Dark matter halo concentrations in the Wilkinson Microwave Anisotropy Probe year 5 cosmology

Abstract

We use a combination of three large N-body simulations to investigate the dependence of dark matter halo concentrations on halo mass and redshift in the WMAP year 5 cosmology. The median relation between concentration and mass is adequately described by a power-law for halo masses in the range 10^11 - 10^15 Msol/h and redshifts z < 2, regardless of whether the halo density profiles are fit using NFW or Einasto profiles. Compared with recent analyses of the Millennium Simulation, which uses a value of sigma_8 that is higher than allowed by WMAP5, z = 0 halo concentrations are reduced by factors ranging from 23 per cent at 10^11 Msol/h to 16 per cent at 10^14 Msol/h. The predicted concentrations are much lower than inferred from X-ray observations of groups and clusters.

6 pages, 4 figures, Accepted by MNRAS letters. Version 4: Typo fixed

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• gamma-rays from annihilating dark matter in galaxy clusters: stacking vs single source analysis
• Using galaxy-galaxy weak lensing measurements to correct the Finger-of-God
• Resolving the hydrostatic mass profiles of galaxy clusters at z~1 with XMM-Newton and Chandra
• Dependence of GAMA galaxy halo masses on the cosmic web environment from 100 square degrees of KiDS weak lensing data
• Stellar mass-gap as a probe of halo assembly history and concentration: youth hidden among old fossils
• The modified gravity lightcone simulation project I: Statistics of matter and halo distributions
• IDCS J1426.5+3508: The Most Massive Galaxy Cluster at $z>1.5$
• The galaxy cluster outskirts probed by Chandra
• Measuring subhalo mass in redMaPPer clusters with CFHT Stripe 82 Survey
• The galaxy-subhalo connection in low-redshift galaxy clusters from weak gravitational lensing
• Spherical collapse, formation hysteresis and the deeply non-linear cosmological power spectrum
• Initial Conditions for Idealised Clusters Mergers, simulating El Gordo
• KiDS-Legacy calibration: unifying shear and redshift calibration with the SKiLLS multi-band image simulations
• The Mass-Concentration Relation and the Stellar-to-Halo Mass Ratio in the CFHT Stripe 82 Survey
• Strong orientation dependence of surface mass density profiles of dark haloes at large scales
• Head-to-Toe Measurement of El Gordo: Improved Analysis of the Galaxy Cluster ACT-CL J0102-4915 with New Wide-field Hubble Space Telescope Imaging Data
• Foreground Biases on Primordial Non-Gaussianity Measurements from the CMB Temperature Bispectrum: Implications for Planck and Beyond
• The halo mass function in interacting Dark Energy models
• Controlling and leveraging small-scale information in tomographic galaxy-galaxy lensing
• Accretion of Galaxy Groups into Galaxy Clusters
• Mass Calibration of Optically Selected DES clusters using a Measurement of CMB-Cluster Lensing with SPTpol Data
• Halo Concentration, Galaxy Red Fraction, and Gas Properties of Optically-defined Merging Clusters
• Combining perturbation theories with halo models for the matter bispectrum
• Deconstructing Thermal Sunyaev-Zel'dovich - Gravitational Lensing Cross-Correlations: Implications for the Intracluster Medium
• A weak gravitational lensing recalibration of the scaling relations linking the gas properties of dark halos to their mass
• Galaxy Populations in the 26 most massive Galaxy Clusters in the South Pole Telescope SZE Survey
• On the over-concentration problem of strong lensing clusters
• MC^2: Mapping the Dark Matter Distribution of the "Toothbrush" Cluster RX J0603.3+4214 with Hubble Space Telescope and Subaru Weak-lensing
• Modelling mass distribution in elliptical galaxies: mass profiles and their correlation with velocity dispersion profiles
• The MUSE Extremely Deep Field: Evidence for SFR-induced cores in dark-matter dominated galaxies at z=1
• Connecting the structure of dark matter haloes to the primordial power spectrum
• Weak Lensing Observables in the Halo Model
• Intensity mapping cross-correlations II: HI halo models including shot noise
• Can giant radio halos probe the merging rate of galaxy clusters?
• The 6dF Galaxy Survey: Dependence of halo occupation on stellar mass
• The effects of baryonic cooling on the concentration-mass relation
• Precision Tests of CO and [CII] Power Spectra Models against Simulated Intensity Maps
• Detection of Enhancement in Number Densities of Background Galaxies due to Magnification by Massive Galaxy Clusters
• Phase-space structure of protohalos: Vlasov versus Particle-Mesh
• Relativistic SZ temperature scaling relations of groups and clusters derived from the BAHAMAS and MACSIS simulations
• Quantifying the Line-of-Sight Halo Contribution to the Dark Matter Convergence Power Spectrum from Strong Gravitational Lenses
• Simulating the galaxy cluster "El Gordo" and identifying the merger configuration
• Sensitivity of strong lensing observations to dark matter substructure: a case study with Euclid
• Comparing Dense Galaxy Cluster Redshift Surveys with Weak Lensing Maps
• Decaying dark matter: a stacking analysis of galaxy clusters to improve on current limits
• Self-calibration of weak lensing systematic effects using combined two- and three-point statistics
• MC${}^2$: Dynamical Analysis of the Merging Galaxy Cluster MACS J1149.5+2223
• The HI Velocity Function: a test of cosmology or baryon physics?
• Optical Confirmation and Redshift Estimation of the Planck Cluster Candidates overlapping the Pan-STARRS Survey
• Cosmic radiation backgrounds from primordial black holes
• Galaxy Kinematics and Mass Calibration in Massive SZE Selected Galaxy Clusters to z=1.3
• Projected-Field Kinetic Sunyaev-Zel'dovich Cross-Correlations: Halo Model and Forecasts
• Physical properties of simulated galaxy populations at z=2 - II. Effects of cosmology, reionization and ISM physics
• How Baryonic Processes affect Strong Lensing properties of Simulated Galaxy Clusters
• CODEX Weak Lensing: Concentration of Galaxy Clusters at z ~ 0.5
• Stellar-to-halo mass relation of cluster galaxies
• Gravitational lensing and dynamics in SL2S\,J02140-0535: Probing the mass out to large radius
• A general framework to test gravity using galaxy clusters II: A universal model for the halo concentration in $f(R)$ gravity
• Weak Lensing Analysis of SPT selected Galaxy Clusters using Dark Energy Survey Science Verification Data
• Investigating Cluster Astrophysics and Cosmology with Cross-Correlation of the Thermal Sunyaev-Zel'dovich Effect and Weak Lensing
• The physical drivers of the atomic hydrogen-halo mass relation
• Constraints on the Mass, Concentration, and Nonthermal Pressure Support of Six CLASH Clusters from a Joint Analysis of X-ray, SZ, and Lensing Data
• Mass functions and bias of dark matter halos
• Statistical uncertainties and systematic errors in weak lensing mass estimates of galaxy clusters
• Re-ionizing the Universe without Stars
• CLUMP-3D: Three-dimensional Shape and Structure of 20 CLASH Galaxy Clusters from Combined Weak and Strong Lensing
• AMICO galaxy clusters in KiDS-DR3: cosmological constraints from large-scale stacked weak lensing profiles
• The Discovery of a Gravitationally Lensed Supernova Ia at Redshift 2.22
• The mass-concentration relationship of virialized halos and its impact on cosmological observables
• Evidence for inhomogeneous reionization in the local Universe from metal-poor globular cluster systems
• The polytropic approximation and X-ray scaling relations: constraints on gas and dark matter profiles for galaxy groups and clusters
• The Origin of Extended Disk Galaxies at z=2
• Dark-ages Reionization & Galaxy Formation Simulation II: Spin and concentration parameters for dark matter haloes during the Epoch of Reionization
• The Massive and Distant Clusters of WISE Survey: MOO J1142+1527, A 10${}^{15}$ M${}_{\odot }$ Galaxy Cluster at z=1.19
• Fast Weak Lensing Simulations with Halo Model
• The mass function dependence on the dynamical state of dark matter haloes
• Offsets between the X-ray and the Sunyaev-Zel'dovich-effect peaks in merging galaxy clusters and their cosmological implications
• Globular Cluster Formation from Colliding Substructure
• GAMA+KiDS: Empirical correlations between halo mass and other galaxy properties near the knee of the stellar-to-halo mass relation
• On the orbital and internal evolution of cluster galaxies
• Exemplary Merging Clusters: Weak-lensing and X-ray Analysis of the Double Radio Relic Merging Galaxy Clusters MACS 1752.0+4440 and ZWCL 1856.8+6616
• SARCS strong-lensing galaxy groups: II - mass-concentration relation and strong-lensing bias
• The Influence of Concentration and Dynamical State on Scatter in the Galaxy Cluster Mass-Temperature Relation
• Rotation Curves of Galaxies and Their Dependence on Morphology and Stellar Mass
• $\text{matryoshka}$: Halo Model Emulator for the Galaxy Power Spectrum
• Vector disformal transformation of generalized Proca theory
• Weak lensing and spectroscopic analysis of the nearby dissociative merging galaxy cluster Abell 3376
• Constraining the halo mass function with observations
• CFHTLenS: Weak lensing constraints on the ellipticity of galaxy-scale matter haloes and the galaxy-halo misalignment
• Weak-lensing-inferred scaling relations of galaxy clusters in the RCS2: mass-richness, mass-concentration, mass-bias, and more
• AMS-02 Positrons from Decaying Wino in the Pure Gravity Mediation Model
• Non-universality of halo profiles and implications for dark matter experiments
• The Effects of Varying Cosmological Parameters on Halo Substructure
• Spurious Small-Scale Structure & Discreteness-Driven Relaxation in Cosmological Simulations
• A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups
• A Consistent Approach to Falsifying Lambda-CDM with Rare Galaxy Clusters
• A multi-wavelength strong lensing analysis of baryons and dark matter in the dynamically active cluster AC 114
• Star-formation driven outflows in local dwarf galaxies as revealed from [CII] observations by Herschel
• Mapping Compound Cosmic Telescopes Containing Multiple, Projected Cluster-Scale Halos
• Breaking the Vainshtein screening in clusters of galaxies
• Are group- and cluster-scale dark matter halos over-concentrated?
• One Thousand and One Clusters: Measuring the Bulk Flow with the Planck ESZ and X-Ray Selected Galaxy Cluster Catalogs
• Optimizing weak lensing mass estimates for cluster profile uncertainty
• The Effect of Large-Scale Structure on the Magnification of High-Redshift Sources by Cluster-Lenses
• Mass-concentration relation of clusters of galaxies from CFHTLenS
• A Very Large (${\theta }_E\gtrsim 40$") Strong Gravitational Lens Selected with the Sunyaev-Zel'dovich Effect: PLCK G287.0+32.9 ($z$ = 0.38)
• Impact of Systematics on SZ-Optical Scaling Relations
• The GOGREEN survey: the internal dynamics of clusters of galaxies at redshift 0.9-1.4
• Subaru weak-lensing measurement of a z = 0.81 cluster discovered by the Atacama Cosmology Telescope Survey
• The Galaxy Cross-Correlation Function as a Probe of the Spatial Distribution of Galactic Satellites
• Measuring the hydrostatic mass bias in galaxy clusters by combining Sunyaev-Zel'dovich and CMB lensing data
• What to expect from dynamical modelling of cluster haloes II. Investigating dynamical state indicators with Random Forest
• Detection of universality of dark matter profile from Subaru weak lensing measurements of 50 massive clusters
• Spectroscopic Confirmation of Five Galaxy Clusters at z > 1.25 in the 2500 sq. deg. SPT-SZ Survey
• The Sloan Bright Arcs Survey: Ten Strong Gravitational Lensing Clusters and Evidence of Overconcentration
• Weak-lensing calibration of a stellar mass-based mass proxy for redMaPPer and Voronoi Tessellation clusters in SDSS Stripe 82
• Magnification of Photometric LRGs by Foreground LRGs and Clusters in SDSS
• First Identification of a CMB Lensing Signal Produced by $1.5$ Million Galaxies at $z\sim$4: Constraints on Matter Density Fluctuations at High Redshift
• Optical & Sunyaev-Zel'dovich Observations of a New Sample of Distant Rich Galaxy Clusters in the ROSAT All Sky Survey
• Weak-lensing mass bias in merging galaxy clusters
• Stability Analysis for Cosmic-Ray Heating of Cool Cores in Galaxy Clusters
• Weak Lensing Analysis of CODEX Clusters using Dark Energy Camera Legacy Survey : Mass-Richness Relation
• Cosmology and Astrophysics from Relaxed Galaxy Clusters V: Consistency with Cold Dark Matter Structure Formation
• Effects of Velocity-Dependent Dark Matter Annihilation on the Energy Spectrum of the Extragalactic Gamma-ray Background
• Large-scale Structure and Dynamics of the Most X-ray Luminous Galaxy Cluster Known -- RX J1347-1145
• Illuminating Dark Matter Halo Density Profiles Without Subhaloes
• Alone on a wide wide sea. The origin of SECCO 1, an isolated star-forming gas cloud in the Virgo cluster
• A general framework to test gravity using galaxy clusters IV: Cluster and halo properties in DGP gravity
• Systematic errors in strong gravitational lensing reconstructions, a numerical simulation perspective
• The Dark Matter Haloes of Chandra X-ray Galaxy Clusters and Baryons Effect
• Galaxy-Mass Correlations on 10 Mpc Scales in the Deep Lens Survey
• Cosmological Constraints from Galaxy Cluster Sparsity, Cluster Gas Mass Fraction and Baryon Acoustic Oscillations Data
• Weak lensing mass modeling bias and the impact of miscentring
• Connection between a possible fifth force and the direct detection of Dark Matter
• New insights on the dissociative merging galaxy cluster Abell 2034
• Major mergers between dark matter haloes -- II. Profile and concentration changes
• The Atacama Cosmology Telescope: the stellar content of galaxy clusters selected using the Sunyaev-Zel'dovich effect
• Known Unknowns of Dark Matter Annihilation over Cosmic Time
• Velocity reconstruction with the cosmic microwave background and galaxy surveys
• CMB lensing reconstruction biases from masking extragalactic sources
• Velocity dispersion and dynamical mass for 270 galaxy clusters in the Planck PSZ1 catalogue
• Evolution of the luminosity-to-halo mass relation of LRGs from a combined SDSS-DR10+RCS2 analysis
• The Dynamical Origin of Early-Type Dwarfs in Galaxy Clusters: A Theoretical Investigation
• Weak lensing clusters from HSC survey first-year data: Mitigating the dilution effect of foreground and cluster member galaxies
• Multi-Phenomena Modeling of the New Bullet Cluster, ZwCl008.8+52, using N-body/hydrodynamical Simulations
• First Weak-lensing Results from "See Change": Quantifying Dark Matter in the Two Z>1.5 High-redshift Galaxy Clusters SPT-CL J2040-4451 and IDCS J1426+3508
• Simulations of the Galaxy Cluster CIZA J2242.8+5301 I: Thermal Model and Shock Properties
• Chemical evolution of giant molecular clouds in simulations of galaxies
• Multi-wavelength scaling relations in galaxy groups: a detailed comparison of GAMA and KiDS observations to BAHAMAS simulations
• Exploring extensions to the standard cosmological model and the impact of baryons on small scales
• Halo collapse: virialization by shear and rotation in dynamical dark-energy models. Effects on weak-lensing peaks
• The Evolution of K* and the Halo Occupation Distribution since z=1.5: Observations vs. Simulations
• The serendipitous observation of a gravitationally lensed galaxy at z = 0.9057 from the Blanco Cosmology Survey: The Elliot Arc
• Radio Relics Tracing the Projected Mass Distribution in CIZA J2242.8+5301
• Cosmological Studies from HSC-SSP Tomographic Weak Lensing Peak Abundances
• Joint Analysis of Galaxy-Galaxy Lensing and Galaxy Clustering: Methodology and Forecasts for DES
• AMICO galaxy clusters in KiDS-DR3: Measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis
• Detecting low-mass haloes with strong gravitational lensing II: constraints on the density profiles of two detected subhaloes
• Imprints of gravitational lensing in the Planck CMB data at the location of WISExSCOS galaxies
• Future constraints on the gravitational slip with the mass profiles of galaxy clusters
• KiDS+GAMA: The weak lensing calibrated stellar-to-halo mass relation of central and satellite galaxies
• A Multi-Wavelength Mass Analysis of RCS2 J232727.6-020437, a ~3x10${}^{15}$M${}_{\odot }$ Galaxy Cluster at z=0.7
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• The clustering of baryonic matter. I: a halo-model approach
• Subhaloes gone Notts: the clustering properties of subhaloes
• Multiwavelength Analysis of A1240, the Double Radio Relic Merging Galaxy Cluster Embedded in a ~80 Mpc-long Cosmic Filament
• The BAHAMAS project: Effects of dynamical dark energy on large-scale structure
• Improving models of the cosmic infrared background using CMB lensing mass maps
• Simulations of the merging galaxy cluster Abell 2034: what determines the level of separation between gas and dark matter
• Hierarchical inference of the relationship between Concentration and Mass in Galaxy Groups and Clusters
• On the change of old neutron star masses with galactocentric distance
• On Mass Concentrations & Magnitude Gaps of Galaxy Systems in the CS82 Survey
• The Mass-Richness Relation of MaxBCG Clusters from Quasar Lensing Magnification using Variability
• eROSITA clusters dynamical state and their impact on the BCG luminosity
• Velocity dispersion and dynamical masses for 388 Galaxy Clusters and groups. Calibrating the $M_{\mathrm{SZ}}$--$M_{\mathrm{dyn}}$ scaling relation for the PSZ2 sample
• Effects of center offset and noise on weak-lensing derived concentration-mass relation of dark matter halos
• An Accurate Analytic Model for the Thermal Sunyaev-Zel'dovich One-Point PDF
• Constraining the Mass of the Emerging Galaxy Cluster SpARCS1049+56 at z=1.71 with Infrared Weak Lensing
• The X-ray Properties of Weak Lensing Selected Galaxy Clusters
• DS+: a method for the identification of cluster substructures
• Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-$y$-maps from SPT and Planck
• Weak lensing magnification of SpARCS galaxy clusters
• Analytic marginalization of $N(z)$ uncertainties in tomographic galaxy surveys
• Accuracy of analytical models of the large-scale matter distribution
• The SRG-eROSITA All-Sky Survey : Constraints on f(R) Gravity from Cluster Abundance
• An Inpainting Approach to Tackle the Kinematic and Thermal SZ Induced Biases in CMB-Cluster Lensing Estimators
• A combined X-ray, optical and radio view of the merging galaxy cluster MACS J0417.5-1154
• Analytical shear and flexion of Einasto dark matter haloes
• Cosmology from weak lensing, galaxy clustering, CMB lensing and tSZ: I. 10x2pt Modelling Methodology
• Patchy Screening of the CMB from Dark Photons
• Probing Theories of Gravity with Phase Space-Inferred Potentials of Galaxy Clusters
• The BAHAMAS project: Effects of a running scalar spectral index on large-scale structure
• Teaching neural networks to generate Fast Sunyaev Zel'dovich Maps
• The stellar mass function and evolution of the density profile of galaxy clusters from the Hydrangea simulations at $0<z<1.5$
• Angular clustering and host halo properties of [OII] emitters at $z>1$ in the Subaru HSC survey
• The Kinematic Sunyaev-Zel'dovich Effect with ACT, DES, and BOSS: a Novel Hybrid Estimator
• CODEX Weak Lensing Mass Catalogue and implications on the mass-richness relation
• Revising the merger scenario of the galaxy cluster Abell 1644: a new gas poor structure discovered by weak gravitational lensing
• HOD modelling of high redshift galaxies using the BLUETIDES simulation
• The effects of local stellar radiation and dust depletion on non-equilibrium interstellar chemistry
• A giant radio halo in a low-mass SZ-selected galaxy cluster: ACT-CL J0256.5+0006
• SALT spectroscopic observations of galaxy clusters detected by ACT and a Type II quasar hosted by a brightest cluster galaxy
• Constraining the Milky Way Dark Matter Density Profile with Gamma-Rays with Fermi-LAT
• Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters
• The Correspondence between Convergence Peaks from Weak Lensing and Massive Dark Matter Haloes
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• JWST's first glimpse of a z > 2 forming cluster reveals a top-heavy stellar mass function
• Galaxy Tagging: photometric redshift refinement and group richness enhancement
• The XXL Survey: XXII. The XXL-North spectrophotometric sample and galaxy stellar mass function in X-ray detected groups and clusters
• Cross Correlation between the Thermal Sunyaev-Zel'dovich Effect and Projected Galaxy Density Field
• Ram pressure stripping: An analytical approach
• Internal Cluster Structure
• Properties and observables of massive galaxies in self-interacting dark matter cosmologies
• A New Interpretation of the Mass-Temperature Relation and Mass Calibration of Galaxy Clusters Based on the Fundamental Plane
• Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
• Mass and pressure constraints on galaxy clusters from interferometric SZ observations
• The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0<z<7
• Unveiling the internal structure of Hercules supercluster
• The effects of primordial non-Gaussianity on giant-arc statistics
• Submillimetre Source Counts in the Fields of High-Redshift Galaxy Clusters
• Future sensitivity of neutrino telescopes to dark matter annihilations from the cosmic diffuse neutrino signal
• The halo model with beyond-linear halo bias: unbiasing cosmological constraints from galaxy-galaxy lensing and clustering
• Shapley Supercluster Survey: mapping the dark matter distribution
• Precise Mass Determination of SPT-CL J2106-5844, the Most Massive Cluster at z>1
• A million-solar-mass object detected at cosmological distance using gravitational imaging
• Measuring the surface mass density ellipticity of redMaPPer galaxy clusters using weak-lensing
• Revised Mass-to-Light Ratios For Nearby Galaxy Groups and Clusters
• Assembly Bias of Dwarf-sized Dark Matter Haloes
• Galaxy-Galaxy Lensing in EAGLE: comparison with data from 180 square degrees of the KiDS and GAMA surveys
• Toward Solving the Puzzle: Dissecting the Complex Merger A521 with Multi-wavelength Data
• Measuring Lensing Magnification of Quasars by Large Scale Structure using the Variability-Luminosity Relation
• Cluster-Cluster Lensing and the Case of Abell 383
• Project Dinos II: Redshift evolution of dark and luminous matter density profiles in strong-lensing elliptical galaxies across 0.1 < z < 0.9
• Enhanced n-body annihilation of dark matter and its indirect signatures
• Detectability of Weak Lensing Modifications under Galileon Theories
• Vector Dark Matter Detection using the Quantum Jump of Atoms
• MC^2: A deeper look at ZwCl 2341.1+0000 with Bayesian galaxy clustering and weak lensing analyses
• On the absence of backsplash analogues to NGC 3109 in the $\Lambda$CDM framework
• IDCS J1426.5+3508: Weak Lensing Analysis of a Massive Galaxy Cluster at $z=1.75$
• An Optical Observational Cluster Mass Function at $z\sim 1$ with the ORELSE Survey
• Tidal stripping as a test of satellite quenching in redMaPPer clusters
• Close galaxy pairs with accurate photometric redshifts
• Dark Energy Survey Year 1 Results: The effect of intracluster light on photometric redshifts for weak gravitational lensing
• Disentangling cosmic-ray and dark-matter induced gamma-rays in galaxy clusters?
• Constraining Halo Occupation Distribution and Cosmic Growth Rate using Multipole Power Spectrum
• Projection effects of large-scale structures on weak-lensing peak abundances
• Accurate Model of the Projected Velocity Distribution of Galaxies in Dark Matter Halos
• Non-steady heating of cool cores of galaxy clusters by ubiquitous turbulence and AGN
• Shedding Light on the Matter of Abell 781
• KiDS+VIKING-450: An internal-consistency test for cosmic shear tomography with a colour-based split of source galaxies
• The first shear measurements from precision weak lensing
• Joint cosmology and mass calibration from tSZ cluster counts and cosmic shear
• Probing the cluster pressure profile with thermal Sunyaev-Zeldovich effect and weak lensing cross-correlation
• The Atacama Cosmology Telescope: The LABOCA/ACT Survey of Clusters at All Redshifts
• Weak lensing mass estimates of galaxy groups and the line-of-sight contamination
• Cosmology with Galaxy Clusters: Systematic Effects in the Halo Mass Function
• Dynamical masses and non-homology of massive elliptical galaxies grown by dry mergers
• The BAHAMAS project: Evaluating the accuracy of the halo model in predicting the non-linear matter power spectrum
• Sunyaev-Zel'dovich Signal from Quasar Hosts: Implications for Detection of Quasar Feedback
• KiDS-1000: Weak lensing and intrinsic alignment around luminous red galaxies
• Probing cosmology with weak lensing selected clusters II: Dark energy and f(R) gravity models
• Contribution of Radio Halos to the Foreground for SKA EoR Experiments
• Dark Matter Annihilation in the Circumgalactic Medium at High Redshifts
• Halo Mass-Concentration Relation at High-Mass End
• On the weak lensing masses of a new sample of galaxy groups
• The quasar-galaxy cross SDSS J1320+1644: A probable large-separation lensed quasar
• A weak lensing analysis of the PLCK G100.2-30.4 cluster
• Subtracting the kinetic Sunyaev-Zeldovich effect from the cosmic microwave background with surveys of large-scale structure
• 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
• Average Dark Matter Halo Sparsity Relations as Consistency Check of Mass Estimates in Galaxy Cluster Samples
• Got plenty of nothing: cosmic voids as a probe of particle dark matter
• The thermal and gravitational energy densities in the large-scale structure of the Universe
• Probing Saraswati's heart: evaluating the dynamical state of the massive galaxy cluster A2631 through a comprehensive weak-lensing and dynamical analysis
• Halo Concentrations and the New Baseline X-ray Luminosity-Temperature and Mass Relations of Galaxy Clusters
• Tightening weak lensing constraints on the ellipticity of galaxy-scale dark matter haloes
• The Epoch of Assembly of Two Galaxy Groups: A comparative study
• Constraints on dark matter and astrophysics from tomographic $\gamma$-ray cross-correlations
• Lensing dispersion of supernova flux: a probe of nonlinear structure growth
• How well do third-order aperture mass statistics separate E- and B-modes?
• Testing General Relativity: new measurements of gravitational redshift in galaxy clusters
• Constraining the Milky Way Mass with Its Hot Gaseous Halo
• Beyond Ultra-diffuse Galaxies. II. Environmental Quenching of Mass-Size Outliers among the Satellites of Milky Way Analogs
• KiDS-Legacy: Covariance validation and the unified OneCovariance framework for projected large-scale structure observables
• A possible challenge for Cold and Warm Dark Matter
• Testing emergent gravity with mass densities of galaxy clusters
• Compact Groups analysis using weak gravitational lensing II: CFHT Stripe 82 data
• Suzaku X-ray Follow-up Observation of Weak-lensing-detected Halos in the Field around ZwCl0823.2+0425
• Simulations of the merging cluster of galaxies Cygnus A
• Cluster-lensing: A Python Package for Galaxy Clusters & Miscentering
• Combining Strong Lensing and Dynamics in Galaxy Clusters: integrating MAMPOSSt within LENSTOOL I. Application on SL2S J02140-0535
• Quantifying and controlling biases in dark matter halo concentration estimates
• On Escaping a Galaxy Cluster in an Accelerating Universe
• Rotation curves of galaxies and the stellar mass-to-light ratio
• Probing Cosmology and Galaxy Cluster Structure with the Sunyaev-Zel'dovich Decrement vs. X-ray Temperature Scaling Relation
• The Stellar Mass - Halo Mass Relation for Low Mass X-ray Groups at 0.5<z<1 in the CDFS with CSI
• The integrated angular bispectrum
• Non-linear power spectra of dark and luminous matter in halo model of structure formation
• Low Surface Brightness Galaxies in z > 1 Galaxy Clusters: HST approaches the Progenitors of Local Ultra Diffuse Galaxies
• A Gemini view of the galaxy cluster RXC J1504-0248: insights on the nature of the central gaseous filaments
• The abundance of satellite galaxies in the inner region of $\Lambda$CDM Milky Way sized haloes
• Statistics of the Sunyaev-Zel'dovich Effect power spectrum
• A general framework to test gravity using galaxy clusters V: A self-consistent pipeline for unbiased constraints of $f(R)$ gravity
• Constraining the mass-concentration relation through weak lensing peak function
• An excursion into the core of the cluster lens Abell 1689
• Galaxy And Mass Assembly (GAMA): Gas Fuelling of Spiral Galaxies in the Local Universe II. -- Direct Measurement of the Dependencies on Redshift and Host Halo Mass of Stellar Mass Growth in Central Disk Galaxies
• Mass Calibration of Galaxy Clusters at Redshift 0.1-1.0 using Weak Lensing in the Sloan Digital Sky Survey Stripe 82 Co-add
• Accurate Analytic Mass-Scale Relations for Dark Matter Haloes of all Masses and Redshifts
• Simulating nearly edge-on sloshing in the galaxy cluster Abell 2199
• CLMM: a LSST-DESC Cluster weak Lensing Mass Modeling library for cosmology
• Self-Interacting Dark Matter Scattering Rates Through Cosmic Time
• Gas accretion and Ram Pressure Stripping of Haloes in Void Walls
• Halo shapes constrained from a pure sample of central galaxies in KiDS-1000
• Concentrating the Dark Matter in Galaxy Clusters through Tidal Stripping of Baryonically-Compressed Galactic Halos
• A Universal Power-law Profile of Pseudo-Phase-Space Density-like Quantities in Elliptical Galaxies
• Studying galaxy cluster morphological metrics with Mock-X
• Core Mass Estimates in Strong Lensing Galaxy Clusters Using a Single-Halo Lens Model
• The importance of the cosmic web and halo substructure for power spectra
• A major galaxy cluster merger caught by eROSITA: weak lensing mass distribution and kinematic description
• NGC 4104: a shell galaxy in a forming fossil group
• An efficient and robust method to estimate halo concentration
• Testing the Large-Scale Environments of Cool-core and Noncool-core Clusters with Clustering Bias
• Weak lensing analysis of galaxy pairs using CS82 data
• Infall Profiles for Supercluster-Scale Filaments
• On the Cooling Flow Problem in the Gaseous Halo of the Milky Way
• Inner structure of dark matter halos at high $z$ in cosmological models with non-power-law primordial spectra
• Shape noise and dispersion in precision weak lensing
• Cluster profiles from beyond-the-QE CMB lensing mass maps
• An expanded merger-tree description of cluster evolution
• The shape of dark matter haloes: results from weak lensing in the Ultraviolet Near-Infrared Optical Northern Survey (UNIONS)
• Importance of intracluster scattering and relativistic corrections from tSZ effect with Cosmic Infrared Background
• Searching for velocity-dependent dark matter annihilation signals from extragalactic halos
• Cosmic star formation history with tomographic cosmic infrared background-galaxy cross-correlation
• Strong Lensing In The Inner Halo Of Galaxy Clusters
• Machine Learning Etudes in Astrophysics: Selection Functions for Mock Cluster Catalogs
• The X-Ray Zurich Environmental Study (X-ZENS). II. X-ray Observations of the Diffuse Intragroup Medium in Galaxy Groups
• SHARP -- IX. The dense, low-mass perturbers in B1938+666 and J0946+1006: implications for cold and self-interacting dark matter
• Testing the Reliability of Fast Methods for Weak Lensing Simulations: WL-MOKA on PINOCCHIO
• Cross-correlation between soft X-rays and galaxies A new benchmark for galaxy evolution models
• The case for two-dimensional galaxy-galaxy lensing
• Sub-MeV Bosonic Dark Matter, Misalignment Mechanism and Galactic Dark Matter Halo Luminosities
• Cosmology and Astrophysics with the Diffuse eRASS1 X-ray Angular Power Spectrum
• Mass - concentration relation and weak lensing peak counts
• Weak lensing magnification of Type Ia Supernovae from the Pantheon sample
• Intrinsic mass-richness relation of clusters from THE THREE HUNDRED hydrodynamic simulations
• Weak gravitational lensing as a probe of physical properties of substructures in dark matter halos
• Clash of Titans: The Impact of Cluster Mergers in the Galaxy Cluster Red Sequence
• AMICO galaxy clusters in KiDS-1000: cosmological constraints and mass calibration from counts and weak lensing
• A Semi-Analytical Model for the Formation and Evolution of Radio Relics in Galaxy Clusters
• Testing the weak equivalence principle with the binary neutron star merger GW170817: the gravitational contribution of the host galaxy
• TDCOSMO. XXIII. Measurement of the Hubble constant from the doubly lensed quasar HE1104-1805
• Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties
• XMM-Newton X-ray and HST weak gravitational lensing study of the extremely X-ray luminous galaxy cluster ClJ120958.9+495352 ($z=0.902$)
• Primordial black holes as dark matter candidates: Multi-frequency constraints from cosmic radiation backgrounds
• Halo Concentrations and the Fundamental Plane of Galaxy Clusters
• Constraints on the Neutrino Mass from SZ Surveys
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Heating of the intracluster medium by buoyant bubbles and sound waves
• Improving lensing cluster mass estimate with flexion
• Proca-stinated Cosmology II: Matter, Halo, and Lensing Statistics in the vector Galileon
• Constraining cosmology with thermal Sunyaev-Zel'dovich maps: Minkowski functionals, peaks, minima, and moments
• The Wendelstein Weak Lensing (WWL) pathfinder: Accurate weak lensing masses for Planck clusters
• X-ray Temperatures, Luminosities, and Masses From XMM-Newton Follow-up of the First Shear-selected Galaxy Cluster Sample
• Deciphering Baryonic Feedback from ACT tSZ Galaxy Clusters
• The impact of halo concentration on the Sunyaev Zel'dovich effect signal from massive galaxy clusters
• Weak lensing peak statistics -- steepness versus height
• Searching for strong lensing by late-type galaxies in UNIONS
• Unveiling the shape: a multi-wavelength analysis of the galaxy clusters Abell 76 and Abell 1307
• The Dependence of Dark Matter Halo Properties on the Morphology of Their Central Galaxies from Weak Lensing
• Effect of lensing magnification on type Ia supernova cosmology
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• The connection between halo concentrations and assembly histories: a probe of gravity?
• The Assembly of the Virgo Cluster, Traced by its Galaxy Halos
• Cosmological parameters from lenses distance ratio
• The dynamical state of RXCJ1230.7+3439: a multi-substructured merging galaxy cluster
• Extreme AGN feedback in the fossil galaxy group SDSSTG 4436
• Inferring Host Dark Matter Halo Masses of Individual Galaxies from Neighboring Galaxy Counts
• Disentangling the Halo: Joint Model for Measurements of the Kinetic Sunyaev-Zeldovich Effect and Galaxy-Galaxy Lensing
• Gravitational and distributed heating effects of a cD galaxy on the hydrodynamical structure of its host cluster
• Two analytic relations connecting the hot gas astrophysics with the cold dark matter model for galaxy clusters
• Evolution of the degree of substructures in simulated galaxy clusters
• SZ power spectrum and cluster numbers from an extended merger-tree model
• Predicting the Scaling Relations between the Dark Matter Halo Mass and Observables from Generalised Profiles II: Intracluster Gas Emission
• JWST Discovery of Strong Lensing from a Galaxy Cluster at Cosmic Noon: Giant Arcs and a Highly Concentrated Core of XLSSC 122
• A halo model approach to describe clustering and emission of the two main star forming galaxy populations for Cosmic Infrared Background studies
• Ellipticities of Galaxy Cluster Halos from Halo-Shear-Shear Correlations
• The AIDA-TNG project: dark matter profiles and concentrations in alternative dark matter models
• The Influence of Subhaloes on Host Halo Properties
• Deep lensing with a twist: E and B modes in a field with multiple lenses
• Revisiting Galaxy Cluster Scaling Relations through Dark Matter-Gas Coherence: Scatter Dependence on Dynamical State
• The non-thermal secondary CMB anisotropies from a cosmic distribution of radio galaxy lobes
• MIGHTEE: The dark matter haloes, duty cycle and mechanical feedback from radio-AGN up to $z\sim 2.5$
• Cosmic magnification on high-redshift submillimeter galaxies
• Dark matter haloes in the multicomponent model. III. From dwarfs to galaxy clusters
• Dissecting the Strong-lensing Galaxy Cluster MS 0440.5+0204. I. The Mass Density Profile
• Measuring the Stellar-to-Halo Mass Relation at $\sim 10^{10}$ Solar masses, using forthcoming space-based imaging of galaxy-galaxy strong lenses
• Constraining Merging Galaxy Clusters with X-ray and Lensing Simulations and Observations: The case of Abell 2146
• Probing baryonic feedback with fast radio bursts: joint analyses with cosmic shear and galaxy clustering
• RXCJ1111.6+4050 galaxy cluster: the observational evidence of a transitional fossil group
• AMICO galaxy clusters in KiDS-1000: Splashback radius from weak lensing and cluster-galaxy correlation function
• The Hydrostatic Mass Bias and the ${\sigma }_8$ Tension: A Multi-Probe Forecast for Stage-IV/V Surveys
• Core Mass Estimates in Strong Lensing Galaxy Clusters: a Comparison Between Masses Obtained from Detailed Lens Models, Single-Halo Lens Models, and Einstein Radii
• Detecting low-mass haloes with strong gravitational lensing I: the effect of data quality and lensing configuration
• Forecasting the potential of weak lensing magnification to enhance LSST large-scale structure analyses
• AMICO galaxy clusters in KiDS-DR3: the impact of estimator statistics on the luminosity-mass scaling relation
• Dissecting the strong lensing galaxy cluster MS 0440$+$0204 II. New optical spectroscopic observations in a wider area and cluster dynamical state
• Is the Sgr dSph a dark matter dominated system?
• Towards a universal model for the density profiles of dark matter haloes
• On Weak Lensing Response Functions
• Cross-correlations between mm-wave line-intensity mapping and weak lensing surveys: preliminary consideration of long-term prospects
• Universal Fitting Formulae for the Peak Concentration of Dark Matter Halos
• Initial Investigations of the Outskirts of XLSSC 122