Carolina Cuesta-Lazaro
Galaxy clustering from the bottom up: A Streaming Model emulator I
Cuesta-Lazaro, Carolina; Nishimichi, Takahiro; Kobayashi, Yosuke; Ruan, Cheng-Zong; Eggemeier, Alexander; Miyatake, Hironao; Takada, Masahiro; Yoshida, Naoki; Zarrouk, Pauline; Baugh, Carlton M; Bose, Sownak; Li, Baojiu
Authors
Takahiro Nishimichi
Yosuke Kobayashi
Cheng-Zong Ruan
Alexander Eggemeier
Hironao Miyatake
Masahiro Takada
Naoki Yoshida
Pauline Zarrouk
Professor Carlton Baugh c.m.baugh@durham.ac.uk
Professor
Dr Sownak Bose sownak.bose@durham.ac.uk
UKRI Future Leaders Fellowship
Professor Baojiu Li baojiu.li@durham.ac.uk
Professor
Abstract
In this series of papers, we present a simulation-based model for the non-linear clustering of galaxies based on separate modelling of clustering in real space and velocity statistics. In the first paper, we present an emulator for the real-space correlation function of galaxies, whereas the emulator of the real-to-redshift space mapping based on velocity statistics is presented in the second paper. Here, we show that a neural network emulator for real-space galaxy clustering trained on data extracted from the DARK QUEST suite of N-body simulations achieves sub-per cent accuracies on scales 1 < r < 30 h−1 Mpc, and better than 3% on scales r < 1 h−1 Mpc in predicting the clustering of dark-matter haloes with number density 10−3.5 (h−1 Mpc)−3, close to that of SDSS LOWZ-like galaxies. The halo emulator can be combined with a galaxy-halo connection model to predict the galaxy correlation function through the halo model. We demonstrate that we accurately recover the cosmological and galaxy-halo connection parameters when galaxy clustering depends only on the mass of the galaxies’ host halos. Furthermore, the constraining power in σ8 increases by about a factor of 2 when including scales smaller than 5 h−1 Mpc. However, when mass is not the only property responsible for galaxy clustering, as observed in hydrodynamical or semi-analytic models of galaxy formation, our emulator gives biased constraints on σ8. This bias disappears when small scales (r < 10 h−1 Mpc) are excluded from the analysis. This shows that a vanilla halo model could introduce biases into the analysis of future datasets.
Citation
Cuesta-Lazaro, C., Nishimichi, T., Kobayashi, Y., Ruan, C., Eggemeier, A., Miyatake, H., …Li, B. (in press). Galaxy clustering from the bottom up: A Streaming Model emulator I. Monthly Notices of the Royal Astronomical Society, https://doi.org/10.1093/mnras/stad1207
Journal Article Type | Article |
---|---|
Online Publication Date | Apr 25, 2023 |
Deposit Date | May 30, 2023 |
Publicly Available Date | May 30, 2023 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
DOI | https://doi.org/10.1093/mnras/stad1207 |
Files
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Copyright Statement
This is a pre-copyedited, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The version of record is available online at: https://doi.org/10.1093/mnras/stad1207.
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