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Fig. 10.


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Cumulative distribution function of angular deflexions of UHECRs (including all species) with energy reconstructed on Earth between 8 and 16 EeV coming from sources in various distance bins (see legend). The cases displayed assume the source model A, 2MRS-based catalogs with source density 1.4 × 10−3 Mpc−3 in the volume-limited approach and a full sky exposure (with twice Auger statistics). The top panel shows the deflexion assuming a 1 nG and no GMF while on the bottom panel the same EGMF is assumed together with the JF12+Planck GMF model with λc = 200 pc.

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