Mean A(Li) computed in 0.1 dex bins vs. mean Age_Param in 0.6 Gyr bins, for stars without known planets (N, left) and those that host confirmed planets (Y, right). Vertical lines show the last star formation burst in Ruiz-Lara et al. (2020) (line colours and styles as in Fig. 6). Colour bars show the logarithm of the number of stars per A(Li)-age bin, normalised to unity. Equivalent plots with only thin- and/or thick-disk stars only are available upon request to the authors.