Radius-mass diagram for the 54 brown dwarfs and low-mass stars presented in Table 4. The five companions presented in this work are highlighted in red. The gray vertical dashed lines display the 13 and 80 M_Jup   approximate boundaries of the brown dwarf regime. The colored lines display isochrone models from Baraffe et al. (2003, 2015) for low mass stars and substellar objects at solar metallicity with ages of 0.1, 0.5, 1, 5, and 10 Gyr. The histogram at the top displays relative occurrence of these transiting objects. We note the brown dwarf RIK 72b is not shown because its radius is 3.1 R_Jup .