Table 3.
Best model results according to Akaike criterion.
| Seyfert 1 |
Seyfert 2 |
||||||||
|---|---|---|---|---|---|---|---|---|---|
| Object | X-ray |
Mid-IR |
Object | X-ray |
Mid-IR |
||||
| ϵ | Model | ϵ | Model | ϵ | Model | ϵ | Model | ||
| Mrk 1018 | 5.50E+00* | S/C | 6.45E+05 | Clumpy | UM 146 | 6.71E−01 | S/C | 8.90E+08 | Clumpy |
| Mrk 590 | 2.55E−01 | S/C | 1.03E+27 | Clumpy | NGC 788 | 2.88E+04 | Smooth | 1.02E+45 | Clumpy |
| PG 0804+761 | 6.97E+02 | Smooth | 8.53E−24 | Smooth | NGC 1052 | 6.48E+00 | S/C | 3.49E+42 | Clumpy |
| RBS0770 | 1.73E+00 | S/C | 1.24E−01 | S/C | NGC 1358 | 2.94E+00 | S/C | 8.06E−01 | S/C |
| I11119+3257 | 7.65E−04 | Clumpy | 2.05E−38* | Smooth | J05081967+1721483 | 1.62E−03 | Clumpy | 1.68E+17 | Clumpy |
| PG 1211+143 | 2.25E+07 | Smooth | 3.31E−07 | Smooth | Mrk3 | 1.54E+101 | Smooth | 6.44E+42* | Clumpy |
| RBS 1125 | 5.59E+01 | S/C | 2.70E+29 | Clumpy | ESO 428-G014 | 4.90E+02* | Smooth | 1.26E+11 | Clumpy |
| Mrk 231 | 2.07E+00 | S/C | 1.20E+03* | Clumpy | Mrk 78 | 6.77E+01 | S/C | 1.76E+22 | Clumpy |
| Mrk 1383 | 2.55E+05 | Smooth | 4.93E+10 | Clumpy | Mrk 1210 | 1.26E−05 | Clumpy | 1.35E+29* | Clumpy |
| Mrk 1392 | 1.21E−04 | Clumpy | 2.26E+26 | Clumpy | J10594361+6504063 | 1.07E+02 | Smooth | 3.43E+00 | S/C |
| Mrk 1393 | 4.81E+00 | S/C | 4.84E+42 | Clumpy | NGC 4388 | 1.71E+21 | Smooth | 2.92E+14* | Clumpy |
| PG 1535+547 | 1.15E−01* | S/C | 1.06E−10 | Smooth | NGC 4507 | 1.51E+57 | Smooth | 6.31E+36 | Clumpy |
| ESO 141-G055 | 2.13E+16 | Smooth | 2.44E+00 | S/C | NGC 4939 | 3.06E+02 | Smooth | 7.53E+29 | Clumpy |
| NGC 7213 | 1.68E+05 | Smooth | 3.14E+177 | Clumpy | ESO-097-G013 | 3.20E+129 | Smooth | 4.99E+120* | Clumpy |
| MCG+01-57-016 | 1.57E−02 | S/C | 3.61E+19 | Clumpy | IC4518W | 1.02E−02 | S/C | 2.15E+12 | Clumpy |
| ESO 138-G1 | 7.01E−02 | S•/C | 1.13E+24 | Clumpy | |||||
| NGC6300 | 5.92E+01 | S•/C | 1.13E+44* | Clumpy | |||||
| ESO 103-G35 | 3.90E+09 | Smooth• | 8.36E+73 | Clumpy | |||||
| MCG+07-41-03 | 1.02E+36 | Smooth | 2.57E+93* | Clumpy | |||||
| IC 5063 | 5.16E−07 | Clumpy | 1.52E+34 | Clumpy | |||||
| PKS 2356−61 | 7.91E+03 | Smooth | 4.52E+00 | S/C | |||||
Notes. Evidence ratio for the Akaike method and resulting model best to each source. S/C is included when either Smooth or Clumpy models provide an equally good fits. Bullets indicate that the best fit is obtained using the baseline model with NHtor independent to the NHl.o.s.. Asterisks indicate poor fits with χ2/d.o.f. > 1.2 (see text).
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