The Canadian Cluster Comparison Project: weak lensing masses and SZ scaling relations

Abstract

The Canadian Cluster Comparison Project is a comprehensive multi-wavelength survey targeting 50 massive X-ray selected clusters of galaxies to examine baryonic tracers of cluster mass and to probe the cluster-to-cluster variation in the thermal properties of the hot intracluster medium. In this paper we present the weak lensing masses, based on the analysis of deep wide-field imaging data obtained using the Canada-France-Hawaii-Telescope. The final sample includes two additional clusters that were located in the field-of-view. We take these masses as our reference for the comparison of cluster properties at other wavelengths. In this paper we limit the comparison to published measurements of the Sunyaev-Zel'dovich effect. We find that this signal correlates well with the projected lensing mass, with an intrinsic scatter of 12\pm5% at ~r_2500, demonstrating it is an excellent proxy for cluster mass.

14 pages, 5 figures, submitted to MNRAS

References in corpus (13)

• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• Concentration, Spin and Shape of Dark Matter Haloes as a Function of the Cosmological Model: WMAP1, WMAP3 and WMAP5 results
• Testing X-ray Measurements of Galaxy Clusters with Cosmological Simulations
• The Shear TEsting Programme 2: Factors affecting high precision weak lensing analyses
• Comparison of weak lensing masses and X-ray properties of galaxy clusters
• A Dark Core in Abell 520
• Evidence for Non-Hydrostatic Gas from the Cluster X-ray to Lensing Mass Ratio
• Image Analysis for Cosmology: Results from the GREAT10 Galaxy Challenge
• Resurrecting the Red from the Dead: Optical Properties of BCGs in X-ray Luminous Clusters
• A Statistical Study of Weak Lensing by Triaxial Dark Matter Halos: Consequences for Parameter Estimation
• A Survey of Galaxy Kinematics to z ~ 1 in the TKRS/GOODS-N Field. II. Evolution in the Tully-Fisher Relation
• LoCuSS: A Comparison of Sunyaev-Zel'dovich Effect and Gravitational Lensing Measurements of Galaxy Clusters
• Full Lensing Analysis of Abell 1703: Comparison of Independent Lens-Modelling Techniques

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• The 400d Galaxy Cluster Survey weak lensing programme: III: Evidence for consistent WL and X-ray masses at $z\approx 0.5$
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