Large-scale disruptive kinetic feedback efficiency (i.e. ratio of jet kinetic energy divided by host halo binding energy) as a function of halo mass for the massive galaxy population (black-hatched area) in the redshift range 0 < z < 0.4. The respective contributions from compact and complex radio AGN are shown in light and dark blue shaded regions respectively. The grey-shaded area shows the large-scale disruptive feedback efficiency on the baryonic halo mass (assuming a mass-dependent gas fraction). The red and purple lines are the same as in Figure 4. The horizontal black dashed line marks the equality of the jetted kinetic energy and the host halo binding energy.