We infer the intrinsic ionized gas kinematics for 383 star-forming galaxies across a range of integrated star formation rates (SFR{in}[10^-3^, 10^2^]M_{sun}/yr) at z~~1M{sun}/yr. This is consistent with recent theoretical models that suggest a {sigma}_v,z floor driven by star formation feedback processes with an upturn in {sigma}v,z at higher SFR driven by gravitational transport of gas through the disc.
Cone search capability for table J/MNRAS/495/2265/tablea1 (Galaxy properties for the from the SAMI Galaxy Survey analysed in this work)