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We introduce ProSpect, a generative galaxy spectral energy distribution (SED)package that encapsulates the best practices for SED methodologies in a numberof astrophysical domains. ProSpect comes with two popular families of stellarpopulation libraries (BC03 and EMILES), and a large variety of methods toconstruct star formation and metallicity histories. It models dust through theuse of a Charlot & Fall attenuation model, with re-emission using Dalefar-infrared templates. It also has the ability to model AGN through theinclusion of a simple AGN and hot torus model. Finally, it makes use ofMAPPINGS-III photoionisation tables to produce line emission features. We testthe generative and inversion utility of ProSpect through application to theShark galaxy formation semi-analytic code, and informed by these resultsproduce fits to the final ultraviolet to far-infrared photometric cataloguesproduces by the Galaxy and Mass Assembly Survey (GAMA). As part of the testingof ProSpect, we also produce a range of simple photometric stellar massapproximations covering a range of filters for both observed frame and restframe photometry.

ProSpect: Generating Spectral Energy Distributions with Complex Star Formation and Metallicity Histories