\begin{table}%t1
\caption{\label{lf_BVR}Parameters of the Gaussian and Schechter components of the
  composite luminosity functions fitted to the ESO-Sculptor
  spectral-type luminosity functions, in the~$R_{\rm c}$,~$V$, and~$B$~filters.}
%\centerline
{
\begin{tabular}{lcccccccc}
\hline
\hline
Sample           & Numb{.}  & Morphol. & \multicolumn{3}{c}{Gaussian component} & \multicolumn{2}{c}{Schechter component}   &~$\phi_0$~\\
                 & of gal{.} & content  &~$M_0-5\log h$~  &~$\Sigma_a$~&~$\Sigma_b$~&~$M^*-5\log h$~  &~$\alpha$~&~$\overline{0.4 \ln10\; \phi^*}$~\\
\hline
\multicolumn{9}{c}{\bf early-type galaxies}  \\
\hline
$R_{\rm c}\le21.5$~& 291 & E+S0+Sa    &~$-20.87\pm0.23$~&~$0.84\pm0.24$~&~$1.37\pm0.36$~\\
$V\le21.0$~           & 156 & E+S0+Sa    &~$-20.37$~       &~$0.84$~       &~$1.37$~       \\
$B\le22.0$~           & 108 & E+S0+Sa    &~$-19.47$~       &~$0.84$~       &~$1.37$~       \\
\hline
\multicolumn{9}{c}{\bf intermediate-type galaxies} \\
\hline
$R_{\rm c}\le21.5$~& 270 & Sb+Sc/dSph &~$-20.27\pm0.21$~&~$0.91\pm0.18$~& &~$-19.28\pm0.37$~&~$-1.53\pm0.33$~&~$0.83$~\\
$V\le21.0$~           & 169 & Sb+Sc/dSph &~$-19.87$~       &~$0.91$~       & &~$-18.88$~       &~$-1.53$~       &~$0.83$~\\
$B\le22.0$~           & 154 & Sb+Sc/dSph &~$-19.27$~       &~$0.91$~       & &~$-18.28$~       &~$-1.53$~       &~$0.83$~\\
\hline
\multicolumn{9}{c}{\bf late-type galaxies} \\
\hline
$R_{\rm c}\le21.5$~& 309 & Sc+Sd/dI   &~$-19.16\pm0.29$~&~$0.97\pm0.13$~& &~$-18.12\pm0.22$~&~$-0.30$~       &~$0.1$~\\
$V\le21.0$~           & 168 & Sc+Sd/dI   &~$-18.76$~       &~$0.97$~       & &~$-17.72$~       &~$-0.30$~       &~$0.1$~\\
$B\le22.0$~           & 190 & Sc+Sd/dI   &~$-18.36$~       &~$0.97$~       & &~$-17.32$~       &~$-0.30$~       &~$0.1$~\\
\hline
\end{tabular}}
\smallskip
\begin{list}{}{}
\item[{Notes:}]
\item[--] For the 2-component luminosity functions fitted to the
intermediate-type and late-type galaxies, the morphological content of
the 2 components appear separated by a "/''.
\item[--] The listed luminosity function parameters correspond to~$H_0 =
100 h$~km s$^{-1}$~Mpc$^{-1}$,~$\Omega_{\rm m}=0.3$, and~$\Omega_\Lambda=0.7$.
\end{list}
\end{table}