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Table B.4

Mean abundances of Fe, Na, and Zr in the three common stars obtained by us from the GIRAFFE and UVES spectra, and those determined by Thygesen et al. (2014) from the same UVES spectra.

ID This study Thygesen et al. 2014)
Teff
K
log g ξmicro
km s–1
[Fe/H]
GIRAFFE
[Na/Fe]
GIRAFFE
[ZrIFe]
GIRAFFE
[ZrI/Fe]
UVES
[ZrII/Fe]
UVES
Teff log g ξmicro [Fe/H]
UVES
[Na/Fe]
UVES
[ZrIFe]
UVES
13396 4245 1.34 1.57 –0.77 0.16 0.36 0.34 0.36 4190 1.45 1.60 –0.83 0.07 0.25
20885 4359 1.41 1.82 –0.74 0.21 0.31 0.27 0.30 4260 1.35 1.90 –0.84 0.11 0.18
29861 4217 1.32 1.61 –0.82 0.28 0.38 0.36 0.39 4160 1.20 1.50 –0.84 0.10 0.23

Note: Abundances obtained by us from the Zr I 614.0460 nm line were not used in the computation of the mean Zr abundances.

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