Comparison between the measured values of ﹩{T}_{\mathrm{eff}\star }﹩ and ﹩{\rho }_{\star }﹩ (from ZASPE applied to the FEROS spectra, and from our modeling of the light curves and RV data, respectively), and the Y² model isochrones from Yi et al. (2001). The best-fit value (dark blue filled circle), and approximate 1σ and 2σ confidence ellipsoids are shown. The value from our initial ZASPE iteration is shown with an open red triangle. Black solid lines show the Y² isochrones for ages indicated (0.2 to 10.0 Gyr). The green dashed lines show evolutionary tracks for stars with masses indicated in solar mass units.