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.
ID z IABa MBb MKb $\delta I$ $r_{\rm half}^c$ id
HDFS4170 0.4602 20.79 -20.43 -22.60 0.56 3.57 51
HDFS5190 0.6952 21.31 -21.25 -21.92 0.60 4.07 59
CFRS03.0619 0.4854 20.80 -20.67 -21.93 0.63 3.87 27
CFRS03.1032 0.6180 20.49 -21.18 -22.64 0.51 1.79 37
CFRS22.0619 0.4676 21.55 -19.33 -19.33 0.70 4.31 68
CFRS03.1349 0.6155 20.87 -21.19 -22.92 0.56 3.84 48
CFRS22.1064 0.5383 22.08 -19.87 -21.64 0.24 2.36 49
HDFS5150 0.6956 22.36 -20.20 -21.03 0.72 3.39 42
CFRS03.0508 0.4642 21.92 -19.61 -20.35 0.46 3.32 38
CFRS03.0645 0.5275 21.36 -20.30 -21.34 0.71 4.57 45
CFRS22.0919 0.4738 21.77 -19.99 -19.53 0.41 2.52 61
CFRS22.0975 0.4211 20.21 -20.40 -22.53 0.59 3.82 50
CFRS03.0523 0.6508 21.31 -20.67 -21.55 0.48 3.57 41
HDFS4130 0.4054 20.09 -20.90 -22.13 0.62 4.04 36
HDFS4090 0.5162 22.15 -19.71 -19.83 0.35 1.54 45
HDFS5140 0.5649 22.38 -19.76 -20.46 0.36 2.57 50
HDFS5030 0.5821 20.40 -21.74 -22.68 0.66 4.19 25
a Isophotal magnitudes; b from Hammer et al. (2005);
c in kpc; d inclination, in deg.

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