Model SEDs for all five objects using the best-fitting parameters from fitting the photometry using MINEsweeper, compared with the observations. J0107−2827 has a visible third companion whose SED is shown in grey. The magenta line is the sum of the two luminous stars (the black line corresponding to the more luminous star lies close to, but under, the magenta line). Note that while GALEX points are plotted, these were not used in the photometric fitting to avoid possible contamination from the WD companions.