Stellar evolution track based on Baraffe et al. (2015) model of the three stars in the system. Panels a and b display the bolometric luminosity and the XUV quiescent luminosity. The observed bolometric luminosity and XUV luminosity were used to determine the A component. Panels c and d display the XUV luminosity from flares and the total XUV luminosity overlaid by the gray dashed line indicating the average observed X-ray flux + estimated EUV flux in d. The ratio of XUV luminosity from flares to bolometric luminosity is displayed in panel e, and the ratio of XUV luminosity from flares to XUV quiescent luminosity is displayed in panel f.