On the kinetic Sunyaev-Zel'dovich effect as an observational probe for halo spin bias

Abstract

We explore the potential of the kinetic Sunyaev-Zel'dovich (kSZ) effect as the cornerstone of a future observational probe for halo spin bias, the secondary dependence of halo clustering on halo spin at fixed halo mass. Using the IllustrisTNG magneto-hydrodynamical cosmological simulation, we measure both the kSZ and the thermal SZ (tSZ) effects produced by the baryonic content of more than 50,000 haloes within the halo mass range $11<{\log }_{10}({\mathrm{M}}_{\mathrm{vir}}/h^{-1}{\mathrm{M}}_{\odot })\lesssim 14.5$. First, we confirm that the magnitude of both effects depends strongly on the total gas and virial mass of the haloes, and that the integrated kSZ signal displays a significant correlation with the angular momentum of the intra-halo gas, particularly for massive haloes. Second, we show that both the integrated kSZ signal and the ratio of the integrated kSZ and tSZ signals trace total halo spin, even though significant scatter exists. Finally, we demonstrate that, in the absence of observational and instrumental uncertainties, these SZ-related statistics can be used to recover most of the underlying IllustrisTNG halo spin bias signal. Our analysis represents the first attempt to develop a future observational probe for halo spin bias, bringing forward alternative routes for measuring the secondary bias effects.

arXiv comment17 pages, 10 figures, submitted to MNRAS

References in corpus (104)

• Planck 2015 results. XIII. Cosmological parameters
• Planck 2013 results. XVI. Cosmological parameters
• Populating a cluster of galaxies - I. Results at z=0
• E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
• Cosmological SPH simulations: A hybrid multi-phase model for star formation
• Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
• The Average Star Formation Histories of Galaxies in Dark Matter Halos from z=0-8
• Simulating Galaxy Formation with the IllustrisTNG Model
• First results from the IllustrisTNG simulations: matter and galaxy clustering
• Properties of galaxies reproduced by a hydrodynamic simulation
• The Temperature of the Cosmic Microwave Background
• Substructures in hydrodynamical cluster simulations
• MultiDark simulations: the story of dark matter halo concentrations and density profiles
• The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and the Y_SZ-M_500 relation
• A universal angular momentum profile for galactic halos
• The Connection between Galaxies and their Dark Matter Halos
• Galaxy Clusters Discovered via the Sunyaev-Zel'dovich Effect in the 2500-square-degree SPT-SZ survey
• The age dependence of halo clustering
• The Dependence of Halo Clustering on Halo Formation History, Concentration, and Occupation
• Calibrator Design for the COBE Far Infrared Absolute Spectrophotometer (FIRAS)
• The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology
• The Atacama Cosmology Telescope: Sunyaev-Zel'dovich Selected Galaxy Clusters at 148 GHz from Three Seasons of Data
• Assembly bias in the clustering of dark matter haloes
• Cluster Cosmology Constraints from the 2500 deg${}^2$ SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope
• On the environmental dependence of halo formation
• The Atacama Cosmology Telescope: Sunyaev Zel'dovich Selected Galaxy Clusters at 148 GHz in the 2008 Survey
• Cosmic flows in the nearby universe from Type Ia Supernovae
• Evidence of Galaxy Cluster Motions with the Kinematic Sunyaev-Zel'dovich Effect
• On the Cluster Physics of Sunyaev-Zel'dovich Surveys I: The Influence of Feedback, Non-thermal Pressure and Cluster Shapes on Y-M Scaling Relations
• The Dark Side of Galaxy Color
• X-ray Properties of the First SZE-selected Galaxy Cluster Sample from the South Pole Telescope
• On Halo Formation Times and Assembly Bias
• Introducing Decorated HODs: modeling assembly bias in the galaxy-halo connection
• Testing $\Lambda$CDM at the lowest redshifts with SN Ia and galaxy velocities
• Evidence for the kinematic Sunyaev-Zeľdovich effect with ACTPol and velocity reconstruction from BOSS
• Beyond Assembly Bias: Exploring Secondary Halo Biases for Cluster-size Haloes
• Exploring Cosmic Origins with CORE: Survey requirements and mission design
• Halo assembly bias and the tidal anisotropy of the local halo environment
• Evidence of Halo Assembly Bias in Massive Clusters
• The 6dF Galaxy Velocity Survey: Cosmological constraints from the velocity power spectrum
• The MUSIC of Galaxy Clusters I: Baryon properties and Scaling Relations of the thermal Sunyaev-Zel'dovich Effect
• Confirmation of the Copernican principle at Gpc radial scale and above from the kinetic Sunyaev Zel'dovich effect power spectrum
• On the Level of Cluster Assembly Bias in SDSS
• The Atacama Cosmology Telescope: Dynamical Masses and Scaling Relations for a Sample of Massive Sunyaev-Zel'dovich Effect Selected Galaxy Clusters
• The 6dF Galaxy Survey: The Near-Infrared Fundamental Plane of Early-Type Galaxies
• On Detecting Halo Assembly Bias with Galaxy Populations
• Dark Energy from the Thermal Sunyaev Zeldovich Power Spectrum
• Are peculiar velocity surveys competitive as a cosmological probe?
• Atomic hydrogen in IllustrisTNG galaxies: the impact of environment parallelled with local 21-cm surveys
• A Measurement of the Kinetic Sunyaev-Zel'dovich Signal Toward MACS J0717.5+3745
• The Dark Side of Galaxy Color: evidence from new SDSS measurements of galaxy clustering and lensing
• Measuring cosmic bulk flows with Type Ia Supernovae from the Nearby Supernova Factory
• The assembly bias of dark matter haloes to higher orders
• Detection of the pairwise kinematic Sunyaev-Zel'dovich effect with BOSS DR11 and the Atacama Cosmology Telescope
• Cosmological Constraints from Type Ia Supernovae Peculiar Velocity Measurements
• Constraints on Assembly Bias from Galaxy Clustering
• Dark Energy Constraints from Galaxy Cluster Peculiar Velocities
• Spatial Clustering of Dark Matter Halos: Secondary Bias, Neighbor Bias, and the Influence of Massive Neighbors on Halo Properties
• The Taipan Galaxy Survey: Scientific Goals and Observing Strategy
• Mapping the kinetic Sunyaev-Zel'dovich effect toward MACS J0717.5+3745 with NIKA
• Constraints on gravity and dark energy from the pairwise kinematic Sunyaev-Zeldovich effect
• The Three Causes of Low-Mass Assembly Bias
• Properties of HI discs in the Auriga cosmological simulations
• Cosmic web anisotropy is the primary indicator of halo assembly bias
• A Multi-wavelength Study of the Sunyaev-Zel'dovich Effect in the Triple-Merger Cluster MACS J0717.5+3745 with MUSTANG and Bolocam
• Evidence for galaxy assembly bias in BOSS CMASS redshift-space galaxy correlation function
• Large-scale assembly bias of dark matter halos
• Correlation properties of the kinematic Sunyaev-Zel'dovich effect and implications for Dark Energy
• The multidimensional dependence of halo bias in the eye of a machine: a tale of halo structure, assembly and environment
• Planck intermediate results. XXXVII. Evidence of unbound gas from the kinetic Sunyaev-Zeldovich effect
• The Scale-Dependence of Halo Assembly Bias
• Improving constraints on the growth rate of structure by modelling the density-velocity cross-correlation in the 6dF Galaxy Survey
• Kinetic Sunyaev-Zel'dovich effect from halo rotation
• Reconstructing cosmic growth with kSZ observations in the era of Stage IV experiments
• Merger induced scatter and bias in the cluster mass - Sunyaev-Zeldovich effect scaling relation
• The dependence of halo bias on age, concentration and spin
• Cosmological Constraints from Galaxy Cluster Velocity Statistics
• The manifestation of secondary halo bias on the galaxy population from IllustrisTNG300
• Observational evidence of galaxy assembly bias
• Imaging the Thermal and Kinematic Sunyaev-Zel'dovich Effect Signals in a Sample of Ten Massive Galaxy Clusters: Constraints on Internal Velocity Structures and Bulk Velocities
• Kinetic Sunyaev-Zeldovich effect from galaxy cluster rotation
• On the measurements of assembly bias and splashback radius using optically selected galaxy clusters
• Combined analysis of galaxy cluster number count, thermal Sunyaev-Zel'dovich power spectrum, and bispectrum
• No evidence for bulk velocity from type Ia supernovae
• The nature of assembly bias - II. Halo spin
• The Secondary Spin Bias of Dark Matter Haloes
• Kinetic Sunyaev--Zel'dovich effect in rotating galaxy clusters from MUSIC simulations
• Probing Galaxy Assembly Bias in BOSS Galaxies Using Void Probabilities
• Measurement of the pairwise kinematic Sunyaev-Zeldovich effect with Planck and BOSS data
• The physical origins of low-mass spin bias
• Complementarity of Peculiar Velocity Surveys and Redshift Space Distortions for Testing Gravity
• Including massive neutrinos in thermal Sunyaev Zeldovich power spectrum and cluster counts analyses
• Exploring Cosmic Origins with CORE: Cluster Science
• Cosmology with the pairwise kinematic SZ effect: Calibration and validation using hydrodynamical simulations
• Anisotropic halo assembly bias and redshift-space distortions
• Probing galaxy assembly bias with LRG weak lensing observations
• Some assembly required: assembly bias in massive dark matter halos
• Testing Gravity Using Type Ia Supernovae Discovered by Next-Generation Wide-Field Imaging Surveys
• Separate Universe calibration of the dependence of halo bias on cosmic web anisotropy
• Probing gaseous galactic halos through the rotational kSZ effect
• Analytical halo models of cosmic tidal fields
• Exploring the dusty star-formation in the early Universe using intensity mapping
• Joint cosmology and mass calibration from tSZ cluster counts and cosmic shear
• Prospects for Detection of Intracluster Gas Bulk Velocities Through the Sunyaev-Zel'dovich Effect

Cited by in corpus (10)

• On the influence of halo mass accretion history on galaxy properties and assembly bias
• The physical origins of low-mass spin bias
• The galaxy size - halo mass scaling relations and clustering properties of central and satellite galaxies
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• Galaxy cluster rotation revealed in the MACSIS simulations with the kinetic Sunyaev-Zeldovich effect
• High-fidelity reproduction of central galaxy joint distributions with Neural Networks
• Spin speed correlations and the evolution of galaxy-halo systems
• Exploring the halo-galaxy connection with probabilistic approaches
• Towards an Observational Detection of Halo Spin Bias using Spin-Orbit Coherence
• Mimicking the halo-galaxy connection using machine learning