Mass-radius relationships for irradiated ocean planets

The aim of this study was to produce mass-radius relationships for irradiated (Tirr = 400 - 1000 K) ocean (10% to 100% of H2O by mass) planets (of masses 0.2 to 20 M🜨) by combining an interior model with an atmosphere model.
Data produced by our model can be download here : Data.
All MR relationships were fitted by a function, and the coefficients obtained by fit can be downloaded here : Fit coefficients.