HIGHLIGHTS
SUMMARY
Other examples include the SFR and stellar mass functions, two demographics that can be computed for galaxies in different redshift bins and are commonly used to either calibrate or validate cos- mological simulations (e_g, Henriques et_al 2013; Furlong et_al 2015; Katsianis et_al 2017; Davé et_al 2017). Those templates are built via stellar population synthesis models (e_g, Bruzual and amp; Charlot 2003; Maraston 2005; Conroy et_al 2009), assuming a grid of ages and metallicity values, different star formation histories (SFHs), and one or more options for dust attenuation (for a review, see Conroy 2013). A . . .
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