Comparison of model predictions for the logarithmic derivative of the three-dimensional cross-correlation function with the best-fitting mass–richness relation parameters for the clusters at 0.1 ≤ z_cl ≤ 0.4 with 15 ≤ N ≤ 200 in Murata et al. (2019) from the fiducial analysis under the Planck cosmology. “Fiducial model” shows our fiducial model in equation (A1) that fully accounts for the scatter in the mass–richness relation, “M_200m > M_min to match 〈M_200m〉” for the method in More et al. (2016), and “〈M_200m〉, 〈z〉” for the method in Zürcher and More (2019) (see the text for more details). The vertical lines show the three-dimensional splashback radius location |$r_{\rm sp}^{\rm 3D}$| for each method. (Color online)