\begin{table}%t4
\caption{Relevant parameters for double sources.}\label{tab:b3-doppie}
%\centering
\par
\begin{tabular}{lcrrrcc}
\hline \hline
 Source & C & $\Sc$ & $\Sx$ & $\Su$ & $\alpha$ & arm-length \\
  &  & mJy   & mJy  & mJy   & & $h^{-1}$ kpc  \\
 (1) & (2) & (3) & (4) & (5) & (6) & (7) \\
\hline
\object{0003+387} &    N     &      53.5 &  22.7 &  7.5  &  [1.77]  &        \\  
                  &    S     &      51.9 &  22.8 & 10.2  &   1.46   &        \\  
\object{0039+398} &    E     &      11.0 &   4.9 &  2.7  &  [1.26]  &  6.27  \\  
                  &    W     &     214.1 & 111.9 & 59.4  &   1.15   &  9.55  \\  
\object{0039+412} &    N     &      90.1 &  48.8 & 26.3  &   1.11   &  3.83  \\  
                  &    S     &      14.8 &   7.7 &  2.2  &  [1.72]  &  4.67  \\  
\object{0041+425} &    N     &      53.7 &  26.6 & 11.9  &   1.36   &        \\  
                  &    S     &      88.5 &  48.0 & 30.7  &  [0.95]  &        \\  
\object{0049+379} &    N     &     124.6 &  56.7 & 28.1  &   1.34   &  4.57  \\  
                  &    S     &      50.2 &  19.7 &  8.6  &   1.58   &  1.55  \\  
\object{0120+405} &    E     &     133.8 &  68.1 & 33.2  &   1.25   &  5.79  \\ 
                  &    W     &      35.5 &  19.7 &  9.9  &   1.15   &  4.43  \\ 
\object{0123+402} &    N     &       2.6 &   1.6 &$<$0.3 &   0.90   &        \\  
                  &    S     &      34.9 &  18.1 &  8.1  &   1.31   &        \\  
\object{0128+394} &    N     &      44.5 &  19.7 & 14.5  &  [1.00]  &        \\  
                  &    S     &      36.6 &  17.9 &  4.0  &  [2.00]  &        \\  
\object{0137+401} &    N     &      19.9 &   9.2 &  2.4  &  [1.91]  &  8.69  \\  
                  &    S     &      36.0 &  19.9 &  9.4  &   1.21   &  8.95  \\  
\object{0140+387} &    N     &      41.6 &  11.8 &  5.5  &  [1.81]  &        \\  
                  &    S     &      35.5 &  14.2 &  4.2  &  [1.92]  &        \\  
\object{0144+432} &    S     &      67.3 &  34.9 & 17.6  &   1.20   &        \\  
                  &    N     &      32.7 &  19.8 & 15.7  &  [0.66]  &        \\  
\object{0213+412} &    N     &      30.0 &  14.0 &  5.6  &   1.51   &  3.86  \\  
                  &    S     &      55.1 &  27.7 & 12.2  &   1.36   &  3.91  \\  
\object{0222+422} &    N     &      46.6 &  22.1 &  7.7  &  [1.62]  &        \\  
                  &    S     &      19.1 &   9.9 &  3.6  &  [1.50]  &        \\  
\object{0228+409} &    E     &      24.1 &  13.8 &  8.0  &   0.99   &        \\  
                  &    W     &      76.0 &  40.8 & 20.1  &   1.20   &        \\  
\object{0254+406} &    N     &      44.0 &  21.0 &  8.6  &   1.47   &        \\  
                  &    S     &     103.1 &  58.9 & 36.8  &   0.93   &        \\  
\object{0255+460} &    E     &      75.3 &  39.9 & 11.4  &  [1.70]  &        \\  
                  &    W+C   &     167.2 &  93.3 & 57.6  &   0.96   &        \\  
\object{0701+392} &    E     &      32.5 &  20.7 &  7.4  &  [1.34]  &  4.03  \\  
                  &    W     &     144.3 &  85.2 & 47.7  &   1.00   &  3.73  \\  
\object{0729+437} &    N     &      22.4 &  14.4 &  5.8  &  [1.22]  &  4.17  \\  
                  &    S     &     111.4 &  67.5 & 42.7  &   0.86   &  1.49  \\  
\object{0744+464} &    E     &      18.5 &   9.1 &  3.6  &   1.47   &  3.36  \\  
                  &    W     &     124.9 &  71.5 & 43.5  &   0.95   &  1.77  \\  
\object{0809+404} &    E     &     407.6 & 263.3 &156.7  &   0.86   &        \\  
                  &    W     &       4.2 &   3.5 &  2.0  &  [0.67]  &        \\  
\object{0810+460} &    S     &     144.8 &  83.2 & 46.4  &   1.02   &        \\ 
                  &    N     &     140.3 &  73.5 & 28.0  &   1.45   &        \\  
\object{0814+441} &    E     &      40.2 &  22.3 &  7.7  &  [1.49]  &  3.15  \\  
                  &    W     &      22.7 &  11.5 &  2.6  &  [1.96]  &  3.87  \\  
\object{0856+406} &    E     &      24.6 &   9.6 &  4.7  &  [1.49]  &        \\  
                  &    W     &      13.7 &   5.7 &$<$0.2 &   1.63   &        \\  
\hline
\object{0930+389} &    N     &      32.6 &  18.5 &  7.3  &  [1.35]  &        \\  
                  &    S     &      37.4 &  21.0 & 12.8  &   0.96   &        \\  
\object{0935+428} &    E     &      63.3 &  34.6 & 24.3  &  [0.86]  &  3.04  \\  
                  &    W     &      57.9 &  32.8 & 12.1  &  [1.41]  &  2.75  \\  
\object{0951+422} &    N     &      70.5 &  45.5 & 22.1  &  [1.05]  &        \\ 
                  &    S     &      28.5 &  14.7 &  4.8  &  [1.61]  &        \\  
\object{0955+390} &    E     &      63.8 &  38.0 & 14.0  &   1.11   &  8.49  \\  
                  &    W     &      85.3 &  51.8 & 26.9  &  [1.97]  &  6.40  \\  
\object{1025+390} &    N     &      50.5 &  32.0 & 13.7  &  [1.18]  &  2.44  \\  
                  &    S     &      89.1 &  53.5 & 25.3  &  [1.13]  &  2.82  \\  
\object{1044+454} &    N     &      86.2 &  39.6 & 21.4  &  [1.25]  &        \\  
                  &    S     &       3.3 &   1.3 &  1.3  &  [0.83]  &        \\ 
\object{1136+420} &    E     &       9.0 &   4.5 &$<$1.4 &   1.29   &        \\  
                  &    W     &     164.5 & 105.3 & 61.0  &   0.89   &        \\  
\object{1143+456} &    N     &      20.8 &   9.2 &  4.0  &   1.48   &        \\  
                  &    S     &     116.7 &  55.7 & 27.7  &   1.29   &        \\  
\object{1157+460} &    N     &     218.3 & 127.4 & 61.5  &   1.14   &  0.80  \\  
                  &    S     &     118.1 &  59.3 & 17.4  &  [1.73]  &  1.29  \\  
\object{1201+394} &    N     &      54.2 &  32.9 &  9.3  &  [1.59]  &  4.54  \\  
                  &    S     &     104.9 &  65.9 & 28.5  &  [1.17]  &  3.84  \\  
\object{1204+401} &    N     &      39.9 &  23.0 &  3.4  &  [2.23]  &        \\  
                  &    S     &      18.5 &   9.0 &  6.8  &  [0.90]  &        \\  
\object{1216+402} &    N     &      42.3 &  23.5 &  8.7  &  [1.43]  &        \\  
                  &    S     &      63.6 &  37.6 & 13.4  &  [1.40]  &        \\  
\object{1217+427} &    N     &      57.7 &  33.6 & 22.7  &  [0.84]  &        \\  
                  &    S     &      31.5 &  18.4 &  8.5  &  [1.18]  &        \\  
\object{1220+408} &    N     &      28.0 &  16.7 &  4.4  &  [1.67]  & 11.20  \\  
                  &    Se    &      73.0 &  39.5 & 15.5  &  [1.40]  &  6.47  \\  
\object{1233+418} &    N     &      55.7 &  38.9 & 24.4  &   0.74   &        \\  
                  &    S     &     141.5 &  98.4 & 64.8  &   0.70   &        \\  
\object{1241+411} &    E     &      37.7 &  24.7 & 10.8  &  [1.13]  &        \\  
                  &    W     &     119.7 &  82.1 & 48.1  &   0.82   &        \\  
\object{1458+433} &    N     &      77.2 &  45.8 & 22.7  &   1.10   &  1.99  \\  
                  &    S     &      37.5 &  22.1 &  9.2  &  [1.27]  &  5.14  \\  
\object{2302+402} &    N     &     375.5 & 194.0 & 95.1  &   1.23   &  1.23  \\  
                  &    S     &      71.9 &  35.7 & 24.1  &  [0.98]  &  1.21  \\  
\object{2311+469} &    N     &     422.5 & 255.0 &170.5  &   0.81   &  6.09  \\  
                  &    S     &     221.7 & 111.6 & 63.2  &   1.13   &  3.36  \\  
\object{2322+403} &    N     &      24.0 &  12.7 &  7.1  &   1.09   &  6.00  \\  
                  &    S    &$\star$72.1 &  36.2 & 17.8  &   1.26   &  4.00  \\  
\object{2349+410} &    E    &$\star$78.4 &  42.4 & 30.2  &  [0.85]  &  1.57  \\  
                  &    W+Wo  &      39.7 &  17.2 &  4.6  &  [1.94]  &  1.76  \\  
\hline
\end{tabular}
\medskip
Sub-components from Table~\ref{tab:b3-parameters} have been summed into major  "lobes''.
Column~1: source name;
Col.~2: component;
Col.~3: 4.9~GHz flux density;
Col.~4: 8.5~GHz flux density;
Col.~5: 15~GHz flux density;
Col.~6: three-frequency spectral index;
Col.~7: hot-spot component distance from the~core.
\end{table}