Corpus ID: 211003887

Characterizing hydrostatic mass bias with Mock-X

@article{Barnes2020CharacterizingHM,
  title={Characterizing hydrostatic mass bias with Mock-X},
  author={D. J. Barnes and M. Vogelsberger and Francesca A. Pearce and A. Pop and R. Kannan and Kaili Cao and S. Kay and Lars Hernquist Mit and Harvard-CfA and T. Manchester},
  journal={arXiv: Cosmology and Nongalactic Astrophysics},
  year={2020}
}
  • D. J. Barnes, M. Vogelsberger, +7 authors T. Manchester
  • Published 2020
  • Physics
  • arXiv: Cosmology and Nongalactic Astrophysics
  • Surveys in the next decade will deliver large samples of galaxy clusters that transform our understanding of their formation. Cluster astrophysics and cosmology studies will become systematics limited with samples of this magnitude. With known properties, hydrodynamical simulations of clusters provide a vital resource for investigating potential systematics. However, this is only realized if we compare simulations to observations in the correct way. Here we introduce the \textsc{Mock-X… CONTINUE READING

    Figures and Tables from this paper.

    Scatter in Sunyaev--Zel'dovich effect scaling relations explained by inter-cluster variance in mass accretion histories.

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