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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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