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Fig. 18.

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Skymaps in galactic coordinates showing the reconstructed directions of the dipoles for various astrophysical scenarios for each of the 300 datasets in five different energy bins (see the color code legend and text). The barycenters of the 300 datasets are shown by large squared markers. The predictions can be compared to the directions reconstructed by Auger shown by full circles and their 1σ error ellipses. The four panels show different scenarios for the GMF model and coherence length based on source model A and 1 nG EGMF (see legend and text).

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