Age_Lite histogram for stars with (right) and without (left) planets. We show the thin disk contribution to the total with a black dotted histogram. The bin width has been obtained by applying the Freeman-Diaconis rule. Vertical lines show the start (dashed), peak (solid), and end (dot-dashed) of MW star formation bursts presented in Ruiz-Lara et al. (2020): in black, the strong star formation burst detected in Mor et al. (2019); in green, the last Sagittarius dwarf galaxy pericentre; and in cyan a very recent star formation burst also detected in the local stellar kinematics (Antoja et al. 2018).