| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| Li I | ... | -1.80-0.2 | +-0.2 | 2.1 |
| CH | ... | -1.88+-0.25 | -0.08+-0.25 | 6.57 |
| CN | ... | <-0.67 | <1.13 | <7.3 |
| O I | ... | -1.65+-0.2 | 0.15+-0.2 | 7.03 |
| Mg I | ... | -1.53+-0.24 | 0.27+-0.24 | 6.07 |
| Al I | ... | -2.84+-0.33 | -1.04+-0.33 | 3.61 |
| Ca I | ... | -1.44+-0.24 | 0.36+-0.24 | 4.9 |
| Sc II | ... | -1.87+-0.14 | -0.07+-0.14 | 1.3 |
| Ti I | ... | -1.61+-0.2 | 0.19+-0.2 | 3.34 |
| Ti II | ... | -1.52+-0.14 | 0.28+-0.14 | 3.44 |
| V II | ... | -1.68+-0.23 | 0.12+-0.23 | 2.27 |
| Cr I | ... | -1.90+-0.2 | -0.1+-0.2 | 3.74 |
| Cr II | ... | -1.53+-0.14 | 0.27+-0.14 | 4.13 |
| Mn I | ... | -2.24+-0.21 | -0.44+-0.21 | 3.18 |
| Fe I | ... | -1.8+-0.2 | ... | 5.7 |
| Fe II | ... | -1.78+-0.14 | ... | 5.72 |
| Co I | ... | -2.00+-0.23 | -0.2+-0.23 | 2.99 |
| Ni I | ... | -1.79+-0.23 | 0.01+-0.23 | 4.43 |
| Zn I | ... | -1.79+-0.2 | 0.01+-0.2 | 2.77 |
| Rb I | ... | <-0.10 | <1.70 | <2.5 |
| Sr II | ... | -1.85+-0.22 | -0.05+-0.22 | 1.03 |
| Y II | ... | -2.28+-0.16 | -0.48+-0.16 | -0.05 |
| Zr II | ... | -1.61+-0.15 | 0.19+-0.15 | 0.99 |
| Nb II | ... | <0.12 | <1.92 | <1.54 |
| Mo I | ... | <-0.75 | <1.05 | <1.17 |
| Tc I | ... | <1.23 | <3.03 | <1.23 |
| Ba II | ... | -1.96+-0.14 | -0.16+-0.14 | 0.24 |
| La II | ... | -1.53+-0.19 | 0.27+-0.19 | -0.41 |
| Ce II | ... | -1.47+-0.3 | 0.33+-0.3 | 0.13 |
| Pr II | ... | <-0.82 | <0.98 | <-0.11 |
| Nd II | ... | -1.67+-0.17 | 0.13+-0.17 | -0.23 |
| Eu II | ... | -1.44+-0.15 | 0.36+-0.15 | -0.9 |
| Gd II | ... | <-0.88 | <0.92 | <0.24 |
| Tb II | ... | <-0.18 | <1.62 | <-0.28 |
| Tm II | ... | <-0.63 | <1.17 | <-0.63 |
| Yb II | ... | -1.76+-0.24 | 0.04+-0.24 | -0.82 |
| Hf II | ... | <-0.42 | <1.38 | <0.46 |
| Ir I | ... | <0.17 | <1.97 | <1.52 |
| Pb I | ... | <-0.55 | <1.25 | <1.4 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
