Using the SED-fitting code ProSpect to trace star formation over the last 8 billion years

The Deep Extragalactic VIsible Legacy Survey (DEVILS) is a new spectroscopic campaign aimed at bridging the near and distant Universe by producing the highest completeness survey of galaxies at intermediate redshifts. It is at this under-sampled epoch where both galaxies and their host halos undergo significant evolution. With preliminary redshifts from DEVILS and the plethora of auxiliary data in the COSMOS field, we can begin to use DEVILS to understand the evolution of galaxies over the last 8 billion years. Using our new spectral energy distribution fitting code ProSpect, we have measured the star formation histories, stellar masses, and star formation rates for half a million galaxies in the D10-COSMOS field and are using these measurements to trace the evolution of star formation and stellar mass build-up in galaxies