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: | , , , , , , , , , , |
|---|---|
| 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 |
| 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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