Distribution of all stellar ages from the final catalogue. The black histogram filled with grey shows ages estimated based on evolutionary tracks from Baraffe et al. (2015) and Siess et al. (2000), while the open blue histogram shows stellar ages based on PARSEC models (Bressan et al. 2012). PARSEC models span ages down to 0.1 Myr, while the other two go to 0.5 Myr. Both histograms have the same bins fixed to the distribution of PARSEC ages.