Abstract
Accurate cosmology from upcoming weak lensing surveys relies on knowledge of the total matter power spectrum at percent level at scales $k < 10$ $h$/Mpc, for which modelling the impact of baryonic physics is crucial. We compare measurements of the total matter power spectrum from the Horizon cosmological hydrodynamical simulations: a dark matter-only run, one with full baryonic physics, and another lacking Active Galactic Nuclei (AGN) feedback. Baryons cause a suppression of power at $k\simeq 10$ $h/$Mpc of $
| Original language | English |
|---|---|
| Publisher | arXiv |
| Pages | 1-19 |
| Publication status | Published - 25 Jan 2018 |
Bibliographical note
19 pages, 14 figures, matches published versionKeywords
- astro-ph.CO
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