The MAGPI Survey: the Interdependence of Mass, Star Formation Rate, and Metallicity in Galaxies at Z 0.3

Star formation rates (SFRs), gas-phase metallicities, and stellar masses are crucial for studying galaxy evolution. The different relations resulting from these properties give insights into the complex interplay of gas inside galaxies and their evolutionary trajectory and current characteristics. We aim to characterize these relations at z∼ 0.3, corresponding to a 3-4 Gyr lookback time. We utilize optical integral field spectroscopy of 65 emission-line galaxies from the MAGPI survey at a redshift of 0.28更多