Next Generation Virgo Cluster Survey. XXI. The weak lensing masses of the CFHTLS and NGVS RedGOLD galaxy clusters and calibration of the optical richness

Abstract

We measured stacked weak lensing cluster masses for a sample of 1325 galaxy clusters detected by the RedGOLD algorithm in the Canada-France-Hawaii Telescope Legacy Survey W1 and the Next Generation Virgo Cluster Survey at $0.2<z<0.5$, in the optical richness range $10<\lambda <70$. After a selection of our best richness subsample ($20<\lambda <50$), this is the most comprehensive lensing study of a $\sim 100\%$ complete and $\sim 90\%$ pure optical cluster catalogue in this redshift range, with a total of 346 clusters in $\sim 164de{g}^2$. We test three different mass models, and our best model includes a basic halo model, with a Navarro Frenk and White profile, and correction terms that take into account cluster miscentering, non-weak shear, the two-halo term, the contribution of the Brightest Cluster Galaxy, and an a posteriori correction for the intrinsic scatter in the mass-richness relation. With this model, we obtain a mass-richness relation of $\log M_{200}/M_{\odot }=(14.48\pm 0.04)+(1.14\pm 0.23)\log (\lambda /40)$ (statistical uncertainties). This result is consistent with other published lensing mass-richness relations. When compared to X-ray masses and mass proxies, we find that on average weak lensing masses are $\sim 10\%$ higher than those derived in the X-ray in the range $2\times 10^{13}{M}_{\odot }<E(z)M_{200}^X<2\times 10^{14}{M}_{\odot }$, in agreement with most previous results and simulations. We also give the coefficients of the scaling relations between the lensing mass and X-ray mass proxies, $L_X$ and $T_X$, and compare them with previous results.

arXiv comment27 pages, 10 figures

References in corpus (97)

• emcee: The MCMC Hammer
• Stellar population synthesis at the resolution of 2003
• The Sloan Digital Sky Survey: Technical Summary
• The Structure of Cold Dark Matter Halos
• Efficient Computation of CMB anisotropies in closed FRW models
• Profiles of dark haloes: evolution, scatter, and environment
• Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample
• Accurate photometric redshifts for the CFHT Legacy Survey calibrated using the VIMOS VLT Deep Survey
• Bayesian photometric redshift estimation
• Cosmological Parameters from Observations of Galaxy Clusters
• Analytic model for galaxy and dark matter clustering
• The Photometric Performance and Calibration of the HST Advanced Camera For Surveys
• The Dark Energy Survey: more than dark energy - an overview
• The Tenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Apache Point Observatory Galactic Evolution Experiment
• Measuring and Modelling the Redshift Evolution of Clustering: the Hubble Deep Field North
• Cold dark matter haloes in the Planck era: evolution of structural parameters for Einasto and NFW profiles
• Tracing cosmic evolution with clusters of galaxies
• redMaPPer I: Algorithm and SDSS DR8 Catalog
• The DEEP2 Galaxy Redshift Survey: Design, Observations, Data Reduction, and Redshifts
• CFHTLenS: The Canada-France-Hawaii Telescope Lensing Survey
• The 10 Meter South Pole Telescope
• Galaxy cluster X-ray luminosity scaling relations from a representative local sample (REXCESS)
• The MCXC: a Meta-Catalogue of X-ray detected Clusters of galaxies
• Science Objectives and Early Results of the DEEP2 Redshift Survey
• The Sloan Lens ACS Survey. IV: the mass density profile of early-type galaxies out to 100 effective radii
• Galaxies in the Hubble Ultra Deep Field: I. Detection, Multiband Photometry, Photometric Redshifts, and Morphology
• Bayesian Galaxy Shape Measurement for Weak Lensing Surveys - III. Application to the Canada-France-Hawaii Telescope Lensing Survey
• CFHTLenS: The Canada-France-Hawaii Telescope Lensing Survey - Imaging Data and Catalogue Products
• The VIMOS VLT Deep Survey final data release: a spectroscopic sample of 35016 galaxies and AGN out to z~6.7 selected with 17.5<=i_{AB}<=24.7
• K-band Properties of Galaxy Clusters and Groups: Luminosity Function, Radial Distribution and Halo Occupation Number
• Virial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Normalization Cosmology
• Ancient Light from Young Cosmic Cities: Physical and Observational Signatures of Galaxy Proto-Clusters
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). An unprecedented view of galaxies and large-scale structure at 0.5<z<1.2
• The redMaPPer Galaxy Cluster Catalog From DES Science Verification Data
• Detection of (dark) matter concentrations via weak gravitational lensing
• The accretion of galaxies into groups and clusters
• A Deep, Wide Field, Optical, and Near Infrared Catalog of a Large Area around the Hubble Deep Field North
• Systematic errors in weak lensing: application to SDSS galaxy-galaxy weak lensing
• On the Accuracy of Weak Lensing Cluster Mass Reconstructions
• GaBoDS: The Garching-Bonn Deep Survey; IV. Methods for the Image reduction of multi-chip Cameras
• CFHTLenS: Improving the quality of photometric redshifts with precision photometry
• Weighing simulated galaxy clusters using lensing and X-ray
• The Atacama Cosmology Telescope: Sunyaev Zel'dovich Selected Galaxy Clusters at 148 GHz in the 2008 Survey
• A Weak Lensing Study of X-ray Groups in the COSMOS survey: Form and Evolution of the Mass-Luminosity Relation
• Measuring the Redshift Evolution of Clustering: the Hubble Deep Field South
• The Palomar Distant Cluster Survey: I. The Cluster Catalog
• Density profiles of galaxy groups and clusters from SDSS galaxy-galaxy weak lensing
• Robust Weak-lensing Mass Calibration of Planck Galaxy Clusters
• Lensing and X-ray mass estimates of clusters (SIMULATION)
• Faint Galaxies in deep ACS observations
• Next Generation Cosmology: Constraints from the Euclid Galaxy Cluster Survey
• LoCuSS: Comparison of Observed X-ray and Lensing Galaxy Cluster Scaling Relations with Simulations
• Weak Lensing Measurement of the Mass--Richness Relation of SDSS redMaPPer Clusters
• Evolution of the Color-Magnitude Relation in Galaxy Clusters at z ~1 from the ACS Intermediate Redshift Cluster Survey
• XMM-Newton and Chandra Cross Calibration Using HIFLUGCS Galaxy Clusters: Systematic Temperature Differences and Cosmological Impact
• Large scale bias and stochasticity of halos and dark matter
• Robust Optical Richness Estimation with Reduced Scatter
• CARS: the CFHTLS-Archive-Research Survey; I. Five-band multi-colour data from 37 sq. deg. CFHTLS-Wide observations
• The XMM Cluster Survey: Optical analysis methodology and the first data release
• 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
• Searching for massive clusters in weak lensing surveys
• The CFHT Legacy Survey: stacked images and catalogs
• Detailed cluster lensing profiles at large radii and the impact on cluster weak lensing studies
• Constraining the Scatter in the Mass-Richness Relation of maxBCG Clusters With Weak Lensing and X-ray Data
• redMaPPer II: X-ray and SZ Performance Benchmarks for the SDSS Catalog
• Size Evolution of Spheroids in a Hierarchical Universe
• Galaxies in X-ray Groups I: Robust Membership Assignment and the Impact of Group Environments on Quenching
• Weighing the Giants V: Galaxy Cluster Scaling Relations
• Calibration of weak-lensing shear in the Kilo-Degree Survey
• Galaxies in X-ray Groups. II. A Weak Lensing Study of Halo Centering
• Confronting theoretical models with the observed evolution of the galaxy population out to z=4
• Constraints on the Richness-Mass Relation and the Optical-SZE Positional Offset Distribution for SZE-Selected Clusters
• The Mean and Scatter of the Velocity Dispersion-Optical Richness Relation for maxBCG Galaxy Clusters
• GaBoDS: The Garching-Bonn Deep Survey -- IX. A sample of 158 shear-selected mass concentration candidates
• The Next Generation Virgo Cluster Survey. VI. The Kinematics of Ultra-compact Dwarfs and Globular Clusters in M87
• Weak Lensing by Galaxies in Groups and Clusters: I.--Theoretical Expectations
• HeCS-SZ: The Hectospec Survey of Sunyaev-Zeldovich Selected Clusters
• The roadmap for unification in galaxy group selection:. I. A search for extended X-ray emission in the CNOC2 survey
• Galaxy Cluster Mass Estimation from Stacked Spectroscopic Analysis
• The XMM-LSS catalogue: X-ray sources and associated optical data. Version I
• On the Self-Similar Appearance of Galaxy Clusters in X-rays
• The impact of AGN feedback and baryonic cooling on galaxy clusters as gravitational lenses
• How does our choice of observable influence our estimation of the centre of a galaxy cluster? Insights from cosmological simulations
• Measurement of the halo bias from stacked shear profiles of galaxy clusters
• The 400d Galaxy Cluster Survey weak lensing programme: III: Evidence for consistent WL and X-ray masses at $z\approx 0.5$
• Mining the gap: evolution of the magnitude gap in X-ray galaxy groups from the 3 square degree XMM coverage of CFHTLS
• CFHTLenS: The Environmental Dependence of Galaxy Halo Masses from Weak Lensing
• CFHTLenS: A Weak Lensing Shear Analysis of the 3D-Matched-Filter Galaxy Clusters
• Measuring the Thermal Sunyaev-Zel'dovich Effect Through the Cross Correlation of Planck and WMAP Maps with ROSAT Galaxy Cluster Catalogs
• The Next Generation Virgo Cluster Survey. XV. The photometric redshift estimation for background sources
• Weak-lensing-inferred scaling relations of galaxy clusters in the RCS2: mass-richness, mass-concentration, mass-bias, and more
• Reproducing the entropy structure in galaxy groups
• Weak lensing calibration of mass bias in the REFLEX+BCS X-ray galaxy cluster catalogue
• A Comparison of Weak Lensing Measurements From Ground- and Space-Based Facilities
• II. Apples to apples $A^2$: cluster selection functions for next-generation surveys
• Effects of center offset and noise on weak-lensing derived concentration-mass relation of dark matter halos

Cited by in corpus (6)

• Constraints from thermal Sunyaev-Zeldovich cluster counts and power spectrum combined with CMB
• AMICO galaxy clusters in KiDS-DR3: weak-lensing mass calibration
• Evolution of the cluster optical galaxy luminosity function in the CFHTLS : breaking the degeneracy between mass and redshift
• Measuring the hydrostatic mass bias in galaxy clusters by combining Sunyaev-Zel'dovich and CMB lensing data
• Tightening weak lensing constraints on the ellipticity of galaxy-scale dark matter haloes
• YOLO-CL cluster detection in the Rubin/LSST DC2 simulation