo, Jingyao Hu +9

We present a catalogue including 11,204 spectra for 10,436 early-type emission-line stars from LAMOST DR2, among which 9,752 early-type emission-line spectra are newly discovered.…

astro-ph.SR2016★ 23 cited

Calibration of LAMOST Stellar Surface Gravities Using the Kepler Asteroseismic Data

Liang Wang, Wei Wang, Yue Wu +7

Asteroseismology is a powerful tool to precisely determine the evolutionary status and fundamental properties of stars. With the unprecedented precision and nearly continuous photo…

astro-ph.SR2016★ 130 cited

Label Transfer from APOGEE to LAMOST: Precise Stellar Parameters for 450,000 LAMOST Giants

Anna Y. Q. Ho, Melissa K. Ness, David W. Hogg +6

In this era of large-scale stellar spectroscopic surveys, measurements of stellar attributes ("labels," i.e. parameters and abundances) must be made precise and consistent across s…

astro-ph.SR2015★ 14 cited

On the LSP3 estimates of surface gravity for LAMOST-Kepler stars with asteroseismic measurements

Juan-Juan Ren, Xiao-Wei Liu, Mao-Sheng Xiang +13

Asteroseismology allows for deriving precise values of surface gravity of stars. The accurate asteroseismic determinations now available for large number of stars in the Kepler fie…

astro-ph.SR2015★ 26 cited

An independent test of the photometric selection of white dwarf candidates using LAMOST DR3

N. P. Gentile Fusillo, A. Rebassa-Mansergas, B. T. Gänsicke +7

In Gentile Fusillo et al. (2015) we developed a selection method for white dwarf candidates which makes use of photometry, colours and proper motions to calculate a probability of…

astro-ph.SR2015★ 8 cited

Member candidates of the star clusters from LAMOST DR2 data

Bo Zhang, Xiao-Yan Chen, Chao Liu +10

In this work, we provide 2189 photometric- and kinematic-selected member candidates of 24 star clusters from the LAMOST DR2 catalog. We perform two-step membership identification:…

astro-ph.SR2015

Spectral classification of stars based on LAMOST spectra

Chao Liu, Wen-Yuan Cui, Bo Zhang +6

In this work, we select the high signal-to-noise ratio spectra of stars from the LAMOST data andmap theirMK classes to the spectral features. The equivalentwidths of the prominent…