Fraction of XXL bright cluster galaxies hosting an X-ray AGN for a flux-limited sample (F_{X [0.5-10 keV]} > 10⁻¹⁴ erg s⁻¹ cm⁻²), divided by the field fraction. The results are plotted as a function of distance from the cluster centre. No AGN suppression is present in our low-mass cluster sample, in contrast to the results of Ehlert et al. (2014) on massive clusters. Error bars indicate the 1σ confidence limits for small numbers of events (Gehrels 1986).