Ionised mass outflow rate as a function of AGN bolometric luminosity. Different shapes represent the literature of the sources. The black dashed line is the scaling relation obtained in Fig. 11. In the left panel of Fig. F.1, the sources are colour coded with the Eddington ratio. In the left panel, the sources are colour-coded with the black hole mass. Among the sources with black hole masses, we observe a correlation trend in the sense that AGNs with high black hole masses also appear to have high bolometric luminosity and higher mass outflow rates. In the right panel, the sources are colour-coded with the Eddington ratio. AGNs with high Eddington ratio values appear to have high mass outflow rates and bolometric luminosity. The error bars on mass outflow rate values were obtained by extrapolating the errors on FWHM or δV whenever available.