| Element | Nline | [X/H] | [X/Fe] | log-e |
| Li I | ... | -2.55-0.2 | +-0.2 | 1.93 |
| CH | ... | -1.97+-0.25 | 0.58+-0.25 | 6.27 |
| CN | ... | <-0.72 | <1.83 | <7.25 |
| O I | ... | <-2.05 | <0.50 | <6.82 |
| Mg I | ... | -2.21+-0.2 | 0.34+-0.2 | 5.39 |
| Al I | ... | -3.04+-0.33 | -0.49+-0.33 | 3.41 |
| Ca I | ... | -2.15+-0.22 | 0.4+-0.22 | 4.19 |
| Sc II | ... | -2.43+-0.14 | 0.12+-0.14 | 0.52 |
| Ti I | ... | -2.35+-0.2 | 0.2+-0.2 | 2.6 |
| Ti II | ... | -2.39+-0.14 | 0.16+-0.14 | 2.36 |
| V I | ... | <-2.20 | <0.35 | <1.8 |
| V II | ... | <-2.06 | <0.49 | <1.94 |
| Cr I | ... | -2.68+-0.22 | -0.13+-0.22 | 2.95 |
| Mn I | ... | -2.84+-0.23 | -0.29+-0.23 | 2.59 |
| Fe I | ... | -2.55+-0.21 | ... | 4.95 |
| Fe II | ... | -2.75+-0.15 | ... | 4.75 |
| Co I | ... | -2.43+-0.22 | 0.12+-0.22 | 2.56 |
| Ni I | ... | -2.46+-0.22 | 0.09+-0.22 | 3.76 |
| Zn I | ... | <-1.91 | <0.64 | <2.69 |
| Rb I | ... | <0.47 | <3.02 | <3.07 |
| Sr II | ... | -2.65+-0.24 | -0.1+-0.24 | 0.02 |
| Y II | ... | -2.68+-0.2 | -0.13+-0.2 | -0.66 |
| Nb II | ... | <0.28 | <2.83 | <1.7 |
| Mo I | ... | <-0.57 | <1.98 | <1.35 |
| Tc I | ... | <1.44 | <3.99 | <1.44 |
| Sn I | ... | <0.62 | <3.17 | <2.62 |
| Ba II | ... | -2.57+-0.15 | -0.02+-0.15 | -0.59 |
| La II | ... | <-1.82 | <0.73 | <-0.65 |
| Pr II | ... | <-0.75 | <1.80 | <-0.04 |
| Nd II | ... | <-1.48 | <1.07 | <0.02 |
| Sm II | ... | <-0.95 | <1.60 | <0.06 |
| Eu II | ... | -1.65+-0.21 | 0.9+-0.21 | -1.33 |
| Gd II | ... | <-0.68 | <1.87 | <0.44 |
| Tb II | ... | <0.08 | <2.63 | <-0.02 |
| Dy II | ... | -1.29+-0.18 | 1.26+-0.18 | -0.39 |
| Er II | ... | <-1.01 | <1.54 | <-0.08 |
| Tm II | ... | <-0.21 | <2.34 | <-0.21 |
| Yb II | ... | -1.69+-0.24 | 0.86+-0.24 | -0.97 |
| Hf II | ... | <-0.11 | <2.44 | <0.77 |
| Pb I | ... | <-0.05 | <2.50 | <1.9 |
| Th II | ... | <-0.38 | <2.17 | <-0.38 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)