Consistency test between the density contrast profiles of clusters observed both in DES (HSC) and KiDS in the upper (lower) panels. Given the correlated intrinsic galaxy shapes, we constructed the statistical uncertainty estimates by bootstrapping on the union of the respective source catalogues. We find that, averaged over all objects, the estimates from the survey pairs are consistent as a function of radius (left column). Also, the uncertainty weighted mean square deviation of all clusters, shown in the right column, is consistent with the expectation (red curve).