| Element | Nline | [X/H] | [X/Fe] | log-e |
| Li I | ... | <-0.09 | <3.14 | <1.07 |
| CH | ... | -2.56+-0.25 | 0.67+-0.25 | 5.64 |
| CN | ... | <-1.37 | <1.86 | <6.6 |
| O I | ... | <-2.11 | <1.12 | <6.76 |
| Na I | ... | -3.49+-0.2 | -0.26+-0.2 | 2.75 |
| Mg I | ... | -2.76+-0.14 | 0.47+-0.14 | 4.84 |
| Al I | ... | -3.64+-0.29 | -0.41+-0.29 | 2.81 |
| Ca I | ... | -2.85+-0.17 | 0.38+-0.17 | 3.49 |
| Sc II | ... | -3.34+-0.17 | -0.11+-0.17 | -0.44 |
| Ti I | ... | -2.97+-0.15 | 0.26+-0.15 | 1.99 |
| Ti II | ... | -3.18+-0.15 | 0.05+-0.15 | 1.53 |
| V I | ... | -3.16+-0.23 | 0.07+-0.23 | 0.77 |
| V II | ... | <-2.69 | <0.54 | <1.31 |
| Cr I | ... | -3.40+-0.15 | -0.17+-0.15 | 2.24 |
| Mn I | ... | -3.52+-0.15 | -0.29+-0.15 | 1.91 |
| Fe I | ... | -3.23+-0.15 | ... | 4.27 |
| Fe II | ... | -3.48+-0.17 | ... | 4.02 |
| Co I | ... | -3.28+-0.18 | -0.05+-0.18 | 1.71 |
| Ni I | ... | -3.21+-0.18 | 0.02+-0.18 | 3.01 |
| Zn I | ... | <-2.90 | <0.33 | <1.7 |
| Rb I | ... | <-0.35 | <2.88 | <2.25 |
| Sr II | ... | -3.79+-0.16 | -0.56+-0.16 | -1.16 |
| Zr II | ... | <-3.14 | <0.09 | <-0.54 |
| Nb II | ... | <-0.39 | <2.84 | <1.03 |
| Mo I | ... | <-1.64 | <1.59 | <0.28 |
| Tc I | ... | <0.88 | <4.11 | <0.88 |
| Sn I | ... | <-0.20 | <3.03 | <1.8 |
| Ba II | ... | -3.37+-0.15 | -0.14+-0.15 | -1.44 |
| La II | ... | <-2.62 | <0.61 | <-1.45 |
| Ce II | ... | <-2.41 | <0.82 | <-0.83 |
| Pr II | ... | <-2.14 | <1.09 | <-1.43 |
| Nd II | ... | <-2.41 | <0.82 | <-0.91 |
| Sm II | ... | <-1.97 | <1.26 | <-0.96 |
| Eu II | ... | <-2.38 | <0.85 | <-1.87 |
| Gd II | ... | <-1.52 | <1.71 | <-0.4 |
| Tb II | ... | <-1.04 | <2.19 | <-1.14 |
| Dy II | ... | <-2.27 | <0.96 | <-1.13 |
| Ho II | ... | <-1.16 | <2.07 | <-0.9 |
| Er II | ... | <-1.85 | <1.38 | <-0.92 |
| Tm II | ... | <-1.20 | <2.03 | <-1.2 |
| Yb II | ... | -2.64+-0.34 | 0.59+-0.34 | -1.97 |
| Hf II | ... | <-1.14 | <2.09 | <-0.26 |
| Ir I | ... | <-0.65 | <2.58 | <0.7 |
| Pb I | ... | <-0.89 | <2.34 | <1.06 |
| Th II | ... | <-1.22 | <2.01 | <-1.22 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)