Fig. 11.
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Histogram of ages of all clusters in this work with median CMD classes greater than 0.5 – specifically, all clusters with photometry that is compatible with a single population of stars. These are compared to the ages of all clusters in the catalogues of Kharchenko et al. (2013), Kounkel et al. (2020), and Cantat-Gaudin et al. (2020). Known GCs are excluded from the results of this work and the results of previous works for this plot.
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