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Fig. A.2.

image

Diagrams comparing the clumpiness of our final galaxy sample to the Gini and M20 coefficients (first and second panels, respectively), and to the mergerness parameter, defined in Eq. (3). Starbursts are shown with red filled circles, while main sequence galaxies are empty squares and color coded in blue. The median clumpiness (and errors), computed in bins of Gini, M20 and mergerness, are represented with gray squares and black error bars.

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