Boryana Hadzhiyska
Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
Hadzhiyska, Boryana; Liu, Sonya; Somerville, Rachel S; Gabrielpillai, Austen; Bose, Sownak; Eisenstein, Daniel; Hernquist, Lars
Authors
Sonya Liu
Rachel S Somerville
Austen Gabrielpillai
Dr Sownak Bose sownak.bose@durham.ac.uk
UKRI Future Leaders Fellowship
Daniel Eisenstein
Lars Hernquist
Abstract
In this work, we compare large scale structure observables for stellar mass selected samples at z = 0, as predicted by two galaxy models, the hydrodynamical simulation IllustrisTNG and the Santa-Cruz semi-analytic model (SC-SAM). Although both models have been independently calibrated to match observations, rather than each other, we find good agreement between the two models for two-point clustering and galaxy assembly bias signatures. The models also show a qualitatively similar response of occupancy and clustering to secondary halo parameters other than mass, such as formation history and concentration, although with some quantitative differences. Thus, our results demonstrate that the galaxy–halo relationships in SC-SAM and TNG are quite similar to first order. However, we also find areas in which the models differ. For example, we note a strong correlation between halo gas content and environment in TNG, which is lacking in the SC-SAM, as well as differences in the occupancy predictions for low-mass haloes. Moreover, we show that higher order statistics, such as cumulants of the density field, help us to accurately describe the galaxy distribution and discriminate between models that show degenerate behaviour for two-point statistics. Our results suggest that SAMs are a promising cost-effective and intuitive method for generating mock catalogues for next generation cosmological surveys.
Citation
Hadzhiyska, B., Liu, S., Somerville, R. S., Gabrielpillai, A., Bose, S., Eisenstein, D., & Hernquist, L. (2021). Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model. Monthly Notices of the Royal Astronomical Society, 508(1), 698-718. https://doi.org/10.1093/mnras/stab2564
Journal Article Type | Article |
---|---|
Acceptance Date | Sep 2, 2021 |
Online Publication Date | Sep 11, 2021 |
Publication Date | 2021-11 |
Deposit Date | Dec 7, 2021 |
Publicly Available Date | Dec 7, 2021 |
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 | 508 |
Issue | 1 |
Pages | 698-718 |
DOI | https://doi.org/10.1093/mnras/stab2564 |
Public URL | https://durham-repository.worktribe.com/output/1219091 |
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Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2021, The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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