collaborators

6 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.IM2026

PhysFormer: A Physics-Embedded Generative Model for Physically Self-Consistent Spectral Synthesis

Siqi Wang, Mengmeng Zhang, Yude Bu +1

In scientific and engineering domains, modeling high-dimensional complex systems governed by partial differential equations (PDEs) remains challenging in terms of physical consiste…

astro-ph.SR2026

Deep learning-driven atmospheric parameter prediction for hot subdwarf stars with synthetic and observed spectra

Zhenxin Lei, Yangyang Dong, Bokai Kou +4

We design a convolutional neural network (CNN) incorporating channel attention and spatial attention mechanisms to predict atmospheric parameters of hot subdwarfs. The experimental…

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

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…