Table 4
Errors owing to uncertainties in stellar atmospheric parameters.
| Sex24-72 | Sex11-04 | Fnx05-42 | Scl07-49 | Scl07-50 | ||||||
| Δ(T,v) | Δg | Δ(T,v) | Δg | Δ(T,v) | Δg | Δ(T,v) | Δg | Δ(T,v) | Δg | |
|
|
||||||||||
| FeI | 0.16 | −0.07 | 0.13 | 0.04 | 0.23 | 0.00 | 0.17 | 0.04 | 0.15 | −0.04 |
| FeII | −0.16 | −0.10 | −0.29 | 0.02 | −0.28 | 0.01 | −0.09 | 0.08 | −0.00 | 0.07 |
| Al | −0.06 | −0.18 | −0.13 | −0.08 | −0.04 | −0.03 | ||||
| Ba | −0.07 | 0.04 | −0.10 | 0.02 | −0.19 | 0.11 | ||||
| C | 0.30 | −0.40 | 0.30 | −0.35 | 0.37 | −0.30 | 0.40 | −0.30 | ||
| Ca | −0.05 | 0.04 | 0.02 | −0.02 | −0.07 | −0.04 | −0.02 | 0.00 | −0.09 | −0.08 |
| Co | −0.04 | −0.07 | −0.17 | 0.00 | −0.05 | −0.02 | 0.04 | −0.01 | ||
| Cr | 0.04 | 0.01 | 0.08 | 0.05 | 0.04 | −0.02 | 0.03 | 0.01 | 0.03 | −0.02 |
| Mg | −0.10 | −0.01 | −0.08 | −0.06 | −0.13 | −0.05 | 0.00 | −0.06 | −0.10 | −0.04 |
| Mn | −0.03 | 0.02 | 0.03 | −0.03 | 0.07 | 0.06 | 0.05 | −0.01 | ||
| Na | −0.09 | 0.06 | 0.05 | 0.05 | −0.01 | 0.01 | 0.01 | 0.03 | −0.01 | 0.01 |
| Ni | −0.04 | −0.05 | −0.05 | 0.01 | −0.08 | −0.02 | 0.02 | 0.02 | −0.00 | −0.03 |
| O | −0.03 | 0.03 | −0.03 | 0.13 | ||||||
| Sc | −0.15 | 0.05 | −0.17 | −0.01 | −0.28 | 0.05 | −0.14 | 0.11 | −0.11 | 0.08 |
| Si | −0.12 | 0.06 | −0.29 | −0.21 | −0.22 | −0.09 | −0.12 | −0.07 | ||
| SrII | −0.28 | −0.29 | ||||||||
| TiI | 0.09 | 0.05 | 0.19 | 0.07 | 0.07 | −0.03 | 0.10 | 0.01 | ||
| TiII | −0.18 | 0.04 | −0.19 | 0.00 | −0.28 | 0.08 | −0.17 | 0.11 | −0.11 | 0.10 |
| Y | −0.12 | −0.14 | 0.00 | −0.23 | ||||||
Notes. Δ(T,v) stands for a simultaneous shift – consequence of their correlated impact on abundances – of Teff by +150 K and vt by +0.2 km s-1 and Δg for a shift of log (g) by +0.3 dex. The uncertainties are roughly symmetric, therefore negative shifts of the atmospheric parameters yield the same errors with opposite signs.
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