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Table C.1.

List of the fit emission lines in the MIRI spectra

Emission line λ(1) IP(1) Ch Flux
[#x03BC;m] [eV] [10−14 erg s−1 cm−2]
[Mg V] 5.61 109 1A 1.75 ± 0.05
Pfα 7.46 - 1C 0.962 ± 0.005
[Ne VI] 7.65 126 2A 8.44 ± 0.09
[Ar V] 7.90 60 2A 1.4 ± 0.1
H2 0-0 S(4) 8.03 - 2A 2.06 ± 0.04
[Ar III] 8.99 28 2B 3.4 ± 0.2
H2 0-0 S(3) 9.66 - 2B 4.6 ± 0.6
[S IV] 10.51 35 2C 24.0 ± 0.4
H2 0-0 S(2) 12.28 - 3A 7.5 ± 0.1
Huα 12.37 - 3A 0.760 ± 0.002
[Ne II] 12.81 23 3A 102.6 ± 0.4
[Ar V] 13.10 60 3A 0.702 ± 0.004
[Ne V] 14.32 97 3B 22.2 ± 0.4
[Cl II] 14.37 13 3B 2.02 ± 0.03
[Ne III] 15.56 41 3C 56.6 ± 0.4
H2 0-0 S(1) 17.04 - 3C 16.3 ± 0.4
[S III] 18.71 23 4A 50.5 ± 0.2
[Ne V] 24.32 97 4C 26.70 ± 0.04
[O IV] 25.89 55 4C 53.0 ± 2.0

Notes. From left to right: the name of the emission line, the corresponding rest-frame wavelength, the IP, the MIRI channel where it is observed, and the integrated flux within the FoV of the respective channel, expressed in units of 10−14 erg s−1 cm−2.

References. (1) ISO Spectrometer Data Centre.

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