Fig. 5.

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Dependence of the HOD with the identification parameters of voids and FVSs for galaxies with Mr − 5log10(h) < − 19.76. In panel (a), we show the HOD measured in voids identified with a different integrated density contrast threshold, from Δlim = −0.9 in dark blue to Δlim = −0.6 in light blue. In panel (b), we show the HOD measured in FVSs with a different global luminosity threshold, from δLglob > 3.5 in light red to δLglob > 6.5 in dark red. In both cases, the HOD measured in the field is shown with green lines. For a better quantification of the differences, inferior panels show the ratio between the HOD measured in super-structures and the HOD of the field. All the uncertainties were calculated using the standard jackknife procedure.
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