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Galaxies as Biased Tracers of the Cosmic Web
The cosmic web consists of a network of clusters, filaments and sheets, which cover the Universe on large scales. Its observation with galaxy surveys provides a powerful way to constrain cosmological models. However, this
are dominated by dark matter. This problem can be tackled with galaxy bias models, which describe the mapping
between the distribution of galaxies and dark matter. I will present recent efforts in testing and advancing these bias models using cosmological simulations.