Fig. 5.
AGN selection via the radio excess parameter. The dotted lines correspond to the AGN selection criteria of Del Moro et al. (2013) and sources below this line are classified as AGN. Upper limits are denoted by the arrows. The local radio-loud AGN, Hydra-A and the hybrid system NGC 1068 are denoted by the triangle and star markers, respectively. Left panel: q24 radio excess parameter for the VLBI selected sample. The shaded region corresponds to the q24 evolution predicted by Del Moro et al. (2013) using a range of star-forming galaxy templates. Right panel: q100 radio excess parameter for the VLBI selected sample.
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