| Element | Nline | [X/H] | [X/Fe] | log-e |
| Li I | ... | <1.25 | <3.96 | <2.41 |
| CH | ... | <-0.20 | <2.51 | <8.35 |
| CN | ... | <0.28 | <2.99 | <8.25 |
| O I | ... | -3.33+-0.18 | -0.62+-0.18 | 5.36 |
| Mg I | ... | -2.37+-0.17 | 0.34+-0.17 | 5.23 |
| Al I | ... | -3.45+-0.19 | -0.74+-0.19 | 3 |
| Si I | ... | -2.91+-0.23 | -0.2+-0.23 | 4.6 |
| Ca I | ... | -2.92+-0.23 | -0.21+-0.23 | 3.42 |
| Sc II | ... | -2.83+-0.17 | -0.12+-0.17 | 0.34 |
| Ti II | ... | -2.62+-0.17 | 0.09+-0.17 | 2.35 |
| V II | ... | <-2.00 | <0.71 | <2 |
| Cr I | ... | -2.82+-0.17 | -0.11+-0.17 | 2.82 |
| Cr II | ... | -2.34+-0.18 | 0.37+-0.18 | 3.32 |
| Mn I | ... | -2.57+-0.19 | 0.14+-0.19 | 2.86 |
| Fe I | ... | -2.71+-0.17 | ... | 4.79 |
| Fe II | ... | -2.69+-0.18 | ... | 4.81 |
| Ni I | ... | -2.66+-0.24 | 0.05+-0.24 | 3.56 |
| Zn I | ... | <-1.34 | <1.37 | <3.26 |
| Rb I | ... | <0.91 | <3.62 | <3.51 |
| Sr II | ... | -3.28+-0.17 | -0.57+-0.17 | -0.4 |
| Y II | ... | <-2.51 | <0.20 | <-0.27 |
| Zr II | ... | <-1.86 | <0.85 | <0.74 |
| Nb II | ... | <0.40 | <3.11 | <1.82 |
| Mo I | ... | <0.47 | <3.18 | <2.39 |
| Tc I | ... | <2.72 | <5.43 | <2.72 |
| Ba II | ... | <-3.20 | <-0.49 | <-1.07 |
| La II | ... | <-1.20 | <1.51 | <-0.03 |
| Ce II | ... | <-1.08 | <1.63 | <0.5 |
| Pr II | ... | <-0.41 | <2.30 | <0.3 |
| Nd II | ... | <-1.01 | <1.70 | <0.49 |
| Sm II | ... | <-0.51 | <2.20 | <0.5 |
| Eu II | ... | <-1.18 | <1.53 | <-0.67 |
| Gd II | ... | <-0.50 | <2.21 | <0.62 |
| Tb II | ... | <0.27 | <2.98 | <0.17 |
| Dy II | ... | <-0.93 | <1.78 | <0.21 |
| Ho II | ... | <-0.32 | <2.39 | <-0.06 |
| Er II | ... | <-0.40 | <2.31 | <0.53 |
| Tm II | ... | <-0.11 | <2.60 | <-0.11 |
| Yb II | ... | <-1.75 | <0.96 | <-0.67 |
| Hf II | ... | <0.13 | <2.84 | <1.01 |
| Pb I | ... | <0.76 | <3.47 | <2.71 |
| Th II | ... | <0.22 | <2.93 | <0.22 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)