... processing?

Based on observations at the Very Large Telescope of the European Southern Observatory, Cerro Paranal/Chile under Program 65.L-0317(A, B).

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...$\log \epsilon({\rm Li}) = 0.1$

Throughout the paper, the Li abundance is given on the scale $\log \epsilon({\rm Li}) = \log N({\rm Li})/N({\rm H}) + 12$. The solar photospheric Li abundance on this scale is $\log \epsilon({\rm Li}) = 1.1$.

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