MESA inlist files for PPISN models in the publication "Rotational Dynamics in Pulsational Pair-Instability Supernovae: Implications for Mass-Loss and Transient Events" submittted to the ApJ

MESA inlist files used in the publication "Rotational Dynamics in Pulsational Pair-Instability Supernovae: Implications for Mass-Loss and Transient Events" are included. We used the version r24.03.1 of MESA and MESASDK version 24.7.1 to generate the PPISN models. The run_star_extras file that are included with the MESA distribution test_suite ppisn were used without any further modifications.