Baraffe et al. (2015) stellar evolutionary models with isochrones ranging from 0.5 Myr to 500 Myr plotted with z′ and K absolute magnitudes. The observed data of J1036 is depicted by the blue diamond and triangles for the A, B, and C components, where we have used the 20.1 pc distance from Shkolnik et al. (2012). Similar to Fig. 5, the models do not agree with the individual dynamical mass of 0.24 M_⊙ for the B and C components. The models also suggest a very young age unless the distance to the system has been overestimated.