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Table A.1

Stellar parameters and abundances from individual lines of Sr II, Ba II, and Eu II from MZ06 and Mashonkina et al. (2007).

Name Pop.* Teff, K log g [Fe/H] ξt, km s−1 [Mg/Fe] log ε
Ba II 4554 Ba II 5853 Ba II 6496 Sr II 4215 Eu II 4129
r, NLTE sol., NLTE NLTE LTE NLTE LTE NLTE LTE NLTE LTE
HD 65583 t 5320 4.55 −0.73 0.80 0.39 1.41 1.49 1.43 1.46 1.44 1.54 2.20 2.21 0.27 0.23
HD 62301 t 5940 4.06 −0.69 1.30 0.30 1.38 1.56 1.48 1.54 1.43 1.65 2.18 2.25 0.21 0.15
HD 30649 t 5820 4.28 −0.47 1.20 0.35 1.60 1.68 1.65 1.72 1.62 1.82 2.34 2.36 0.39 0.35
72 Her t 5735 4.24 −0.34 1.00 0.38 1.71 1.83 1.74 1.81 1.74 1.94 2.52 2.54 0.54 0.51
HD 69611 t 5820 4.18 −0.60 1.20 0.43 1.39 1.55 1.52 1.57 1.48 1.69 2.35 2.37 0.30 0.26
HD 102158 t 5760 4.24 −0.46 1.10 0.40 1.63 1.70 1.63 1.70 1.61 1.83 2.44 2.46 0.42 0.38
HD 22879 t 5870 4.27 −0.86 1.20 0.44 1.24 1.39 1.34 1.37 1.31 1.48 2.13 2.17 0.10 0.04
HD 201891 t 5940 4.24 −1.05 1.20 0.41 1.05 1.20 1.10 1.10 1.11 1.21 1.85 1.89 −0.09 −0.16
HD 84937 h 6350 4.03 −2.07 1.70 0.36 0.12 0.19 0.14 −0.04 0.73 0.69 −0.96 −1.12
HD 68017 t 5630 4.45 −0.40 0.90 0.34 1.59 1.73 1.69 1.74 1.69 1.84 2.43 2.45 0.42 0.38
HD 45282 h 5280 3.12 −1.52 1.40 0.37 0.62 0.81 0.64 0.66 0.59 0.79 1.32 1.36 −0.38 −0.44
HD 18757 t 5710 4.34 −0.28 1.00 0.32 1.69 1.85 1.82 1.88 1.81 1.98 2.56 2.58 0.51 0.47
HD 3795 t 5370 3.82 −0.64 1.00 0.39 1.59 1.68 1.59 1.68 1.58 1.79 2.32 2.34 0.46 0.43
HD 103095 h 5110 4.66 −1.35 0.85 0.28 0.80 0.90 0.85 0.84 0.87 0.91 1.46 1.47 −0.26 −0.29
HD 194598 h 6060 4.27 −1.12 1.45 0.29 0.95 1.12 1.11 1.09 1.01 1.08 1.69 1.75 −0.00 −0.07
HD 37124 t 5610 4.44 −0.44 0.90 0.32 1.56 1.66 1.66 1.71 1.63 1.78 2.39 2.41 0.40 0.36
HD 10519 t 5710 4.00 −0.64 1.10 0.43 1.50 1.63 1.53 1.59 1.51 1.71 2.33 2.34 0.28 0.24
HD 222794 t 5620 3.94 −0.69 1.20 0.40 1.34 1.47 1.41 1.48 1.44 1.65 2.25 2.26 0.23 0.18
HD 64606 t 5320 4.54 −0.89 0.95 0.37 1.15 1.28 1.25 1.27 1.20 1.29 1.99 2.01 0.14 0.10
HD 132142 t 5240 4.58 −0.39 0.70 0.31 1.67 1.75 1.73 1.76 1.73 1.83 2.41 2.42 0.41 0.38
HD 112758 t 5240 4.62 −0.43 0.70 0.36 1.60 1.68 1.64 1.67 1.66 1.76 2.34 2.35 0.39 0.36
HD 144579 t 5330 4.59 −0.69 0.80 0.38 1.45 1.48 1.44 1.48 2.16 2.17 0.31 0.28
HD 148816 t 5880 4.07 −0.78 1.20 0.41 1.21 1.37 1.30 1.35 1.29 1.49 2.07 2.09 0.06 0.00
HD 193901 h 5780 4.46 −1.08 0.90 0.18 1.07 1.19 1.12 1.13 1.06 1.16 1.70 1.73 −0.10 −0.16

1 – ’t’ and ’h’ stellar population types correspond to the thick disc and halo, respectively.

Here we present the digitalised hand-written line-by-line abundances used for average abundance calculations in MZ06 and Mashonkina et al. (2007). We only include MP stars where abundances of the three elements: Sr, Ba, and Eu, are available.

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