Planck 2015 results. XXVII. The Second Planck Catalogue of Sunyaev-Zeldovich Sources

preprint2015arXivOpen access
Planck CollaborationP. A. R. AdeN. AghanimM. ArnaudM. AshdownJ. AumontC. BaccigalupiA. J. BandayR. B. BarreiroR. BarrenaJ. G. BartlettN. BartoloE. BattanerR. BattyeK. BenabedA. BenoîtA. Benoit-LévyJ. -P. BernardM. BersanelliP. BielewiczI. BikmaevH. BöhringerA. BonaldiL. BonaveraJ. R. BondJ. BorrillF. R. BouchetM. BucherR. BureninC. BuriganaR. C. ButlerE. CalabreseJ. -F. CardosoP. CarvalhoA. CatalanoA. ChallinorA. ChamballuR. -R. CharyH. C. ChiangG. ChonP. R. ChristensenD. L. ClementsS. ColombiL. P. L. ColomboC. CombetB. ComisF. CouchotA. CoulaisB. P. CrillA. CurtoF. CuttaiaH. DahleL. DaneseR. D. DaviesR. J. DavisP. de BernardisA. De RosaG. De ZottiJ. DelabrouilleF. -X. DésertC. DickinsonJ. M. DiegoK. DolagH. DoleS. DonzelliO. DoréM. DouspisA. DucoutX. DupacG. EfstathiouP. R. M. EisenhardtF. ElsnerT. A. EnßlinH. K. EriksenE. FalgaroneJ. FergussonF. FerozA. FerragamoF. FinelliO. ForniM. FrailisA. A. FraisseE. FranceschiA. FrejselS. GaleottaS. GalliK. GangaR. T. Génova-SantosM. GiardY. Giraud-HéraudE. GjerløwJ. González-NuevoK. M. GórskiK. J. B. GraingeS. GrattonA. GregorioA. GruppusoJ. E. GudmundssonF. K. HansenD. HansonD. L. HarrisonA. HempelS. Henrot-VersilléC. Hernández-MonteagudoD. HerranzS. R. HildebrandtE. HivonM. HobsonW. A. HolmesA. HornstrupW. HovestK. M. HuffenbergerG. HurierA. H. JaffeT. R. JaffeT. JinW. C. JonesM. JuvelaE. KeihänenR. KeskitaloI. KhamitovT. S. KisnerR. KneisslJ. KnocheM. KunzH. Kurki-SuonioG. LagacheJ. -M. LamarreA. LasenbyM. LattanziC. R. LawrenceR. LeonardiJ. LesgourguesF. LevrierM. LiguoriP. B. LiljeM. Linden-VørnleM. López-CaniegoP. M. LubinJ. F. Macías-PérezG. MaggioD. MainoD. S. Y. MakN. MandolesiA. MangilliP. G. MartinE. Martínez-GonzálezS. MasiS. MatarreseP. MazzottaP. McGeheeS. MeiA. MelchiorriJ. -B. MelinL. MendesA. MennellaM. MigliaccioS. MitraM. -A. Miville-DeschênesA. MonetiL. MontierG. MorganteD. MortlockA. MossD. MunshiJ. A. MurphyP. NaselskyA. NastasiF. NatiP. NatoliC. B. NetterfieldH. U. Nørgaard-NielsenF. NovielloD. NovikovI. NovikovM. OlamaieC. A. OxborrowF. PaciL. PaganoF. PajotD. PaolettiF. PasianG. PatanchonT. J. PearsonO. PerdereauL. PerottoY. C. PerrottF. PerrottaV. PettorinoF. PiacentiniM. PiatE. PierpaoliD. PietrobonS. PlaszczynskiE. PointecouteauG. PolentaG. W. PrattG. PrézeauS. PrunetJ. -L. PugetJ. P. RachenW. T. ReachR. ReboloM. ReineckeM. RemazeillesC. RenaultA. RenziI. RistorcelliG. RochaC. RossetM. RossettiG. RoudierE. RozoJ. A. Rubiño-MartínC. RumseyB. RusholmeE. S. RykoffM. SandriD. SantosR. D. E. SaundersM. SavelainenG. SaviniM. P. SchammelD. ScottM. D. SeiffertE. P. S. ShellardT. W. ShimwellL. D. SpencerS. A. StanfordD. SternV. StolyarovR. StomporA. StreblyanskaR. SudiwalaR. SunyaevD. SuttonA. -S. Suur-UskiJ. -F. SygnetJ. A. TauberL. TerenziL. ToffolattiM. TomasiD. TramonteM. TristramM. TucciJ. TuovinenG. UmanaL. ValenzianoJ. ValiviitaB. Van TentP. VielvaF. VillaL. A. WadeB. D. WandeltI. K. WehusS. D. M. WhiteE. L. WrightD. YvonA. ZaccheiA. Zonca

Abstract

We present the all-sky Planck catalogue of Sunyaev-Zeldovich (SZ) sources detected from the 29 month full-mission data. The catalogue (PSZ2) is the largest SZ-selected sample of galaxy clusters yet produced and the deepest all-sky catalogue of galaxy clusters. It contains 1653 detections, of which 1203 are confirmed clusters with identified counterparts in external data-sets, and is the first SZ-selected cluster survey containing > 10310^3 confirmed clusters. We present a detailed analysis of the survey selection function in terms of its completeness and statistical reliability, placing a lower limit of 83% on the purity. Using simulations, we find that the Y5R500 estimates are robust to pressure-profile variation and beam systematics, but accurate conversion to Y500 requires. the use of prior information on the cluster extent. We describe the multi-wavelength search for counterparts in ancillary data, which makes use of radio, microwave, infra-red, optical and X-ray data-sets, and which places emphasis on the robustness of the counterpart match. We discuss the physical properties of the new sample and identify a population of low-redshift X-ray under- luminous clusters revealed by SZ selection. These objects appear in optical and SZ surveys with consistent properties for their mass, but are almost absent from ROSAT X-ray selected samples.

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