Uncertainty σ_reco on the log of the reconstructed black hole mass M_BH for Type 1 and 2 AGN, with and without z information (estimated with ML_w/z and ML_wo/z respectively). The & values correspond to the median of their distributions. All AGN types can be reconstructed, as proven by their characteristic PDF structures, although the overall reconstructed uncertainties worsen as a function of the AGN class.