Observed number counts (left), two-point correlation function (middle), and weak-lensing masses (right), compared to the corresponding predicted quantities evaluated at the best-fit cosmology of the contours in Fig. 1 (same color code). The black dots are the observed points, and the colored lines and shaded areas represent the mean and standard deviation of each statistics, respectively, evaluated at 100 cosmologies that were randomly extracted from the posterior distribution, convoluted with the covariance matrix through a multivariate Gaussian distribution.