Data associated with publication: Evidence for the late arrival of hot Jupiters in systems with high host-star obliquities

In the associated publication, we homogeneously derive photospheric stellar parameters from photometry and then run stellar models in MESA to derive convective envelope masses. This data archive includes a machine-readable table containing the input and output data for the isochrone analysis as well as the surface convective envelope masses we derived using MESA models. The data archive also includes directories for each star containing the MESA configuration files for each star and the MESA output files for each star.