Issue |
A&A
Volume 698, May 2025
|
|
---|---|---|
Article Number | A322 | |
Number of page(s) | 16 | |
Section | Stellar atmospheres | |
DOI | https://doi.org/10.1051/0004-6361/202452365 | |
Published online | 26 June 2025 |
Directly deriving atmospheric parameters for one million stars from SMSS photometric images
1
School of Mathematics and Statistics, Shandong University,
Weihai
264209,
Shandong,
PR China
2
School of Mechanical, Electrical and Information Engineering, Shandong University,
Weihai
264209,
Shandong,
PR China
★ Corresponding author: buyude@sdu.edu.cn
Received:
25
September
2024
Accepted:
28
April
2025
The precise determination of stellar atmospheric parameters (effective temperature Teff, surface gravity log g, and metallicity [Fe/H]) serves as a cornerstone of Galactic studies. In this work, we develop a novel deep learning approach, the Atmospheric CSWin Framework (ACF), to measure these parameters with high precision. The ACF employs a dual-input architecture that combines astrometric data (parallaxes and their corresponding errors) from Gaia Early Data Release 3 with photometric images from the fourth data release (DR4) of the SkyMapper Southern Survey (SMSS). The framework utilizes a CSWin Transformer backbone for hierarchical feature extraction from photometric images, integrated with Monte Carlo dropout in the prediction module for robust uncertainty quantification. Trained on cross-matched stars between SMSS DR4 and the third data release of the Galactic Archaeology with HERMES spectroscopic survey, the ACF achieves parameter estimates with dispersions of 95.02 K for Teff, 0.07 dex for log g, and 0.14 dex for [Fe/H]. Systematic experiments demonstrate that incorporating parallax information significantly improves the precision of all three parameters, especially log g. Our image-based methods outperform traditional approaches based on stellar magnitudes or colors, with improvements ranging from 2% to 14%. The ACF yields parameter estimates approaching those of high-resolution spectroscopic analyses, and the framework remains effective even for low-quality samples, highlighting its robustness and general applicability. Using the ACF, we compiled a comprehensive catalog of atmospheric parameters for one million SMSS DR4 stars.
Key words: methods: data analysis / methods: statistical / techniques: photometric / stars: abundances / stars: fundamental parameters
© The Authors 2025
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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