The abundance patterns of the three CEMP-rs stars are compared with nucleosynthesis predictions from the STAREVOL code. The measured abundances are indicated by red circles. Upper limits are indicated with downward arrows. In all cases, the best-fitting theoretical predictions for both the i-process (black) and s-process (blue) are displayed. The gray shaded area corresponds to the typical i-process nuclear parameter uncertainties computed in S. Martinet et al. (2024) and based on a 1 M_⊙, [Fe/H] = − 2.5 model.