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.