\begin{table}%T3
\caption{\label{phistar_noevol}Normalizing amplitudes~$\phi_0$~and~$\phi^*$~of the Gaussian
and Schechter components of the early-type, intermediate-type and
\emph{non-evolving} late-type luminosity functions of the ESO-Sculptor
survey, in the Johnson-Cousins~$B$,~$V$~and~$R_{\rm c}$~bands.}
%\centerline
{
\begin{tabular}{lcccccccccc}
\hline 
\hline 
& \multicolumn{5}{l}{($\Omega_{\rm m}$,~$\Omega_\Lambda)=(0.3$,~0.7)} & \multicolumn{5}{l}{($\Omega_{\rm m}$,~$\Omega_\Lambda)=(1.0$,~0.0)}\\ 
              & Early-type & \multicolumn{2}{c}{Intermediate-type} & \multicolumn{2}{c}{Late-type} & Early-type & \multicolumn{2}{c}{Intermediate-type}& \multicolumn{2}{c}{Late-type}\\
                     &~$\phi_0$~ &~$\phi_0$~ &~$\phi^*$~ &~$\phi_0$~ &~$\phi^*$~&~$\phi_0$~ &~$\phi_0$~ &~$\phi^*$~ &~$\phi_0$~ &~$\phi^*$~ \\
\hline
$R_{\rm c}\le21.5$~&~$0.00310$~&~$0.00296$~&~$0.00387$~&~$0.00339$~&~$0.03678$~&~$0.00504$~&~$0.00489$~&~$0.00639$~&~$0.00520$~&~$0.05649$~\\
$V\le21.0$~          &~$0.00323$~&~$0.00287$~&~$0.00375$~&~$0.00271$~&~$0.02939$~&~$0.00497$~&~$0.00444$~&~$0.00581$~&~$0.00410$~&~$0.04450$~\\
$B\le22.0$~          &~$0.00344$~&~$0.00294$~&~$0.00385$~&~$0.00299$~&~$0.03247$~&~$0.00523$~&~$0.00458$~&~$0.00600$~&~$0.00457$~&~$0.04961$~ \\
\hline
\end{tabular}}
\smallskip
\begin{list}{}{}
\item[{Notes:}]
\item[--]The listed values of~$\phi_0$~and~$\phi^*$~are in units of
\phiunit, and are obtained with~$H_0 = 100 h$~km~s$^{-1}$~Mpc$^{-1}$.
\item[--]$\phi_0$~and~$\phi^*$~are calculated
by normalizing the integral of the expected redshift distribution with
the listed apparent magnitude limit to the observed number of galaxies
in the interval~$0.01\le z\le0.81$~(see \sct~\ref{nz}).
\item[--]The value of~$\phi^*$~for the \emph{intermediate-type}
and \emph{late-type} galaxies is related to the corresponding value of~$\phi_0$~by the ratio~$\phi_0/0.4\ln10\;\phi^*$, listed in
Table~\ref{lf_BVR}.
\end{list}
\end{table}