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20232026
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Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2026

Difference Between Half-mass Radius and Half-light Radius of Galaxies at 0.2 2.5 Revealed by JWST/NIRCam Data

Mingen Xin, Guanwen Fang, Jie Song +3

Using JWST observations in CANDELS fields, we measure the half-light radius () and half-mass radius () for 14,333 galaxies with stellar masses $M_*…

astro-ph.GA2025

Dual-coding contrastive learning based on ConvNeXt and ViT models for morphological classification of galaxies in COSMOS-Web

Shiwei Zhu, Guanwen Fang, Chichun Zhou +4

In our previous works, we proposed a machine learning framework named \texttt{USmorph} for efficiently classifying galaxy morphology. In this study, we propose a self-supervised me…

astro-ph.GA2025

The H concentration of local star-forming galaxies: implications for galaxy structure formation

Zhizheng Pan, Xianzhong Zheng, Xu Kong

In this work, we present a study on the H emission line flux concentration of 3098 low-redshift star-forming galaxies (SFGs) using the MaNGA data available in the Data Release 1…

astro-ph.GA2025

A Glimpse of Satellite Galaxies in the Milky Way with the 2.5-meter Wide Field Survey Telescope (WFST): Bootes III and Draco

Chao Yang, Zhizheng Pan, Min Fang +34

We carry out deep imaging of the Milky Way satellite galaxies, Bootes III and Draco, with WFST as one pilot observing program to demonstrate the capability of WFST. Combining catal…

astro-ph.GA2025

Dominant Role of Coplanar Inflows in Driving Disk Evolution Revealed by Gas-Phase Metallicity Gradients

Cheqiu Lyu, Enci Wang, Hongxin Zhang +8

Using spatially resolved spectroscopic data from the MaNGA sample, we investigate the parameters influencing the radial gradients of gas-phase metallicity ($\nabla\log(\mathrm{O/H}…

astro-ph.GA2023

The Ly non-detection by JWST NIRSpec of a strong Ly emitter at confirmed by MUSE

Haochen Jiang, Xin Wang, Cheng Cheng +6

The detections of Lyman- () emission in galaxies with redshifts above 5 are of utmost importance for constraining the cosmic reionization timeline, yet such detections…