Left: $\mathrm{\Xi_c^0}$/$\mathrm{D^0}$ ratio as a function of $p_{\rm T}$ in p-Pb collisions at $\sqrt{s_\mathrm{NN}}=5.02$ TeV and in pp collisions at $\sqrt{s}=5.02$ TeV compared to QCM, POWHEG + PYTHIA 6, and PYTHIA 8 Angantyr predictions. Right: $\mathrm{\Xi_c^0}$/$\mathrm{\Lambda_c^+}$ ratio as a function of $p_{\rm T}$ in p-Pb collisions at $\sqrt{s_\mathrm{NN}}=5.02$ TeV and in pp collisions at $\sqrt{s}=13$ TeV compared to QCM, POWHEG + PYTHIA 6, and PYTHIA 8 Angantyr calculations. The BR uncertainties for the $\mathrm{\Lambda_c^+}$ are evaluated as the weighted average on the two decay channels and are included in the systematic uncertainty box for each $p_{\rm T}$ bin.