All Tables

Table 1: A summary of the photometric data of the GOODS-South field used in this work.
Table 2: Magnitude intervals that we used to divide the overall sample into subsamples with well-defined magnitude limits and corresponding areas for the z and Ks bands. See also Figs. 3 and 4. $\it MAGLIM1$ and $\it MAGLIM2$ (in magnitudes per sq. arcsec) define the limits of each magnitude bin. $\it MAGTOT$ is the corresponding limit for the total magnitude of the objects, obtained using the simulations described in Sect. 3.2.
Table 3: SExtractor parameters for detection in the z band.
Table 4: Parameters used for the PEGASE 2.0 library. Other models were added to reproduce the colours of red galaxies at high redshift, as described in the text.
Table 5: Extract of the GOODS-MUSIC web catalog: coordinates, spectroscopy and magnitude limits.
Table 6: Extract of the GOODS-MUSIC web catalog: optical photometry.
Table 7: Extract of the GOODS-MUSIC web catalog: infrared photometry.
Table A.1: Correlation matrix of noise in the ACS z band.