How do galaxies populate halos in extreme density environments? An
  analysis of the Halo Occupation Distribution in SDSS
  Recent works have shown that the properties of galaxy populations in dark
matter halos vary with large-scale environments. These results suggest a
variation in the halo occupation distribution (HOD) in extreme density
environments. To analyse these effects, we identify cosmic voids and future
virialised structures (FVS) in the SDSS-DR12 and estimate the HOD within these
superstructures using group catalogues as dark matter halo proxies.
  Our goal is to use observational galaxy data to characterise the HOD within
voids and FVS, explore the different properties of these galaxies populations
and compare them with the general results outside these superstructures.
  Using a galaxy group catalogue we compute the HOD within both types of
superstructures. We also study the dependence on the results on the main void
and FVS properties. We also analysed the mean stellar age of the galaxies
inside these regions. In all cases, we compare the results with those derived
from the Field sample.
  Inside voids, we find a strong decrease in HOD concerning the Field results.
The mean number of satellites fall to 50%. Inside FVS, the HOD shows a
significant increase to the Field, with a 40% excess in the mean number of
satellites. In both regions, the differences with respect to the Field
increases for the extreme values of the density environments. We obtain no
signs of variations related to intrinsic characteristics of voids and FVS. We
find that the cumulative distribution of the mean age of stars of the central
galaxy also varies in these regions. Finally, we explore the HOD for the 25%
youngest (oldest) galaxies. We find that for the low-mass groups the youngest
galaxies are only present inside voids. On the other hand, for the high-mass
groups the FVS environments show the same increase in the HOD concerning the
Field. We find that cosmic voids lack of oldest galaxies.
