no code implementations • 4 Nov 2013 • Francisco Villaescusa-Navarro, Federico Marulli, Matteo Viel, Enzo Branchini, Emanuele Castorina, Emiliano Sefusatti, Shun Saito
We compute the bias between the spatial distribution of dark matter haloes and the overall matter and cold dark matter distributions using statistical tools such as the power spectrum and the two-point correlation function.
Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology
