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Table A.1

Lines used in the abundance analysis.

Elem. λ [Å] χ [eV] log gf Weq       ⊙ [mÅ]

Li I 6707.761 0.00 0.167 4.1 synth
C I 5380.337 7.68 1.842 23.8 b
O I 6158.186 10.74 0.409 4.8 siu
O I 6300.304 0.00 9.819 6.2 siu
Na I 6154.226 2.10 1.560 40.6 b
Na I 6160.747 2.10 1.260 62.2 b
Mg I 5711.088 4.35 1.833 108.0 s
Mg I 5183.604 2.72 0.180 s,synth
Al I 6696.185 4.02 1.576 39.4 b
Al I 6698.673 3.14 1.647 22.4 b
Si I 5665.555 4.92 2.040 42.9
Si I 5690.425 4.93 1.870 53.3
Si I 6125.021 5.61 1.464 35.2
Si I 6131.852 5.62 1.615 26.0 b
Si I 6721.848 5.86 1.516 49.7
S I 6046.027 7.87 1.030 11.6 b
S I 6052.674 7.87 0.740 13.4
S I 6757.171 7.87 0.310 15.6 b
Ca I 5590.114 2.52 0.571 96.2 b,s
Ca I 5867.562 2.93 1.570 27.9
Ca I 6166.439 2.52 1.142 73.8 s
Ca I 6169.042 2.52 0.797 100.2 b,s
Sc II 5684.202 1.51 1.074 39.4 b
Sc II 6245.637 1.51 1.030 36.6 b
Ti I 5219.702 0.02 2.292 30.2 b
Ti I 6126.216 1.07 1.425 24.1
Ti I 6258.102 1.44 0.355 52.9
Ti II 5490.690 1.57 2.430 23.6
Ti II 6491.561 2.06 1.793 41.4 b
V I 5670.853 1.08 0.420 20.3
V I 6090.214 1.08 0.062 35.7
Cr I 5238.961 2.71 1.305 18.2 b
Cr I 5287.178 3.44 0.907 12.4 b
Mn I 5377.637 3.84 0.109 50.3
Fe I 5295.312 4.41 0.967 91.4 b
Fe I 5522.446 4.21 1.514 65.2
Fe I 6151.617 2.18 1.530 125.4
Fe I 6229.226 2.85 2.482 84.7
Fe I 6498.938 0.96 2.027 108.6 b
Fe II 5414.073 3.22 3.645 32.0 b
Co I 5342.695 4.02 0.690 35.4 b
Co I 5530.774 1.71 2.060 17.2 b
Co I 5647.234 2.28 1.560 14.8
Ni I 5589.357 3.90 1.140 31.2 b
Ni I 6086.276 4.27 0.530 46.2 b
Ni I 6130.130 4.27 0.960 23.4
Ni I 6204.600 4.09 1.100 23.2
Ni I 6223.981 4.11 0.910 29.6
Ni I 6772.313 3.66 0.980 52.7
Cu I 5218.197 3.82 0.476 58.0 b,s
Cu I 5220.066 3.82 0.448 15.2 b
Y II 4900.120 1.03 0.090 59.2 b,s
Y II 5087.416 1.08 0.170 50.6 b,s

Notes. Column description (left to right): Atomic element, wavelength, excitation energy, oscillator strength according to VALD, measured equivalent width from the Kitt Peak Solar Atlas, comments. b: blend in wing(s), parts of line used to calculate Weq; s: strong- or intermediate strong line in stellar spectra, log   (Weq/λ) > −5; synth: abundance determined directly from synthetic fit; siu: abundance determination and synthetic fit made in SIU.

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