\begin{table}%t2
\caption {\label{table:2}Sample of methanol masers observed with the EVN. The names
are the Galactic coordinates of the brightest spot of each target
obtained in post-processing EVN data. The dates of each observing run
are listed in Table \ref{table:4}. The phase-calibrator names and
angular separations from the targets are given.}     
%\centerline
 {          
\begin{tabular}{cccc}     
\hline\hline       
Source&  Observing & Phase-calibrator& Separation \\
Gll.lll~$\pm$~bb.bbb& run      &                  &  (\fdg) \\
\hline                    
 G21.407$-$00.254 & 3a & J1825$-$0737 & 3.1 \\
 G22.335$-$00.155 & 3a & J1825$-$0737 & 2.5 \\
 G22.357$+$00.066$^1$ & 4a & J1825$-$0737 & 2.3 \\
 G23.207$-$00.377 & 2  & J1825$-$0737 & 2.6 \\
 G23.389$+$00.185 & 2  & J1825$-$0737 & 2.1 \\
 G23.657$-$00.127 & 2  & J1825$-$0737 & 2.4 \\
                  & 3a & J1825$-$0737 & 2.4 \\
                  & 4a & J1825$-$0737 & 2.4 \\                 
 G23.707$-$00.198 & 2  & J1825$-$0737 & 2.5 \\
                  & 3a & J1825$-$0737 & 2.5 \\
 G23.966$-$00.109 & 3a & J1825$-$0737 & 2.5 \\
 G24.148$-$00.009 & 3a & J1825$-$0737 & 2.4 \\
 G24.541$+$00.312 & 2  & J1825$-$0737 & 2.4 \\
 G24.634$-$00.324 & 4a & J1825$-$0737 & 2.9 \\
 G25.411$+$00.105$^2$ & 4a & J1825$-$0737 & 3.1 \\
 G26.598$-$00.024 & 4a & J1825$-$0737 & 4.1 \\
 G27.221$+$00.136 & 2  & J1825$-$0737 & 4.5 \\
 G28.817$+$00.365 & 4b & J1834$-$0301 & 2.2 \\
 G30.318$+$00.070 & 4b & J1834$-$0301 & 3.2 \\
 G30.400$-$00.296 & 4b & J1834$-$0301 & 3.5 \\
 G31.047$+$00.356 & 4b & J1834$-$0301 & 3.5 \\
 G31.156$+$00.045 & 4b & J1834$-$0301 & 3.8 \\
 G31.581$+$00.077 & 4b & J1834$-$0301 & 4.1 \\
 G32.992$+$00.034$^2$ & 4c & J1907$+$0127 & 4.2 \\
 G33.641$-$00.228 & 1  & J1907$+$0127 & 3.5 \\
 G33.980$-$00.019 & 4c & J1907$+$0127 & 3.5 \\
 G34.751$-$00.093 & 4c & J1907$+$0127 & 3.0 \\
 G35.793$-$00.175 & 1  & J1907$+$0127 & 2.7 \\
 G36.115$+$00.552 & 1  & J1907$+$0127 & 3.4 \\
                  & 4c & J1907$+$0127 & 3.0 \\
 G36.705$+$00.096 & 4c & J1907$+$0127 & 3.1 \\
 G37.030$-$00.039 & 3b & J1856$+$0610 & 2.6 \\
 G37.479$-$00.105 & 3b & J1856$+$0610 & 2.4 \\
 G37.598$+$00.425 & 3b & J1856$+$0610 & 1.9 \\
 G38.038$-$00.300 & 3b & J1856$+$0610 & 2.2 \\
 G38.203$-$00.067 & 3b & J1856$+$0610 & 2.0 \\
 G39.100$+$00.491 & 3b & J1856$+$0610 & 1.2 \\
\hline
\end{tabular}}
\par
\smallskip
{$^1$ Source from Walsh et~al. (\cite{walsh98}).}\\
{$^2$ Sources from Beuther et~al. (\cite{beuther02}).}                                      
\end{table}