Issue |
A&A
Volume 536, December 2011
Planck early results
|
|
---|---|---|
Article Number | A18 | |
Number of page(s) | 30 | |
Section | Cosmology (including clusters of galaxies) | |
DOI | https://doi.org/10.1051/0004-6361/201116461 | |
Published online | 01 December 2011 |
Planck early results. XVIII. The power spectrum of cosmic infrared background anisotropies⋆
1
Aalto University Metsähovi Radio Observatory, Metsähovintie 114, 02540 Kylmälä, Finland
2
Agenzia Spaziale Italiana Science Data Center, c/o ESRIN, via Galileo Galilei, Frascati, Italy
3
Astroparticule et Cosmologie, CNRS (UMR7164), Université Denis Diderot Paris 7, Bâtiment Condorcet, 10 rue A. Domon et Léonie Duquet, Paris, France
4
Astrophysics Group, Cavendish Laboratory, University of Cambridge, J J Thomson Avenue, Cambridge CB3 0HE, UK
5
Atacama Large Millimeter/submillimeter Array, ALMA Santiago Central Offices, Alonso de Cordova 3107, Vitacura, Casilla 763 0355, Santiago, Chile
6
Australia Telescope National Facility, CSIRO, P.O. Box 76, Epping, NSW 1710, Australia
7
CITA, University of Toronto, 60 St. George St., Toronto, ON M5S 3H8, Canada
8
CNRS, IRAP, 9 Av. Colonel Roche, BP 44346, 31028 Toulouse Cedex 4, France
9
California Institute of Technology, Pasadena, California, USA
10 Centre of Mathematics for Applications, University of Oslo, Blindern, Oslo, Norway
11
DAMTP, University of Cambridge, Centre for Mathematical Sciences, Wilberforce Road, Cambridge CB3 0WA, UK
12
DSM/Irfu/SPP, CEA-Saclay, 91191 Gif-sur-Yvette Cedex, France
13
DTU Space, National Space Institute, Juliane Mariesvej 30, Copenhagen, Denmark
14
Departamento de Física, Universidad de Oviedo, Avda. Calvo Sotelo s/n, Oviedo, Spain
15
Department of Astronomy and Astrophysics, University of Toronto, 50 Saint George Street, Toronto, Ontario, Canada
16
Department of Physics & Astronomy, University of BritishColumbia, 6224 Agricultural Road, Vancouver, British Columbia, Canada
17
Department of Physics and Astronomy, University of Sussex, Brighton BN1 9QH, UK
18
Department of Physics, Gustaf Hällströmin katu 2a, University of Helsinki, Helsinki, Finland
19
Department of Physics, Princeton University, Princeton, New Jersey, USA
20
Department of Physics, Purdue University, 525 Northwestern Avenue, West Lafayette, Indiana, USA
21
Department of Physics, University of California, Berkeley, California, USA
22
Department of Physics, University of California, One Shields Avenue, Davis, California, USA
23
Department of Physics, University of California, Santa Barbara, California, USA
24
Department of Physics, University of Illinois at Urbana-Champaign, 1110 West Green Street, Urbana, Illinois, USA
25
Dipartimento di Fisica G. Galilei, Università degli Studi di Padova, via Marzolo 8, 35131 Padova, Italy
26
Dipartimento di Fisica, Università La Sapienza, P. le A. Moro 2, Roma, Italy
27
Dipartimento di Fisica, Università degli Studi di Milano, via Celoria, 16, Milano, Italy
28
Dipartimento di Fisica, Università degli Studi di Trieste, via A. Valerio 2, Trieste, Italy
29
Dipartimento di Fisica, Università di Ferrara, via Saragat 1, 44122 Ferrara, Italy
30
Dipartimento di Fisica, Università di Roma Tor Vergata, via della Ricerca Scientifica, 1, Roma, Italy
31
Discovery Center, Niels Bohr Institute, Blegdamsvej 17, Copenhagen, Denmark
32
Dpto. Astrofísica, Universidad de La Laguna (ULL), 38206 La Laguna, Tenerife, Spain
33
European Southern Observatory, ESO Vitacura, Alonso de Cordova 3107, Vitacura, Casilla 19001, Santiago, Chile
34
European Space Agency, ESAC, Planck Science Office, Camino bajo del Castillo, s/n, Urbanización Villafranca del Castillo, Villanueva de la Cañada, Madrid, Spain
35
European Space Agency, ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands
36
Helsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, Helsinki, Finland
37
INAF – Osservatorio Astrofisico di Catania, via S. Sofia 78, Catania, Italy
38
INAF – Osservatorio Astronomico di Padova, vicolo dell’Osservatorio 5, Padova, Italy
39
INAF – Osservatorio Astronomico di Roma, via di Frascati 33, Monte Porzio Catone, Italy
40
INAF – Osservatorio Astronomico di Trieste, via G.B. Tiepolo 11, Trieste, Italy
41
INAF/IASF Bologna, via Gobetti 101, Bologna, Italy
42
INAF/IASF Milano, via E. Bassini 15, Milano, Italy
43
INRIA, Laboratoire de Recherche en Informatique, Université Paris-Sud 11, Bâtiment 490, 91405 Orsay Cedex, France
44
IPAG: Institut de Planétologie et d’Astrophysique de Grenoble, Université Joseph Fourier, Grenoble 1/CNRS-INSU, UMR 5274, 38041 Grenoble, France
45
Imperial College London, Astrophysics group, Blackett Laboratory, Prince Consort Road, London, SW7 2AZ, UK
46
Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125, USA
47
Institut Néel, CNRS, Université Joseph Fourier Grenoble I, 25 rue des Martyrs, Grenoble, France
48
Institut d’Astrophysique Spatiale, CNRS (UMR8617) Université Paris-Sud 11, Bâtiment 121, Orsay, France
49
Institut d’Astrophysique de Paris, CNRS UMR7095, Université Pierre & Marie Curie, 98bis boulevard Arago, Paris, France
50
Institut de Ciències de l’Espai, CSIC/IEEC, Facultat de Ciències, Campus UAB, Torre C5 par-2, Bellaterra 08193, Spain
51
Institute of Astronomy and Astrophysics, Academia Sinica, Taipei, Taiwan
52
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
53 Institute of Theoretical Astrophysics, University of Oslo, Blindern, Oslo, Norway
54
Instituto de Astrofísica de Canarias, C/Vía Láctea s/n, La Laguna, Tenerife, Spain
55
Instituto de Física de Cantabria (CSIC-Universidad de Cantabria), Avda. de los Castros s/n, Santander, Spain
56
Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
57
Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester, M13 9PL, UK
58
Kavli Institute for Cosmology Cambridge, Madingley Road, Cambridge, CB3 0HA, UK
59
LERMA, CNRS, Observatoire de Paris, 61 avenue de l’Observatoire, Paris, France
60
Laboratoire AIM, IRFU/Service d’Astrophysique – CEA/DSM – CNRS – Université Paris Diderot, Bât. 709, CEA-Saclay, 91191 Gif-sur-Yvette Cedex, France
61
Laboratoire Traitement et Communication de l’Information, CNRS (UMR 5141) and Télécom ParisTech, 46 rue Barrault, 75634 Paris Cedex 13, France
62
Laboratoire de Physique Subatomique et de Cosmologie, CNRS/IN2P3, Université Joseph Fourier Grenoble I, Institut National Polytechnique de Grenoble, 53 rue des Martyrs, 38026 Grenoble Cedex, France
63
Laboratoire de l’Accélérateur Linéaire, Université Paris-Sud 11, CNRS/IN2P3, Orsay, France
64
Lawrence Berkeley National Laboratory, Berkeley, California, USA
65
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741 Garching, Germany
66
MilliLab, VTT Technical Research Centre of Finland, Tietotie 3, Espoo, Finland
67
NRAO, P.O. Box 2, Rt 28/92, Green Bank, WV 24944-0002, USA
68
National University of Ireland, Department of Experimental Physics, Maynooth, Co. Kildare, Ireland
69
Niels Bohr Institute, Blegdamsvej 17, Copenhagen, Denmark
70
Observational Cosmology, Mail Stop 367-17, California Institute of Technology, Pasadena, CA, 91125, USA
71
Optical Science Laboratory, University College London, Gower Street, London, UK
72
SISSA, Astrophysics Sector, via Bonomea 265, 34136, Trieste, Italy
73
SUPA, Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK
74
School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
75
Space Research Institute (IKI), Russian Academy of Sciences, Profsoyuznaya Str, 84/32, Moscow, 117997, Russia
76
Space Sciences Laboratory, University of California, Berkeley, California, USA
77
Stanford University, Dept of Physics, Varian Physics Bldg, 382 via Pueblo Mall, Stanford, California, USA
78
Université de Toulouse, UPS-OMP, IRAP, 31028 Toulouse Cedex 4, France
79
Universities Space Research Association, Stratospheric Observatory for Infrared Astronomy, MS 211-3, Moffett Field, CA 94035, USA
80
University of Granada, Departamento de Física Teórica y del Cosmos, Facultad de Ciencias, Granada, Spain
81
University of Miami, Knight Physics Building, 1320 Campo Sano Dr., Coral Gables, Florida, USA
82
Warsaw University Observatory, Aleje Ujazdowskie 4, 00-478 Warszawa, Poland
Received: 7 January 2011
Accepted: 17 June 2011
Using Planck maps of six regions of low Galactic dust emission with a total area of about 140 deg2, we determine the angular power spectra of cosmic infrared background (CIB) anisotropies from multipole ℓ = 200 to ℓ = 2000 at 217, 353, 545 and 857 GHz. We use 21-cm observations of Hi as a tracer of thermal dust emission to reduce the already low level of Galactic dust emission and use the 143 GHz Planck maps in these fields to clean out cosmic microwave background anisotropies. Both of these cleaning processes are necessary to avoid significant contamination of the CIB signal. We measure correlated CIB structure across frequencies. As expected, the correlation decreases with increasing frequency separation, because the contribution of high-redshift galaxies to CIB anisotropies increases with wavelengths. We find no significant difference between the frequency spectrum of the CIB anisotropies and the CIB mean, with ΔI / I = 15% from 217 to 857 GHz. In terms of clustering properties, the Planck data alone rule out the linear scale- and redshift-independent bias model. Non-linear corrections are significant. Consequently, we develop an alternative model that couples a dusty galaxy, parametric evolution model with a simple halo-model approach. It provides an excellent fit to the measured anisotropy angular power spectra and suggests that a different halo occupation distribution is required at each frequency, which is consistent with our expectation that each frequency is dominated by contributions from different redshifts. In our best-fit model, half of the anisotropy power at ℓ = 2000 comes from redshifts z < 0.8 at 857 GHz and z < 1.5 at 545 GHz, while about 90% come from redshifts z > 2 at 353 and 217 GHz, respectively.
Key words: diffuse radiation / submillimeter: diffuse background / submillimeter: galaxies / cosmology: observations
© ESO, 2011
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