Table 1: The completeness magnitudes. ${m^{\rm c}}$ is the completeness magnitude as estimated on the photometric catalogues according to Garilli et al. (1999). ${m^{\rm c}_{\rm zp}}$ defines the central position of the faintest magnitude bin with completeness higher than $50\%$ in the sample with photometric redshifts (see Sect. 2.2). The bin width is 0.5 mag.
Band ${m^{\rm c}}$ ${m^{\rm c}_{\rm zp}}$

mag mag

V 25.7 24.25

R 25.0 23.25

I 23.2 22.75

K 21.2 19.75

**Table 1:** The completeness magnitudes. ${m^{\rm c}}$ is the completeness magnitude as estimated on the photometric catalogues according to Garilli et al. (1999). ${m^{\rm c}_{\rm zp}}$ defines the central position of the faintest magnitude bin with completeness higher than $50\%$ in the sample with photometric redshifts (see Sect. 2.2). The bin width is 0.5 mag.
Band	${m^{\rm c}}$	${m^{\rm c}_{\rm zp}}$
	mag	mag
V	25.7	24.25
R	25.0	23.25
I	23.2	22.75
K	21.2	19.75

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