\begin{table}%T2
%\centering
\small
\caption{Dynamical properties of the sample of LCGs. The column
entries are ({\it from left to right}): id, dynamical class (RD~= Rotating
Disk, PR~= Perturbed Rotation, CK~= Complex Kinematics), maximal
rotational velocity (corrected from inclination, but not from GIRAFFE
spatial sampling), intensity-weighted velocity dispersion calculated
from the $\sigma$-map, velocity dispersion derived from integrated
spectra, and stellar masses derived from photometry (in solar masses).
The objects for which the kinematical classification is uncertain are
indicated by a star; see individual comments.}
\label{tab2}
\begin{tabular}{llrrrr}\hline\hline
ID    & class & $V_{\rm rot}$ &  $\sigma$  & $\sigma _{\rm intg}$ & $M_*$\\\hline
HDFS4170      & RD   & 173 & 75  & 111 & 10.83 \\
HDFS5190      & RD   & 168 & 64  & 126 & 10.51  \\
CFRS03.0619   & RD   & 155 & 57  & 88  & 10.50 \\\hline
CFRS03.1032   & PR*  & 139 & 162 & 168 & 10.87 \\
CFRS22.0619   & PR   & 67  & 36  & 64  & 9.50  \\
CFRS03.1349   & PR*  & 235 & 70  & 183 & 10.91 \\
CFRS22.1064   & PR   & 124 & 107 & 124 & 10.39 \\
HDFS5150      & PR   & 77  & 69  & 78  & 10.14 \\\hline
CFRS03.0508   & CK   & 78  & 37  & 54  & 9.87  \\
CFRS03.0645   & CK   & 125 & 58  & 67  & 10.27 \\
CFRS22.0919   & CK   & 45  & 46  & 51  & 9.54  \\
CFRS22.0975   & CK   & 409 & 82  & 182 & 10.82 \\
CFRS03.0523   & CK   & 97  & 156 & 148 & 10.35 \\
HDFS4130      & CK   & 153 & 76  & 97  & 10.63 \\
HDFS4090      & CK   & 20  & 51  & 49  & 9.67  \\
HDFS5140      & CK   & 224 & 69  & 133 & 9.91  \\
HDFS5030      & CK   & 74  & 59  & 65  & 10.81 \\\hline
\end{tabular}
\end{table}