AMICO galaxy clusters in KiDS-DR3: cosmological constraints from counts and stacked weak-lensing

Abstract

We present a cosmological analysis of abundances and stacked weak-lensing profiles of galaxy clusters, exploiting the AMICO KiDS-DR3 catalogue. The sample consists of 3652 galaxy clusters with intrinsic richness ${\lambda }^{\ast }\ge 20$, over an effective area of 377 deg${}^2$, in the redshift range $z\in [0.1,0.6]$. We quantified the purity and completeness of the sample through simulations. The statistical analysis has been performed by simultaneously modelling the comoving number density of galaxy clusters and the scaling relation between the intrinsic richnesses and the cluster masses, assessed through a stacked weak-lensing profile modelling. The fluctuations of the matter background density, caused by super-survey modes, have been taken into account in the likelihood. Assuming a flat $\Lambda$CDM model, we constrained ${\Omega }_{\mathrm{m}}$, ${\sigma }_8$, $S_8\equiv {\sigma }_8({\Omega }_{\mathrm{m}}/0.3{)}^{0.5}$, and the parameters of the mass-richness scaling relation. We obtained ${\Omega }_{\mathrm{m}}=0.24_{-0.04}^{+0.03}$, ${\sigma }_8=0.86_{-0.07}^{+0.07}$, $S_8=0.78_{-0.04}^{+0.04}$. The constraint on $S_8$ is consistent within 1$\sigma$ with the results from WMAP and Planck. Furthermore, we got constraints on the cluster mass scaling relation in agreement with those obtained from a previous weak-lensing only analysis.

arXiv comment12 pages, 7 figures, 2 tables. Accepted by A&A

References in corpus (67)

• Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
• Large scale bias and the peak background split
• Toward a halo mass function for precision cosmology: the limits of universality
• Cosmological Parameters from Observations of Galaxy Clusters
• The Dark Energy Survey: more than dark energy - an overview
• Chandra Cluster Cosmology Project III: Cosmological Parameter Constraints
• KiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing
• Cosmology and Fundamental Physics with the Euclid Satellite
• Euclid Definition Study Report
• redMaPPer I: Algorithm and SDSS DR8 Catalog
• KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics
• Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic Shear
• The ROSAT-ESO Flux Limited X-ray (REFLEX) Galaxy Cluster Survey. V. The cluster catalogue
• Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data
• Scaling relations for galaxy clusters in the Millennium-XXL simulation
• Cluster Cosmology Constraints from the 2500 deg${}^2$ SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope
• The fourth data release of the Kilo-Degree Survey: ugri imaging and nine-band optical-IR photometry over 1000 square degrees
• The first and second data releases of the Kilo-Degree Survey
• The halo mass function through the cosmic ages
• Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances and Weak Lensing
• The XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme
• The universality of the virial halo mass function and models for non-universality of other halo definitions
• Halo mass function: Baryon impact, fitting formulae and implications for cluster cosmology
• The third data release of the Kilo-Degree Survey and associated data products
• Next Generation Cosmology: Constraints from the Euclid Galaxy Cluster Survey
• The impact of galaxy formation on the total mass, mass profile and abundance of haloes
• Cosmological simulations of galaxy clusters
• The Atacama Cosmology Telescope: The Two-Season ACTPol Sunyaev-Zel'dovich Effect Selected Cluster Catalog
• The Canadian Cluster Comparison Project: weak lensing masses and SZ scaling relations
• Dark Energy Survey Year 1 Results: Methods for Cluster Cosmology and Application to the SDSS
• KiDS-450: Cosmological Constraints from Weak Lensing Peak Statistics - II: Inference from Shear Peaks using N-body Simulations
• Cluster Mass Calibration at High Redshift: HST Weak Lensing Analysis of 13 Distant Galaxy Clusters from the South Pole Telescope Sunyaev-Zel'dovich Survey
• CoMaLit-IV. Evolution and self-similarity of scaling relations with the galaxy cluster mass
• KiDS+VIKING-450: A new combined optical & near-IR dataset for cosmology and astrophysics
• LoCuSS: Calibrating Mass-Observable Scaling Relations for Cluster Cosmology with Subaru Weak Lensing Observations
• KiDS-450: Cosmological Constraints from Weak Lensing Peak Statistics-I: Inference from Analytical Prediction of High Signal-to-Noise Ratio Convergence Peaks
• The effects of baryons on the halo mass function
• 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
• AMICO: optimised detection of galaxy clusters in photometric surveys
• A Lensing Survey of X-ray Luminous Galaxy Clusters at Redshift z ~ 0.2: II: CFH12k Weak Lensing Analysis and Global Correlations
• AMICO galaxy clusters in KiDS-DR3: weak-lensing mass calibration
• The mass-richness relation of optically-selected clusters from weak gravitational lensing and abundance with Subaru HSC first-year data
• CosmoBolognaLib: C++ libraries for cosmological calculations
• The XXL Survey XXV. Cosmological analysis of the C1 cluster number counts
• On the impact of baryons on the halo mass function, bias, and cluster cosmology
• CoMaLit III. Literature Catalogs of weak Lensing Clusters of galaxies (LC^2)
• Mass and galaxy distributions of four massive galaxy clusters from Dark Energy Survey Science Verification data
• A large sample of shear selected clusters from the Hyper Suprime-Cam Subaru Strategic Program S16A wide field mass maps
• The XMM-LSS survey: the Class 1 cluster sample over the extended 11 deg${}^2$ and its spatial distribution
• 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
• Imprints of Dark Energy on Cosmic Structure Formation: III. Sparsity of Dark Matter Halo Profiles
• Imprints of primordial non-Gaussianity on the number counts of cosmic shear peaks
• Measuring the distance-redshift relation with the baryon acoustic oscillations of galaxy clusters
• Fast and easy super-sample covariance of large scale structure observables
• Weak Lensing Analysis of SPT selected Galaxy Clusters using Dark Energy Survey Science Verification Data
• AMICO galaxy clusters in KiDS-DR3: cosmological constraints from large-scale stacked weak lensing profiles
• C${}^3$-Cluster Clustering Cosmology I. New constraints on the cosmic growth rate at z~0.3 from redshift-space clustering anisotropies
• Weak Lensing Peaks in Simulated Light-Cones: Investigating the Coupling between Dark Matter and Dark Energy
• Cosmological Constraints from Galaxy Cluster Sparsity, Cluster Gas Mass Fraction and Baryon Acoustic Oscillations Data
• Redshift-space distortions of galaxies, clusters and AGN: testing how the accuracy of growth rate measurements depends on scales and sample selections
• Extreme value statistics of weak lensing shear peak counts
• CoMaLit -- VI. Intrinsic scatter in stacked relations. The weak lensing AMICO galaxy clusters in KiDS-DR3
• Formation of the First Two Black Hole-Neutron Star Mergers (GW200115 and GW200105) from Isolated Binary Evolution

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