Relation between outflow velocity and Σ_SFR. Our sample is color-coded by the SFR(Hβ)/SFR_SED ratio. Our sample is divided into galaxies with blue- (crosses) and redshifted (pentagons) broad components. The dashed black line corresponds to the best slope from Arribas et al. (2014), and the black squares show their observed data. The dashed green line is our best fit. The dashed red line is the best fit from Xu et al. (2022b). Two galaxies with broad components (CDFS023527 and 511245444) are excluded from this plot because Hα and Hβ are not included in the observed spectral range.