Fig. B.3

Comparison of the atmospheric parameters determined by us with those from Valdes et al. (2004). We plot 84 O, B, and A type stars in common between the two data sets. Two Teff outliers are not displayed. Five log g and 18 [Fe/H] discrepant measurements are shown as red crosses and are discussed in the text. The axes are as in Fig. 8, besides Teff is in log10.
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