Upper panel: mass and radius of the secondary component as a function of inclination angle, as inferred by the mass function and the M/R relationship for M-dwarfs. Middle panel: model light-curves for a few inclination angles, computed using the radius relationship from the upper panel. I₁ is the model flux of the primary alone, and I is the total model flux from the system. Lower panel: peak-to-peak amplitude of the reflection effect for all inclination angles. ΔI is the difference in model flux at phase 0 and phase 0.5, when ignoring eclipses.