First results from the IllustrisTNG simulations: matter and galaxy clustering

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 baryons, dark matter, gala...

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Main Authors: Springel, Volker (Author) , Pakmor, Rüdiger (Author) , Pillepich, Annalisa (Author) , Weinberger, Rainer (Author) , Nelson, Dylan (Author) , Hernquist, Lars (Author) , Vogelsberger, Mark (Author) , Genel, Shy (Author) , Torrey, Paul (Author) , Marinacci, Federico (Author) , Naiman, Jill P. (Author)
Format: Article (Journal) Chapter/Article
Language:English
Published: 21 Dec 2017
Edition:Version V2
In: Arxiv
Year: 2017, Pages: 1-24
DOI:10.48550/arXiv.1707.03397
Online Access:Resolving-System, kostenfrei, Volltext: https://doi.org/10.48550/arXiv.1707.03397
Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1707.03397
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Author Notes:Volker Springel, Rüdiger Pakmor, Annalisa Pillepich, Rainer Weinberger, Dylan Nelson, Lars Hernquist, Mark Vogelsberger, Shy Genel, Paul Torrey, Federico Marinacci, Jill Naiman
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First results from the IllustrisTNG simulations: matter and galaxy clustering by Springel, Volker (Author) , Pakmor, Rüdiger (Author) , Pillepich, Annalisa (Author) , Weinberger, Rainer (Author) ,


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