In the Guo et al. semi-analytic model on the Millennium Simulation, most cosmic-web effects on galaxy properties reduce to a halo mass bias plus a satellite and backsplash excess.
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The relation of galaxies and dark matter haloes to the filamentary cosmic web
In the Guo et al. semi-analytic model on the Millennium Simulation, most cosmic-web effects on galaxy properties reduce to a halo mass bias plus a satellite and backsplash excess.