Table B.1.
MIRI/MRS emission lines.
| Transition | λrest | IP a | log ncrit b | AGN | N2 | S2 | |||
|---|---|---|---|---|---|---|---|---|---|
| Flux | σ | Flux | σ | Flux | σ | ||||
| μm | eV | cm−3 | 10−16 erg cm−2 s−1 | km s−1 | 10−16 erg cm−2 s−1 | km s−1 | 10−16 erg cm−2 s−1 | km s−1 | |
| MIRI/MRS Channel 1 | |||||||||
| [Fe II] | 4.889 | 7.9 | 4.39 | < 1.45 | ⋯ | < 0.87 | ⋯ | ⋯ | ⋯ |
| H2 0–0 S(8) | 5.053 | ⋯ | ⋯ | 4.2 ± 1.1 | ⋯ | 5.5 ± 1.2 | ⋯ | ⋯ | ⋯ |
| [Fe II] | 5.340 | 7.9 | 3.09 | 27.5 ± 1.4 | 253 ± 47 | 51.27 ± 0.44 | 336 ± 6 | ⋯ | ⋯ |
| [Fe VIII] | 5.447 | 125 | 6.41 | 14.13 ± 0.63 | ⋯ | < 0.69 | ⋯ | ⋯ | ⋯ |
| [Mg VII] | 5.503 | 187 | 6.53 | 19.5 ± 1.5 | ⋯ | < 0.70 | ⋯ | ⋯ | ⋯ |
| H2 0–0 S(7) | 5.511 | ⋯ | ⋯ | 19.1 ± 2.3 | ⋯ | 19.02 ± 0.40 | 134 ± 16 | ⋯ | ⋯ |
| [Mg V] | 5.610 | 109 | 6.60 | 34.5 ± 1.3 | 168 ± 49 | 3.43 ± 0.33 | ⋯ | ⋯ | ⋯ |
| H2 0–0 S(6) | 6.109 | ⋯ | ⋯ | 6.11 ± 0.65 | ⋯ | 6.58 ± 0.49 | ⋯ | ⋯ | ⋯ |
| [Ni II] | 6.636 | 7.6 | 5.92 | < 0.68 | ⋯ | 2.74 ± 0.23 | 241 ± 69 | ⋯ | ⋯ |
| [Fe II] | 6.721 | 7.9 | 3.09 | < 1.70 | ⋯ | 1.79 ± 0.23 | 222 ± 67 | ⋯ | ⋯ |
| H2 0–0 S(5) | 6.909 | ⋯ | ⋯ | 34.8 ± 1.0 | 196 ± 37 | 33.05 ± 0.28 | 144 ± 17 | ⋯ | ⋯ |
| [Ar II] | 6.985 | 15.8 | 5.62 | 87.1 ± 1.8 | 176 ± 24 | 48.97 ± 0.27 | 328 ± 3 | ⋯ | ⋯ |
| [Na III] | 7.318 | 47.3 | 6.80 | 8.6 ± 1.1 | 321 ± 71 | 2.73 ± 0.18 | 367 ± 38 | ⋯ | ⋯ |
| MIRI/MRS Channel 2 | |||||||||
| H I 6-5 | 7.460 | ⋯ | ⋯ | 7.2 ± 1.2 | ⋯ | 2.89 ± 0.34 | 307 ± 75 | ⋯ | ⋯ |
| [Ne VI] | 7.652 | 126 | 5.80 | 208.4 ± 1.6 | 127 ± 15 | 12.48 ± 0.23 | 193 ± 22 | ⋯ | ⋯ |
| [Fe VII] | 7.814 | 99.0 | 6.10 | 7.0 ± 1.6 | ⋯ | < 0.39 | ⋯ | ⋯ | ⋯ |
| [Ar V] | 7.902 | 59.6 | 5.20 | 11.62 ± 0.85 | ⋯ | 1.03 ± 0.23 | ⋯ | ⋯ | ⋯ |
| H2 0–0 S(4) | 8.026 | ⋯ | ⋯ | 15.7 ± 1.0 | 195 ± 58 | 14.44 ± 0.21 | 178 ± 26 | ⋯ | ⋯ |
| [Ar III] | 8.991 | 27.6 | 5.28 | 62.5 ± 1.1 | 128 ± 16 | 19.02 ± 0.29 | 264 ± 12 | ⋯ | ⋯ |
| [Mg VII] | 9.009 | 187 | 5.87 | < 2.76 | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ |
| [Fe VII] | 9.527 | 99.0 | 5.74 | 9.73 ± 0.78 | ⋯ | 2.27 ± 0.17 | 298 ± 77 | ⋯ | ⋯ |
| H2 0–0 S(3) | 9.665 | ⋯ | ⋯ | 39.25 ± 0.96 | 200 ± 38 | 33.05 ± 0.29 | 170 ± 13 | ⋯ | ⋯ |
| [S IV] | 10.51 | 34.9 | 4.75 | 220.0 ± 1.9 | 138 ± 16 | 49.94 ± 0.41 | 260 ± 6 | ⋯ | ⋯ |
| MIRI/MRS Channel 3 | |||||||||
| H2 0–0 S(2) | 12.28 | ⋯ | ⋯ | 22.06 ± 0.92 | 299 ± 27 | 10.51 ± 0.13 | 141 ± 16 | 1.30 ± 0.18 | ⋯ |
| H I 7-6 | 12.37 | ⋯ | ⋯ | < 1.51 | ⋯ | 1.01 ± 0.10 | 327 ± 70 | < 0.20 | ⋯ |
| [Ne II] | 12.81 | 21.6 | 5.80 | 222.1 ± 3.3 | 171 ± 23 | 112.8 ± 1.0 | 311 ± 6 | 8.36 ± 0.14 | 239 ± 25 |
| [Ar V] | 13.10 | 59.6 | 4.47 | 17.1 ± 1.5 | ⋯ | 1.84 ± 0.21 | ⋯ | < 0.23 | ⋯ |
| [Mg V] | 13.52 | 109 | 5.70 | < 2.75 | ⋯ | < 0.22 | ⋯ | < 0.13 | ⋯ |
| [Ne V] | 14.32 | 97.2 | 4.51 | 213.4 ± 1.4 | 126 ± 9 | 24.70 ± 0.17 | ⋯ | 5.03 ± 0.06 | 149 ± 9 |
| [Cl II] | 14.37 | 13.0 | 4.59 | < 3.66 | ⋯ | 1.64 ± 0.12 | ⋯ | < 0.16 | ⋯ |
| [Ne III] | 15.56 | 41.0 | 5.32 | 462.5 ± 3.2 | 154 ± 12 | 131.3 ± 1.1 | 280 ± 7 | 27.68 ± 0.33 | 191 ± 29 |
| H2 0–0 S(1) | 17.03 | ⋯ | ⋯ | 20.2 ± 2.4 | ⋯ | 13.35 ± 0.66 | ⋯ | 3.52 ± 0.21 | ⋯ |
| MIRI/MRS Channel 4 | |||||||||
| [Fe II] | 17.94 | 7.9 | 4.39 | 12.1 ± 2.1 | 311 ± 97 | 8.35 ± 0.21 | 366 ± 15 | < 0.33 | ⋯ |
| [S III] | 18.71 | 23.3 | 4.07 | 218.5 ± 1.8 | 141 ± 18 | 60.43 ± 0.63 | 242 ± 10 | 12.17 ± 0.25 | 202 ± 34 |
| [Ne V] | 24.32 | 97.2 | 3.77 | 312.3 ± 10.4 | 178 ± 47 | 23.81 ± 0.34 | 194 ± 29 | 5.27 ± 0.41 | ⋯ |
| [O IV] | 25.89 | 54.9 | 4.00 | 1167.2 ± 4.9 | ⋯ | 127.1 ± 1.1 | ⋯ | 48.45 ± 0.92 | 191 ± 8 |
| [Fe II] | 25.99 | 7.9 | 3.95 | 42.4 ± 4.3 | ⋯ | 11.93 ± 0.67 | ⋯ | < 1.90 | ⋯ |
Notes. Flux (zeroth moment) and velocity dispersion (second moment; σ) measured at the AGN, N2, and S2 regions. The diameter of the apertures is 1″. A point-source aperture correction is applied to the AGN spectra. The quoted uncertainties are 1σ statistical uncertainties. The absolute calibration uncertainty is ∼10% (Rigby et al. 2022). For the non-detections, we list the 3σ upper limits for a line with a width of ∼200 km s−1.
Ionization potential of the transition defined as the energy needed to reach the ionization stage producing that transition (Kramida et al. 2022).
Critical density at T = 10000 K for collisions with e− calculated using PyNeb v1.1.15 (Luridiana et al. 2015).
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