CDFs of the largest effective (left panels) and median (right panels) Einstein radius for a different number of maxima in the range between 125 and 4000, assuming the Tinker et al. (2008) mass function, M_lim = 2×10¹⁴ M_⊙ / h and the redshift interval of 0.5 ≤ z ≤ 1.0 on the full sky. The upper row shows the CDFs directly based on the MC simulations, and the lower row presents the corresponding fits of the GEV distribution. The small lower panels show the difference, ΔCDF, with respect to the high-resolution run based on 4000 maxima.