Comparison of the best fit (violet stars) and Pattern 2 (red stars) with data (black symbols; I. U. Roederer et al. 2022b) on ﹩\mathrm{log}({\rm{E}}/{\rm{Eu}})﹩ for HD 222925. The best fit corresponds to a mixing parameter x_Eu = 3.2 × 10⁻², and its difference from Pattern 2 shows that contributions from Pattern 1 are mostly limited to the light r-process elements, Te, and Pt.