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Fig. 13

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Illustration of the impact of an unsubtracted nucleus on the quantitative morphologies of the simulated AGN galaxies in concentration index C (upper left), asymmetry A (upper right), Gini coefficient G (bottom left), and M20 (bottom right). As a function of H/N, both plots show the initial value before (index ini) and after the addition of a synthetic nucleus (index unsub), normalized to the initial value. See text for a discussion.

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