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Fig. 11.

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Comparison of Hδ measurements of CIGALE with the input (data) values for the AGNs (top panel) and the galaxies in the reference catalogue (bottom panel) when the line is not used as an input in the fitting process. The algorithm tends to overestimate the true values, in particular for EWs higher than ∼0.1. Solid black lines present the 1:1 relation.

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