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 1 x 10(15) M-circle dot.
Original language | English |
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Article number | A8 |
Number of pages | 28 |
Journal | Astronomy and Astrophysics |
Volume | 536 |
DOIs | |
Publication status | Published - Dec 2011 |
MoE publication type | A1 Journal article-refereed |
Keywords
- cosmology: observations
- galaxies: clusters: general
- catalogs
- SOUTH-POLE TELESCOPE
- X-RAY-PROPERTIES
- MICROWAVE BACKGROUND TEMPERATURE
- CORONA BOREALIS SUPERCLUSTER
- MASSIVE GALAXY CLUSTERS
- COSMIC DISTANCE SCALE
- COSMOLOGICAL PARAMETERS
- HYDRODYNAMICAL SIMULATIONS
- NEARBY CLUSTERS
- HUBBLE CONSTANT
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Equipment
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Metsähovi Radio Observatory
Joni Tammi (Manager)
School of Electrical EngineeringFacility/equipment: Facility