Time and (sub)stellar mass dependencies on the luminosity of the host based on the evolutionary model of Baraffe et al. (2003, 2015). The solid lines from thick to thin indicate the systems’ ages from 1 Myr to 10 Myr, 100 Myr, and 1 Gyr. Thegreen dashed lines correspond to a linear, quadratic, cubic, and fourth power correlation between the luminosity and mass. We find that when the central host is younger than 10 Myr, , while when hosts are generally older than 10 Myr.