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Fig. 3

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Time-delay in the arriving γ-ray flux following a flaring episode obstained with both Monte Carlo and analytic (Eq. (22)) methods. The time’s shown are measured relative to the straight line (SO in Fig. 1) arrival time. For this plot, the time-delay of 1−3 GeV photons in a cascade from a source at z = 0.13 for a 10-15 G IGMF with coherence lengths 10 kpc (black lines) and 10 Mpc (red lines) are shown.

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