| Element | Nline | [X/H] | [X/Fe] | log-e |
| Li I | ... | -2.91-0.2 | +-0.2 | 1.96 |
| CH | ... | -2.22+-0.25 | 0.69+-0.25 | 6.3 |
| NH | ... | <-1.17 | <1.74 | <6.8 |
| Na I | ... | -3.04+-0.24 | -0.13+-0.24 | 3.2 |
| Mg I | ... | -2.54+-0.22 | 0.37+-0.22 | 5.06 |
| Al I | ... | -3.61+-0.23 | -0.7+-0.23 | 2.84 |
| Si I | ... | -2.49+-0.36 | 0.42+-0.36 | 5.02 |
| Ca I | ... | -2.41+-0.22 | 0.5+-0.22 | 3.92 |
| Sc II | ... | -2.82+-0.15 | 0.09+-0.15 | 0.43 |
| Ti I | ... | -2.42+-0.22 | 0.49+-0.22 | 2.53 |
| Ti II | ... | -2.63+-0.14 | 0.28+-0.14 | 2.42 |
| V II | ... | <-2.21 | <0.70 | <1.79 |
| Cr I | ... | -3.10+-0.2 | -0.19+-0.2 | 2.54 |
| Mn I | ... | -3.37+-0.21 | -0.46+-0.21 | 2.05 |
| Mn II | ... | -3.36+-0.21 | -0.45+-0.21 | 2.17 |
| Fe I | ... | -2.91+-0.22 | ... | 4.59 |
| Fe II | ... | -2.81+-0.16 | ... | 4.69 |
| Co I | ... | -2.70+-0.25 | 0.21+-0.25 | 2.29 |
| Ni I | ... | -2.95+-0.26 | -0.04+-0.26 | 3.27 |
| Zn I | ... | <-1.17 | <1.74 | <3.43 |
| Sr II | ... | -2.92+-0.2 | -0.01+-0.2 | 0.05 |
| Zr II | ... | <-2.24 | <0.67 | <0.36 |
| Nb II | ... | <0.04 | <2.95 | <1.46 |
| Mo I | ... | <-0.68 | <2.23 | <1.24 |
| Tc I | ... | <1.59 | <4.50 | <1.59 |
| Ba II | ... | -3.56+-0.15 | -0.65+-0.15 | -1.28 |
| Ce II | ... | <-1.59 | <1.32 | <-0.01 |
| Pr II | ... | <-0.93 | <1.98 | <-0.22 |
| Nd II | ... | <-1.66 | <1.25 | <-0.16 |
| Sm II | ... | <-1.05 | <1.86 | <-0.04 |
| Eu II | ... | <-1.76 | <1.15 | <-1.25 |
| Gd II | ... | <-0.76 | <2.15 | <0.36 |
| Tb II | ... | <0.63 | <3.54 | <0.53 |
| Dy II | ... | <-1.38 | <1.53 | <-0.24 |
| Ho II | ... | <-0.77 | <2.14 | <-0.51 |
| Er II | ... | <-1.01 | <1.90 | <-0.08 |
| Tm II | ... | <-0.43 | <2.48 | <-0.43 |
| Yb II | ... | <-2.05 | <0.86 | <-0.97 |
| Hf II | ... | <-0.26 | <2.65 | <0.62 |
| Pb I | ... | <-0.22 | <2.69 | <1.73 |
| Th II | ... | <-0.17 | <2.74 | <-0.17 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)