| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| Mg I | ... | -2.40+-0.1 | 0.05+-0.1 | 5.18+-0.1 |
| Al I | ... | -2.06+-0.1 | 0.39+-0.1 | 4.41+-0.1 |
| Si I | ... | -2.09 | 0.36 | 5.46 |
| Ca I | ... | -2.19+-0.06 | 0.26+-0.06 | 4.17+-0.06 |
| Sc II | ... | -2.40+-0.15 | 0.05+-0.15 | 0.77+-0.15 |
| Ti II | ... | -2.16+-0.11 | 0.29+-0.11 | 2.86+-0.11 |
| Cr I | ... | -2.77+-0.03 | -0.32+-0.03 | 2.90+-0.03 |
| Mn I | ... | -3.10+-0.07 | -0.65+-0.07 | 2.29+-0.07 |
| Fe I | ... | -2.45+-0.14 | ... | 5.05+-0.14 |
| Fe II | ... | -2.44+-0.16 | 0.01+-0.16 | 5.06+-0.16 |
| Co I | ... | -2.58 | -0.13 | 2.34 |
| Ni I | ... | -2.37 | 0.08 | 3.88 |
| Sr II | ... | -2.62+-0.04 | -0.17+-0.04 | 0.35+-0.04 |
| Ba II | ... | -2.82 | -0.37 | -0.69 |
| Eu II | ... | <-1.23 | <1.22 | <-0.72 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
