Left: mass outflow rate as a function of the AGN bolometric luminosity. The black dots mark the ionized outflow measurements from Fiore et al. (2017), and red stars show our estimate for the four galaxies of our sample. The dashed black line is the best-fit correlation from Fiore et al. (2017) for their ionized outflow sample. Middle: kinetic power as a function of the AGN bolometric luminosity. Right: AGN bolometric luminosity as a function of the maximum outflow velocity.