Fig. B.2.
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Same as Fig. 1. Magenta and blue lines correspond to the calculation of the diffuse flux assuming that all the sources have the same spectral shape as NGC 1068 (for sp = 2 and 3 respectively – see fig. B.1) re-normalized in respect to LX and the pγ efficiency. Dashed lines refer to the coronal model itself while solid lines also include the BL Lac population.
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