Table D.1.
Overview of the number of levels and lines per ion handled in non-LTE in the calculated atmosphere models.
| Elem. | ion | levels | lines | Elem. | ion | levels | lines |
| H | I | 22 | 231 | Ne | VII | 1 | 0 |
| H | II | 1 | 0 | Al | II | 10 | 45 |
| He | I | 35 | 595 | Al | III | 10 | 45 |
| He | II | 26 | 325 | Al | IV | 10 | 45 |
| He | III | 1 | 0 | Al | V | 10 | 45 |
| N | I | 10 | 45 | Mg | I | 1 | 0 |
| N | II | 38 | 703 | Mg | II | 12 | 66 |
| N | III | 36 | 630 | Mg | III | 10 | 45 |
| N | IV | 38 | 703 | Mg | IV | 1 | 0 |
| N | V | 20 | 190 | Si | II | 1 | 0 |
| N | VI | 14 | 91 | Si | III | 24 | 276 |
| C | I | 15 | 105 | Si | IV | 23 | 253 |
| C | II | 32 | 496 | Si | V | 1 | 0 |
| C | III | 40 | 780 | P | IV | 12 | 66 |
| C | IV | 25 | 300 | P | V | 11 | 55 |
| C | V | 5 | 10 | P | VI | 1 | 0 |
| C | VI | 15 | 105 | S | III | 23 | 253 |
| O | I | 13 | 78 | S | IV | 11 | 55 |
| O | II | 37 | 666 | S | V | 10 | 45 |
| O | III | 33 | 528 | S | VI | 1 | 0 |
| O | IV | 25 | 300 | G(S) | I | 1 | 0 |
| O | V | 36 | 630 | G(S) | II | 3 | 2 |
| O | VI | 16 | 120 | G(S) | III | 13 | 40 |
| O | VII | 15 | 105 | G(S) | IV | 18 | 77 |
| Ne | I | 8 | 28 | G(S) | V | 22 | 107 |
| Ne | II | 1 | 0 | G(S) | VI | 29 | 194 |
| Ne | III | 18 | 153 | G(S) | VII | 19 | 87 |
| Ne | IV | 35 | 595 | G(S) | VIII | 14 | 49 |
| Ne | V | 54 | 1431 | G(S) | IX | 15 | 56 |
| Ne | VI | 49 | 1176 | G(S) | X | 1 | 0 |
Notes. Meta element containing the iron group elements Sc, Ti, V, Cr, Mn, Fe, Co, and Ni. The level and line numbers denote superlevels and superlines for this element, which are treated in non-LTE. Each superlevel contains a large set of explicit levels (of the same parity) within an energy band. Superlines describe the combined treatment of all transitions between two superlevels and contain a complex, pre-calculated cross section incorporating all explicit line transitions between levels within the two superlevels (see Gräfener et al. 2002, for more details).
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