Left-hand plots: comparisons of Li abundances and effective temperatures for 117 stars in common with Ramírez et al. (2012); right-hand plots: comparisons for 33 stars in common with Delgado Mena et al. (2015). The red dotted lines show the one-to-one relationships, and the average differences (ΔA(Li) and ΔT_eff, calculated as our values minus theirs) and one sigma dispersions are indicated in the plots. The stars have been colour-coded according to their effective temperatures.