Statistical characteristics of simulated walls
The matter distribution is investigated in both real and redshift spaces. In both cases almost the same particles form the walls, and we estimate differences in corresponding wall characteristics. The same methods are applied to several mock catalogues of ‘galaxies’, which allows us to characterize a large-scale bias between the spatial distribution of dark matter and of simulated ‘galaxies’.
Document Type: Research Article
Affiliations: 1: Astrophysikalisches Institute Potsdam, An der Sternwarte 16, D-14482 Potsdam, Germany 2: Keldysh Institute of Applied Mathematics, Russian Academy of Sciences, 125047 Moscow, Russia
Publication date: November 1, 2000