Distribution of the locations of the BS maxima for the 300 datasets. The case of the JF+Planck model with λ_c = 200 pc (left) and the Sun+Planck model with λ_c = 100 pc (right) are shown. The colour scale represents the fraction of realisations for which the BS maximum is found in a given pixel of the sky (the pixel size correspond to Nside = 8 on these plots). The position of the CenA radio galaxy as well as the BS maximum location reported by Auger at the ICRC 2019 are shown with a red full circle and black star respectively (the two markers are practically on top of each other). The large red star shows the direction of the asymptotic BS maximum obtained with a 300 times larger simulated dataset (see text).