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Table 3.
Derived chemical abundances with errors for our sample stars.
| Star | Nlines | A(FeI) | s(FeI) | [FeI/H] | Nlines | A(FeII) | s(FeII) | [FeII/H] | ... |
|---|---|---|---|---|---|---|---|---|---|
| (dex) | (dex) | (dex) | (dex) | ||||||
| CES0031–1647 | 304 | 5.03 | 0.12 | −2.49 | 26 | 5.22 | 0.09 | −2.31 | ... |
| CES0045–0932 | 176 | 4.57 | 0.14 | −2.95 | 12 | 4.72 | 0.19 | −2.80 | ... |
| CES0048–1041 | 314 | 5.04 | 0.13 | −2.48 | 26 | 5.19 | 0.13 | −2.33 | ... |
| CES0055–3345 | 340 | 5.16 | 0.11 | −2.36 | 28 | 5.28 | 0.12 | −2.24 | ... |
| CES0059–4524 | 146 | 5.13 | 0.09 | −2.39 | 8 | 5.26 | 0.09 | −2.26 | ... |
| ... |
Notes. The complete table is available in machine readable format at the CDS.
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