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Open AccessJournal ArticleDOI

Evidence for galaxy assembly bias in BOSS CMASS redshift-space galaxy correlation function

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TLDR
In this article, an extended halo occupation distribution model (HOD) is proposed that includes both a concentration-based assembly bias term and an environment-based bias term, and it achieves a good fit (chi 2/DoF = 1.35) on the 2D redshift-space 2-point correlation function (2PCF) of the Baryon Oscillation Spectroscopic Survey (BOSS) CMASS galaxy sample.
Abstract
Building accurate and flexible galaxy-halo connection models is crucial in modeling galaxy clustering on non-linear scales. Recent studies have found that halo concentration by itself cannot capture the full galaxy assembly bias effect and that the local environment of the halo can be an excellent indicator of galaxy assembly bias. In this paper, we propose an extended halo occupation distribution model (HOD) that includes both a concentration-based assembly bias term and an environment-based assembly bias term. We use this model to achieve a good fit (chi^2/DoF = 1.35) on the 2D redshift-space 2-point correlation function (2PCF) of the Baryon Oscillation Spectroscopic Survey (BOSS) CMASS galaxy sample. We find that the inclusion of both assembly bias terms is strongly favored by the data and the standard 5-parameter HOD is strongly rejected. More interestingly, the redshift-space 2PCF drives the assembly bias parameters in a way that preferentially assigns galaxies to lower mass halos. This results in galaxy-galaxy lensing predictions that are within 1sigma agreement with the observation, alleviating the perceived tension between galaxy clustering and lensing. We also showcase a consistent 3-5sigma preference for a positive environment-based assembly bias that persists over variations in the fit. We speculate that the environmental dependence might be driven by underlying processes such as mergers and feedback, but might also be indicative of a larger halo boundaries such as the splashback radius. Regardless, this work highlights the importance of building flexible galaxy-halo connection models and demonstrates the extra constraining power of the redshift-space 2PCF.

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Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing

- 13 Jan 2022 - 
TL;DR: The first cosmology results from large-scale structure in the Dark Energy Survey (DES) spanning 5000 deg$^2 were presented in this paper , where the authors performed an analysis combining three two-point correlation functions (3$\times$2pt): (i) cosmic shear using 100 million source galaxies, (ii) galaxy clustering, and (iii) cross-correlation of source galaxy shear with lens galaxy positions.
Journal ArticleDOI

Arbitrating the S8 discrepancy with growth rate measurements from redshift-space distortions

TL;DR: In this paper, the authors examined the role of measurements of the growth rate in arbitrating the $S_8$ discrepancy, considering measurements of $f\sigma_8(z)$ from Redshift-Space Distortions (RSD) from Baryon Acoustic Oscillations (BAO) and Type Ia Supernovae (SNeIa).

The Scale-Dependence of Halo Assembly Bias

TL;DR: In this article, the scale-dependent assembly bias of the two-point clustering of dark matter halos is studied and shown to be influenced by halo properties besides mass, a phenomenon referred to as halo assembly bias.
Journal ArticleDOI

The galaxy–halo connection of emission-line galaxies in IllustrisTNG

TL;DR: In this article, the authors employ the hydrodynamical simulation IllustrisTNG-300-1 to explore the halo occupation distribution and environmental dependence of luminous star-forming emission-line galaxies (ELGs) at $z \sim 1$.
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Consistent lensing and clustering in a low-S8 Universe with BOSS, DES Year 3, HSC Year 1 and KiDS-1000

Alexandra Amon, +107 more
TL;DR: In this article , the authors evaluate the consistency between lensing and clustering based on measurements from BOSS combined with galaxy-galaxy lensing from DES-Y3, HSC-Y1, KiDS-1000.
References
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Journal ArticleDOI

On the halo-mass and radial scale dependence of the lensing is low effect

TL;DR: In this article, the authors present new measurements and modelling of galaxies in the Baryon Oscillation Spectroscopic Survey (BOSS) low-lowz sample, focusing on the radial and stellar mass dependence of the lensing amplitude mis-match and find an amplitude mismatch of around $35\%$ when assuming the canonical $Lambda$CDM with Planck Cosmological Microwave Background (CMB) constraints.
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Cosmological Evidence Modelling: a new simulation-based approach to constrain cosmology on non-linear scales

TL;DR: Cosmological Evidence Modelling (CEM) as mentioned in this paper is a surrogate model for the MCMC analysis of galaxy-galaxy and galaxy-matter correlation functions on non-linear scales.
Journal ArticleDOI

Filaments in VIPERS: Galaxy quenching in the infalling regions of groups

TL;DR: Salerno et al. as discussed by the authors presented a model for astronomy at the Centro Cientifico Tecnologico Conicet (CCTC) in Cordoba, Argentina.
Journal ArticleDOI

Does the galaxy–halo connection vary with environment?

TL;DR: In this article, the authors show that SHAM fails to reproduce the correct dependence between environmental density and g-r color for all galaxies and central galaxies, although it better reproduces the color dependence on environmental density of satellite galaxies.
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Regardless, this work highlights the importance of building flexible galaxy-halo connection models and demonstrates the extra constraining power of the redshift-space 2PCF.