Table 1
Main properties of the obtained VL samples with K-corrections and without E-corrections.
| VL sample | R min | R max | M min | M max | N | Λ |
|
|
||||||
| VL1 | 70 | 450 | –20.8 | –21.8 | 112 860 | 1.5 |
| VL2 | 50 | 200 | –18.9 | –21.1 | 73 810 | 0.6 |
| VL3 | 200 | 600 | –21.6 | –22.8 | 51 697 | 2.6 |
Notes. Rmin, Rmax (in Mpc h-1) are the chosen limits for the metric distance; Mmin,Mmax define the interval for the absolute magnitude in each sample. Finally, N is the number of galaxies in the sample and Λ is the nearest neighbor distance (in Mpc h-1).
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