Modified H-R diagrams for WASP-113 on the left and WASP-114 on the right. We display the stellar models of YY (Demarque et al. 2004). The isochrones are shown solid black line (for 1,2,3,4,5,6,7,8,9,10 Gyr old stars from left to right) and and the mass tracks in red (from left to right we show 1.3, 1.2, and 1.1 M⊙ ) for the corresponding metallicity given in Table 4.
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