Hertzsprung-Russell diagrams (left) and Kiel diagrams (right) based on parameters obtained by cINN in this work using all 2051 Tr14 samples (upper panels) and using only 177 stars with surface gravities higher than 4.5 considering 3-σ estimation uncertainty. The colour in the HR diagrams indicates log g estimates while the colour in the log g – T_eff diagrams represents stellar age derived from bolometric luminosity and T_eff using PARSEC evolutionary tracks (Bressan et al. 2012). We overplot PARSEC theoretical evolutionary tracks (Bressan et al. 2012) where solid lines indicate isochrones from 0.2 to 100 Myr and dashed lines indicate isomasses of 0.3, 0.7, 1, and 3 M_⊙.