A multimodal neural network trained on MPA-JHU references produces SFR, stellar mass, and metallicity estimates for 547 million low-redshift galaxies in DESI LS DR10.
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Green valley galaxies live preferentially in the outskirts of galaxy clusters as satellites, consistent with environmental quenching processes.
Merger-disturbed cluster galaxies remain bluer than undisturbed ones across all locations and morphologies, possibly because mergers trigger star formation or protect central gas from stripping.
citing papers explorer
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A Value-added Physical Properties Catalog for Low-redshift Galaxies from DESI Legacy Imaging Surveys DR10
A multimodal neural network trained on MPA-JHU references produces SFR, stellar mass, and metallicity estimates for 547 million low-redshift galaxies in DESI LS DR10.
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Cluster-green galaxy correlations: where do these galaxies live?
Green valley galaxies live preferentially in the outskirts of galaxy clusters as satellites, consistent with environmental quenching processes.
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Impact of Galaxy Mergers on the Colours of Cluster Galaxies
Merger-disturbed cluster galaxies remain bluer than undisturbed ones across all locations and morphologies, possibly because mergers trigger star formation or protect central gas from stripping.