Figure 20.
Average mass density of neighbouring haloes, |$\overline{\rho }$|, as a function of the sphere's radius around the EIGs or random galaxies, r, in which the density is averaged (calculated using Mill2).
Average mass density of neighbouring haloes, |$\overline{\rho }$|, as a function of the sphere's radius around the EIGs or random galaxies, r, in which the density is averaged (calculated using Mill2).
