Modelling baryonic feedback for survey cosmology

Modelling baryonic feedback for survey cosmology

Observational cosmology in the next decade will rely on probes of the distribution of matter in the redshift range between 0<z<3 to elucidate the nature of dark matter and dark energy. In this redshift range, galaxy formation is known to have a significant impact on observables such as two-poi...

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Bibliographic Details
Main Authors: Elisa Chisari, Alexander J. Mead, Shahab Joudaki, Pedro G. Ferreira, Aurel Schneider, Joseph Mohr, Tilman, David Alonso, Ian G. McCarthy, Sergio Martin-Alvarez, Julien Devriendt, Adrianne Slyz, Marcel P. van Daalen
Format: Article
Language:English
Published: Maynooth Academic Publishing 2019-06-01
Series:The Open Journal of Astrophysics
Subjects:
large-scale structure of the universe
cosmology
baryonic physics
redshift surveys
galaxy clustering
Online Access:https://astro.theoj.org/article/9452-modelling-baryonic-feedback-for-survey-cosmology

Internet

https://astro.theoj.org/article/9452-modelling-baryonic-feedback-for-survey-cosmology

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