Table B.3
Abundances of Zr in the three stars common to the GIRAFFE (used in this work) and UVES samples (Thygesen et al. 2014), determined from Zr I and Zr II lines in the UVES spectra.
| ID | Teff K |
log g | ξmicro km s–1 |
A(Zr)I 612.7475 nm |
A(Zr)I 613.4585 nm |
A(Zr)I 614.0535 nm |
A(Zr)I 614.3252 nm |
A(Zr)II 511.2270 nm |
A(Zr)II 535.0089 nm |
A(Zr)II 535.0350 nm |
|---|---|---|---|---|---|---|---|---|---|---|
| 13396 | 4245 | 1.34 | 1.57 | 2.24 | 2.18 | 2.17* | 2.16 | 2.26 | 2.14 | 2.23 |
| 20885 | 4359 | 1.41 | 1.82 | 2.16 | 2.13* | 2.12* | – | 2.18 | 2.16 | 2.20 |
| 29861 | 4217 | 1.32 | 1.61 | 2.12* | 2.18 | – | 2.18 | 2.20 | 2.15 | 2.22 |
Note: Atmospheric parameters used in the abundance analysis were those determined in our study (Sect 2.1). Abundances marked with the asterisks were determined from the weak and/or noisy lines.
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