\begin{table}%T4
\caption{\label{evol_BVR}Evolution rates and zero-points for the amplitudes~$\phi_0$
and~$\phi^*$~of the Gaussian and Schechter components of the late-type
luminosity function in the ESO-Sculptor Survey, as derived from the
number-counts in the Johnson~$B$,~$V$~and Cousins~$R_{\rm c}$
bands.}
%\centerline
{
\begin{tabular}{lcccccccccccc}
\hline 
\hline 
& \multicolumn{6}{l}{($\Omega_{\rm m}$,~$\Omega_\Lambda)=(0.3$,~0.7)} & \multicolumn{6}{l}{($\Omega_{\rm m}$,~$\Omega_\Lambda)=(1.0$,~0.0)}\\ 
            & ~$P_{0.15}$~&~$\phi_0(0.15)$~&~$\phi^*(0.15)$~&~$\gamma$~&~$\phi_0(0)$~&~$\phi^*(0)$~&~$P_{0.15}$~&~$\phi_0(0.15)$~&~$\phi^*(0.15)$~&~$\gamma$~&~$\phi_0(0)$~&~$\phi^*(0)$~ \\
\hline
$R_{\rm c}$~&~$2.2$~&~$0.00252$~&~$0.02732$~&~$1.8$~&~$0.00211$~&~$0.02292$~&~$4.6$~&~$0.00320$~&~$0.03470$~&~$2.5$~&~$0.00287$~&~$0.03119$~\\
$V$~           &~$4.3$~&~$0.00216$~&~$0.02347$~&~$2.5$~&~$0.00186$~&~$0.02019$~&~$5.7$~&~$0.00322$~&~$0.03493$~&~$2.8$~&~$0.00283$~&~$0.03072$~\\
$B$~           &~$3.3$~&~$0.00267$~&~$0.02899$~&~$2.2$~&~$0.00226$~&~$0.02449$~&~$5.0$~&~$0.00355$~&~$0.03857$~&~$2.6$~&~$0.00313$~&~$0.03399$~\\
\hline
\end{tabular}}
\smallskip
\begin{list}{}{}
\item[{Note:}]
\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[--]The linear, power-law parameterization of the evolution in~$\phi_0$~and~$\phi^*$
is defined in Eqs.~(\ref{phi_evol_late})  and (\ref{phi_evol_power})
respectively.
\item[--]Each value of~$\phi^*$~is related to the corresponding
value of~$\phi_0$~by the ratio~$\phi_0/0.4\ln10\;\phi^*=0.1$~(see
Table~\ref{lf_BVR}).
\end{list}
\end{table}