\begin{table}%t8
  \caption{\label{tab:final}The Effelsberg measured flux densities along with the NVSS ones and the computed spectral indices (it is assumed that $S\sim \nu^{\alpha}$).}   
%\centerline
{                    
  \begin{tabular}{l r r r r r r r c r c r c} 
    \hline\hline
\multicolumn{1}{c}{Source} &\multicolumn{1}{c}{$S_{1.4}$} &\multicolumn{1}{c}{err} &\multicolumn{1}{c}{$S_{4.85}$} &\multicolumn{1}{c}{err} &\multicolumn{1}{c}{$S_{10.45}$} &\multicolumn{1}{c}{err}  &\multicolumn{1}{c}{$\alpha_{1.4}^{4.85}$} &err &\multicolumn{1}{c}{$\alpha_{4.85}^{10.45}$} &err &\multicolumn{1}{c}{$\alpha$} &err\\
&\multicolumn{1}{c}{(mJy)} &\multicolumn{1}{c}{(mJy)} &\multicolumn{1}{c}{(mJy)} &\multicolumn{1}{c}{(mJy)} &\multicolumn{1}{c}{(mJy)} &\multicolumn{1}{c}{(mJy)} & & & &  &  &\\
    \hline                         
023958+0137 &4.0 &0.5 &$<$12.5 &  &$<$8.0 &  & &  &  &  & &  \\
024013+0127 &9.4 &0.6 &$<$6.0 &  &$<$6.5 &  & &  &  &  & &  \\
024031+0140 &3.6 &0.5 &$<$18.5 &  &$<$9.5 &  & &  &  &  & &  \\
024057+0129 &7.3 &0.6 &$<$6.0 &  &$<$6.5 &  & &  &  &  & &  \\
024058+0133 &7.5 &0.5 &$<$7.5 &  &$<$12.0 &  & &  &  &  & &  \\
024119+0126 &7.8 &0.6 &9.3 &1.2 &$<$16.0 &  &$+$0.14 &0.12 &  &  & &  \\
024124+0154 &49.0 &1.5 &15.6 &2.0 &$<$14.5 &  &$-$0.92 &0.11 &  &  & &  \\
024234+0135 &58.2 &1.8 &35.7 &1.3 &24.9 &1.4 &$-$0.39 &0.04 &$-$0.47 &0.09 &$-$0.41 &0.02  \\
024402+0140 &4.2 &0.5 &$<$19.5 &  &$<$6.5 &  & &  &  &  & &  \\
024456+0141 &12.3 &0.6 &$<$7.5 &  &$<$8.0 &  & &  &  &  & &  \\
    \hline                         
 \end{tabular}}
\par
  \medskip
   Cases of $\textit{SNR}< 5$ at either of 4.85 or 10.45~GHz are noted
    with upper limits of $5\sigma$. The source name is marked with
    $^{\star}$ or $^{\dagger}$ in case de-confusion correction has
    been applied at 4.85 or 10.45 GHz, respectively. The complete
    table is available in electronic form at the CDS.
\end{table}