Description
The list of the measured galaxies is given in Table 3 together with COSMOS coordinates and apparent magnitude. These parameters (plus diameter, axis ratio and position angle) were used to perform cross-identification with the PGC/LEDA objects after reduction to the RC3 system (de Vaucouleurs et al., 1990, see cat. <VII/155>). Both cross correlation results (from `rvsao') and emission line results (from `emsao') are presented. A few galaxies with published redshifts were also observed to derive our external error (see section 3 of the paper).
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