NLTE Li abundance as a function of [α/Fe] in each log(g) bin for our sample stars with Li measurements. The range of log(g) is specified in each plot, with bin size of 0.235 dex. We label the mean correlation coefficient (R₀ (P)) between A_Li and [α/Fe], the mean correlation significance level (P₀), the possibility of Li-[α/Fe] anticorrelation (β < 0) if consider the abundance uncertainties, and the possibility of P < 0.05 for the anticorrelation.