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Caption: Fig. 12.
Comparison of computed fractional radius ﹩\left[R( S) -R_{0}\right]/ R_{0}﹩ (solid line) to fitting formula ﹩R( S) =R_{0}+\delta R_{S}e^{\eta m_{p}S/ k_{\mathrm{B}\,}}﹩ (dashed line) for a ﹩M=1M_{\mathrm{J}\,}﹩ planet with ﹩T_{\mathrm{deep}\,}=1000﹩ K.
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