Comparison of median kinematic radial profiles. The symbols and colours are identical to those of Fig. 5. First row: a comparison between AGNs and controls. From left to right: residual between the [O III]λ5007 gas and stellar velocities and residual between the corresponding velocity dispersions. Second row: same as in first row, but comparing strong and weak AGN hosts. Third row: same as first, but comparing early- and late-type AGN hosts.