\begin{table}%T6
\caption{Results of modelfit -- VLBA images.\label{res_vlba}}
%\centerline
 {
\begin{tabular}{llrrcc}
\hline\hline
Source & Component & Peak & Flux & Size & $\alpha_{1.6}^{22}$ \\ %&  R.A.} &  Dec.} &  size} \\
 & & $\left(\frac{{\rm mJy}}{{\rm beam}}\right)$ & (mJy) & (mas) \\[1mm] 
\hline
0222+36 & core  & 61 & 71 & 2  & $0.05 \pm 0.02$ \\ %& 02 25 27.32717 & 37 10 27.7458 
        & N jet &  6 & 16 & 13 \\ %&   &  
        & S jet &  3 & 26 & 29 \\ %&   &  
        & total & -- & 102 &  \\
\hline
0258+35 & core  & 3.3 & 7.4 &  6 & $-0.24 \pm 0.02$ \\
        & blob  & 7.5 & 236 & 44 & $0.54 \pm 0.02$ \\
        & total &  -- & 243 & \\
\hline
0648+27 & core  & 4.3 & 10  & 5 & $0.47 \pm 0.03$ \\% & 06 52 02.51671 & 27 27 39.4047
        & jet   & 1.1 & 3.4 & 5 & \\
        & total &  -- & 12.8 & \\
\hline
1037+30 & core  & 3.4 & 3.8 & 5 & $0.14 \pm 0.04$ \\%& 10 40 29.94495 & 29 57 57.79017 
        & hot spot & 1.0 & 40 & 60 & $0.46 \pm 0.02$ \\
        & total &  -- & 14  \\
\hline
1855+37 & \multicolumn{5}{l}{N.D.} \\
\hline 
\end{tabular}
}\smallskip
Note -- The spectral index for 0222+36 is computed considering the total flux
density detected at 1.6~GHz by the VLBA, which extends over a region smaller
than the beam of the VLA at 22~GHz. Spectral index uncertainties are $1\sigma$
values.
\end{table}