All Tables

• Table 1: Summary of the best fit clustering parameters. Poissonian uncertainties (only) are quoted here to allow comparison between different galaxy samples within the same GOODS field (see text). When comparing the results between the two fields, or when comparing the average properties of GOODS sources with those of other fields, cosmic variance uncertainties must also be included (see Table 2).
• Table 2: Combined GOODS-S plus GOODS-N sample. The uncertainties take into account cosmic variance and have been computed as described in Sect. 4.