| Element | Nline | [X/H] | [X/Fe] | log-e |
| CH | ... | -3.03 | 0.35 | 5.52 |
| Na I | ... | -3.71+-0.01 | -0.33+-0.01 | 2.62+-0.01 |
| Mg I | ... | -3.37+-0.08 | 0.01+-0.08 | 4.21+-0.08 |
| Al I | ... | -3.88 | -0.5 | 2.59 |
| Si I | ... | -3.33 | 0.05 | 4.22 |
| Ca I | ... | -3.57+-0.13 | -0.19+-0.13 | 2.79+-0.13 |
| Sc II | ... | -3.39+-0.03 | -0.01+-0.03 | -0.22+-0.03 |
| Ti II | ... | -3.35+-0.07 | 0.03+-0.07 | 1.67+-0.07 |
| Cr I | ... | -3.90+-0.11 | -0.52+-0.11 | 1.77+-0.11 |
| Mn I | ... | -4.00+-0.02 | -0.62+-0.02 | 1.39+-0.02 |
| Fe I | ... | -3.38+-0.16 | ... | 4.12+-0.16 |
| Fe II | ... | -3.32+-0.08 | 0.06+-0.08 | 4.18+-0.08 |
| Co I | ... | -2.97 | 0.41 | 1.95 |
| Ni I | ... | -2.89 | 0.49 | 3.36 |
| Sr II | ... | -4.40+-0.04 | -1.02+-0.04 | -1.43+-0.04 |
| Ba II | ... | <-4.70 | <-1.32 | <-2.57 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)