\begin{table}%T3
\par
\caption{WSRT observation details.}
\label{tab:wsrtobs}
%\centerline
{
\begin{tabular}{lcc}%{cclc}
\hline\hline
Galaxy    & Array$^a$ & Date \\
\hline
NGC~4244 & 36 & 2003, Feb. 13 \\
          & 54 & 2003, Feb. 19 \\
          & 72 & 2003, Feb. 20 \\
          & 90 & 2003, Apr. 13 \\
NGC~4565 & 36 & 2003, Feb. 16 \\
          & 54 & 2003, Apr. 14 \\
          & 72 & 2003, May 14 \\
          & 90 & 2003, May 19 \\
\hline
\end{tabular}}
\par
\medskip
Note: \\
$^{a}$ The so-called "traditional'' array configuration was used
in all cases (see WSRT documentation for details). We list
here the shortest RT9$-$RTA baselines of the four configurations
that the traditional array configuration comprises.
\end{table}