activity
20222026
most citedEdge-on Low-surface-brightness Galaxy Candidates Detected from SDSS Images Using YOLO

12 citations · 19 across the 10 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2026

Morphology classification for galaxies in the Kilo Degree Survey using a label-efficient self-supervised learning framework

Xu Huang, Rui Li, Liang Gao +14

Galaxy morphology classification is fundamental to understanding galaxy formation and evolution. The advent of large-scale sky surveys has produced an unprecedented volume of galax…

astro-ph.SR2026

A Generalist Model Including Evolved Star Mass and Age

Mengmeng Zhang, Yude Bu, Siqi Wang +10

Determining precise stellar ages and masses for evolved giants is crucial for Galactic archaeology but challenged by spectral degeneracies. Gaia's low-resolution XP spectra offer a…

astro-ph.GA2025★ 1 cited

Using Deep Learning Methods to Detect for Ultra-diffuse Galaxies in KiDS

Hao Su, Rui Li, Nicola R. Napolitano +13

Ultra-diffuse Galaxies (UDGs) are a subset of Low Surface Brightness Galaxies (LSBGs), showing mean effective surface brightness fainter than and a d…

astro-ph.GA2025

Identifying Ring Galaxies in DESI Legacy Imaging Surveys Using Machine Learning Methods

Aina Zhang, Xiaoming Kong, Bowen Liu +4

The formation and evolution of ring structures in galaxies are crucial for understanding the nature and distribution of dark matter, galactic interactions, and the internal secular…

astro-ph.GA2025★ 4 cited

Deblending Overlapping Galaxies in DECaLS Using Transformer-Based Algorithm: A Method Combining Multiple Bands and Data Types

Ran Zhang, Meng Liu, Zhenping Yi +8

In large-scale galaxy surveys, particularly deep ground-based photometric studies, galaxy blending is inevitable and poses a potential primary systematic uncertainty for upcoming s…

astro-ph.SR2024

An adaptive parameter estimator for poor-quality spectral data of white dwarfs

Duo Xie, Jiangchuan Zhang, Yude Bu +3

White dwarfs represent the end stage for 97% of stars, making precise parameter measurement crucial for understanding stellar evolution. Traditional estimation methods involve fitt…

astro-ph.IM2024

A Versatile Framework for Analyzing Galaxy Image Data by Implanting Human-in-the-loop on a Large Vision Model

Mingxiang Fu, Yu Song, Jiameng Lv +14

The exponential growth of astronomical datasets provides an unprecedented opportunity for humans to gain insight into the Universe. However, effectively analyzing this vast amount…

astro-ph.GA2024★ 2 cited

Low surface brightness galaxies from BASS+MzLS with Machine Learning

Peng-Liang Du, Wei Du, Bing-Qing Zhang +3

From 5000 deg of the combination of the Beijing-Arizona Sky Survey (BASS) and Mayall -band Legacy Survey (MzLS) which is also the northern sky region of the Dark En…

astro-ph.SR2024

SPT: Spectral Transformer for Red Giant Stars Age and Mass Estimation

Mengmeng Zhang, Fan Wu, Yude Bu +4

The age and mass of red giants are essential for understanding the structure and evolution of the Milky Way. Traditional isochrone methods for these estimations are inherently limi…

astro-ph.GA2023★ 12 cited

Edge-on Low-surface-brightness Galaxy Candidates Detected from SDSS Images Using YOLO

Yongguang Xing, Zhenping Yi, Zengxu Liang +7

Low-surface-brightness galaxies (LSBGs), fainter members of the galaxy population, are thought to be numerous. However, due to their low surface brightness, the search for a wide-a…

astro-ph.SR2022

Se-ResNet+SVM model: an effective method of searching for hot subdwarfs from LAMOST

Cheng Zhongding, Kong xiaoming, Wu Tianmin +5

In this paper, we apply the feature-integration idea to fuse the abstract features extracted by Se-ResNet with experience features into hybrid features and input the hybrid feature…