Table A.1.
Detailed abundances of the GBS with respect to the Sun analyzed in this work (rows marked as “here”) with the dispersion among the spectra quoted as uncertainty.
| Star | Nspec | [Ca I/H] | [Co I/H] | [Cr I/H] | [Fe I/H] | [Mg I/H] | [Mn I/H] | [Ni I/H] | [Sc II/H] | [Si I/H] | [Ti I/H] | [V I/H] | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 18Sco | here | 24 | 0.04 ± 0.01 | 0.02 ± 0.01 | 0.04 ± 0.01 | 0.03 ± 0.01 | 0.02 ± 0.01 | 0.02 ± 0.01 | 0.02 ± 0.01 | 0.03 ± 0.01 | 0.03 ± 0.01 | 0.02 ± 0.01 | 0.01 ± 0.01 |
| (0.03) | (0.03) | (0.03) | (0.03) | (0.01) | (0.05) | (0.04) | (0.02) | (0.04) | (0.04) | (0.04) | |||
| Ref | 0.06 ± 0.06 | 0.02 ± 0.07 | 0.05 ± 0.06 | 0.03 ± 0.03 | 0.04 ± 0.05 | 0.04 ± 0.09 | 0.04 ± 0.07 | 0.04 ± 0.05 | 0.05 ± 0.03 | 0.05 ± 0.08 | 0.04 ± 0.07 | ||
| Arcturus | here | 5 | −0.55 ± 0.02 | −0.41 ± 0.02 | −0.58 ± 0.01 | −0.66 ± 0.01 | −0.26 ± 0.01 | −0.91 ± 0.01 | −0.59 ± 0.01 | −0.59 ± 0.01 | −0.37 ± 0.02 | −0.34 ± 0.01 | −0.34 ± 0.02 |
| (0.07) | (0.07) | (0.07) | (0.10) | (0.04) | (0.09) | (0.08) | (0.08) | (0.06) | (0.10) | (0.07) | |||
| Ref | −0.41 ± 0.13 | −0.41 ± 0.07 | −0.58 ± 0.08 | −0.52 ± 0.08 | −0.16 ± 0.11 | −0.89 ± 0.16 | −0.49 ± 0.10 | −0.43 ± 0.15 | −0.25 ± 0.07 | −0.31 ± 0.11 | −0.44 ± 0.14 | ||
Notes. The number of used spectra fo each star is listed in the column Nspec. The median of the individual quoted uncertainties per spectra is indicated in parenthesis. In the rows marked as “Ref”, we list the reference values of the GBS abundances. The full version of the table is available at the CDS.
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