Fig. 15.
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Scatter plot of the dipole amplitude reconstructed for 300 datasets computed for various astrophysical scenarios, based on source model A, a 1 nG EGMF, the JF12+Planck GMF with λc = 200 pc, in the energy bins 4 ≤ E < 8 EeV and E ≥ 8 EeV. The cases of the four volume-limited catalogs listed in Table 1, which differ by their densities, are considered.
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