Fig. 9.

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CMD of the HST data for Rup 106 and IC 4499 (left and right bi-panels, respectively). The ACS data used to sample the core region are complemented with a catalogue obtained with ACS and WFC3 parallel observations for Rup 106 and IC 4499, respectively. The open squares indicate the mean ridge lines of the clusters, while the solid curve shows the best-fit isochrones.
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