Overabundance (mass fraction relative to solar; X/X_⊙) of stable isotopes in the ejecta of simulation G14a after decaying for 10¹⁶ s. The two lines correspond to post-processing nucleosynthesis simulations where Nabi & Klapdor-Kleingrothaus (2004, NKK) weak reaction rates were included ("NKK") and when they were not. Including the NKK rates results in a larger yield of ⁴⁸Ca and smaller yields of ⁵⁰Ti and ⁵⁴Cr. The yields of the trans-iron elements from Ga to Nb are substantially increased when the NKK rates are included.