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Table 7
Abundance errors due to atmospheric parameter uncertainties as examples for HE 1523-0901 with the stellar parameters Teff = 4550 K, log 𝑔 = 0.80, Vt = 2.5 km s−1 and [Fe/H] = −2.82.
AN | El | Δ Teff+ | Δ log 𝑔+ | Δ Vt+ | tot+ |
---|---|---|---|---|---|
06 | C | −0.1 | 0.15 | −0.01 | 0.18 |
07 | N | 0.19 | −0.10 | −0.01 | 0.21 |
08 | OI | 0.07 | 0.12 | −0.01 | 0.14 |
11 | NaI | 0.05 | −0.03 | −0.01 | 0.07 |
12 | MgI | 0.13 | −0.13 | −0.03 | 0.19 |
13 | AlI | 0.13 | −0.04 | −0.01 | 0.14 |
14 | SiI | 0.04 | −0.01 | −0.01 | 0.05 |
19 | KI | 0.05 | −0.03 | −0.01 | 0.07 |
20 | CaI | 0.08 | −0.04 | −0.01 | 0.09 |
23.01 | ScII | 0.04 | 0.12 | −0.01 | 0.13 |
22 | TiI | 0.13 | −0.04 | −0.01 | 0.14 |
22.01 | TiII | 0.02 | 0.12 | −0.01 | 0.13 |
23 | VI | 0.13 | −0.05 | −0.01 | 0.14 |
24 | CrI | 0.09 | −0.03 | −0.01 | 0.10 |
25 | MnI | 0.08 | −0.03 | −0.01 | 0.09 |
26 | FeI | 0.09 | −0.03 | −0.01 | 0.10 |
26.01 | FeII | 0.01 | 0.13 | 0.01 | 0.13 |
27 | CoI | 0.13 | −0.04 | −0.01 | 0.14 |
28 | NiI | 0.09 | −0.02 | −0.01 | 0.10 |
29 | CuI | 0.08 | −0.03 | 0.0 | 0.09 |
30 | ZnI | 0.04 | 0.06 | −0.01 | 0.08 |
38 | SrII | 0.05 | 0.12 | −0.02 | 0.14 |
39 | YII | 0.05 | 0.12 | −0.01 | 0.13 |
40 | ZrII | 0.04 | 0.12 | −0.01 | 0.13 |
44 | RuI | 0.14 | −0.03 | −0.01 | 0.15 |
56 | BaII | 0.12 | 0.07 | −0.05 | 0.15 |
57 | LaII | 0.08 | 0.12 | −0.01 | 0.15 |
58 | CeII | 0.07 | 0.12 | −0.01 | 0.14 |
59 | PrII | 0.07 | 0.12 | −0.01 | 0.14 |
60 | NdII | 0.07 | 0.12 | −0.01 | 0.14 |
62 | SmII | 0.084 | 0.12 | −0.01 | 0.15 |
63 | EuII | 0.05 | 0.12 | −0.03 | 0.14 |
64 | GdII | 0.05 | 0.12 | −0.01 | 0.13 |
65 | TbII | 0.07 | 0.14 | −0.01 | 0.16 |
66 | DyII | 0.07 | 0.13 | −0.01 | 0.15 |
67 | HoII | 0.06 | 0.13 | −0.01 | 0.15 |
68 | ErI | 0.15 | −0.03 | −0.01 | 0.16 |
69 | TmII | 0.09 | 0.13 | −0.01 | 0.16 |
72 | HfI | 0.17 | −0.03 | −0.01 | 0.18 |
76 | OsI | 0.15 | 0.02 | −0.01 | 0.15 |
77 | IrI | 0.14 | 0.08 | −0.01 | 0.16 |
90 | ThII | 0.06 | 0.14 | −0.01 | 0.15 |
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