| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| C | ... | 0.20+-0.18 | 2.25+-0.18 | 8.77 |
| Mg | ... | -1.55+-0.19 | 0.50+-0.19 | 6.08 |
| Sc | ... | -1.55+-0.16 | 0.50+-0.16 | 1.67 |
| Ti | ... | -1.31+-0.14 | 0.74+-0.14 | 3.76 |
| Cr | ... | -1.65+-0.13 | 0.40+-0.13 | 4.07 |
| Fe I | ... | -2.05 | ... | 5.45 |
| Fe II | ... | -2.00 | ... | 5.50 |
| Zn | ... | -1.47+-0.3 | 0.58+-0.30 | 3.18 |
| Sr II | ... | -2.11+-0.16 | -0.06+-0.16 | 0.91 |
| Y | ... | -2.17+-0.13 | -0.12+-0.13 | 0.12 |
| Zr | ... | -2.07+-0.3 | -0.02+-0.30 | 0.58 |
| Ba | ... | -1.30+-0.13 | 0.75+-0.13 | 0.88 |
| La | ... | -1.47+-0.21 | 0.58+-0.21 | -0.29 |
| Ce | ... | -1.45+-0.16 | 0.60+-0.16 | 0.30 |
| Nd | ... | -1.45+-0.12 | 0.60+-0.12 | 0.05 |
| Eu | ... | -2.06+-0.2 | -0.01+-0.20 | -1.49 |
| Gd | ... | -2.05+-0.21 | 0.00+-0.21 | -0.88 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
