activity
20222026
most citedAutomatic Classification of Galaxy Morphology: a rotationally invariant supervised machine learning method based on the UML-dataset

34 citations · 73 across the 21 of their papers we have counts for

collaborators

21 papers

astro-ph.HE2026

Searching for Type Ia Supernovae in the Dark Energy Spectroscopic Instrument

Xiaoyu Zhuang, Song Ran, Dezheng Meng +9

With the development of large-scale photometric surveys, an increasing number of supernova candidates are being discovered, leading to a rapidly growing demand for supernova spectr…

astro-ph.GA2026

SDSS+JWST Census of Stellar and Nebular Dust Attenuation at -7: Mass Dependence and Redshift Evolution

Jie Song, Masami Ouchi, Tomokazu Kiyota +3

We present the demography of dust attenuation, including its mass dependence and redshift evolution, using spectroscopic samples of 34,182 SDSS galaxies at and 863 JWST/…

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.GA2026

Robustness Analysis of USmorph: II. Optimizing Feature Extraction, Dimensionality Reduction, and Clustering for Unsupervised Galaxy Morphology Classification

Guanwen Fang, Xiaolei Yin, Yirui Zheng +5

We conduct a systematic robustness analysis of the unsupervised machine learning module within the hybrid framework \texttt{USmorph}. This module automatically discovers morphologi…

astro-ph.GA2026★ 1 cited

Discovery of low-redshift analogues to "Little Red Dots" in DESI: A later evolutionary stage of compact LRDs?

Weiyu Ding, Xu Kong, Wei-Jian Guo +8

The James Webb Space Telescope (JWST) has recently discovered a population of compact, red sources at z > 4 known as "Little Red Dots" (LRDs). They are characterized by their V-sha…

astro-ph.GA2025

Robustness Analysis of USmorph: I. Generalization Efficiency of Unsupervised Strategies and Supervised Learning in Galaxy Morphological Classification

Shiwei Zhu, Guanwen Fang, Yao Dai +5

We conduct a systematic robustness analysis of the hybrid machine learning framework \texttt{USmorph}, which integrates unsupervised and supervised learning for galaxy morphologica…

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

First Statistical Detection of MgII-traced Cool Gas Outflows with JWST Towards Cosmic Dawn

Cheqiu Lyu, Haoran Yu, Enci Wang +9

Galactic-scale outflows are a crucial component of galaxy evolution, yet their properties in the early universe remain poorly constrained. We present the first statistical investig…

astro-ph.GA2025

Transition from Outside-in to Inside-Out at : Evidence from Radial Profiles of Specific Star Formation Rate based on JWST/HST

Jie Song, Enci Wang, Cheng Jia +7

By combining high-resolution observations from JWST and HST, we have measured the stellar masses, star formation rates (SFRs), and multi-wavelength morphologies of galaxies in the…

astro-ph.GA2025

Central Concentration and Escape of Ionizing Photons in Galaxies at the Epoch of Reionization

Cheqiu Lyu, Enci Wang, Junxian Wang +9

Compact, low-mass galaxies with strong nebular emission are considered promising candidates for efficient ionizing photon production and escape. We present a spatially resolved ana…

astro-ph.GA2025

Potential-Driven Metal Cycling: JADES Census of Gas-Phase Metallicity for galaxies at 1 < z < 7

Cheng Jia, Enci Wang, Cheqiu Lyu +9

The gravitational potential is established as a critical determinant of gas-phase metallicity (12+log(O/H)) in low-redshift galaxies, whereas its influence remains unconfirmed at h…

astro-ph.GA2024★ 4 cited

An efficient unsupervised classification model for galaxy morphology: Voting clustering based on coding from ConvNeXt large model

Guanwen Fang, Yao Dai, Zesen Lin +6

In this work, we update the unsupervised machine learning (UML) step by proposing an algorithm based on ConvNeXt large model coding to improve the efficiency of unlabeled galaxy mo…

astro-ph.GA2024★ 1 cited

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

Cheng Jia, Enci Wang, Huiyuan Wang +11

We investigate size variation with rest-frame wavelength for star-forming galaxies based on the second JWST Advanced Deep Extragalactic Survey data release. Star-forming galaxies a…

astro-ph.GA2024★ 7 cited

Preparation for CSST: Star-galaxy Classification using a Rotationally Invariant Supervised Machine Learning Method

Shiliang Zhang, Guanwen Fang, Jie Song +6

Most existing star-galaxy classifiers depend on the reduced information from catalogs, necessitating careful data processing and feature extraction. In this study, we employ a supe…

astro-ph.GA2024

USmorph: An Updated Framework of Automatic Classification of Galaxy Morphologies and Its Application to Galaxies in the COSMOS Field

Jie Song, GuanWen Fang, Shuo Ba +9

Morphological classification conveys abundant information on the formation, evolution, and environment of galaxies. In this work, we refine the two-step galaxy morphological classi…

astro-ph.GA2023★ 15 cited

Solution to the conflict between the resolved and unresolved galaxy stellar mass estimation from the perspective of JWST

Jie Song, GuanWen Fang, Zesen Lin +2

By utilizing the spatially-resolved photometry of galaxies at in the CEERS field, we estimate the resolved and unresolved stellar mass via spectral energy distribution…

astro-ph.GA2023★ 7 cited

Strong [O III] λ5007 Compact Galaxies Identified from SDSS DR16 and Their Scaling Relations

Weiyu Ding, Hu Zou, Xu Kong +11

Green pea galaxies are a special class of star-forming compact galaxies with strong [O III]λ5007 and considered as analogs of high-redshift Lyα-emitting galaxies and potential sour…

astro-ph.GA2023★ 1 cited

Evolution of Non-parametric Morphology of Galaxies in the JWST CEERS Field at 0.8-3.0

Yao Yao, Jie Song, Xu Kong +3

Galaxy morphology is one of the most fundamental ways to describe galaxy properties, but the morphology we observe may be affected by wavelength and spatial resolution, which may i…

astro-ph.GA2023

The Classification of Galaxy Morphology in H-band of COSMOS-DASH Field: a combination-based machine learning clustering model

Yao Dai, Jun Xu, Jie Song +6

By applying our previously developed two-step scheme for galaxy morphology classification, we present a catalog of galaxy morphology for H-band selected massive galaxies in the COS…

astro-ph.GA2023★ 3 cited

The effect of environment on the properties of the most massive galaxies at in the cosmos-dash field

Jie Song, Guanwen Fang, Yizhou Gu +2

How the environment influences the most massive galaxies is still unclear. To explore the environmental effects on morphology and star formation in the most massive galaxies at hig…

astro-ph.GA2022★ 34 cited

Automatic Classification of Galaxy Morphology: a rotationally invariant supervised machine learning method based on the UML-dataset

G. W. Fang, S. Ba, Y. Z. Gu +8

Classification of galaxy morphology is a challenging but meaningful task for the enormous amount of data produced by the next-generation telescope. By introducing the adaptive pola…