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Fig. 6.

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Fraction of the secondary γ-ray flux in the energy range 1−10 GeV that is removed by the bubbles as a function of the size of the host AGN bubble. Red circles show the flux fractions that are removed by all bubbles. Black crosses and blue squares show the flux fractions that are removed by all bubbles, except for the host AGN bubble and a linear fraction of the LOS that is occupied by these bubbles. The dashed blue horizontal line marks the average linear fraction of the LOS that is occupied by all bubbles, except for the host AGN bubble.

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