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Table 5
Fit results for all sources in this sample.
| Name | Case | F tot | f p | F p | F g | Θg | r 1/2 | r 1/2 | Comment |
| [Jy] | [Jy] | [Jy] | [mas] | [mas] | [pc] | ||||
|
|
|||||||||
| I Zw 1 | 1 | 0.53 ± 0.02 | 0.73 |
0.31 |
0.11 |
24 |
<2.5 | <2.7 | resolved and unresolved |
| NGC 424 | 1 | 0.72 ± 0.03 | 0.54 ± 0.05 | 0.31 |
0.50 |
28.7 |
5.9 |
1.28 |
resolved and unresolved |
| NGC 1068 | 1 | 16.08 ± 0.16 | 0.09 ± 0.01 | 1.48 |
14.60 |
47.9 |
22.2 |
1.55 |
resolved and unresolved |
| NGC 1365 | 3 | 0.30 ± 0.01 | 1.00 | ... | ... | 5.75 |
2.88 |
0.25 |
marginally resolved |
| IRAS 05189-2524 | 1 | 0.56 ± 0.03 | 0.53 |
0.24 |
0.22 |
30 |
<4.3 | <3.56 | resolved and unresolved |
| H 0557-385 | 1 | 0.50 ± 0.03 | 0.58 |
0.28 |
0.13 |
42 |
<2.5 | <1.6 | resolved and unresolved |
| IRAS 09149-6206 | 2 | 0.57 ± 0.03 | 0.72 ± 0.06 | 0.34 |
0.13 |
>31 | <2.5 | <2.7 | over-resolved and unresolved |
| MCG-05-23-16 | 1 | 0.73 ± 0.01 | 0.28 ± 0.04 | 0.21 |
0.53 |
27.3 |
9.9 |
1.86 |
resolved and unresolved |
| Mrk 1239 | 3 | 0.57 ± 0.05 | 1.00 | ... | ... | 3.97 |
1.99 |
0.81 |
marginally resolved |
| NGC 3281 | 2 | 0.32 ± 0.01 | 0.77 ± 0.03 | 0.25 |
0.07 |
>15 | <2.5 | <0.58 | over-resolved and unresolved |
| NGC 3783 | 1 | 0.76 ± 0.02 | 0.37 |
0.28 |
0.58 |
31.7 |
9.2 |
1.96 |
resolved and unresolved |
| NGC 4151 | 2 | 1.18 ± 0.03 | 0.26 ± 0.01 | 0.30 |
0.87 |
>56 | >21.3 | >1.7 | over-resolved and unresolved |
| 3C 273 | 3 | 0.32 ± 0.04 | 1.00 | ... | ... | 6.15 |
3.07 |
8.1 |
marginally resolved |
| NGC 4507 | 1 | 0.53 ± 0.02 | 0.26 ± 0.03 | 0.16 |
0.57 |
31.9 |
12.1 |
3.03 |
resolved and unresolved |
| NGC 4593 | 2 | 0.25 ± 0.01 | 0.51 ± 0.03 | 0.13 |
0.12 |
>52 | ... | ... | over-resolved and unresolved |
| ESO 323-77 | 3 | 0.38 ± 0.01 | 1.00 | ... | ... | 6.74 |
3.37 |
1.05 |
marginally resolved |
| Centaurus A | 2 | 1.57 ± 0.03 | 0.58 ± 0.02 | 0.91 |
0.56 |
>24 | <2.5 | <0.05 | over-resolved and unresolved |
| IRAS 13349+2438 | 4 | 0.50 ± 0.02 | 1.00 | ... | ... | <6.54 | <3.3 | <6.2 | unresolved |
| IC 4329 A | 1 | 1.03 ± 0.02 | 0.56 ± 0.05 | 0.58 |
0.55 |
30 |
<2.5 | <0.83 | resolved and unresolved |
| Circinus | 1 | 10.23 ± 0.05 | 0.06 ± 0.012 | 0.51 |
9.61 |
80.2 |
38.3 |
0.78 |
resolved and unresolved |
| NGC 5506 | 2 | 0.97 ± 0.08 | 0.52 ± 0.05 | 0.50 |
0.37 |
>37 | <2.5 | <0.35 | over-resolved and unresolved |
| NGC 5995 | 1 | 0.33 ± 0.01 | 0.57 |
0.15 |
0.18 |
22.8 |
<5.0 | <2.48 | resolved and unresolved |
| NGC 7469 | 1 | 0.52 ± 0.02 | 0.37 ± 0.05 | 0.23 |
0.39 |
46.7 |
13.6 |
4.0 |
resolved and unresolved |
|
|
|||||||||
| NGC 3227 | 0 | 0.32 ± 0.02 | <0.57 | <0.150 | ... | ... | ... | ... | limit on Fp from non-detection |
| IC 3639 | 0 | 0.54 ± 0.03 | <0.28 | <0.150 | ... | ... | ... | ... | limit on Fp from non-detection |
Notes. For the model case selection, see Fig. 2 and text. Case “0” refers to those sources for which we only have upper limits on the total flux, no model was fitted here.
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