Fig. 8.
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Optical Gaia EDR3 (right panel) and near-IR VVVX+2MASS (left panel) CMDs for the GC Garro 02. We have included only PM-selected members, considering also those stars with a membership probability greater than 50%. The isochrone-fitting method yields an Age = 12 Gyr and [Fe/H] = −1.30 dex. We have superimposed the PARSEC model represented as red dotted lines in both panels.
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