Planck Early Results: Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations

Planck Collaboration,P. A. R. Ade,N. Aghanim,M. Arnaud,M. Ashdown,J. Aumont,C. Baccigalupi,A. Balbi,A. J. Banday,R. B. Barreiro,M. Bartelmann,J. G. Bartlett,E. Battaner,K. Benabed,A. Benoît,J.-P. Bernard,M. Bersanelli,R. Bhatia,J. J. Bock,A. Bonaldi,J. R. Bond,J. Borrill,F. R. Bouchet,H. Bourdin,M. L. Brown,M. Bucher,C. Burigana,P. Cabella,J.-F. Cardoso,A. Catalano,L. Cayón,A. Challinor,A. Chamballu,L.-Y Chiang,C. Chiang,G. Chon,P. R. Christensen,E. Churazov,D. L. Clements,S. Colafrancesco,S. Colombi,F. Couchot,A. Coulais,B. P. Crill,F. Cuttaia,A. Da Silva,H. Dahle,L. Danese,P. de Bernardis,G. de Gasperis,A. de Rosa,G. de Zotti,J. Delabrouille,J.-M. Delouis,F.-X. Désert,J. M. Diego,K. Dolag,S. Donzelli,O. Doré,U. Dörl,M. Douspis,X. Dupac,G. Efstathiou,T. A. Ensslin,F. Finelli,I. Flores,O. Forni,M. Frailis,E. Franceschi,S. Fromenteau,S. Galeotta,K. Ganga,R. T. Génova-Santos,M. Giard,G. Giardino,Y. Giraud-Héraud,J. González-Nuevo,K. M. Górski,S. Gratton,A. Gregorio,A. Gruppuso,D. Harrison,S. Henrot-Versillé,C. Hernández-Monteagudo,D. Herranz,S. R. Hildebrandt,E. Hivon,M. Hobson,W. A. Holmes,W. Hovest,R. J. Hoyland,K. M. Huffenberger,A. H. Jaffe,W. C. Jones,M. Juvela,E. Keihänen,R. Keskitalo,T. S. Kisner,R. Kneissl,L. Knox,H. Kurki-Suonio,G. Lagache,J.-M. Lamarre, J. Lanoux,A. Lasenby,R. J. Laureijs,C. R. Lawrence,S. Leach,R. Leonardi,A. Liddle,P. B. Lilje,M. Linden-Vornle,M. López-Caniego,P. M. Lubin,J. F. Macías-Pérez,C. J. MacTavish,B. Maffei,D. Maino,N. Mandolesi,R. Mann,M. Maris,F. Marleau,E. Martínez-González,S. Masi,S. Matarrese,F. Matthai,P. Mazzotta,A. Melchiorri,J.-B. Melin,L. Mendes,A. Mennella,S. Mitra,M.-A. Miville-Deschênes,A. Moneti,L. Montier,G. Morgante,D. Mortlock,D. Munshi,A. Murphy,P. Naselsky,P. Natoli,C. B. Netterfield,H. U. Norgaard-Nielsen,F. Noviello,D. Novikov,I. Novikov,S. Osborne,F. Pajot,F. Pasian,G. Patanchon,O. Perdereau,L. Perotto,F. Perrotta,F. Piacentini,M. Piat,E. Pierpaoli,R. Piffaretti,S. Plaszczynski,E. Pointecouteau,G. Polenta,N. Ponthieu,T. Poutanen,G. W. Pratt,G. Prézeau,S. Prunet,J.-L. Puget,J. P. Rachen,R. Rebolo,M. Reinecke,C. Renault,S. Ricciardi,T. Riller,I. Ristorcelli,G. Rocha,C. Rosset,J. A. Rubiño-Martín,B. Rusholme,M. Sandri,D. Santos,G. Savini,B. M. Schaefer,D. Scott,M. D. Seiffert,P. Shellard,G. F. Smoot,J.-L. Starck,F. Stivoli,V. Stolyarov,R. Sudiwala,R. Sunyaev,J.-F. Sygnet,J. A. Tauber,L. Terenzi,L. Toffolatti,M. Tomasi,J.-P. Torre,M. Tristram,J. Tuovinen,L. Valenziano,L. Vibert,P. Vielva,F. Villa,N. Vittorio,L. A. Wade,B. D. Wandelt, S. D. M. White,M. White,D. Yvon,A. Zacchei,A. Zonca

msra(2011)

引用 186|浏览67
暂无评分
摘要
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 dataset. The sample spans approximately a decade in total mass, 10^14 < M_500 < 10^15, 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,500, temperature T_X, luminosity L_X, SZ signal analogue Y_X,500 = M_g,500 * 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.
更多
查看译文
AI 理解论文
溯源树
样例
生成溯源树,研究论文发展脉络
Chat Paper
正在生成论文摘要