In this directory you can find some pratical use cases to get you up to speed!
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A first glimpse about creating and manipulating an
SSPobject is provided in simple_stellar_population.ipynb. -
Several examples of how to build a
ChemicalEvolutionModelcan be found in the models directory.- Many of them are based on analytical expressions for the star formation and chemical enrichemt histories.
- A
TabularCEMcan be used to build models from tabulated data. - A set of individual simple stellar populations (referred to as "particles") can be combined using
ParticleListCEM.
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There is also a tutorial showing how to generate a grid of photometric fluxes from a given model, including the effects of redshift, and dust attenuation.