CoMaLit III. Literature Catalogs of weak Lensing Clusters of galaxies (LC^2)

Abstract

The measurement of the mass of clusters of galaxies is crucial for their use in cosmology and astrophysics. Masses can be efficiently determined with weak lensing (WL) analyses. I compiled Literature Catalogs of weak Lensing Clusters (LC${}^2$). Cluster identifiers, coordinates, and redshifts have been standardised. WL masses were reported to over-densities of 2500, 500, 200, and to the virial one in the reference $\Lambda$CDM model. Duplicate entries were carefully handled. I produced three catalogs: LC${}^2$-single, with 485 unique groups and clusters analysed with the single-halo model; LC${}^2$-substructure, listing substructures in complex systems; LC${}^2$-all, listing all the 822 WL masses found in literature. The catalogs and future updates are publicly available at http://pico.bo.astro.it/~sereno/CoMaLit/LC2/.

10 pages, 4 figures. v2: MNRAS in press; minor changes; updated link. The catalogs and future updates will be hosted at http://pico.bo.astro.it/~sereno/CoMaLit/LC2/

References in corpus (29)

• The redshift dependence of the structure of massive LCDM halos
• A universal model for halo concentrations
• Strong and weak lensing united III: Measuring the mass distribution of the merging galaxy cluster 1E0657-56
• Combining Strong and Weak Gravitational Lensing in Abell 1689
• Revealing the properties of dark matter in the merging cluster MACSJ0025.4-1222
• CLASH: Weak-Lensing Shear-and-Magnification Analysis of 20 Galaxy Clusters
• CIRS: Cluster Infall Regions in the Sloan Digital Sky Survey I. Infall Patterns and Mass Profiles
• Cosmological Constraints from Strong Gravitational Lensing in Galaxy Clusters
• X-ray and Sunyaev-Zel'dovich Effect Measurements of the Gas Mass Fraction in Galaxy Clusters
• Parametric Strong Gravitational Lensing Analysis of Abell 1689
• CLASH-X: A Comparison of Lensing and X-ray Techniques for Measuring the Mass Profiles of Galaxy Clusters
• The Cluster Mass Function from Weak Gravitational Lensing
• A New Look at Massive Clusters: weak lensing constraints on the triaxial dark matter halos of Abell 1689, Abell 1835, & Abell 2204
• Dark Matter and Baryons in the Most X-ray Luminous and Merging Galaxy Cluster RX J1347.5-1145
• Weak lensing survey of galaxy clusters in the CFHTLS Deep
• A Lensing Survey of X-ray Luminous Galaxy Clusters at Redshift z ~ 0.2: II: CFH12k Weak Lensing Analysis and Global Correlations
• Hubble Frontier Fields: The Geometry and Dynamics of the Massive Galaxy Cluster Merger MACSJ0416.1-2403
• Mass and galaxy distributions of four massive galaxy clusters from Dark Energy Survey Science Verification data
• The mass-concentration relation in lensing clusters: the role of statistical biases and selection effects
• Calibration of the Mass-Temperature Relation for Clusters of Galaxies Using Weak Gravitational Lensing
• CoMaLit - II. The scaling relation between mass and Sunyaev-Zel'dovich signal for Planck selected galaxy clusters
• On the deprojection of clusters of galaxies combining X-ray, Sunyaev-Zeldovich temperature decrement and gravitational lensing maps
• Mass, Light and Colour of the Cosmic Web in the Supercluster SCL2243-0935 (z=0.447)
• Shear-Selected Clusters From the Deep Lens Survey III: Masses from Weak Lensing
• A weak lensing analysis of the Abell 2163 cluster
• The Sloan Nearby Cluster Weak Lensing Survey
• Weak Lensing Mass Reconstruction of the Galaxy Cluster Abell 209
• J0454-0309: Evidence for a strong lensing fossil group falling into a poor galaxy cluster
• A Multiwavelength Analysis of the Strong Lensing Cluster RCS 022434-0002.5 at z=0.778

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• Linking a universal gas density profile to the core-excised X-ray luminosity in galaxy clusters up to z ~ 1.1
• Physical properties of Brightest Cluster Galaxies up to redshift 1.80 based on HST data
• Cosmological Constraints from Galaxy Cluster Sparsity, Cluster Gas Mass Fraction and Baryon Acoustic Oscillations Data
• HIFLUGCS: X-ray luminosity -- dynamical mass relation and its implications for mass calibrations with the SPIDERS and 4MOST surveys
• The thermalisation of massive galaxy clusters
• Multiwavelength Analysis of A1240, the Double Radio Relic Merging Galaxy Cluster Embedded in a ~80 Mpc-long Cosmic Filament
• Understanding X-ray and optical selection of galaxy clusters: A comparison of the XXL and CAMIRA cluster catalogues obtained in the common XXL-HSC SSP area
• Multi-probe analysis of the galaxy cluster CL J1226.9+3332: Hydrostatic mass and hydrostatic-to-lensing bias
• Dark Matter Halo Sparsity of Modified Gravity Scenarios
• Field-Based Physical Inference From Peculiar Velocity Tracers
• CHANCES, the Chilean Cluster Galaxy Evolution Survey: Selection and initial characterisation of clusters and superclusters
• CoMaLit -- VI. Intrinsic scatter in stacked relations. The weak lensing AMICO galaxy clusters in KiDS-DR3
• On Escaping a Galaxy Cluster in an Accelerating Universe
• Cosmology with Galaxy Cluster Properties using Machine Learning
• The hydrostatic-to-lensing mass bias from resolved X-ray and optical-IR data
• AMICO galaxy clusters in KiDS-1000: cosmological constraints and mass calibration from counts and weak lensing
• Triggering nuclear and galaxy activity in the Bullet cluster
• Morphology of relaxed and merging galaxy clusters. Analytical models for monolithic Minkowski functionals
• A new non-parametric method to infer galaxy cluster masses from weak lensing
• Improving lensing cluster mass estimate with flexion
• AMICO galaxy clusters in KiDS-DR3: constraints on $\Lambda$CDM from extreme value statistics
• Radio emission from a massive node of the cosmic web. A discovery powered by machine learning
• Galaxy cluster count cosmology with simulation-based inference
• Galaxy Cluster Mass Estimation Through The Splashback Radius
• On the generalized Faber-Jackson relation for galaxy clusters
• STRAWBERRY: Finding haloes in the gravitational potential
• Timing the last major merger of galaxy clusters with large halo sparsity
• The Splashback Mass Function of Galaxy Clusters from Photometric Data
• Cluster gravitational redshifts: uncertainties and survey requirements