\begin{table}%t4
\caption{\label{table:3}Newly derived coordinates, half-light radius, integrated magnitudes, reddening, age and metallicity for the cluster~VdB0. The origin of each parameter is described in the last column.}             
\par
%\centering
\small
\begin{tabular}{c c c}        
\hline\hline                 
par & Value & Note \\    
\hline   
&& \\[-8pt]
$\alpha_{J2000}$& $\rm 00^h$$\rm 40^m$$\rm 29.4^s$               & from 2MASS-XSC\\                  $\delta_{J2000}$& $+40\degr$$36\arcmin$$15.2\arcsec$ & from 2MASS-XSC \\                  
\hline                        
$r_{\rm h}$       & 1\farcs93 $\pm$ 0\farcs66  & from intensity profile (i.p.)
fit \\    
\hline
$B$     &  14.94 $\pm$ 0.09  & $r=14$\farcs4 ap. phot. on M06 images\\                               $V$     &  14.67 $\pm$ 0.05  & $r=14$\farcs4 ap. phot. on M06 images\\                               $R$     &  14.45 $\pm$ 0.11  & $r=14$\farcs4 ap. phot. on M06 images\\                               $I$     &  14.01 $\pm$ 0.11  & $r=14$\farcs4 ap. phot. on M06 images\\                               $J$     &  13.26 $\pm$ 0.07  & $r=15$\farcs0 ap. phot. from 2MASS-XSC\\                              $H$     &  12.76 $\pm$ 0.12  & $r=15$\farcs0 ap. phot. from 2MASS-XSC\\                              $K$     &  12.77 $\pm$ 0.15  & $r=15$\farcs0 ap. phot. from 2MASS-XSC\\                              \hline    
age & 25 Myr               & value of adopted best-fit isochrone\\ 
$Z$   & 0.019                & value of adopted best-fit isochrone\\                             
$E(B-V)$   & 0.20            & adopted best-fit value\\                             
\hline    
\end{tabular}
\end{table}