Result of the BS and CenA flux excess analyses for our baseline volume-limited scenario, after scanning over the same parameter space in E_th and ψ as Auger (see text). Scatter plot of the CenA flux excess maximum significance versus the BS maximum significance obtained for 300 datasets using the JF+Planck (left) and the Sun+Planck (right) GMF models. Various coherence lenghts λ_c are considered for the GMF turbulent component (see legends). The values reported for Auger dataset at the ICRC 2019 are shown with a large black circle, the distributions of $({\sigma }_{\max }^{\mathrm{BS}}$ and ${\sigma }_{\max }^{\mathrm{CenA}})$ are also shown separately on top of the coordinate axis.