log g versus Teff distribution for DA white dwarfs in the GB11 sample derived from ⟨3D⟩ (top) and 1D spectra (bottom). An evolutionary model from Fontaine et al. (2001) at the median mass of the sample (0.61 M⊙, 13 000 < Teff (K) < 40 000) is shown as a dashed line. The error bars on the top left represent the mean uncertainties in this Teff range.
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