Notes. The spectral types were taken from Véron-Cetty & Véron (2006). The luminosity distance and spatial scale were calculated using a cosmology with H₀ = 70 km s⁻¹ Mpc⁻¹, Ω_m = 0.3, and Ω_Λ = 0.7. The ionised mass outflow rates are from Davies et al. (2020). The intrinsic L_{14 − 195 keV} and N${}_{\mathrm{H}}^{\mathrm{X}-\mathrm{ray}}$ were taken from Ricci et al. (2017). Bolometric luminosities are obtained from the 14–195 keV X-ray intrinsic luminosities by multiplying by a factor of 7.42 as in García-Bernete et al. (2019). The inclinations of the disk and ionisation cones are from Fischer et al. (2013), Shimizu et al. (2019) and Alonso-Herrero et al. (2023).