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Table A.6.
Iron lines observed in EBIT-I within the wavelength band λ320–λ350.
| Known lines | ||||||
|---|---|---|---|---|---|---|
| XIII | 3s–3p | 0.8 | 320.7 | 100 | 320.8000 | 320.800 |
| XIII | 3s–3p | … | … | … | 321.4660 | 321.455 |
| XV | 3s–3p | 0.2 | 321.7 | 150 | 321.7690 | … |
| XII | 3s–3p | … | … | … | 323.4110 | … |
| XVII | 3s–3p | 0.2 | 323.6 | 150 | 323.4880 | 323.65 |
| XI | 3s–3p | 0.2 | 326.4 | 150 | 326.3230 | … |
| XV | 3s–3p | 0.2 | 327.0 | 150 | 327.0330 | … |
| XIII | 3s–3p | … | … | … | 328.9410 | … |
| IX | 3s–3p | 0.2 | 329.8 | 100 | 329.8970 | … |
| XIII | 3s–3p | … | … | … | 332.0250 | … |
| XII | 3s–3p | … | … | … | 333.1550 | 333.181 |
| XIV | 3s–3p | 0.8 | 334.1 | 100 | 334.1783 | 334.171 |
| IX | 3s–3p | Blended | … | … | 335.2900 | … |
| XII | 3s–3p | Blended | … | … | 335.3800 | 335.06 |
| XVI | 3s–3p | 10 | 335.3 | 100 | 335.4090 | 335.409 |
| XXI | 2s–2p | … | … | … | 335.6925 | 335.514 |
| X | 3s–3p | 0.6 | 337.2 | 100 | 337.2350 | … |
| XII | 3s–3p | … | … | … | 338.2630 | 338.263 |
| X | 3s–3p | 0.3 | 339.5 | 150 | 339.4340 | … |
| IX | 3s–3p | 0.3 | 339.7 | 150 | 339.8370 | … |
| XVII | 3s–3p | … | … | … | 340.1220 | 340.12 |
| XII | 3s–3p | 0.3 | 340.3 | 150 | … | 340.200 |
| XVII | 3s–3p | … | … | … | 340.4950 | … |
| XII | 3s–3p | Blended | … | … | 340.5570 | … |
| XI | 3s–3p | 0.3 | 341.1 | 150 | … | 341.113 |
| IX | 3s–3p | … | … | … | 341.1590 | … |
| IX | 3s–3p | … | … | … | 341.3960 | … |
| IX | 3s–3p | 4.5 | 342.3 | 100 | 171.0733 (II) | 171.073 (II) |
| X | 3s–3p | 3.9 | 345.7 | 100 | 345.7380 | 345.723 |
| XII | 3s–3p | 0.3 | 346.7 | 150 | 346.8520 | 346.852 |
| XVII | 3s–3p | 0.5 | 347.8 | 100 | 347.8160 | … |
| IX | 3s–3p | 0.2 | 348.1 | 150 | 348.1230 | … |
| XIII | 3s–3p | Blended | 348.1 | 100 | 348.1830 | 348.184 |
| XI | 3s–3p | Blended | … | … | 349.0460 | 349.046 |
| X | 3p–3d | 0.3 | 349.2 | 100 | 174.5310 (II) | 174.534 (II) |
| X | 3s–3p | … | … | … | 349.3020 | … |
| Unidentified lines | ||||||
| ≤XXI | … | 0.04 | 331.8 | 200 | … | … |
| ≤XXI | … | 0.3 | 332.7 | 150 | … | … |
| ≤XVII | … | 1.7 | 336.3 | 100 | … | … |
| ≤XII | … | 1.2 | 336.9 | 100 | … | … |
| ≤XVII | … | 0.8 | 337.9 | 100 | … | … |
| ≤XII | … | 4.1 | 341.9 | 100 | … | … |
| ≤XII | … | 2.6 | 348.9 | 100 | … | … |
Notes. The other about 90 lines named in the literature are too weak individually to be distinguished in our spectra.
References.
(a)
From the CHIANTI database v.8 (Del Zanna et al. 2015);
(b)
from the online database at NIST (Kramida et al. 2015).
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