Summary of the wind properties in the DWALIN-19 sample. Ionised gas outflow rate, Ṁ_wind, (left-hand panels) and mass-loading factors β (right-hand panels) as a function of galaxy M_⋆ (first row), SFR (second row), mean SFR surface density (third row), and sSFR (fourth row). Each galaxy is labelled with an ID number (see legend on top). Data points are based on the average of values from the turbulence and TES scenarios; error-bars account both for the difference between the two scenarios and for the uncertainties associated with each of them (see text). Spearman (S) and Pearson (P) correlation coefficients are reported on top of each panel. Blue-dashed lines show the best-fit linear relations determined with the LTSFIT Python package (Cappellari et al. 2013), with the blue-shaded region showing the resulting intrinsic scatter σ_int. Values for the line slope, m, intercept, c, and σ_int are reported in each panel.