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Fig. 8


Angular profiles of the images of the sources represented in Fig. 7. We represent the gamma-ray flux integrated over energies Eγ = 1−100   GeV averaged over angular bins, for a filament seen along its axis, at 1 Gpc and LE,19 = 1046 erg s-1 (black solid line), and at 100 Mpc and LE,19 = 1044 erg s-1 (green dashed line). The black stars and green crosses present the corresponding integrated flux up to a given angular extension in the sky θ.

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