Table 3.

MIR spectral feature luminosity.

HighIntermediateLow
λaIPbluminosityluminosityluminosity
Feature(μm)(eV)(erg s−1)(erg s−1)(erg s−1)
H2 S(7) 5.4942.9741.7640.51
H2 S(6) 6.0643.0741.5040.69
H2 S(5) 6.8941.4040.93
[Ar ii] 6.9715.7641.2141.59
H2 S(4) 7.9841.3641.69
[Ar iii] 8.9727.6340.34
H2 S(3)10.5243.1441.8841.49
[S iv]12.3134.7943.2842.3941.46
H2 S(2)12.8243.1141.0540.86
[Ne ii]14.3121.5643.5242.3241.83
[Ne v] 1414.3197.1143.1642.1441.45
[Ne iii]15.5740.9643.5942.5741.93
H2 S(1)17.0642.6941.7441.56
[S iii] 1818.7223.3343.3642.0641.73
[Ne v] 2424.3497.1142.3741.82
[O iv]25.8654.9343.56c42.6942.06
[Fe ii]26.04 7.8742.1041.42
HighIntermediateLow
λaIPbluminosityluminosityluminosity
Feature(μm)(eV)(erg s−1)(erg s−1)(erg s−1)
H2 S(7) 5.4942.9741.7640.51
H2 S(6) 6.0643.0741.5040.69
H2 S(5) 6.8941.4040.93
[Ar ii] 6.9715.7641.2141.59
H2 S(4) 7.9841.3641.69
[Ar iii] 8.9727.6340.34
H2 S(3)10.5243.1441.8841.49
[S iv]12.3134.7943.2842.3941.46
H2 S(2)12.8243.1141.0540.86
[Ne ii]14.3121.5643.5242.3241.83
[Ne v] 1414.3197.1143.1642.1441.45
[Ne iii]15.5740.9643.5942.5741.93
H2 S(1)17.0642.6941.7441.56
[S iii] 1818.7223.3343.3642.0641.73
[Ne v] 2424.3497.1142.3741.82
[O iv]25.8654.9343.56c42.6942.06
[Fe ii]26.04 7.8742.1041.42

Note. Line luminosities calculated for model outputs from PAHFIT for each luminosity template. Blank spaces indicate the feature was not detected by PAHFIT.

aWavelengths are the best-fitting values from PAHFIT.

bIonization potentials taken from Cox (2000).

cCalculated from fitting the local continuum around [O iv] because the PAHFIT model was overpredicting the continuum at longer wavelengths. This value is used for Figs 12–14.

Table 3.

MIR spectral feature luminosity.

HighIntermediateLow
λaIPbluminosityluminosityluminosity
Feature(μm)(eV)(erg s−1)(erg s−1)(erg s−1)
H2 S(7) 5.4942.9741.7640.51
H2 S(6) 6.0643.0741.5040.69
H2 S(5) 6.8941.4040.93
[Ar ii] 6.9715.7641.2141.59
H2 S(4) 7.9841.3641.69
[Ar iii] 8.9727.6340.34
H2 S(3)10.5243.1441.8841.49
[S iv]12.3134.7943.2842.3941.46
H2 S(2)12.8243.1141.0540.86
[Ne ii]14.3121.5643.5242.3241.83
[Ne v] 1414.3197.1143.1642.1441.45
[Ne iii]15.5740.9643.5942.5741.93
H2 S(1)17.0642.6941.7441.56
[S iii] 1818.7223.3343.3642.0641.73
[Ne v] 2424.3497.1142.3741.82
[O iv]25.8654.9343.56c42.6942.06
[Fe ii]26.04 7.8742.1041.42
HighIntermediateLow
λaIPbluminosityluminosityluminosity
Feature(μm)(eV)(erg s−1)(erg s−1)(erg s−1)
H2 S(7) 5.4942.9741.7640.51
H2 S(6) 6.0643.0741.5040.69
H2 S(5) 6.8941.4040.93
[Ar ii] 6.9715.7641.2141.59
H2 S(4) 7.9841.3641.69
[Ar iii] 8.9727.6340.34
H2 S(3)10.5243.1441.8841.49
[S iv]12.3134.7943.2842.3941.46
H2 S(2)12.8243.1141.0540.86
[Ne ii]14.3121.5643.5242.3241.83
[Ne v] 1414.3197.1143.1642.1441.45
[Ne iii]15.5740.9643.5942.5741.93
H2 S(1)17.0642.6941.7441.56
[S iii] 1818.7223.3343.3642.0641.73
[Ne v] 2424.3497.1142.3741.82
[O iv]25.8654.9343.56c42.6942.06
[Fe ii]26.04 7.8742.1041.42

Note. Line luminosities calculated for model outputs from PAHFIT for each luminosity template. Blank spaces indicate the feature was not detected by PAHFIT.

aWavelengths are the best-fitting values from PAHFIT.

bIonization potentials taken from Cox (2000).

cCalculated from fitting the local continuum around [O iv] because the PAHFIT model was overpredicting the continuum at longer wavelengths. This value is used for Figs 12–14.

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