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Fig. 14


Measurements of the detached eclipsing binaries V18 and V20 and the cluster (V − I)0,V CMD compared to isochrones with  [Fe/H]  =  +0.30 and Y = 0.33. The observations in the CMD are from a 2010 re-reduction of the SBG03 data set by Stetson (see VandenBerg et al. 2010). Only the stars with the highest precision VI photometry have been plotted.

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