| Element | Nline | [X/H] | [X/Fe] | log-e |
| Li I | ... | -2.28-0.2 | +-0.2 | 2.09 |
| CH | ... | -2.24+-0.25 | 0.04+-0.25 | 6.38 |
| NH | ... | <-1.07 | <1.21 | <6.9 |
| O I | ... | -1.78+-0.2 | 0.5+-0.2 | 6.9 |
| Na I | ... | -2.43+-0.32 | -0.15+-0.32 | 3.81 |
| Mg I | ... | -1.92+-0.24 | 0.36+-0.24 | 5.67 |
| Al I | ... | -3.07+-0.33 | -0.79+-0.33 | 3.38 |
| Si I | ... | -1.84+-0.37 | 0.44+-0.37 | 5.67 |
| Ca I | ... | -1.78+-0.22 | 0.5+-0.22 | 4.56 |
| Sc II | ... | -2.18+-0.14 | 0.1+-0.14 | 1.16 |
| Ti I | ... | -1.86+-0.2 | 0.42+-0.2 | 3.08 |
| Ti II | ... | -1.90+-0.14 | 0.38+-0.14 | 3.24 |
| V II | ... | -2.07+-0.25 | 0.21+-0.25 | 2.05 |
| Cr I | ... | -2.38+-0.21 | -0.1+-0.21 | 3.26 |
| Cr II | ... | -2.00+-0.14 | 0.28+-0.14 | 3.83 |
| Mn I | ... | -2.52+-0.22 | -0.24+-0.22 | 2.9 |
| Mn II | ... | -2.56+-0.2 | -0.28+-0.2 | 3.06 |
| Fe I | ... | -2.28+-0.21 | ... | 5.22 |
| Fe II | ... | -2.09+-0.14 | ... | 5.41 |
| Co I | ... | -2.34+-0.24 | -0.06+-0.24 | 2.65 |
| Ni I | ... | -2.18+-0.29 | 0.1+-0.29 | 4.04 |
| Zn I | ... | -1.92+-0.21 | 0.36+-0.21 | 2.64 |
| Rb I | ... | <0.00 | <2.28 | <2.6 |
| Sr II | ... | -2.08+-0.23 | 0.2+-0.23 | 0.98 |
| Zr II | ... | -1.88+-0.16 | 0.4+-0.16 | 0.89 |
| Nb II | ... | <0.07 | <2.35 | <1.49 |
| Mo I | ... | <-0.79 | <1.49 | <1.13 |
| Tc I | ... | <1.47 | <3.75 | <1.47 |
| Ba II | ... | -2.50+-0.14 | -0.22+-0.14 | -0.13 |
| Ce II | ... | <-1.40 | <0.88 | <0.18 |
| Pr II | ... | <-0.71 | <1.57 | <0 |
| Nd II | ... | <-1.58 | <0.70 | <-0.08 |
| Sm II | ... | <-0.84 | <1.44 | <0.17 |
| Eu II | ... | -1.73+-0.17 | 0.55+-0.17 | -1.02 |
| Gd II | ... | <-0.79 | <1.49 | <0.33 |
| Tb II | ... | <0.05 | <2.33 | <-0.05 |
| Dy II | ... | <-1.17 | <1.11 | <-0.03 |
| Ho II | ... | <-0.31 | <1.97 | <-0.05 |
| Er II | ... | <-0.97 | <1.31 | <-0.04 |
| Tm II | ... | <-0.56 | <1.72 | <-0.56 |
| Yb II | ... | -2.10+-0.26 | 0.18+-0.26 | -0.99 |
| Hf II | ... | <-0.10 | <2.18 | <0.78 |
| Pb I | ... | <-0.22 | <2.06 | <1.73 |
| Th II | ... | <-0.23 | <2.05 | <-0.23 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)