Planck 2013 results. XXIX. Planck catalogue of Sunyaev-Zeldovich sources
arXiv:1303.5089 · doi:10.1051/0004-6361/201321523
Abstract
We describe the all-sky Planck catalogue of clusters and cluster candidates derived from Sunyaev--Zeldovich (SZ) effect detections using the first 15.5 months of Planck satellite observations. The catalogue contains 1227 entries, making it over six times the size of the Planck Early SZ (ESZ) sample and the largest SZ-selected catalogue to date. It contains 861 confirmed clusters, of which 178 have been confirmed as clusters, mostly through follow-up observations, and a further 683 are previously-known clusters. The remaining 366 have the status of cluster candidates, and we divide them into three classes according to the quality of evidence that they are likely to be true clusters. The Planck SZ catalogue is the deepest all-sky cluster catalogue, with redshifts up to about one, and spans the broadest cluster mass range from (0.1 to 1.6) 10^{15}Msun. Confirmation of cluster candidates through comparison with existing surveys or cluster catalogues is extensively described, as is the statistical characterization of the catalogue in terms of completeness and statistical reliability. The outputs of the validation process are provided as additional information. This gives, in particular, an ensemble of 813 cluster redshifts, and for all these Planck clusters we also include a mass estimated from a newly-proposed SZ-mass proxy. A refined measure of the SZ Compton parameter for the clusters with X-ray counter-parts is provided, as is an X-ray flux for all the Planck clusters not previously detected in X-ray surveys.
42 pages, accepted for publication by A&A, catalogue available at ESA's Planck Legacy Archive and at SZ cluster database http://szcluster-db.ias.u-psud.fr
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- Re-Examination of Globally Flat Space-Time
- The XXL Survey L. Active galactic nucleus contamination in galaxy clusters: Detection and cosmological impact
- Multi-frequency constraints on the non-thermal pressure in galaxy clusters
- Cluster Cosmology with the Velocity Distribution Function of the HeCS-SZ Sample
- Complex diffuse emission in the cluster PLCK~G004.5-19.5
- Reconstructing the Thermal Sunyaev-Zel'dovich Effect in 3D
- Polarization of Sunyaev-Zeldovich signal due to electron pressure anisotropy in galaxy clusters
- The Swift X-ray Telescope Cluster Survey II. X-ray spectral analysis
- Spectral imaging of the thermal Sunyaev-Zel'dovich effect in X-COP galaxy clusters: method and validation
- Growth and disruption in the Lyra complex
- Fast multiscale galaxy cluster detection with weak lensing: towards a mass-selected sample
- Mass bias and cosmological constraints from Planck cluster clustering
- CARMA observations of massive Planck-discovered cluster candidates at z>0.5 associated with WISE overdensities: Breaking the size-flux degeneracy
- A Semi-Analytical Model for the Formation and Evolution of Radio Relics in Galaxy Clusters
- Helium abundance (and ) in X-COP galaxy clusters
- Tracing the assembly histories of galaxy clusters in the nearby universe
- Characterising galaxy clusters' completeness function in Planck with hydrodynamical simulations
- Evolution of X-ray galaxy Cluster Properties in a Representative Sample (EXCPReS). Optimal binning for temperature profile extraction
- The First SRG/eROSITA All-Sky Survey. Characterization of clusters of galaxies misclassified in the eRASS1 point source catalog
- Introducing the Descriptive Parametric Model: Gaseous Profiles for Galaxies, Groups, and Clusters
- Resolving the Merging Planck Cluster PLCK G147.3-16.6 with GISMO
- An Empirical Mass Function Distribution
- Why are some galaxy clusters underluminous? The very low concentration of the CL2015 mass profile
- A CMB Gibbs sampler for localized secondary anisotropies
- The imprints of galaxy cluster internal dynamics on the Sunyaev-Zeldovich effect
- The XMM-SERVS X-ray eXtended Galaxy Cluster (XVXGC) catalog
- Strong Lensing Analysis of PLCK G004.519.5, a Planck-Discovered Cluster Hosting a Radio Relic at
- CARMA observations of massive Planck-discovered cluster candidates at z>0.5 associated with WISE overdensities: strategy, observations and validation
- Molecular gas in cool-core brightest cluster galaxies at
- The Wendelstein Weak Lensing (WWL) pathfinder: Accurate weak lensing masses for Planck clusters
- Measuring the scatter of the mass-richness relation in galaxy clusters in photometric imaging surveys by means of their correlation function
- Chandra observations of the Abell S0295 cluster
- Searching for galaxy clusters in the VST-KiDS Survey
- Characterising the optical properties of galaxy clusters with GMPhoRCC
- Optical Identification and Spectroscopic Redshift Measurements of 216 Galaxy Clusters from the SRG/eROSITA All-Sky Survey
- On the Scarcity of Dense Cores ( cm) in High Latitude Planck Galactic Cold Clumps
- Optical Identification of Galaxy Clusters among SRG/eROSITA X-ray Sources Based on Photometric Redshift Estimates for Galaxies
- Environment-based selection effects of Planck clusters
- Observations of compact sources in galaxy clusters using MUSTANG2
- Does the Fe L-shell blend bias abundance measurements in intermediate-temperature clusters?
- Radio and mid-infrared properties of the blazar J14190838
- Chandra and XMM-Newton observations of the merging cluster of galaxies PLCK G036.7+14.9
- Revisiting the temperature evolution law of the CMB with gaussian processes
- The phase-space of tailed radio galaxies in massive clusters
- Searching for rotation in X-COP galaxy clusters
- VST ATLAS Galaxy Cluster Catalogue I: cluster detection and mass calibration
- A strong lensing model of the galaxy cluster PSZ1 G311.65-18.48
- Probing gravity with PLANCK data on cluster pressure profiles
- Forecasts for Next Generation tSZ Surveys: the Impact of a Cosmology-Dependent Selection Function
- A test of galaxy cluster fundamental plane for the X-COP sample
- Gas thermodynamics meets galaxy kinematics: Joint mass measurements for eROSITA galaxy clusters
- RXCJ1111.6+4050 galaxy cluster: the observational evidence of a transitional fossil group
- The Integrated Cluster Finder for the ARCHES project
- Empirical formulae to describe some physical properties of small groups of protogalaxies with multiplicity
- Optical Follow-up of Planck Cluster Candidates with Small Instruments
- The Swift AGN and Cluster Survey. II. Cluster Confirmation with SDSS Data
- HSC-XXL : Baryon budget of the 136 XXL Groups and Clusters
- Galaxy Cluster Science with the Sunyaev-Zel'dovich Effect
- CFHTLenS: Weak lensing calibrated scaling relations for low mass clusters of galaxies
- The Multi-Epoch Jet Outbursts in Abell 496: synchrotron ageing and buoyant X-ray cavities draped by warm gas filaments
- The scaling relation and its difference between cool-core and non-cool-core clusters
- Testing the thermal Sunyaev-Zel'dovich power spectrum of a halo model using hydrodynamical simulations
- Deriving accurate galaxy cluster masses using X-ray thermodynamic profiles and graph neural networks
- Increase in the Brightness of the Cosmic Radio Background toward Galaxy Clusters
- Radio halos in a mass-selected sample of 75 galaxy clusters. I. Sample selection and data analysis
- Forecasting Galaxy Cluster HI Mass Recovery with CHIME at Redshifts z = 1 and 2 via the IllustrisTNG Simulations
- The ROSAT Raster Survey in the North-Ecliptic Pole Field: X-ray Catalogue and Optical Identifications
- Hydrostatic equilibrium of X-ray gas in X-COP clusters with HMG
- A Spectroscopic View of the JWST/GTO Strong Lensing Cluster A1489
- Evidence for a moderate spin from X-ray reflection of the high-mass supermassive black hole in the cluster-hosted quasar H1821+643
- Godzilla, a monster lurks in the Sunburst galaxy
- KAT-7 detection of radio halo emission in the Triangulum Australis galaxy cluster
- A VLT/VIMOS view of two multiple-cluster systems: structure and galaxy properties
- High resolution SZ observations at the IRAM 30-m telescope with NIKA
- Timing the last major merger of galaxy clusters with large halo sparsity
- CHEX-MATE: Morphological analysis of the sample
- Probing the evolution of galaxy clusters with the SZ Effect