dependence on the presence of a stellar bar or AGN. Top row: s of PHANGS galaxies as a function of the host galaxy’s stellar mass (left) or SFR (right) for barred (blue circles) and unbarred galaxies (cyan diamonds) (galaxies without a bar classification: grey cross). Histograms of the barred (blue) and unbarred (cyan) sub-sample are added for stellar mass (top left), SFR (top right panel) and (far right panel). Bottom row: Analogous plot for galaxies hosting an AGN (purple circles) or not (orange diamonds). Histograms of the AGN (purple) and non-AGN (orange) sub-samples are added for stellar mass (top left), SFR (top right) and s (far right panel). Spearman rank correlation coefficient between and galaxy property are listed at the bottom of each panel, for the respective sub-samples (ρ_bar, ρ_no bar, ρ_AGN, ρ_no AGN). For comparison, the Spearman rank correlation coefficient of the full sample between and stellar mass is ρ_M⋆ = 0.56 ± 0.03 and between and SFR is ρ_SFR = 0.40 ± 0.03. Typical uncertainties for and the galaxy property are added in the upper left corner of each panel.