Table A.1.
Line parameters of the Fe I lines.
| Element | Wavelength | log (gf) | Broadening | α |
|---|---|---|---|---|
| (Å) | by H a | |||
| Fe | 15485.454 3 | -0.828 3* | -7.290 | |
| 15490.881 3 | 0.789 3 | 1618 1 | 0.325 | |
| 15500.799 3 | 0.789 3* | 1772 1 | 0.320 | |
| 15501.320 3 | 0.789 3* | 1620 1 | 0.325 | |
| 15502.174 3 | -1.034 3* | 1876 1 | 0.317 | |
| 15662.013 3 | 0.145 3* | 1326 2 | 0.235 | |
| 15878.444 3 | -0.339 3* | -7.450 | ||
| 16153.247 3 | -0.682 3* | 924 2 | 0.229 | |
| 16165.029 3 | 0.782 3* | 1598 2 | 0.325 | |
| 16171.930 3 | -0.399 3* | 1858 2 | 0.373 | |
| 16174.975 3 | 0.201 3* | 1861 1 | 0.316 | |
| 16177.085 3 | -1.089 3* | -7.330 | ||
| 16179.583 3 | 0.118 3* | 1600 1 | 0.325 | |
| 16180.900 3 | 0.203 3* | 1431 1 | 0.329 | |
| 16182.170 3 | -0.805 3* | 1599 1 | 0.325 | |
| 16185.799 3 | 0.211 3* | 1919 1 | 0.313 | |
| 16245.763 3 | -0.652 3* | 1602 1 | 0.325 | |
| 16246.458 4 | -0.106 3* | 1419 1 | 0.329 | |
| 16258.912 3 | -0.825 3* | -7.290 | ||
| 16316.320 3 | 0.887 3* | 1424 1 | 0.329 | |
| 16318.690 3 | -0.436 3* | -7.550 | ||
| 16324.451 3 | -0.522 3* | 936 1 | 0.229 | |
| 16331.524 3 | -0.506 3* | -7.470 | ||
| 16333.141 3 | -1.356 3* | -7.450 | ||
| 16517.223 3 | 0.572 3* | 1414 1 | 0.329 | |
| 16612.761 3 | 0.018 3* | 1846 1 | 0.315 | |
| 16619.737 3 | -1.524 3* | 1082 1 | 0.228 | |
| 16783.037 3 | -0.695 3* | 1409 1 | 0.329 | |
| 16792.224 3 | -0.890 3* | 1588 1 | 0.324 | |
| 16794.210 3 | -0.362 3* | -7.430 |
Notes. a: Collisional broadening by neutral hydrogen gives either the broadening cross section σ(v = 104m/s) in atomic units (
), with the velocity parameter α (see text for more details), or, if the value is negative and no α is given, then the line width is given in the standard form logΓ/NH at T = 10000 K, where Γ is the full width at half maximum in rad/s and NH is in cm−3. 1: BSYN based on routines from the MARCS code (Gustafsson et al. 2008), 2: Paul Barklem (private communication), 3: Kurucz (2014), 4: Biemont et al. (1985), and the asterisk indicates an astrophysical estimate.
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