Li abundances vs. T_eff for the microlensed dwarf sample. The stars are colour coded based on the effective temperatures of the stars. Triangles represent those stars for which we can only determine upper limits on the abundances. The grey plus signs in the background represent the 714 stars from Bensby et al. (2014) for which Li abundances were determined in Bensby & Lind (2018) in the exact same way as for the microlensed bulge dwarfs. The dotted lines show the solar values with the solar photospheric Li abundance taken from Asplund et al. (2009).