| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| Li I | ... | -2.29-0.13 | +-0.13 | 1.25 |
| CH | ... | -2.57+-0.25 | -0.28+-0.25 | 5.85 |
| Mg I | ... | -2.16+-0.17 | 0.13+-0.17 | 5.43 |
| Ca I | ... | -1.97+-0.16 | 0.32+-0.16 | 4.37 |
| Sc II | ... | -2.22+-0.28 | 0.07+-0.28 | 0.92 |
| Ti I | ... | -2.08+-0.1 | 0.21+-0.1 | 2.86 |
| Ti II | ... | -1.98+-0.2 | 0.31+-0.2 | 2.97 |
| V I | ... | -2.43+-0.16 | -0.14+-0.16 | 1.5 |
| Cr I | ... | -2.37+-0.1 | -0.08+-0.1 | 3.26 |
| Mn I | ... | -3.01+-0.24 | -0.72+-0.24 | 2.41 |
| Fe I | ... | -2.29+-0.11 | ... | 5.21 |
| Fe II | ... | -2.3+-0.24 | ... | 5.2 |
| Co I | ... | -2.37+-0.23 | -0.08+-0.23 | 2.62 |
| Ni I | ... | -2.33+-0.18 | -0.04+-0.18 | 3.89 |
| Cu I | ... | <-2.53 | <-0.24 | <1.68 |
| Zn I | ... | -2.13+-0.15 | 0.16+-0.15 | 2.42 |
| Sr II | ... | -2.26+-0.14 | 0.03+-0.14 | 0.61 |
| Zr II | ... | <-1.59 | <0.70 | <1.01 |
| Tc I | ... | <1.48 | <3.77 | <1.48 |
| Ba II | ... | -2.64+-0.19 | -0.35+-0.19 | -0.47 |
| Ce II | ... | <-1.16 | <1.13 | <0.42 |
| Pr II | ... | <-0.80 | <1.49 | <-0.09 |
| Nd II | ... | <-0.90 | <1.39 | <0.6 |
| Sm II | ... | <-0.79 | <1.50 | <0.22 |
| Eu II | ... | <-1.03 | <1.26 | <-0.52 |
| Gd II | ... | <-0.62 | <1.67 | <0.5 |
| Tb II | ... | <0.72 | <3.01 | <0.62 |
| Dy II | ... | <-0.17 | <2.12 | <0.97 |
| Tm II | ... | <1.00 | <3.29 | <1 |
| Hf II | ... | <0.22 | <2.51 | <1.1 |
| Pb I | ... | <0.25 | <2.54 | <2.2 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
