Fig. 15

Comparison between our 1D NLTE A(Li) corrections with the other authors for the model with Teff=6500 K, log g =4.0 and [Fe∕H] = −1.0. Our original corrections (M19, black solid line) have been shifted down (M19, black dots) by 0.055 as found by Harutyunyan et al. (2018) to account for the difference between LHD and MARCS model atmospheres. The version of the models adopted by the different authors are indicated in the legend.
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