The PSCz Galaxy Power Spectrum Compared to N-Body Simulations
Mark C. Neyrinck, Andrew J. S. Hamilton, Nickolay Y. Gnedin
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.
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