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Fig. A.1.
Comparison between the parameters (Teff, log g, and log nhe) derived for the stars in common between the VIMOS sample and the other samples. The differences (Δ) are expressed in terms of the value derived with the VIMOS spectrum minus the value derived from the other sample, e.g. ΔTeff = Teff (vimos) − Teff (other).
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