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Fig. 3

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Simulated all-sky maps of the 511 keV intensity distribution (in ph cm-2 s-1 sr-1) for all nucleosynthesis positrons, with an SN Ia escape fraction of 5% for 56Ni positrons, and for the three halo GMF configurations. From top to bottom, the maps correspond to no halo field, the dipole field, and the X-shape field. The sky maps have been put on the same intensity logarithmic scale.

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