The Dependence of Halo Clustering on Halo Formation History, Concentration, and Occupation

Abstract

We investigate the dependence of dark matter halo clustering on halo formation time, density profile concentration, and subhalo occupation number, using high-resolution numerical simulations of a LCDM cosmology. We confirm results that halo clustering is a function of halo formation time, and that this trend depends on halo mass. For the first time, we show unequivocally that halo clustering is a function of halo concentration and show that the dependence of halo bias on concentration, mass, and redshift can be accurately parameterized in a simple way: b(c,M|z) = b(M|z) b(c|M/M*). The scaling between bias and concentration changes sign with the value of M/M*: high concentration (early forming) objects cluster more strongly for M <~ M* while low concentration (late forming) objects cluster more strongly for rare high-mass halos, M >~ M*. We show the first explicit demonstration that host dark halo clustering depends on the halo occupation number (of dark matter subhalos) and discuss implications for halo model calculations of dark matter power spectra and galaxy clustering statistics. The effect of these halo properties on clustering is strongest for early-forming dwarf-mass halos, which are significantly more clustered than typical halos of their mass. Our results suggest that isolated low-mass galaxies (e.g. low surface-brightness dwarfs) should have more slowly-rising rotation curves than their clustered counterparts, and may have consequences for the dearth of dwarf galaxies in voids. They also imply that self calibrating richness-selected cluster samples with their clustering properties might overestimate cluster masses and bias cosmological parameter estimation.

arXiv comment13 pages, 6 figures; Figure 3 best viewed in color, ApJ in press (replaced to match accepted version, updated literature discussion)

References in corpus (91)

• A Universal Density Profile from Hierarchical Clustering
• Simulating the joint evolution of quasars, galaxies and their large-scale distribution
• Large scale bias and the peak background split
• Populating a cluster of galaxies - I. Results at z=0
• The broken hierarchy of galaxy formation
• Profiles of dark haloes: evolution, scatter, and environment
• Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons
• Halo Models of Large Scale Structure
• Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes
• An analytic model for the spatial clustering of dark matter haloes
• Chandra sample of nearby relaxed galaxy clusters: mass, gas fraction, and mass-temperature relation
• Concentrations of Dark Halos from their Assembly Histories
• Analytic model for galaxy and dark matter clustering
• The Fourth Data Release of the Sloan Digital Sky Survey
• The formation history of elliptical galaxies
• Halo occupation numbers and galaxy bias
• The Dark Side of the Halo Occupation Distribution
• The Halo Occupation Distribution: Towards an Empirical Determination of the Relation Between Galaxies and Mass
• Reionization and the abundance of galactic satellites
• Modeling Luminosity-Dependent Galaxy Clustering Through Cosmic Time
• The age dependence of halo clustering
• Adaptive Refinement Tree - a new high-resolution N-body code for cosmological simulations
• The subhalo populations of LCDM dark haloes
• How Many Galaxies Fit in a Halo? Constraints on Galaxy Formation Efficiency from Spatial Clustering
• Galaxy Clustering in Early SDSS Redshift Data
• The tumultuous lives of galactic dwarfs and the missing satellites problem
• The Shape of Dark Matter Halos: Dependence on Mass, Redshift, Radius, and Formation
• Constraints from Dynamical Friction on the Dark Matter Content of Barred Galaxies
• Galaxies in N-body simulations: overcoming the overmerging problem
• The 2dF Galaxy Redshift Survey: The dependence of galaxy clustering on luminosity and spectral type
• The Nature of Galaxy Bias and Clustering
• The 2dF Galaxy Redshift Survey: Luminosity dependence of galaxy clustering
• Halo Substructure And The Power Spectrum
• The Halo Occupation Distribution and the Physics of Galaxy Formation
• On the Mass-to-Light Ratio of Large Scale Structure
• The DEEP2 Galaxy Redshift Survey: The Galaxy Luminosity Function to z ~ 1
• How to Plant a Merger Tree
• The Growth and Structure of Dark Matter Haloes
• The Physics of Galaxy Clustering I: A Model for Subhalo Populations
• The origin of angular momentum in dark matter halos
• Cosmic Star Formation History and its Dependence on Galaxy Stellar Mass
• Deriving the Nonlinear Cosmological Power Spectrum and Bispectrum from Analytic Dark Matter Halo Profiles and Mass Functions
• High-Resolution Measurements of the Halos of Four Dark Matter-Dominated Galaxies: Deviations from a Universal Density Profile
• Numerical study of halo concentrations in dark-energy cosmologies
• On the environmental dependence of halo formation
• GALICS I: A hybrid N-body semi-analytic model of hierarchical galaxy formation
• The Void Phenomenon
• The overdensities of galaxy environments as a function of luminosity and color
• Galaxy Formation and Large-Scale Bias
• Dwarf Galaxy Rotation Curves and the Core Problem of Dark Matter Halos
• The Radial Distribution of Galaxies in LCDM clusters
• Linking Early and Late Type Galaxies to their Dark Matter Haloes
• Constraints on the Structure of Dark Matter Halos from the Rotation Curves of Low Surface Brightness Galaxies
• A marked correlation function analysis of halo formation times in the Millennium Simulation
• Self Calibration in Cluster Studies of Dark Energy: Combining the Cluster Redshift Distribution, the Power Spectrum and Mass Measurements
• Semi-analytical model of galaxy formation with high-resolution N-body simulations
• On the Life and Death of Satellite Haloes
• Self-Calibration of Cluster Dark Energy Studies: Observable-Mass Distribution
• Modeling Galaxy-Mass Correlations in Dissipationless Simulations
• Large scale bias and stochasticity of halos and dark matter
• The DEEP2 Galaxy Redshift Survey: Clustering of Galaxies in Early Data
• Squelched Galaxies and Dark Halos
• Galaxy Halo Occupation at High Redshift
• CDM and Strong Lensing: Concord or Conflict?
• The Luminosity-Weighted or `Marked' Correlation Function
• Origin and evolution of halo bias in linear and non-linear regimes
• Towards Cosmological Concordance on Galactic Scales
• The dependence on environment of Cold Dark Matter Halo properties
• Galaxy formation using halo merger histories taken from N-body simulations
• Inflation, cold dark matter, and the central density problem
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• Galaxy Voids in Cold Dark Matter Universes
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• The Evidence of Absence: Galaxy Voids in the Excursion Set Formalism
• Close Galaxy Counts as a Probe of Hierarchical Structure Formation
• Spatial Distribution of Low Surface Brightness Galaxies
• Redshift-Space Distortions with the Halo Occupation Distribution I: Numerical Simulations
• Observational Evidence for an Age Dependence of Halo Bias
• Voids in the Simulated Local Universe
• Interpreting the Relationship Between Galaxy Luminosity, Color and Environment
• Galaxy Formation at z~3: Constraints from Spatial Clustering
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• The environmental dependence of galaxy clustering in the Sloan Digital Sky Survey
• Constraining the Projected Radial Distribution of Galactic Satellites with the Sloan Digital Sky Survey
• The Evolution of Substructure in Galaxy, Group and Cluster Haloes II: Global Properties
• Spatial distribution of galactic halos and their merger histories
• The halo-model description of marked statistics
• The environment of Low Surface Brightness Galaxies
• The environmental dependence of clustering in hierarchical models
• Marked correlations in galaxy formation models

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• Modeling Redshift-Space Clustering with Abundance Matching
• Analytical halo model of galactic conformity
• Halo Histories vs. Galaxy Properties at z=0, III: The Properties of Star-Forming Galaxies
• The Effect of Assembly Bias on Redshift Space Distortions
• Alignments of dark matter halos with large-scale tidal fields: mass and redshift dependence
• Connections between galaxy properties and halo formation time in the cosmic web
• Rosella: A mock catalogue from the P-Millennium simulation
• Spin and structural halo properties at high redshift in a LCDM Universe
• The galaxy - halo connection in low mass halos
• HOD modelling of high redshift galaxies using the BLUETIDES simulation
• Investigation of the orientation of galaxies in clusters: the importance, methods and results of research
• Close Pairs as Proxies for Galaxy Cluster Mergers
• On the kinetic Sunyaev-Zel'dovich effect as an observational probe for halo spin bias
• Modeling assembly bias with machine learning and symbolic regression
• Halo assembly bias from a deep learning model of halo formation
• Using galaxy pairs to investigate the three-point correlation function in the squeezed limit
• The halo model with beyond-linear halo bias: unbiasing cosmological constraints from galaxy-galaxy lensing and clustering
• AXES-SDSS: comparison of SDSS galaxy groups with all-sky X-ray extended sources
• Separate Universe calibration of the dependence of halo bias on cosmic web anisotropy
• Assembly Bias of Dwarf-sized Dark Matter Haloes
• How the Galaxy-Halo Connection Depends on Large-Scale Environment
• 2D k-th nearest neighbor statistics: a highly informative probe of galaxy clustering
• Mock halo catalogs: assigning unresolved halo properties using correlations with local halo environment
• Denser Environments Cultivate Larger Galaxies: A Comprehensive Study beyond the Local Universe with 3 Million Hyper Suprime-Cam Galaxies
• SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model
• The impact of environment on the dynamical structure of satellite systems
• The Local Void: for or against LCDM?
• Tidal stripping as a test of satellite quenching in redMaPPer clusters
• Disentangling cosmic-ray and dark-matter induced gamma-rays in galaxy clusters?
• Interpreting the cosmic far-infrared background anisotropies using a gas regulator model
• The Tessellation-Level-Tree: characterising the nested hierarchy of density peaks and their spatial distribution in cosmological N-body simulations
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• Spatial and Kinematic Clustering of Stars in the Galactic Disk
• The Beyond-Halo Mass Effects of the Cosmic Web Environment on Galaxies
• Environmental Effects of Dark Matter Haloes: The Clustering-Substructure relation of Group-size Haloes
• Groups of two galaxies in SDSS: implications of colours on star formation quenching time-scales
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Constraining the Galaxy-Halo Connection with Optimal Statistics
• BASILISK: Bayesian Hierarchical Inference of the Galaxy-Halo Connection using Satellite Kinematics--I. Method and Validation
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension
• On merger bias and the clustering of quasars
• On the origin of red spirals: Does assembly bias play a role?
• Resolving the problem of galaxy clustering on small scales: any new physics needed?
• The phenomenology of the external field effect in cold dark matter models
• Global analysis of luminosity- and colour-dependent galaxy clustering in the Sloan Digital Sky Survey
• Approximations to galaxy star formation rate histories: properties and uses of two examples
• The Last Journey. II. SMACC -- Subhalo Mass-loss Analysis using Core Catalogs
• The mass accretion history of dark matter haloes down to Earth mass
• Close Galaxy Pairs at z = 3: A Challenge to UV Luminosity Abundance Matching
• PRIMUS: Clustering of Star-forming and Quiescent Central Galaxies at $0.2<z<0.9$
• Galaxy assembly bias in the stellar-to-halo mass relation for red central galaxies from SDSS
• The quasi-adiabatic relaxation of haloes in the IllustrisTNG and EAGLE cosmological simulations
• Constraining the mass-concentration relation through weak lensing peak function
• LARgE Survey -- II. The Dark Matter Halos and the Progenitors and Descendants of Ultra-Massive Passive Galaxies at Cosmic Noon
• Dark matter halo assembly bias: environmental dependence in the non-Markovian excursion set theory
• Merging Tree Algorithm of Growing Voids in Self Similar and CDM Models
• Screened fifth forces in parity-breaking correlation functions
• A new test of gravity -- I: Introduction to the method
• Beyond Mass: Detecting Secondary Halo Properties with Galaxy-Galaxy Lensing
• The morphology of star-forming gas and its alignment with galaxies and dark matter haloes in the EAGLE simulations
• A Pair of Early- and Late-Forming Galaxy Cluster Samples: a Novel Way of Studying Halo Assembly Bias Assisted by a Constrained Simulation
• Exploring the physical origins of halo assembly bias from early times
• Astraeus VII: The environmental-dependent assembly of galaxies in the Epoch of Reionization
• Star-forming and Quiescent Central Galaxies Cluster Similarly: Implications for the Galaxy-Halo Connection
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• Cluster Assembly Times as a Cosmological Test
• New insight into the variability of the Be star $\pi$ Aquarii: Determination of stellar and disk parameters
• Testing the Large-Scale Environments of Cool-core and Noncool-core Clusters with Clustering Bias
• Unexpected clustering pattern in dwarf galaxies challenges formation models
• Secondary halo bias through cosmic time II: Reconstructing halo properties using clustering information
• Evaluating the origins of the secondary bias based on the correlation of halo properties with the linear density field
• Non-Gaussian assembly bias from a semi-analytic galaxy formation model
• Characterizing the assembly of dark matter halos with protohalo size histories: I. Redshift evolution, relation to descendant halos, and halo assembly bias
• Subhalo abundance matching using progenitor mass at varying redshift: Two modes of stellar mass growth imprinted into the Subaru HSC galaxy clustering
• Dark Matter Halos: The Dynamical Basis of Effective Empirical Models
• Cosmological constraints from galaxy clustering and galaxy-galaxy lensing with extended SubHalo Abundance Matching
• Unraveling emission line galaxy conformity at z~1 with DESI early data
• Mass accretion rates and multi-scale halo environment in cold and warm dark matter cosmologies
• How do uncertainties in galaxy formation physics impact field-level galaxy bias?
• Probabilistic Estimators of Lagrangian Shape Biases: Universal Relations and Physical Insights
• Dependence on the environment of the abundance function of light-cone simulation dark matter haloes
• The SRG/eROSITA All-Sky Survey: Exploring halo assembly bias with X-ray selected superclusters
• Fundamental properties of the dark and the luminous matter from Low Surface Brightness discs
• Properties beyond mass for unresolved haloes across redshift and cosmology using correlations with local halo environment
• The impact of halo concentration on the Sunyaev Zel'dovich effect signal from massive galaxy clusters
• FLORAH: A generative model for halo assembly histories
• Caught in the cosmic web: environmental effects on subhalo abundance and internal density profiles
• The Dependence of Dark Matter Halo Properties on the Morphology of Their Central Galaxies from Weak Lensing
• Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
• BASILISK II. Improved Constraints on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• Dark matter halo concentrations: a short review
• Inverse Hubble Flows in Molecular Clouds
• Statistical Decoupling of Lagrangian Fluid Parcel in Newtonian Cosmology
• Probabilistic Lagrangian bias estimators and the cumulant bias expansion
• Bounds on galaxy stochasticity from halo occupation distribution modeling
• The Pseudo Evolution of Galaxy-Cluster Masses and Its Connection to Mass Density Profile
• DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [OII] Luminosity
• Gamma Rays from Annihilations at the Galactic Center in a Physical Dark Matter Distribution
• Assembly bias in quadratic bias parameters of dark matter halos from forward modeling
• Atomic Hydrogen Shows its True Colours: Correlations between HI and Galaxy Colour in Simulations
• One-point Statistics in various cosmic environments in the presence of massive neutrinos
• MIGHTEE: The dark matter haloes, duty cycle and mechanical feedback from radio-AGN up to $z\sim 2.5$
• One Galaxy Sample to Rule Them All: Halo Occupation Distribution Modeling of DES Year 3 Source Galaxies
• Cosmo-Paleontology: Statistics of Fossil Groups in a Gravity-Only Simulation
• The multi-dimensional halo assembly bias can be preserved when enhancing halo properties with HALOSCOPE
• Predicting halo occupation and galaxy assembly bias with machine learning
• Individual halo bias in models of $f(R)$ gravity
• Exploiting Non-linear Scales in Galaxy-Galaxy Lensing and Galaxy Clustering: A Forecast for the Dark Energy Survey
• On the dependence of galaxy assembly bias on the selection criteria, number density, and redshift of galaxy samples
• Elucidating the impact of massive neutrinos on halo assembly bias
• On the Assembly Bias of Cool Core Clusters Traced by H$\alpha$ Nebulae
• Galaxy assembly bias in cosmological hydrodynamical simulations: a comparison between SIMBA and IllustrisTNG
• Towards an Observational Detection of Halo Spin Bias using Spin-Orbit Coherence
• Reconciling concentration to virial mass relations
• Tidal Grinding of Dwarf Galaxies in Cluster Environments
• Testing subhalo abundance matching with galaxy kinematics
• Predicting Halo Formation Time Using Machine Learning
• The impact of projection effects on cluster observables: stacked lensing and projected clustering
• Origin & evolution of the Universe
• Correlation between Outlying Halo Abundance and Host Halo Properties
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• Clustering and physical properties of AGN and Star-Forming Galaxies at fixed stellar mass: does assembly bias have a role in AGN activity?
• Towards a universal model for the density profiles of dark matter haloes
• A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution