| Element | Nline | [X/H] | [X/Fe] | log-e |
| Li | ... | <1.14 | <3.19 | <2.3 |
| C | ... | -0.05+-0.32 | 2.00+-0.32 | 8.34+-0.32 |
| Na I | ... | -1.72+-0.28 | 0.33+-0.28 | 4.45+-0.28 |
| Mg I | ... | -1.78+-0.18 | 0.27+-0.18 | 5.75+-0.18 |
| Ca I | ... | -1.73+-0.13 | 0.32+-0.13 | 4.59+-0.13 |
| Ti II | ... | -1.61+-0.15 | 0.44+-0.15 | 3.29+-0.15 |
| Cr I | ... | -2.15+-0.15 | -0.10+-0.15 | 3.49+-0.15 |
| Fe I | ... | -2.05+-0.15 | ... | 5.40+-0.15 |
| Fe II | ... | -2.05+-0.13 | ... | 5.40+-0.13 |
| Ni I | ... | -1.97+-0.15 | 0.08+-0.15 | 4.26+-0.15 |
| Sr II | ... | -1.37+-0.29 | 0.68+-0.29 | 1.56+-0.29 |
| Y II | ... | -1.26 | 0.79 | 0.95 |
| Zr II | ... | -1.09 | 0.96 | 1.5 |
| Ba II | ... | -0.55+-0.24 | 1.50+-0.24 | 1.62+-0.24 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)