“…Results have been reported for stable and radioactive samples, i.e., 24,25,26 Mg, 54,57 Fe, 58,59,62,63 Ni, 70,72,73 Ge, 90,91,92,93,94,96 Zr, 139 La, 140 Ce, 147 Pm, 151 Sm, 154,155,157 Gd, 171 Tm, 186,187,188 Os, 197 Au, 203,204 Tl, 204,206,207 Pb and 209 Bi isotopes (see [8] for more details), and others are being studied or planned to be studied in the near future. In some cases, these results were then used to improve Evaluated Nuclear Data File such as ENDF/B-VIII.0 [9], JENDL-5.0 [10] and JEFF-3.3 [11] or TENDL-2021 [12] and other international projects. The same data were used to derive the neutron-induced cross section averaged over the stellar neutron-energy distribution, typically referred to as Maxwellian averaged cross section (MACS) -more details in Sec.…”