\begin{table}%T1
%\centering
\par
\caption{The completeness magnitudes. ${m^{\rm c}}$ is the
completeness magnitude as estimated on the photometric catalogues
according to Garilli et al. (\cite{GAR99}). ${m^{\rm c}_{\rm zp}}$
defines the central position of the faintest magnitude bin with
completeness higher than $50\%$ in the sample with photometric
redshifts (see Sect.~\ref{BS}). The bin width is 0.5 mag.}
\label{TABCOMP}
\begin{tabular}{ccc}
\hline\hline
%\noalign{\smallskip}
{Band} & ${m^{\rm c}}$ & ${m^{\rm c}_{\rm zp}}$\\
& {mag} & {mag}  \\
%\noalign{\smallskip}
\hline
%\noalign{\smallskip}
{$V$} & 25.7 & 24.25 \\
{$R$} & 25.0 & 23.25 \\
{$I$} & 23.2 & 22.75 \\
{$K$} & 21.2 & 19.75 \\
%\noalign{\smallskip}
\hline
\end{tabular}
\end{table}