| Element | Nline | [X/H] | [X/Fe] | log-e |
| Li I | ... | <-0.54 | <2.06 | <0.62 |
| CH | ... | -2.93+-0.25 | -0.33+-0.25 | 5.62 |
| CN | ... | -1.75+-0.28 | 0.85+-0.28 | 6.2 |
| O I | ... | <-2.05 | <0.55 | <6.82 |
| Mg I | ... | -2.40+-0.16 | 0.2+-0.16 | 5.2 |
| Al I | ... | -3.41+-0.3 | -0.81+-0.3 | 3.04 |
| Ca I | ... | -2.44+-0.17 | 0.16+-0.17 | 3.9 |
| Sc II | ... | -3.04+-0.15 | -0.44+-0.15 | 0.22 |
| Ti I | ... | -2.50+-0.14 | 0.1+-0.14 | 2.44 |
| Ti II | ... | -2.47+-0.15 | 0.13+-0.15 | 2.59 |
| V I | ... | -2.81+-0.17 | -0.21+-0.17 | 1.12 |
| V II | ... | -2.81+-0.24 | -0.21+-0.24 | 1.23 |
| Cr I | ... | -2.70+-0.14 | -0.1+-0.14 | 2.94 |
| Cr II | ... | -2.36+-0.15 | 0.24+-0.15 | 3.39 |
| Mn I | ... | -2.65+-0.14 | -0.05+-0.14 | 2.77 |
| Mn II | ... | -2.62+-0.21 | -0.02+-0.21 | 2.92 |
| Fe I | ... | -2.6+-0.15 | ... | 4.9 |
| Fe II | ... | -2.49+-0.15 | ... | 5.01 |
| Co I | ... | -2.89+-0.22 | -0.29+-0.22 | 2.09 |
| Ni I | ... | -2.39+-0.18 | 0.21+-0.18 | 3.83 |
| Cu I | ... | <-3.06 | <-0.46 | <1.15 |
| Zn I | ... | -2.14+-0.14 | 0.46+-0.14 | 2.42 |
| Rb I | ... | <-0.53 | <2.07 | <2.07 |
| Sr II | ... | -2.84+-0.25 | -0.24+-0.25 | 0.14 |
| Y II | ... | -3.41+-0.17 | -0.81+-0.17 | -1.09 |
| Zr II | ... | -2.89+-0.16 | -0.29+-0.16 | -0.2 |
| Nb II | ... | <-0.78 | <1.82 | <0.64 |
| Mo I | ... | <-1.76 | <0.84 | <0.16 |
| Tc I | ... | <0.30 | <2.90 | <0.3 |
| Sn I | ... | <-0.56 | <2.04 | <1.44 |
| Ba II | ... | -3.72+-0.15 | -1.12+-0.15 | -1.43 |
| La II | ... | -3.05+-0.21 | -0.45+-0.21 | -1.84 |
| Ce II | ... | <-2.81 | <-0.21 | <-1.23 |
| Pr II | ... | <-2.11 | <0.49 | <-1.4 |
| Nd II | ... | <-3.20 | <-0.60 | <-1.7 |
| Sm II | ... | <-2.23 | <0.37 | <-1.22 |
| Eu II | ... | <-2.73 | <-0.13 | <-2.22 |
| Gd II | ... | <-1.92 | <0.68 | <-0.8 |
| Tb II | ... | <-0.87 | <1.73 | <-0.97 |
| Dy II | ... | <-1.87 | <0.73 | <-0.73 |
| Tm II | ... | <-1.56 | <1.04 | <-1.56 |
| Yb II | ... | <-2.76 | <-0.16 | <-1.68 |
| Hf II | ... | <-1.55 | <1.05 | <-0.67 |
| Pb I | ... | <-1.50 | <1.10 | <0.45 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)