All Tables

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.
Table 2: The values of M^* computed from the fits of the Schechter function to the CLFs of EIS 0048. M^* is obtained by fixing $\alpha = -0.9$ .