Peer-Reviewed Journal Details
Mandatory Fields
Ade, PAR;Aghanim, N;Arnaud, M;Ashdown, M;Aumont, J;Baccigalupi, C;Balbi, A;Banday, AJ;Barreiro, RB;Bartelmann, M;Bartlett, JG;Battaner, E;Battye, R;Benabed, K;Benoit, A;Bernard, JP;Bersanelli, M;Bhatia, R;Bock, JJ;Bonaldi, A;Bond, JR;Borrill, J;Bouchet, FR;Brown, ML;Bucher, M;Burigana, C;Cabella, P;Cantalupo, CM;Cardoso, JF;Carvalho, P;Catalano, A;Cayon, L;Challinor, A;Chamballu, A;Chary, RR;Chiang, LY;Chiang, C;Chon, G;Christensen, PR;Churazov, E;Clements, DL;Colafrancesco, S;Colombi, S;Couchot, F;Coulais, A;Crill, BP;Cuttaia, F;Da Silva, A;Dahle, H;Danese, L;Davis, RJ;de Bernardis, P;de Gasperis, G;de Rosa, A;de Zotti, G;Delabrouille, J;Delouis, JM;Desert, FX;Dickinson, C;Diego, JM;Dolag, K;Dole, H;Donzelli, S;Dore, O;Dorl, U;Douspis, M;Dupac, X;Efstathiou, G;Eisenhardt, P;Ensslin, TA;Feroz, F;Finelli, F;Flores-Cacho, I;Forni, O;Fosalba, P;Frailis, M;Franceschi, E;Fromenteau, S;Galeotta, S;Ganga, K;Genova-Santos, RT;Giard, M;Giardino, G;Giraud-Heraud, Y;Gonzalez-Nuevo, J;Gonzalez-Riestra, R;Gorski, KM;Grainge, KJB;Gratton, S;Gregorio, A;Gruppuso, A;Harrison, D;Heinamaki, P;Henrot-Versille, S;Hernandez-Monteagudo, C;Herranz, D;Hildebrandt, SR;Hivon, E;Hobson, M;Holmes, WA;Hovest, W;Hoyland, RJ;Huffenberger, KM;Hurier, G;Hurley-Walker, N;Jaffe, AH;Jones, WC;Juvela, M;Keihanen, E;Keskitalo, R;Kisner, TS;Kneissl, R;Knox, L;Kurki-Suonio, H;Lagache, G;Lamarre, JM;Lasenby, A;Laureijs, RJ;Lawrence, CR;Le Jeune, M;Leach, S;Leonardi, R;Li, C;Liddle, A;Lilje, PB;Linden-Vornle, M;Lopez-Caniego, M;Lubin, PM;Macias-Perez, JF;MacTavish, CJ;Maffei, B;Maino, D;Mandolesi, N;Mann, R;Maris, M;Marleau, F;Martinez-Gonzalez, E;Masi, S;Matarrese, S;Matthai, F;Mazzotta, P;Mei, S;Meinhold, PR;Melchiorri, A;Melin, JB;Mendes, L;Mennella, A;Mitra, S;Miville-Deschenes, MA;Moneti, A;Montier, L;Morgante, G;Mortlock, D;Munshi, D;Murphy, A;Naselsky, P;Nati, F;Natoli, P;Netterfield, CB;Norgaard-Nielsen, HU;Noviello, F;Novikov, D;Novikov, I;Olamaie, M;Osborne, S;Pajot, F;Pasian, F;Patanchon, G;Pearson, TJ;Perdereau, O;Perotto, L;Perrotta, F;Piacentini, F;Piat, M;Pierpaoli, E;Piffaretti, R;Plaszczynski, S;Pointecouteau, E;Polenta, G;Ponthieu, N;Poutanen, T;Pratt, GW;Prezeau, G;Prunet, S;Puget, JL;Rachen, JP;Reach, WT;Rebolo, R;Reinecke, M;Renault, C;Ricciardi, S;Riller, T;Ristorcelli, I;Rocha, G;Rosset, C;Rubino-Martin, JA;Rusholme, B;Saar, E;Sandri, M;Santos, D;Saunders, RDE;Savini, G;Schaefer, BM;Scott, D;Seiffert, MD;Shellard, P;Smoot, GF;Stanford, A;Starck, JL;Stivoli, F;Stolyarov, V;Stompor, R;Sudiwala, R;Sunyaev, R;Sutton, D;Sygnet, JF;Taburet, N;Tauber, JA;Terenzi, L;Toffolatti, L;Tomasi, M;Torre, JP;Tristram, M;Tuovinen, J;Valenziano, L;Vibert, L;Vielva, P;Villa, F;Vittorio, N;Wade, LA;Wandelt, BD;Weller, J;White, SDM;White, M;Yvon, D;Zacchei, A;Zonca, A
2011
December
Astronomy and Astrophysics
Planck early results. VIII. The all-sky early Sunyaev-Zeldovich cluster sample
Published
232 ()
Optional Fields
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
536
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.
LES ULIS CEDEX A
0004-6361
10.1051/0004-6361/201116459
Grant Details