| Element | Nline | [X/H] | [X/Fe] | log-e |
| Li I | ... | -3.47-0.2 | +-0.2 | 1.47 |
| CH | ... | <-3.05 | <0.42 | <5.5 |
| NH | ... | <-2.02 | <1.45 | <5.95 |
| O I | ... | <-2.27 | <1.20 | <6.6 |
| Na I | ... | -3.67+-0.22 | -0.2+-0.22 | 2.57 |
| Mg I | ... | -2.97+-0.23 | 0.5+-0.23 | 4.64 |
| Al I | ... | -4.26+-0.22 | -0.79+-0.22 | 2.19 |
| Si I | ... | -3.12+-0.35 | 0.35+-0.35 | 4.39 |
| Ca I | ... | -2.81+-0.22 | 0.66+-0.22 | 3.53 |
| Sc II | ... | -3.58+-0.15 | -0.11+-0.15 | -0.1 |
| Ti I | ... | -2.86+-0.21 | 0.61+-0.21 | 2.09 |
| Ti II | ... | -3.09+-0.14 | 0.38+-0.14 | 2.19 |
| V II | ... | <-2.74 | <0.73 | <1.26 |
| Cr I | ... | -3.63+-0.2 | -0.16+-0.2 | 2.01 |
| Mn I | ... | -4.25+-0.22 | -0.78+-0.22 | 1.18 |
| Fe I | ... | -3.47+-0.22 | ... | 4.03 |
| Fe II | ... | -3.14+-0.14 | ... | 4.36 |
| Co I | ... | -3.22+-0.23 | 0.25+-0.23 | 1.77 |
| Cu I | ... | <-1.91 | <1.56 | <2.3 |
| Zn I | ... | <-2.39 | <1.08 | <2.21 |
| Rb I | ... | <-0.09 | <3.38 | <2.51 |
| Sr II | ... | -3.54+-0.18 | -0.07+-0.18 | -0.34 |
| Y II | ... | <-2.71 | <0.76 | <-0.47 |
| Zr II | ... | <-2.32 | <1.15 | <0.28 |
| Mo I | ... | <-1.12 | <2.35 | <0.8 |
| Tc I | ... | <1.01 | <4.48 | <1.01 |
| Ba II | ... | -4.11+-0.14 | -0.64+-0.14 | -1.6 |
| Ce II | ... | <-1.77 | <1.70 | <-0.19 |
| Pr II | ... | <-1.15 | <2.32 | <-0.44 |
| Nd II | ... | <-2.06 | <1.41 | <-0.56 |
| Sm II | ... | <-1.50 | <1.97 | <-0.49 |
| Eu II | ... | <-1.96 | <1.51 | <-1.45 |
| Gd II | ... | <-1.08 | <2.39 | <0.04 |
| Tb II | ... | <-0.47 | <3.00 | <-0.57 |
| Dy II | ... | <-1.57 | <1.90 | <-0.43 |
| Er II | ... | <-1.30 | <2.17 | <-0.37 |
| Tm II | ... | <-0.75 | <2.72 | <-0.75 |
| Yb II | ... | <-2.17 | <1.30 | <-1.09 |
| Hf II | ... | <-0.54 | <2.93 | <0.34 |
| Pb I | ... | <-0.45 | <3.02 | <1.5 |
| Th II | ... | <-0.55 | <2.92 | <-0.55 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)