Fig. 6
Relationship between radio luminosity and black hole mass for bright galaxies detected at 43 GHz. Filled circles and open squares indicate detected and non-detected galaxies at 43 GHz. The crosses represent detected galaxies with L43 GHz < 1023 W Hz-1. The correlation coefficients are derived from the sample of bright L43 GHz > 1023 W Hz-1 galaxies detected at 43 GHz. There is no apparent correlation between black hole mass and radio luminosity at any frequency.
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