Theoretically calculated fluxes of Galactic cosmic ray protons, helium, boron, carbon, oxygen as supporting data for preprint arXiv:2511.06733

This dataset includes theoretical fluxes of Galactic cosmic rays presented in figures 2 - 5 of preprint arXiv:2511.06733. They are obtained with the cosmic ray propagation code GALPROP (https://galprop.stanford.edu/). Specifically:figure 2: boron, carbon, and oxygen fluxes before and after the solar modulationfigure 3: proton (a) and helium (b) fluxes from the background sources and a nearby sourcefigure 4: proton (a) and helium (b) fluxes from the background sources and two nearby sourcefigure 5: proton (a) and helium (b) fluxes from two background sources and a nearby sourceThe detailed column information can be found in the data files.