Fig. 1

A comparison of the Earth-arrival directions of all UHECRs with energies above 56 EeV detected by PAO (blue for UHECRs with energies ≥75 EeV and green for UHECRs with energies between 56 and 75 EeV) and AGASA (red open circles of radius 3.5°) with the estimated outside-the-Galaxy arrival directions of the same UHECRs (small colored dots) for our Monte Carlo simulations of the BS-S (red), AS-S (green), BS-A (blue), and AS-A (yellow) GMFs using a proton composition for the UHECRs. The colored circular symbols indicate the positions of galaxies with radio jets at D ≤ 75 Mpc (red), 75 Mpc < D ≤ 200 Mpc (blue), and 200 Mpc < D ≤ 500 Mpc (black). In all redshift bins, filled circular symbols are used for galaxies with radio structures more extended than 180 kpc, and open circular symbols for galaxies with radio structures less extended than 180 kpc. Galactic SGRs (red triangles) and AXPs (blue triangles) are also plotted. The Supergalactic plane is marked by the dashed line. In this and following figures we use an Aitoff-Hammer (equi-area) projection in Galactic coordinates.
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