activity
20242026
most citedHalf a Million Binary Stars from the low resolution spectra of LAMOST

5 citations · 5 across the 17 of their papers we have counts for

collaborators

18 papers

astro-ph.GA2026

Decoding RR Lyrae light curves with deep learning for accurate absolute magnitude estimation

Shunxuan He, Huiwen Wu, Yang Huang +6

RR Lyrae stars are essential standard candles for distance measurements in the Milky Way and nearby galaxies. Traditional estimates rely on the Period--Absolute Magnitude--Metallic…

astro-ph.GA2026

Differential Reddening and Extinction Law Analyses of Galactic Open Clusters

Xiaohan Chen, Shu Wang, Xiaodian Chen

Extinction significantly affects open cluster parameters and their use in studies of Galactic structure, yet homogeneous large sample measurements of open cluster extinction proper…

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.SR2026

Surface brightness-color relations for red giant branch stars: Observational constraints on metallicity effects using the ARD method

Jianping Xiong, Xiaodian Chen, Jiao Li +5

Aims: We aim to quantify the metallicity dependence of the SBCR for red giant branch (RGB) stars and to test the robustness of the relation using asteroseismic radii, Gaia distance…

astro-ph.SR2026

A Search for Variability of Ultracool Dwarfs with the Zwicky Transient Facility

Haomiao Huang, Shu Wang, Xiaodian Chen +2

Rotationally modulated photometric variability of ultracool dwarfs encodes key information about cloud structure and temperature contrasts. Large homogeneous optical datasets are c…

astro-ph.SR2026

The Phenomenological Classification of TESS Eclipsing Binaries

Shi-Qi Liu, Kai Li, Xiao-Dian Chen +1

Eclipsing binaries are crucial astrophysical laboratories for studying stellar parameters and evolutionary processes. In this study, we constructed a machine-learning-based model f…

astro-ph.SR2026

StarCLR: Contrastive Learning Representation for Astronomical Light Curves

Junyao Ding, Xiaodian Chen, Xinyi Gao +7

With the rapid development of time-domain surveys, the availability of massive light curve data offers new opportunities for studying stellar evolution and variable star classifica…

astro-ph.SR2026

SPHEREx Ultracool Dwarf spectrophotometric Atlas (SUDA): Atmospheric and Fundamental Parameters of Ultracool Dwarfs

Zhijun Tu, Shu Wang, Haomiao Huang +2

We present the SPHEREx Ultracool Dwarf spectrophotometric Atlas (SUDA), a homogeneous sample of 1675 field ultracool dwarfs with continuous 0.75--5~m spectrophotometry from SPHE…

astro-ph.GA2025

The Dependence of the Extinction Coefficient on Reddening for Galactic Cepheids

Huajian Wang, Xiaodian Chen, Shu Wang

Cepheids are fundamental distance indicators, playing a crucial role not only in the cosmic distance ladder but also in mapping the structure, kinematics, and extinction properties…

astro-ph.SR2025

A Large Sample of JWST/NIRSpec Brown Dwarfs: New Distant Discoveries

Zhijun Tu, Shu Wang, Xiaodian Chen +1

Brown dwarfs are essential probes of stellar and planetary formation, yet their low luminosities pose challenges for detection at large Galactic distances. The James Webb Space Tel…

astro-ph.GA2025

Distances of Supernova Remnants Associated with Neutron Stars in the Galaxy

Xiaohan Chen, Shu Wang, Xiaodian Chen

Accurate distance measurements to supernova remnants (SNRs) are essential for determining their physical parameters, such as size, age, explosion energy, and for constraining the p…

astro-ph.SR2025

Three Brown Dwarfs Masquerading as High-Redshift Galaxies in JWST Observations

Zhijun Tu, Shu Wang, Xiaodian Chen +1

We report the spectroscopic identification of three brown dwarf candidates -- o005_s41280, o006_s00089, and o006_s35616 -- discovered in the RUBIES using James Webb Space Telescope…

astro-ph.SR2025

Optical Flares Detected on a Contact Binary: The First Photometric and Spectroscopic Analysis of a Long-period Low Mass Ratio Contact Binary HAT 307-0007476

Ling-Zhi Li, Kai Li, Xiang Gao +10

This paper presents the photometric and spectroscopic analysis of a long-period totally eclipsing contact binary (HAT 307-0007476) for the first time. This system is a low mass rat…

astro-ph.SR2025

Periodic Variability of the Central Stars of Planetary Nebulae Surveyed through the Zwicky Transient Facility

Pinjian Chen, Xuan Fang, Xiaodian Chen +1

A consensus has been reached in recent years that binarity plays an important role in the formation and evolution of a significant fraction of planetary nebulae (PNe). Utilizing th…

astro-ph.SR2024

Discoveries and Properties of EL CVn-type Binaries in the TESS Survey

Jianping Xiong, Zhenwei Li, Jiao Li +5

EL CVn-type systems represent a rare evolutionary stage in binary star evolution, providing ideal laboratories for investigating stable mass transfer processes and the formation of…

astro-ph.SR2024

Classification of Periodic Variable Stars from TESS

Xinyi Gao, Xiaodian Chen, Shu Wang +1

The number of known periodic variable stars has increased rapidly in recent years. As an all-sky transit survey, the Transiting Exoplanet Survey Satellite (TESS) plays an important…

astro-ph.SR2024★ 5 cited

Half a Million Binary Stars from the low resolution spectra of LAMOST

Yingjie Jing, Tian-Xiang Mao, Jie Wang +2

Binary stars are prevalent yet challenging to detect. We present a novel approach using convolutional neural networks (CNNs) to identify binary stars from low-resolution spectra ob…

astro-ph.GA2024

Milky Way Classical Cepheids Distances from Calibrated Infrared Period-Luminosity-Metallicity Relations

Huajian Wang, Xiaodian Chen

Classical Cepheids (DCEPs) serve as fundamental standard candles for measuring cosmic distances and investigating the structure and evolution of the Milky Way disc. However, accura…