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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.

This figure is made of several images, please see below:

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