Table F.1.
Optical emission lines fit by the HOMERUN code
| Emission line | λ [Å] | Obs. Luminosity | Model | Mod/Obs | AGN frac. | SF frac. | AGN dered. | SF dered. |
|---|---|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
| Hβ | 4861 | 100.00 ± 10.00 | 90.34 | 0.90 | 0.76 | 0.24 | 302.27 | 702.62 |
| [O III] | 5007 | 465.99 ± 46.60 | 500.05 | 1.07 | 0.97 | 0.04 | 2022.68 | 500.44 |
| [N I]* | 5199 | 7.51 ± 0.75 | 7.53 | 1.00 | 1.00 | 0.00 | 29.67 | 0.00 |
| He II | 5411 | 3.04 ± 0.32 | 3.08 | 1.01 | 1.00 | 0.00 | 11.39 | 0.00 |
| [Fe VII] | 5721 | 4.77 ± 0.95 | 3.64 | 0.76 | 1.00 | 0.00 | 12.35 | 0.00 |
| [N II] | 5755 | 2.41 ± 0.42 | 2.51 | 1.04 | 0.64 | 0.36 | 5.37 | 15.75 |
| [He I]* | 5876 | 19.75 ± 1.97 | 19.45 | 0.99 | 0.69 | 0.31 | 43.90 | 95.28 |
| [Fe VII] | 6087 | 6.30 ± 0.63 | 5.98 | 0.95 | 1.00 | 0.00 | 18.46 | 0.00 |
| [O I] | 6300 | 13.55 ± 1.35 | 13.68 | 1.01 | 0.75 | 0.25 | 30.01 | 43.22 |
| [S III] | 6312 | 1.43 ± 0.42 | 1.90 | 1.33 | 0.82 | 0.18 | 4.55 | 4.34 |
| [O I] | 6364 | 4.60 ± 0.46 | 4.48 | 0.98 | 0.75 | 0.25 | 9.67 | 13.81 |
| [Fe X] | 6375 | 1.19 ± 0.28 | 1.22 | 1.03 | 1.00 | 0.00 | 3.53 | 0.00 |
| Hα | 6563 | 622.41 ± 62.24 | 660.61 | 1.06 | 0.72 | 0.28 | 1322.36 | 2000.05 |
| [N II] | 6583 | 378.71 ± 37.87 | 369.45 | 0.98 | 0.31 | 0.69 | 318.65 | 2748.56 |
| He I | 6678 | 7.00 ± 0.70 | 6.75 | 0.96 | 0.62 | 0.38 | 11.25 | 26.74 |
| [S II] | 6716 | 68.33 ± 6.83 | 71.35 | 1.04 | 0.26 | 0.74 | 49.67 | 535.85 |
| [S II] | 6731 | 63.03 ± 6.30 | 52.86 | 0.84 | 0.27 | 0.73 | 38.19 | 388.58 |
| [Ar V] | 7006 | 2.07 ± 0.46 | 1.72 | 0.83 | 1.00 | 0.00 | 4.36 | 0.00 |
| [He I]* | 7065 | 2.56 ± 25.62 | 12.78 | 4.98 | 0.79 | 0.21 | 25.34 | 22.95 |
| [Ar III] | 7136 | 17.56 ± 1.76 | 16.34 | 0.93 | 0.61 | 0.40 | 24.44 | 54.04 |
| Ca II | 7291 | < 1.10 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 |
| [O II]* | 7323 | 3.11 ± 0.68 | 2.87 | 0.92 | 0.60 | 0.40 | 4.10 | 8.94 |
| [O II]* | 7332 | 2.41 ± 0.76 | 2.35 | 0.97 | 0.60 | 0.40 | 3.34 | 7.32 |
| [Ni II] | 7378 | 2.86 ± 0.43 | 2.75 | 0.96 | 1.00 | 0.00 | 6.52 | 0.00 |
| [Ar III] | 7751 | 4.54 ± 0.45 | 4.56 | 1.00 | 0.57 | 0.43 | 5.80 | 12.83 |
| [Cl II] | 8579 | 2.48 ± 0.68 | 3.52 | 1.42 | 0.00 | 1.00 | 0.00 | 17.57 |
| [Fe II] | 8617 | 0.85 ± 0.67 | 0.74 | 0.88 | 0.51 | 0.49 | 0.75 | 1.79 |
| [S III] | 9069 | 61.72 ± 6.20 | 62.49 | 1.01 | 0.49 | 0.52 | 56.72 | 140.12 |
Notes. (1) Name of the emission line. Lines marked with an asterisk correspond to transitions that in the CLOUDY framework are treated as blended multiplets. (2) Rest-frame wavelength of the emission line. (3) Observed luminosity scaled to an Hβ flux of 100. For some emission lines, error is set to 1000% to reflect highly uncertain measurements, marginal line detections dominated by noise, or to exclude those lines from the fit. (4) Line luminosity predicted by the model. (5) Ratio between the model and observed luminosity. (6) Fractional contribution of the AGN component to the observed line luminosity. (7) Fractional contribution of the SF component to the observed line luminosity. (8) Dereddened model luminosity of the AGN component normalized as in column 3. (9) Dereddened model luminosity of the SF component normalized as in column 3.
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