Mass outflow rate versus AGN luminosity. Diamonds symbols show the sample from Cicone et al. (2014), for which Ṁ_out have been scaled down by a factor of three to match our outflow geometry definition. The sample of Ramos Almeida et al. (2022) is shown with triangles. Horizontal lines for the Ramos Almeida et al. (2022) sample indicate the position that they would occupy if we were to use the L_AGN derived from SED fitting from Jarvis et al. (2019), instead of the one derived from the [O III] luminosity (see Ramos Almeida et al. 2022, for details). The Lutz et al. (2020) sample is shown with red pentagons. For the Stuber et al. (2021) sample (stars), the AGN luminosities have been derived from the 14–195 keV X-ray luminosity. Symbols for the PUMA sample are as in Fig. 1. The dashed and dotted lines show the relations presented by Cicone et al. (2014) and by Fiore et al. (2017), respectively, scaled down by a factor of three to match our outflow geometry definition.