Fig. 6.

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144 MHz radio luminosity as a function of absolute rest-frame UV magnitude at 1450 Å determined by SED fitting with EAZY. The upper axis indicates the corresponding black hole masses based on the empirical relation given in Eq. (1). The errors in M1450 are given by the 16th and 84th percentile on the M1450 distribution determined by randomly varying the measured fluxes within the error and refitting the SED.
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