Models for paper: Pulsational pair-instability supernovae in very close binaries

Models of pulsational pair-instability supernovae arising from the evolution of metal poor helium stars. These simulations have been made using the MESA code for stellar evolution, and are used in the paper "Pulsational pair-instability supernovae in very close binaries" (to be submitted). Data includes both history and profile files from the simulations, as well as the terminal output and a movie for each.