Table 4
Stellar elemental abundances in differential logarithmic units (dex) from Brewer et al. (2016).
| Star | [C/H] | [O/H] | [Na/H] | [Mg/H] | [Al/H] | [Si/H] | [Ca/H] | [Ti/H] | [Cr/H] | [Fe/H] | [Ni/H] | [S/H] |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Kepler-62 | −0.22 | −0.17 | −0.41 | −0.30 | −0.29 | −0.27 | −0.29 | −0.28 | −0.39 | −0.37 | −0.40 | −0.29(*) |
| HD 97658 | −0.24 | −0.17 | −0.30 | −0.22 | −0.24 | −0.23 | −0.25 | −0.23 | −0.27 | −0.28 | −0.29 | −0.22(*) |
| Kepler-102 | 0.03 | −0.06 | 0.13 | 0.07 | 0.08 | 0.12 | 0.15 | 0.09 | 0.09 | 0.12 | 0.10 | 0.07(*) |
| Kepler-113 | 0.47 | 0.53 | 0.22 | 0.17 | 0.22 | 0.21 | 0.19 | 0.17 | 0.13 | 0.15 | 0.17 | 0.09(*) |
| HD 18143 | 0.24 | 0.25 | 0.35 | 0.24 | 0.30 | 0.22 | 0.25 | 0.25 | 0.26 | 0.26 | 0.27 | 0.17(*) |
| Kepler-94 | 0.22 | 0.11 | 0.70 | 0.34 | 0.48 | 0.38 | 0.45 | 0.36 | 0.36 | 0.41 | 0.47 | 0.28(*) |
Notes. The uncertainties in the table are between ~0.01 and ~0.04 dex (Brewer et al. (2016), Table 6). The asterisk(*) is used to denote S abundances estimated based on their respective [Fe/H] values. The S abundances might carry a larger uncertainty due to the scatter in the fit (about 0.1 dex, which is the quadratic sum of the error in [Fe/H] and the scatter in the relation).
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