Photoevaporation vs. Core-Powered Mass-Loss: Posterior Distributions

Here we provide the Monte Carlo chains to accompany the associated paper 'Photoevaporation vs. core-powered mass-loss: model comparison with the 3D radius gap'. Two .zip files are included for the two models presented in this work. Files within are formatted in the following manner:

xNp_smass0.5-1.5-y.csv

where x is the number of detected planets for the synthetic survey and y is the standard deviation in underlying stellar mass distribution. Each file contains an array with measured values of \(\alpha\) and \(\beta\).