Table 1
Ba II lines used in the abundance analysis of the Sun.
| Wavelength (Å) | Elow (eV) | Eup (eV) | Conf. | Conf. | log gf | VdW | EW (mÅ) |
|---|---|---|---|---|---|---|---|
| 4554.033 | 0.00 | 2.72 |  |
 |
0.170 ± 0.004 | 303.222 | 207 |
| 5853.675 | 0.60 | 2.72 |  |
 |
−1.023 ± 0.005 | 365.264 | 68 |
| 6141.713 | 0.70 | 2.72 |  |
 |
−0.070 ± 0.005 | 365.264 | 126 |
| 6496.898 | 0.60 | 2.51 |  |
 |
−0.365 ± 0.004 | 365.264 | 102 |
Notes. The wavelengths are given in air. The equivalent widths correspond to the measurements in the solar KPNO flux atlas and are given in mÅ. The Van der Waals broadening parameters are taken from Barklem et al. (2000). The log gf values reported here are derived from the very accurate transition probabilities taken from De Munshi et al. (2015) and Dutta et al. (2016).
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