Absence of a correlation between the radio luminosity obtained with the VLA versus the X-ray luminosity in the 2–10 keV range (Pearson correlation coefficient = 0.31, p-value = 0.0055). In our analysis, we include all the Palomar LLAGN that have been detected by the VLA at 15 GHz (see Table A.3). While the new detections reported in this paper are shown with filled circles, the old detections are depicted by open circles.The relevant references to the X-ray data points are listed in the caption of Table A.3. Luminosities are given in erg s⁻¹.