Radial acceleration relation for X-COP galaxy clusters. The solid colored curves show the result of the Einasto fit to the baryons+DM model, whereas the individual data points indicate the accelerations computed using the nonparametric log-normal mixture model (NP). For comparison, the solid black curve and shaded area show the RAR obtained by McGaugh et al. (2016) for rotationally supported galaxies and the associated 0.06 dex scatter. The dashed line indicates the one-to-one relation.