Fig. 7.

image

Left panel: fraction of galaxies that host a radio AGN with L150 MHz ≥ 1022.5 W Hz−1, as a function of the black hole mass, for multiple stellar mass bins (shown in different colours). Right panel: fraction of galaxies hosting radio-AGN with L150 MHz ≥ 1022.5 W Hz−1, as a function of the stellar mass, separated by their black hole mass (shown in different colours).

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