All Tables

Table 1: Main characterictics of the detectors.
Table 2: Filter characterictics.
Table 3: First epoch observations.
Table 4: Second epoch observations.
Table 5: Fit of the magnitude uncertainty as a function of magnitude deduced from the common areas. This was used to compute uncertainties for individual galaxies: Uncertainty = slope $\times$ magnitude + constant term.
Table 6: 90% and 50% completeness levels for point-like and faint low surface brightness galaxies.
Table 7: Literature red sequences in the B-R/R sequence.