Table 1
Spectral line and dust continuum data in our study.
| Transition | Rest wavelength |  |
FWHM(b) | σs,med(c),(d),(e) | σf,med(f),(d),(e) | Reference |
|---|---|---|---|---|---|---|
| (μm) | (K) | (″) | (10−11 W m−2 sr−1) | (10−11 W m−2 sr−1) | ||
| 12CO J = 1–0 | 2600.8 | 6 | 45 | 0.1 | 0.1 | (1) |
| 12CO J = 3–2 | 867.0 | 33 | 22 | 2.2 | 5.1 | (2) |
| 12CO J = 4–3 | 650.3 | 55 | 42 | 24.0 | 26.5 | (3) |
| 12CO J = 5–4 | 520.2 | 83 | 34 | 15.9 | 20.7 | (3) |
| 12CO J = 6–5 | 433.6 | 116 | 29 | 9.2 | 16.7 | (3) |
| 12CO J = 7–6 | 371.7 | 155 | 33 | 7.4 | 18.4 | (3) |
| 12CO J = 8–7 | 325.2 | 199 | 33 | 18.7 | 25.3 | (3) |
| 12CO J = 9–8 | 289.1 | 249 | 19 | 25.2 | 30.2 | (3) |
| 12CO J = 10–9 | 260.2 | 304 | 18 | 27.6 | 30.6 | (3) |
| 12CO J = 11–10 | 236.6 | 365 | 17 | 28.7 | 32.2 | (3) |
| 12CO J = 12–11 | 216.9 | 431 | 17 | 26.6 | 30.3 | (3) |
| 12CO J = 13–12 | 200.3 | 503 | 17 | 39.8 | 43.0 | (3) |
| [C I] 3P1–3P0 | 609.1 | 24 | 38 | 28.3 | 29.2 | (3) |
| [C I] 3P2–3P1 | 370.4 | 62 | 33 | 7.0 | 7.9 | (3) |
| [C II] 2P3∕2–2P1∕2 | 157.7 | 91 | 12 | 294.6 | 8092.0 | (4) |
| [O I] 3P0–3P1 | 145.5 | 327 | 12 | 110.2 | 788.0 | (4) |
| [N II] 3P1–3P0 | 205.2 | 70 | 17 | 43.6 | 99.0 | (3) |
| H2 0–0 S(3) | 9.7 | 2504 | 6 | – | 1036.0 | (3,5) |
| FIR | 60–200 | – | 42 | – | 2.9 × 106 | (3,4) |
Notes. (a) Upper level energy. (b) Angular resolution of the original data. (c)Median σs (statistical 1σ uncertainty) on 42″ scales. (d) CO(1–0) is exceptionally on 45″ scales. (e)All pixels are considered. (f)Median σf (final 1σ uncertainty; statistical and calibration errors added in quadrature) on 42″ scales.
References.(1) Wong et al. (2011); (2) Minamidani et al. (2008); (3) this work; (4) Chevance et al. (2016); (5) Indebetouw et al. (2009).
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