Table D.1.
Comparison between mid-IRw and X-ray parameters.
| Objname | Type | NH | Model |
Cf | σ | i | N0 | τν | log(NHtor) | Comment | ||
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| variable | X-ray | Mid-IR | Mid-IR | X-ray | Mid-IR | mid-IR | X-ray | |||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) |
| Seyfert 1 | ||||||||||||
| Mrk 1393 | Sy1 | Y | Clumpy* | Clumpy | 0.61 |
– | < 25.3 | 10.7 |
> 14.1 | < 10.6 | 23.9 |
|
| PG 0804+761 | Sy1 | N | Smooth | Smooth | 0.07 |
36.9 |
< 21.1 | < 0.1 | – | 18.4 |
24.5 |
|
| PG 1211+143 | Sy1 | N | Smooth | Smooth | 0.12 |
64.2 |
< 20.3 | 25.3 |
– | > 153.9 | 24.2 |
|
| Mrk 1383 | Sy1 | N | Smooth | Clumpy | 0.82 |
65.1 |
< 62.9 | > 16.8 | 3.1 |
75.7 |
24.3 |
|
| Mrk 590 | Sy1 | N | Smooth* | Clumpy | 0.81 |
– | > 31.7 | > 55.7 | 4.2 |
135.0 |
23.7 |
|
| NGC 7213 | Sy1 | N | Smooth | Clumpy | 0.37 |
– | < 15.1 | < 88.5 | 7.0 |
55.8 |
22.8 |
|
| Seyfert 2 | ||||||||||||
| NGC 4507 | Sy2 | Y | Clumpy* | Clumpy | 0.81 |
9.9 |
> 47.6 | > 35.3 | 3.1 |
70.8 |
23.8 |
|
| NGC 1052 | Sy2 | Y | Clumpy* | Clumpy | 0.87 |
27.8 |
> 46.6 | > 51.0 | 3.5 |
199.9 |
23.4 |
|
| NGC 4939 | Sy2 | Y | Clumpy* | Clumpy | 0.95 |
> 21.4 | > 54.2 | < 71.7 | > 8.2 | > 216.6 | 23.7 |
|
| IC 5063 | Sy2 | Y | Clumpy | Clumpy | 0.86 |
> 16.5 | 38.2 |
< 60.0 | > 8.8 | 95.3 |
23.5 |
|
| ESO 138-G1 | Sy2 | N | Smooth* | Clumpy | 0.95 |
79.4 |
> 66.8 | < 87.7 | 5.5 |
19.0 |
24.5 |
|
| PKS 2356−61 | Sy2 | N | Smooth | S/C | 0.14 /0.8 |
– | < 21.7/35.0 |
24.8 /40.2 |
5.4 |
> 204.4/40.0 |
23.1 |
|
| NGC 788 | Sy2 | N | Smooth | Clumpy | 0.92 |
– | > 46.8 | > 28.9 | 10.4 |
43.3 |
23.8 |
|
| Unclassified | ||||||||||||
| Mrk 1392 | Sy1 | – | Clumpy | Clumpy | 0.52 |
3.0 |
< 17.9 | 6.1 |
> 13.6 | 12.7 |
22.4 |
Panel 1 of Fig. 7 |
| RBS 0770 | Sy1 | – | S/C | S/C | 0.11 /0.8 |
–/5.4 |
< 20.4/< 57.4 | 0.0 /> 16.3 |
5.0 |
166.4 /28.0 |
25.0 /22.1 |
Panel 3 of Fig. 7 |
| RBS 1125 | Sy1 | – | S/C | Clumpy | 0.77 |
–/> 0.1 | < 44.5 | > 4.9 | 6.2 |
20.0 |
24.3 /24.0 |
Panel 3 of Fig. 7 |
| MCG+01-57-016 | Sy1 | – | S/C | Clumpy | 0.87 |
> 80.5/0.3 |
42.6 |
< 8.5 | > 6.7 | 198.9 |
24.3 /22.6 |
Panel 3 of Fig. 7 |
| ESO 141-G055 | Sy1 | – | Smooth | S/C | 0.08 /0.62 |
59.5 |
< 21.6/< 36.9 | 44.7 /> 2.7 |
3.1 |
> 215.9/50.4 |
24.4 |
unclassified |
| UM 146 | Sy2 | – | S/C | Clumpy | 0.92 |
–/1.8 |
> 55.4 | > 37.9 | 4.8 |
24.7 |
23.3 /23.4 |
Panel 5 of Fig. 8 |
| NGC 1358 | Sy2 | – | S/C | S/C | 0.42 /0.84 |
> 26.1/< 9.6 | < 58.6/– | < 42.1/< 55.6 | 7.7 |
> 53.0/< 16.0 | 24.2 /24.2 |
Panel 5 of Fig. 8 |
| IC 4518W | Sy2 | – | S/C | Clumpy | 0.92 |
–/2.7 |
> 48.1 | > 51.5 | 8.3 |
27.2 |
23.4 /23.3 |
Panel 5 of Fig. 8 |
| Mrk 78 | Sy2 | – | S/C | Clumpy | 0.94 |
–/– | > 55.7 | > 21.8 | > 13.9 | 53.6 |
23.8 /23.8 |
Panel 5 of Fig. 8 |
| J05081967+1721483 | Sy2 | – | Clumpy | Clumpy | 0.83 |
> 3.3 | 53.3 |
< 75.4 | 4.3 |
> 139.7 | 23.5 |
Unclassified |
| ESO 103-G35 | Sy2 | – | Smooth | Clumpy | 0.85 |
– | < 46.6 | > 22.7 | 8.8 |
46.8 |
24.3 |
Panel 6 of Fig. 8 |
| J10594361+6504063 | Sy2 | – | Smooth | S/C | 0.93 /0.96 |
– | < 22.1/> 68.9 | 74.6 /54.2 |
> 14.7 | > 196.7/20.1 |
22.7 |
Panel 6 of Fig. 8 |
Notes. S/C is included in Cols. 4 and 5 when neither of the two models is preferred. Objects marked as “Clumpy*” in Col. 4 are variable at X-rays (denoting a clumpy medium) but preferred at smooth model statistically. In Col. 6 we show the covering factors estimated to mid-IR. In Cols. 8 and 9 we show the half-opening angles using the preferred model at X-ray and mid-IR wavelengths, respectively. Both half-opening angle and inclination angles are measured from the equator of the system to its pole. The optical depth is also converted to the 9.7 μm optical depth as τ9.7 μm = 0.042 τV.
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