AMICO galaxy clusters in KiDS-DR3: cosmological constraints from large-scale stacked weak lensing profiles

Abstract

Context. The large-scale mass distribution around dark matter haloes hosting galaxy clusters provides sensitive cosmological information. Aims. In this work, we make use of a large photometric galaxy cluster sample, constructed from the public Third Data Release of the Kilo-Degree Survey, and the corresponding shear signal, to assess cluster masses and test the concordance $\Lambda$-cold dark matter ($\Lambda$CDM) model. In particular, we study the weak gravitational lensing effects on scales beyond the cluster virial radius, where the signal is dominated by correlated and uncorrelated matter density distributions along the line-of-sight. The analysed catalogue consists of 6962 galaxy clusters, in the redshift range $0.1\le z\le 0.6$ and with signal-to-noise ratio larger than 3.5. Methods. We perform a full Bayesian analysis to model the stacked shear profiles of these clusters. The adopted likelihood function considers both the small-scale 1-halo term, used primarily to constrain the cluster structural properties, and the 2-halo term, that can be used to constrain cosmological parameters. Results. We find that the adopted modelling is successful to assess both the cluster masses and the total matter density parameter, ${\Omega }_M$, when fitting shear profiles up to the largest available scales of 35 Mpc/h. Moreover, our results provide a strong observational evidence of the 2-halo signal in the stacked gravitational lensing of galaxy clusters, further demonstrating the reliability of this probe for cosmological studies. The main result of this work is a robust constraint on ${\Omega }_M$, assuming a flat $\Lambda$CDM cosmology. We get ${\Omega }_M=0.29\pm 0.02$, estimated from the full posterior probability distribution, consistent with the estimates from cosmic microwave background experiments.

arXiv commentAccepted for publication on A&A, replaced to match the final version: minor comments

References in corpus (94)

• Planck 2015 results. XIII. Cosmological parameters
• A Universal Density Profile from Hierarchical Clustering
• Efficient Computation of CMB anisotropies in closed FRW models
• Large scale bias and the peak background split
• Populating a cluster of galaxies - I. Results at z=0
• Weak Gravitational Lensing
• Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
• Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes
• Planck 2013 results. I. Overview of products and scientific results
• An analytic model for the spatial clustering of dark matter haloes
• Concentrations of Dark Halos from their Assembly Histories
• Bayesian photometric redshift estimation
• Chandra Cluster Cosmology Project III: Cosmological Parameter Constraints
• KiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing
• The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests
• MultiDark simulations: the story of dark matter halo concentrations and density profiles
• Dark matter halo concentrations in the Wilkinson Microwave Anisotropy Probe year 5 cosmology
• Power Spectra for Cold Dark Matter and its Variants
• The statistics of LCDM Halo Concentrations
• CFHTLenS: The Canada-France-Hawaii Telescope Lensing Survey
• Concentration, Spin and Shape of Dark Matter Haloes as a Function of the Cosmological Model: WMAP1, WMAP3 and WMAP5 results
• Halo concentrations in the standard LCDM cosmology
• Galaxy And Mass Assembly (GAMA): end of survey report and data release 2
• Concentration, Spin and Shape of Dark Matter Haloes: Scatter and the Dependence on Mass and Environment
• Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data
• Accurate universal models for the mass accretion histories and concentrations of dark matter halos
• Scaling relations for galaxy clusters in the Millennium-XXL simulation
• The Power Spectrum Dependence of Dark Matter Halo Concentrations
• Planck 2015 results. XXIV. Cosmology from Sunyaev-Zeldovich cluster counts
• Bayesian Galaxy Shape Measurement for Weak Lensing Surveys - III. Application to the Canada-France-Hawaii Telescope Lensing Survey
• Gravitational Lensing Analysis of the Kilo Degree Survey
• The Kilo-Degree Survey
• X-ray properties of galaxy clusters and groups from a cosmological hydrodynamical simulation
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic correlation function between redshifts 0.6 and 1
• Numerical study of halo concentrations in dark-energy cosmologies
• The Universal Mass Accretion History of CDM Haloes
• CFHTLenS: Improving the quality of photometric redshifts with precision photometry
• Weighing simulated galaxy clusters using lensing and X-ray
• Cosmological parameter constraints from galaxy-galaxy lensing and galaxy clustering with the SDSS DR7
• The first and second data releases of the Kilo-Degree Survey
• The Mass-Concentration-Redshift Relation of Cold Dark Matter Halos
• Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances and Weak Lensing
• Cosmological constraints from cosmic shear two-point correlation functions with HSC survey first-year data
• Detection of large scale intrinsic ellipticity-density correlation from the Sloan Digital Sky Survey and implications for weak lensing surveys
• Bayesian Galaxy Shape Measurement for Weak Lensing Surveys -I. Methodology and a Fast Fitting Algorithm
• Lensing and X-ray mass estimates of clusters (SIMULATION)
• Halo mass - concentration relation from weak lensing
• The third data release of the Kilo-Degree Survey and associated data products
• Next Generation Cosmology: Constraints from the Euclid Galaxy Cluster Survey
• Weak Lensing Measurement of the Mass--Richness Relation of SDSS redMaPPer Clusters
• Galaxy Clustering & Galaxy-Galaxy Lensing: A Promising Union to Constrain Cosmological Parameters
• Cosmological simulations of galaxy clusters
• Analytic models of plausible gravitational lens potentials
• Combining cluster observables and stacked weak lensing to probe dark energy: Self-calibration of systematic uncertainties
• Dark matter halo properties of GAMA galaxy groups from 100 square degrees of KiDS weak lensing data
• Detailed cluster lensing profiles at large radii and the impact on cluster weak lensing studies
• Calibration of weak-lensing shear in the Kilo-Degree Survey
• The MUSIC of CLASH: predictions on the concentration-mass relation
• Dark Energy Survey Year 1 Results: Methods for Cluster Cosmology and Application to the SDSS
• The stellar mass fraction and baryon content of galaxy clusters and groups
• Cluster-galaxy weak lensing
• Galaxies in X-ray Groups. II. A Weak Lensing Study of Halo Centering
• Cross-correlation Weak Lensing of SDSS Galaxy Clusters I: Measurements
• The Dynamical State and Mass-Concentration Relation of Galaxy Clusters
• Weak Lensing by Galaxies in Groups and Clusters: I.--Theoretical Expectations
• Formation times, mass growth histories and concentrations of dark matter haloes
• An optimal filter for the detection of galaxy clusters through weak lensing
• AMICO galaxy clusters in KiDS-DR3: sample properties and selection function
• The Assembly of Matter in Galaxy Clusters
• PSZ2LenS. Weak lensing analysis of the Planck clusters in the CFHTLenS and in the RCSLenS
• AMICO: optimised detection of galaxy clusters in photometric surveys
• AMICO galaxy clusters in KiDS-DR3: weak-lensing mass calibration
• Turbulent pressure support and hydrostatic mass-bias in the intracluster medium
• The mass-richness relation of optically-selected clusters from weak gravitational lensing and abundance with Subaru HSC first-year data
• The XXL Survey XXV. Cosmological analysis of the C1 cluster number counts
• CosmoBolognaLib: C++ libraries for cosmological calculations
• Halo model description of the non-linear dark matter power spectrum at $k\gg 1$ Mpc${}^{-1}$
• On Combining Galaxy Clustering and Weak Lensing to Unveil Galaxy Biasing via the Halo Model
• MOKA: a new tool for Strong Lensing Studies
• Galaxy Populations in Massive Galaxy Clusters to z=1.1: Color Distribution, Concentration, Halo Occupation Number and Red Sequence Fraction
• Mass and Concentration estimates from Weak and Strong Gravitational Lensing: a Systematic Study
• Galaxies in X-ray Selected Clusters and Groups in Dark Energy Survey Data I: Stellar Mass Growth of Bright Central Galaxies Since z~1.2
• Optimal filtering of optical and weak lensing data to search for galaxy clusters: application to the COSMOS field
• An improved measurement of baryon acoustic oscillations from the correlation function of galaxy clusters at $z\sim 0.3$
• The XXL Survey: XVI. The clustering of X-ray selected galaxy clusters at z~0.3
• New constraints on ${\sigma }_8$ from a joint analysis of stacked gravitational lensing and clustering of galaxy clusters
• On the Discrepancy between Theoretical and X-Ray Concentration-Mass Relations for Galaxy Clusters
• Searching for galaxy clusters in the Kilo-Degree Survey
• Galaxy Populations in the 26 most massive Galaxy Clusters in the South Pole Telescope SZE Survey
• Measuring the distance-redshift relation with the baryon acoustic oscillations of galaxy clusters
• Mesh-free free-form lensing I: Methodology and application to mass reconstruction
• Searching dark-matter halos in the GaBoDS survey
• CoMaLit -- VI. Intrinsic scatter in stacked relations. The weak lensing AMICO galaxy clusters in KiDS-DR3
• Constraints on the inner density profile of dark-matter haloes from weak gravitational lensing

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• Euclid. I. Overview of the Euclid mission
• AMICO galaxy clusters in KiDS-DR3: cosmological constraints from counts and stacked weak-lensing
• Fast full N-body simulations of generic modified gravity: conformal coupling models
• AMICO galaxy clusters in KiDS-DR3: Constraints on cosmological parameters and on the normalisation of the mass-richness relation from clustering
• Fast full $N$-body simulations of generic modified gravity: derivative coupling models
• Euclid preparation. XXXII. Evaluating the weak lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations
• AMICO galaxy clusters in KiDS-DR3: Measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis
• Brightest Cluster Galaxies Trace Weak Lensing Mass Bias and Halo Triaxiality in The Three Hundred Project
• The miniJPAS survey: clusters and galaxy groups detection with AMICO
• AMICO galaxy clusters in KiDS-DR3: measuring the splashback radius from weak gravitational lensing
• AMICO galaxy clusters in KiDS-DR3: Cosmological constraints from angular power spectrum and correlation function
• Bayesian Control Variates for optimal covariance estimation with pairs of simulations and surrogates
• AMICO-COSMOS galaxy cluster and group catalogue up to $z=2$: Sample properties and X-ray counterparts
• Cosmology with Galaxy Cluster Properties using Machine Learning
• Exploring the mass and redshift dependence of the cluster pressure profile with stacks on thermal SZ maps
• Euclid preparation: Determining the weak lensing mass accuracy and precision for galaxy clusters
• AMICO galaxy clusters in KiDS-1000: cosmological constraints and mass calibration from counts and weak lensing
• AMICO galaxy clusters in KiDS-1000: cosmological sample
• The Three Hundred Project hydrodynamical simulations: Hydrodynamical weak-lensing cluster mass biases and richnesses using different hydro models
• On the tomographic cluster clustering as a cosmological probe
• AMICO-WL: an optimal filtering algorithm for galaxy cluster detections with weak lensing
• AMICO galaxy clusters in KiDS-1000: Splashback radius from weak lensing and cluster-galaxy correlation function
• AMICO galaxy clusters in KiDS-DR3: the impact of estimator statistics on the luminosity-mass scaling relation