We present precise Sunyaev-Zeldovich (SZ) effect measurements in the direction of 62 nearby galaxy clusters (z < 0.5) detected at high signal-to-noise in the first Planck all-sky data set. The sample spans approximately a decade in total mass, 2 x 10(14) M-circle dot < M-500 < 2 x 10(15) M-circle dot, where M-500 is the mass corresponding to a total density contrast of 500. Combining these high quality Planck measurements with deep XMM-Newton X-ray data, we investigate the relations between D-A(2) Y-500, the integrated Compton parameter due to the SZ effect, and the X-ray-derived gas mass M-g,M-500, temperature T-X, luminosity L-X,L-500, SZ signal analogue Y-X,Y-500 = M-g,M-500 x T-X, and total mass M-500. After correction for the effect of selection bias on the scaling relations, we find results that are in excellent agreement with both X-ray predictions and recently-published ground-based data derived from smaller samples. The present data yield an exceptionally robust, high-quality local reference, and illustrate Planck's unique capabilities for all-sky statistical studies of galaxy clusters.

Ade, P., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., et al. (2011). Planck early results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations. ASTRONOMY & ASTROPHYSICS, 536 [10.1051/0004-6361/201116458].

Planck early results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations

BALBI, AMEDEO;Bourdin, H;CABELLA, PAOLO;DE GASPERIS, GIANCARLO;MAZZOTTA, PASQUALE;NATOLI, PAOLO;VITTORIO, NICOLA;
2011-01-01

Abstract

We present precise Sunyaev-Zeldovich (SZ) effect measurements in the direction of 62 nearby galaxy clusters (z < 0.5) detected at high signal-to-noise in the first Planck all-sky data set. The sample spans approximately a decade in total mass, 2 x 10(14) M-circle dot < M-500 < 2 x 10(15) M-circle dot, where M-500 is the mass corresponding to a total density contrast of 500. Combining these high quality Planck measurements with deep XMM-Newton X-ray data, we investigate the relations between D-A(2) Y-500, the integrated Compton parameter due to the SZ effect, and the X-ray-derived gas mass M-g,M-500, temperature T-X, luminosity L-X,L-500, SZ signal analogue Y-X,Y-500 = M-g,M-500 x T-X, and total mass M-500. After correction for the effect of selection bias on the scaling relations, we find results that are in excellent agreement with both X-ray predictions and recently-published ground-based data derived from smaller samples. The present data yield an exceptionally robust, high-quality local reference, and illustrate Planck's unique capabilities for all-sky statistical studies of galaxy clusters.
2011
Pubblicato
Rilevanza internazionale
Articolo
Esperti anonimi
Settore FIS/05 - ASTRONOMIA E ASTROFISICA
English
Con Impact Factor ISI
Ade, P., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., et al. (2011). Planck early results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations. ASTRONOMY & ASTROPHYSICS, 536 [10.1051/0004-6361/201116458].
Ade, P; Aghanim, N; Arnaud, M; Ashdown, M; Aumont, J; Baccigalupi, C; Balbi, A; Banday, A; Barreiro, R; Bartelmann, M; Bartlett, J; Battaner, E; Benabed, K; Benoit, A; Bernard, J; Bersanelli, M; Bhatia, R; Bock, J; Bonaldi, A; Bond, J; Borrill, J; Bouchet, F; Bourdin, H; Brown, M; Bucher, M; Burigana, C; Cabella, P; Cardoso, J; Catalano, A; Cayon, L; Challinor, A; Chamballu, A; Chiang, L; Chiang, C; Chon, G; Christensen, P; Churazov, E; Clements, D; Colafrancesco, S; Colombi, S; Couchot, F; Coulais, A; Crill, B; Cuttaia, F; Da Silva, A; Dahle, H; Danese, L; de Bernardis, P; DE GASPERIS, G; de Rosa, A; de Zotti, G; Delabrouille, J; Delouis, J; Desert, F; Diego, J; Dolag, K; Donzelli, S; Dore, O; Doerl, U; Douspis, M; Dupac, X; Efstathiou, G; Ensslin, T; Finelli, F; Flores Cacho, I; Forni, O; Frailis, M; Franceschi, E; Fromenteau, S; Galeotta, S; Ganga, K; Genova Santos, R; Giard, M; Giardino, G; Giraud Heraud, Y; Gonzalez Nuevo, J; Gorski, K; Gratton, S; Gregorio, A; Gruppuso, A; Harrison, D; Henrot Versille, S; Hernandez Monteagudo, C; Herranz, D; Hildebrandt, S; Hivon, E; Hobson, M; Holmes, W; Hovest, W; Hoyland, R; Huffenberger, K; Jaffe, A; Jones, W; Juvela, M; Keihanen, E; Keskitalo, R; Kisner, T; Kneissl, R; Knox, L; Kurki Suonio, H; Lagache, G; Lamarre, J; Lanoux, J; Lasenby, A; Laureijs, R; Lawrence, C; Leach, S; Leonardi, R; Liddle, A; Lilje, P; Linden Vornle, M; Lopez Caniego, M; Lubin, P; Macias Perez, J; Mactavish, C; Maffei, B; Maino, D; Mandolesi, N; Mann, R; Maris, M; Marleau, F; Martinez Gonzalez, E; Masi, S; Matarrese, S; Matthai, F; Mazzotta, P; Melchiorri, A; Melin, J; Mendes, L; Mennella, A; Mitra, S; Miville Deschenes, M; Moneti, A; Montier, L; Morgante, G; Mortlock, D; Munshi, D; Murphy, A; Naselsky, P; Natoli, P; Netterfield, C; Norgaard Nielsen, H; Noviello, F; Novikov, D; Novikov, I; Osborne, S; Pajot, F; Pasian, F; Patanchon, G; 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, G; Prezeau, G; Prunet, S; Puget, J; Rachen, J; Rebolo, R; Reinecke, M; Renault, C; Ricciardi, S; Riller, T; Ristorcelli, I; Rocha, G; Rosset, C; Rubino Martin, J; Rusholme, B; Sandri, M; Santos, D; Savini, G; Schaefer, B; Scott, D; Seiffert, M; Shellard, P; Smoot, G; Starck, J; Stivoli, F; Stolyarov, V; Sudiwala, R; Sunyaev, R; Sygnet, J; Tauber, J; Terenzi, L; Toffolatti, L; Tomasi, M; Torre, J; Tristram, M; Tuovinen, J; Valenziano, L; Vibert, L; Vielva, P; Villa, F; Vittorio, N; Wade, L; Wandelt, B; White, S; White, M; Yvon, D; Zacchei, A; Zonca, A
Articolo su rivista
File in questo prodotto:
Non ci sono file associati a questo prodotto.

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2108/64148
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus 63
  • ???jsp.display-item.citation.isi??? 170
social impact