activity
20242026
most citedUnveiling Galactic substructures with M Giant stars: A kinematic and chemical study based on LAMOST DR9, Gaia DR3 and APOGEE DR17

2 citations · 3 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.IM2026

Stellar Density Classification and Regression for CSST Multi-color Imaging Using Deep Learning

Jinzhi Lai, Man I Lam, Jianjun Chen +6

The Chinese Space Station Survey Telescope (CSST) aims to map the universe across an unprecedented dynamic range of stellar densities, spanning from extragalactic voids to the crow…

astro-ph.GA2026

Exploring the formation mechanisms of tidal structures in globular clusters of extragalactic origin

Shouzhi Wang, Jundan Nie, Biwei Jiang +3

Tidal structures around globular clusters provide valuable insights into cluster evolution and the hierarchical assembly of the Milky Way. Using wide-field imaging data from the DE…

astro-ph.IM2025

Mock Observations for the CSST Mission: Main Surveys-the Slitless Spectroscopy Simulation

Xin Zhang, Yue-dong Fang, Cheng-liang Wei +14

The China Space Station Telescope (CSST), slated to become China's largest space-based optical telescope in the coming decade, is designed to conduct wide-field sky surveys with hi…

astro-ph.IM2025

Mock Observations for the CSST Mission: Main Surveys -- the Mock Catalogue

Cheng-Liang Wei, Yu Luo, Hao Tian +17

The Chinese Space Station Survey Telescope (CSST) is a flagship space mission, designed to carry out a large-area sky survey to explore the nature of dark matter and dark energy in…

astro-ph.IM2025

Mock Observations for the CSST Mission: Main Surveys--An Overview of Framework and Simulation Suite

Cheng-Liang Wei, Guo-Liang Li, Yue-Dong Fang +26

The Chinese Space Station Survey Telescope (CSST) is a flagship space-based observatory. Its main survey camera is designed to conduct high spatial resolution near-ultraviolet to n…

astro-ph.IM2025

Mock Observations for the CSST Mission: Main Surveys--the Stray Light

Xian Jing-Tian, Lin Lin, Fang Yue-Dong +9

Stray light significantly influences the detection capabilities of astronomical telescopes. The actual stray-light level during observations depends not only on the telescope's inh…

astro-ph.IM2025★ 1 cited

CSST Slitless Spectra: Target Detection and Classification with YOLO

Yingying Zhou, Chao Liu, Hao Tian +2

Addressing the spatial uncertainty and spectral blending challenges in CSST slitless spectroscopy, we present a deep learning-driven, end-to-end framework based on the You Only Loo…

astro-ph.IM2025

Slitless Spectroscopy Source Detection Using YOLO Deep Neural Network

Xiaohan Chen, Man I Lam, Yingying Zhou +6

Slitless spectroscopy eliminates the need for slits, allowing light to pass directly through a prism or grism to generate a spectral dispersion image that encompasses all celestial…

astro-ph.GA2025★ 2 cited

Unveiling Galactic substructures with M Giant stars: A kinematic and chemical study based on LAMOST DR9, Gaia DR3 and APOGEE DR17

Longfei Ding, Jing Li, Xiang-Xiang Xue +3

Based on the updated M giant star catalog selected from LAMOST DR9, we iden-tify substructures within the integrals-of-motion space through Friends-of-Friends cluster-ing algorithm…

astro-ph.IM2025

Toward High-Precision Astrometry with CSST Using Multi-Gaussian Fitting of PSF

Jialu Nie, Peng Wei, Zihuang Cao +5

The Chinese Space Station Survey Telescope (CSST) presents significant potential for high-precision astrometry. In this study, we show that the point spread function (PSF) modeled…

astro-ph.GA2024

Assessing the Association between the Globular Cluster NGC 4147 and the Sagittarius Dwarf Galaxy

YingHua Zhang, Jundan Nie, Hao Tian +1

The potential association of the globular cluster (GC) NGC 4147 with the Sagittarius (Sgr) dwarf spheroidal galaxy has been proposed due to their comparable locations and radial ve…

astro-ph.GA2024

The Star Formation History of Nearby Galaxies: A Machine Learning Approach

Yujiao Yang, Chao Liu, Ming Yang +2

Reproducing color-magnitude diagrams (CMDs) of star-resolved galaxies is one of the most precise methods for measuring the star formation history (SFH) of nearby galaxies back to t…