Simulation Data for A Non-Primordial Origin for the Widest Binaries in the Kuiper Belt

This is the raw simulation data for Campbell, Anderson, & Kaib (2024). These simulations were run with a modified version of the SWIFT RMVS4 integrator and have output format identical to standard versions of this code. Each tared file is a folder of binary bin.dat files directly output by the simulation. Each binary file encodes the orbital properties of 10 binaries over the lifetime of the simulation. They are binary files with identical headers and formats of typical SWIFT RMVS4 output files.