Issue |
A&A
Volume 571, November 2014
Planck 2013 results
|
|
---|---|---|
Article Number | A19 | |
Number of page(s) | 23 | |
Section | Cosmology (including clusters of galaxies) | |
DOI | https://doi.org/10.1051/0004-6361/201321526 | |
Published online | 29 October 2014 |
Planck 2013 results. XIX. The integrated Sachs-Wolfe effect
1 APC, AstroParticule et
Cosmologie,Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Observatoire de
Paris, Sorbonne Paris Cité, 10 rue
Alice Domon et Léonie Duquet, 75205
Paris Cedex 13,
France
2 Aalto University Metsähovi Radio
Observatory, Metsähovintie
114, 02540
Kylmälä,
Finland
3 African Institute for Mathematical
Sciences, 6−8 Melrose Road,
Muizenberg, 7945
Cape Town, South
Africa
4 Agenzia Spaziale Italiana Science
Data Center, via del Politecnico snc, 00133
Roma,
Italy
5 Agenzia Spaziale Italiana, Viale
Liegi 26, 00198
Roma,
Italy
6 Astrophysics Group, Cavendish
Laboratory, University of Cambridge, J J Thomson Avenue, Cambridge
CB3 0HE,
UK
7 Astrophysics & Cosmology Research
Unit, School of Mathematics, Statistics & Computer Science, University of
KwaZulu-Natal, Westville Campus,
Private Bag X54001, 4000
Durban, South
Africa
8 CITA, University of
Toronto, 60 St. George St.,
Toronto, ON
M5S 3H8,
Canada
9 CNRS, IRAP, 9 Av. colonel Roche, BP 44346, 31028
Toulouse Cedex 4,
France
10 California Institute of
Technology, Pasadena,
California,
USA
11 Centre for Theoretical Cosmology,
DAMTP, University of Cambridge, Wilberforce Road, Cambridge
CB3 0WA,
UK
12 Centro de Estudios de Física del
Cosmos de Aragón (CEFCA), Plaza San Juan 1, planta 2, 44001
Teruel,
Spain
13 Computational Cosmology Center,
Lawrence Berkeley National Laboratory, Berkeley, California, USA
14 Consejo Superior de Investigaciones
Científicas (CSIC), 28006
Madrid,
Spain
15 DSM/Irfu/SPP,
CEA-Saclay, 91191
Gif-sur-Yvette Cedex,
France
16 DTU Space, National Space
Institute, Technical University of Denmark, Elektrovej 327, 2800
Kgs. Lyngby,
Denmark
17 Département de Physique Théorique,
Université de Genève, 24 quai E.
Ansermet, 1211
Genève 4,
Switzerland
18 Departamento de Física Fundamental,
Facultad de Ciencias, Universidad de Salamanca, 37008
Salamanca,
Spain
19 Departamento de Física, Universidad
de Oviedo, Avda. Calvo Sotelo
s/n, 33007
Oviedo,
Spain
20 Department of Astronomy and
Astrophysics, University of Toronto, 50 Saint George Street, Toronto, Ontario,
Canada
21 Department of Astrophysics/IMAPP,
Radboud University Nijmegen, PO Box
9010, 6500 GL
Nijmegen, The
Netherlands
22 Department of Electrical
Engineering and Computer Sciences, University of California,
Berkeley, California,
USA
23 Department of Physics &
Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver,
British Columbia,
Canada
24 Department of Physics and
Astronomy, Dana and David Dornsife College of Letter, Arts and Sciences, University of
Southern California, Los
Angeles, CA
90089,
USA
25 Department of Physics and
Astronomy, University College London, London
WC1E 6BT,
UK
26 Department of Physics, Carnegie
Mellon University, 5000 Forbes
Ave, Pittsburgh,
PA
15213,
USA
27 Department of Physics, Florida
State University, Keen Physics
Building, 77 Chieftan Way, Tallahassee, Florida, USA
28 Department of Physics, Gustaf
Hällströmin katu 2a, University of Helsinki, 00014
Helsinki,
Finland
29 Department of Physics, Princeton
University, Princeton, New
Jersey, USA
30 Department of Physics, University
of California, Berkeley, California, USA
31 Department of Physics, University
of California, One Shields
Avenue, Davis,
California,
USA
32 Department of Physics, University
of California, Santa
Barbara, California, USA
33 Department of Physics, University
of Illinois at Urbana- Champaign, 1110 West Green Street, Urbana, Illinois,
USA
34 Dipartimento di Fisica e Astronomia
G. Galilei, Università degli Studi di Padova, via Marzolo 8, 35131
Padova,
Italy
35 Dipartimento di Fisica e Scienze
della Terra, Università di Ferrara, via Saragat 1, 44122
Ferrara,
Italy
36 Dipartimento di Fisica, Università
La Sapienza, P.le A. Moro
2, 00185
Roma,
Italy
37 Dipartimento di Fisica, Università
degli Studi di Milano, via Celoria,
16, 20133
Milano,
Italy
38 Dipartimento di Fisica, Università
degli Studi di Trieste, via A.
Valerio 2, 34127
Trieste,
Italy
39 Dipartimento di Fisica, Università
di Roma Tor Vergata, via della
Ricerca Scientifica, 1, 00133
Roma,
Italy
40 Discovery Center, Niels Bohr
Institute, Blegdamsvej
17, 2100
Copenhagen,
Denmark
41 Dpto. Astrofísica, Universidad de
La Laguna (ULL), 38206 La
Laguna, Tenerife,
Spain
42 European SpaceAgency, ESAC, Planck
Science Office, Camino bajo del Castillo s/n, Urbanización Villafranca del Castillo,
28692 Villanueva de la Cañada, Madrid, Spain
43 European Space Agency, ESTEC,
Keplerlaan 1, 2201
AZ
Noordwijk, The
Netherlands
44 Haverford College Astronomy
Department, 370 Lancaster
Avenue, Haverford,
Pennsylvania,
USA
45 Helsinki Institute of Physics,
Gustaf Hällströmin katu 2, University of Helsinki, 00014
Helsinki,
Finland
46 INAF − Osservatorio Astrofisico di
Catania, via S. Sofia 78, 95123
Catania,
Italy
47 INAF − Osservatorio Astronomico di
Padova, Vicolo dell’Osservatorio 5, Padova, Italy
48 INAF − Osservatorio Astronomico di
Roma, via di Frascati 33, Monte Porzio Catone, 00040
Rome,
Italy
49 INAF − Osservatorio Astronomico di
Trieste, via G.B. Tiepolo 11, 34143
Trieste,
Italy
50 INAF Istituto di Radioastronomia,
via P. Gobetti 101, 40129
Bologna,
Italy
51 INAF/IASF Bologna, via Gobetti
101, 40129
Bologna,
Italy
52 INAF/IASF Milano, via E. Bassini
15, 20133
Milano,
Italy
53 INFN, Sezione di Bologna, via
Irnerio 46, 40126
Bologna,
Italy
54 INFN, Sezione di Roma 1, Università
di Roma Sapienza, Piazzale Aldo
Moro 2, 00185
Roma,
Italy
55 INFN/National Institute for Nuclear
Physics, via Valerio
2, 34127
Trieste,
Italy
56 IPAG: Institut de Planétologie et
d’Astrophysique de Grenoble, Université Joseph Fourier, Grenoble 1/CNRS-INSU, UMR
5274, 38041
Grenoble,
France
57 IUCAA, Post Bag 4, Ganeshkhind,
Pune University Campus, Pune
411 007,
India
58 Imperial College London,
Astrophysics group, Blackett Laboratory, Prince Consort Road, London, SW7
2AZ, UK
59 Infrared Processing and Analysis
Center, California Institute of Technology, Pasadena, CA
91125,
USA
60 Institut Néel, CNRS, Université
Joseph Fourier Grenoble I, 25 rue
des Martyrs, 38042
Grenoble,
France
61 Institut Universitaire de
France, 103 bd
Saint-Michel, 75005
Paris,
France
62 Institut d’Astrophysique Spatiale,
CNRS (UMR 8617) Université Paris-Sud 11, Bâtiment 121, 91405
Orsay,
France
63 Institut d’Astrophysique de Paris,
CNRS (UMR 7095), 98bis boulevard
Arago, 75014
Paris,
France
64 Institut de Ciències de l’Espai,
CSIC/IEEC, Facultat de Ciències, Campus UAB, Torre C5 par-2, 08193
Bellaterra,
Spain
65 Institute for Space
Sciences, 76900
Bucharest-Magurale,
Romania
66 Institute of Astronomy and
Astrophysics, Academia Sinica, Taipei, Taiwan
67 Institute of Astronomy, University
of Cambridge, Madingley
Road, Cambridge
CB3 0HA,
UK
68 Institute of Theoretical
Astrophysics, University of Oslo, Blindern, 0315
Oslo,
Norway
69 Instituto de Astrofísica de
Canarias, C/Vía Láctea s/n, 38200
La Laguna, Tenerife, Spain
70 Instituto de Física de Cantabria
(CSIC-Universidad de Cantabria), Avda. de los Castros s/n, 39005
Santander,
Spain
71 Jet Propulsion Laboratory,
California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
72 Jodrell Bank Centre for
Astrophysics, Alan Turing Building, School of Physics and Astronomy, The University of
Manchester, Oxford
Road, Manchester,
M13 9PL,
UK
73 Kavli Institute for Cosmology
Cambridge, Madingley
Road, Cambridge,
CB3 0HA,
UK
74 LAL, Université Paris-Sud,
CNRS/IN2P3, 91898
Orsay,
France
75 LERMA, CNRS, Observatoire de Paris,
61 avenue de l’Observatoire, 75014
Paris,
France
76 Laboratoire AIM, IRFU/Service
d’Astrophysique − CEA/DSM − CNRS − Université Paris Diderot, Bât. 709,
CEA-Saclay, 91191
Gif-sur-Yvette Cedex,
France
77 Laboratoire Traitement et
Communication de l’Information, CNRS (UMR 5141) and Télécom ParisTech,
46 rue Barrault, 75634
Paris Cedex 13,
France
78 Laboratoire de Physique Subatomique
et de Cosmologie, Université Joseph Fourier Grenoble I, CNRS/IN2P3, Institut National
Polytechnique de Grenoble, 53 rue
des Martyrs, 38026
Grenoble Cedex,
France
79 Laboratoire de Physique Théorique,
Université Paris-Sud 11 & CNRS, Bâtiment 210, 91405
Orsay,
France
80 Lawrence Berkeley National
Laboratory, Berkeley,
California,
USA
81 Max-Planck-Institut für
Astrophysik, Karl-Schwarzschild-Str. 1, 85741
Garching,
Germany
82 McGill Physics, Ernest Rutherford
Physics Building, McGill University, 3600 rue University, Montréal, QC, H3A 2T8,
Canada
83 MilliLab, VTT Technical Research
Centre of Finland, Tietotie 3, 02044
Espoo,
Finland
84 Niels Bohr Institute,
Blegdamsvej 17, Copenhagen,
Denmark
85 Observational Cosmology, Mail
Stop367-17, California Institute of Technology, Pasadena, CA
91125,
USA
86 Optical Science Laboratory,
University College London, Gower
Street, London,
UK
87 SB-ITP-LPPC, EPFL,
1015
Lausanne,
Switzerland
88 SISSA, Astrophysics Sector, via
Bonomea 265, 34136
Trieste,
Italy
89 School of Physics and Astronomy,
Cardiff University, Queens
Buildings, The Parade, Cardiff, CF24
3AA, UK
90 School of Physics and Astronomy,
University of Nottingham, Nottingham
NG7 2RD,
UK
91 Space Research Institute (IKI),
Russian Academy of Sciences, Profsoyuznaya Str, 84/32, Moscow
117997,
Russia
92 Space Sciences Laboratory,
University of California, Berkeley, California, USA
93 Special Astrophysical Observatory,
Russian Academy of Sciences, Nizhnij Arkhyz, Zelenchukskiy region, 369167
Karachai-Cherkessian Republic,
Russia
94 Stanford University,
Dept of Physics, Varian Physics Bldg, 382 via
Pueblo Mall, Stanford, California, USA
95 Sub-Department of Astrophysics,
University of Oxford, Keble
Road, Oxford
OX1 3RH,
UK
96 Theory Division, PH-TH,
CERN, 1211
Geneva 23,
Switzerland
97 UPMC Univ. Paris 06, UMR
7095, 98bis boulevard
Arago, 75014
Paris,
France
98 Universität Heidelberg, Institut
für Theoretische Astrophysik, Philosophenweg 12, 69120
Heidelberg,
Germany
99 Université de
Toulouse, UPS-OMP,
IRAP, 31028
Toulouse Cedex 4,
France
100 University Observatory, Ludwig
Maximilian University of Munich, Scheinerstrasse 1, 81679
Munich,
Germany
101 University of Granada,
Departamento de Física Teórica y del Cosmos, Facultad de Ciencias,
18071
Granada,
Spain
102 Warsaw University
Observatory, Aleje Ujazdowskie
4, 00-478
Warszawa,
Poland
Received:
21
March
2013
Accepted:
25
November
2013
Based on cosmic microwave background (CMB) maps from the 2013 Planck Mission data release, this paper presents the detection of the integrated Sachs-Wolfe (ISW) effect, that is, the correlation between the CMB and large-scale evolving gravitational potentials. The significance of detection ranges from 2 to 4σ, depending on which method is used. We investigated three separate approaches, which essentially cover all previous studies, and also break new ground. (i) We correlated the CMB with the Planck reconstructed gravitational lensing potential (for the first time). This detection was made using the lensing-induced bispectrum between the low-ℓ and high-ℓ temperature anisotropies; the correlation between lensing and the ISW effect has a significance close to 2.5σ. (ii) We cross-correlated with tracers of large-scale structure, which yielded a significance of about 3σ, based on a combination of radio (NVSS) and optical (SDSS) data. (iii) We used aperture photometry on stacked CMB fields at the locations of known large-scale structures, which yielded and confirms a 4σ signal, over a broader spectral range, when using a previously explored catalogue, but shows strong discrepancies in amplitude and scale when compared with expectations. More recent catalogues give more moderate results that range from negligible to 2.5σ at most, but have a more consistent scale and amplitude, the latter being still slightly higher than what is expected from numerical simulations within ΛCMD. Where they can be compared, these measurements are compatible with previous work using data from WMAP, where these scales have been mapped to the limits of cosmic variance. Planck’s broader frequency coverage allows for better foreground cleaning and confirms that the signal is achromatic, which makes it preferable for ISW detection. As a final step we used tracers of large-scale structure to filter the CMB data, from which we present maps of the ISW temperature perturbation. These results provide complementary and independent evidence for the existence of a dark energy component that governs the currently accelerated expansion of the Universe.
Key words: cosmic background radiation / large-scale structure of Universe / dark energy / galaxies: clusters: general / methods: data analysis
© ESO, 2014
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