Notes. Remnant properties are inferred from the values of the ¹²C mass fraction and the CO core mass, both evaluated at the end of core O-burning (or at the end of core C-burning if O-burning is not finished), following the prescription of Patton & Sukhbold (2020). Initial mass (Col. 1), rates reference where K02 and DB17 refer to Kunz et al. (2002) and deBoer et al. (2017), respectively (Col. 2), ¹²C mass fraction (Col. 3), CO core mass (Col. 4), remnant type where NS and BH refer to neutron star and black hole, respectively (Col. 5), remnant mass (Col. 6), M₄ to CO core mass ratio (Col. 7, models marked with ^* have a CO core mass outside the Patton & Sukhbold (2020) grid, whose minimum of 2.5 M_⊙, predictions for these cases rely on a small extrapolation and final mass (Col. 8). We note that M₄ is only computed at the end of O-burning, but using the results of Griffiths et al. (2025) we checked that this value is at most 5% off from the value at pre-SN. We expect this to hold true here also.