The age dependence of halo clustering

Abstract

We use a very large simulation of the concordance LCDM cosmogony to study the clustering of dark matter haloes. For haloes less massive than about 1e13Msun/h, the amplitude of the two-point correlation function on large scales depends strongly on halo formation time. Haloes that assembled at high redshift are substantially more clustered than those that assembled more recently. The effect is a smooth function of halo formation time and its amplitude increases with decreasing halo mass. At 1e11 Msun/h the ``oldest'' 10% of haloes are more than 5 times more strongly correlated than the ``youngest'' 10%. This unexpected result is incompatible with the standard excursion set theory for structure growth, and it contradicts a fundamental assumption of the halo occupation distribution models often used to study galaxy clustering, namely that the galaxy content of a halo of given mass is statistically independent of its larger scale environment.

5 pages, 5 figures, MNRAS in press. Full resolution pdf file is avaliable at http://www.mpa-garching.mpg.de/~gaoliang/GSW.pdf

References in corpus (1)

• The Physics of Galaxy Clustering I: A Model for Subhalo Populations

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• The halo model with beyond-linear halo bias: unbiasing cosmological constraints from galaxy-galaxy lensing and clustering
• Separate Universe calibration of the dependence of halo bias on cosmic web anisotropy
• Analytical halo models of cosmic tidal fields
• The environment and redshift dependence of accretion onto dark matter halos and subhalos
• Galaxy clustering from the bottom up: A Streaming Model emulator I
• Assembly Bias of Dwarf-sized Dark Matter Haloes
• Evolution of central galaxy alignments in simulations
• 2D k-th nearest neighbor statistics: a highly informative probe of galaxy clustering
• Tidal stripping as a test of satellite quenching in redMaPPer clusters
• 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
• Hubble Frontier Field Clusters and their Parallel Fields: Photometric and Photometric Redshift Catalogs
• The Local Void: for or against LCDM?
• Close galaxy pairs with accurate photometric redshifts
• The scale dependence of mass assembly in galaxies
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• Environmental Effects of Dark Matter Haloes: The Clustering-Substructure relation of Group-size Haloes
• The Beyond-Halo Mass Effects of the Cosmic Web Environment on Galaxies
• Galaxy and Mass Assembly (GAMA): The Weak Environmental Dependence of Quasar Activity at 0.1<z<0.35
• The Tessellation-Level-Tree: characterising the nested hierarchy of density peaks and their spatial distribution in cosmological N-body simulations
• The impact of assembly history on the X-ray detectability of halos. From galaxy groups to galaxy clusters
• Using the Star Forming Main Sequence To Explore Quiescent Galaxies Across Cosmic Time
• Early results from GLASS-JWST. XX: Unveiling a population of "red-excess'' galaxies in Abell2744 and in the coeval field
• The Bridge Effect of Void Filaments
• The Ultramarine Simulation: properties of dark matter haloes before redshift 5.5
• The Large-scale Effect of Environment on Galactic Conformity
• Revisiting the clustering of narrow-line AGN in the local Universe: Joint dependence on stellar mass and color
• An Enhanced Massive Black Hole Occupation Fraction Predicted in Cluster Dwarf Galaxies
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Constraining the Galaxy-Halo Connection with Optimal Statistics
• The contribution of star-forming galaxies to fluctuations in the cosmic background light
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• Quenching in the Right Place at the Right Time: Tracing the Shared History of Starbursts, AGNs, and Post-starburst Galaxies Using Their Structures and Multiscale Environments
• Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF
• On the origin of red spirals: Does assembly bias play a role?
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension
• Direct signatures of the formation time of galaxies
• Resolving the problem of galaxy clustering on small scales: any new physics needed?
• On merger bias and the clustering of quasars
• 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
• Constraining galaxy-halo connection with high-order statistics
• Cosmological test of local position invariance from the asymmetric galaxy clustering
• A Machine Learning Approach to Galaxy-LSS Classification I: Imprints on Halo Merger Trees
• The mass accretion history of dark matter haloes down to Earth mass
• Lagrangian Methods Of Cosmic Web Classification
• Assembly bias evidence in close galaxy pairs
• LARgE Survey -- II. The Dark Matter Halos and the Progenitors and Descendants of Ultra-Massive Passive Galaxies at Cosmic Noon
• Beyond Mass: Detecting Secondary Halo Properties with Galaxy-Galaxy Lensing
• The fractional Brownian motion and the halo mass function
• FLY: MPI-2 High Resolution code for LSS Cosmological Simulations
• A sparse regression approach to modeling the relation between galaxy stellar masses and their host halos
• Andromeda XXV -- a dwarf galaxy with a low central dark matter density
• Merging Tree Algorithm of Growing Voids in Self Similar and CDM Models
• Screened fifth forces in parity-breaking correlation functions
• Effects of correlation between merging steps on the global halo formation
• Dark matter halo assembly bias: environmental dependence in the non-Markovian excursion set theory
• A Pair of Early- and Late-Forming Galaxy Cluster Samples: a Novel Way of Studying Halo Assembly Bias Assisted by a Constrained Simulation
• MultiCAM: A multivariable framework for connecting the mass accretion history of haloes with their properties
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• Star-forming and Quiescent Central Galaxies Cluster Similarly: Implications for the Galaxy-Halo Connection
• Exploring the physical origins of halo assembly bias from early times
• New insight into the variability of the Be star $\pi$ Aquarii: Determination of stellar and disk parameters
• Cluster Assembly Times as a Cosmological Test
• Testing the Large-Scale Environments of Cool-core and Noncool-core Clusters with Clustering Bias
• The Two-Point Correlation Function of Gamma-ray Bursts
• Unexpected clustering pattern in dwarf galaxies challenges formation models
• 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
• On the Constraints of Galaxy Assembly Bias in Velocity Space
• Large scale correlations in gas traced by MgII absorbers around low mass galaxies
• Bimodal Formation Time Distribution for Infall Dark Matter Halos
• Secondary halo bias through cosmic time II: Reconstructing halo properties using clustering information
• The formation and disruption of globular cluster populations in simulations of present-day $L^{\ast }$ galaxies with controlled assembly histories
• Unraveling emission line galaxy conformity at z~1 with DESI early data
• Anisotropy and characteristic scales in halo density gradient profiles
• The galaxy bias profile of cosmic voids
• Evaluating the origins of the secondary bias based on the correlation of halo properties with the linear density field
• Cosmological constraints from galaxy clustering and galaxy-galaxy lensing with extended SubHalo Abundance Matching
• 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?
• The SRG/eROSITA All-Sky Survey: Exploring halo assembly bias with X-ray selected superclusters
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• Satellite Content and Halo Mass of Galaxy Clusters: Comparison between Red-Sequence and Halo-based Optical Cluster Finders
• Dependence on the environment of the abundance function of light-cone simulation dark matter haloes
• Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties
• Probabilistic Estimators of Lagrangian Shape Biases: Universal Relations and Physical Insights
• BASILISK II. Improved Constraints on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
• Environmental history of filament galaxies: stellar mass assembly and star-formation of filament galaxies
• Caught in the cosmic web: environmental effects on subhalo abundance and internal density profiles
• Properties beyond mass for unresolved haloes across redshift and cosmology using correlations with local halo environment
• Star-forming galaxies in the cosmic web in the last 11 Gyr
• The relation of galaxies and dark matter haloes to the filamentary cosmic web
• DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [OII] Luminosity
• Distinguishing thermal histories of dark matter from structure formation
• Atomic Hydrogen Shows its True Colours: Correlations between HI and Galaxy Colour in Simulations
• On the tomographic cluster clustering as a cosmological probe
• Distinguishing Orbiting and Infalling Dark Matter Particles with Machine Learning
• Probabilistic Lagrangian bias estimators and the cumulant bias expansion
• Assembly bias in quadratic bias parameters of dark matter halos from forward modeling
• Properties of Barred Galaxies with the Environment: II. The case of the Cosmic Web around the Virgo cluster
• Assessing the connection between galactic conformity and assembly-type bias
• Ultra High Energy Cosmic Rays from Sequestered X Bursts
• On the dependence of galaxy assembly bias on the selection criteria, number density, and redshift of galaxy samples
• The multi-dimensional halo assembly bias can be preserved when enhancing halo properties with HALOSCOPE
• Individual halo bias in models of $f(R)$ gravity
• MIGHTEE: The dark matter haloes, duty cycle and mechanical feedback from radio-AGN up to $z\sim 2.5$
• Predicting halo occupation and galaxy assembly bias with machine learning
• One Galaxy Sample to Rule Them All: Halo Occupation Distribution Modeling of DES Year 3 Source Galaxies
• Exploiting Non-linear Scales in Galaxy-Galaxy Lensing and Galaxy Clustering: A Forecast for the Dark Energy Survey
• Strong Conformity and Assembly Bias: Towards a Physical Understanding of the Galaxy-Halo Connection in SDSS Clusters
• Mechanisms Affecting Galaxies Nearby and Environmental Trends (MAGNET)
• Photometric and Spectroscopic Study of Abell 0671
• Elucidating the impact of massive neutrinos on halo assembly bias
• Galaxy assembly bias in cosmological hydrodynamical simulations: a comparison between SIMBA and IllustrisTNG
• On the Assembly Bias of Cool Core Clusters Traced by H$\alpha$ Nebulae
• The invariance of group occupation across the cosmic web
• Two-phase formation of galaxies: the coevolution between galaxies and dark matter halos
• Towards an Observational Detection of Halo Spin Bias using Spin-Orbit Coherence
• Insights into the dependence of galaxy properties on the environment with explainable machine learning models
• Investigation of homogeneity and matter distribution on large scales using large quasar groups
• Imprints of tidal interactions on the stellar distribution of satellite galaxies: implications for dark matter deficient galaxies
• Correlation between Outlying Halo Abundance and Host Halo Properties
• Tidal Grinding of Dwarf Galaxies in Cluster Environments
• A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
• The life and times of dark matter haloes: what will I be when I grow up?
• Clustering and physical properties of AGN and Star-Forming Galaxies at fixed stellar mass: does assembly bias have a role in AGN activity?
• Testing subhalo abundance matching with galaxy kinematics
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• Mimicking the halo-galaxy connection using machine learning
• Predicting Halo Formation Time Using Machine Learning