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First results from the IllustrisTNG simulations: matter and galaxy clustering

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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, gal...

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Main Authors: Springel, Volker (Author) , Pakmor, Rüdiger (Author) , Pillepich, Annalisa (Author) , Weinberger, Rainer (Author)
Format: Article (Journal)
Language:English
Published: 2018
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Volume: 475, Issue: 1, Pages: 676-698
ISSN:1365-2966
DOI:10.1093/mnras/stx3304
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stx3304
Verlag, kostenfrei, Volltext: https://academic.oup.com/mnras/article/475/1/676/4772886
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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 and 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) , Nelson, Dylan (Author) , Hernquist, Lars (Author) , Vogelsberger, Mark (Author) , Genel, Shy (Author) , Torrey, Paul (Author) , Marinacci, Federico (Author) , Naiman, Jill P. (Author) ,


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