Difference in the amplitude of the isothermal sphere shear profile models fitted to clusters with coverage by DES and KiDS (HSC and KiDS) in the left (right) panel plotted relative to the uncertainty of this difference and as a function of cluster redshift and richness (columns) for the different KiDS tomographic redshift bins (rows). We found excellent overall agreement, while no richness or redshift trends are evident from visual inspection, also after binning (black points).