Table C.2.
Results of the abundance determination using different combinations of stellar parameters.
| Teff | log g | ξ | ϵN; measured EW | ϵN; nominal EW |
|---|---|---|---|---|
| [kK] | [dex] | [km s−1] | [dex] | [dex] |
| 32.0 | 3.8 | 11 | 8.1 | 8.1 |
| 32.0 | 3.8 | 11 | 8.10 ± 0.08 | 8.10 ± 0.00 |
| 32.0 | 3.8 | 8 | 8.16 ± 0.09 | 8.14 ± 0.03 |
| 32.0 | 3.8 | 14 | 8.07 ± 0.08 | 8.08 ± 0.02 |
| 31.0 | 3.8 | 11 | 8.06 ± 0.18 | 8.11 ± 0.21 |
| 33.0 | 3.8 | 11 | 8.17 ± 0.16 | 8.13 ± 0.21 |
| 32.0 | 3.7 | 11 | 8.11 ± 0.12 | 8.08 ± 0.12 |
| 32.0 | 3.9 | 11 | 8.10 ± 0.10 | 8.12 ± 0.08 |
| 31.0 | 3.7 | 11 | 8.06 ± 0.13 | 8.08 ± 0.10 |
| 33.0 | 3.9 | 11 | 8.16 ± 0.11 | 8.13 ± 0.13 |
Notes. In the table header, for reference, below the parameter in the column, the model value. The fourth column shows the results obtained with the measured EW values, while the fifth column presents the results when using the EW values from the original model.
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