Fig. 8
Comparison of Ag and Pd abundances of common stars in this study with those in Hansen et al. (2012). The dashed lines represent 1:1 ratios, and solid lines represent the linear least-square fitting functions y = (1.09 ± 0.09)x + (0.11 ± 0.10) for [Pd/H], and y = (1.01 ± 0.15)x + (−0.05 ± 0.14) for [Ag/H], where x denotes our abundances and y denotes those of Hansen et al. (2012).
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