\begin{table} %t3
     \caption{\label{fitsLF}Fits to the Luminosity Functions. Errors on the
      ${M^*}$ and~$\alpha$ parameters can be obtained by the
      confidence contours shown in Fig.~\ref{centLF}.}
%\begin{center}
\par
     $$
           \begin{array}{c| c c c c| c c c c }
            \hline\hline
                        {\rm Band} & \multicolumn{4}{c|}{{\rm ~~~~~Single~Schechter~function}~~~~~} & \multicolumn{4}{c}{{ ~~~~~{\rm Two~Schechter~functions}^{a}~}}\\
				\hline
		 		 &~~~~~~{ M^*}~~~~~~&~~~~\alpha~~~~&~~~~~{\chi^{2b}_{\nu}}~~~~~&{P(\chi^2>\chi^2_{\nu})}~&~~~{ M}^*_{\rm faint}~~~&~~\alpha_{\rm faint}~~&~~~{\chi^2_{\nu}}~~~&{P(\chi^2>\chi^2_{\nu})}\\
            \hline
            {B} & -21.03 & -1.26 & 0.96 & 46\% &        &	    &      &      \\
            {V^{c}} & -22.03 & -1.25 & 1.04 & 40\% &	    &       &      &      \\
            {V} & -22.18 & -1.27 & 1.46 & 15\% & -18.72 & -2.00 & 1.09 & 37\% \\
            {R} & -22.48 & -1.20 & 1.24 & 27\% & -19.14 & -1.24 & 1.06 & 39\% \\
                        \hline
            \multicolumn{1}{c} {{\rm     }} & \multicolumn{4}{c}{{\rm ~~~~~Galaxies~on~the~red~sequence}~~~~~} & \multicolumn{4}{c}{}\\
            \hline
            {V} & -22.60 & -1.33 & 2.10 &  2\% &   -18.68	&  -2.19  & 1.68	  &  9 \%   \\
            {R} & -22.76 & -1.27 & 1.30 & 23\% &   -19.15	  &  -1.39     &  1.09    &  37 \% \\
                        \hline
         \end{array}
    $$
\parbox{11.5cm} { 
$^a$ The bright--end LF is fixed (see text).\\
$^b$ The reduced ${\rm \chi^2}$.\\
$^c$ Total observed field (see Sect. \ref{sec:6}).}
%\end{center}
   \end{table}