Fig. 22.

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Fraction of GAMA09 galaxies hosting both compact and complex radio AGN as a function of the specific black hole kinetic power, λJet, in different stellar mass and redshift bins. The markers plot all the sources, while the shaded region shows the incidences of just the S_code = S sources. In contrast to the compact-only case, a larger mass dependence is present, as well as a boosted incidence at high λJet (diamonds) values, indicating a jet power dependence. A power law plus Gaussian fit is used to approximate the data (solid curves), for which fit parameters are presented in Table 3.
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