Differences between NLTE abundances from individual lines computed with F_odd = 0.10 (s-process) and 0.75 (r-process) in the sample stars known in the literature as CEMP-s (circles) and CEMP-rs (squares), and in stars with an unclear classification (triangles). For comparison, we show data for normal VMP stars from Sitnova et al. (2025, diamonds). The open and filled symbols correspond to the Ba II 4554 Å and 4934 Å lines, respectively.