Fig. 10.
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SAPP best-fit parameters of Gaia-ESO HR10 spectra produced using the Bayesian scheme, with resolution R = 20 000 and coverage λ ⊂ [5300, 5600] Å. In total there are 17 benchmark stars depicting a different parameter (Teff log g, [Fe/H] and [Mg/Fe]) derived from SAPP (vertical axes) versus the given reference parameter (horizontal axes). The panels represent data determined using the Bayesian scheme without asteroseismology (upper) and with asteroseismology (lower). The red data points represent stars without any asteroseismic parameters.
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