All Tables
- Table 1:
Main properties of the obtained VL samples:
,
are the chosen limits for the metric distance;
are the interval for
the absolute magnitude and
is the resulting number of galaxies
in each sample.
- Table 2:
Characteristic scales of the VL samples:
is the average separation distance
between nearest neighbor galaxies (in 2dFGRS and Poisson distribution
within the same volume and for the same number of galaxies),
is the maximum sphere completely contained in the sample. All distances are in Mpc (H0=100 km s-1 Mpc-1).