All Tables

Table 1: Main properties of the angular regions considered: The limits in degrees of the cuts are chosen using the intrinsic coordinates of the survey $\eta$ and $\lambda$ (in degrees). The last column $\Omega$ gives the solid angle of three angular regions in steradians.
Table 2: Main properties of the obtained VL samples: $r_{\rm min}$ , $r_{\rm max}$ (in Mpc/h) are the chosen limits for the metric distance; ${M_{\rm min}, ~M_{\rm max}}$ define the interval for the absolute magnitude in each sample. The quantity $\langle \Lambda \rangle$ (in Mpc/h) is the average distance between nearest-neighbor galaxies.
Table 3: Number of galaxies in each of the VL samples. Names are given according to the discussion in the text. The scale $R_{\rm c}$ (in Mpc/h) is discussed in Sect. 3.2 below.
Table 4: Main properties of the different subsamples considered in the R1 region. The angular limits of the cuts in the intrinsic coordinates of the survey $\eta$ and $\lambda$ (in degrees). The last column gives the number of points in the sample.