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A Convolutional Neural Network–Transformer Denoiser for Low-signal-to-noise-ratio Galaxy Spectra: Stellar Population Recovery in Synthetic Tests

Suk Kim et al · IOP Publishing · 2026

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Stellar population measurements in integral field unit surveys are often limited by low signal-to-noise ratios (S/Ns) in low-surface-brightness spaxels. Using controlled synthetic experiments, we investigate whether a deep-learning-based denoising can recover stellar population information from such spectra without requiring spatial binning. We introduce the Enhanced U-Net Transformer (EUT), a one-dimensional convolutional neural network–transformer model trained on 90,000 synthetic spectra constructed from MILES simple stellar population (SSP) models following J. H. Lee et al., with wavelength-dependent noise injected on the fly to emulate SAMI-like data (S/N ≃ 5–20, measured in a 4484.77–4573.12 Å continuum window). Utilizing an independent test set of 10,000 spectra, the EUT reduces the full-spectrum rms residual by ≃96.5% at S/N = 5 (and by ≃94% at S/N = 20), achieving recovery rates of ≥99.8% (the Pearson correlation coefficient between the noise-free and comparison spectra expressed in percent). In fixed windows around Ca ii H, H δ , H β , Fe i 4383, Mg b, and Na D, residuals decrease by ≳88% while preserving line-profile structure. In downstream analysis with p PXF we assess parameter recovery using the Pearson correlation coefficient R _p and the rms scatter: the scatter in recovered mass-weighted age decreases from ≃0.41 to ≃0.25 dex at S/N = 5 and from ≃0.32 to ≃0.22 dex at S/N = 10; the corresponding mass-weighted global metallicity, [M/H], scatter decreases from ≃0.45 to ≃0.36 dex and from ≃0.32 to ≃0.28 dex. At S/N = 20, denoising yields results consistent with those from the noisy inputs within the synthetic-test uncertainties. These controlled experiments suggest that hybrid CNN–transformer denoisers can enhance the usable low-surface-brightness area for stellar population studies, although further validation with observed spectra will be needed before practical application.

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APA 7

al, S. K. E. (2026). A Convolutional Neural Network–Transformer Denoiser for Low-signal-to-noise-ratio Galaxy Spectra: Stellar Population Recovery in Synthetic Tests. https://doi.org/10.3847/1538-3881/ae5a8c

MLA

al, Suk Kim et. "A Convolutional Neural Network–Transformer Denoiser for Low-signal-to-noise-ratio Galaxy Spectra: Stellar Population Recovery in Synthetic Tests." 2026. https://doi.org/10.3847/1538-3881/ae5a8c.

Chicago

al, Suk Kim et. 2026. "A Convolutional Neural Network–Transformer Denoiser for Low-signal-to-noise-ratio Galaxy Spectra: Stellar Population Recovery in Synthetic Tests.". https://doi.org/10.3847/1538-3881/ae5a8c.

Harvard

al, S. K. E. 2026, A Convolutional Neural Network–Transformer Denoiser for Low-signal-to-noise-ratio Galaxy Spectra: Stellar Population Recovery in Synthetic Tests, IOP Publishing, available at: https://doi.org/10.3847/1538-3881/ae5a8c [Accessed 29 Jun. 2026].

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Título
A Convolutional Neural Network–Transformer Denoiser for Low-signal-to-noise-ratio Galaxy Spectra: Stellar Population Recovery in Synthetic Tests
Autor / colaboradores
Suk Kim et al
Editorial
IOP Publishing
Año de publicación
2026
ISSN
1538-3881
ISSN
1538-3881
Idioma
eng

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