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Electron capture (EC) decay relies on attachment and strippingcross-sections, that in turn, depend on the atomic number of the nucleus. Werevisit the impact of EC decay in the context of the high-precision cosmic-rayfluxes measured by the AMS-02 experiment. We derive the solution of thesteady-state fluxes in a 1D thin disk model including EC decay. We compare ourresults with relevant elemental and isotopic fluxes and evaluate the impact ofthis process, given the precision of recent AMS-02, ACE-CRIS, SuperTIGER, andVoyager data. We find this impact to be at the level or larger than theprecision of recently collected data for several species, e.g. $_{31}$Ga and$_{33}$As, indicating that EC decay must be properly taken into account in thecalculation.

The role of electron capture decay in the precision era of Galactic cosmic-ray data