| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| Li I | ... | -1.59-0.16 | +-0.16 | 1.15 |
| CH | ... | -2.00+-0.25 | -0.41+-0.25 | 6.43 |
| Na I | ... | -1.74+-0.15 | -0.15+-0.15 | 4.5 |
| Mg I | ... | -1.41+-0.12 | 0.18+-0.12 | 6.19 |
| Si I | ... | -1.28+-0.2 | 0.31+-0.2 | 6.23 |
| Ca I | ... | -1.29+-0.18 | 0.3+-0.18 | 5.06 |
| Sc II | ... | -1.53+-0.13 | 0.06+-0.13 | 1.64 |
| Ti I | ... | -1.37+-0.1 | 0.22+-0.1 | 3.58 |
| Ti II | ... | -1.22+-0.12 | 0.37+-0.12 | 3.74 |
| V I | ... | -1.73+-0.17 | -0.14+-0.17 | 2.2 |
| Cr I | ... | -1.59+-0.1 | 0.00+-0.1 | 4.06 |
| Cr II | ... | -1.27+-0.14 | 0.32+-0.14 | 4.39 |
| Mn I | ... | -1.97+-0.11 | -0.38+-0.11 | 3.46 |
| Fe I | ... | -1.59+-0.11 | ... | 5.91 |
| Fe II | ... | -1.58+-0.14 | ... | 5.92 |
| Co I | ... | -1.74+-0.22 | -0.15+-0.22 | 3.25 |
| Ni I | ... | -1.55+-0.14 | 0.04+-0.14 | 4.67 |
| Cu I | ... | -2.07+-0.12 | -0.48+-0.12 | 2.12 |
| Zn I | ... | -1.49+-0.09 | 0.1+-0.09 | 3.07 |
| Sr II | ... | -1.63+-0.1 | -0.04+-0.1 | 1.25 |
| Y II | ... | -1.83+-0.16 | -0.24+-0.16 | 0.39 |
| Zr II | ... | -1.23+-0.2 | 0.36+-0.2 | 1.36 |
| Ba II | ... | -1.54+-0.1 | 0.05+-0.1 | 0.66 |
| La II | ... | -1.75+-0.47 | -0.16+-0.47 | -0.64 |
| Ce II | ... | <-1.18 | <0.41 | <0.4 |
| Nd II | ... | -1.69+-0.4 | -0.1+-0.4 | -0.26 |
| Sm II | ... | -1.07+-0.17 | 0.52+-0.17 | -0.1 |
| Eu II | ... | -1.12+-0.19 | 0.47+-0.19 | -0.59 |
| Tb II | ... | <0.63 | <2.22 | <0.53 |
| Dy II | ... | <-0.03 | <1.56 | <1.11 |
| Tm II | ... | <1.27 | <2.86 | <1.27 |
| Hf II | ... | <0.05 | <1.64 | <0.93 |
| Pb I | ... | <-0.13 | <1.46 | <1.82 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
