Table 2
Line transitions in the MIRI wavelength range included in the line radiative transfer.
| Species | Treatment | #lines | Reference |
|---|---|---|---|
| CO | NLTE | 123 | (1) |
| H2O | NLTE | 7370 | (2) |
| OH | NLTE | 219 | (3) |
| H2 | NLTE | 165 | (4,5) |
| O | NLTE | 30 | (2,6,7) |
| CH | NLTE | 4 | (2) |
| CH4 | LTE | 9662 | (8) |
| C2H2 | LTE | 26 457 | (8) |
| HCN | LTE | 5753 | (8) |
| CO2 | LTE | 5746 | (8) |
| NH3 | LTE | 8526 | (8) |
| SO2 | LTE | 8230 | (8) |
| NO | LTE | 4204 | (8) |
| O2 | LTE | 435 | (8) |
| Ne+ | NLTE | 1 | (9) |
| Ne++ | NLTE | 2 | (2) |
| Ar+ | NLTE | 1 | (2) |
| Ar++ | NLTE | 3 | (2) |
| CH+ | NLTE | 3 | (2) |
| Si+ | NLTE | 3 | (9) |
| SH+ | NLTE | 4 | (10) |
| Fe+ | NLTE | 10 | (9) |
| S++ | NLTE | 2 | (2) |
| S | NLTE | 2 | (2) |
| Total lines | 76 957 | ||
Notes. (1) Thi et al. (2013), (2) LAMDA (Schöier et al. 2005), (3) See Appendix A, (4) Wrathmall et al. (2007), (5) Lique (2015), (6) Kramida et al. (2024), (7) Wiese et al. (1996), (8) HITRAN (Gordon et al. 2022), (9) CHIANTI (Dere et al. 1997), (10) John Black (priv. commun.)
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