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High-precision cosmic-ray data from ongoing and recent past experiments(Voyager, ACE-CRIS, PAMELA, ATIC, CREAM, NUCLEON, AMS-02, CALET, DAMPE) arebeing released in the tens of MeV/n to multi-TeV/n energy range. Astrophysicaland dark matter interpretations of these data are limited by the precision ofnuclear production cross-sections. In Paper I, PRC 98, 034611 (2018), we set upa procedure to rank nuclear reactions whose desired measurements will enable usto fully exploit currently available data on CR Li to N ($Z=3-7$) species. Herewe extend these rankings to O up to Si nuclei ($Z=8-14$), also updating ourresults on the LiBeB species. We also highlight how comprehensive new highprecision nuclear data, that could e.g. be obtained at the SPS at CERN, wouldbe a game-changer for the determination of key astrophysical quantities(diffusion coefficient, halo size of the Galaxy) and indirect searches for darkmatter signatures.

Current status and desired accuracy of the isotopic production  cross-sections relevant to astrophysics of cosmic rays II. Fluorine to  Silicon (and updated LiBeB)