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Table A.8.

Spectral fit results for Type-2 Seyferts.

Obj. Mod. dof E(B-V) Parameters
F06 i σ Γ β Y τ9.7μm
N08 i N0 σ Y q τv
H10 i N0 θ a τcl
S16 i σ p q Y τ9.7μm
H17 i N0 a σ θ aw h fw
H17D i N0 a h

ESO005-G004* F06 2.27 / 2.89 84 / 36 0.86 61.4 < 20.6 < 0.0 > -0.0 < 10.1 > 9.5
N08 2.24 / 2.74 84 / 36 0.99 > 67.4 > 13.2 > 45.9 10.0 < 1.0 22.8
H10 2.07 / 2.62 85 / 37 0.85 > 78.0 > 9.3 < 41.7 > -0.0 < 36.5
S16 2.23 / 2.53 84 / 36 1.12 70.0 > 78.4 < 0.0 < 0.0 > 11.5 > 10.8
H17 2.20 / 2.60 82 / 34 1.42 85.0 > 8.5 > -0.6 > 13.9 > 43.9 -1.5 > 0.1 > 0.7
H17D 2.17 / 2.64 89 / 38 0.98 > 77.9 < 5.6 -0.9±0.1 0.4
MCG-05-23-016 F06 0.96 / 1.39 421 / 32 0.47±0.02 34.2±1.5 > 27.3 < 5.3 > -0.7 > 26.0 7.4±0.4
N08• 0.66 / 1.61 421 / 32 0.50±0.01 < 12.3 > 14.9 > 37.0 < 5.1 < 0.0 39.7
H10• 0.44 / 0.26 422 / 33 0.42±0.03 19.7 > 9.3 37.3 -0.7±0.1 75.1
S16• 0.40 / 0.97 421 / 32 0.61 54.9 39.9 1.02 < 0.0 < 12.0 < 10.2
H17• 0.60 / 0.42 419 / 30 0.27±0.01 81.1 7.01 -2.00 < 7.1 > 44.6 -1.89 > 0.2 > 0.7
H17D• 0.36 / 0.31 423 / 34 0.43 29.7 7.7 -1.36 > 0.7
NGC2110 F06 1.82 / 4.36 447 / 39 0.0* < 0.0 < 20.3 < 5.2 -0.75±0.01 30.0 1.17
N08• 0.59 / 1.85 447 / 39 0.78 72.1 > 1.1 < 17.7 < 5.6 > 2.5 73.9
H10• 0.42 / 1.30 448 / 40 0.72±0.03 48.5 3.3 > 57.8 -1.10±0.03 > 78.0
S16 1.24 / 4.67 447 / 39 0.0* > 89.6 > 79.7 0.8±0.1 > 1.4 20.0 < 3.0
H17• 0.37 / 0.90 445 / 37 0.64 75.4 < 5.3 -2.00 < 8.0 < 35.9 -2.00 < 0.1 0.30
H17D• 0.34 / 0.96 449 / 41 0.67 46.2 < 5.6 -2.03 0.32
NGC3081 F06• 0.92 / 1.43 186 / 19 0.0* 24.2±0.04 < 20.3 > 6.0 < -0.5 > 27.8 > 9.8
N08• 0.98 / 0.73 186 / 19 0.26 < 12.0 > 10.5 44.5 < 5.2 1.1 > 71.4
H10• 0.92 / 0.66 187 / 20 0.30 63.0 > 9.6 > 51.4 < -1.1 > 79.2
S16• 0.67 / 0.60 186 / 19 0.0* 20.2 75.3 0.61 < 0.0 < 10.4 6.2
H17• 0.91 / 0.75 184 / 17 0.29 59.8 > 9.2 -1.35 > 12.5 < 31.8 -1.5±0.1 < 0.3 < 0.2
H17D• 0.77 / 0.66 189 / 21 0.17 71.5 7.04 -1.64 0.25
NGC4388 F06 2.09 / 3.52 211 / 31 1.25 49.7 > 27.4 < 0.0 > -0.0 > 12.0 6.0
N08 2.24 / 4.65 211 / 31 1.73 > 0.0 > 14.9 > 48.4 19.9 > 0.0 < 71.7
H10• 1.36 / 1.99 212 / 32 1.14 30.2 > 7.5 < 5.1 > -0.4 > 79.6
S16 2.01 / 3.94 211 / 31 1.27±0.10 76.2 24.9 > 1.5 < 0.0 18.2±1.4 > 10.9
H17 1.64 / 2.27 209 / 29 1.24 60.4 > 9.9 -1.50 < 7.0 > 44.3 -0.97 > 0.4 > 0.7
H17D 1.90 / 2.42 213 / 33 1.69 49.8 > 9.9 -1.5±0.01 > 0.6
NGC4945 F06• 1.15 / 1.32 76 / 45 1.43 49.4 25.1 < 0.0 < -1.0 > 41.6 6.0
N08• 0.79 / 0.97 76 / 45 1.02 < 0.3 > 14.3 64.9 20.5 < 0.1 42.2
H10• 1.23 / 1.22 77 / 46 1.64±0.06 14.5 > 9.9 13.5 -0.50 > 79.6
S16• 0.96 / 1.07 76 / 45 1.49 77.9 22.9 > 1.4 < 0.0 > 27.9 > 10.7
H17 1.90 / 1.98 74 / 43 1.58 > 89.8 9.4±0.4 -2.00±0.01 > 14.5 > 43.8 -2.00 > 0.5 0.60±0.01
H17D 1.87 / 1.75 78 / 47 2.06 36.6 > 9.9 -1.50±0.01 > 0.7
NGC5128 F06• 1.40 / 1.96 184 / 24 2.16±0.09 31.5 < 27.0 > 5.7 -0.64±0.04 > 11.5 5.0
N08 1.74 / 2.32 184 / 24 2.05 < 60.4 > 14.6 > 21.6 < 5.0 > 2.4 < 35.6
H10• 1.00 / 1.62 185 / 25 1.71 < 0.5 > 9.9 < 36.4 -0.82 > 79.0
S16• 1.06 / 1.88 184 / 24 2.14±0.04 > 23.1 40.8 > 0.0 < 0.0 < 10.3 > 10.9
H17• 1.19 / 1.70 182 / 22 1.89±0.03 85.4 > 8.2 < -2.9 > 12.9 > 43.0 -1.78±0.05 < 0.1 > 0.7
H17D• 1.09 / 1.80 186 / 26 1.87 < 0.0 > 9.9 -1.07±0.02 > 0.7
NGC6300* F06 5.65 / 6.97 81 / 47 1.69 > 87.3 > 20.0 < 0.0 < -1.0 > 147.2 > 9.9
N08 2.35 / 3.65 81 / 47 0.86 < 0.0 > 14.6 > 68.3 46.8 < 0.2 40.1
H10 4.18 / 4.53 82 / 48 1.77 14.9 > 10.0 > 22.0 -0.50 > 79.7
S16 6.55 / 7.70 81 / 47 1.72 87.2 < 13.2 > 0.0 < 0.0 < 10.2 < 10.2
H17 3.46 / 4.47 79 / 45 1.79 > 90.0 < 5.0 -1.50 > 14.9 > 44.8 < -2.5 < 0.1 0.45±0.01
H17D 4.80 / 5.10 83 / 49 2.06 < 40.0 > 9.9 -1.74 > 0.7
NGC7172* F06 2.51 / 3.50 74 / 34 2.76 > 44.7 > 58.4 < 0.0 -0.75±0.01 < 10.2 0.31
N08 5.48 / 8.03 74 / 34 1.60 > 53.6 > 14.6 > 66.0 < 5.0 > 2.5 < 10.1
H10 3.47 / 5.01 74 / 35 2.35±0.06 59.7±1.0 5.0 > 57.9 < -2.0 > 76.6
S16 4.65 / 7.20 74 / 34 2.58±0.07 29.8 59.9 > 1.5 > 1.4 < 10.2 < 3.3
H17 1.86 / 2.56 71 / 32 2.18±0.06 < 0.4 < 5.2 < -3.0 > 14.3 > 44.3 -2.33 < 0.1 > 0.7
H17D 3.48 / 5.15 75 / 36 1.49±0.05 < 0.0 > 9.9 -1.75 > 0.7
NGC7582 F06• 0.41 / 0.64 196 / 45 2.42 23.9 > 51.1 < 0.0 < -1.0 > 147.5 4.0
N08 1.07 / 1.29 196 / 45 1.45 < 0.2 > 14.8 55.1 < 5.0 0.5 20.0
H10• 1.08 / 1.11 197 / 46 1.55 < 0.0 > 9.9 30.0 < -0.9 < 69.5
S16• 0.56 / 0.76 196 / 45 2.52 > 84.2 < 10.1 > 1.2 1.0 > 29.0 9.0
H17• 0.61 / 0.95 194 / 43 1.50 > 90.0 < 5.0 -2.00 10.0 > 44.7 < -2.5 < 0.1 0.6±0.6
H17D• 0.72 / 1.00 198 / 47 1.76±0.04 < 0.0 > 9.9 -1.75 > 0.7

Notes. Best-fit results per object and model. Models are quoted in Col. 2 as follows. F06: [Fritz06]; N08: [Nenkova08]; H10: [Hoenig10]; S16: [Stalev16]; and H17: [Hoenig17]. The reduced χ2 (χ2/dof) is included in Col. 3, colour excess for the foreground extinction E(B − V) is included in Col. 4, and the final parameters per model are included in Cols. 5-13. Comparably good fits (χ2/dof <  min(χ2/dof)+0.5) are marked with filled circles next to the model name.

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