Absolute logϵ (X) abundances for the three CEMP-r/s stars in our sample compared to scaled i-process yields from Choplin et al. (2022) and the scaled Solar r- and s-process patterns from Sneden et al. (2008). The bottom panel in each plot shows the residual for the match to the i-process yields. The Solar s- and r-process patterns are scaled to the stellar Ba and Eu abundances, respectively, while the average difference between yields and stellar abundances from Ba to Dy was used to scale the i-process yields.