| Element | Nline | [X/H] | [X/Fe] | log-e |
| Li I | ... | -2.92-0.2 | +-0.2 | 2.36 |
| CH | ... | -2.80+-0.25 | 0.12+-0.25 | 5.84 |
| NH | ... | <-1.77 | <1.15 | <6.2 |
| O I | ... | -2.39+-0.22 | 0.53+-0.22 | 6.3 |
| Mg I | ... | -2.55+-0.21 | 0.37+-0.21 | 5.05 |
| Al I | ... | -3.69+-0.23 | -0.77+-0.23 | 2.76 |
| Si I | ... | -2.57+-0.36 | 0.35+-0.36 | 4.94 |
| Ca I | ... | -2.48+-0.22 | 0.44+-0.22 | 3.86 |
| Sc II | ... | -2.94+-0.15 | -0.02+-0.15 | 0.42 |
| Ti I | ... | -2.42+-0.21 | 0.5+-0.21 | 2.53 |
| Ti II | ... | -2.59+-0.14 | 0.33+-0.14 | 2.57 |
| Cr I | ... | -3.03+-0.2 | -0.11+-0.2 | 2.61 |
| Cr II | ... | -2.79+-0.17 | 0.13+-0.17 | 3.06 |
| Mn I | ... | -3.34+-0.2 | -0.42+-0.2 | 2.09 |
| Mn II | ... | -3.40+-0.21 | -0.48+-0.21 | 2.25 |
| Fe I | ... | -2.92+-0.21 | ... | 4.58 |
| Fe II | ... | -2.71+-0.15 | ... | 4.79 |
| Co I | ... | -2.78+-0.25 | 0.14+-0.25 | 2.21 |
| Ni I | ... | -2.93+-0.25 | -0.01+-0.25 | 3.29 |
| Zn I | ... | -2.32+-0.23 | 0.6+-0.23 | 2.24 |
| Rb I | ... | <0.21 | <3.13 | <2.81 |
| Sr II | ... | -2.97+-0.16 | -0.05+-0.16 | 0.11 |
| Y II | ... | -3.49+-0.29 | -0.57+-0.29 | -1.07 |
| Zr II | ... | <-1.65 | <1.27 | <0.95 |
| Nb II | ... | <0.03 | <2.95 | <1.45 |
| Mo I | ... | <-0.81 | <2.11 | <1.11 |
| Tc I | ... | <1.33 | <4.25 | <1.33 |
| Ba II | ... | -3.42+-0.14 | -0.5+-0.14 | -1.03 |
| Ce II | ... | <-1.55 | <1.37 | <0.03 |
| Pr II | ... | <-0.91 | <2.01 | <-0.2 |
| Nd II | ... | <-1.47 | <1.45 | <0.03 |
| Sm II | ... | <-0.95 | <1.97 | <0.06 |
| Eu II | ... | <-1.53 | <1.39 | <-1.02 |
| Gd II | ... | <-0.86 | <2.06 | <0.26 |
| Tb II | ... | <-0.16 | <2.76 | <-0.26 |
| Ho II | ... | <-0.84 | <2.08 | <-0.58 |
| Er II | ... | <-1.14 | <1.78 | <-0.21 |
| Tm II | ... | <-0.43 | <2.49 | <-0.43 |
| Yb II | ... | <-2.41 | <0.51 | <-1.33 |
| Hf II | ... | <-0.29 | <2.63 | <0.59 |
| Pb I | ... | <-0.28 | <2.64 | <1.67 |
| Th II | ... | <-0.26 | <2.66 | <-0.26 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)