The input files for "The long-term accretion luminosity of V4641 Sgr through binary evolution simulations: implications for its ultrahigh-energy gamma-ray emission"

Simulations were made using the version 10398 of the MESA code together with the -x86_64-linux-20180822 MESA SDK. "BHXB.zip" provides the MESA inlist files to reproduce our simulations. File inlist1 includes the settings of the donor star. File inlist_project includes the input initial orbital parameters and settings of binary evolution. BH_4Msun.zip and BH_5Msun.zip include the simulation data of black hole X-ray binary containing an incipient 4Msun and 5Msun neutron star, respectively.