Table A.1.
Fine-structure lines in the mid- to far-IR range.
Line | λ | ν | IP | E | ncr | Spec. res. | Ang. res. |
---|---|---|---|---|---|---|---|
(μm) | (GHz) | (eV) | (K) | (cm−3) | (km s−1) | (arcsec) | |
[Ne VI]2P3/2–2P1/2 | 7.65 | 39188.56 | 126.21 | 1888 | 2.5 × 105 | ∼1500 | 14 × 20 |
H2 (0,0) S(3) | 9.66 | 31034.41 | 4.48 | 2504 | 9 × 105(a) | ∼500 | 4.7 × 11.3 |
[S IV]2P3/2–2P1/2 | 10.51 | 28524.50 | 34.79 | 1369 | 5.39 × 104 | ∼500 | 4.7 × 11.3 |
H2 (0,0) S(2) | 12.28 | 24413.07 | 4.48 | 1682 | 2 × 105(a) | ∼500 | 4.7 × 11.3 |
[Ne II]2P1/2–2P3/2 | 12.81 | 23403.00 | 21.56 | 1123 | 7.00 × 105 | ∼500 | 4.7 × 11.3 |
[Ne V]3P2–3P1 | 14.32 | 20935.23 | 97.12 | 1892 | 3 × 104 | ∼500 | 4.7 × 11.3 |
[Ne III]3P1–3P2 | 15.56 | 19266.87 | 40.96 | 925 | 2.68 × 105 | ∼500 | 4.7 × 11.3 |
H2 (0,0) S(1) | 17.03 | 17603.78 | 4.48 | 1015 | 2 × 104(a) | ∼500 | 4.7 × 11.3 |
[S III]3P2–3P1 | 18.71 | 16023.11 | 23.34 | 769 | 2.22 × 104 | ∼500 | 4.7 × 11.3 |
[Ne V]3P1–3P0 | 24.32 | 12326.99 | 97.12 | 596 | 5.0 × 105 | ∼500 | 11.1 × 22.3 |
[O IV]2P3/2–2P1/2 | 25.89 | 11579.47 | 54.94 | 555 | 104 | ∼500 | 11.1 × 22.3 |
[Fe II]a6D7/2–a6D9/2 | 25.98 | 11539.35 | 7.9 | 553 | 2.2 × 106 | ∼500 | 11.1 × 22.3 |
H2 (0,0) S(1) | 17.03 | 17603.78 | 4.48 | 1015 | 2 × 104(a) | ∼500 | 4.7 × 11.3 |
[S III]3P1–3P0 | 33.48 | 8954.37 | 23.34 | 430 | 7.04 × 103 | ∼500 | 11.1 × 22.3 |
[Si II]2P3/2–2P1/2 | 34.81 | 8612.25 | 8.15 | 413 | 3.4 × 105(a), 103 | ∼500 | 11.1 × 22.3 |
[O III]3P2–3P1 | 51.81 | 5787.57 | 35.12 | 441 | 3.6 × 103 | ∼105 | 9.4 (c) |
[N III]2P3/2–2P1/2 | 57.32 | 5230.43 | 29.60 | 251 | 3.0 × 103 | ∼105 | 9.4 |
[O I]3P2–3P1 | 63.18 | 4744.77 | – | 228 | 4.7 × 105(a) | ∼86 | 9.4 |
[O III]3P1–3P0 | 88.36 | 3393.01 | 35.12 | 163 | 510 | ∼124 | 9.4 |
[N II]3P2–3P1 | 121.90 | 2459.38 | 14.53 | 118 | 310 | ∼290 | 9.4 |
[O I]3P1–3P0 | 145.52 | 2060.07 | – | 98 | 9.5 × 104(a) | ∼256 | 10.3 |
[C II]2P3/2–2P1/2 | 157.74 | 1900.54 | 11.26 | 91 | 20,[2.2 (a), 4.4 (b)] × 103 | ∼238 | 11.2 |
[N II]3P1–3P0 | 205.3 | 1460.27 | 14.53 | 70 | 48 | ∼297 | ∼16.8 |
Notes. The columns correspond to the central wavelength, frequency, ionisation potential, excitation temperature, critical density, spectral and spatial resolution of the data presented in this work, and the number of AGN, starburst, and dwarfs galaxies with line detections above 3 × rms. Critical densities and excitation temperatures from: Launay & Roueff (1977), Tielens & Hollenbach (1985), Greenhouse et al. (1993), Sturm et al. (2002), Cormier et al. (2012), Goldsmith et al. (2012), Farrah et al. (2013).
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