Table C.1.
Used linelist.
| Element | Wavelength [Å] | Excitation potential [eV] | log(gf) | Weights | # Stars | Lit. |
|---|---|---|---|---|---|---|
| Mg I | 5183.60 | 2.700 | −0.17 | 1.0 | 49 | 1 |
| Mg I | 5528.48 | 4.330 | −0.51 | 1.0 | 348 | 1 |
| Mg I | 6318.72 | 5.104 | −2.02 | 1.0 | 138 | 1 |
| Mg I | 6319.24 | 5.104 | −2.24 | 1.0 | 138 | 1 |
| Mg I | 6319.50 | 5.104 | −2.72 | 1.0 | 138 | 1 |
| Sc II | 5526.80 | 1.767 | 0.13 (HFS) | 1.0 | 319 | 2 |
| Sc II | 6309.90 | 1.496 | −1.52 (HFS) | 1.0 | 128 | 2 |
| Ti II | 5418.77 | 1.582 | −2.13 | 1.0 | 293 | 3 |
| Ti II | 6606.95 | 2.060 | −2.79 | 1.0 | 104 | 4 |
| Cr I | 5409.77 | 1.029 | −0.67 | 1.0 | 270 | 5 |
| Cr I | 6330.09 | 0.941 | −2.92 | 1.0 | 147 | 5 |
| Mn I | 5420.36 | 2.141 | −1.46 (HFS) | 1.0 | 210 | 6 |
| Mn I | 5432.55 | 0.000 | −3.80 (HFS) | 1.0 | 230 | 6 |
| Mn I | 6013.51 | 3.070 | −0.35 (HFS) | 1.0 | 36 | 7 |
| Mn I | 6021.82 | 3.073 | −0.05 (HFS) | 1.0 | 36 | 7 |
| Ni I | 5476.92 | 1.825 | −0.89 | 0.3 | 351 | 8 |
| Ni I | 6176.82 | 4.085 | −0.26 | 1.0 | 133 | 9 |
| Ni I | 6177.25 | 1.825 | −3.51 | 1.0 | 126 | 10 |
| Ni I | 6643.56 | 1.676 | −2.30 | 0.5 | 335 | 11 |
| Zn I | 4810.54 | 4.075 | −0.17 | 1.0 | 113 | 12 |
| Sr II | 4077.71 | 0.000 | 0.16 (HFS) | 1.0 | 26 | 13 |
| Sr II | 4215.52 | 0.000 | −0.16 (HFS) | 1.0 | 36 | 13 |
| Y II | 4883.68 | 1.084 | 0.07 | 1.0 | 131 | 6 |
| Y II | 5402.78 | 1.838 | −0.51 | 1.0 | 97 | 6 |
| Ba II | 5853.69 | 0.604 | −1.01 (HFS) | 1.0 | 60 | 14 |
| Ba II | 6141.73 | 0.704 | −0.08 (HFS) | 0.5 | 332 | 14 |
| Ba II | 6496.90 | 0.604 | −0.38 (HFS) | 1.0 | 340 | 14 |
| Eu II | 4205.05 | 0.000 | 0.21 (HFS) | 1.0 | 31 | 2 |
| Eu II | 6645.21 | 1.379 | 0.12 (HFS) | 1.0 | 181 | 2 |
Notes. The first column lists the element together with the ionization state, and the second column the wavelength of the absorption line. The third and fourth column show excitation potential and oscillator strength, respectively. The fifth column contains the weight given to the abundance of the absorption feature. The final two columns show the number of stars for that we measured this absorption feature and the source of the atomic data.
References. (1) Pehlivan Rhodin et al. (2017); (2) Lawler & Dakin (1989); (3) Wood et al. (2013); (4) Martin et al. (1988); (5) Sobeck et al. (2007); (6) Kurucz (2011); (7) Den Hartog et al. (2011); (8) Roederer & Lawler (2012); (9) Wood et al. (2014); (10) Kostyk (1982); (11) Lennard et al. (1975); (12) Biemont & Godefroid (1980) (13) Bergemann et al. (2012); (14) Gallagher et al. (2012).
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