Deep Extragalactic VIsible Legacy Survey (DEVILS): Evolution of the σSFR-M⋆ relation and implications for self-regulated star formation
We present the evolution of the star-formation dispersion – stellar mass relation (σSFR-M⋆) in the DEVILS D10 region using new measurements derived using the ProSpect spectral energy distribution fitting code. We find that σSFR-M⋆ shows the characteristic ‘U-shape’ at intermediate stellar masses from 0.1<z<0.7 for a number of metrics, including using the deconvolved intrinsic dispersion. A physical …