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The MillenniumTNG Project: inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching

Contreras, Sergio; Angulo, Raul E; Springel, Volker; White, Simon D M; Hadzhiyska, Boryana; Hernquist, Lars; Pakmor, Rüdiger; Kannan, Rahul; Hernández-Aguayo, César; Barrera, Monica; Ferlito, Fulvio; Delgado, Ana Maria; Bose, Sownak; Frenk, Carlos

The MillenniumTNG Project: inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching Thumbnail


Authors

Sergio Contreras

Raul E Angulo

Volker Springel

Simon D M White

Boryana Hadzhiyska

Lars Hernquist

Rüdiger Pakmor

Rahul Kannan

César Hernández-Aguayo

Monica Barrera

Fulvio Ferlito

Ana Maria Delgado

Sownak Bose



Abstract

We introduce a novel technique for constraining cosmological parameters and galaxy assembly bias using non-linear redshift-space clustering of galaxies. We scale cosmological N-body simulations and insert galaxies with the SubHalo Abundance Matching extended (SHAMe) empirical model to generate over 175 000 clustering measurements spanning all relevant cosmological and SHAMe parameter values. We then build an emulator capable of reproducing the projected galaxy correlation function at the monopole, quadrupole, and hexadecapole level for separations between
and
⁠. We test this approach by using the emulator and Monte Carlo Markov Chain (MCMC) inference to jointly estimate cosmology and assembly bias parameters both for the MTNG740 hydrodynamic simulation and for a semi-analytical model (SAM) galaxy formation built on the MTNG740-DM dark matter-only simulation, obtaining unbiased results for all cosmological parameters. For instance, for MTNG740 and a galaxy number density of
⁠, we obtain
and
(which are within 0.4 and 0.2σ of the MTNG cosmology). For fixed Hubble parameter (h), the constraint becomes
⁠. Our method performs similarly well for the SAM and for other tested sample densities. We almost always recover the true amount of galaxy assembly bias within 1σ. The best constraints are obtained when scales smaller than
are included, as well as when at least the projected correlation function and the monopole are incorporated. These methods offer a powerful way to constrain cosmological parameters using galaxy surveys.

Citation

Contreras, S., Angulo, R. E., Springel, V., White, S. D. M., Hadzhiyska, B., Hernquist, L., …Frenk, C. (2023). The MillenniumTNG Project: inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching. Monthly Notices of the Royal Astronomical Society, 524(2), 2489-2506. https://doi.org/10.1093/mnras/stac3699

Journal Article Type Article
Acceptance Date Dec 13, 2022
Online Publication Date Jul 20, 2023
Publication Date 2023-09
Deposit Date Jan 24, 2024
Publicly Available Date Jan 24, 2024
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Royal Astronomical Society
Peer Reviewed Peer Reviewed
Volume 524
Issue 2
Pages 2489-2506
DOI https://doi.org/10.1093/mnras/stac3699
Keywords Space and Planetary Science; Astronomy and Astrophysics
Public URL https://durham-repository.worktribe.com/output/2163199

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Copyright Statement
© 2023 The Author(s)
Published by Oxford University Press on behalf of Royal Astronomical Society




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