MultiDark simulations: the story of dark matter halo concentrations and density profiles

Abstract

Accurately predicting structural properties of dark matter halos is one of the fundamental goals of modern cosmology. We use the new suite of MultiDark cosmological simulations to study the evolution of dark matter halo density profiles, concentrations, and velocity anisotropies. The MultiDark simulations cover a large range of masses 1e10-1e15Msun and volumes upto 50Gpc**3. The total number of dark matter halos in all the simulations exceeds 60 billion. We find that in order to understand the structure of dark matter halos and to make ~1% accurate predictions for density profiles, one needs to realize that halo concentration is more complex than the traditional ratio of the virial radius to the core radius in the NFW profile. For massive halos the averge density profile is far from the NFW shape and the concentration is defined by both the core radius and the shape parameter alpha in the Einasto approximation. Combining results from different redshifts, masses and cosmologies, we show that halos progress through three stages of evolution. (1) They start as rare density peaks that experience very fast and nearly radial infall. This radial infall brings mass closer to the center producing a high concentrated halo. Here, the halo concentration increases with the increasing halo mass and the concentration is defined by the alpha parameter with nearly constant core radius. Later halos slide into (2) the plateau regime where the accretion becomes less radial, but frequent mergers still affect even the central region. Now the concentration does not depend on halo mass. (3) Once the rate of accretion slows down, halos move into the domain of declining concentration-mass relation because new accretion piles up mass close to the virial radius while the core radius is staying constant. We provide accurate analytical fits to the numerical results for halo density profiles and concentrations.

22 pages, 23 figures, accepted by MNRAS

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• Cosmological Simulations of Dwarf Galaxies with Cosmic Ray Feedback
• Tracing the gravitational potential using cosmic voids
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• Tempestuous life beyond R500: X-ray view on the Coma cluster with SRG/eROSITA. II. Shock & Relic
• A model of spectral line broadening in signal forecasts for line-intensity mapping experiments
• DAWIS, a Detection Algorithm with Wavelets for Intracluster light Studies
• General relativistic 'screening' in cosmological simulations
• First Constraints on the Epoch of Reionization Using the non-Gaussianity of the Kinematic Sunyaev-Zel{'}dovich Effect from the South Pole Telescope and {\it Herschel}-SPIRE Observations
• Baryon Pasting Algorithm: Halo-based and Particle-based Pasting Methods
• Some assembly required: assembly bias in massive dark matter halos
• Machine Learning methods to estimate observational properties of galaxy clusters in large volume cosmological N-body simulations
• The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
• Evidence of Galaxy Assembly Bias in SDSS DR7 Galaxy Samples from Count Statistics
• The Effective Field Theory of Large-Scale Structure and Multi-tracer
• What to expect from dynamical modelling of cluster haloes II. Investigating dynamical state indicators with Random Forest
• UniverseMachine: Predicting Galaxy Star Formation over Seven Decades of Halo Mass with Zoom-in Simulations
• The halo mass function and inner structure of ETHOS haloes at high redshift
• On the Cosmic Web Elongation in Fuzzy Dark Matter Cosmologies: Effects on Density Profiles, Shapes and Alignments of Halos
• A population of ultraviolet-dim protoclusters detected in absorption
• The Three Hundred project: galaxy cluster mergers and their impact on the stellar component of brightest cluster galaxies
• Analysis of Unified Galaxy Power Spectrum Multipole Measurements
• AstraeusIV : Quantifying the star formation histories of galaxies in the Epoch of Reionization
• GalWeight Application: A publicly-available catalog of dynamical parameters of 1,800 galaxy clusters from SDSS-DR13, ($GalWCat19$)
• The bivariate gas-stellar mass distributions and the mass functions of early- and late-type galaxies at $z\sim 0$
• The Three Hundred: Cluster Dynamical States and Relaxation Time Scale
• Cosmology and Astrophysics from Relaxed Galaxy Clusters V: Consistency with Cold Dark Matter Structure Formation
• The Uchuu-UniverseMachine dataset: Galaxies in and around Clusters
• The BINGO Project VI: HI Halo Occupation Distribution and Mock Building
• Illuminating Dark Matter Halo Density Profiles Without Subhaloes
• The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmic Flows and Cosmic Web from Luminous Red Galaxies
• The HI intensity mapping bispectrum including observational effects
• Emission from the Ionized Gaseous Halos of Low Redshift Galaxies and Their Neighbors
• Power spectrum multipole expansion for HI intensity mapping experiments: unbiased parameter estimation
• Generating Synthetic Cosmological Data with GalSampler
• Stellar and Weak Lensing Profiles of Massive Galaxies in the Hyper-Suprime Cam Survey and in Hydrodynamic Simulations
• Synthetic ${}^{26}$Al emission from galactic-scale superbubble simulations
• The Outer Stellar Mass of Massive Galaxies: A Simple Tracer of Halo Mass with Scatter Comparable to Richness and Reduced Projection Effects
• Cosmological Constraints from Galaxy Cluster Sparsity, Cluster Gas Mass Fraction and Baryon Acoustic Oscillations Data
• Multipolar moments of weak lensing signal around clusters. Weighing filaments in harmonic space
• Effects of long-wavelength fluctuations in large galaxy surveys
• The bias of dark matter tracers: assessing the accuracy of mapping techniques
• Weak lensing mass modeling bias and the impact of miscentring
• Constraining the cross-section of dark matter with giant radial arcs in galaxy clusters
• Major mergers between dark matter haloes -- II. Profile and concentration changes
• Scaling relations for globular cluster systems in early-type galaxies
• Which Milky Way masses are consistent with the slightly declining 5-25 kpc rotation curve?
• Reconstruction of Radio Relics and X-ray Tails in an Off-axis Cluster Merger: Hydrodynamical Simulations of A115
• The Three Hundred project: Galaxy groups do not survive cluster infall
• Can intrinsic alignments of elongated low-mass galaxies be used to map the cosmic web at high redshift?
• Building robust AGN mock catalogs to unveil black hole evolution and for survey planning
• New Analytic Solutions for Galaxy Evolution II: Wind Recycling, Galactic Fountains and Late-Type Galaxies
• RedMaPPer: Evolution and Mass Dependence of the Conditional Luminosity Functions of Red Galaxies in Galaxy Clusters
• DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
• PNG-UNITsims: Halo clustering response to primordial non-Gaussianities as a function of mass
• GalWeight: A New and Effective Weighting Technique for Determining Galaxy Cluster and Group Membership
• Understanding large-scale structure in the SSA22 protocluster region using cosmological simulations
• [OII] emitters in MultiDark-Galaxies and DEEP2
• The Three Hundred project: A Machine Learning method to infer clusters of galaxies mass radial profiles from mock Sunyaev-Zel'dovich maps
• Universal clustering of dark matter in phase space
• Surrogate modelling the Baryonic Universe II: on forward modelling the colours of individual and populations of galaxies
• The assembly bias of emission line galaxies
• A measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel'dovich effect with SPT-3G and DES
• ROGER: Reconstructing Orbits of Galaxies in Extreme Regions using machine learning techniques
• The Three Hundred Project: The gas disruption of infalling objects in cluster environments
• On the Prevalence of Super-Massive Black Holes over Cosmic Time
• Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
• Beta-Skeleton Analysis of the Cosmic Web
• Astraeus VI: Hierarchical assembly of AGN and their large-scale effect during the Epoch of Reionization
• Maturing Satellite Kinematics into a Competitive Probe of the Galaxy-Halo Connection
• Turning Around along the Cosmic Web
• The distribution of dark matter and gas spanning six megaparsecs around the post-merger galaxy cluster MS0451-03
• Improving baryon acoustic oscillation measurement with the combination of cosmic voids and galaxies
• Pushing down the low-mass halo concentration frontier with the Lomonosov cosmological simulations
• MultiDark-Clusters: Galaxy Cluster Mock Light-Cones, eROSITA and the Cluster Power Spectrum
• The Three Hundred project: connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
• Clustering Constraints on the Relative Sizes of Central and Satellite Galaxies
• What to expect from dynamical modelling of cluster haloes I. The information content of different dynamical tracers
• Hierarchical inference of the relationship between Concentration and Mass in Galaxy Groups and Clusters
• Constraining Reionization in Progress at z=5.7 with Lyman-$\alpha$ Emitters: Voids, Peaks, and Cosmic Variance
• Main Sequence Scatter is Real: The Joint Dependence of Galaxy Clustering on Star Formation and Stellar Mass
• Assessing the accuracy of cosmological parameters estimated from velocity -- density comparisons via simulations
• The Dark Side of Using Dark Sirens to Constrain the Hubble-Lemaître Constant
• The Concentration-Mass Relation of Massive, Dynamically Relaxed Galaxy Clusters: Agreement Between Observations and $\Lambda$CDM Simulations
• Thermodynamic evolution of the $z=1.75$ galaxy cluster IDCS J1426.5+3508
• The galaxy HI-(sub)halo connection and the HI spatial clustering of local galaxies
• Effects of Completeness and Purity on Cluster Dark Energy Constraints
• The Three Hundred Project: the evolution of physical baryon profiles
• Some observational tests of a minimal galaxy formation model
• BASS. XXXVI. Constraining the Local Supermassive Black Hole - Halo Connection with BASS DR2 AGN
• On the coherent rotation of diffuse matter in numerical simulations of galaxy clusters
• Major mergers between dark matter haloes -- I. Predictions for size, shape, and spin
• Structure and dynamics in low density regions: galaxy-galaxy correlations inside cosmic voids
• The HI-halo mass relation at redshift $z\sim 1$ from the Minkowski functionals of 21 cm intensity maps
• Modeling Redshift-Space Clustering with Abundance Matching
• New Local Volume Dwarf Galaxy Candidates from the DESI Legacy Imaging Surveys
• Detecting the Figure Rotation of Dark Matter Halos with Tidal Streams
• Monte Carlo Physarum Machine: Characteristics of Pattern Formation in Continuous Stochastic Transport Networks
• Revisiting the Galaxy Shape and Spin Alignments with the Large-Scale Tidal Field: An Effective Practical Model
• The SAGA Survey. V. Modeling Satellite Systems around Milky Way-mass Galaxies with Updated UniverseMachine
• The cosmic web around the Coma cluster from constrained cosmological simulations: I. Filaments connected to Coma at $z=0$
• Tidal Stripping and Post-Merger Relaxation of Dark Matter Halos: Causes and Consequences of Mass Loss
• Biases and Cosmic Variance in Molecular Gas Abundance Measurements
• Accurate halo-galaxy mocks from automatic bias estimation and particle mesh gravity solvers
• Setting firmer constraints on the evolution of the most massive, central galaxies from their local abundances and ages
• Virial halo mass function in the $Planck$ cosmology
• Brightest Cluster Galaxies Trace Weak Lensing Mass Bias and Halo Triaxiality in The Three Hundred Project
• From Cosmicflows distance moduli to unbiased distances and peculiar velocities
• Dynamical masses of brightest cluster galaxies I: stellar velocity anisotropy and mass-to-light ratios
• Predicting fully self-consistent satellite richness, galaxy growth and starformation rates from the STastical sEmi-Empirical modeL STEEL
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). The matter density and baryon fraction from the galaxy power spectrum at redshift $0.6<z<1.1$
• Halo concentrations from extended Press-Schechter merger histories
• Estimating the Turn-Around Radii of Six Isolated Galaxy Groups in the Local Universe
• On estimating the cosmic molecular gas density from CO Line Intensity Mapping observations
• The Origin of Lopsided Satellite Galaxy Distribution in Galaxy Pairs
• Hybrid analytic and machine-learned baryonic property insertion into galactic dark matter haloes
• Kinematics of cluster galaxies and their relation to galaxy evolution
• Exploring the High-Mass End of the Stellar Mass Function of Star Forming Galaxies at Cosmic Noon
• Astraeus III: The environment and physical properties of reionization sources
• The effects of peculiar velocities in SN Ia environments on the local $H_0$ measurement
• Emission line ratios for the Circumgalactic Medium and the "Bimodal" Nature of Galaxies
• Mass Functions, Luminosity Functions, and Completeness Measurements from Clustering Redshifts
• Extragalactic diffuse gamma-rays from dark matter annihilation: revised prediction and full modelling uncertainties
• Galaxy Three-Point Correlation Functions and Halo/Subhalo Models
• A minimal empirical model for the cosmic far-infrared background anisotropies
• Modelling the star-formation activity and ionizing properties of high-redshift galaxies
• The Relevance of Dynamical Friction for the MW/LMC/SMC Triple System
• Discriminating power of milli-lensing observations for dark matter models
• Reconsidering the dynamical states of galaxy clusters using PCA and UMAP
• Testing the parametric model for self-interacting dark matter using matched halos in cosmological simulations
• On the kinetic Sunyaev-Zel'dovich effect as an observational probe for halo spin bias
• Bayesian redshift-space distortions correction from galaxy redshift surveys
• Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
• Correlation function: biasing and fractal properties of the cosmic web
• The redshift dependence of Alcock-Paczynski effect: cosmological constraints from the current and next generation observations
• Detecting clusters and groups of galaxies populating the local Universe in large optical spectroscopic surveys
• On The Effect of Environment on Line Emission from the Circumgalactic Medium
• The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0<z<7
• Deep+Wide Lensing Surveys will Provide Exquisite Measurements of the Dark Matter Halos of Dwarf Galaxies
• On the origin of the gamma-ray emission from Omega Centauri: Milisecond pulsars and dark matter annihilation
• Forecasting the success of the WEAVE Wide-Field Cluster Survey on the extraction of the cosmic web filaments around galaxy clusters
• AXES-SDSS: comparison of SDSS galaxy groups with all-sky X-ray extended sources
• Improving the Cosmological Constraints by Inferring the Formation Channel of Extreme-mass-ratio Inspirals
• On the general nature of 21cm-Lyman-$\alpha$ emitters cross-correlations during reionisation
• Characterising the Structure of Halo Merger Trees Using a Single Parameter: The Tree Entropy
• Constraining Scatter in the Stellar Mass--Halo Mass Relation for Haloes Less Massive than the Milky Way
• The Sejong Suite: Cosmological Hydrodynamical Simulations with Massive Neutrinos, Dark Radiation, and Warm Dark Matter
• Super-sample covariance of the thermal Sunyaev-Zel'dovich effect
• Constraining the scatter in the galaxy-halo connection at Milky Way masses
• A multi-tracer empirically-driven approach to line-intensity mapping lightcones
• Enhanced n-body annihilation of dark matter and its indirect signatures
• A joint 2- and 3-point clustering analysis of the VIPERS PDR2 catalogue at z~1: breaking the degeneracy of cosmological parameters
• Prospects for Determining the Mass Distributions of Galaxy Clusters on Large Scales Using Weak Gravitational Lensing
• Do satellite galaxies trace matter in galaxy clusters?
• ΛCDM is still not broken: empirical constraints on the star formation efficiency at z ~ 12-30
• Quasars at intermediate redshift are not special; but they are often satellites
• Dynamics of Merging Galaxy Clusters from Simulated Analogs
• The Multi-Tracer Optimal Estimator applied to VIPERS
• The Unusually High Halo Concentration of the Fossil Group NGC 6482: Evidence for Weak Adiabatic Contraction
• Bayesian framework to infer the Hubble constant from the cross-correlation of individual gravitational wave events with galaxies
• Recoiling Supermassive Black Hole Escape Velocities from Dark Matter Halos
• The SRG/eROSITA All-Sky Survey : Subaru/HSC-SSP weak-lensing mass measurements for the eRASS1 Galaxy Clusters
• OpenUniverse2024: A shared, simulated view of the sky for the next generation of cosmological surveys
• Clustering of CODEX clusters
• Dark matter halos in the multicomponent model. II. Density profiles of galactic halos
• The SFR-radius connection: data and implications for wind strength and halo concentration
• The SRG/eROSITA all-sky survey. X-ray emission from the warm-hot phase gas in long cosmic filaments
• Using GAMA to probe the impact of small-scale galaxy physics on nonlinear redshift-space distortions
• Observing Correlations Between Dark Matter Accretion and Galaxy Growth: I. Recent Star Formation Activity in Isolated Milky Way-Mass Galaxies
• Tidal stripping as a test of satellite quenching in redMaPPer clusters
• Not Hydro: Using Neural Networks to estimate galaxy properties on a Dark-Matter-Only simulation
• The Uchuu-GLAM BOSS and eBOSS LRG lightcones: Exploring clustering and covariance errors
• Distinctive GWBs from eccentric inspiraling SMBH binaries with a DM spike
• The Past History of Galaxy Clusters told by their present neighbors
• Accurate Model of the Projected Velocity Distribution of Galaxies in Dark Matter Halos
• Chandra Observations of the Spectacular A3411-12 Merger Event
• Tracking the orbit of unresolved subhalos for semi-analytic models
• Interferometric HI intensity mapping: perturbation theory predictions and foreground removal effects
• Constraining Cosmological Parameters using the Cluster Mass-Richness Relation
• Evolution of superclusters and supercluster cocoons in various cosmologies
• Painting baryons onto N-body simulations of galaxy clusters with image-to-image deep learning
• Probabilistic fibre-to-target assignment algorithm for multi-object spectroscopic surveys
• Anisotropic Satellite Galaxy Quenching: A Unique Signature of Energetic Feedback by Supermassive Black Holes?
• Large Scale Structure Reconstruction with Short-Wavelength Modes
• Reconstructing Orbits of Galaxies in Extreme Regions (ROGER) II: reliability of projected phase-space in our understanding of galaxy populations
• Validating the methodology for constraining the linear growth rate from clustering anisotropies
• Searching for dark matter annihilation from individual halos: uncertainties, scatter and signal-to-noise ratios
• Machine learning synthetic spectra for probabilistic redshift estimation: SYTH-Z
• Star Formation of Merging Disk Galaxies with AGN Feedback Effects
• A semi-analytical perspective on massive galaxies at $z\sim 0.55$
• Overdensity of VVV galaxies behind the Galactic bulge
• The Ultramarine Simulation: properties of dark matter haloes before redshift 5.5
• MaNGA DynPop -- IV. Stacked total density profile of galaxy groups and clusters from combining dynamical models of integral-field stellar kinematics and galaxy-galaxy lensing
• A deeper look into the structure of ΛCDM haloes: correlations between halo parameters from Einasto fits
• Halo Mass-Concentration Relation at High-Mass End
• Average Dark Matter Halo Sparsity Relations as Consistency Check of Mass Estimates in Galaxy Cluster Samples
• The causal effect of environment on halo mass and concentration
• Using the Mark Weighted Correlation Functions to Improve the Constraints on Cosmological Parameters
• Modelling Dark Matter Halo Spin using Observations and Simulations: application to UGC 5288
• BASILISK: Bayesian Hierarchical Inference of the Galaxy-Halo Connection using Satellite Kinematics--I. Method and Validation
• The probability of identifying the cosmic web environment of galaxies around clusters motivated by the Weave Wide Field Cluster Survey
• Dark-siren Cosmology with Decihertz Gravitational-wave Detectors
• Backsplash galaxies and their impact on galaxy evolution: a three-stage, four-type perspective
• Cluster-lensing: A Python Package for Galaxy Clusters & Miscentering
• First test of the consistency relation for the large-scale structure using the anisotropic three-point correlation function of BOSS DR12 galaxies (An explanatory video is available at https://youtu.be/Zi36ooLPhss.)
• A universal model for the evolution of tidally stripped systems
• Mass Estimation of Planck Galaxy Clusters using Deep Learning
• Testing emergent gravity with mass densities of galaxy clusters
• Statistics of Two-point Correlation and Network Topology for Lyman Alpha Emitters at $z\approx 2.67$
• An Empirical Model For Intrinsic Alignments: Insights From Cosmological Simulations
• Quantifying and controlling biases in dark matter halo concentration estimates
• Cosmic evolution of the incidence of Active Galactic Nuclei in massive clusters: Simulations versus observations
• Gravity and the Nonlinear Growth of Structure in the Carnegie-Spitzer-IMACS Redshift Survey
• An optimised tiling pattern for multi-object spectroscopic surveys: application to the 4MOST survey
• A Universal Profile for Stacked Filaments from Cold Dark Matter Simulations
• The extended Baryon Oscillation Spectroscopic Survey (eBOSS): testing a new approach to measure the evolution of the structure growth
• Constraining quenching timescales in galaxy clusters by forward-modelling stellar ages and quiescent fractions in projected phase space
• Boundless baryons: how diffuse gas contributes to anisotropic tSZ signal around simulated Three Hundred clusters
• Galaxy populations in haloes in high-density environments
• The Three Hundred project: Estimating the dependence of gas filaments on the mass of galaxy clusters
• The Dark Matter Halos of HI Selected Galaxies
• High-accuracy analytical solutions for the projected mass (counts) and surface density (brightness) of Einasto profiles
• PRIMUS: Clustering of Star-forming and Quiescent Central Galaxies at $0.2<z<0.9$
• Observing the Effects of Galaxy Interactions on the Circumgalactic Medium
• Physical modelling of galaxy clusters using Einasto dark matter profiles
• How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations
• Halo formation and evolution in scalar field dark matter and cold dark matter: New insights from the fluid approach
• Cross-Correlation Forecast of CSST Spectroscopic Galaxy and MeerKAT Neutral Hydrogen Intensity Mapping Surveys
• Galaxy assembly bias in the stellar-to-halo mass relation for red central galaxies from SDSS
• Foreground Removal of CO Intensity Mapping Using Deep Learning
• Disentangling the co-evolution of galaxies and supermassive black holes with PRIMA
• The impact of the halo spin-concentration relation on disc scaling laws
• Reconstructing Orbits of Galaxies in Extreme Regions (ROGER) III: galaxy evolution patterns in projected phase space around massive X-ray clusters
• The XXL survey. XLIX. Linking the members star formation histories to the cluster mass assembly in the z=1.98 galaxy cluster XLSSC 122
• Addressing $\gamma$-ray emissions from dark matter annihilations in 45 milky way satellite galaxies and in extragalactic sources with particle dark matter models
• Universal dark halo scaling relation for the dwarf spheroidal satellites
• CHEX-MATE: the intracluster medium entropy distribution in the gravity-dominated regime
• An efficient and robust method to estimate halo concentration
• Cosmological gravity on all scales III: non-linear matter power spectrum in phenomenological modified gravity
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• X-ray cluster cosmology
• The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
• Unveiling the Universe with Emerging Cosmological Probes
• Velocity dispersion vs cluster mass: a new scaling law with The Three Hundred clusters
• Geometric and growth rate tests of General Relativity with recovered linear cosmological perturbations
• Studying galaxy cluster morphological metrics with Mock-X
• A Random Walk Model for Dark Matter Halo Concentrations
• CHEX-MATE: A non-parametric deep learning technique to deproject and deconvolve galaxy cluster X-ray temperature profiles
• Accurate Analytic Mass-Scale Relations for Dark Matter Haloes of all Masses and Redshifts
• A stochastic model to reproduce the star-formation history of individual galaxies in hydrodynamic simulations
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• ISW in $\Lambda$CDM or something else?
• Quantifying the statistics of CMB-lensing-derived galaxy cluster mass measurements with simulations
• Segmenting the Universe into dynamically coherent basins
• Probing gaseous halos of galaxies with radio jets
• Accurate Modeling of the Projected Galaxy Clustering in Photometric Surveys: I. Tests with Mock Catalogs
• The abundance and environment of dark matter haloes
• A Model of the Cosmic Infrared Background Produced by Distant Galaxies
• SHARP -- IX. The dense, low-mass perturbers in B1938+666 and J0946+1006: implications for cold and self-interacting dark matter
• Estimating the confusion noise for the Millimetron space telescope
• Assessing the reliability of the Bisous filament finder
• Testing black holes in a perfect fluid dark matter environment using quasinormal modes
• Cluster Cosmology with the Velocity Distribution Function of the HeCS-SZ Sample
• Test of Cosmic Web-feeding Model for Star Formation in Galaxy Clusters in the COSMOS Field
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: Fourier space analysis
• Stellar Populations in a semi-analytic model I: bulges of Milky Way-like galaxies
• Star-forming and Quiescent Central Galaxies Cluster Similarly: Implications for the Galaxy-Halo Connection
• NeutralUniverseMachine: How Filaments and Dark Matter Halo Influence the Galaxy Cold Gas Content
• Galaxy pairs in The Three Hundred simulations: a study on the performance of observational pair-finding techniques
• The Three Hundred Project: Mapping The Matter Distribution in Galaxy Clusters Via Deep Learning from Multiview Simulated Observations
• Dark Matter Spike surrounding Supermassive Black Holes Binary and the Nanohertz Stochastic Gravitational Wave Background
• MultiCAM: A multivariable framework for connecting the mass accretion history of haloes with their properties
• CosmoDRAGoN simulations -- I. Dynamics and observable signatures of radio jets in cosmological environments
• The Galaxy Halo Connection in Modified Gravity Cosmologies: Environment Dependence of Galaxy Luminosity function
• On the contributions of extragalactic CO emission lines to ground-based CMB observations
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• Cosmic void exclusion models and their impact on the distance scale measurements from large scale structure
• Complementary Cosmological Simulations
• The size function of massive satellites from the $R_e-R_h$ and $M_{star}-M_h$ relations: constraining the role of environment
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: Possibility of estimateing the non-linear systematics using fast simulations
• "Observing" Unrelaxed Clusters in Dark Matter Simulations
• Galaxy pairs in The Three Hundred simulations II: studying bound ones and identifying them via machine learning
• Identifying Galaxy Cluster Mergers with Deep Neural Networks using Idealized Compton-y and X-ray maps
• The role of scatter and satellites in shaping the large-scale clustering of X-ray AGN as a function of host galaxy stellar mass
• Inferring Cosmological Parameters on SDSS via Domain-Generalized Neural Networks and Lightcone Simulations
• Extended Fast Action Minimisation method: application to SDSS-DR12 Combined Sample
• On the Constraints of Galaxy Assembly Bias in Velocity Space
• Cosmic Void Baryon Acoustic Oscillation Measurement: Evaluation of Sensitivity to Selection Effects
• Protoclusters at z=5.7: A view from the MultiDark galaxies
• The Three Hundred-NIKA2 Sunyaev-Zeldovich Large Program twin samples: Synthetic clusters to support real observations
• The Three Hundred Project: Modeling Baryon and Hot-Gas Fraction Evolution in Simulated Clusters
• Covariance matrices for variance-suppressed simulations
• The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar and APOGEE-2 Data
• Orbits and adiabatic contraction in scalar field dark matter halos: revisiting the cusp-core problem in dwarf galaxies
• The Spatial Range of Conformity
• Redshifted 21-cm emission signal from the halos in Dark Ages
• Probing Self-Interacting Dark Matter via Gravitational-Wave Background from Eccentric Supermassive Black Hole Mergers
• Improving Constraint on ${\Omega }_m$ from SDSS Using Marked Correlation Functions
• Constraining cosmology with the velocity function of low-mass galaxies
• Intrinsic mass-richness relation of clusters from THE THREE HUNDRED hydrodynamic simulations
• The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• Measuring the growth of structure by matching dark matter haloes to galaxies with VIPERS and SDSS
• LATIS: A Sample of IGM-selected Protoclusters and Protogroups at $z\sim 2.5$
• The evolution of low-mass central galaxies in the vicinity of massive structures and its impact on the two-halo conformity
• Environmental effects on associations of dwarf galaxies
• Resummed Kinetic Field Theory: a model of coupled baryonic and dark matter
• Shape and connectivity of groups and clusters: Impact of dynamical state and accretion history
• Leveraging cross-correlations and linear covariance-based filtering for line-intensity map reconstructions at linear scales
• CHEX-MATE: Multi-probe analysis of Abell 1689
• The Three Hundred: $M_{sub}-V_{circ}$ relation
• The Three Hundred Project hydrodynamical simulations: Hydrodynamical weak-lensing cluster mass biases and richnesses using different hydro models
• Universal conditional distribution function of [OII] luminosity of galaxies, and prediction for the [OII] luminosity function at redshift $z<3$
• Searching for [CII] Emission from the First Sample of $z\sim 6$ OI Absorption-Associated Galaxies with ALMA
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• Improving SDSS cosmological constraints through $\beta$-skeleton weighted correlation functions
• Compact groups of galaxies in GAMA -- Probing the densest minor systems at intermediate redshifts
• A probabilistic framework for cosmological inference of peculiar velocities
• Modelling the selection of galaxy groups with end to end simulations
• The THREEHUNDRED project: the effect of baryon processes at galaxy cluster scale
• Angular Correlation Function from sample covariance with BOSS and eBOSS LRG
• The Three Hundred Project: The stellar angular momentum evolution of cluster galaxies
• Universal multi-stream radial structures of cold dark matter halos
• A graph model for the clustering of dark matter halos
• The Assembly of the Virgo Cluster, Traced by its Galaxy Halos
• Turnaround density evolution encodes cosmology in simulations
• The impact of halo concentration on the Sunyaev Zel'dovich effect signal from massive galaxy clusters
• Prospects for studying the mass and gas in protoclusters with future CMB observations
• FLORAH: A generative model for halo assembly histories
• BASILISK II. Improved Constraints on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• The Three Hundred Project: deducing the stellar splashback structure of galaxy clusters from their orbiting profiles
• Observing Correlations Between Dark Matter Accretion and Galaxy Growth: II. Testing the Impact of Galaxy Mass, Star Formation Indicator, and Neighbour Colours
• Deep Chandra Observations of the z = 1.16 Relaxed, Cool-core Galaxy Cluster SPT-CL J2215-3537
• The mass and galaxy distribution around SZ-selected clusters
• Impact of Cosmic Variance on the Galaxy-Halo Connection for Lyman-$\alpha$ Emitters
• Assembly Conformity of Structure Growth: Fossil versus Normal Groups of Galaxies
• LATIS: Comparing Galaxy and IGM Tomography Maps as Tracers of Large-scale Structure and Protoclusters at $z\sim 2.5$
• Some Implications of the Leptonic Annihilation of Dark Matter: Possible Galactic Radio Emission Signatures and the Excess Radio Flux of Extragalactic Origin
• Splashback radius and the mass accretion rate of RASS MCMF galaxy clusters
• Cosmological gravity on all scales IV: 3x2pt Fisher forecasts for pixelised phenomenological modified gravity
• Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
• CLIMBER: Galaxy-Halo Connection Constraints from Next-Generation Surveys
• Improving Galaxy Cluster Selection with the Outskirt Stellar Mass of Galaxies
• Associations of dwarf galaxies in a $\Lambda$CDM Universe
• Stochastic Order Redshift Technique (SORT): a simple, efficient and robust method to improve cosmological redshift measurements
• Galaxy Correlation Function and Local Density from Photometric Redshifts Using the Stochastic Order Redshift Technique (SORT)
• Testing Models of Quasar Hosts With Strong Gravitational Lensing by Quasar Hosts
• The Correlation Function and Detection of Baryon Acoustic Oscillation Peak from the Spectroscopic SDSS GalWCat Galaxy Cluster Catalogue
• The connection between halo concentrations and assembly histories: a probe of gravity?
• The Three Hundred: The existence of massive dark matter-deficient satellite galaxies in cosmological simulations
• Measurement of the evolving galaxy luminosity and mass function using clustering-based redshift inference
• Hermeian haloes: extreme objects with two interactions in the past
• The Three Hundred: Gas Properties Outside of Galaxy Cluster with the WHIM Contribution and Detection
• Tomographic Alcock-Paczynski Method with Redshift Errors
• Detecting deviations from Gaussianity in high-redshift CMB lensing maps
• Extended Enriched Gas in a Multi-Galaxy Merger at Redshift 6.7
• The impact of baryons on the sparsity of simulated galaxy clusters from The Three Hundred Project
• Chameleon Screening Depends on the Shape and Structure of NFW Halos
• Self-Interacting Dark-Matter Spikes and the Final-Parsec Problem: Bayesian constraints from the NANOGrav 15-Year Gravitational-Wave Background
• Dynamical friction can flip the hierarchical three-body system
• The Three Hundred Project: dissecting the fundamental plane of galaxy clusters up to $z=1$
• Directional miscentering dependence in weak lensing mass bias
• Impact of filaments on galaxy cluster properties in The Three Hundred simulation
• Independent Measurements of the Dynamical Masses of Six Galaxy Clusters in the Local Universe
• Searching for Dark Matter Annihilation with IceCube and P-ONE
• A mock redshift catalogue of the dusty star-forming galaxy population with intrinsic clustering and lensing for deep millimetre surveys
• The evolution of the halo occupation distribution in cosmic voids
• Physical modelling of galaxy clusters and Bayesian inference in astrophysics
• The Influence of Subhaloes on Host Halo Properties
• A Generative Model for Realistic Galaxy Cluster X-ray Morphologies
• Spatial correlations of extended cosmological structures
• Void Formation: Does the Void-in-Cloud Process Matter?
• Assessing the connection between galactic conformity and assembly-type bias
• Using photometric redshift data to improve the detection of galactic filaments with the Bisous model
• One Galaxy Sample to Rule Them All: Halo Occupation Distribution Modeling of DES Year 3 Source Galaxies
• Deriving accurate galaxy cluster masses using X-ray thermodynamic profiles and graph neural networks
• Observed versus Simulated Halo c-Mvir Relations
• A Hydro-Particle-Mesh Code for Efficient and Rapid Simulations of the Intracluster Medium
• Strong Conformity and Assembly Bias: Towards a Physical Understanding of the Galaxy-Halo Connection in SDSS Clusters
• Cosmology behind the mask: Constraining the parameters of $\Lambda$CDM with the unmasked galaxy density field from VIPERS
• Galaxy Velocity Bias in Cosmological Simulations: Towards Percent-level Calibration
• Delensing CMB B-modes using galaxy surveys: the effect of galaxy bias and matter clustering non-linearities
• Inference of morphology and dynamical state of nearby $Planck$-SZ galaxy clusters with Zernike polynomials
• A Random Walk Model for Halo Triaxiality
• The mass profile of NGC 3377 from a Bayesian approach
• Success of Machine Learning algorithms in Dynamical Mass Measurements of Galaxy Clusters
• How the Coherent Tides Obstruct the Radial Infalls of Satellite Galaxies onto Clusters
• Dissecting the Thermal SZ Power Spectrum by Halo Mass and Redshift in SPT-SZ Data and Simulations
• Improving the accuracy of observable distributions for galaxies classified in the Projected Phase Space Diagram
• The Three Hundred : contrasting clusters galaxy density in hydrodynamical and dark matter simulations
• Cross-correlating the patchy screening and kinetic Sunyaev-Zel'dovich effects as a new probe of reionization
• Baryon Acoustic Oscillations from galaxy surveys
• Constraining Galaxy-Halo Connection Using Machine Learning
• Spherical bias on the 3D reconstruction of the ICM density profile in galaxy clusters
• The Three Hundred Project: A fast semi-analytic model emulator of hydrodynamical galaxy cluster simulations
• LATIS Data Release: $\sim 4200$ Spectra of $z\sim 2-3$ Galaxies, Redshifts, and Intergalactic Medium Tomography Maps
• Cosmological constraints from the density gradient weighted correlation function
• Generating Galaxy Clusters Mass Density Maps from Mock Multiview Images via Deep Learning
• CHEX-MATE: Morphological analysis of the sample
• Dark Matter Energy Deposition and Production from the Table-Top to the Cosmos
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• Measurements of cosmic expansion and growth rate of structure from voids in the Sloan Digital Sky Survey between redshift 0.07 and 1.0
• New leaves of the tree: percolation analysis for cosmic web with discrete points
• Dynamical Properties and Velocity Dispersion-Mass Relation of $z\sim 1$ Galaxy Clusters from the GOGREEN and GCLASS Surveys
• NeutralUniverseMachine: Predictions of HI gas in Different Theoretical Models
• The hydrostatic mass bias in The Three Hundred clusters
• Deep Learning generated observations of galaxy clusters from dark-matter-only simulations
• From the Densest Clusters to the Emptiest Voids: No Evidence For Environmental Effects on the Galaxy Size-Mass Relation at Low Redshift
• Multi-scale weak lensing detection of galaxy clusters with source redshift tomography
• Capability for detection of GW190521-like binary black holes with TianQin
• Timing the last major merger of galaxy clusters with large halo sparsity
• The origin of the intra-cluster light in The Three Hundred simulations
• The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics
• Extragalactic Searches for Dark Matter Annihilation
• Sahyadri: A simulation suite for the cosmology dependence of the Cosmic Web
• Properties of the Intracluster Medium Assuming an Einasto Dark Matter Profile
• 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?
• A preliminary study about gravitational wave radiation and cosmic heat death
• Universal Fitting Formulae for the Peak Concentration of Dark Matter Halos
• Using Unreal Engine to Visualize a Cosmological Volume
• Black Hole-Galaxy Correlations in Cluster Zoomed-in Simulations: GIZMO-SIMBA and TNG-Cluster
• Dynamical Models of the Milky Way in Action Space with LAMOST DR8 and GAIA EDR3
• Hybrid $P_{\ell }(k)$: general, unified, non-linear matter power spectrum in redshift space
• A Non-parametric Method for the Inference of Halo Occupation Distributions
• Tomographic Alcock-Paczynski Test with Marked Correlation Functions
• Dissecting the strong lensing galaxy cluster MS 0440$+$0204 II. New optical spectroscopic observations in a wider area and cluster dynamical state
• Predicting Halo Formation Time Using Machine Learning
• Testing the key role of the stellar mass-halo mass relation in galaxy merger rates and morphologies via DECODE, a novel Discrete statistical sEmi-empiriCal mODEl