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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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