The PSCz Galaxy Power Spectrum Compared to N-Body Simulations
arXiv:astro-ph/0301559 · doi:10.1007/978-94-010-0115-1_37
Abstract
By comparing the PSCz galaxy power spectrum with haloes from nested and phased N-body simulations, we try to understand how IRAS infrared-selected galaxies populate dark-matter haloes. We pay special attention to the way we identify haloes in the simulations.
2 pages, 1 figure, to appear in "The IGM/Galaxy Connection: The Distribution of Baryons at z=0," eds. J.L. Rosenberg and M.E. Putman