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Fig. 5.

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Outflow mass rate and kinetic power as a function of the bolometric luminosity of the AGN. Light and dark blue squares correspond to the values derived from the parametric method using vs and vmax, respectively. Green and orange circles are the values from the flux-weighted and peak-weighted nonparametric methods. The values from Fiore et al. (2017) are shown as gray triangles for comparison.

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