Table 5.
Mean and standard deviation values of the mid-IR parameters obtained for Sy1 and Sy2 when using the smooth and clumpy baseline models.
Parameter | Baseline | Sy1 | Sy2 | ||||
---|---|---|---|---|---|---|---|
model | # | Mean | Std | # | Mean | Std | |
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
i | Smooth | 3 | 23.4 | 18.3 | 3 | 36.4 | 27.7 |
Clumpy | 2 | 81.6 | 2.3 | 2 | 42.8 | 7.0 | |
σ | Smooth | 0 | – | – | 1 | – | – |
Clumpy | 2 | 48.5 | 5.9 | 3 | 42.2 | 7.9 | |
Y | Smooth | 3 | 11.7 | 0.5 | 5 | 33.5 | 15.8 |
Clumpy | 9 | 14.5 | 4.3 | 9 | 17.8 | 8.33 | |
τ9.7 μm | Smooth | 5 | 4.9 | 2.3 | 1 | – | – |
τν | Clumpy | 10 | 65.8 | 55.3 | 12 | 55.6 | 48.6 |
β | Smooth | 4 | −0.51 | 0.19 | 1 | – | – |
γ | Smooth | 3 | 4.5 | 0.85 | 2 | 2.84 | 2.81 |
N0 | Clumpy | 8 | 4.35 | 1.45 | 10 | 6.19 | 2.34 |
q | Clumpy | 5 | 1.41 | 0.48 | 9 | 1.37 | 0.47 |
Notes. Column (1): parameter name. Column (2): mid-IR baseline model. Column (3): number of sources considered to calculate the mean and standard values. We only considered AGN for which the parameters are well constrained. Columns (4) and (7): Mean values to Sy1 and Sy2, respectively. Columns (7) and (8): Standard deviation values to Sy1 and Sy2, respectively.
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