Fig. 9
Relation between radio luminosity and the Eddington ratio for bright and detected galaxies at 22 GHz. Filled circles and open squares indicate the detected and non-detected galaxies at 22 GHz. The crosses represent the detected galaxies, but with L22 GHz < 1023 W Hz-1. The correlation coefficients are derived from the sample of bright L22 GHz > 1023 W Hz-1 and detected galaxies at 22 GHz.
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