activity
20162026
most citedThe Zwicky Transient Facility Catalog of Periodic Variable Stars

303 citations · 1.2k across the 30 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

18 papers · 1 filter

astro-ph.GA2026

Correlation between the two-armed spiral in the -- plane and moving groups

Yan Xu, Chao Liu, Chengdong Li +5

We use a cross-matched sample of 3.7 million stars from Gaia DR3 and LAMOST DR7 to investigate the velocity substructures in the Milky Way disk. The median radial velocity as…

astro-ph.GA2024★ 3 cited

Detailed Mapping of the Galactic Disk Structure in the Solar Neighborhood through LAMOST K Dwarfs

Xi-Can Tang, Hao Tian, Jing Li +4

The Galactic disk is one of the main components of the Milky Way, which contributes most of the luminosity. Its structure is essential for understanding the formation and evolution…

astro-ph.GA2023

On the identification of N-rich metal-poor field stars with future China space station telescope

Jiajun Zhang, Baitian Tang, Jiang Chang +6

During the long term evolution of globular clusters (GCs), a part of member stars are lost to the field. The recently found nitrogen-rich (N-rich) metal-poor field stars are promis…

astro-ph.GA2023

Exploring asymmetric substructures of the outer disk based on the conjugate angle of the radial action

Y. Xu, C. Liu, Z. Li +5

We use the conjugate angle of radial action (), the best representation of the orbital phase, to explore the "mid-plane, north branch, south branch" and "Monoceros area" disk…

astro-ph.GA2023★ 11 cited

The first comprehensive Milky Way stellar mock catalogue for the Chinese Space Station Telescope Survey Camera

Yang Chen, Xiaoting Fu, Chao Liu +9

The Chinese Space Station Telescope (CSST) is a cutting-edge two-meter astronomical space telescope currently under construction. Its primary Survey Camera (SC) is designed to cond…

astro-ph.GA2023★ 75 cited

Stellar Initial Mass Function Varies with Metallicities and Time

Jiadong Li, Chao Liu, Zhi-Yu Zhang +4

Most structural and evolutionary properties of galaxies strongly rely on the stellar initial mass function (IMF), namely the distribution of the stellar mass formed in each episode…

astro-ph.GA2022★ 11 cited

Is the core-cusp problem a matter of perspective: Jeans Anisotropic Modeling against numerical simulations

Wenting Wang, Ling Zhu, Zhaozhou Li +14

Mock member stars for 28 dwarf galaxies are constructed from the cosmological Auriga simulation, which reflect the dynamical status of realistic stellar tracers. The axis-symmetric…

astro-ph.GA2022★ 8 cited

Searching Extra-tidal Features around the Globular Cluster Whiting 1

Jundan Nie, Hao Tian, Jing Li +14

Whiting 1 is a faint and young globular cluster in the halo of the Milky Way, and was suggested to have originated in the Sagittarius spherical dwarf galaxy (Sgr dSph). In this pap…

astro-ph.GA2021★ 3 cited

Search for the metal-weak thick disk from the LAMOST DR5

T. -S. Yan, J. -R. Shi, H. Tian +2

Based on the data release of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope survey (LAMOST DR5) and the \emph{Gaia} Early Data Release 3 (\emph{Gaia} EDR3), we const…

astro-ph.GA2021★ 25 cited

The Flare and Warp of the Young Stellar Disk traced with LAMOST DR5 OB-type stars

Yang Yu, Hai-Feng Wang, Wen-Yuan Cui +9

We present analysis of the spatial density structure for the outer disk from 814 \,kpc with the LAMOST DR5 13534 OB-type stars and observe similar flaring on north and south sid…

astro-ph.GA2021★ 15 cited

Exploring the Galactic Anticenter substructure with LAMOST & Gaia DR2

Jing Li, Xiang-Xiang Xue, Chao Liu +12

We characterize the kinematic and chemical properties of 589 Galactic Anticenter Substructure Stars (GASS) with K-/M- giants in Integrals-of-Motion space. These stars likely includ…

astro-ph.GA2020★ 11 cited

Differential rotation of the halo traced by the K-giant stars

Hao Tian, Chao Liu, Yougang Wang +4

We use K-giant stars selected from the LAMOST DR5 to study the variation of the rotational velocity of the galactic halo at different space positions. Modelling the rotational velo…

astro-ph.GA2019★ 40 cited

Tracing Kinematic and Chemical Properties of Sagittarius Stream by K-Giants, M-Giants, and BHB stars

Chengqun Yang, Xiang-Xiang Xue, Jing Li +12

We characterize the kinematic and chemical properties of 3,000 Sagittarius (Sgr) stream stars, including K-giants, M-giants, and BHBs, select from SEGUE-2, LAMOST, and SDSS s…

astro-ph.GA2019★ 28 cited

Identifying Galactic Halo Substructure in 6D Phase-space Using 13,000 LAMOST K Giants

Chengqun Yang, Xiang-Xiang Xue, Jing Li +6

We construct a large halo K-giant sample by combining the positions, distances, radial velocities, and metallicities of over 13,000 LAMOST DR5 halo K giants with the Gaia DR2 prope…

astro-ph.GA2019★ 33 cited

Detecting the Sagittarius stream with LAMOST DR4 M giants \& Gaia DR2

Jing Li, Chao Liu, Xiangxiang Xue +4

We use LAMOST DR4 M giants combined with Gaia DR2 proper motions and ALLWISE photometry to obtain an extremely pure sample of Sagittarius (Sgr) stream stars. Using TiO5 and CaH spe…

astro-ph.GA2019★ 134 cited

An intuitive 3D map of the Galactic warp's precession traced by classical Cepheids

Xiaodian Chen, Shu Wang, Licai Deng +3

The Milky Way's neutral hydrogen (HI) disk is warped and flared. However, a dearth of accurate HI-based distances has thus far prevented the development of an accurate Galactic dis…

astro-ph.GA2018★ 34 cited

Rotating halo traced by the K giant stars from LAMOST and Gaia

Hao Tian, Chao Liu, Yan Xu +1

With the help of Gaia DR2, we are able to obtain the full 6-D phase space information for stars from LAMOST DR5. With high precision of position, velocity, and metallicity, the rot…

astro-ph.GA2016★ 38 cited

Selecting M-giants with infra-red photometry: Distances, metallicities and the Sagittarius stream

Jing Li, Martin C. Smith, Jing Zhong +9

Using a spectroscopically confirmed sample of M-giants, M-dwarfs and quasars from the LAMOST survey, we assess how well WISE 2MASS color-cuts can be used to select M-giant sta…