Table 2.
Best model results according to Akaike criterion.
| Name | ϵ | Model |
|---|---|---|
| NGC 3998 | 8.06E–01 | T/D |
| NGC 3718 | 1.68E+00 | T/D |
| NGC 4258* | 2.57E–16 | Torus |
| NGC 5033 | 5.67E–04 | Torus |
| ESO 253-G003* | 1.20E+00 | T/D |
| NGC 1052 | 3.86E–59 | Torus |
| NGC 2655 | 3.86E–02 | T/D |
| NGC 3147* | 6.44E–02 | T/D |
| NGC 2110* | 1.65E–53 | Torus |
| LEDA 96373* | 8.97E–26 | Torus |
| NGC 2992 | 1.77E–74 | Torus |
| M 51 | 1.68E–04 | Torus |
| NGC 2273* | 4.41E+07 | D |
| HE 1136-2304 | 5.31E–15 | Torus |
| IGRJ 11366-6002 | 2.49E+00 | T/D |
| IC 4518A | 1.18E–06 | Torus |
| NGC 7674* | 2.23E+02 | D |
Notes. Evidence ratio for the Akaike method and resulting model best to each source. T/D represents the cases when either torus or disk models provide equally good fits. T represents the torus model (borus02) and D the disk model (XILLVER). Objects marked with * are the galaxies with non-simultaneous observations with XMM-Newton and NuSTAR.
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