SIMBAD references

We infer the intrinsic ionized gas kinematics for 383 star-forming galaxies across a range of integrated star formation rates (SFR ∈ [10^–3, 10²] M_☉ yr^–1) at z <= 0.1 using a consistent 3D forward-modelling technique. The total sample is a combination of galaxies from the Sydney-AAO Multiobject Integral field Spectrograph (SAMI) Galaxy survey and DYnamics of Newly Assembled Massive Objects survey. For typical low-z galaxies taken from the SAMI Galaxy Survey, we find the vertical velocity dispersion (σ_v,z) to be positively correlated with measures of SFR, stellar mass, H I gas mass, and rotational velocity. The greatest correlation is with SFR surface density (Σ_SFR). Using the total sample, we find σ_v,z increases slowly as a function of integrated SFR in the range SFR ∈ [10^–3, 1] M_☉ yr^–1 from 17 ± 3 to 24 ± 5 km s^–1 followed by a steeper increase up to σ_v,z ∼80 km s^–1 for SFR >= 1 M_☉ yr^–1. This is consistent with recent theoretical models that suggest a σ_v,z floor driven by star formation feedback processes with an upturn in σ_v,z at higher SFR driven by gravitational transport of gas through the disc.