Fig. A.1
Top four panels: stellar parameters recovered by BeSPP for the ideal synthetic stellar sample drawn from the tracks (see text). Bottom four panels: stellar parameters (Teff, log g, [Fe/H]) recovered by BeSPP compared with the input spectroscopic values for the UVES stars. The total χ2 was computed summing over the three spectroscopic parameters and using only the observational errors.
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