Same as Fig. 6, but here we compare the M_BH and Ṁ/Ṁ_Edd estimates obtained from the MCMC combined analysis that includes both the AGN X-ray non-detection and the broad-line emission constraints, with those from L24, where the MCMC analysis was based only on the broad-line emission properties. For reference, black data points show, on the y axis, the values reported in the literature based on single-epoch estimates. For each object, the low-mass, high-mass, and literature estimates are shown with the same marker.