Fig. 7
The K-band and 1 GHz luminosity (νLν) for all extra-galactic radio sources in our sample (top) and a volume-limited sample (bottom). Most sources that are morphologically classified as AGN (i.e., the Jets and Lobes class) are more luminous than νLν = 1039+erg s-1. Our volume-limited sample shows that the galaxy NIR luminosity and radio luminosity are not strongly correlated.
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