Supporting data for “Formation of Our Solar System's Giant Planets via Pebble Accretion"

The data set include simulations output and plots for the thesis titled “Formation of Our Solar System's Giant Planets via Pebble Accretion". It contains initial conditions to reproduce the simulations with SyMBA modified by Matsumura et al. (2017) as well as the binary data output of the simulations. A tool in Fortran is provided to extract orbital elements from the binary output. Plots of the orbital elements are also included in the data set.