\begin{table}%t6
  \caption{\label{tab:confflavors}The frequencies of confusion flavors of the observed 
    scans (measurements) for each field and observing frequency.}  
  %\centerline
{
  \begin{tabular}{ccrrr} 
    \hline\hline                 
    Field  &{\it Clean} &\multicolumn{1}{c}{\it Cluster$^\star$} &\multicolumn{1}{c}{\it Confused}&\multicolumn{1}{c}{\it de-confused} \\    
           &(\%) &\multicolumn{1}{c}{(\%)} &\multicolumn{1}{c}{(\%)} &\multicolumn{1}{c}{(\%)} \\    \hline    
         &\multicolumn{4}{c}{4.85~GHz ($FWHM\approx145\arcsec$)} \\
    \cline{2-5}                   
    02$^{\rm h}$     &59  &18  &23 &4 (17)\\
    08$^{\rm h}$     &57  &18  &25 &9 (36)\\
    14$^{\rm h}$     &60  &20  &20 &4 (20)\\
    20$^{\rm h}$     &59  &19  &22 &6 (27) \\
    Average      &59  &19  &22 &6 (27) \\ 
         &\multicolumn{4}{c}{10.45~GHz ($FWHM\approx67\arcsec$)} \\
    \cline{2-5}                   
    02$^{\rm h}$     &92  &1  &7  &0  (0) \\
    08$^{\rm h}$     &93  &2  &5  &0  (0) \\
    14$^{\rm h}$     &90  &1  &9  &2 (22)\\
    20$^{\rm h}$     &92  &2  &6  &1 (17) \\
  Average       &92  &$\sim $1  &$\sim $7  &$\sim $2 (20)\\
    \hline                                  
  \end{tabular}}
\par
  \medskip
   It must be made clear that this result is based solely on the
    position of the dual-beam system in the sky and the spatial
    distribution of the field NVSS radio sources. In Col.~5 we give
    the fraction of the total number of scans that have been
    de-confused and in parenthesis the same number but as a fraction
    of the confused scans which is given in Col.~4.\\
  $^\star$ Here the term {\it cluster} is meant to represent
    both, the cases of pure clustering flavour and those that are
    clustered and confused \mbox{simultaneously}.
\end{table}