Issue |
A&A
Volume 594, October 2016
Planck 2015 results
|
|
---|---|---|
Article Number | A21 | |
Number of page(s) | 30 | |
Section | Cosmology (including clusters of galaxies) | |
DOI | https://doi.org/10.1051/0004-6361/201525831 | |
Published online | 20 September 2016 |
Planck 2015 results
XXI. 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 and Dept of Radio Science and Engineering, PO Box 13000, 00076 Aalto, 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 Aix Marseille Université, CNRS, LAM (Laboratoire d’Astrophysique de Marseille) UMR 7326, 13388 Marseille, France
6 Aix Marseille Université, Centre de Physique Théorique, 163 Avenue de Luminy, 13288 Marseille, France
7 Astrophysics Group, Cavendish Laboratory, University of Cambridge, J J Thomson Avenue, Cambridge CB3 0HE, UK
8 Astrophysics & Cosmology Research Unit, School of Mathematics, Statistics & Computer Science, University of KwaZulu-Natal, Westville Campus, Private Bag X54001, 4000 Durban, South Africa
9 Atacama Large Millimeter/submillimeter Array, ALMA Santiago Central Offices, Alonso de Cordova 3107, Vitacura, Casilla 763 0355, Santiago, Chile
10 CGEE, SCS Qd 9, Lote C, Torre C, 4° andar, Ed. Parque Cidade Corporate, CEP 70308-200, Brasília, DF, Brazil
11 CITA, Universityof Toronto, 60 St. George St., Toronto, ON M5S 3H8, Canada
12 CNRS, IRAP, 9 Av. colonel Roche, BP 44346, 31028 Toulouse Cedex 4, France
13 CRANN, Trinity College, Dublin 2, Ireland
14 California Institute of Technology, Pasadena, California, CA 91125, USA
15 Centre for Theoretical Cosmology, DAMTP, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, UK
16 Centro de Estudios de Física del Cosmos de Aragón (CEFCA), Plaza San Juan, 1, planta 2, 44001 Teruel, Spain
17 Computational Cosmology Center, Lawrence Berkeley National Laboratory, Berkeley, California, CA 94720, USA
18 Consejo Superior de Investigaciones Científicas (CSIC), Madrid, Spain
19 DSM/Irfu/SPP, CEA-Saclay, 91191 Gif-sur-Yvette Cedex, France
20 DTU Space, National Space Institute, Technical University of Denmark, Elektrovej 327, 2800 Kgs. Lyngby, Denmark
21 Département de Physique Théorique, Université de Genève, 24, Quai E. Ansermet, 1211 Genève 4, Switzerland
22 Departamento de Astrofísica, Universidad de La Laguna (ULL), 38206 La Laguna, Tenerife, Spain
23 Departamento de Física, Universidad de Oviedo, Avda. Calvo Sotelo s/n, 33007 Oviedo, Spain
24 Department of Astronomy and Astrophysics, University of Toronto, 50 Saint George Street, Toronto, Ontario, Canada
25 Department of Astrophysics/IMAPP, Radboud University Nijmegen, PO Box 9010, 6500 GL Nijmegen, The Netherlands
26 Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, British Columbia, Canada
27 Department of Physics and Astronomy, Dana and David Dornsife College of Letter, Arts and Sciences, University of Southern California, Los Angeles, CA 90089, USA
28 Department of Physics and Astronomy, University College London, London WC1E 6BT, UK
29 Department of Physics, Florida State University, Keen Physics Building, 77 Chieftan Way, Tallahassee, Florida, USA
30 Department of Physics, Gustaf Hällströmin katu 2a, University of Helsinki, 00560 Helsinki, Finland
31 Department of Physics, Princeton University, Princeton, New Jersey, 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, 00133 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 Matematica, Università di Roma Tor Vergata, via della Ricerca Scientifica, 1, 00133 Roma, Italy
40 Discovery Center, Niels Bohr Institute, Blegdamsvej 17, 1165 Copenhagen, Denmark
41 Discovery Center, Niels Bohr Institute, Copenhagen University, Blegdamsvej 17, 1165 Copenhagen, Denmark
42 European Southern Observatory, ESO Vitacura, Alonso de Cordova 3107, Vitacura, Casilla 19001, Santiago, Chile
43 European Space Agency, ESAC, Planck Science Office, Camino bajo del Castillo, s/n, Urbanización Villafranca del Castillo, 28691 Villanueva de la Cañada, Madrid, Spain
44 European Space Agency, ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands
45 Gran Sasso Science Institute, INFN, viale F. Crispi 7, 67100 L’ Aquila, Italy
46 HGSFP and University of Heidelberg, Theoretical Physics Department, Philosophenweg 16, 69120 Heidelberg, Germany
47 Helsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, 00560 Helsinki, Finland
48 INAF−Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, 35131 Padova, Italy
49 INAF−Osservatorio Astronomico di Roma, via di Frascati 33, Monte Porzio Catone, Italy
50 INAF−Osservatorio Astronomico di Trieste, via G.B. Tiepolo 11, 34127 Trieste, Italy
51 INAF/IASF Bologna, via Gobetti 101, 40127 Bologna, Italy
52 INAF/IASF Milano, via E. Bassini 15, 20133 Milano, Italy
53 INFN, Sezione di Bologna, viale Berti Pichat 6/2, 40127 Bologna, Italy
54 INFN, Sezione di Ferrara, via Saragat 1, 44122 Ferrara, Italy
55 INFN, Sezione di Roma 1, Università di Roma Sapienza, Piazzale Aldo Moro 2, 00185 Roma, Italy
56 INFN, Sezione di Roma 2, Università di Roma Tor Vergata, via della Ricerca Scientifica, 1, 00185 Roma, Italy
57 INFN/National Institute for Nuclear Physics, via Valerio 2, 34127 Trieste, Italy
58 IPAG: Institut de Planétologie et d’Astrophysique de Grenoble, Université Grenoble Alpes, IPAG; CNRS, IPAG, 38000 Grenoble, France
59 IUCAA, Post Bag 4, Ganeshkhind, Pune University Campus, 411 007 Pune, India
60 Imperial CollegeLondon, Astrophysics group, Blackett Laboratory, Prince Consort Road, London, SW7 2AZ, UK
61 Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125, USA
62 Institut Néel, CNRS, Université Joseph Fourier Grenoble I, 25 rue des Martyrs, 38000 Grenoble, France
63 Institut Universitaire de France, 103, bd Saint-Michel, 75005 Paris, France
64 Institut d’Astrophysique Spatiale, CNRS, Univ. Paris-Sud, Université Paris-Saclay, Bât. 121, 91405 Orsay Cedex, France
65 Institut d’Astrophysique de Paris, CNRS (UMR7095), 98bis Boulevard Arago, 75014, Paris, France
66 Institut für Theoretische Teilchenphysik und Kosmologie, RWTH Aachen University, 52056 Aachen, Germany
67 Institute for Space Sciences, Bucharest-Magurale, Romania
68 Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
69 Institute of Theoretical Astrophysics, University of Oslo, Blindern, 0371 Oslo, Norway
70 Instituto de Astrofísica de Canarias, C/Vía Láctea s/n, 38205 La Laguna, Tenerife, Spain
71 Instituto de Física de Cantabria (CSIC-Universidad de Cantabria), Avda. de los Castros s/n, 39005 Santander, Spain
72 Istituto Nazionale di Fisica Nucleare, Sezione di Padova, via Marzolo 8, 35131 Padova, Italy
73 Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
74 Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester, M13 9PL, UK
75 Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA
76 Kavli Institute for Cosmology Cambridge, Madingley Road, Cambridge, CB3 0HA, UK
77 Kazan Federal University, 18 Kremlyovskaya St., 420008 Kazan, Russia
78 LAL, Université Paris-Sud, CNRS/IN2P3, 91898 Orsay, France
79 LERMA, CNRS, Observatoire de Paris, 61 Avenue de l’Observatoire, Paris, France
80 Laboratoire AIM, IRFU/Service d’Astrophysique−CEA/DSM−CNRS−Université Paris Diderot, Bât. 709, CEA-Saclay, 91191 Gif-sur-Yvette Cedex, France
81 Laboratoire Traitement et Communication de l’Information, CNRS (UMR 5141) and Télécom ParisTech, 46 rue Barrault 75634 Paris Cedex 13, France
82 Laboratoire de Physique Subatomique et Cosmologie, Université Grenoble-Alpes, CNRS/IN2P3, 53 rue des Martyrs, 38026 Grenoble Cedex, France
83 Laboratoire de Physique Théorique, Université Paris-Sud 11 & CNRS, Bâtiment 210, 91405 Orsay, France
84 Lawrence Berkeley National Laboratory, Berkeley, California, USA
85 Lebedev Physical Institute of the Russian Academy of Sciences, Astro Space Centre, 84/32 Profsoyuznaya st., 117997 Moscow, GSP-7, Russia
86 Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741 Garching, Germany
87 McGill Physics, Ernest Rutherford Physics Building, McGill University, 3600 rue University, Montréal, QC, H3A 2T8, Canada
88 National University of Ireland, Department of Experimental Physics, Maynooth, Co. Kildare, Ireland
89 Nicolaus Copernicus Astronomical Center, Bartycka 18, 00-716 Warsaw, Poland
90 Niels Bohr Institute, Blegdamsvej 17, 1165 Copenhagen, Denmark
91 Niels Bohr Institute, Copenhagen University, Blegdamsvej 17, 1165 Copenhagen, Denmark
92 Nordita (Nordic Institute for Theoretical Physics), Roslagstullsbacken 23, 106 91 Stockholm, Sweden
93 Optical Science Laboratory, University College London, Gower Street, WC1E 6BT, London, UK
94 SISSA, Astrophysics Sector, via Bonomea 265, 34136 Trieste, Italy
95 SMARTEST Research Centre, Università degli Studi e-Campus, via Isimbardi 10, 22060 Novedrate (CO), Italy
96 School of Chemistry and Physics, University of KwaZulu-Natal, Westville Campus, Private Bag X54001, 4000 Durban, South Africa
97 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
98 School of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RD, UK
99 Sorbonne Université-UPMC, UMR7095, Institut d’Astrophysique de Paris, 98bis Boulevard Arago, 75014 Paris, France
100 Space Research Institute (IKI), Russian Academy of Sciences, Profsoyuznaya Str, 84/32, 117997 Moscow, Russia
101 Space Sciences Laboratory, University of California, Berkeley, California, CA 94720, USA
102 Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnij Arkhyz, Zelenchukskiy region, 369167 Karachai-Cherkessian Republic, Russia
103 Stanford University, Dept of Physics, Varian Physics Bldg, 382 via Pueblo Mall, Stanford, California, USA
104 Sub-Department of Astrophysics, University of Oxford, Keble Road, Oxford OX1 3RH, UK
105 The Oskar Klein Centre for Cosmoparticle Physics, Department of Physics, Stockholm University, AlbaNova, 106 91 Stockholm, Sweden
106 Theory Division, PH-TH,CERN, 1211 Geneva 23, Switzerland
107 UPMC Univ Paris 06, UMR7095, 98bis Boulevard Arago, 75014 Paris, France
108 Universität Heidelberg, Institut für Theoretische Astrophysik, Philosophenweg 12, 69120 Heidelberg, Germany
109 Université de Toulouse, UPS-OMP, IRAP, 31028 Toulouse Cedex 4, France
110 Universities Space Research Association, Stratospheric Observatory for Infrared Astronomy, MS 232-11, Moffett Field, CA 94035, USA
111 University of Granada, Departamento de Física Teórica y del Cosmos, Facultad de Ciencias, 18071 Granada, Spain
112 University of Granada, Instituto Carlos I de Física Teórica y Computacional, 18071 Granada, Spain
113 Warsaw University Observatory, Aleje Ujazdowskie 4, 00-478 Warszawa, Poland
⋆
Corresponding author: P. Vielva, e-mail: vielva@ifca.unican.es
Received: 6 February 2015
Accepted: 21 May 2016
This paper presents a study of the integrated Sachs-Wolfe (ISW) effect from the Planck 2015 temperature and polarization data release. This secondary cosmic microwave background (CMB) anisotropy caused by the large-scale time-evolving gravitational potential is probed from different perspectives. The CMB is cross-correlated with different large-scale structure (LSS) tracers: radio sources from the NVSS catalogue; galaxies from the optical SDSS and the infrared WISE surveys; and the Planck 2015 convergence lensing map. The joint cross-correlation of the CMB with the tracers yields a detection at 4σ where most of the signal-to-noise is due to the Planck lensing and the NVSS radio catalogue. In fact, the ISW effect is detected from the Planck data only at ≈3σ (through the ISW-lensing bispectrum), which is similar to the detection level achieved by combining the cross-correlation signal coming from all the galaxy catalogues mentioned above. We study the ability of the ISW effect to place constraints on the dark-energy parameters; in particular, we show that ΩΛ is detected at more than 3σ. This cross-correlation analysis is performed only with the Planck temperature data, since the polarization scales available in the 2015 release do not permit significant improvement of the CMB-LSS cross-correlation detectability. Nevertheless, the Planck polarization data are used to study the anomalously large ISW signal previously reported through the aperture photometry on stacked CMB features at the locations of known superclusters and supervoids, which is in conflict with ΛCDM expectations. We find that the current Planck polarization data do not exclude that this signal could be caused by the ISW effect. In addition, the stacking of the Planck lensing map on the locations of superstructures exhibits a positive cross-correlation with these large-scale structures. Finally, we have improved our previous reconstruction of the ISW temperature fluctuations by combining the information encoded in all the previously mentioned LSS tracers. In particular, we construct a map of the ISW secondary anisotropies and the corresponding uncertainties map, obtained from simulations. We also explore the reconstruction of the ISW anisotropies caused by the large-scale structure traced by the 2MASS Photometric Redshift Survey (2MPZ) by directly inverting the density field into the gravitational potential field.
Key words: cosmology: observations / cosmic background radiation / large-scale structure of Universe / dark energy / galaxies: clusters: general / methods: data analysis
© ESO, 2016
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