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Planck early results. VIII. ESZ sample. (Planck+, 2011)

Planck, Collaboration; Ade, P A R; Aghanim, N; Arnaud, M; Ashdown, M; Aumont, J; Baccigalupi, C; Baker, M; Balbi, A; Banday, A J; Barreiro, R B; Bartlett, J G; Battaner, E; Benabed, K; Bennett, K; Benoit, A; Bernard, J P; Bersanelli, M; Bhatia, R; Bock, J J; Bonaldi, A; Bond, J R; Borrill, J; Bouchet, F R; Bradshaw, T; Bremer, M; Bucher, M; Burigana, C; Butler, R C; Cabella, P; Cantalupo, C M; Cappellini, B; Cardoso, J F; Carr, R; Casale, M; Catalano, A; Cayon, L; Challinor, A; Chamballu, A; Charra, J; Chary, R R; Chiang, L Y; Chiang, C; Christensen, P R; Clements, D L; Colombi, S; Couchot, F; Coulais, A; Crill, B P; Crone, G; Crook, M; Cuttaia, F; Danese, L; D'Arcangelo, O; Davies, R D; Davis, R J; de Bernardis, P; de Bruin, J; de Gasperis, G; de Rosa, A; de Zotti, G; Delabrouille, J; Delouis, J M; Desert, F X; Dick, J; Dickinson, C; Dolag, K; Dole, H; Donzelli, S; Dore, O; Doerl, U; Douspis, M; Dupac, X; Efstathiou, G; Ensslin, T A; Eriksen, H K; Finelli, F; Foley, S Forni O Fosalba P Frailis M Franceschi E Freschi M Gaier T C Galeotta S Gallegos J Gandolfo B Ganga K Giard M Giardino G Gienger G Giraud-Heraud Y Gonzalez J Gonzalez-Nuevo J Gorski K M Gratton S Gregorio A Gruppuso A Guyot G Haissinski J Hansen F K Harrison D Helou G Henrot-Versille S Hernandez-Monteagudo C Herranz D Hildebrandt S R Hivon E Hobson M Holmes W A Hornstrup A Hovest W Hoyland R J Huffenberger K M Jaffe A H Jagemann T Jones W C Juillet J J Juvela M Kangaslahti P Keihaenen E Keskitalo R Kisner T S Kneissl R Knox L Krassenburg M Kurki-Suonio H Lagache G Laehteenmaeki A Lamarre J M Lange A E Lasenby A Laureijs R J Lawrence C R Leach S Leahy J P Leonardi R Leroy C Lilje P B Linden-Vornle M Lopez-Caniego M Lowe S Lubin P M Macias-Perez J F Maciaszek T Mactavish C J Maffei B Maino D Mandolesi N Mann R Maris M Martinez-Go nzalez E Masi S Massardi M Matarrese S Matthai F Mazzotta P McDonald A McGehee P Meinhold P R Melchiorri A Melin J B Mendes L Mennella A Mevi C Miniscalco R Mitra S Miville-Deschenes M A Moneti A Montier L Morgante G Morisset N Mortlock D Munshi D Murphy A Naselsky P Natoli P Netterfield C B Norgaard-Nielsen H U Noviello F Novikov D Novikov I O'dwyer I J Ortiz I Osborne S Osuna P Oxborrow C A Pajot F Paladini R Partridge B Pasian F Passvogel T Patanchon G Pearson D Pearson T J Perdereau O Perotto L Perrotta F Piacentini F Piat M Pierpaoli E Plaszczynski S Platania P Pointecouteau E Polenta G Ponthieu N Popa L Poutanen T Prezeau G Prunet S Puget J L Rachen J P Reach W T Rebolo R Reinecke M Reix J M Renault C Ricciardi S Riller T Ristorcelli I Rocha G Rosset C Rowan-Robinson M Rubino-Martin J A Rusholme B Salerno E Sandri M Santos D Savini G Schaefer B M Scott D Seiffert M D Shellard P Simonetto A Smoot G F Sozzi C Starck J L Sternberg J Stivoli F Stolyarov V Stompor R Stringhetti L Sudiwala R Sunyaev R Sygnet J F Tapiador D Tauber J A Tavagnacco D Taylor D Terenzi L Texier D Toffolatti L Tomasi M Torre J P Tristram M Tuovinen J Tuerler M Tuttlebee M Umana G Valenziano L Valiviita J Varis J Vibert L Vielva P Villa F Vittorio N Wade L A Wandelt B D Watson C White S D M White M Wilkinson A Yvon D Zacchei A Zonca A

VizieR Online Data Catalog. 2012;353:69008.

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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 1x10<SUP>15</SUP>M<SUB>⊙</SUB>. (1 data file).

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Volume:
353
Pagination:
69008
Related website(s):
  • Related website http://adsabs.harvard.edu/abs/2012yCat..35369008P
General notes:
  • tablea1.dat 189x98 *The Early Sunyaev-Zeldovich (ESZ) sample
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Active

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Manchester eScholar ID:
uk-ac-man-scw:195418
Created by:
Davis, Richard
Created:
20th May, 2013, 11:09:23
Last modified by:
Davis, Richard
Last modified:
20th May, 2013, 11:09:23

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