Open Access
Table 1.
Main properties of spectral features used to compute stellar abundances with SME.
| Element | Ion | λ, Å | log(gf) | Elow, eV | Eup, eV |
|---|---|---|---|---|---|
| Fe | 1 | 5339.929 | −0.667 | 3.266 | 5.587 |
| Fe | 1 | 5364.871 | 0.228 | 4.446 | 6.756 |
| Fe | 1 | 5373.709 | −0.760 | 4.473 | 6.780 |
| Fe | 1 | 5379.574 | −1.514 | 3.695 | 5.999 |
| Fe | 1 | 5389.479 | −0.410 | 4.415 | 6.715 |
| Fe | 1 | 5393.167 | −0.715 | 3.241 | 5.539 |
| Fe | 1 | 5398.279 | −0.630 | 4.446 | 6.742 |
| Fe | 1 | 5434.524 | −2.121 | 1.011 | 3.292 |
| Fe | 1 | 5445.042 | −0.020 | 4.387 | 6.663 |
| Fe | 1 | 5506.779 | −2.795 | 0.990 | 3.241 |
| Fe | 1 | 5560.212 | −1.090 | 4.435 | 6.664 |
| Fe | 1 | 5587.574 | −1.750 | 4.143 | 6.361 |
| Fe | 1 | 6494.980 | −1.268 | 2.404 | 4.313 |
| Fe | 1 | 6593.870 | −2.420 | 2.433 | 4.313 |
| Fe | 1 | 6710.318 | −4.764 | 1.485 | 3.332 |
| Fe | 2 | 5425.249 | −3.220 | 3.199 | 5.484 |
| Fe | 2 | 6516.077 | −3.310 | 2.891 | 4.793 |
| Ca | 1 | 5349.465 | −0.310 | 2.709 | 5.026 |
| Ca | 1 | 5512.980 | −0.464 | 2.933 | 5.181 |
| Ca | 1 | 5581.965 | −0.555 | 2.523 | 4.744 |
| Ca | 1 | 5588.749 | 0.358 | 2.526 | 4.744 |
| Ca | 1 | 5590.114 | −0.571 | 2.521 | 4.739 |
| Ca | 1 | 5594.462 | 0.097 | 2.523 | 4.739 |
| Ca | 1 | 5601.277 | −0.523 | 2.526 | 4.739 |
| Ca | 1 | 5602.842 | −0.564 | 2.523 | 0.000 |
| Ca | 1 | 6471.662 | −0.686 | 2.526 | 4.441 |
| Ca | 1 | 6499.650 | −0.818 | 2.523 | 4.430 |
| Mg | 1 | 5528.405 | −0.498 | 4.346 | 6.588 |
| Li | 1 | 6707.764 | −0.002 | 0.000 | 1.848 |
| Li | 1 | 6707.915 | −0.303 | 0.000 | 1.848 |
| Li | 1 | 6707.922 | −1.122 | 0.000 | 0.000 |
| Li | 1 | 6708.073 | −1.423 | 0.000 | 0.000 |
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