Large-scale bias and stochasticity of haloes and dark matter
Large-scale bias and stochasticity of haloes and dark matter
On large scales, galaxies and their haloes are usually assumed to trace the dark matter with a constant bias and dark matter is assumed to trace the linear density field. We test these assumption using several large N‐body simulations with 3843–10243 particles and box sizes of 96–1152 h−1 Mpc, which …