All Tables

• Table 1: Performance of the different parameter estimators. The given uncertainties is the standard deviation of the fit parameters obtained from different artificial datasets.
• Table 2: Best fit results for the KFC sample and the original and edited MHDM sample. Besides the full sample we also give the parameters for the subsamples containing only a limited set of AGN classes. Note that LINER sources classified by MHDM are not limited to LLAGN. The LH XRB sample is defined in Sect. 2.1. The column N denotes the number of sources in the sample.
• Table 3: Effect of the observing flux limits on correlated data: most radio fluxes in our sample are obtained with the VLA, which can detect 0.1 mJy within a 10 min snapshot. Chandra can go as deep as 10^-14 erg/s/cm² in a 1000 s observation.