Fig. 8

Weight distribution as a function of Teff for NGC 1705-1. Left panel: stellar parameters extracted from the empirical CMD, with a peak around ~3700 K. Middle panel: stellar parameters obtained from the theoretical isochrone for log (age) = 7.1 and Z = 0.008, the distribution peaks at ~3700 K. Right panel: stellar parameters extracted from the theoretical isochrone for log (age) = 7.1 and Z = 0.004, the peak is located at ~4000 K.
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