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 -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.

ID	class				M*
HDFS4170	RD	173	75	111	10.83
HDFS5190	RD	168	64	126	10.51
CFRS03.0619	RD	155	57	88	10.50
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
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

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