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Fig. 10.

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Redshift distribution of the values of AV inferred from the Balmer decrement in sources with detected Hα and Hβ lines. For sources with upper limits on Hβ we derived lower limits on AV. On the left, we also report the median values of AV for NLAGN (magenta), non-AGN (cyan) and for the global population (black) in four different redshift bins. Errors are derived using the bootstrap procedure. On the right, we report the histogram of the AV distribution for AGN (red) and non-AGN (blue).

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