Table C.1.
Summary of the results of fitting the Li region of the solar flux spectrum (Kurucz 2005) with 1D LHD and 3D CO5BOLD synthetic spectra.
| Fit ID | Model | Continuum level | Abundances | Wavelengths | A(Li) (dex) | q(Li) (%) | χ2 |
|---|---|---|---|---|---|---|---|
| I | 1D LHD | 0.9977 | adjusted | G09 | 0.94 | 0.69 | 8.2 |
| Ia | 3D CO5BOLD | 0.9977 | as Fit I | G09 | 1.05 | 1.86 | 251.3 |
| Ib | 3D CO5BOLD | 0.9977 | Fit I +ΔA | G09 | 1.04 | <−2.0 | 53.6 |
| Ic | 3D CO5BOLD | 0.9977 | Fit I +ΔA | G09 +Δλ | 1.05 | −0.18 | 7.3 |
| II | 1D LHD | 0.9980 | adjusted | G09 | 0.96 | 1.67 | 7.9 |
| IIa | 3D CO5BOLD | 0.9980 | as Fit II | G09 | 1.06 | 2.88 | 247.3 |
| IIb | 3D CO5BOLD | 0.9980 | Fit II +ΔA | G09 | 1.06 | −0.89 | 54.0 |
| IIc | 3D CO5BOLD | 0.9980 | Fit II +ΔA | G09 +Δλ | 1.06 | 0.88 | 6.1 |
| IIx | 3D CO5BOLD | 0.9980 | SIS18 | G09 | 1.09 | 1.77 | 29.5 |
Notes. Column (4): ΔA symbolizes the individual 3D abundance corrections; “SIS18” indicates the same abundances as used in Strassmeier et al. (2018). Column (5): G09 denotes the line list of Ghezzi et al. (2009), Δλ symbolizes the individual convective line shifts. The relative quality of the fits can be judged by comparing their χ2 (given on a common absolute scale).
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