Histograms showing the parameter distributions of the G9 radio AGN split into different environments. Radio AGN in dense environments (black unfilled, magenta hatched) are not the cause for the upturn in the measured incidence seen in Fig. 22, as they have the same λ_Jet distribution as the ones in low density (light blue filled) environments. We note that the GAMA cosmic web environment catalogue is limited to 0.04 < z < 0.263, so this is applied to all datasets shown here, along with the appropriate mass completeness cuts.