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Table 2.
Abundance sensitivity assuming a change Δ in the stellar parameters for a representative virtual star with Teff = 4400 K, log g = 1, [Fe/H] = −1.5 and ξt = 1.8 km s−1.
| Element | ΔTeff | Δlog g | Δ[M/H] | Δξt | σtot |
|---|---|---|---|---|---|
| 140 K | 0.25 dex | 0.2 dex | 0.15 km s−1 | dex | |
| Δlog ϵ(Mg) | 0.13 | 0.07 | 0.06 | 0.03 | 0.16 |
| Δlog ϵ(Sc) | 0.02 | 0.11 | 0.07 | 0.01 | 0.13 |
| Δlog ϵ(Ti) | 0.03 | 0.14 | 0.05 | 0.12 | 0.19 |
| Δlog ϵ(Cr) | 0.30 | 0.05 | 0.05 | 0.10 | 0.32 |
| Δlog ϵ(Mn) | 0.22 | 0.03 | 0.03 | 0.03 | 0.23 |
| Δlog ϵ(Ni) | 0.19 | 0.01 | 0.01 | 0.06 | 0.20 |
| Δlog ϵ(Zn) | 0.06 | 0.07 | 0.03 | 0.05 | 0.11 |
| Δlog ϵ(Sr) | 0.04 | 0.04 | 0.01 | 0.16 | 0.17 |
| Δlog ϵ(Y) | 0.01 | 0.09 | 0.05 | 0.02 | 0.11 |
| Δlog ϵ(Ba) | 0.03 | 0.10 | 0.05 | 0.07 | 0.14 |
| Δlog ϵ(Eu) | 0.08 | 0.05 | 0.06 | 0.07 | 0.13 |
Notes. Uncertainties added in quadrature are listed in σtot.
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