Table B.1
Spectroscopic parameters used in the radiative transfer of the CH (J = 6 − 5) multiplet.
| Eu | E1 [cm−1] | ΔE | AE [s−1] | Ju | gu | J1 | g1 |
|---|---|---|---|---|---|---|---|
| 219.915010 | 157.138882 | 62.776128 | 1.5609 × 10−8 | 6 | 39 | 5 | 33 |
| 219.913337 | 157.137091 | 62.776246 | 2.0894 × 10−8 | 6 | 26 | 5 | 22 |
| 219.915010 | 157.124300 | 62.790710 | 1.3265 × 10−9 | 6 | 39 | 5 | 33 |
| 219.936727 | 157.138882 | 62.797845 | 6.6280 × 10−9 | 6 | 39 | 5 | 33 |
| 219.936727 | 157.124300 | 62.812427 | 1.4037 × 10−9 | 6 | 39 | 5 | 33 |
| 219.941223 | 157.127890 | 62.813333 | 2.6164 × 10−9 | 6 | 39 | 5 | 33 |
Notes. Energy levels and Einstein coefficients are from Yurchenko et al. (2024, computed). Pressure-induced broadening parameters for collisions with H2 are γL,0 = 0.015 cm−1 atm−1 and n = 0.84. Spectra were synthesized both without pressure-induced line shift and with (adopting the parameters for HD). For details see text.
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