\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}