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Table 2
List of Fe, Ca, Ni, Ba, Eu, and La lines used in this analysis.
| Wavelength (Å) | Species | χ (eV) | log gf | Reference | Method | Sol* |
|
|
||||||
| 6439.0700 | 20.0 | 2.526 | 0.470 | NIST | SS | 6.41 |
| 6471.6600 | 20.0 | 2.526 | –0.590 | NIST | SS | ′′ |
| 6318.0171 | 26.0 | 2.453 | –1.804 | NIST | EW | 7.54 |
| 6322.6851 | 26.0 | 2.588 | –2.426 | NIST | EW | ′′ |
| 6335.3304 | 26.0 | 2.198 | –2.177 | NIST | EW | ′′ |
| 6336.8239 | 26.0 | 3.686 | –0.856 | NIST | EW | ′′ |
| 6344.1487 | 26.0 | 2.433 | –2.923 | NIST | EW | ′′ |
| 6355.0286 | 26.0 | 2.845 | –2.291 | NIST | EW | ′′ |
| 6393.6009 | 26.0 | 2.433 | –1.576 | NIST | EW | ′′ |
| 6408.0179 | 26.0 | 3.686 | –1.018 | NIST | EW | ′′ |
| 6411.6489 | 26.0 | 3.654 | –0.718 | NIST | EW | ′′ |
| 6421.3504 | 26.0 | 2.279 | –2.027 | NIST | EW | ′′ |
| 6430.8460 | 26.0 | 2.176 | –2.006 | NIST | EW | ′′ |
| 6475.6240 | 26.0 | 2.559 | –2.942 | NIST | EW | ′′ |
| 6481.8699 | 26.0 | 2.279 | –2.984 | NIST | EW | ′′ |
| 6518.3667 | 26.0 | 2.832 | –2.298 | NIST | EW | ′′ |
| 6575.0154 | 26.0 | 2.588 | –2.710 | NIST | EW | ′′ |
| 6592.9134 | 26.0 | 2.728 | –1.473 | NIST | EW | ′′ |
| 6593.8701 | 26.0 | 2.433 | –2.422 | NIST | EW | ′′ |
| 6432.6800 | 26.1 | 2.891 | –3.500 | NIST | EW | ′′ |
| 6456.3760 | 26.1 | 3.903 | –2.190 | NIST | EW | ′′ |
| 6516.0530 | 26.1 | 2.891 | –3.372 | NIST | EW | ′′ |
| 6643.6300 | 28.0 | 1.675 | –2.300 | NIST | SS | 6.29 |
| 6496.8980 | Ba II | 0.604 | –0.407 | D12a | SS | 2.25 |
| 6390.4770 | La II | 0.321 | –1.410 | L01aa | SS | 1.25 |
| 6437.6400 | Eu II | 1.320 | –0.320 | L01bb | SS | 0.60 |
| 6645.1270 | Eu II | 1.380 | 0.120 | L01bc | SS | ′′ |
Notes.Includes the associated excitation potential (χ), log gf, the method of analysis used: spectrum synthesis (SS) or equivalent width curve of growth (EW), and reference solar abundances.
(*)
Solar reference abundances taken from Lodders (2003).
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