All Tables

• Table 1: Best fit parameters for the IT effect on the catalogue presented in this paper. The first line, in bold face, refers to the entire catalogue, while the following lines refers to Seyfert galaxies (S), Quasars (Q), Broad-line objects (B) and Narrow-line objects (N). Correlations with Eddington ratio (LD/C: luminosity-dependent or constant X-ray bolometric correction), BH mass and redshift follow.