\begin{table}%t1
\caption{\label{tab1}Morpho-kinematical classification of 52  $z_{\rm median}$~= 0.65~galaxies.}
\small%\centerline
 {
\begin{tabular}{lcccc} 
\hline\hline
\noalign{\smallskip}
Redshift   & $z_{\rm median}$ = 0.65 & $z_{\rm median}$ = 0.65 & $z_{\rm median}$ = 0.65   & $z=0$ \\ 
   & Starburst (60\%) & Quiescent (40\%) & All   & local \\ 
       & $W_0({\rm OII})\ge$ 15~\AA\ & $W_0({\rm OII})<$ 15~\AA\ & All & All \\
references       & N08  & Z06  & N08 & N04 \\
       & &  & & H05 \\ 
type       &  &    &   & \\ 
\hline
 E/S0        &   0\% &  57\% & 23\% & 27\%\\
Rotating spiral disks   &  23\% & 43\%  &  31\% & 70\%\\
Non-relaxed \&  &  77\% & 0\% &  46\% & $\sim$3\%\\
intermediate systems  &  &    &   & \\ 
\hline
Galaxies with &  &    &   & \\ 
anomalous &  68\% & 0\%   & 41\%  & \\ 
kinematics &  &    &   & \\ 
\hline
\end{tabular}}
\medskip
From \citet{Neichel08} (see their Table~4); for comparison, the last column shows the fractions derived from the SDSS \citep{Nakamura2004} for galaxies in the same mass range (e.g. \citealt{Hammer05}). CFRS \citep{Hammer97} found that 60\% of $z_{\rm median}$~= 0.65~galaxies have spectra with $W_0({\rm OII})$~$\ge$ 15~\AA\ and are classified as starbursts. References are \citet{Neichel08}: N08, \citet{2004A&A...421..847Z}: Z06, \citet{Nakamura2004}: N04 and \citet{Hammer05}: H05.
\end{table}