\begin{table}%t6
\caption{\label{Summary}Object summary.}
\small%\centerline
 {
\begin{tabular}{c c c c c c c}  
\hline\hline  
  & & & Types & & & \\  
  & All & Classic & Cold & Hot & SDOs & Cent\\
\hline   
This work & 30 & 19 & 9  & 10 & 10$^{(\star)}$ &  1\\  
LP		  & 53 & 33	& 16 & 17 &	10 & 10$^{(\bullet)}$\\
2MS		  & 33 & 21	& 6	 & 15 &	5  &  7\\	
\hline
Total	&  116 & 73	& 31 & 42 & 25 & 18\\	 
\hline 
\end{tabular}}
\medskip
Number of objects for the different dynamical groups (except the 2~Neptune{'}s resonant objects):
All (the whole sample), {Classic} (classical TNOs),  {Cold} (classical TNOs with inclinations $<$$4.5^{\circ}$),  {hot} (classical TNOs with inclinations $>$$4.5^{\circ}$),  {SDOs} (scattered disk objects), and  {Cent} (Centaurs).  {LP} is the ESO Large Program
(Boehnhardt et~al. \cite{Boe02}; Peixinho et~al. \cite{Peix}), and  {2MS} the Meudon Multicolor Survey (Doressoundiram et~al. \cite{Doress_b}). $^{(\star)}$~We include the peculiar distant object~2000CR$_{105}$. $^{(\bullet)}$~We include the uncertain Centaur~2002CB$_{249}$.
\end{table}