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10 5
W1
W2
W3
10 5
W1
W2
W3
N gal 0.5 mag −1 deg −2
10 4
10 3
10 2
10 1
W4
N gal 0.5 mag −1 deg −2
10 4
10 3
10 2
10 1
W4
10 0
14 16 18 20
u
22 24 26 28
10 0
14 16 18 20
g
22 24 26 28
10 5
W1
W2
W3
10 5
W1
W2
W3
N gal 0.5 mag −1 deg −2
10 4
10 3
10 2
10 1
W4
McCracken et al. 2003
N gal 0.5 mag −1 deg −2
10 4
10 3
10 2
10 1
W4
McCracken et al. 2003
10 0
14 16 18 20
r
22 24 26 28
10 0
14 16 18 20 22 24 26 28
i
10 5
W1
W2
W3
10 5
W1
W2
W3
N gal 0.5 mag −1 deg −2
10 4
10 3
10 2
10 1
W4
N gal 0.5 mag −1 deg −2
10 4
10 3
10 2
10 1
W4
10 0
14 16 18 20
z
22 24 26 28
10 0
14 16 18 20
z
22 24 26 28
Figure 33: Galaxy counts for the four Wide patches in all bands. The dotted red line corresponds to the 80%
completeness for extended sources computed from the simulations. In r and i band counts are compared those in
the VLT-VIRMOS deep field (McCracken et al., 2003).
46