Astronomy & Astrophysics

Table 1: Details of the images used. We list the total integration time in each of the four pointings and the completeness limit of each filter, based on simulations described fully in Sect. 4.1.
Table 2: Differential galaxy number counts. Counts are shown in half-magnitude bins selected in $(BVRI)_{\rm AB}$ . Also shown are the logarithmic counts, normalised to the effective area of the survey field (1.18 deg²).
Table 3: Best-fitting galaxy count slopes in BVRI bands for our catalogue, computed in the specified magnitude ranges.