pith. sign in

arxiv: astro-ph/0301559 · v1 · pith:A7VQ5F7Xnew · submitted 2003-01-28 · 🌌 astro-ph

The PSCz Galaxy Power Spectrum Compared to N-Body Simulations

classification 🌌 astro-ph
keywords haloessimulationsgalaxyn-bodypowerpsczspectrumattention
0
0 comments X
read the original 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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.