activity
20232026
most citedSolution to the conflict between the resolved and unresolved galaxy stellar mass estimation from the perspective of JWST

15 citations · 30 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.HE2026

Discovery of a Featureless Tidal Disruption Event at z~1 with the Wide Field Survey Telescope

Jiazheng Zhu, Zelin Xu, Ning Jiang +31

We report the discovery of tidal disruption event (TDE) WFST250820mmsw/AT2025wet by the 2.5-meter Wide Field Survey Telescope (WFST). It exhibits a blue nuclear flare throughout th…

astro-ph.GA2026

The FAST Hundred-Deg HI Deep (HD) Survey: Early Results from the Pilot Survey

Chen Xu, Yingjie Jing, Jie Wang +26

The Hundred-deg HI Deep (HD) survey carried out with the Five-hundred-meter Aperture Spherical Telescope (FAST) is planned to map a contiguous region within the DESI DR1 fo…

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

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.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

An updated efficient galaxy morphology classification model based on ConvNeXt encoding with UMAP dimensionality reduction

Guanwen Fang, Shiwei Zhu, Jun Xu +5

We present an enhanced unsupervised machine learning (UML) module within our previous \texttt{USmorph} classification framework featuring two components: (1) hierarchical feature e…

astro-ph.HE2025★ 3 cited

Insights from the "Red devil" AT 2022fpx: A Dust-reddened Family of Tidal Disruption Events Excluded by Their Apparent Red Color?

Zheyu Lin, Ning Jiang, Yibo Wang +5

We report unnoticed but intriguing features in the peculiar nuclear transient AT 2022fpx, and investigate its type. These features include the constantly red optical color of $g-r>…

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

Local star-forming galaxies build up central mass concentration most actively near

Zhizheng Pan, Xianzhong Zheng, Xu Kong

To understand in what mass regime star-forming galaxies (SFGs) build up central mass concentration most actively, we present a study on the luminosity-weighted stellar age radial g…

astro-ph.GA2023

Dwarf galaxies with the highest concentration are not thicker than ordinary dwarf galaxies

Lijun Chen, Hong-Xin Zhang, Zesen Lin +5

The formation mechanism of high-concentration dwarf galaxies is still a mystery. We perform a comparative study of the intrinsic shape of nearby low-mass galaxies with different st…

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…