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Table A.1

Line data for spectral lines used in the abundance analyses.

Wavelength Transition Jlow–Jupp E low log gf a Ref. Γ6
[Å] [eV] [dex] σ [a.u.] α
2103.017 3p 2P0  – 14d 2D 3/2 –5/2 0.014 −1.619 1
2103.024 3p 2P0  – 14d 2D 3/2 –3/2 0.014 −2.566 1
2118.312 3p 2P0  – 11d 2D 1/2 –3/2 0.000 −1.557  ± 0.10 2
2134.732 3p 2P0  – 10d 2D 3/2 –5/2 0.014 −1.129  ± 0.10 2
2134.760 3p 2P0  – 10d 2D 3/2 –3/2 0.014 −2.090  ± 0.18 2
2145.555 3p 2P0  – 9d 2D 1/2 –3/2 0.000 −1.244  ± 0.10 2
2174.027 3p 2P0  – 8d 2D 3/2 –5/2 0.014 −0.824  ± 0.10 2
2174.113 3p 2P0  – 8d 2D 3/2 –3/2 0.014 −1.778  ± 0.30 2
2204.590 3p 2P0  – 8s 2S 3/2 –1/2 0.014 −2.293  ± 0.10 2
2204.660 3p 2P0  – 7d 2D 1/2 –3/2 0.000 −0.895  ± 0.06 2 2340 1.07
2210.046 3p 2P0  – 7d 2D 3/2 –5/2 0.014 −0.641  ± 0.06 2 2340 1.07
2210.130 3p 2P0  – 7d 2D 3/2 –3/2 0.014 −1.595  ± 0.06 2 2340 1.07
2269.096 3p 2P0  – 6d 2D 3/2 –5/2 0.014 −0.454  ± 0.04 2, 3 2084 0.960
2269.220 3p 2P0  – 6d 2D 3/2 –3/2 0.014 −1.409  ± 0.06 3 2084 0.960
2367.052 3p 2P0  – 5d 2D 1/2 –3/2 0.000 −0.592  ± 0.06 2
2372.070 3p 2P0  – 6s 2S 1/2 –1/2 0.000 −2.012  ± 0.10 2
2373.124 3p 2P0  – 5d 2D 3/2 –5/2 0.014 −0.337  ± 0.04 2
2373.349 3p 2P0  – 5d 2D 3/2 –3/2 0.014 −1.291  ± 0.06 2
2567.984 3p 2P0  – 4d 2D 1/2 –3/2 0.000 −1.119  ± 0.04 3 1385 0.249
2575.094 3p 2P0  – 4d 2D 3/2 –5/2 0.014 −0.668  ± 0.06 2, 3 1387 0.249
2575.393 3p 2P0  – 4d 2D 3/2 –3/2 0.014 −1.623  ± 0.06 3 1385 0.249
2652.484 3p 2P0  – 5s 2S 1/2 –1/2 0.000 −1.523  ± 0.04 4 2150 0.307
2660.392 3p 2P0  – 5s 2S 3/2 –1/2 0.014 −1.219  ± 0.04 4 2150 0.307
3082.153 3p 2P0  – 3d 2D 1/2 –3/2 0.000 −0.476  ± 0.025 2, 3 576 0.292
3092.710 3p 2P0  – 3d 2D 3/2 –5/2 0.014 −0.202  ± 0.025 2, 5 576 0.292
3092.839 3p 2P0  – 3d 2D 3/2 –3/2 0.014 −1.175  ± 0.04 2 576 0.292
3944.006 3p 2P0  – 4s 2S 1/2 –1/2 0.000 −0.635  ± 0.025 2, 5 655 0.243
3961.520 3p 2P0  – 4s 2S 3/2 –1/2 0.014 −0.333  ± 0.025 2 655 0.243
6696.015 4s 2S  – 5p 2P0 1/2 –3/2 3.143 −1.569  ± 0.06 2 1860 0.226
6698.672 4s 2S  – 5p 2P0 1/2 –1/2 3.143 −1.870  ± 0.06 2 1860 0.226
7835.309 3d 2D  – 6f 2F0 3/2 –5/2 4.022 −0.689  ± 0.04 2 3850 1.60
7836.134 3d 2D  – 6f 2F0 5/2 –5/2 4.022 −1.834  ± 0.06 2 3850 1.60
7836.134 3d 2D  – 6f 2F0 5/2 –7/2 4.022 −0.534  ± 0.025 2 3850 1.60
8772.866 3d 2D  – 5f 2F0 3/2 –5/2 4.022 −0.349  ± 0.025 2 2983 0.344
8773.895 3d 2D  – 5f 2F0 5/2 –5/2 4.022 −1.495  ± 0.06 2 2983 0.344
8773.895 3d 2D  – 5f 2F0 5/2 –7/2 4.022 −0.192  ± 0.025 2 2983 0.344
8912.900 4p 2P0  – 6d 2D 1/2 –3/2 4.085 −1.963  ± 0.06 2
8923.555 4p 2P0  – 6d 2D 3/2 –5/2 4.087 −1.709  ± 0.06 2
8925.503 4p 2P0  – 6d 2D 3/2 –3/2 4.087 −2.663 2
10768.363 4p 2P0  – 5d 2D 1/2 –3/2 4.085 −2.020  ± 0.06 2
10782.046 4p 2P0  – 5d 2D 3/2 –5/2 4.087 −1.764  ± 0.06 2
10786.770 4p 2P0  – 5d 2D 3/2 –3/2 4.087 −2.719  ± 0.10 2
10872.975 4p 2P0  – 6s 2S 1/2 –1/2 4.085 −1.326  ± 0.06 2
10891.732 4p 2P0  – 6s 2S 3/2 –1/2 4.087 −1.027  ± 0.04 2
13123.416 4s 2S  – 4p 2P0 1/2 –3/2 3.143 0.219  ± 0.013 2 815 0.223
13150.753 4s 2S  – 4p 2P0 1/2 –1/2 3.143 −0.083  ± 0.013 2 815 0.223
16718.974 4p 2P0  – 4d 2D 1/2 –3/2 4.085 0.220  ± 0.013 2 1147 0.311
16750.519 4p 2P0  – 4d 2D 3/2 –5/2 4.087 0.474  ± 0.013 2 1147 0.311
16763.369 4p 2P0  – 4d 2D 3/2 –3/2 4.087 −0.480  ± 0.025 2 1147 0.311
21093.082 4p 2P0  – 5s 2S 1/2 –1/2 4.085 −0.398  ± 0.025 4 1838 0.279
21163.803 4p 2P0  – 5s 2S 3/2 –1/2 4.087 −0.093  ± 0.025 4 1838 0.279
21208.171 4f 2F0  – 7g 2G 7/2 –9/2 5.123 −0.307 2 3260 1.68
21208.171 4f 2F0  – 7g 2G 5/2 –7/2 5.123 −0.461 2 3260 1.68
21208.191 4f 2F0  – 7g 2G 7/2 –7/2 5.123 −1.608 2 3260 1.68
123349.6b 6h 2H0  – 7i 2I 5.614 1.647 6 4830 1.84

Notes. Only lines used in the spectrum analyses are listed.

(a)

Uncertainties (90%) to the transition probabilities are taken from Kelleher & Podobedova (2008), when available.

(b)

Multiplet components with identical wavelength have been merged. We adopt the wavelength measured from the solar spectrum by Brault & Noyes (1983), and the oscillator strength has been adjusted accordingly.

Reference. (1) Wiese et al. (1969); (2) TOPbase: Mendoza et al. (1995) and C. Mendoza, W. Eissner, M. Le Dourneuf, & C. J. Zeippen (unpublished); (3) Davidson et al. (1990); (4) Vujnović et al. (2002); (5) Tachiev & Froese Fischer (2002); (6) Kurucz (2012, online data; http://kurucz.harvard.edu/atoms/1300/).

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