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Table 1:

Main properties of the obtained VL samples. $R_{\min}$, $R_{\max}$ are the chosen limits for the metric distance; ${M_{\min}, ~M_{\max}}$ are the corresponding limits in the absolute magnitude; $N_{\rm g}$ is the number of galaxies in the sample.
VL sample $R_{\min}$ $R_{\max}$ $M_{\min}$ $M_{\max}$ $N_{\rm g}$
SGC400 100 400 -20.8 -19.0 29373
NGC400 100 400 -20.8 -19.0 23208
SGC550 150 550 -21.2 -19.8 26289
NGC550 150 550 -21.2 -19.8 18030

Source LaTeX | All tables | In the text

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