Table D.4.
Final compilation of the reflector parameters of the best-fit models for the sample.
PEXMON | borus02 | XILLVER | |||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Name | Rf | Incl | χ2/d.o.f. | ![]() |
log(NH − refl) | CF | Cos(θincl) | χ2/d.o.f. | ![]() |
log ξ | Rf | Incl (deg) | χ2/d.o.f. | ![]() |
BM |
NGC 3998 | 0.07![]() |
0.01![]() |
840.7/896 | 0.938 | 22.50![]() |
1.00![]() |
0.18![]() |
837.6/895 | 0.936 | 4.07![]() |
4.1![]() |
18.33![]() |
837.95/895 | 0.936 | T/D |
NGC 3718 | 0.01![]() |
0.02![]() |
408.2/371 | 1.100 | 22.78![]() |
0.99![]() |
0.30![]() |
405.9/369 | 1.100 | 3.12![]() |
4.91![]() |
88.74![]() |
404.8/369 | 1.097 | T/D |
NGC 4258* | 0.78![]() |
80.14![]() |
740.0/666 | 1.111 | 23.29![]() |
0.38![]() |
0.95![]() |
731.5/665 | 1.100 | 0.48![]() |
5.39![]() |
87.97![]() |
739.3/668 | 1.187 | Torus |
ESO 253-G003 | 10.00![]() |
86.60![]() |
107.1/121 | 0.885 | 24.04![]() |
0.73![]() |
0.76![]() |
108.6/120 | 0.905 | 2.68![]() |
2.08![]() |
65.99![]() |
108.3/120 | 0.903 | T/D |
NGC 1052 | 1.26![]() |
74.71![]() |
956.7/872 | 1.097 | 24.35![]() |
0.50![]() |
0.55![]() |
949.9/872 | 1.089 | 1.88![]() |
10.00![]() |
88.12![]() |
1286.0/872 | 1.4747 | Torus |
NGC 2655 | 0.07![]() |
0.01![]() |
171.8/168 | 1.022 | 23.24![]() |
0.83![]() |
0.85![]() |
159.4/167 | 0.954 | 1.85![]() |
9.84![]() |
89.09![]() |
178.1/169 | 1.054 | T/D |
NGC 3147* | 3.99![]() |
87.11![]() |
394.3/378 | 1.043 | 23.27![]() |
0.89![]() |
0.90![]() |
379.3/377 | 1.006 | 0.79![]() |
9.48![]() |
87.61![]() |
384.7/377 | 1.020 | T/D |
NGC 2110* | 1.01![]() |
79.58![]() |
1600.4/1261 | 1.2691 | 23.49![]() |
0.13![]() |
0.45![]() |
1293.2/1260 | 1.026 | 1.99![]() |
10.00![]() |
88.94![]() |
1564.3/1263 | 1.236 | Torus |
LEDA 96373* | 10.00![]() |
65.49![]() |
403.1/276 | 1.460 | 23.40![]() |
0.59![]() |
0.95![]() |
309.9/275 | 1.127 | 2.08![]() |
10.00![]() |
19.10![]() |
461.0/276 | 1.670 | Torus |
NGC 2992 | 0.37![]() |
0![]() |
2092.1/1619 | 1.292 | 23.17![]() |
0.75![]() |
0.85![]() |
1738.7/1618 | 1.075 | 0.006![]() |
10.00![]() |
88.41![]() |
2140.5/1620 | 1.3213 | Torus |
M 51 | 10.00![]() |
0.06![]() |
482.9/341 | 1.416 | 25.40![]() |
0.34![]() |
0.95![]() |
470.5/343 | 1.372 | 0.05![]() |
10.00![]() |
18.00![]() |
493.8/341 | 1.448 | Torus |
NGC 2273* | 10.00![]() |
0.09![]() |
226.8/197 | 1.151 | 23.75![]() |
0.15![]() |
0.94![]() |
173.5/196 | 0.882 | 2.14![]() |
9.99![]() |
8.90![]() |
246.3/196 | 1.257 | D |
HE 1136-2304 | 3.99![]() |
87.77![]() |
1066.0/987 | 1.080 | 23.52![]() |
0.59![]() |
0.05![]() |
1054.5/986 | 1.069 | 3.78![]() |
9.93![]() |
0.05![]() |
1126.3/986 | 1.142 | Torus |
IGRJ 11366-6002 | 0.68![]() |
18.37![]() |
261.9/245 | 1.069 | 24.75![]() |
0.93![]() |
0.94![]() |
252.3/244 | 1.034 | 3.19![]() |
3.68![]() |
63.99![]() |
250.49/244 | 1.026 | T/D |
IC 4518A* | 3.41![]() |
75.58![]() |
245.7/215 | 1.143 | 24.59![]() |
0.56![]() |
0.55![]() |
222.6/217 | 1.026 | 1.35![]() |
9.99![]() |
82.47![]() |
250.4/217 | 1.154 | Torus |
NGC 7674* | 3.22![]() |
18.17![]() |
189.0/169 | 1.118 | 25.40![]() |
0.70![]() |
0.95![]() |
190.7/168 | 1.135 | 2.82![]() |
3.25![]() |
0.0001![]() |
179.4/168 | 1.068 | D |
NGC 5033 | 1.35![]() |
78.47![]() |
1232.9/1058 | 1.165 | 23.49![]() |
0.77![]() |
0.95![]() |
1177.4/1058 | 1.113 | 0.45![]() |
10.00![]() |
87.41![]() |
1193.8/1054 | 1.133 | Torus |
Notes: Reflection fraction (Rf), the inclination (Incl) and the ionization degree (in log) of PEXMON and XILLVER models. The column density of the torus like reflector (log(NH, refl)), the covering factor (CF) and the inclination (Cos(θincl)) for borus02. BM shows the best model according with Akaike criterion. The symbol T/D represents that the models are indistinguishable. Objects with * symbols are the galaxies with not simultaneous observations. The quantities in this table marked with ** are unconstrained errors except in the case of the CF, where we report the cases the error is limited by the model.
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