Notes. The data cover the initial mass M_ini, the model case (single or accretor; in the case of the latter, indication of evolutionary state of the accretor), the fraction f_acc of accreted mass in terms of M_ini, the lifetime t_cc until core collapse, the final mass M_final of the models, the He, CO, and iron core masses M_He, M_CO, and M_Fe, respectively, at core collapse, the compactness ξ_2.5, the radial mass derivative μ₄ and mass M₄ at a specific entropy of s = 4, the central entropy s_c at core collapse, the SN type (BH indicates direct collapse to BH), the gravitational compact-object remnant mass M_rm, the SN ejecta mass M_ej, a flag indicating the likely occurrence of SN fallback, the luminosity log L_cc, effective temperature T_eff, cc, and radius R_* at core collapse, average hydrogen mass fraction ⟨X_env⟩_cc in the hydrogen-rich envelope at core collapse, time $\delta t_{\mathrm{CHeB}}^{\mathrm{BSG}}$ spent as a BSG at log T_eff/K > 3.9 during core-helium burning, and the time δt_LBV spent in the LBV regime in the HR diagram. The full table is only available in electronic form at the CDS, and Zenodo at https://zenodo.org/doi/10.5281/zenodo.10731998.