Trajectories used in Phys. Rev. C 101, 055807 (2020)
Representative trajectories for the nuclear physics uncertainties study on neutrino-driven supernova ejecta. The steady-state trajectories are calculated in Bliss et al., ApJ 855, 135 (2018). If you use these data please cite Bliss et al., Phys. Rev. C 101, 055807 (2020) and Bliss et al., ApJ 855, 135 (2018).