Fig. 9
Comparison of integrated colours as a function of age and metallicity, from models using different sets of isochrones with Magellanic Clouds cluster observations of González et al. (2004, G04) and Pessev et al. (2008, P08), and Milky Way clusters from Cohen et al. (2007, C07). These data have estimated metallicities of ~−0.9 dex or higher. The error bars represent the typical uncertainties of the cluster colours and inferred ages.
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