Examples of typical sky maps corresponding to the proton-dominated MC-high model with extremely high source density, n_s = 1.6 10^-3 Mpc^-3. The first (top) panel shows one of the realizations that gave the weakest signal of anisotropy (out of the 500 realizations simulated) with the current Pierre Auger Observatory statistics. The second panel shows the realization lying in the middle of the distribution (see text). The third and fourth panels show the expected sky maps with the reference statistics of JEM-EUSO with thresholds at 80 EeV and 100 EeV, respectively, for the same realization as in the second panel (Pierre Auger Observatory energy scale).