Assembly bias in the clustering of dark matter haloes

Abstract

We use a very large simulation of structure growth in a LCDM universe -- the Millennium Simulation -- to study assembly bias, the fact that the large-scale clustering of haloes of given mass varies significantly with their assembly history. We extend earlier work based on the same simulation by superposing results for redshifts from 0 to 3, by defining a less noisy estimator of clustering amplitude, and by considering halo concentration, substructure mass fraction and spin, as well as formation time, as additional parameters. These improvements lead to results with less noise than previous studies and covering a wider range of halo masses and structural properties. We find significant and significantly different assembly bias effects for all the halo properties we consider, although in all cases the dependences on halo mass and on redshift are adequately described as a dependence on equivalent peak height nu(M,z). The nu-dependences for different halo properties differ qualitatively and are not related as might naively be expected given the relations between formation time, concentration, substructure fraction and spin found for the halo population as a whole. These results suggest that it will be difficult to build models for the galaxy populations of dark haloes which can robustly relate the amplitude of large-scale galaxy clustering to that for mass clustering at better than the 10% level.

arXiv comment5 pages, 1 figures. MNRAS letters in press, Error analysis added

References in corpus (25)

• A Universal Density Profile from Hierarchical Clustering
• The cosmological simulation code GADGET-2
• Simulating the joint evolution of quasars, galaxies and their large-scale distribution
• Populating a cluster of galaxies - I. Results at z=0
• A Line of Sight Approach to Cosmic Microwave Background Anisotropies
• An analytic model for the spatial clustering of dark matter haloes
• Using the Evolution of Clusters to Constrain Omega
• Halo occupation numbers and galaxy bias
• A universal angular momentum profile for galactic halos
• The age dependence of halo clustering
• The subhalo populations of LCDM dark haloes
• Constraining Galaxy Formation and Cosmology with the Conditional Luminosity Function of Galaxies
• The Dependence of Halo Clustering on Halo Formation History, Concentration, and Occupation
• Properties of Dark Matter Haloes in Clusters, Filaments, Sheets and Voids
• The Nature of Galaxy Bias and Clustering
• Spatial correlation function and pairwise velocity dispersion of galaxies: CDM models versus the Las Campanas Survey
• The Halo Occupation Distribution and the Physics of Galaxy Formation
• Galaxy Formation and Large-Scale Bias
• A marked correlation function analysis of halo formation times in the Millennium Simulation
• Environmental Dependence of Cold Dark Matter Halo Formation
• The Clustering of Massive Halos
• Asymmetries in the inner regions of LCDM haloes
• The Dependence of the Occupation of Galaxies on the Halo Formation Time
• Observational Evidence for an Age Dependence of Halo Bias
• Galaxy Formation at z~3: Constraints from Spatial Clustering

Cited by in corpus (297)

• A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: I. Galaxy Mergers & Quasar Activity
• Observational Probes of Cosmic Acceleration
• Resolving Cosmic Structure Formation with the Millennium-II Simulation
• Large-Scale Galaxy Bias
• How do galaxies populate Dark Matter halos?
• Galaxy Evolution from Halo Occupation Distribution Modeling of DEEP2 and SDSS Galaxy Clustering
• Concentration, Spin and Shape of Dark Matter Haloes: Scatter and the Dependence on Mass and Environment
• Dark matter and cosmic structure
• The Connection between Galaxies and Dark Matter Structures in the Local Universe
• The realm of the galaxy protoclusters
• Ly Alpha-Emitting Galaxies at z=3.1: L* Progenitors Experiencing Rapid Star Formation
• The Evolution of Dark Matter Halo Properties in Clusters, Filaments, Sheets and Voids
• Cosmological parameter constraints from galaxy-galaxy lensing and galaxy clustering with the SDSS DR7
• Halo Assembly Bias in Hierarchical Structure Formation
• Cosmological Constraints from a Combination of Galaxy Clustering and Lensing -- I. Theoretical Framework
• The Hydrangea simulations: galaxy formation in and around massive clusters
• Lensing is Low: Cosmology, Galaxy Formation, or New Physics?
• Galaxy Assembly Bias: A Significant Source of Systematic Error in the Galaxy-Halo Relationship
• Ingredients for 21cm intensity mapping
• Mapping stellar content to dark matter halos using galaxy clustering and galaxy-galaxy lensing in the SDSS DR7
• Detection of the Splashback Radius and Halo Assembly bias of Massive Galaxy Clusters
• An algorithm to build mock galaxy catalogues using MICE simulations
• The spin and orientation of dark matter halos within cosmic filaments
• Tidal Effects and the Environment Dependence of Halo Assembly
• Introducing Decorated HODs: modeling assembly bias in the galaxy-halo connection
• On Halo Formation Times and Assembly Bias
• Subhalo abundance matching and assembly bias in the EAGLE simulation
• Galaxy alignments: Theory, modelling and simulations
• Understanding the shape of the halo-mass and galaxy-mass cross-correlation functions
• The Weak Lensing Signal and the Clustering of BOSS Galaxies II: Astrophysical and Cosmological Constraints
• Cosmological Constraints from Galaxy Clustering and the Mass-to-Number Ratio of Galaxy Clusters
• The Impact of Assembly Bias on the Galaxy Content of Dark Matter Halos
• Environmental Dependence of Dark Matter Halo Growth I: Halo Merger Rates
• Assembly bias and the dynamical structure of dark matter halos
• Beyond Assembly Bias: Exploring Secondary Halo Biases for Cluster-size Haloes
• The Cusp/Core problem and the Secondary Infall Model
• Full calculation of clumpiness boost factors for antimatter cosmic rays in the light of Lambda-CDM N-body simulation results
• Orbits of Massive Satellite Galaxies: I. A Close Look at the Large Magellanic Cloud and a New Orbital History for M33
• Evidence of Halo Assembly Bias in Massive Clusters
• The Evolution of Central Group Galaxies in Hydrodynamical Simulations
• The origin of scatter in the star formation rate - stellar mass relation
• The impact of assembly bias on the halo occupation in hydrodynamical simulations
• Beyond Halo Mass: Galactic Conformity as a Smoking Gun of Central Galaxy Assembly Bias
• Internal properties and environments of dark matter halos
• On the Level of Cluster Assembly Bias in SDSS
• The Dependence of Subhalo Abundance on Halo Concentration
• SDSS Galaxy Clustering: Luminosity & Colour Dependence and Stochasticity
• Disentangling galaxy environment and host halo mass
• Limitations to the "basic'' HOD model and beyond
• Optimal Constraints on Local Primordial Non-Gaussianity from the Two-Point Statistics of Large-Scale Structure
• The Co-Formation of Spheroids and Quasars Traced in their Clustering
• The Copernicus Complexio: a high-resolution view of the small-scale Universe
• Dark Matter Halo Growth II: Diffuse Accretion and its Environmental Dependence
• ZOMG-I. How the cosmic web inhibits halo growth and generates assembly bias
• The assembly bias of dark matter haloes to higher orders
• Revealing the galaxy-halo connection in IllustrisTNG
• Mapping the Dark Matter From UV Light at High Redshift: An Empirical Approach to Understand Galaxy Statistics
• The Void Phenomenon Explained
• The New Horizon Run Cosmological N-Body Simulations
• Consistent lensing and clustering in a low-$S_8$ Universe with BOSS, DES Year 3, HSC Year 1 and KiDS-1000
• The Baryonic Tully-Fisher Relationship for S${}^4$G Galaxies and the "Condensed" Baryon Fraction of Galaxies
• Constraints on Assembly Bias from Galaxy Clustering
• Spatial Clustering of Dark Matter Halos: Secondary Bias, Neighbor Bias, and the Influence of Massive Neighbors on Halo Properties
• Connecting massive galaxies to dark matter halos in BOSS - I. Is galaxy color a stochastic process in high-mass halos?
• Assembly Bias and Splashback in Galaxy Clusters
• Detecting Neutrino Mass by Combining Matter Clustering, Halos, and Voids
• Radiative Transfer Modeling of Lyman Alpha Emitters. II. New Effects in Galaxy Clustering
• Dissecting and Modelling Galaxy Assembly Bias
• Environmental dependence in the ellipsoidal collapse model
• The Three Causes of Low-Mass Assembly Bias
• The Evolution of Assembly Bias
• The statistical properties of LCDM halo formation
• Transformation of Morphology and Luminosity Classes of the SDSS Galaxies
• Cosmic web anisotropy is the primary indicator of halo assembly bias
• Constraints on the correlation between QSO luminosity and host halo mass from high-redshift quasar clustering
• The distribution of ejected subhalos and its implication for halo assembly bias
• On the Physical Origin of Galactic Conformity
• The Peaks Formalism and the Formation of Cold Dark Matter Haloes
• Stringent ${\sigma }_8$ constraints from small-scale galaxy clustering using a hybrid MCMC+emulator framework
• The GOGREEN survey: The environmental dependence of the star-forming galaxy main sequence at $1.0<z<1.5$
• Evidence for galaxy assembly bias in BOSS CMASS redshift-space galaxy correlation function
• Statistics of Dark Matter Substructure: III. Halo-to-Halo Variance
• Density profile slope in Dwarfs and environment
• N-body simulations with generic non-Gaussian initial conditions II: Halo bias
• Large-scale assembly bias of dark matter halos
• The Galaxy Clustering Crisis in Abundance Matching
• The clustering of SDSS galaxy groups: mass and color dependence
• Connecting Reionization to the Local Universe
• A flexible modelling of galaxy assembly bias
• The atomic Hydrogen content of the post-reionization Universe
• Galaxy And Mass Assembly (GAMA): growing up in a bad neighbourhood - how do low-mass galaxies become passive?
• Properties of Dark Matter Halos as a Function of Local Environment Density
• A Confirmation of the Strong Clustering of Distant Red Galaxies at 2 < z <3
• The Birth and Growth of Neutralino Haloes
• On the Density profile slope of Clusters of Galaxies
• Clustering properties of galaxies selected in stellar mass: Breaking down the link between luminous and dark matter in massive galaxies from z=0 to z=2
• The multidimensional dependence of halo bias in the eye of a machine: a tale of halo structure, assembly and environment
• Constraining the HI-Halo Mass Relation From Galaxy Clustering
• Non-Gaussian halo assembly bias
• The Scale-Dependence of Halo Assembly Bias
• Intrinsic alignments in redMaPPer clusters -- I. Central galaxy alignments and angular segregation of satellites
• Merger induced scatter and bias in the cluster mass - Sunyaev-Zeldovich effect scaling relation
• Halo Histories vs. Galaxy Properties at z=0 II: Large-Scale Galactic Conformity
• Caught in the cosmic web: Environmental effect on halo concentrations, shape, and spin
• The dependence of halo bias on age, concentration and spin
• Mapping stellar content to dark matter halos - III.Environmental dependence and conformity of galaxy colours
• The nature of assembly bias - I. Clues from a LCDM cosmology
• A KiDS weak lensing analysis of assembly bias in GAMA galaxy groups
• Interpreting the Clustering of Distant Red Galaxies
• A natural boundary of dark matter haloes revealed around the minimum bias and maximum infall locations
• Exploring the squeezed three-point galaxy correlation function with generalized halo occupation distribution models
• Direct Measurement of the HI-Halo Mass Relation through Stacking
• The manifestation of secondary halo bias on the galaxy population from IllustrisTNG300
• The impact of galaxy formation on satellite kinematics and redshift-space distortions
• Environmental Effects on Real-Space and Redshift-Space Galaxy Clustering
• On the influence of halo mass accretion history on galaxy properties and assembly bias
• Elucidating Galaxy Assembly Bias in SDSS
• Cosmic Ballet III: halo spin evolution in the cosmic web
• The Immitigable Nature of Assembly Bias: The Impact of Halo Definition on Assembly Bias
• The MillenniumTNG Project: An improved two-halo model for the galaxy-halo connection of red and blue galaxies
• Illustrating galaxy-halo connection in the DESI era with IllustrisTNG
• Baryons in the CosmicWeb of IllustrisTNG -- II: the Connection among Galaxies, Halos, their Formation Time and their Location in the Cosmic Web
• Halo Histories vs. Galaxy Properties at z=0, I: The Quenching of Star Formation
• Exploring galaxy colour in different environments of the cosmic web with SDSS
• On the measurements of assembly bias and splashback radius using optically selected galaxy clusters
• Modeling color-dependent galaxy clustering in cosmological simulations
• The nature of assembly bias - III. Observational properties
• The nature of assembly bias - II. Halo spin
• PRIMUS: One- and Two-Halo Galactic Conformity at $0.2<z<1$
• Halo stochasticity in global clustering analysis
• The Effects of Halo Assembly Bias on Self-Calibration in Galaxy Cluster Surveys
• BAM: Bias Assignment Method to generate mock catalogs
• Galaxy formation on the largest scales: The impact of astrophysics on the BAO peak
• Detection of anisotropic galaxy assembly bias in BOSS DR12
• Assembly bias in the local PNG halo bias and its implication for $f_{\mathrm{NL}}$ constraints
• Halo abundances within the cosmic web
• The Secondary Spin Bias of Dark Matter Haloes
• Relating the structure of dark matter halos to their assembly and environment
• Tidal-induced lopsidedness in Magellanic-type galaxies
• Does the Galaxy-Halo Connection Vary with Environment?
• Testing Cold Dark Matter with the hierarchical buildup of stellar light
• How are galaxies assigned to halos? Searching for assembly bias in the SDSS galaxy clustering
• Cosmology with Stacked Cluster Weak Lensing and Cluster-Galaxy Cross-Correlations
• The Correlated Formation Histories of Massive Galaxies and Their Dark Matter Halos
• Galaxy assembly bias of central galaxies in the Illustris simulation
• Scale dependence of galaxy biasing investigated by weak gravitational lensing: An assessment using semi-analytic galaxies and simulated lensing data
• Void Galaxies Follow a Distinct Evolutionary Path in the Environmental COntext Catalog
• Effects of large-scale environment on the assembly history of central galaxies
• $\mathrm{S}\mathrm{IM}\mathrm{BIG}$: Mock Challenge for a Forward Modeling Approach to Galaxy Clustering
• A First Look at creating mock catalogs with machine learning techniques
• Extensions to the halo occupation distribution model for more accurate clustering predictions
• The physical origins of low-mass spin bias
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): ${\Omega }_{{\mathrm{m}}_0}$ from the galaxy clustering ratio measured at $z\sim 1$
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• Relative clustering and the joint halo occupation distribution of red-sequence and blue-cloud galaxies in COMBO-17
• Cosmological Evidence Modelling: a new simulation-based approach to constrain cosmology on non-linear scales
• Predictably Missing Satellites: Subhalo Abundance in Milky Way-like Halos
• The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching
• What determines large scale galaxy clustering: halo mass or local density?
• Revealing the cosmic web dependent halo bias
• Cross-correlation of galaxies and galaxy clusters in the Sloan Digital Sky Survey and the importance of non-Poissonian shot noise
• A Flexible Analytic Model of Cosmic Variance in the First Billion Years
• The influence of halo assembly on galaxies and galaxy groups
• Probing dark energy with future redshift surveys: A comparison of emission line and broad band selection in the near infrared
• On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection
• The cosmological dependence of halo and galaxy assembly bias
• The galaxy size - halo mass scaling relations and clustering properties of central and satellite galaxies
• Can Assembly Bias Explain the Lensing Amplitude of the BOSS CMASS Sample in a Planck Cosmology?
• Local and global environmental effects on galaxies and active galactic nuclei
• Galactic conformity measured in semi-analytic models
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• The binary-host connection: astrophysics of gravitational wave binaries from their host galaxy properties
• Probing the galaxy-halo connection with total satellite luminosity
• Cosmological information content in redshift-space power spectrum of SDSS-like galaxies in the quasi-nonlinear regime up to $k=0.3h$Mpc${}^{-1}$
• Anisotropic halo assembly bias and redshift-space distortions
• The MillenniumTNG Project: The large-scale clustering of galaxies
• Probing galaxy assembly bias with LRG weak lensing observations
• Deviations from tidal torque theory: environment dependences on halo angular momentum growth
• First measurement of the characteristic depletion radius of dark matter haloes from weak lensing
• An accurate method to determine the systematics due to the peculiar velocities of galaxies in measuring the Hubble constant from gravitational wave standard sirens
• Characterizing dark interactions with the halo mass accretion history and structural properties
• The effects of halo alignment and shape on the clustering of galaxies
• Galaxy star formation in different environments
• Some assembly required: assembly bias in massive dark matter halos
• Evidence of Galaxy Assembly Bias in SDSS DR7 Galaxy Samples from Count Statistics
• SDSS-IV MaNGA: Signatures of halo assembly in kinematically misaligned galaxies
• SHAM through the lens of a hydrodynamical simulation
• The age dependence of galaxy clustering
• Don't Forget the Forest for the Trees: The Stellar-Mass Halo-Mass Relation in Different Environments
• Illuminating Dark Matter Halo Density Profiles Without Subhaloes
• Observational Measures of Halo Properties Beyond Mass
• ZOMG III: The effect of Halo Assembly on the Satellite Population
• The Dark Matter Haloes of Chandra X-ray Galaxy Clusters and Baryons Effect
• Halo Properties and Mass Functions of Groups/Clusters from the DESI Legacy Imaging Surveys DR9
• Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
• Testing Galaxy Quenching Theories with Scatter in the Stellar to Halo Mass Relation
• A study on the statistical significance of mutual information between morphology of a galaxy and its large-scale environment
• Extracting HI Astrophysics from Interferometric Intensity Mapping
• The Effects of Galaxy Assembly Bias on the Inference of Growth Rate from Redshift-Space Distortions
• Dark matter halo occupation: environment and clustering
• Passive Evolution of Galaxy Clustering
• Luminosity bias: from haloes to galaxies
• One simulation to have them all: performance of the Bias Assignment Method against N-body simulations
• Dissecting the spin distribution of Dark Matter halos
• Halo Assembly Bias in the Quasi-linear Regime
• The assembly bias of emission line galaxies
• The cosmic web connection to the dark matter halo distribution through gravity
• Dark Matter Halo Mergers I: Dependence on Environment & Redshift Evolution
• Halo Histories vs. Galaxy Properties at z=0, III: The Properties of Star-Forming Galaxies
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• Revisiting the Galaxy Shape and Spin Alignments with the Large-Scale Tidal Field: An Effective Practical Model
• Interrelation of the environment of Ly$\alpha$ emitters and massive galaxies at $2<z<4.5$
• Connections between galaxy properties and halo formation time in the cosmic web
• The Effect of Assembly Bias on Redshift Space Distortions
• Rosella: A mock catalogue from the P-Millennium simulation
• Spin and structural halo properties at high redshift in a LCDM Universe
• Halo assembly bias from a deep learning model of halo formation
• Statistical properties of dark matter mini-haloes at z >= 15
• On the kinetic Sunyaev-Zel'dovich effect as an observational probe for halo spin bias
• Close Pairs as Proxies for Galaxy Cluster Mergers
• Green valley galaxies in the cosmic web: internal versus environmental quenching
• 2D k-th nearest neighbor statistics: a highly informative probe of galaxy clustering
• The environment and redshift dependence of accretion onto dark matter halos and subhalos
• Assembly Bias of Dwarf-sized Dark Matter Haloes
• Galaxy clustering from the bottom up: A Streaming Model emulator I
• KiDS+VIKING+GAMA: Halo occupation distributions and correlations of satellite numbers with a new halo model of the galaxy-matter bispectrum for galaxy-galaxy-galaxy lensing
• SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model
• Opening Reionization: Quantitative Morphology of the Epoch of Reionization and Its Connection to the Cosmic Density Field
• Determining the large-scale environmental dependence of gas-phase metallicity in dwarf galaxies
• Denser Environments Cultivate Larger Galaxies: A Comprehensive Study beyond the Local Universe with 3 Million Hyper Suprime-Cam Galaxies
• The impact of environment on the dynamical structure of satellite systems
• The Tessellation-Level-Tree: characterising the nested hierarchy of density peaks and their spatial distribution in cosmological N-body simulations
• 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
• Do galactic bars depend on environment?: An information theoretic analysis of Galaxy Zoo 2
• The impact of assembly history on the X-ray detectability of halos. From galaxy groups to galaxy clusters
• The causal effect of environment on halo mass and concentration
• Revisiting the clustering of narrow-line AGN in the local Universe: Joint dependence on stellar mass and color
• Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• An Enhanced Massive Black Hole Occupation Fraction Predicted in Cluster Dwarf Galaxies
• Biasing relation, environmental dependencies and estimation of the growth rate from star forming galaxies
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension
• On merger bias and the clustering of quasars
• Resolving the problem of galaxy clustering on small scales: any new physics needed?
• On the origin of red spirals: Does assembly bias play a role?
• Can a conditioning on stellar mass explain the mutual information between morphology and environment?
• A Framework for Simultaneously Measuring Field Densities and the High-z Luminosity Function
• The mass accretion history of dark matter haloes down to Earth mass
• The Planck SZ Cluster Catalog: Expected X-ray Properties
• A sparse regression approach to modeling the relation between galaxy stellar masses and their host halos
• Assembly bias evidence in close galaxy pairs
• Dark matter halo assembly bias: environmental dependence in the non-Markovian excursion set theory
• The correlations between galaxy properties in different environments of the cosmic web
• LARgE Survey -- II. The Dark Matter Halos and the Progenitors and Descendants of Ultra-Massive Passive Galaxies at Cosmic Noon
• New insight into the variability of the Be star $\pi$ Aquarii: Determination of stellar and disk parameters
• Astraeus VII: The environmental-dependent assembly of galaxies in the Epoch of Reionization
• Constraining cosmological parameters using void statistics from the SDSS survey
• Exploring the physical origins of halo assembly bias from early times
• Testing the Large-Scale Environments of Cool-core and Noncool-core Clusters with Clustering Bias
• Subhalo abundance matching using progenitor mass at varying redshift: Two modes of stellar mass growth imprinted into the Subaru HSC galaxy clustering
• Characterizing the assembly of dark matter halos with protohalo size histories: I. Redshift evolution, relation to descendant halos, and halo assembly bias
• Bimodal Formation Time Distribution for Infall Dark Matter Halos
• Non-Gaussian assembly bias from a semi-analytic galaxy formation model
• Unraveling emission line galaxy conformity at z~1 with DESI early data
• Flattening of dark matter cusps during mergers: model of M31
• Evaluating the origins of the secondary bias based on the correlation of halo properties with the linear density field
• Secondary halo bias through cosmic time II: Reconstructing halo properties using clustering information
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• Probabilistic Estimators of Lagrangian Shape Biases: Universal Relations and Physical Insights
• Making use of sub-resolution halos in N-body simulations
• The SRG/eROSITA All-Sky Survey: Exploring halo assembly bias with X-ray selected superclusters
• 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
• The viability of low-mass subhaloes as targets for gamma-ray dark matter searches
• Mass accretion rates and multi-scale halo environment in cold and warm dark matter cosmologies
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• Properties beyond mass for unresolved haloes across redshift and cosmology using correlations with local halo environment
• Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• The Pseudo Evolution of Galaxy-Cluster Masses and Its Connection to Mass Density Profile
• Assembly bias in quadratic bias parameters of dark matter halos from forward modeling
• Probabilistic Lagrangian bias estimators and the cumulant bias expansion
• Towards an Observational Detection of Halo Spin Bias using Spin-Orbit Coherence
• Exploiting Non-linear Scales in Galaxy-Galaxy Lensing and Galaxy Clustering: A Forecast for the Dark Energy Survey
• Predicting halo occupation and galaxy assembly bias with machine learning
• On the Assembly Bias of Cool Core Clusters Traced by H$\alpha$ Nebulae
• MIGHTEE: The dark matter haloes, duty cycle and mechanical feedback from radio-AGN up to $z\sim 2.5$
• Galaxy assembly bias in cosmological hydrodynamical simulations: a comparison between SIMBA and IllustrisTNG
• How the Coherent Tides Obstruct the Radial Infalls of Satellite Galaxies onto Clusters
• Disc instability and bar formation: view from the IllustrisTNG simulations
• Individual halo bias in models of $f(R)$ gravity
• On the dependence of galaxy assembly bias on the selection criteria, number density, and redshift of galaxy samples
• One Galaxy Sample to Rule Them All: Halo Occupation Distribution Modeling of DES Year 3 Source Galaxies
• Elucidating the impact of massive neutrinos on halo assembly bias
• Clustering and physical properties of AGN and Star-Forming Galaxies at fixed stellar mass: does assembly bias have a role in AGN activity?
• Galaxy quenching across the Cosmic Web: disentangling mass and environment with SDSS DR18