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Fig. 18.

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Fraction of GAMA09 galaxies hosting both complex and compact radio AGN as a function of stellar mass, in different redshift (purple and green) and luminosity (panels) bins. A strong increase in the fraction of detected radio AGN with increasing stellar mass is observed. Orange shaded curves mark the results from Fig. 5 of Sabater et al. (2019) in the redshift range 0 < z < 0.3.

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