Hertzsprung-Russell diagrams of Tr14 stars based on the stellar parameters from IT24 (left panels) and the stellar parameters from this work (right panels). In the upper panels, we plot 2D histograms using all samples, while in the lower panels, we plot contours dividing the samples into the Clean (red) and the Uncertain (blue) groups. We overplot PARSEC theoretical evolutionary tracks (Bressan et al. 2012) where solid lines indicate isochrones from 0.2 to 20 Myr and dashed lines indicate isomasses of 0.3, 0.7, 1, and 3 M_⊙.