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The paper presents a method for calculating K-corrections and filter transformations for galaxies using nonnegative matrix factorization, which allows for the creation of model-based templates from heterogeneous photometric and spectroscopic data. This approach is designed to handle uncertainties and missing data while providing interpretable results in terms of stellar masses and star formation histories. The authors also release software for estimating K-corrections and fitting templates to galaxy data, a

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Meet Panchal

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EN