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Fig. A.1.

Fig. A.1. Refer to the following caption and surrounding text.

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Top: Best-fit SE++ single-Sérsic effective radius versus IE magnitude diagram with highlighted unsaturated stars (blue) and galaxies (green). The morphological distinction is based on the size boundary overlaid in red. Bottom: Galaxies (green) and stars (blue) distributed in the B − IE versus IE − HE plane, showing the stellar locus and the red sequence of passive cluster member galaxies.

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