Fig. 4.
Comparison between the MILES and ELODIE solutions in the UVB for the stars with Teff (MILES)> 4000 K. Each atmospheric parameter is shown in a separate panel, and the colour of the symbols identify two temperature ranges (dividing at 5500 K). Stars hotter than 7000 K are shown as crosses. In the Teff and logg panels, seven and two outliers, respectively, are not shown (all hot stars). The dispersion σ and mean offset μ for the two temperature ranges are indicated.
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