Table 3.
Line properties from our observations.
Line | νrest | Iline | FWHM | Lmol (a) | Lmol (b) |
---|---|---|---|---|---|
[GHz] | [Jy km s−1] | [km s−1] | [109 L⊙] | [109 L⊙] | |
CO(5–4) | 576.26 | 1.4 ± 0.30 | 278 ± 46 | 0.066 ± 0.014 | 0.063 ± 0.02 |
CO(7–6) | 806.65 | 1.7 ± 0.18 | 82 ± 48 | 0.12 ± 0.012 | 0.10 ± 0.01 |
259 ± 20 | |||||
CO(12–11) | 1381.95 | 2.0 ± 0.18 | 258 ± 17 | 0.24 ± 0.02 | 0.22 ± 0.02 |
[C I] | 809.34 | 0.36 ± 0.30 | 195 ± 123 | 0.024 ± 0.020 | |
[C II] | 1900.54 | 15.45 ± 1.5 | 182 ± 5 | 2.5 ± 0.23 | 2.3 ± 0.19 |
410 ± 21 | |||||
H2O(211 − 202) | 752.03 | 0.31 ± 0.12 | 257 ± 74 | 0.020 ± 0.0075 | |
OH(c) | 1834.75 | 1.78 ± 0.13 | 270 ± 15 | 1.1 ± 0.080 | |
OH(c) | 1837.75 | 1.90 ± 0.14 | 295 ± 16 | 1.1 ± 0.08 | |
OH+ | 1892.23 | 0.14 ± 0.04 | 275 ± 57 | 0.02 ± 0.006 |
Notes.
Corrected for lensing using μ = 3.92 from Kade et al. (2023).
Corrected for lensing using the per-channel magnification factor from the [C II] emission as described in Sect. 3.3.
As the OH line is a doublet, we fit it with two single Gaussian components with a fixed distance between peaks, see Sect. 3.2.3 for further discussion.
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