Notes. We show the results from both single massive stars and binary-stripped stars. The values for binary-stripped stars are weighted by a log-flat initial orbital period distribution. Given that our binary grid is equally spaced in log₁₀P_ini, we directly take the mean value of the binary grid results as the weighted value for binary-stripped stars. The ¹²C yields are broken down by mass-loss type. The CO core mass is measured at central helium depletion. The supernova ¹²C yield is reported assuming all stars explode. The total ¹²C yield is reported assuming the explodability criterion from Maltsev et al. (2025), where we mark the models that directly collapse as x in the last column. When the values for ¹²C M_SN and ¹²C M_Total are all missing, it means the model did not reach core collapse due to numerical difficulties. This is only shown for the single stars, because the values for binary-stripped stars are not for individual model. When only the value in the column ¹²C M_Total is missing, it means the model experiences anomalous helium burning due to helium-carbon shell mergers.