The fundamental plane of black hole accretion (Merloni et al. 2003) is shown with the solid line, with its ~0.88 dex scatter. We show all the sources in our low-z sample which can be matched to an archival radio observation. We highlight in orange galaxies with a SFR estimate and a radio luminosity brighter than that predicted by SFR. The top panel shows radio fluxes extrapolated assuming a radio spectral index of -1, the bottom using a flat slope.