Issue |
A&A
Volume 617, September 2018
|
|
---|---|---|
Article Number | A48 | |
Number of page(s) | 17 | |
Section | Cosmology (including clusters of galaxies) | |
DOI | https://doi.org/10.1051/0004-6361/201731489 | |
Published online | 24 September 2018 |
Planck intermediate results
LIII. Detection of velocity dispersion from the kinetic Sunyaev-Zeldovich 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
African Institute for Mathematical Sciences, 6-8 Melrose Road, Muizenberg, Cape Town, South Africa
3
Agenzia Spaziale Italiana, Via del Politecnico snc, 00133 Roma, Italy
4
Astrophysics Group, Cavendish Laboratory, University of Cambridge, J J Thomson Avenue, Cambridge, CB3 0HE, UK
5
Astrophysics & Cosmology Research Unit, School of Mathematics, Statistics & Computer Science, University of KwaZulu-Natal, Westville Campus, Private Bag X54001, Durban, 4000, South Africa
6
CITA, University of Toronto, 60 St. George St., Toronto, ON M5S 3H8, Canada
7
CNRS, IRAP, 9 Av. colonel Roche, BP 44346, 31028 Toulouse Cedex 4, France
8
California Institute of Technology, Pasadena, California, USA
9
Computational Cosmology Center, Lawrence Berkeley National Laboratory, Berkeley, California, USA
10
DTU Space, National Space Institute, Technical University of Denmark, Elektrovej 327, DK-2800 Kgs., Lyngby, Denmark
11
Département de Physique Théorique, Université de Genève, 24, Quai E. Ansermet, 1211 Genève 4, Switzerland
12
Departamento de Astrofísica, Universidad de La Laguna (ULL), 38206 La Laguna, Tenerife, Spain
13
Departamento de Física, Universidad de Oviedo, C/Federico García Lorca 18, Oviedo, Spain
14
Department of Astrophysics/IMAPP, Radboud University, PO Box 9010, 6500 GL Nijmegen, The Netherlands
15
Department of Mathematics, University of Stellenbosch, Stellenbosch, 7602, South Africa
16
Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, British Columbia, Canada
17
Department of Physics & Astronomy, University of the Western Cape, Cape Town, 7535, South Africa
18
Department of Physics and Astronomy, University of Sussex, Brighton, BN1 9QH, UK
19
Department of Physics, Gustaf Hällströmin katu 2a, University of Helsinki, Helsinki, Finland
20
Department of Physics, Princeton University, Princeton, New Jersey, USA
21
Department of Physics, University of California, Santa Barbara, CA, USA
22
Department of Physics, University of Illinois at Urbana-Champaign, 1110 West Green Street, Urbana, IL, USA
23
Dipartimento di Fisica e Astronomia G. Galilei, Università degli Studi di Padova, via Marzolo 8, 35131 Padova, Italy
24
Dipartimento di Fisica e Scienze della Terra, Università di Ferrara, Via Saragat 1, 44122 Ferrara, Italy
25
Dipartimento di Fisica, Università La Sapienza, P. le A. Moro 2, Roma, Italy
26
Dipartimento di Fisica, Università degli Studi di Milano, Via Celoria, 16, Milano, Italy
27
Dipartimento di Fisica, Università degli Studi di Trieste, via A. Valerio 2, Trieste, Italy
28
Dipartimento di Fisica, Università di Roma Tor Vergata, Via della Ricerca Scientifica 1, Roma, Italy
29
European Space Agency, ESAC, Planck Science Office, Camino bajo del Castillo, s/n, Urbanización Villafranca del Castillo, Villanueva de la Cañada, Madrid, Spain
30
European Space Agency, ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands
31
Gran Sasso Science Institute, INFN, viale F. Crispi 7, 67100 L’Aquila, Italy
32
HGSFP and University of Heidelberg, Theoretical Physics Department, Philosophenweg 16, 69120 Heidelberg, Germany
33
Haverford College Astronomy Department, 370 Lancaster Avenue, Haverford, Pennsylvania, USA
34
Helsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, Helsinki, Finland
35
INAF – OAS Bologna, Istituto Nazionale di Astrofisica - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Area della Ricerca del CNR, Via Gobetti 101, 40129 Bologna, Italy
36
INAF – Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, Padova, Italy
37
INAF – Osservatorio Astronomico di Trieste, Via G.B. Tiepolo 11, Trieste, Italy
38
INAF, Istituto di Radioastronomia, Via Piero Gobetti 101, 40129 Bologna, Italy
39
INAF/IASF Milano, Via E. Bassini 15, Milano, Italy
40
INFN – CNAF, viale Berti Pichat 6/2, 40127 Bologna, Italy
41
INFN, Sezione di Bologna, viale Berti Pichat 6/2, 40127 Bologna, Italy
42
INFN, Sezione di Ferrara, Via Saragat 1, 44122 Ferrara, Italy
43
INFN, Sezione di Milano, Via Celoria 16, Milano, Italy
44
INFN, Sezione di Roma 1, Università di Roma Sapienza, Piazzale Aldo Moro 2, 00185 Roma, Italy
45
INFN, Sezione di Roma 2, Università di Roma Tor Vergata, Via della Ricerca Scientifica 1, Roma, Italy
46
INFN/National Institute for Nuclear Physics, Via Valerio 2, 34127 Trieste, Italy
47
Imperial College London, Astrophysics group, Blackett Laboratory, Prince Consort Road, London, SW7 2AZ, UK
48
Institut d’Astrophysique Spatiale, CNRS, Univ. Paris-Sud, Université Paris-Saclay, Bât. 121, 91405 Orsay Cedex, France
49
Institut d’Astrophysique de Paris, CNRS (UMR7095), 98 bis Boulevard Arago, 75014 Paris, France
50
Institute Lorentz, Leiden University, PO Box 9506, Leiden 2300 RA, The Netherlands
51
Institute of Theoretical Astrophysics, University of Oslo, Blindern, Oslo, Norway
52
Instituto de Astrofísica de Canarias, C/Vía Láctea s/n, La Laguna, Tenerife, Spain
53
Instituto de Física de Cantabria (CSIC-Universidad de Cantabria), Avda. de los Castros s/n, Santander, Spain
54
Istituto Nazionale di Fisica Nucleare, Sezione di Padova, via Marzolo 8, 35131 Padova, Italy
55
Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
56
Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester, M13 9PL, UK
57
Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA
58
Kavli Institute for Cosmology Cambridge, Madingley Road, Cambridge, CB3 0HA, UK
59
LAL, Université Paris-Sud, CNRS/IN2P3, Orsay, France
60
LERMA, CNRS, Observatoire de Paris, 61 Avenue de l’Observatoire, Paris, France
61
Laboratoire de Physique Subatomique et Cosmologie, Université Grenoble-Alpes, CNRS/IN2P3, 53, rue des Martyrs, 38026 Grenoble Cedex, France
62
Laboratoire de Physique Théorique, Université Paris-Sud 11 & CNRS, Bâtiment 210, 91405 Orsay, France
63
Lawrence Berkeley National Laboratory, Berkeley, CA, USA
64
Low Temperature Laboratory, Department of Applied Physics, Aalto University, Espoo, 00076 AALTO, Finland
65
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741 Garching, Germany
66
Mullard Space Science Laboratory, University College London, Surrey, H5 6NT, UK
67
NAOC-UKZN Computational Astrophysics Centre (NUCAC), University of KwaZulu-Natal, Durban, 4000 South Africa
e-mail: ma@ukzn.ac.za
68
Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Bartycka 18, 00-716 Warsaw, Poland
69
Nordita (Nordic Institute for Theoretical Physics), Roslagstullsbacken 23, 106 91 Stockholm, Sweden
70
SISSA, Astrophysics Sector, via Bonomea 265, 34136 Trieste, Italy
71
San Diego Supercomputer Center, University of California, San Diego, 9500 Gilman Drive, La Jolla, CA, 92093, USA
72
School of Chemistry and Physics, University of KwaZulu-Natal, Westville Campus, Private Bag X54001, Durban, 4000, South Africa
73
School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
74
School of Physics and Astronomy, Sun Yat-Sen University, 135 Xingang Xi Road, Guangzhou, PR China
75
School of Physics, Indian Institute of Science Education and Research Thiruvananthapuram, Maruthamala PO, Vithura, Thiruvananthapuram, 695551 Kerala, India
76
Simon Fraser University, Department of Physics, 8888 University Drive, Burnaby BC, Canada
77
Sorbonne Université-UPMC, UMR7095, Institut d’Astrophysique de Paris, 98 bis Boulevard Arago, 75014 Paris, France
78
Space Research Institute (IKI), Russian Academy of Sciences, Profsoyuznaya Str, 84/32, Moscow, 117997, Russia
79
Space Science Data Center - Agenzia Spaziale Italiana, Via del Politecnico snc, 00133 Roma, Italy
80
Space Sciences Laboratory, University of California, Berkeley, California, USA
81
The Oskar Klein Centre for Cosmoparticle Physics, Department of Physics, Stockholm University, AlbaNova, 106 91 Stockholm, Sweden
82
UPMC Univ. Paris 06, UMR7095, 98 bis Boulevard Arago, 75014 Paris, France
83
Université de Toulouse, UPS-OMP, IRAP, 31028 Toulouse Cedex 4, France
84
Warsaw University Observatory, Aleje Ujazdowskie 4, 00-478 Warszawa, Poland
Received:
2
July
2017
Accepted:
12
June
2018
Using the Planck full-mission data, we present a detection of the temperature (and therefore velocity) dispersion due to the kinetic Sunyaev-Zeldovich (kSZ) effect from clusters of galaxies. To suppress the primary CMB and instrumental noise we derive a matched filter and then convolve it with the Planck foreground-cleaned “2D-ILC” maps. By using the Meta Catalogue of X-ray detected Clusters of galaxies (MCXC), we determine the normalized rms dispersion of the temperature fluctuations at the positions of clusters, finding that this shows excess variance compared with the noise expectation. We then build an unbiased statistical estimator of the signal, determining that the normalized mean temperature dispersion of 1526 clusters is 〈(ΔT/T)2 〉 = (1.64 ± 0.48) × 10−11. However, comparison with analytic calculations and simulations suggest that around 0.7 σ of this result is due to cluster lensing rather than the kSZ effect. By correcting this, the temperature dispersion is measured to be 〈(ΔT/T)2〉 = (1.35 ± 0.48) × 10−11, which gives a detection at the 2.8 σ level. We further convert uniform-weight temperature dispersion into a measurement of the line-of-sight velocity dispersion, by using estimates of the optical depth of each cluster (which introduces additional uncertainty into the estimate). We find that the velocity dispersion is 〈υ2〉 = (123 000 ± 71 000) (km s−1)2, which is consistent with findings from other large-scale structure studies, and provides direct evidence of statistical homogeneity on scales of 600 h−1 Mpc. Our study shows the promise of using cross-correlations of the kSZ effect with large-scale structure in order to constrain the growth of structure.
Key words: cosmic background radiation / large-scale structure of Universe / galaxies: clusters: general / methods: data analysis
© ESO 2018
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