Planck Early Results VIII: The all-sky Early Sunyaev-Zeldovich cluster sample

Abstract

We present the first all-sky sample of galaxy clusters detected blindly by the Planck satellite through the Sunyaev-Zeldovich (SZ) effect from its six highest frequencies. This early SZ (ESZ) sample is comprised of 189 candidates, which have a high signal-to-noise ratio ranging from 6 to 29. Its high reliability (purity above 95%) is further ensured by an extensive validation process based on Planck internal quality assessments and by external cross-identification and follow-up observations. Planck provides the first measured SZ signal for about 80% of the 169 previously-known ESZ clusters. Planck furthermore releases 30 new cluster candidates, amongst which 20 meet the ESZ signal-to-noise selection criterion. At the submission date, twelve of the 20 ESZ candidates were confirmed as new clusters, with eleven confirmed using XMM-Newton snapshot observations, most of them with disturbed morphologies and low luminosities. The ESZ clusters are mostly at moderate redshifts (86% with z below 0.3) and span more than a decade in mass, up to the rarest and most massive clusters with masses above 10^15 Msol.

arXiv commentAccepted for publication in a special issue of A&A, 26 pages, this paper is part of a package of papers describing first results of the Planck mission

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• Optical Galaxy Clusters in the Deep Lens Survey
• Multi-wavelength mock observations of the WHIM in a simulated galaxy cluster
• Chandra and XMM-Newton Observations of the Bimodal Planck SZ-detected Cluster PLCKG345.40-39.34 (A3716) with High and Low Entropy Subcluster Cores
• The Science Cases for Building a Band 1 Receiver Suite for ALMA
• The XMM Cluster Survey analysis of the SDSS DR8 redMaPPer Catalogue: Implications for scatter, selection bias, and isotropy in cluster scaling relations
• Redshift-space correlation functions in large galaxy cluster surveys
• WMAP Observations of Planck ESZ Clusters
• Probing the Scale of ALP Interactions with Fermi Blazars
• A matched filter approach for blind joint detection of galaxy clusters in X-ray and SZ surveys
• Reconstructing three-dimensional parameters of galaxy clusters via multifrequency SZ observations
• Examining transitional galaxies to understand the role of clusters and their dynamical status in galaxy quenching
• AMICO galaxy clusters in KiDS-DR3: Cosmological constraints from angular power spectrum and correlation function
• Optical validation and characterization of \Planck\ PSZ2 sources at the Canary Islands observatories. I. First year of LP15 observations
• Probing the time variation of fine structure constant using galaxy clusters and quintessence model
• Bolocam Observations of Two Unconfirmed Galaxy Cluster Candidates from the Planck Early SZ Sample
• Measurement of Galaxy Cluster Integrated Comptonization and Mass Scaling Relations with the South Pole Telescope
• Constraints on the duality relation from ACT cluster data
• Magnetic fields in the outskirts of PSZ2 G096.88+24.18 from depolarization analysis of radio relics
• Sunyaev-Zel'dovich Signal from Quasar Hosts: Implications for Detection of Quasar Feedback
• Chandra Observations of the Spectacular A3411-12 Merger Event
• CARMA follow-up of the northern unconfirmed PLANCK galaxy cluster candidates
• Bayes-X: a Bayesian inference tool for the analysis of X-ray observations of galaxy clusters
• Clusters of galaxies and the cosmic web with SKA
• Planck intermediate results. VI: The dynamical structure of PLCKG214.6+37.0, a Planck discovered triple system of galaxy clusters
• A joint analysis of AMI and CARMA observations of the recently discovered SZ galaxy cluster system AMI-CL J0300+2613
• An Optical Analysis of the Merging Cluster Abell 3888
• Recent developments in astrophysical and cosmological exploitation of microwave surveys
• Modeling the cross power spectrum of Sunyaev-Zel'dovich and X-ray surveys
• MILCANN : A neural network assessed tSZ map for galaxy cluster detection
• A weak lensing analysis of the PLCK G100.2-30.4 cluster
• Parameterization Effects in the analysis of AMI Sunyaev-Zel'dovich Observations
• SZ observations with AMI of the hottest galaxy clusters detected in the XMM-Newton Cluster Survey
• Joint signal extraction from galaxy clusters in X-ray and SZ surveys: A matched-filter approach
• Pairwise kSZ signal extraction efficacy and optical depth estimation
• Exploring the mass and redshift dependence of the cluster pressure profile with stacks on thermal SZ maps
• Distinguishing AGN Feedback Models with the Thermal Sunyaev-Zel'dovich Effect
• Optical validation and characterisation of Planck PSZ1 sources at the Canary Islands observatories. II. Second year of ITP13 observations
• Physical modelling of galaxy clusters detected by Planck
• Evidence of Extended Dust and Feedback around z$\approx$1 Quiescent Galaxies via Millimeter Observations
• The Planck SZ Cluster Catalog: Expected X-ray Properties
• The hydrostatic-to-lensing mass bias from resolved X-ray and optical-IR data
• Constraints on Non-Gaussianity from Sunyaev--Zeldovich Cluster Surveys
• Studying galaxy cluster morphological metrics with Mock-X
• CHEX-MATE: the intracluster medium entropy distribution in the gravity-dominated regime
• Constraints on the Sunyaev-Zel'dovich signal from the Warm Hot Intergalactic Medium from WMAP and SPT data
• Galaxy clusters as probes for cosmology and dark matter
• From "universal" profiles to "universal" scaling laws in X-ray galaxy clusters
• Photon interactions with superconducting topological defects
• Identification of galaxy clusters in cosmic microwave background maps using the Sunyaev-Zel'dovich effect
• Probing galaxy cluster and intra-cluster gas with luminous red galaxies
• Analytical studies on the Sunyaev Zeldovich effect in the cluster of galaxies for three Lorentz frames
• Multi-frequency constraints on the non-thermal pressure in galaxy clusters
• CARMA observations of massive Planck-discovered cluster candidates at z>0.5 associated with WISE overdensities: Breaking the size-flux degeneracy
• Testing the WMAP cosmology via Planck radio catalogues
• The XMM Cluster Survey: Predicted overlap with the Planck Cluster Catalogue
• Evolution of X-ray galaxy Cluster Properties in a Representative Sample (EXCPReS). Optimal binning for temperature profile extraction
• Analytical studies on the Sunyaev-Zeldovich effect in the cluster of galaxies for three Lorentz frames II: single integral formula
• Resolving the Merging Planck Cluster PLCK G147.3-16.6 with GISMO
• Characterising galaxy clusters' completeness function in Planck with hydrodynamical simulations
• Testing for evolution in scaling relations of galaxy clusters: Cross analysis between X-ray and SZ observations
• The XMM-SERVS X-ray eXtended Galaxy Cluster (XVXGC) catalog
• The Wendelstein Weak Lensing (WWL) pathfinder: Accurate weak lensing masses for Planck clusters
• Some results on the radio-SZ correlation for galaxy cluster radio halos
• Lensing Noise in mm-wave Galaxy Cluster Surveys
• Strong Lensing Analysis of PLCK G004.5$-$19.5, a Planck-Discovered Cluster Hosting a Radio Relic at $z=0.52$
• CARMA observations of massive Planck-discovered cluster candidates at z>0.5 associated with WISE overdensities: strategy, observations and validation
• An Optimal and Model-Independent Measurement of the Intracluster Pressure Profile I: Methodology and First Applications
• Evolution of the degree of substructures in simulated galaxy clusters
• The Coma cluster at LOFAR frequencies II: the halo, relic, and a new accretion relic
• VST ATLAS Galaxy Cluster Catalogue I: cluster detection and mass calibration
• Chandra and XMM-Newton observations of the merging cluster of galaxies PLCK G036.7+14.9
• Radio observations of Planck clusters
• The phase-space of tailed radio galaxies in massive clusters
• Galaxy Cluster Science with the Sunyaev-Zel'dovich Effect
• The Swift AGN and Cluster Survey. II. Cluster Confirmation with SDSS Data
• Inference of morphology and dynamical state of nearby $Planck$-SZ galaxy clusters with Zernike polynomials
• The ${\mathrm{Y}}_{\mathrm{SZ},\mathrm{Planck}}-{\mathrm{Y}}_{\mathrm{SZ},\mathrm{XMM}}$ scaling relation and its difference between cool-core and non-cool-core clusters
• X-ray analysis of the Planck-detected triplet-cluster system PLCK G334.8-38
• The comptonization parameter from simulations of single-frequency, single-dish, dual-beam, cm-wave observations of galaxy clusters and mitigating CMB confusion using the Planck sky survey
• Asymmetry and non-random orientation of the inflight effective beam pattern in the WMAP Data
• A VLT/VIMOS view of two $Planck$ multiple-cluster systems: structure and galaxy properties
• The XMM-BCS galaxy cluster survey: I. The X-ray selected cluster catalog from the initial 6 deg${}^2$
• X-ray characterisation of the massive galaxy clusterClG-J104803.7+313843 at z=0.76 with XMM-Newton
• CHEX-MATE: Morphological analysis of the sample
• Testing the correlation between bending angle and polarization properties of bent radio galaxies
• Optimizing Observational Strategy for Future Fgas Constraints
• SZ effect or Not? - Detecting most galaxy clusters' main foreground effect