\begin{table}%t4
\caption{\label{tab:catalogtab}WINGS-NIR catalogs useful parameters$^a$.}
\par
%%\centerline

{\small
\begin{tabular}{lcccccccccc}
\hline\hline
Cluster & DM & Band & $m_{\lim}$ & ${\mu}_{\rm thresh}$ & Cum &
\multicolumn{2}{c}{Stars} &
\multicolumn{2}{c}{Gals} & Notes\\
%\cline{7-8}\cline{9-10}
  & & mag & mag & mag/$''^2$ & Det&Det& Clas & Det & Clas &\\
\hline
A119         &36.46 & $K$ & 21.2 &  21.02  &  20.0  & 19.8 & 18.2 & 19.3 & 19.0 & \\%\hline
A376          & 36.66 & $J$ & 21.5 &  22.11  &   20.2 & 20.4 & 19.0 & 20.0 & 19.6 & 1\\%\hline
              && $J$ & 21.6 &  21.93  & 21.0   & 20.0 & 18.0 & 19.6 & 19.2 & 1,~2	\\
\rb{A500}     &\rb{37.40} & $K$ & 20.8 &  21.02  &  19.7  & 19.2 & 17.7 & 18.7 & 18.3 & 2,~4\\%\hline
A602         & 37.22 & $K$ & 21.2 &  21.68  & 20.0   & 20.3 & 18.7 & 19.3 & 19.2 & 1,~3\\%\hline
             && $J$ & 21.5 &  22.11  &  20.3  & 20.3 & 18.5 & 19.8 & 19.4 & 2,~4	\\
\rb{A957x}    &\rb{36.43} & $K$ & 21.1 &  21.49  &  20.0  & 20.0 & 18.7 & 19.7 & 19.4 & 	\\%\hline
             && $J$ & 21.8   & 22.31    & 21.0    & 20.6   & 18.6    & 20.0  & 19.5   & 2		\\
\rb{A970}    &\rb{37.10} & $K$ & 20.9 &  21.13  & 19.7   & 19.5 & 17.7 &18.9 & 18.5 & 1,~4  \\%\hline
             & & $J$ & 21.9 &  21.95 &  21.2  & 20.2 & 18.6 & 19.8 & 19.5 & 5,~6	\\ 
\rb{A1069}   &\rb{37.33} & $K$ & 20.6 &  21.32  & 19.2   & 20.3 & 18.7 & 19.7 & 19.4 & \\%\hline
             & & $J$ & 21.8 &  22.37  & 21.0   & 21.1 & 19.2 & 20.3 & 20.2 & 	\\
\rb{A1291}   &\rb{36.85} & $K$ & 20.6 &  21.29  & 19.5   & 19.5 & 18.2 & 19.0 & 18.8 & 1,~2,~5\\%\hline
              && $J$ & 21.2 &  22.09  & 20.0   & 20.1 & 18.5 & 19.5 & 19.1 & 	\\
\rb{A1631a}   &\rb{36.56} & $K$ & 20.7 &  21.02  & 19.1   & 19.7 & 18.4 & 19.3 & 18.7 & 1,~3\\%\hline
              && $J$ & 21.8 &  21.98  &  20.2  & 20.7 & 19.2 & 20.0 & 19.6 & 1,~4 	\\
\rb{A1644}    &\rb{36.61} & $K$ & 20.6 &  20.90  & 19.0  & 19.5 & 18.1 & 18.9 & 18.7 & 1,~4,~6\\%\hline
              && $J$ & 22.0 &  22.27  & 21.5   & 20.1 & 18.0 & 19.8 & 18.0 & 2,~5 	\\
\rb{A1795}    &\rb{37.24} & $K$ & 20.8 &  21.07  & 19.0  & 19.1 & 18.0 & 18.7 & 18.5 & 2	\\%\hline
              && $J$ & 21.7 &  22.34  & 21.1 & 21.0   & 19.5  & 20.5  & 20.1    & 6	\\
\rb{A1831}    &\rb{37.20} & $K$ & 20.5 &  21.19  & 19.3 & 19.3 & 17.5 & 19.0 & 18.6 & 1,~6	\\%\hline
              && $J$ & 21.9 &  22.63  & 20.6 & 21.0 & 19.5 & 20.3 & 20.0 & 1,~4	\\
\rb{A1983}    &\rb{36.43}  & $K$ & 20.2 &  20.74  & 18.9 & 19.0 & 18.0 & 18.5 & 18.5 & 4	\\%\hline
A1991         & 37.10 & $J$ & 21.7 &  22.10  &  21.1  & 20.8 & 19.0 &20.0 & 19.5 & 	\\ %\hline
              && $J$ & 21.7 &  22.22  &  21.2  & 20.7 & 19.1 & 20.0 & 19.6 & 2	\\
\rb{A2107}    &\rb{36.30} & $K$ & 20.8 &  21.08  & 19.2 & 19.2 & 18.0 & 19.3 & 19.1 & 1,~4	\\%\hline
              && $J$ & 21.7 &  22.29  &  21.2  & 20.2 & 18.7 & 20.0 & 19.7 & 	\\
\rb{A2124}    &\rb{37.35} & $K$ & 21.1 &  21.36  & 20.0   & 19.8 & 18.3 & 19.2 & 19.1 & 	\\%\hline
A2149         & 37.43 & $K$ & 20.9 &  21.11  &  20.0  & 19.7 & 18.3 & 19.3 & 19.0 & 6	\\%\hline
              && $J$ & 21.7 &  22.14  & 21.0   & 20.8 & 19.1 & 20.1 & 19.8 & 	\\
\rb{A2169}    &\rb{37.09} & $K$ & 20.6 &  20.99  & 19.7   & 19.5 & 18.2 & 19.3 & 18.9 & 	\\%\hline
A2382         & 37.21 & $K$ & 20.3 &  20.57  &  19.5  & 19.2 & 17.7 & 18.8 & 18.3 & 2	\\%\hline
A2399         & 37.07 & $K$ & 20.8 &  21.04  &  19.6  & 19.5 & 18.2 & 19.2 & 18.6 & 1,~4	\\%\hline
A2457         & 37.12 & $K$ & 20.9 &  21.14  &  19.8  & 19.7 & 18.0 & 19.3 & 18.7 & 4	\\%\hline
A2572a        & 36.25 & $K$ & 21.0 &  21.25  &  19.9  & 19.7 & 18.4 & 19.3 & 19.2 & 2,~5	\\%\hline
A2589         & 36.31 & $K$ & 21.1 &  21.36  &  20.0  & 19.8 & 18.0 & 19.5 & 18.8 & 2,~5	\\%\hline
             && $J$ & 21.5 &  21.83  & 20.4   & 20.5 & 19.0 & 19.8 & 19.0 & 1,~2,~4	\\
\rb{IIZW108} &\rb{36.70} & $K$ & 21.03 &  21.32  & 19.8   & 19.8 & 18.3 & 19.5 & 19.0 & 1,~4,~6\\%\hline
             && $J$ & 21.9 &  22.56  & 20.5   & 21.0 & 19.6 & 20.3 & 20.0 & 1	\\
\rb{MKW3s}   &\rb{36.50} & $K$ & 21.0 & 21.35 & 20.0   & 19.7  & 18.3  & 19.3  & 18.7  & 	2,~4\\%\hline
             && $J$ & 21.5 &  22.10  &  20.2  & 20.5 & 18.9 & 19.9 & 19.6 & 	2	\\
\rb{RX1022}  &\rb{36.69} & $K$ & 21.2 &  21.53  & 20.1   & 19.8 & 18.2 & 19.3 & 19.2 & 2	\\%\hline
RX1740       & 36.40 & $K$ & 20.6 &  20.86  & 19.1   & 19.1 & 17.8 & 18.7 & 18.2 & 1,~2,~4	\\%\hline
             && $J$ & 21.7 &  22.16  & 20.9   & 20.7 & 19.2 & 20.0 & 19.9 & 2		\\
\rb{Z8338}   &\rb{36.61} & $K$ & 20.7 &  21.06  & 19.5   & 19.6 & 18.6 & 19.3 & 18.9 &	\\
\hline
\end{tabular}}
\par
\medskip
$^a$~The Cluster   column identifies  the   cluster, the DM  column  is the
cluster  distance modulus in magnitudes,  the $m_{\lim}$ column is
the    theoretical  magnitude   detection    limit calculated     with
Eq.~(\ref{eq:mlim}),  ${\mu}_{\rm thresh}$ column is the minimum surface
brightness  at  the     detection  threshold   cut    calculate   with
Eq.~(\ref{eq:mulim}),  the cumulative   detection column (``Cum  Det'')
lists the turnover magnitude of the number  counts diagram for all the
detected sources (see  Fig.~\ref{fig:limiting}), ``Stars'' and ``Gals''
columns   represent the   average   90{\%} completeness   detection  and
classification   limits for   stars  and  galaxies   as  deduced  from
simulations. 
\\
Notes legend:\\ 1:=  patchy and/or noisy background; 2:=
strongly  variable PSF; 3:=  many spurious  detections; 4:= excess of
classified stars; 5:= deficient in classified stars; 6:= exceptionally
bright star(s).
\end{table}