activity
20142026
most citedExoplanet Orbital Eccentricities Derived From LAMOST-Kepler Analysis

243 citations · 622 across the 27 of their papers we have counts for

collaborators

27 papers

astro-ph.IM2026

A Gaia-linked High-purity QSO Candidate Catalog in Selected Fields with Extinction-binned Calibration and Spectrum-informed Training

Zi-Huang Cao, Zhao-Xiang Qi, Juan-Juan Ren +11

We present an extinction-calibrated, Gaia-source-level QSO candidate catalog for selected fields, designed as a high-purity input catalog for fiber-spectroscopic follow-up rather t…

astro-ph.IM2026

Evaluating the spatial intra-pixel sensitivity variations and influence based on space observation

Peipei Wang, Zihuang Cao, Chao Liu +3

Intra-pixel sensitivity variations (IPSVs) in charge-coupled devices (CCDs) and complementary metal-oxide-semiconductor (CMOS) detectors constitute a significant source of astromet…

astro-ph.IM2023★ 2 cited

Satellite Impact on Astronomical Observations Based on Elliptical Orbit Model

Tianzhu Hu, Yong Zhang, Xiangqun Cui +5

Space-based and ground-based telescopes have extensively documented the impact of satellites on astronomical observations. With the proliferation of satellite mega-constellation pr…

astro-ph.SR2022★ 20 cited

The Eclipsing Binaries from the LAMOST Medium-resolution Survey.III. A High-precision Empirical Stellar Mass Library

Jianping Xiong, Chao Liu, Jiao Li +6

High-precision stellar mass and radius measured directly from binaries can effectively calibrate the stellar models. However, such a database containing full spectral types and lar…

astro-ph.GA2021★ 2 cited

A catalog of quasar candidates identified by astrometric and mid-infrared methods in Gaia EDR3

Qiqi Wu, Shilong Liao, Zhaoxiang Qi +3

Quasars are very important in materializing the reference frame. The excess emission of AGNs (active galactic nuclei) in the mid infrared band can be used to identify quasar candid…

astro-ph.GA2018★ 15 cited

Identifying quasars with astrometric and mid-infrared methods from APOP and ALLWISE

Sufen Guo, Zhaoxiang Qi, Shilong Liao +5

Context. Quasars are spatially stationary, and they are essential objects in astrometry when defining reference frames. However, the census of quasars is far from complete. Mid-inf…

astro-ph.GA2018★ 19 cited

Metallicity and Kinematics of the Galactic halo from the LAMOST sample stars

Shuai Liu, Cuihua Du, Heidi Jo Newberg +8

We study the metallicity distribution and kinematic properties of 4,680 A/F/G/K-type giant stars with 5 kpc selected from the LAMOST spectroscopic survey. The metallicity di…

astro-ph.GA2018★ 17 cited

A compilation of known QSOs for the Gaia mission

Shi-long Liao, Zhao-xiang Qi, Su-fen Guo +1

Quasars are essential for astrometric in the sense that they are spatial stationary because of their large distance from the Sun. The European Space Agency (ESA) space astrometric…

astro-ph.GA2018★ 4 cited

The properties of the quasars astrometric solution in Gaia DR2

Shilong Liao, Beatric Bucciarelli, Zhaoxiang Qi +3

Gaia data release 2 (DR2) provides the best non-rotating optical frame aligned with the radio frame (ICRF) thanks to the inclusion of about half-million quasars in the 5-parameter…

cs.DC2018

A hybrid architecture for astronomical computing

Changhua Li, Chenzhou Cui, Boliang He +17

With many large science equipment constructing and putting into use, astronomy has stepped into the big data era. The new method and infrastructure of big data processing has becom…

astro-ph.GA2017★ 42 cited

Spectral classification and composites of galaxies in LAMOST DR4

Li-Li Wang, A-Li Luo, Shi-Yin Shen +10

We study the classification and composite spectra of galaxy in the fourth data release (DR4) of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST). We select 40…

astro-ph.GA2017★ 39 cited

Mapping the Milky Way with LAMOST II: the stellar halo

Yan Xu, Chao Liu, Xiang-Xiang Xue +9

The radial number density and flattening of the Milky Way's stellar halo is measured with metal-poor ([Fe/H]) K giants from LAMOST DR3, using a nonparametric m…

astro-ph.GA2017★ 5 cited

Quasars in the Galactic Anti-Center Area from the LAMOST DR3

Zhi-Ying Huo, Xiao-Wei Liu, Jian-Rong Shi +11

We present a sample of quasars discovered in the area of Galactic Anti-Center (GAC) of and , based on the LAMOST Data Rel…

astro-ph.IM2017★ 2 cited

AstroCloud: A Distributed Cloud Computing and Application Platform for Astronomy

Chenzhou Cui, Boliang He, Ce Yu +28

Virtual Observatory (VO) is a data-intensively online astronomical research and education environment, which takes advantages of advanced information technologies to achieve seamle…

astro-ph.GA2017★ 17 cited

The local spiral arm in the LAMOST-Gaia common stars?

Chao Liu, You-Gang Wang, Juntai Shen +7

Using the LAMOST-Gaia common stars, we demonstrate that the in-plane velocity field for the nearby young stars are significantly different from that for the old ones. For the young…

astro-ph.GA2017★ 12 cited

A sample of metal-poor galaxies identified from the LAMOST spectral survey

Yulong Gao, Jianhui Lian, Xu Kong +8

We present a sample of 48 metal-poor galaxies at selected from 92,510 galaxies in the LAMOST survey. These galaxies are identified for their detection of the auroral em…

astro-ph.GA2017★ 58 cited

Mapping the Milky Way with LAMOST I: Method and overview

Chao Liu, Yan Xu, Jun-Chen Wan +8

We present a statistical method to derive the stellar density profiles of the Milky Way from spectroscopic survey data, taking into account selection effects. We assume that the se…

astro-ph.EP2016★ 243 cited

Exoplanet Orbital Eccentricities Derived From LAMOST-Kepler Analysis

Ji-Wei Xie, Subo Dong, Zhaohuan Zhu +14

The nearly circular (mean eccentricity <e>~0.06) and coplanar (mean mutual inclination <i>~3 deg) orbits of the Solar System planets motivated Kant and Laplace to put forth the hyp…

astro-ph.GA2016★ 14 cited

Kinematics of the Galactic disk from LAMOST Dwarf sample

Yingjie Jing, Cuihua Du, Jiayin Gu +10

Based on the LAMOST survey and Sloan Digital Sky Survey (SDSS), we use low-resolution spectra of 130,043 F/G-type dwarf stars to study the kinematics and metallicity properties of…

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.GA2016★ 24 cited

The peculiar velocities in the Galactic outer disk--hints of the elliptical disk and the perturbation of the spiral structures

Hai-Jun Tian, Chao Liu, Jun-Chen Wan +7

We present the peculiar in-plane velocities derived from the LAMOST red clump stars. From the variations of the in-plane velocity with the Galactocentric radius for the young and o…

astro-ph.IM2016

Update of the China-VO AstroCloud

Chenzhou Cui, Ce Yu, Jian Xiao +19

As the cyber-infrastructure for Astronomical research from Chinese Virtual Observatory (China-VO) project, AstroCloud has been archived solid progresses during the last one year. P…