Table 1: Main properties of the obtained VL samples: $r_{{\rm min}}$ , $r_{{\rm max}}$ are the chosen limits for the metric distance; ${M_{{\rm min}}, M_{{\rm max}}}$ are the interval for the absolute magnitude and $N_{\rm g}$ is the resulting number of galaxies in each sample.
VL sample $r_{{\rm min}}$ $r_{{\rm max}}$ $M_{{\rm min}}$ $M_{{\rm max}}$ $N_{\rm g}$

SGP250 50 250 -19.5 -17.8 14 177

SGP400 100 400 -20.8 -19.0 29 373

SGP550 150 550 -21.2 -19.8 26 289

NGP250 50 250 -19.5 -17.8 12 474

NGP400 100 400 -20.8 -19.0 23 208

NGP550 150 550 -21.2 -19.8 18 030

**Table 1:** Main properties of the obtained VL samples: $r_{{\rm min}}$ , $r_{{\rm max}}$ are the chosen limits for the metric distance; ${M_{{\rm min}}, M_{{\rm max}}}$ are the interval for the absolute magnitude and $N_{\rm g}$ is the resulting number of galaxies in each sample.
VL sample	$r_{{\rm min}}$	$r_{{\rm max}}$	$M_{{\rm min}}$	$M_{{\rm max}}$	$N_{\rm g}$
SGP250	50	250	-19.5	-17.8	14 177
SGP400	100	400	-20.8	-19.0	29 373
SGP550	150	550	-21.2	-19.8	26 289
NGP250	50	250	-19.5	-17.8	12 474
NGP400	100	400	-20.8	-19.0	23 208
NGP550	150	550	-21.2	-19.8	18 030

Source LaTeX | All tables | In the text