Simulation data for "DUETS: Setting expectations for asteroseismic binaries and binary products with synthetic populations"

The paper presents results from three simulations that adopt different prescriptions for the initial orbital parameters of the binaries, namely: E06 - Eggleton (2006) MDS17 - Moe & Di Stefano (2017) no-interact - non-interacting binaries, orbital parameters not simulated Two files are included for each simulation: *_singles.csv contains the simulation data for single stars, while *_binaries.csv contains the simulated data for binary stars.