\begin{table}%T5
\caption{Results of modelfit -- VLA images. \label{res_vla}}
%\centerline
 {
\begin{tabular}{llrrrrcc}
\hline\hline
 & & \multicolumn{2}{c}{8.4~GHz} & \multicolumn{2}{c}{22.5~GHz} \\
Source & Component & Peak & Flux & Peak & Flux & $\alpha_{8.4}^{22}$ & Size \\
 & & $\left(\frac{{\rm mJy}}{{\rm beam}}\right)$ & (mJy) & $\left(\frac{{\rm mJy}}{{\rm beam}}\right)$ & (mJy) & & \arcsec \\[1mm]
\hline
0222+36 & core    & 174 & 179 &  89 &  91 & $0.69 \pm 0.02$ & 0.05 \\
        & NE lobe & 5.7 & 7.0 & 1.5 & 2.8 & $0.93 \pm 0.04$ & 0.2 \\
        & SW lobe & 3.2 & 5.7 & 0.6 & 2.2 & $0.97 \pm 0.04$ & 0.4 \\
        & total   &  -- & 192 &  -- &  95 & $0.71 \pm 0.02$ & 1.6 \\
\hline
0258+35 & core region & 119 & 167 &  52 & 14+57 & $0.87 \pm 0.02$ & 0.08 \\
        & SE jet      &  58 & 134 &  15 &    77 & $0.56 \pm 0.02$ & 1.0 \\
        & E lobe      &  21 & 197 & 4.8 &    77 & $0.95 \pm 0.02$ & 1.6 \\
        & NW lobe     &  14 &  93 & 2.6 &    37 & $0.93 \pm 0.02$ & 1.6 \\
        & total       &  -- & 610 &  -- &   255 & $0.88 \pm 0.01$ & 3.5 \\
\hline
0648+27 & N lobe &  11 & 19 & 2.2 & 2.9+2.3 & $1.31 \pm 0.03$ & 0.6 \\
        & S lobe & 8.4 & 14 & 0.9 &     4.9 & $1.06 \pm 0.03$ & 0.6 \\
        & total  &  -- & 31 &  -- &     9.3 & $1.22 \pm 0.02$ & \\
\hline
1037+30 & core      & 2.2 & 3.9 & 1.0 & 2.6 & $0.41 \pm 0.06$ & 0.04 \\
        & jet knot  & 1.2 & 2.4 &  -- &  -- &   -- & 0.4 \\
        & S lobe    & 1.2 &  10 &  -- &  -- &   -- & 1.2 \\
        & S hotspot & 2.3 & 8.6 &  -- &  -- &   -- & 0.4 \\
        & N lobe    & 5.7 &  22 &  -- &  -- &   -- & 0.8 \\
        & N hotspot &  13 &  20 & 4.3 & 12  & $0.52 \pm 0.02$ & 0.4 \\
        & total     &  -- &  63 &  -- & 14  & $1.53 \pm 0.02$ & 3 \\
\hline 
1855+37 & core  & 0.6 &  0.9 & -- & -- & -- & 0.3 \\
        & total &  -- & 35.9 & -- & -- & -- & 8 \\
\hline 
\end{tabular}
}\smallskip
Note -- Uncertainties in Col.~7 are $1\sigma$ values based on the absolute
flux calibration and noise in the images. The core region in 0258+35 and the
northern lobe in 0648+27 are resolved in two components at 22~GHz, therefore we
give two values in Col.~6 and the spectral index is spurious. See Table
\ref{res_vlba} for a more reliable estimate of the cores spectral index. The
source 1855+37 is not detected at 22~GHz.
\end{table}