Cluster-satellite correlation signal, measured using red-sequence candidates brighter than M^⋆ + 1, as a function of projected separation from the BCG, for the different cluster samples, split in richness (as indicated on top of each column) and redshift (indicated in each panel). The solid black lines indicate the best-fit cluster halo models, obtained from simultaneous fits to the lensing signal and the cluster-satellite correlation signal in the range Mpc. The dotted red line shows the contribution from correctly centred clusters, the dashed green line the contribution from miscentred clusters, and the dotted-dashed blue line the contribution from neighbouring haloes. Note that the measurements are correlated at large scale (see Fig. 5), which is accounted for in the fit. The dark red, orange and yellow shaded areas correspond to the 1, 2 and 3σ model uncertainty.