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Fig. 3

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Simultaneous fit of the Balmer lines, from Hβ to H8, for WD 1053−290 from the sample of Gianninas et al. (2011) by relying on ⟨3D⟩ (left panel) and 1D ML2/α = 0.8 (right panel) model spectra. Line profiles are offset vertically from each other for clarity and the best-fit atmospheric parameters are identified at the bottom of the panels. The instrumental resolution is of 6 Å. Line cores were partially removed from the ⟨3D⟩ fits (see Eq. (4)).

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