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

preprint2011arXivOpen access
Planck CollaborationP. A. R. AdeN. AghanimM. ArnaudM. AshdownJ. AumontC. BaccigalupiA. BalbiA. J. BandayR. B. BarreiroM. BartelmannJ. G. BartlettE. BattanerR. BattyeK. BenabedA. BenoîtJ. -P. BernardM. BersanelliR. BhatiaJ. J. BockA. BonaldiJ. R. BondJ. BorrillF. R. BouchetM. L. BrownM. BucherC. BuriganaP. CabellaC. M. CantalupoJ. -F. CardosoP. CarvalhoA. CatalanoL. CayónA. ChallinorA. ChamballuR. -R. CharyL. -Y ChiangC. ChiangG. ChonP. R. ChristensenE. ChurazovD. L. ClementsS. ColafrancescoS. ColombiF. CouchotA. CoulaisB. P. CrillF. CuttaiaA. Da SilvaH. DahleL. DaneseR. J. DavisP. de BernardisG. De GasperisA. De RosaG. De ZottiJ. DelabrouilleJ. -M. DelouisF. -X. DésertC. DickinsonJ. M. DiegoK. DolagH. DoleS. DonzelliO. DoréU. DörlM. DouspisX. DupacG. EfstathiouP. EisenhardtT. A. EnßlinF. FerozF. FinelliI. FloresO. ForniP. FosalbaM. FrailisE. FranceschiS. FromenteauS. GaleottaK. GangaR. T. Génova-SantosM. GiardG. GiardinoY. Giraud-HéraudJ. González-NuevoR. González-RiestraK. M. GórskiK. J. B. GraingeS. GrattonA. GregorioA. GruppusoD. HarrisonP. HeinämäkiS. Henrot-VersilléC. Hernández-MonteagudoD. HerranzS. R. HildebrandtE. HivonM. HobsonW. A. HolmesW. HovestR. J. HoylandK. M. HuffenbergerG. HurierN. Hurley-WalkerA. H. JaffeW. C. JonesM. JuvelaE. KeihänenR. KeskitaloT. S. KisnerR. KneisslL. KnoxH. Kurki-SuonioG. LagacheJ. -M. LamarreA. LasenbyR. J. LaureijsC. R. LawrenceM. Le JeuneS. LeachR. LeonardiC. LiA. LiddleP. B. LiljeM. Linden-VørnleM. López-CaniegoP. M. LubinJ. F. Macías-PérezC. J. MacTavishB. MaffeiD. MainoN. MandolesiR. MannM. MarisF. MarleauE. Martínez-GonzálezS. MasiS. MatarreseF. MatthaiP. MazzottaS. MeiP. R. MeinholdA. MelchiorriJ. -B. MelinL. MendesA. MennellaS. MitraM. -A. Miville-DeschênesA. MonetiL. MontierG. MorganteD. MortlockD. MunshiA. MurphyP. NaselskyF. NatiP. NatoliC. B. NetterfieldH. U. Nørgaard-NielsenF. NovielloD. NovikovI. NovikovM. OlamieS. OsborneF. PajotF. PasianG. PatanchonT. J. PearsonO. PerdereauL. PerottoF. PerrottaF. PiacentiniM. PiatE. PierpaoliR. PiffarettiS. PlaszczynskiE. PointecouteauG. PolentaN. PonthieuT. PoutanenG. W. PrattG. PrézeauS. PrunetJ. -L. PugetJ. P. RachenW. T. ReachR. ReboloM. ReineckeC. RenaultS. RicciardiT. RillerI. RistorcelliG. RochaC. RossetJ. A. Rubiño-MartínB. RusholmeE. SaarM. SandriD. SantosR. D. E. SaundersG. SaviniB. M. SchaeferD. ScottM. D. SeiffertP. ShellardG. F. SmootA. StanfordJ. -L. StarckF. StivoliV. StolyarovR. StomporR. SudiwalaR. SunyaevD. SuttonJ. -F. SygnetN. TaburetJ. A. TauberL. TerenziL. ToffolattiM. TomasiJ. -P. TorreM. TristramJ. TuovinenL. ValenzianoL. VibertP. VielvaF. VillaN. VittorioL. A. WadeB. D. WandeltJ. WellerS. D. M. WhiteM. WhiteD. YvonA. ZaccheiA. Zonca

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.

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