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20102026
most citedExoplanet Orbital Eccentricities Derived From LAMOST-Kepler Analysis

243 citations · 2.4k across the 71 of their papers we have counts for

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24 papers · 1 filter

astro-ph.SR2022★ 8 cited

The Properties and Evolutions of Starspots on Three Detached Eclipsing Binaries in the LAMOST-Kepler survey

Jiaxin Wang, Jianning Fu, Weikai Zong +4

The spotted detached eclipsing binary (DEB) offers insights into starspots on the binary. Three spotted DEBs, KIC 8097825, KIC 6859813, and KIC 5527172, which were observed by the…

astro-ph.SR2021★ 19 cited

The Lithium Abundances from the Large Sky Area Multi-object Fiber Spectroscopic Telescope Medium-resolution Survey. I. The Method

Qi Gao, Jian-Rong Shi, Hong-Liang Yan +9

Standard stellar evolution model predicts a severe depletion of lithium (Li) abundance during the first dredge-up process (FDU). Yet a small fraction of giant stars are still found…

astro-ph.SR2020★ 65 cited

Phase II of the LAMOST-Kepler/K2 survey. I. Time series of medium-resolution spectroscopic observations

Weikai Zong, Jian-Ning Fu, Peter De Cat +20

Phase \RNum{2} of the LAMOST-{\sl Kepler/K}2 survey (LK-MRS), initiated in 2018, aims at collecting medium-resolution spectra (; hereafter MRS) for more than s…

astro-ph.SR2019★ 3 cited

X-ray Activity from Different Types of Stars

Lin He, Song Wang, Xiaojie Xu +10

X-ray emission is an important indicator of stellar activity. In this paper, we study stellar X-ray activity using the XMM-Newton and LAMOST data for different types of stars. We p…

astro-ph.SR2018★ 44 cited

White dwarf-main sequence binaries from LAMOST: the DR5 catalogue

J. -J. Ren, A. Rebassa-Mansergas, S. G. Parsons +4

We present the data release (DR) 5 catalogue of white dwarf-main sequence (WDMS) binaries from the Large Area Multi-Object fiber Spectroscopic Telescope (LAMOST). The catalogue con…

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★ 1 cited

FGK 22 m Excess Stars in LAMOST DR2 Stellar Catalog

Chao-Jian Wu, Hong Wu, Kang Liu +8

Since the release of LAMOST (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope) catalog, we have the opportunity to use the LAMOST DR2 stellar catalog and \emph{WISE Al…

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★ 19 cited

Validation of LAMOST Stellar Parameters with the PASTEL Catalog

Hua Gao, Huawei Zhang, Maosheng Xiang +8

Recently the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) published its first data release (DR1), which is ranked as the largest stellar spectra dataset in th…

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…

astro-ph.SR2015★ 32 cited

A Large Sample of Am Candidates from LAMOST Data Release 1

Wen Hou, ALi Luo, Haifeng Yang +9

We present a sample of metallic-line star (Am) candidates from the Large sky Area Multi-Object fiber Spectroscopic Telescope Data Release one (LAMOST DR1). According to the charact…

astro-ph.SR2015★ 80 cited

Spectroscopic analysis of metal-poor stars from LAMOST: early results

Hai-Ning Li, Gang Zhao, Norbert Christlieb +5

We report on early results from a pilot program searching for metal-poor stars with LAMOST and follow-up high-resolution observation acquired with the MIKE spectrograph attached to…

astro-ph.SR2014★ 141 cited

LAMOST Spectroscopic Survey of the Galactic Anti-centre (LSS-GAC): target selection and the first release of value-added catalogues

Haibo Yuan, Xiaowei Liu, Zhiying Huo +16

As a major component of the LAMOST Galactic surveys, the LAMOST Spectroscopic Survey of the Galactic Anti-centre (LSS-GAC) aims to survey a significant volume of the Galactic thin/…

astro-ph.SR2014★ 58 cited

Stellar loci II. a model-free estimate of the binary fraction for field FGK stars

Haibo Yuan, Xiaowei Liu, Maosheng Xiang +2

We propose a Stellar Locus OuTlier (SLOT) method to determine the binary fraction of main-sequence stars statistically. The method is sensitive to neither the period nor mass-ratio…

astro-ph.SR2014★ 36 cited

White dwarf-main sequence binaries from LAMOST: the DR1 catalogue

Juanjuan Ren, Alberto Rebassa-Mansergas, Ali Luo +6

Context. White dwarf-main sequence (WDMS) binaries are used to study several different important open problems in modern astrophysics. Aims. The Sloan Digital Sky Survey (SDSS) ide…

astro-ph.SR2014★ 17 cited

Three Moving Groups Detected in the LAMOST DR1 Archive

Jingkun Zhao, Gang Zhao, Yuqin Chen +3

We analyze the kinematics of thick disk and halo stars observed by the Large sky Area Multi-Object Fiber Spectroscopic Telescope. We have constructed a sample of 7,993 F, G and K n…