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

被引：92

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

来源：

ASTRONOMY & ASTROPHYSICS | 2016年 / 594卷

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.

引用

页数：17

共 37 条

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PHYSICAL REVIEW D, 2014, 89 (02)
[32] Simple halo model formalism for the cosmic infrared background and its correlation with the thermal Sunyaev-Zel'dovich effect
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ASTRONOMY & ASTROPHYSICS, 2021, 645
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