The PSCz Galaxy Power Spectrum Compared to N-Body Simulations
Astrophysics
2016-01-27 v1
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.
Cite
@article{arxiv.astro-ph/0301559,
title = {The PSCz Galaxy Power Spectrum Compared to N-Body Simulations},
author = {Mark C. Neyrinck and Andrew J. S. Hamilton and Nickolay Y. Gnedin},
journal= {arXiv preprint arXiv:astro-ph/0301559},
year = {2016}
}
Comments
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