Table 8
Excerpt from the list of abundances of α elements for each spectrum of the 20 calibrating Cepheids.
Name | Dataset | MJD [d] | [Mg/H] ± σ | NMg | … | Ti I ± σ | NTi I | Ti II ± σ | NTi II | [Ti/H] ± σ |
---|---|---|---|---|---|---|---|---|---|---|
R TrA | HARPS | 53 150.1353086 | 0.17 ± 0.11 | 1 | −0.17 ± 0.27 | 12 | 0.01 ± 0.10 | 3 | −0.14 ± 0.25 | |
R TrA | HARPS | 53 150.1453265 | 0.20 ± 0.11 | 1 | −0.21 ± 0.15 | 8 | 0.05 ± 0.10 | 2 | −0.12 ± 0.19 | |
… | … | … | … | … | … | … | … | … | … | … |
RS Pup | STELLA | 57 704.2420857 | 0.01 ± 0.11 | 1 | … | 0.03 ± 0.14 | 10 | 0.11 ± 0.10 | 3 | 0.05 ± 0.14 |
RS Pup | STELLA | 57 708.2167938 | 0.24 ± 0.11 | 2 | … | −0.06 ± 0.28 | 15 | 0.22 ± 0.10 | 4 | 0.09 ± 0.19 |
Notes. The first three columns give the target name, spectroscopic dataset, and Modified Julian Date at which the spectrum was collected. The other columns give the abundances from both neutral and ionized lines, their standard deviations, and the number of lines used. For each element X, the weighted mean of X I and X II abundances (weighted by 1/σ2) and its intrinsic error is also shown. Magnesium and sulfur abundances are from neutral lines only. The complete table is available at the CDS.
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