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Table B.1.

Chemical abundances derived for the metal-poor stars presented in this work.

201359581 – S1 205997746 – S2 206034668 – S3 206443679 – S4




Species At. N. Nlin Abd. eA Nlin Abd. eA Nlin Abd. eA Nlin Abd. eA Met.
C 6.0 6.92 0.15 6.94 0.10 7.08 0.11 6.48 0.09 f
Na I 11.0 2 4.71 0.06 2 6.07 0.12 2 4.96 0.05 2 4.68 0.08 ew
Mg I 12.0 3 6.24 0.11 3 6.92 0.05 3 6.34 0.15 3 6.36 0.10 ew
Si I 14.0 2 6.45 0.07 2 6.81 0.03 2 6.60 0.10 2 6.36 0.10 ew
Ca I 20.0 7 5.01 0.05 7 5.45 0.10 7 5.05 0.13 7 4.95 0.13 ew
Sc II 21.1 3 1.66 0.11 3 1.84 0.14 3 1.74 0.11 3 1.53 0.14 ew
Ti I 22.0 11 3.40 0.08 11 3.91 0.15 9 3.59 0.10 11 3.58 0.10 ew
Ti II 22.1 17 3.56 0.10 17 3.95 0.11 16 3.68 0.12 17 3.60 0.09 ew
Cr I 24.0 9 3.84 0.22 9 4.38 0.11 7 3.98 0.09 9 3.87 0.09 ew
Cr II 24.1 2 4.70 0.08 2 4.04 0.08 2 4.18 0.07 ew
Mn I 25.0 1 3.69 0.08 1 4.32 0.10 1 3.82 0.09 1 3.48 0.08 ew
Fe I 26.0 69 5.59 0.11 68 6.16 0.10 67 6.05 0.12 63 5.51 0.10 ew
Fe II 26.1 10 5.63 0.10 9 6.18 0.09 7 6.11 0.10 7 5.61 0.12 ew
Ni I 28.0 3 4.57 0.10 3 5.08 0.09 3 4.67 0.11 3 4.49 0.07 ew
Cu I 29.0 1 2.19 0.07 1 3.06 0.10 1 2.49 0.08 1 2.03 0.10 ew
Zn I 30.0 2 3.05 0.11 2 3.51 0.11 2 3.42 0.14 2 3.00 0.11 ew
Sr I 38.0 1 1.16 0.08 1 1.47 0.09 1 1.37 0.11 1 1.64 0.11 f
Ba II 56.1 2 0.87 0.08 3 1.18 0.09 2 1.57 0.10 2 1.05 0.13 f
Eu II 63.1 1 −0.49 0.07 1 −0.38 0.08 1 −0.98 0.08 1 −0.66 0.08 f
Gd II 64.1 1 −0.69 0.07 1 −0.58 0.08 1 −0.03 0.10 f

Notes. Values were derived from UVES spectra via equivalent width measurement (ew) or line fitting (f) using the atmospheric parameters derived using the seismic log(g).

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