Table 4.
Spectral model fit results for the one-component case.
Model | α | νp | Sp | β | p | αthick | lnlike |
---|---|---|---|---|---|---|---|
(GHz) | (mJy) | ||||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
J0131−0321 | |||||||
Internal FFA | ![]() |
![]() |
![]() |
– | – | ![]() |
18.17 |
Inhomogeneous FFA |
![]() |
![]() |
![]() |
– |
![]() |
![]() |
18.20 |
J0741+2520 | |||||||
Inhomogeneous FFA |
![]() |
![]() |
![]() |
– |
![]() |
![]() |
240.59 |
J0836+0054 | |||||||
Inhomogeneous FFA |
![]() |
![]() |
![]() |
– |
![]() |
![]() |
18.49 |
J0913+5919 | |||||||
Internal FFA |
![]() |
![]() |
![]() |
– | – |
![]() |
6.16 |
Inhomogeneous FFA |
![]() |
![]() |
![]() |
– |
![]() |
![]() |
5.93 |
J1034+2033 | |||||||
Inhomogeneous FFA |
![]() |
![]() |
![]() |
– |
![]() |
![]() |
243.05 |
J1427+3312 | |||||||
Homogeneous SSA |
![]() |
![]() |
![]() |
![]() |
– | – | 22.52 |
Homogeneous FFA |
![]() |
![]() |
![]() |
– | – | – | 22.57 |
Internal FFA |
![]() |
![]() |
![]() |
– | – |
![]() |
22.51 |
Inhomogeneous FFA |
![]() |
![]() |
![]() |
– |
![]() |
![]() |
22.51 |
J1614+4640 | |||||||
Internal FFA |
![]() |
![]() |
![]() |
– | – |
![]() |
231.17 |
Inhomogeneous FFA |
![]() |
![]() |
![]() |
– |
![]() |
![]() |
231.20 |
J2245+0024 | |||||||
Inhomogeneous FFA |
![]() |
![]() |
![]() |
– |
![]() |
![]() |
242.02 |
Notes. Column 1: model case. Column 2: the power-law index of the intrinsic radio source. Column 3: the frequency at which the source becomes optically thick in the rest frame. Column 4: source flux density in the rest frame at the νp shown in Col. 3. Column 5: the power-law index of the electron energy distribution only for the homogeneous SSA case. Column 6: the distribution of absorbing clouds only for the inhomogeneous FFA case. Column 7: power-law index for the optically thick part (i.e., below the turnover frequency). Column 8: likelihood for the best-fit model.
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