Goodness of fit for the three WL surveys, DES (top panel), HSC (middle panel), and KiDS (bottom panel). Each panel shows a stacked observed profile in the count rate and redshift bin (stars), compared with the best-fitting weak lensing shear profiles according to mass calibration, i.e., the weak lensing masses based on the count rates of the clusters and calibrated scaling relations. The color bar indicates the count rate binning applied to DES and HSC, while tomographic bins for KiDS. For a more extensive description of the weak lensing goodness of fit, see Grandis et al. (2024), and Kleinebreil et al. (2024).