Notes. From left to right, the name of the simulation and of the NR-extracted initial ejecta profile (see Table 1), the NSE initialization method employed (BK6 and BK8 stand for the backtracking procedure starting at T = 6, 8 GK, CNSE for the cold-NSE method; Apr2 simulations are performed without in situ NN), the thermalization scheme used (DT08 and ST05 stand for the detailed thermalization scheme described in Sect. 2.4 with $f_{\mathrm{th}}^{\mathrm{oth}}=0.8$ or the simple thermalization from Wu et al. (2022) with $f_{\mathrm{th}}^{\mathtt{kNEC}}=0.5$). The next columns state wether a frequency-dependent (and with how many frequency groups) or a gray opacity is used, which model is employed (LANL stands for the atomic calculations, J[22] for the analytical model from Just et al. (2022), and W[22] for the opacity from Wu et al. 2022), and which atomic opacities are read from the NIST-LANL database (see Sect. 2.5). The last three columns report the peak of the bolometric luminosity, the time of this peak, and the final mass fraction of lanthanides produced.