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Table 1
Diagnostic Y II and Eu II lines used for the solar-abundance analysis in this work.
| λ [Å] | States | Elow [eV] | Eup [eV] | log g f |
|---|---|---|---|---|
| Y II | ||||
| 4883.682 |  |
1.08 | 3.62 | 0.15 |
| 4900.118 |  |
1.03 | 3.56 | −0.02 |
| 5087.418 |  |
1.08 | 3.52 | −0.18 |
| 5200.406 |  |
0.99 | 3.38 | −0.62 |
| Eu II | ||||
| 6645.104 |  |
1.38 | 3.24 | 0.12 |
Notes. The log g f values are adopted from Palmeri et al. (2017, their uncorrected values) for Y and from Lawler et al. (2001) for Eu.
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