Table 3.
Results of the Wilcoxon rank-sum test: probability of rejecting, while it would be true, the null hypothesis that the two groups of measured abundances of element X for CEMP-rs and CEMP-s stars are drawn from the same distribution, and the same for the [hs/ls] value, where ls and hs are defined as in Fig. 14.
| Element | Y | Zr | Ba | La | Ce | Pr | Nd | Sm | Eu | Gd | Dy | [hs/ls] |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Probability (%) | 11.7 | 14.2 | 13.0 | 9.7 | 11.7 | 3.2 | 4.9 | 21.8 | 0.2 | 0.2 | 2.5 | 2.6 |
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