\begin{table}%t2
\caption{\label{t_morph}Bar fractions per Hubble type for bright and faint subsamples.}
\small%\centerline
 {
\begin{tabular}{c c c}
\hline \hline
Hubble & \multicolumn{2}{c}{Bar fraction (Number of objects)} \\
type & $<$$-21.0$ mag & $\ge$$-21.0$ mag \\
\hline
 S0 & $14\%$ (44) & $6\%$ (89) \\
 Sa & $21\%$ (121) & $11\%$ (180) \\
 Sb & $40\%$ (117) & $31\%$ (151) \\
 Sc & $32\%$ (59) & $38\%$ (135) \\
\hline
\end{tabular}}
\medskip
Notes: the table shows results for 896 objects in the range $0.4<z<0.8$. (The 52~Sd/Sm/Im~galaxies are not considered in this table.) The samples are split at $M_V=-21.0$~mag, which is the mean
$V$-band magnitude of the total sample.
\end{table}