CLASH: Weak-Lensing Shear-and-Magnification Analysis of 20 Galaxy Clusters

Abstract

We present a joint shear-and-magnification weak-lensing analysis of a sample of 16 X-ray-regular and 4 high-magnification galaxy clusters at 0.19<z<0.69 selected from the Cluster Lensing And Supernova survey with Hubble (CLASH). Our analysis uses wide-field multi-color imaging, taken primarily with Suprime-Cam on the Subaru Telescope. From a stacked shear-only analysis of the X-ray-selected subsample, we detect the ensemble-averaged lensing signal with a total signal-to-noise ratio of ~25 in the radial range of 200 to 3500kpc/h. The stacked tangential-shear signal is well described by a family of standard density profiles predicted for dark-matter-dominated halos in gravitational equilibrium, namely the Navarro-Frenk-White (NFW), truncated variants of NFW, and Einasto models. For the NFW model, we measure a mean concentration of $c_{200c}=4.01_{-0.32}^{+0.35}$ at $M_{200c}=1.34_{-0.09}^{+0.10}10^{15}{M}_{\odot }$. We show this is in excellent agreement with Lambda cold-dark-matter (LCDM) predictions when the CLASH X-ray selection function and projection effects are taken into account. The best-fit Einasto shape parameter is ${\alpha }_E=0.191_{-0.068}^{+0.071}$, which is consistent with the NFW-equivalent Einasto parameter of $\sim 0.18$. We reconstruct projected mass density profiles of all CLASH clusters from a joint likelihood analysis of shear-and-magnification data, and measure cluster masses at several characteristic radii. We also derive an ensemble-averaged total projected mass profile of the X-ray-selected subsample by stacking their individual mass profiles. The stacked total mass profile, constrained by the shear+magnification data, is shown to be consistent with our shear-based halo-model predictions including the effects of surrounding large-scale structure as a two-halo term, establishing further consistency in the context of the LCDM model.

Accepted by ApJ on 11 August 2014. Textual changes to improve clarity (e.g., Sec.3.2.2 "Number-count Depletion", Sec.4.3 "Shape Measurement", Sec.4.4 "Background Galaxy Selection"). Results and conclusions remain unchanged. For the public release of Subaru data, see http://archive.stsci.edu/prepds/clash/

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• Extended Gravity Constraints at Different Scales
• Constraining dark matter halo profiles with symbolic regression
• CLASH-VLT: The variance in the velocity anisotropy profiles of galaxy clusters
• The Three Hundred Project: dissecting the fundamental plane of galaxy clusters up to $z=1$
• Kinematic Lensing Inference II: Cluster Lensing with $\mathcal{O}$(1) Galaxies
• JWST Discovery of Strong Lensing from a Galaxy Cluster at Cosmic Noon: Giant Arcs and a Highly Concentrated Core of XLSSC 122
• CLASH-VLT velocity anisotropy profiles in a stack of massive galaxy clusters
• The uncommon intracluster medium features of the first massive clusters selected independently of their baryon content
• The LPSZ-CLASH galaxy cluster sample: combining lensing and hydrostatic mass estimates
• Parametric strong lensing model of the galaxy cluster Abell 2390 from Euclid and MUSE observations
• Correlations in the matter distribution in CLASH galaxy clusters
• Constraining the Nature of Dark Matter from Tidal Radii of Cluster Galaxy Subhalos
• Galaxies at the edges: a complete census of MACS J0416.1-2403 cluster
• Deriving accurate galaxy cluster masses using X-ray thermodynamic profiles and graph neural networks
• A New Estimate of Galaxy Mass-to-Light Ratios from Flexion Lensing Statistics
• VENUS: Strong-lensing model of MACS J1931.8-2635 -- revealing the farthest multiply imaged supernova
• The Swift AGN and Cluster Survey. II. Cluster Confirmation with SDSS Data
• AMiBA: Cluster Sunyaev-Zel'dovich Effect Observations with the Expanded 13-Element Array
• A Novel Framework for Modeling Weakly Lensing Shear Using Kinematics and Imaging at Moderate Redshift
• Self-similarity of the mass distribution in rich galaxy clusters up z~1 tracked with weak lensing
• Gravitational Lensing of the supernovae from the Supernova Legacy Survey (SNLS)
• Properties of the Intracluster Medium Assuming an Einasto Dark Matter Profile
• Lensing cosmic drift
• First Steps Toward a Method for Estimating Cosmological Parameters using Strong Lensing, X-ray and Dynamics Total Mass Estimates
• CLASH-VLT: The Fifth Force in Chameleon Gravity from Joint Lensing and Kinematics Cluster Mass Profiles
• The BUFFALO HST Survey
• The thermodynamic structure and large-scale structure filament in MACS J0717.5+3745