First results from the IllustrisTNG simulations: matter and galaxy clustering

First results from the IllustrisTNG simulations: matter and galaxy clustering

© 2017 The Author(s). Hydrodynamical simulations of galaxy formation have now reached sufficient volume to make precision predictions for clustering on cosmologically relevant scales. Here, we use our new IllustrisTNG simulations to study the non-linear correlation functions and power spectra of bar...

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Bibliographic Details
Main Authors: Springel, Volker, Pakmor, Rüdiger, Pillepich, Annalisa, Weinberger, Rainer, Nelson, Dylan, Hernquist, Lars, Vogelsberger, Mark, Genel, Shy, Torrey, Paul, Marinacci, Federico, Naiman, Jill
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:English
Published: Oxford University Press (OUP) 2021
Online Access:https://hdl.handle.net/1721.1/134594

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https://hdl.handle.net/1721.1/134594

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