An analysis of the evolving comoving number density of galaxies in hydrodynamical simulations

An analysis of the evolving comoving number density of galaxies in hydrodynamical simulations

We present an analysis of the evolving comoving cumulative number density of galaxy populations found in the Illustris simulation. Cumulative number density is commonly used to link galaxy populations across different epochs by assuming that galaxies preserve their number density in time. Our analys...

Full description

Bibliographic Details
Main Authors: Wellons, Sarah, Nelson, Dylan, Rodriguez-Gomez, Vicente, McKinnon, Ryan, Pillepich, Annalisa, Ma, Chung-Pei, Springel, Volker, Hernquist, Lars, Torrey, Paul A., Leal Machado, Francisco, Griffen, Brendan F., McKinnon, Ryan Michael, Vogelsberger, Mark
Other Authors: MIT Kavli Institute for Astrophysics and Space Research
Format: Article
Language:en_US
Published: Oxford University Press 2017
Online Access:http://hdl.handle.net/1721.1/108494
https://orcid.org/0000-0002-5653-0786
https://orcid.org/0000-0001-8745-5830
https://orcid.org/0000-0001-9018-1180
https://orcid.org/0000-0001-8593-7692

Internet

http://hdl.handle.net/1721.1/108494
https://orcid.org/0000-0002-5653-0786
https://orcid.org/0000-0001-8745-5830
https://orcid.org/0000-0001-9018-1180
https://orcid.org/0000-0001-8593-7692

Similar Items