Fig. C.2.
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Distribution of the non-parametric image morphological parameters for galaxies in our sample, with different colour as a function of their merger stage, according to the legend. From left-to right: Clumpiness (S), Gini index (G), Moment of light (M20), inverse concentration index (ICI), and asymmetry (A). The distribution of the same parameters for all MaNGA galaxies is shown (in grey) for reference.
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