\begin{table}%t4
\caption{\label{3a}SDSS photometry of LGG 225 members.}
%\centering
\par
\begin{tabular}{lllllllllcll}
\hline\hline\noalign{\smallskip}
 Galaxy &  $u$  & $g$ & $r$ & $i$ & $z$  \\
    & [AB mag]  &  [AB mag]  &[AB mag] &[AB mag] &[AB mag]     &    \\
\hline
NGC 3370 &      13.31 $\pm$ 0.06& 12.31 $\pm$ 0.02& 11.85 $\pm$ 0.03& 11.59 $\pm$ 0.03& 11.38 $\pm$ 0.06 \\   
NGC 3443\tablefootmark{b} &  15.91 $\pm$ 0.14& 14.79 $\pm$ 0.05& 14.33 $\pm$ 0.05& 14.11 $\pm$ 0.06& 13.90 $\pm$ 0.18 \\ 
NGC 3447\tablefootmark{b}  & 14.47 $\pm$ 0.12& 13.22 $\pm$ 0.04& 12.90 $\pm$ 0.05& 12.78 $\pm$ 0.06& 12.06 $\pm$ 0.10   \\ 
NGC 3447A&      15.34 $\pm$ 0.16& 14.89 $\pm$ 0.09& 14.71 $\pm$ 0.13& 14.65 $\pm$ 0.19& 14.32 $\pm$ 0.44  \\  
NGC 3454 &      15.08 $\pm$ 0.12& 13.84 $\pm$ 0.03& 13.23 $\pm$ 0.03& 12.91 $\pm$ 0.04& 12.66 $\pm$ 0.09  \\  
NGC 3455 &      13.98 $\pm$ 0.09& 13.02 $\pm$ 0.03& 12.66 $\pm$ 0.04& 12.50 $\pm$ 0.05& 12.31 $\pm$ 0.12  \\  
NGC 3457 &      14.69 $\pm$ 0.06& 13.05 $\pm$ 0.02& 12.37 $\pm$ 0.02& 12.01 $\pm$ 0.02& 11.77 $\pm$ 0.04 \\ 
NGC 3501 &      14.41 $\pm$ 0.07& 13.06 $\pm$ 0.02& 12.40 $\pm$ 0.02& 11.99 $\pm$ 0.03& 11.68 $\pm$ 0.05 \\                
NGC 3507\tablefootmark{a,b} & 12.16  $\pm$ 0.02& 10.75  $\pm$ 0.02& 10.18  $\pm$ 0.02& 9.78  $\pm$ 0.02& 9.62  $\pm$ 0.03 \\   
NGC 3522 &      15.16 $\pm$ 0.11& 13.59 $\pm$ 0.03& 12.88 $\pm$ 0.02& 12.52 $\pm$ 0.03& 12.37 $\pm$ 0.06  \\
UGC 6022 &      16.94 $\pm$ 0.35 & 15.84 $\pm$ 0.11& 15.52 $\pm$ 0.14& 15.38 $\pm$ 0.19& 15.07 $\pm$ 0.51  \\
UGC 6035\tablefootmark{a} &  13.77 $\pm$ 0.11& 12.90 $\pm$ 0.04& 12.21 $\pm$ 0.06& 11.75 $\pm$ 0.05&10.92 $\pm$ 0.13 \\
UGC 6083 &      16.31 $\pm$ 0.17& 15.17 $\pm$ 0.05& 14.71 $\pm$ 0.06& 14.43 $\pm$ 0.07&14.35 $\pm$ 0.23 \\   
UGC 6112\tablefootmark{b}  & 15.22 $\pm$ 0.14& 14.29 $\pm$ 0.05& 13.94 $\pm$ 0.06& 13.76 $\pm$ 0.08&13.75 $\pm$ 0.31 \\
UGC 6171\tablefootmark{a} &  15.50 $\pm$ 0.15& 13.41 $\pm$ 0.05& 13.03 $\pm$ 0.06& 12.79 $\pm$ 0.06&12.69 $\pm$ 0.14 \\
\hline
\end{tabular}
\tablefoot {\tablefoottext{a}{Magnitude of the foreground stars have been subtracted;}
\tablefoottext{b}{Galaxy is near SDSS edge, magnitudes have been computed in a reduced area (elliptical aperture with $a=0.5\arcmin$, $b=0.3\arcmin$ for NGC~3443, with $a=1.6\arcmin$, $b=0.8\arcmin$ for NGC~3447, with $a=1\arcmin$, $b=0.4\arcmin$ for UGC~6112 and aperture of radius~0.9\arcmin\ for NGC~3507 respectively, and scaled to the total area using the UV~ratio to derive their mass.}}
\end{table}