| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| Li I | ... | <-0.51 | <2.61 | <0.65 |
| CH | ... | -2.67+-0.25 | 0.45+-0.25 | 5.75 |
| CN | ... | <-2.17 | <0.95 | <5.8 |
| O I | ... | <-1.84 | <1.28 | <7.03 |
| Mg I | ... | -2.70+-0.1 | 0.42+-0.1 | 4.89 |
| Al I | ... | -3.36+-0.25 | -0.24+-0.25 | 3.09 |
| K I | ... | -2.97+-0.16 | 0.15+-0.16 | 2.06 |
| Ca I | ... | -2.75+-0.13 | 0.37+-0.13 | 3.59 |
| Sc II | ... | -3.21+-0.17 | -0.09+-0.17 | -0.07 |
| Ti I | ... | -2.91+-0.1 | 0.21+-0.1 | 2.03 |
| Ti II | ... | -2.97+-0.18 | 0.15+-0.18 | 1.96 |
| V I | ... | -3.07+-0.14 | 0.05+-0.14 | 0.86 |
| Cr I | ... | -3.17+-0.1 | -0.05+-0.1 | 2.46 |
| Mn I | ... | -3.56+-0.14 | -0.44+-0.14 | 1.87 |
| Fe I | ... | -3.12+-0.1 | ... | 4.38 |
| Fe II | ... | -3.13+-0.19 | ... | 4.37 |
| Co I | ... | -3.31+-0.16 | -0.19+-0.16 | 1.68 |
| Ni I | ... | -3.19+-0.16 | -0.07+-0.16 | 3.03 |
| Zn I | ... | -2.76+-0.2 | 0.36+-0.2 | 1.8 |
| Sr II | ... | -3.88+-0.16 | -0.76+-0.16 | -1.02 |
| Y II | ... | <-3.78 | <-0.66 | <-1.54 |
| Zr II | ... | <-2.44 | <0.68 | <0.16 |
| Mo I | ... | <-2.23 | <0.89 | <-0.31 |
| Tc I | ... | <-0.10 | <3.02 | <-0.1 |
| Ba II | ... | -4.32+-0.19 | -1.2+-0.19 | -2.15 |
| Ce II | ... | <-2.37 | <0.75 | <-0.79 |
| Pr II | ... | <-1.92 | <1.20 | <-1.21 |
| Nd II | ... | <-2.19 | <0.93 | <-0.69 |
| Sm II | ... | <-1.91 | <1.21 | <-0.9 |
| Eu II | ... | <-2.65 | <0.47 | <-2.14 |
| Gd II | ... | <-1.61 | <1.51 | <-0.49 |
| Tb II | ... | <-1.05 | <2.07 | <-1.15 |
| Dy II | ... | <-2.25 | <0.87 | <-1.11 |
| Er II | ... | <-1.73 | <1.39 | <-0.8 |
| Tm II | ... | <-1.35 | <1.77 | <-1.35 |
| Yb II | ... | <-2.80 | <0.32 | <-1.72 |
| Hf II | ... | <-1.12 | <2.00 | <-0.24 |
| Pb I | ... | <-1.37 | <1.75 | <0.58 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
