Fig. 4
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Results of the isochrone fitting for ESO452-11. Panels a) and b) show the (mF606W − mF814W, mF606W) and the (mF606W − mF814W, mF814W) CMDs, respectively. The grey symbols describe the whole sample of stars in the cluster catalogue, while green symbols show the stars effectively used for the isochrone fit, selected as described in the text. The red line corresponds to the best-fit model. Panels c) and d) show the corresponding corner plots of the MCMC sampling.
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