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Fig. 6.

image

Comparison of the stellar parameters for GBS as estimated by this analysis and Heiter et al. (2015a), Jofré et al. (2014) (shown as ours theirs versus ours). The fundamental parameters Teff and log g are shown in the two top panels, together with comparisons of metallicity with their recommended iron abundance [Fe/H], microturbulence velocity, and broadening velocity, a convolved parameter of macroturbulence and rotational velocity, in the three bottom panels. Black error bars are the combined uncertainties of GBS as well as the error output of our analysis pipeline (SME). Green error bars include precision uncertainties from repeated observations and blue error bars include both precision and accuracy estimates.

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