Fig. 24.

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Fraction of GAMA09 galaxies hosting purely X-ray-detected AGN (blue) and both X-ray and radio AGN (green) as a function of λEdd. The stellar mass, radio luminosity and X-ray luminosity are ensured for completeness. The pure X-ray fractions follow well the Aird et al. (2012) trend, whilst the radio and X-ray AGN lie an order of magnitude below it.
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