All Tables

Table 1: Main properties of the sample of LCGs: galaxies names, redshifts, isophotal I magnitudes, absolute B and K magnitudes, light concentration, half light radii, inclination.
Table 2: Dynamical properties of the sample of LCGs. The column entries are ( 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.
Table A.1: Dynamical properties of the sample of LCGs. The column entries are ( from left to right): id, dynamical class (RD = Rotating Disk, PR = Perturbed Rotation, CK = Complex Kinematics), intensity-weighted velocity dispersion corrected from GIRAFFE sampling effect (see text), ${\cal M}^E$ supported by rotation (corrected from GIRAFFE sampling effect), ${\cal M}^E$ supported by random motions, total dynamical ${\cal M}^E$ , and dynamical ${\cal M}^E$ estimated by integrated velocity dispersion.