The MUSIC of CLASH: predictions on the concentration-mass relation
arXiv:1404.1384 · doi:10.1088/0004-637X/797/1/34
Abstract
We present the results of a numerical study based on the analysis of the MUSIC-2 simulations, aimed at estimating the expected concentration-mass relation for the CLASH cluster sample. We study nearly 1400 halos simulated at high spatial and mass resolution, which were projected along many lines-of-sight each. We study the shape of both their density and surface-density profiles and fit them with a variety of radial functions, including the Navarro-Frenk-White, the generalised Navarro-Frenk-White, and the Einasto density profiles. We derive concentrations and masses from these fits and investigate their distributions as a function of redshift and halo relaxation. We use the X-ray image simulator X-MAS to produce simulated Chandra observations of the halos and we use them to identify objects resembling the X-ray morphologies and masses of the clusters in the CLASH X-ray selected sample. We also derive a concentration-mass relation for strong-lensing clusters. We find that the sample of simulated halos which resemble the X-ray morphology of the CLASH clusters is composed mainly by relaxed halos, but it also contains a significant fraction of un-relaxed systems. For such a sample we measure an average 2D concentration which is ~11% higher than found for the full sample of simulated halos. After accounting for projection and selection effects, the average NFW concentrations of CLASH clusters are expected to be intermediate between those predicted in 3D for relaxed and super-relaxed halos. Matching the simulations to the individual CLASH clusters on the basis of the X-ray morphology, we expect that the NFW concentrations recovered from the lensing analysis of the CLASH clusters are in the range [3-6], with an average value of 3.87 and a standard deviation of 0.61. Simulated halos with X-ray morphologies similar to those of the CLASH clusters are affected by a modest orientation bias.
arXiv comment21 pages, 16 figures, 3 tables, submitted to ApJ
References in corpus (75)
- A Universal Density Profile from Hierarchical Clustering
- The Structure of Cold Dark Matter Halos
- The cosmological simulation code GADGET-2
- Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons
- Dark matter halo concentrations in the Wilkinson Microwave Anisotropy Probe year 5 cosmology
- Resolving the Structure of Cold Dark Matter Halos
- The Diversity and Similarity of Simulated Cold Dark Matter Halos
- Triaxial Modeling of Halo Density Profiles with High-resolution N-body Simulations
- Cluster Lensing And Supernova survey with Hubble (CLASH): An Overview
- The statistics of LCDM Halo Concentrations
- Adaptive Refinement Tree - a new high-resolution N-body code for cosmological simulations
- Analytical Models For Galactic Nuclei
- Improved constraints on dark energy from Chandra X-ray observations of the largest relaxed galaxy clusters
- Empirical models for Dark Matter Halos. I. Nonparametric Construction of Density Profiles and Comparison with Parametric Models
- Accurate universal models for the mass accretion histories and concentrations of dark matter halos
- Resolving the Structure of Cold Dark Matter Halos II
- CLASH: Three Strongly Lensed Images of a Candidate z ~ 11 Galaxy
- On the connection between giant radio halos and cluster mergers
- Numerical study of halo concentrations in dark-energy cosmologies
- A highly magnified candidate for a young galaxy seen when the Universe was 500 Myrs old
- On the Accuracy of Weak Lensing Cluster Mass Reconstructions
- Weighing simulated galaxy clusters using lensing and X-ray
- A complete sample of twelve very X-ray luminous galaxy clusters at z>0.5
- Simulating the effect of AGN feedback on the metal enrichment of galaxy clusters
- Creation of cosmic structure in the complex galaxy cluster merger Abell 2744
- Combined strong and weak lensing analysis of 28 clusters from the Sloan Giant Arcs Survey
- Lensing and X-ray mass estimates of clusters (SIMULATION)
- Dark Matter Halo Profiles of Massive Clusters: Theory vs. Observations
- Gas expulsion by quasar-driven winds as a solution to the over-cooling problem in galaxy groups and clusters
- Quantifying the Morphologies and Dynamical Evolution of Galaxy Clusters. II. Application to a Sample of ROSAT Clusters
- The Phoenix Project: the Dark Side of Rich Galaxy Clusters
- Are Brightest Halo Galaxies Central Galaxies?
- CLASH: The enhanced lensing efficiency of the highly elongated merging cluster MACS J0416.1-2403
- The Redshift Evolution of LCDM Halo Parameters: Concentration, Spin, and Shape
- A Census of Star-Forming Galaxies in the z~9-10 Universe based on HST+Spitzer Observations Over 19 CLASH clusters: Three Candidate z~9-10 Galaxies and Improved Constraints on the Star Formation Rate Density at z~9
- CLASH-VLT: The mass, velocity-anisotropy, and pseudo-phase-space density profiles of the z=0.44 galaxy cluster MACS 1206.2-0847
- Characterizing the Cluster Lens Population
- CLASH: Precise New Constraints on the Mass Profile of Abell 2261
- On the role of AGN feedback on the thermal and chemodynamical properties of the hot intra-cluster medium
- Analytical properties of Einasto dark matter haloes
- A non-ideal MHD Gadget: Simulating massive galaxy clusters
- CLASH-X: A Comparison of Lensing and X-ray Techniques for Measuring the Mass Profiles of Galaxy Clusters
- The Dark Matter Distribution in Abell 383: Evidence for a Shallow Density Cusp from Improved Lensing, Stellar Kinematic and X-ray Data
- What is the largest Einstein radius in the universe?
- CLASH: Mass Distribution in and around MACS J1206.2-0847 from a Full Cluster Lensing Analysis
- CLASH: A Census of Magnified Star-Forming Galaxies at z ~ 6-8
- The MUSIC of Galaxy Clusters I: Baryon properties and Scaling Relations of the thermal Sunyaev-Zel'dovich Effect
- The impact of cluster mergers on arc statistics
- A New Survey for Giant Arcs
- Combining weak and strong cluster lensing: Applications to simulations and MS 2137
- Subaru Weak Lensing Measurements of Four Strong Lensing Clusters: Are Lensing Clusters Over-Concentrated?
- Formation times, mass growth histories and concentrations of dark matter haloes
- Strong lensing in the MareNostrum Universe: biases in the cluster lens population
- CLASH: Complete Lensing Analysis of the Largest Cosmic Lens MACS J0717.5+3745 and Surrounding Structures
- The Cluster Lensing and Supernova Survey with Hubble (CLASH): Strong Lensing Analysis of Abell 383 from 16-Band HST WFC3/ACS Imaging
- CLASH: New Multiple-Images Constraining the Inner Mass Profile of MACS J1206.2-0847
- Simulating Chandra observations of galaxy clusters
- Profiles of Dark Matter Velocity Anisotropy in Simulated Clusters
- Ellipsoidal halo finders and implications for models of triaxial halo formation
- CLASH-VLT: spectroscopic confirmation of a z=6.11 quintuply lensed galaxy in the Frontier Fields Cluster RXC J2248.7-4431
- Cosmology in 2D: the concentration-mass relation for galaxy clusters
- Weak lensing analysis of RXC J2248.7-4431
- Properties of Dark Matter Haloes and their Correlations: the Lesson from Principal Component Analysis
- CLASH: Discovery of a Bright z~6.2 Dwarf Galaxy Quadruply Lensed by MACS J0329.6-0211
- Hydrodynamical simulations of galaxy clusters in dark energy cosmologies: II. c-M relation
- The strongest gravitational lenses: I. The statistical impact of cluster mergers
- The MUSIC of Galaxy Clusters II: X-ray global properties and scaling relations
- On the Discrepancy between Theoretical and X-Ray Concentration-Mass Relations for Galaxy Clusters
- Line-of-Sight Structure Toward Strong Lensing Galaxy Clusters
- Sunyaev Zel'dovich Effect Observations of Strong Lensing Galaxy Clusters: Probing the Over-Concentration Problem
- Imprints of Dark Energy on Cosmic Structure Formation: III. Sparsity of Dark Matter Halo Profiles
- The Contribution of Halos with Different Mass Ratios to the Overall Growth of Cluster-Sized Halos
- How Baryonic Processes affect Strong Lensing properties of Simulated Galaxy Clusters
- Scaling Rrelation in two situations of extreme mergers
- Cluster contribution to the X-ray background as a cosmological probe
Cited by in corpus (123)
- MultiDark simulations: the story of dark matter halo concentrations and density profiles
- Euclid. I. Overview of the Euclid mission
- COLOSSUS: A python toolkit for cosmology, large-scale structure, and dark matter halos
- A universal model for halo concentrations
- Hubble Space Telescope Combined Strong and Weak Lensing Analysis of the CLASH Sample: Mass and Magnification Models and Systematic Uncertainties
- The galaxy cluster mass scale and its impact on cosmological constraints from the cluster population
- An accurate physical model for halo concentrations
- On the nature of hydrostatic equilibrium in galaxy clusters
- CLASH: The Concentration-Mass Relation of Galaxy Clusters
- CLASH: Joint Analysis of Strong-Lensing, Weak-Lensing Shear and Magnification Data for 20 Galaxy Clusters
- CLASH-VLT: Insights on the mass substructures in the Frontier Fields Cluster MACS J0416.1-2403 through accurate strong lens modeling
- An excess of small-scale gravitational lenses observed in galaxy clusters
- LoCuSS: Weak-lensing mass calibration of galaxy clusters
- Hydrostatic mass profiles in X-COP galaxy clusters
- Cluster-galaxy weak lensing
- CLASH-X: A Comparison of Lensing and X-ray Techniques for Measuring the Mass Profiles of Galaxy Clusters
- CLASH-VLT: Dissecting the Frontier Fields Galaxy Cluster MACS J0416.1-2403 with Spectra of Member Galaxies
- Modelling the line-of-sight contribution in substructure lensing
- Cosmology and Astrophysics from Relaxed Galaxy Clusters I: Sample Selection
- The impact of baryons on massive galaxy clusters: halo structure and cluster mass estimates
- Pressure of the hot gas in simulations of galaxy clusters
- Interplay among Cooling, AGN Feedback and Anisotropic Conduction in the Cool Cores of Galaxy Clusters
- Lensing Constraints on the Mass Profile Shape and the Splashback Radius of Galaxy Clusters
- Illuminating a Dark Lens : A Type Ia Supernova Magnified by the Frontier Fields Galaxy Cluster Abell 2744
- PSZ2LenS. Weak lensing analysis of the Planck clusters in the CFHTLenS and in the RCSLenS
- The Three Hundred Project: Dynamical state of galaxy clusters and morphology from multi-wavelength synthetic maps
- The concentration-mass relation of clusters of galaxies from the OmegaWINGS survey
- The Morphologies and Alignments of Gas, Mass, and the Central Galaxies of CLASH Clusters of Galaxies
- Weak lensing Analysis of X-Ray-selected XXL Galaxy Groups and Clusters with Subaru HSC Data
- A Free-Form Prediction for the Reappearance of Supernova Refsdal in the Hubble Frontier Fields Cluster MACSJ1149.5+2223
- Three-dimensional Multi-probe Analysis of the Galaxy Cluster A1689
- The Radial Acceleration Relation in CLASH Galaxy Clusters
- The Projected Dark and Baryonic Ellipsoidal Structure of 20 CLASH Galaxy Clusters
- Calibrating the Planck Cluster Mass Scale with CLASH
- Dependency of halo concentration on mass, redshift and fossilness in Magneticum hydrodynamic simulations
- A look to the inside of haloes: a characterisation of the halo shape as a function of overdensity in the Planck cosmology
- CLASH: Accurate Photometric Redshifts with 14 HST bands in Massive Galaxy Cluster Cores
- CLUMP-3D. Testing CDM with galaxy cluster shapes
- The mass-concentration relation in lensing clusters: the role of statistical biases and selection effects
- A Free-Form mass model of the Hubble Frontier Fields Cluster AS1063 (RXC J2248.7-4431) with over one hundred constraints
- Cosmology dependency of halo masses and concentrations in hydrodynamic simulations
- Galaxy cluster lensing masses in modified lensing potentials
- A persistent excess of galaxy-galaxy strong lensing observed in galaxy clusters
- Revisiting the bulge-halo conspiracy I: Dependence on galaxy properties and halo mass
- The relation between mass and concentration in X-ray galaxy clusters at high redshift
- Morphological estimators on Sunyaev--Zel'dovich maps of MUSIC clusters of galaxies
- The Mass-Concentration Relation and the Stellar-to-Halo Mass Ratio in the CFHT Stripe 82 Survey
- Offset between X-ray and optical centers in clusters of galaxies: connecting eROSITA data and simulations
- Halo Concentration, Galaxy Red Fraction, and Gas Properties of Optically-defined Merging Clusters
- CLUMP-3D. Three dimensional lensing and multi-probe analysis of MACS J1206.2-0847, a remarkably regular cluster
- The Galaxy Cluster Concentration-Mass Scaling Relation
- PICS: Simulations of Strong Gravitational Lensing in Galaxy Clusters
- Weak lensing study of 16 DAFT/FADA clusters: substructures and filaments
- Deriving the Hubble constant using Planck and XMM-Newton observations of galaxy clusters
- Comparison of weak lensing by NFW and Einasto halos and systematic errors
- CODEX Weak Lensing: Concentration of Galaxy Clusters at z ~ 0.5
- AMICO galaxy clusters in KiDS-DR3: cosmological constraints from large-scale stacked weak lensing profiles
- CLUMP-3D: Three-dimensional Shape and Structure of 20 CLASH Galaxy Clusters from Combined Weak and Strong Lensing
- Statistical uncertainties and systematic errors in weak lensing mass estimates of galaxy clusters
- Constraints on the Mass, Concentration, and Nonthermal Pressure Support of Six CLASH Clusters from a Joint Analysis of X-ray, SZ, and Lensing Data
- Euclid preparation. XXXII. Evaluating the weak lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations
- The Detection and Statistics of Giant Arcs Behind CLASH Clusters
- Breaking the Vainshtein screening in clusters of galaxies
- The GOGREEN survey: the internal dynamics of clusters of galaxies at redshift 0.9-1.4
- Discovery of a new fundamental plane dictating galaxy cluster evolution from gravitational lensing
- Detection of universality of dark matter profile from Subaru weak lensing measurements of 50 massive clusters
- Precise weak lensing constraints from deep high-resolution images: VLT/HAWK-I analysis of the super-massive galaxy cluster RCS2232727.7020437 at
- The Lack of Non-Thermal Motions in Galaxy Cluster Cores
- Constraining interacting dark energy models with the halo concentration-mass relation
- 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
- RAY-RAMSES: a code for ray tracing on the fly in N-body simulations
- Mesh-free free-form lensing I: Methodology and application to mass reconstruction
- AMICO galaxy clusters in KiDS-DR3: Measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis
- The XXL Survey: XXIII. The Mass Scale of XXL Clusters from Ensemble Spectroscopy
- The thermalisation of massive galaxy clusters
- The Concentration-Mass Relation of Massive, Dynamically Relaxed Galaxy Clusters: Agreement Between Observations and CDM Simulations
- On the coherent rotation of diffuse matter in numerical simulations of galaxy clusters
- Brightest Cluster Galaxies Trace Weak Lensing Mass Bias and Halo Triaxiality in The Three Hundred Project
- Testing non-local gravity by clusters of galaxies
- Gas Density Perturbations in Cool Cores of CLASH Galaxy Clusters
- Cosmology through arc statistics I: sensitivity to and
- The importance of secondary halos for strong lensing in massive galaxy clusters across redshift
- Detection of Strongly Lensed Arcs in Galaxy Clusters with Transformers
- Multi-component DHOST analysis in galaxy clusters
- A New Interpretation of the Mass-Temperature Relation and Mass Calibration of Galaxy Clusters Based on the Fundamental Plane
- Dynamical analysis of clusters of galaxies from cosmological simulations
- Measurements of the Sunyaev-Zel'dovich Effect in MACS J0647.7+7015 and MACS J1206.2-0847 at High Angular Resolution with MUSTANG
- The absolute proper motions of the Arches and Quintuplet clusters
- Non-steady heating of cool cores of galaxy clusters by ubiquitous turbulence and AGN
- A weak lensing analysis of the PLCK G100.2-30.4 cluster
- Halo Concentrations and the New Baseline X-ray Luminosity-Temperature and Mass Relations of Galaxy Clusters
- Physical modelling of galaxy clusters using Einasto dark matter profiles
- Joint Strong and Weak Lensing Analysis of the Massive Cluster Field J0850+3604
- Core Mass Estimates in Strong Lensing Galaxy Clusters Using a Single-Halo Lens Model
- Testing the Collisionless Nature of Dark Matter with the Radial Acceleration Relation in Galaxy Clusters
- Euclid preparation: Determining the weak lensing mass accuracy and precision for galaxy clusters
- Strong Lensing In The Inner Halo Of Galaxy Clusters
- Selecting background galaxies in weak-lensing analysis of galaxy clusters
- AMICO galaxy clusters in KiDS-1000: cosmological constraints and mass calibration from counts and weak lensing
- CHEX-MATE: exploring the kinematical properties of Planck galaxy clusters
- Testing the Reliability of Fast Methods for Weak Lensing Simulations: WL-MOKA on PINOCCHIO
- Accurate dark matter halo elongation from weak-lensing stacking analysis
- Halo Concentrations and the Fundamental Plane of Galaxy Clusters
- Morphology of relaxed and merging galaxy clusters. Analytical models for monolithic Minkowski functionals
- Simulation-based marginal likelihood for cluster strong lensing cosmology
- Dark matter halo concentrations: a short review
- SLICE: SPT-CL J0546-5345 -- A prominent strong-lensing cluster at
- Strong Lensing Analysis of the Galaxy Cluster MACS J1319.9+7003 and the Discovery of a Shell Galaxy
- Galaxy cluster mass bias from projected mass maps: The Three Hundred-NIKA2 LPSZ twin samples
- The AIDA-TNG project: dark matter profiles and concentrations in alternative dark matter models
- The Three Hundred Project: dissecting the fundamental plane of galaxy clusters up to
- Systematic search for lensed X-ray sources in the CLASH fields
- Physical modelling of galaxy clusters and Bayesian inference in astrophysics
- Directional miscentering dependence in weak lensing mass bias
- A test of galaxy cluster fundamental plane for the X-COP sample
- A strong lensing model of the galaxy cluster PSZ1 G311.65-18.48
- Dark matter haloes in the multicomponent model. III. From dwarfs to galaxy clusters
- Correlations in the matter distribution in CLASH galaxy clusters
- Parametric strong lensing model of the galaxy cluster Abell 2390 from Euclid and MUSE observations
- CLASH-VLT: The Fifth Force in Chameleon Gravity from Joint Lensing and Kinematics Cluster Mass Profiles
- Core Mass Estimates in Strong Lensing Galaxy Clusters: a Comparison Between Masses Obtained from Detailed Lens Models, Single-Halo Lens Models, and Einstein Radii