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Fig. 12


18 Sco MC output distributions of λ8542 and as a function of Teff, [Fe/H] and log gare shown. Upper panels: we consider input errors of 50 K, 0.1 dex, and 0.07 dex of Teff, [Fe/H], and log g. Middle panels: λ8542 output distribution. Solid gray line refers to the photospheric correction and the solid red lines are 1σ and 2σ confidence intervals. Lower panels: correlations with atmospheric parameters.

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