activity
20222026
most citedAutomatic detection of low surface brightness galaxies from SDSS images

24 citations · 61 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.SR2026

MSFA-Net: An Advanced Deep Learning Model for Identifying Blue Horizontal-Branch Stars from LAMOST DR12

Mingyuan Wang, Xiaoming Kong, Jie Ju +2

Blue horizontal-branch (BHB) stars are low-mass, core helium-burning objects with nearly constant luminosities, making them powerful tracers of old, metal-poor populations and valu…

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

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.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.IM2023★ 8 cited

L dwarfs detection from SDSS images using improved Faster R-CNN

Zhi Cao, Zhenping Yi, Jingchang Pan +4

We present a data-driven approach to automatically detect L dwarfs from Sloan Digital Sky Survey(SDSS) images using an improved Faster R-CNN framework based on deep learning. The e…

astro-ph.SR2023

Estimating Stellar Parameters and Identifying Very Metal-poor Stars Using Convolutional Neural Networks for Low-resolution Spectra (R~200)

Tianmin Wu, Yude Bu, Jianhang Xie +5

Very metal-poor (VMP, [Fe/H]<-2.0) stars offer a wealth of information on the nature and evolution of elemental production in the early galaxy and universe. The upcoming China Spac…

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…

astro-ph.SR2022

Identifying hot subdwarf stars from photometric data using Gaussian mixture model and graph neural network

Wei Liu, Yude Bu, Xiaoming Kong +2

Hot subdwarf stars are very important for understanding stellar evolution, stellar astrophysics, and binary star systems. Identifying more such stars can help us better understand…

astro-ph.SR2022★ 4 cited

Searching for Barium Stars from the LAMOST Spectra Using the Machine Learning Method: I

Fengyue Guo, Zhongding Cheng, Xiaoming Kong +5

Barium stars are chemically peculiar stars that exhibit enhancement of s-process elements. Chemical abundance analysis of barium stars can provide crucial clues for the study of th…

astro-ph.GA2022★ 9 cited

Li-rich Giants Identified from LAMOST DR8 Low-Resolution Survey

BeiChen Cai, XiaoMing Kong, JianRong Shi +3

A small fraction of giants possess photospheric lithium(Li) abundance higher than the value predicted by the standard stellar evolution models, and the detailed mechanisms of Li en…

astro-ph.IM2022★ 24 cited

Automatic detection of low surface brightness galaxies from SDSS images

Zhenping Yi, Jia Li, Wei Du +7

Low surface brightness (LSB) galaxies are galaxies with central surface brightness fainter than the night sky. Due to the faint nature of LSB galaxies and the comparable sky backgr…