\begin{table}
        \caption{\label{tabv}Kinematical properties of cluster and subclumps.}
         \begin{tabular}{l c c c c}
            \hline
            \hline
            \noalign{\smallskip}
{\rm Analysis}  &  {\rm System}  &  $N_{\rm g}$  & {$\langle v\rangle$} & $\sigma_{V}$\\
   &   &   & ${\rm km\ s^{-1}}$ & ${\rm km\ s^{-1}}$\\
         \hline
         \noalign{\smallskip}
          & {\rm A2345}  & 98 & $53\,645\pm108$ & $\rm 1069_{-62}^{+75}$ \\
{\rm 1D}\,{\rm DEDICA} & {\rm low}\,\,{\rm vel.}\,{\rm peak}\textrm{\tablefootmark{a}}  & 53 & 53202 & ${>}604$\\
{\rm 1D}\,{\rm DEDICA} & {\rm high}\,\,{\rm vel.}\,{\rm peak}\textrm{\tablefootmark{a}}   & 45 & 54142 & ${>}538$\\
${\rm {<}0.3}\,h_{70}^{-1}\,{\rm Mpc}$ & 
${\rm E{-}clump}$  & 18 & $54\,573\pm232$ & $\rm 944_{-297}^{+303}$ \\
${\rm {<}0.3}\,h_{70}^{-1}\,{\rm Mpc} $ & 
${\rm SW{-}clump}$  &  8 & $53\,995\pm540$ & $\rm 1346_{-102}^{+289}$ \\
${\rm {<}0.3}\,h_{70}^{-1}\,{\rm Mpc}$ & 
${\rm NW{-}clump}$  &  9 & $53\,487\pm407 $ & $\rm 1105_{-122}^{+182}$ \\
{\rm 3D}\,{\rm KMM} & 
${\rm E{-}clump}$  & 52 & $53\,908\pm162$ & $\rm 1155_{-70}^{+119}$ \\
${\rm 3D}\,{\rm KMM}$ & 
${\rm SW{-}clump}$  & 17 & $53\,517\pm261$ & $\rm 1032_{-106}^{+218}$ \\
{\rm 3D}\,{\rm KMM} & 
${\rm NW{-}clump}$  & 29 & $53\,312\pm166$ &  $\rm 873_{-91}^{+167}$ \\
${\rm 3D}\,{\rm KMM}\,{\rm (}r{\rm ^{\prime}<20)}$  & 
${\rm E{-}clump}$  & 45 & $54\,077\pm170 $ & $\rm 1128_{-89}^{+123}$ \\
${\rm 3D}\,{\rm KMM}\,{\rm (}r{\rm ^{\prime}<20)}$  & 
${\rm SW{-}clump}$  & 13 & $53\,079\pm244$ &  $\rm 831_{-110}^{+217}$ \\
${\rm 3D}\,{\rm KMM}\,{\rm (}r{\rm ^{\prime}<20)}$ & 
${\rm NW{-}clump}$  & 30 & $53\,296\pm159$ &  $\rm 852_{-74}^{+165}$ \\
            \hline
         \end{tabular}
\tablefoot{\tablefootmark{a}{For this galaxy clump we report the velocity
  peak instead on the mean velocity. The value of velocity dispersion
  should be considered a minor limit due to the abruptal truncation of
  the velocity distribution.}}
\end{table}