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tagline ="Fitting astrophysical star formation histories via CMD modeling",
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descr ="""
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- Implements methods for modeling observed Hess diagrams (i.e., binned color-magnitude diagrams) and using them to fit astrophysical star formation histories (SFHs)
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- Provides utilities for simulating CMDs given input SFHs and photometric error and completeness functions, which can be useful for planning observations and writing proposals
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