activity
20242026
most citedSize Growth on Short Timescales of Star-Forming Galaxies: Insights from Size Variation with Rest-Frame Wavelength with JADES

1 citations · 1 across the 6 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2026

Updated Metallicity Diagnostics for Precision Oxygen Abundance Measurements in High-redshift Galaxies with JWST

Shihong Liu, Yu Rong, Tie Li +7

Recent work has demonstrated that widely used strong-line oxygen abundance indicators, such as O3N2, , and , suffer from large uncertainties when applied…

astro-ph.GA2025

Warped Disk Galaxies: Statistical Properties from DESI Legacy Imaging Surveys DR8

Yiheng Wang, Han Qu, Jiafeng Lu +3

Warped structures are often observed in disk galaxies, yet their physical origin is still under investigation. We present a systematic study of warped edge-on disk galaxies based o…

astro-ph.GA2025

The Cosmic Evolution and Spatial Distribution of Multiphase Gas associated with QSOs

Zeyu Chen, Enci Wang, Hu Zou +10

We investigate the multi-phase gas surrounding QSOs traced by 33 absorption lines (e.g., Ly, C\,\textsc{iv}, Fe\,\textsc{ii}, Mg\,\textsc{ii}, etc.) in the stacked spectra of ba…

astro-ph.GA2025

The Internal Kinematics, Stellar Population, and Gas-phase Properties of The Pseudobulge in An Ultra-diffuse Galaxy: AGC721966

Shihong Liu, Yu Rong, Huiyuan Wang +8

Leveraging spectroscopic data from the Sloan Digital Sky Survey, we conduct a comprehensive analysis of the central stellar velocity dispersion, stellar population properties, star…

astro-ph.CO2025

The Three Hundred: Gas Properties Outside of Galaxy Cluster with the WHIM Contribution and Detection

Renjie Li, Weiguang Cui, Ang Liu +4

We investigate the physical properties and detectability of warm-hot intergalactic medium (WHIM) gas with temperatures in the range K around galaxy clusters using simu…

astro-ph.GA2025

Central Velocity Dispersion being the Primary Driver of Abundance Patterns in Quenched Galaxies

Haixin Li, Enci Wang, Cheqiu Lyu +6

The element abundances of galaxies provide crucial insights into their formation and evolution. Using high-resolution IFU data from the MaNGA survey, we analyze the central spectra…