Planck early results. VIII. The all-sky early Sunyaev-Zeldovich cluster sample

被引:319
作者
Ade, P. A. R. [74 ]
Aghanim, N. [1 ]
Arnaud, M. [60 ]
Ashdown, M. [5 ,58 ]
Aumont, J. [1 ]
Baccigalupi, C. [72 ]
Balbi, A. [31 ]
Banday, A. J. [8 ,67 ,81 ]
Barreiro, R. B. [55 ]
Bartelmann, M. [67 ,80 ]
Bartlett, J. G. [56 ]
Battaner, E. [84 ]
Battye, R. [57 ]
Benabed, K. [49 ]
Benoit, A. [48 ]
Bernard, J-P [8 ,81 ]
Bersanelli, M. [28 ,43 ]
Bhatia, R. [6 ]
Bock, J. J. [56 ]
Bonaldi, A. [39 ]
Bond, J. R. [7 ]
Borrill, J. [65 ,76 ]
Bouchet, F. R. [49 ]
Brown, M. L. [5 ,58 ]
Bucher, M. [4 ]
Burigana, C. [42 ]
Cabella, P. [31 ]
Cantalupo, C. M. [65 ]
Cardoso, J-F [49 ,61 ,62 ]
Carvalho, P. [5 ]
Catalano, A. [59 ]
Cayon, L. [21 ]
Challinor, A. [11 ,52 ,58 ]
Chamballu, A. [46 ]
Chary, R-R [47 ]
Chiang, L-Y [51 ]
Chiang, C. [20 ]
Chon, G. [5 ,68 ]
Christensen, P. R. [32 ]
Churazov, E. [67 ,75 ]
Clements, D. L. [46 ]
Colafrancesco, S. [40 ]
Colombi, S. [49 ]
Couchot, F. [64 ]
Coulais, A. [59 ]
Crill, B. P. [56 ]
Cuttaia, F. [42 ]
Da Silva, A. [10 ]
Dahle, H. [9 ,53 ]
Danese, L. [72 ]
机构
[1] Univ Paris 11, CNRS, Inst Astrophys Spatiale, UMR8617, Batiment 121, F-91405 Orsay, France
[2] Aalto Univ Metsahovi Radio Observ, Kylmala 02540, Finland
[3] ESRIN, Agenzia Spaziale Italiana Sci Data Ctr, Frascati, Italy
[4] Univ Paris 07, CNRS, UMR7164, F-75205 Paris 13, France
[5] Univ Cambridge, Cavendish Lab, Astrophys Grp, Cambridge CB3 0HE, England
[6] ALMA Santiago Cent Off, Santiago, Chile
[7] Univ Toronto, CITA, Toronto, ON M5S 3H8, Canada
[8] IRAP, CNRS, F-31028 Toulouse 4, France
[9] Univ Oslo, Ctr Math Applicat, Oslo, Norway
[10] Univ Porto, Ctr Astrofis, P-4150762 Oporto, Portugal
[11] Univ Cambridge, DAMTP, Ctr Math Sci, Cambridge CB3 0WA, England
[12] CEA Saclay, DSM Irfu SPP, F-91191 Gif Sur Yvette, France
[13] Natl Space Inst, DTU Space, Copenhagen, Denmark
[14] Univ Oviedo, Dept Fis, E-33007 Oviedo, Spain
[15] Univ Toronto, Dept Astron & Astrophys, Toronto, ON M5S 3H8, Canada
[16] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V5Z 1M9, Canada
[17] Univ So Calif, Dept Phys & Astron, Los Angeles, CA USA
[18] Univ Sussex, Dept Phys & Astron, Brighton BN1 9QH, E Sussex, England
[19] Univ Helsinki, Dept Phys, Helsinki, Finland
[20] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA
[21] Purdue Univ, Dept Phys, W Lafayette, IN 47907 USA
[22] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
[23] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA
[24] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA
[25] Univ Illinois, Dept Phys, Urbana, IL USA
[26] Univ Padua, Dipartimento Fis G Galilei, I-35131 Padua, Italy
[27] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy
[28] Univ Milan, Dipartimento Fis, Milan, Italy
[29] Univ Trieste, Dipartimento Fis, Trieste, Italy
[30] Univ Ferrara, Dipartimento Fis, I-44122 Ferrara, Italy
[31] Univ Roma Tor Vergata, Dipartimento Fis, I-00173 Rome, Italy
[32] Niels Bohr Inst, Discovery Ctr, DK-2100 Copenhagen, Denmark
[33] Univ La Laguna, Dpto Astrofis, E-38206 Tenerife, Spain
[34] European So Observ, ESO Vitacura, Santiago 19, Chile
[35] European Space Agcy, Planck Sci Off, ESAC, Madrid, Spain
[36] European Space Agcy, ESTEC, NL-2201 AZ Noordwijk, Netherlands
[37] Observ Paris, GEPI, Sect Meudon, F-92195 Meudon, France
[38] Aalto Univ, Univ Helsinki, Helsinki Inst Phys, Helsinki, Finland
[39] Osserv Astron Padova, INAF, Padua, Italy
[40] Osserv Astron Roma, INAF, I-00040 Monte Porzio Catone, Italy
[41] Osserv Astron Trieste, INAF, I-34131 Trieste, Italy
[42] IASF Bologna, INAF, Bologna, Italy
[43] IASF Milano, INAF, Milan, Italy
[44] Univ Paris 11, INRIA, Rech Informat Lab, F-91405 Orsay, France
[45] Univ Grenoble 1, CNRS, IPAG, INSU,UMR 5274, F-38041 Grenoble, France
[46] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Astrophys Grp, London SW7 2AZ, England
[47] CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA
[48] Univ Grenoble 1, CNRS, Inst Neel, F-38041 Grenoble, France
[49] Univ Paris 06, CNRS, Inst Astrophys Paris, UMR7095, Paris, France
[50] Fac Ciencies, CSIC IEEC, Inst Ciencies Espai, Bellaterra 08193, Spain
基金
美国国家航空航天局;
关键词
cosmology: observations; galaxies: clusters: general; catalogs; MICROWAVE BACKGROUND TEMPERATURE; X-RAY-PROPERTIES; MASSIVE GALAXY CLUSTERS; COSMIC DISTANCE SCALE; HYDRODYNAMICAL SIMULATIONS; NEARBY CLUSTERS; HUBBLE CONSTANT; COSMOLOGY; CATALOG; CALIBRATION;
D O I
10.1051/0004-6361/201116459
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
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