The basic idea of silkscreen is to use simulation based inference combined with artpop to infer properties of dwarf galaxies directly from their images. The original goal was to accurately measure distances in the semi-resolved regime but it can also be used to infer metallicites and star-formation histories. Check back soon for a more detailed tutorial!
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This package is still under active development and testing and should not be used in its current state. Please check back soon for updates!
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