HD 221170 abundance comparisons of the heavy n‐capture elements to the predicted scaled solar r‐process pattern of Simmerer et al. (2004). Top: Difference in the abundances reported by Yushchenko et al. (2005). Bottom: Differences derived in this study. The derived abundances have been normalized to the value derived for ﹩\mathrm{log}\,\epsilon ( \mathrm{Eu}\,) ﹩ in the corresponding study. The error bars displayed are those of the ﹩1-\sigma _{\mathrm{adopted}\,}﹩ values.