| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| Mg I | ... | -2.33+-0.16 | 0.53+-0.16 | 5.25+-0.16 |
| Al I | ... | -2.83+-0.07 | 0.03+-0.07 | 3.64+-0.07 |
| Si I | ... | -2.85 | 0.01 | 4.70 |
| Ca I | ... | -2.84+-0.17 | 0.02+-0.17 | 3.52+-0.17 |
| Sc II | ... | -2.47+-0.07 | 0.39+-0.07 | 0.70+-0.07 |
| Ti I | ... | <-2.26+-0.18 | <0.6+-0.18 | <2.76+-0.18 |
| Ti II | ... | -2.63+-0.12 | 0.23+-0.12 | 2.39+-0.12 |
| Cr I | ... | -3.21+-0.11 | -0.35+-0.11 | 2.46+-0.11 |
| Mn I | ... | -3.59+-0.02 | -0.73+-0.02 | 1.80+-0.02 |
| Fe I | ... | -2.86+-0.13 | ... | 4.64+-0.13 |
| Fe II | ... | ... | 0.08+-0.19 | ... |
| Co I | ... | -2.26+-0.17 | 0.6+-0.17 | 2.66+-0.17 |
| Ni I | ... | -2.96 | -0.1 | 3.29 |
| Sr II | ... | -4.45 | -1.59 | -1.48 |
| Ba II | ... | <-3.68 | <-0.82 | <-1.55 |
| Eu II | ... | <-1.38 | <1.48 | <-0.87 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
