collaborators

6 papers

astro-ph.IM2026

A Robust Geometric Distortion Solution for Main Survey Camera of CSST

Yibo Yan, You Wu, Jundan Nie +30

The advancement in sensitivity and field of view of next-generation wide-field survey telescopes requires astrometric measurements with high precision, even in the presence of sign…

astro-ph.IM2026

Detection and classification of astronomical sources with Astro-RetinaNet in crowded stellar fields

Yibo Yan, Chao Liu, Jiadong Li +1

Upcoming next-generation sky surveys will detect large number of faint objects with magnitudes larger than 25. When objects are crowded within a limited a field of view, blending b…

astro-ph.SR2025

Stellar Parameters of BOSS M dwarfs in SDSS-V DR19

Dan Qiu, Jennifer A. Johnson, Chao Liu +15

We utilized the Stellar LAbel Machine (SLAM), a data-driven model based on Support Vector Regression, to derive stellar parameters ([Fe/H], , and ) for SDSS-V…

astro-ph.GA2025

The structural and kinematical properties of NGC 5634, a globular cluster associated with the Sagittarius dwarf galaxy?

Shouzhi Wang, Jundan Nie, Biwei Jiang +3

We investigate the origin of NGC 5634 through a comprehensive analysis of its morphology, kinematics and dynamics. Utilizing data from the DESI Legacy Survey, we refined its fundam…

astro-ph.GA2025

Distance estimation of the high-velocity cloud Anti-Center Shell

Yu-Ting Wang, Chao Liu, Zhi-Yu Zhang

High-velocity clouds (HVCs) are interstellar gas clouds whose velocities are incompatible with Galactic rotation. Since the first discovery of HVCs in 1963, their origins have been…

astro-ph.GA2025

LAMOST medium-resolution spectroscopic survey of Galactic Open Clusters (LAMOST-MRS-O): An overview of survey plan and preliminary results

Xi Zhang, Chengzhi Liu, Jing Zhong +7

As part of the LAMOST medium-resolution spectroscopic survey, the LAMOST-MRS-O is a non-time domain survey that aims to perform medium-resolution spectral observations for member s…