Planck 2015 results XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation

被引:95
作者
Ade, P. A. R. [84 ]
Aghanim, N. [58 ]
Arnaud, M. [72 ]
Aumont, J. [58 ]
Baccigalupi, C. [83 ]
Banday, A. J. [9 ,91 ]
Barreiro, R. B. [63 ]
Bartlett, J. G. [1 ,65 ]
Bartolo, N. [27 ,64 ]
Battaner, E. [92 ,93 ]
Benabed, K. [59 ,90 ]
Benoit-Levy, A. [21 ,59 ,90 ]
Bernard, J. -P. [9 ,91 ]
Bersanelli, M. [30 ,48 ]
Bielewicz, P. [9 ,80 ,83 ]
Bock, J. J. [10 ,65 ]
Bonaldi, A. [66 ]
Bonavera, L. [63 ]
Bond, J. R. [8 ]
Borrill, J. [12 ,87 ]
Bouchet, F. R. [59 ,85 ]
Burigana, C. [28 ,44 ,47 ]
Butler, R. C. [47 ]
Calabrese, E. [89 ]
Catalano, A. [71 ,73 ]
Chamballu, A. [13 ,58 ,72 ]
Chiang, H. C. [6 ,24 ]
Christensen, P. R. [33 ,81 ]
Churazov, E. [78 ,86 ]
Clements, D. L. [55 ]
Colombo, L. P. L. [20 ,65 ]
Combet, C. [73 ]
Comis, B. [73 ]
Couchot, F. [70 ]
Coulais, A. [71 ]
Crill, B. P. [10 ,65 ]
Curto, A. [5 ,63 ,68 ]
Cuttaia, F. [47 ]
Danese, L. [83 ]
Davies, R. D. [66 ]
Davis, R. J. [66 ]
de Bernardis, P. [29 ]
de Rosa, A. [47 ]
de Zotti, G. [44 ,83 ]
Delabrouille, J. [1 ]
Dickinson, C. [66 ]
Diego, J. M. [63 ]
Dole, H. [57 ,58 ]
Donzelli, S. [48 ]
Dore, O. [10 ,65 ]
机构
[1] Univ Paris Diderot, APC AstroParticule & Cosmol, CNRS IN2P3, CEA Irfu,Observ Paris,Sorbonne Paris Cite, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France
[2] African Inst Math Sci, 6-8 Melrose Rd, Cape Town, South Africa
[3] Agenzia Spaziale Italiana Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy
[4] Aix Marseille Univ, CNRS, LAM Lab Astrophys Marseille, UMR 7326, F-13388 Marseille, France
[5] Univ Cambridge, Cavendish Lab, Astrophys Grp, JJ Thomson Ave, Cambridge CB3 0HE, England
[6] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, Westville Campus,Private Bag X54001, ZA-4000 Durban, South Africa
[7] ALMA Santiago Cent Off, Atacama Large Millimeter Submillimeter Array, Alonso de Cordova 3107,Vitacura,Casilla 763 0355, Santiago, Chile
[8] Univ Toronto, CITA, 60 St George St, Toronto, ON M5S 3H8, Canada
[9] CNRS, IRAP, 9 Av Colonel Roche,BP 44346, F-31028 Toulouse 4, France
[10] CALTECH, Pasadena, CA 91125 USA
[11] CEFCA, Plaza San Juan,1 Planta 2, Teruel 44001, Spain
[12] Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA USA
[13] CEA Saclay, DSM Irfu SPP, F-91191 Gif Sur Yvette, France
[14] Tech Univ Denmark, Natl Space Inst, DTU Space, Elektrovej 327, DK-2800 Lyngby, Denmark
[15] Univ Geneva, Dept Phys Theor, 24 Quai Ansermet, CH-1211 Geneva 4, Switzerland
[16] Univ La Laguna ULL, Dept Astrofis, San Cristobal la Laguna 38206, Tenerife, Spain
[17] Univ Oviedo, Dept Fis, Avda Calvo Sotelo S-N, Oviedo, Spain
[18] Radboud Univ Nijmegen, IMAPP, Dept Astrophys, POB 9010, NL-6500 GL Nijmegen, Netherlands
[19] Univ British Columbia, Dept Phys & Astron, 6224 Agr Rd, Vancouver, BC, Canada
[20] Univ Southern Calif, Dept Phys & Astron, Dana & David Dornsife Coll Letter Arts & Sci, Los Angeles, CA 90089 USA
[21] UCL, Dept Phys & Astron, London WC1E 6BT, England
[22] Florida State Univ, Dept Phys, Keen Phys Bldg,77 Chieftan Way, Tallahassee, FL 32306 USA
[23] Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2a, Helsinki 00560, Finland
[24] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA
[25] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA
[26] Univ Illinois, Dept Phys, 1110 W Green St, Urbana, IL USA
[27] Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy
[28] Univ Ferrara, Dipartimento Fis & Sci Terra, Via Saragat 1, I-44122 Ferrara, Italy
[29] Univ Roma La Sapienza, Dipartimento Fis, Ple A Moro 2, I-00133 Rome, Italy
[30] Univ Milan, Dipartimento Fis, Via Celoria 16, I-20133 Milan, Italy
[31] Univ Trieste, Dipartimento Fis, Via A Valerio 2, I-34127 Trieste, Italy
[32] Univ Roma Tor Vergata, Dipartimento Matemat, Via Ric Sci 1, I-00133 Rome, Italy
[33] Niels Bohr Inst, Discovery Ctr, Blegdamsvej 17, Copenhagen, Denmark
[34] European Southern Observ ESO Vitacura, Alonso de Cordova 3107,Vitacura,Casilla 19001, Santiago, Chile
[35] European Space Agcy ESAC, Planck Sci Off, Camino Bajo del Castillo S-N, Madrid 28692, Spain
[36] ESTEC, European Space Agcy, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands
[37] Univ E Campus, Fac Ingn, Via Isimbardi 10, I-22060 Novedrate, CO, Italy
[38] INFN, Gran Sasso Sci Inst, Viale F Crispi 7, I-67100 Laquila, Italy
[39] HGSFP, Philosophenweg 16, D-69120 Heidelberg, Germany
[40] Heidelberg Univ, Dept Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany
[41] Haverford Coll, Dept Astron, 370 Lancaster Ave, Haverford, PA 19041 USA
[42] Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, Helsinki 00560, Finland
[43] INAF, Osservatorio Astrofis Catania, Via S Sofia 78, Catania, Italy
[44] INAF, Osservatorio Astron Padova, Vicolo Osservatorio 5, Padua, Italy
[45] INAF, Osservatorio Astron Roma, Via Frascati 33, Monte Porzio Catone, Italy
[46] INAF, Osservatorio Astron Trieste, Via GB Tiepolo 11, Trieste, Italy
[47] IASF Bologna, INAF, Via Gobetti 101, I-40127 Bologna, Italy
[48] IASF Milano, INAF, Via E Bassini 15, I-20133 Milan, Italy
[49] INFN, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy
[50] Univ Roma Sapienza, INFN, Sez Roma 1, Ple Aldo Moro 2, I-00185 Rome, Italy
基金
美国国家科学基金会;
关键词
galaxies: clusters: general; infrared: galaxies; large-scale structure of Universe; methods: data analysis; ANGULAR POWER SPECTRUM; GALAXY CLUSTER; STAR-FORMATION; SUBMILLIMETER GALAXIES; COSMOLOGY; CONSTRAINTS; ANISOTROPIES; MODEL; PROFILES; CATALOG;
D O I
10.1051/0004-6361/201527418
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We use Planck data to detect the cross-correlation between the thermal Sunyaev-Zeldovich (tSZ) effect and the infrared emission from the galaxies that make up the the cosmic infrared background (CIB). We first perform a stacking analysis towards Planck-confirmed galaxy clusters. We detect infrared emission produced by dusty galaxies inside these clusters and demonstrate that the infrared emission is about 50% more extended than the tSZ effect. Modelling the emission with a Navarro-Frenk-White profile, we find that the radial profile concentration parameter is c(500) = 1.00(-0.15)(+0.18). This indicates that infrared galaxies in the outskirts of clusters have higher infrared flux than cluster-core galaxies. We also study the cross-correlation between tSZ and CIB anisotropies, following three alternative approaches based on power spectrum analyses: (i) using a catalogue of confirmed clusters detected in Planck data; (ii) using an all-sky tSZ map built from Planck frequency maps; and (iii) using cross-spectra between Planck frequency maps. With the three different methods, we detect the tSZ-CIB cross-power spectrum at significance levels of (i) 6 sigma; (ii) 3 sigma; and (iii) 4 sigma. We model the tSZ-CIB cross-correlation signature and compare predictions with the measurements. The amplitude of the cross-correlation relative to the fiducial model is A(tSZ-CIB) = 1.2 +/- 0.3. This result is consistent with predictions for the tSZ-CIB cross-correlation assuming the best-fit cosmological model from Planck 2015 results along with the tSZ and CIB scaling relations.
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页数:17
相关论文
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