Issue |
A&A
Volume 596, December 2016
|
|
---|---|---|
Article Number | A109 | |
Number of page(s) | 26 | |
Section | Cosmology (including clusters of galaxies) | |
DOI | https://doi.org/10.1051/0004-6361/201629022 | |
Published online | 12 December 2016 |
Planck intermediate results
XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies
1 APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Observatoire de ParisSorbonne 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 7945, Cape Town, South Africa
3 Agenzia Spaziale Italiana Science Data Center, 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, CA 91125, USA
9 Computational Cosmology Center, Lawrence Berkeley National Laboratory, Berkeley, California, CA 94720, USA
10 DTU Space, National Space Institute, Technical University of Denmark, Elektrovej 327, 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, Avda. Calvo Sotelo s/n, 33007 Oviedo, Spain
14 Department of Astrophysics/IMAPP, Radboud University Nijmegen, PO Box 9010, 6500 GL Nijmegen, The Netherlands
15 Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, British Columbia, Canada
16 Department of Physics and Astronomy, Dana and David Dornsife College of Letter, Arts and Sciences, University of Southern California, Los Angeles, CA 90089, USA
17 Department of Physics and Astronomy, University College London, London WC1E 6BT, UK
18 Department of Physics and Astronomy, University of Sussex, Brighton BN1 9QH, UK
19 Department of Physics, Gustaf Hällströmin katu 2a, University of Helsinki, 00014 Helsinki, Finland
20 Department of Physics, Princeton University, Princeton, New Jersey, NJ 08544, USA
21 Department of Physics, University of California, Santa Barbara, California, CA 93106, USA
22 Department of Physics, University of Illinois at Urbana-Champaign, 1110 West Green Street, Urbana, Illinois, 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 Astronomia, Alma Mater Studiorum, Università degli Studi di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy
25 Dipartimento di Fisica e Scienze della Terra, Università di Ferrara, via Saragat 1, 44122 Ferrara, Italy
26 Dipartimento di Fisica, Università La Sapienza, P. le A. Moro 2, 00185 Roma, Italy
27 Dipartimento di Fisica, Università degli Studi di Milano, via Celoria 16, 20133 Milano, Italy
28 Dipartimento di Fisica, Università degli Studi di Trieste, via A. Valerio 2, 34127 Trieste, Italy
29 Dipartimento di Fisica, Università di Roma Tor Vergata, via della Ricerca Scientifica 1, Roma, Italy
30 Dipartimento di Matematica, Università di Roma Tor Vergata, Via della Ricerca Scientifica, 1, 00133 Roma, Italy
31 European Space Agency, ESAC, Planck Science Office, Camino bajo del Castillo, s/n, Urbanización Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, Spain
32 European Space Agency, ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands
33 Gran Sasso Science Institute, INFN, viale F. Crispi 7, 67100 L’ Aquila, Italy
34 HGSFP and University of Heidelberg, Theoretical Physics Department, Philosophenweg 16, 69120 Heidelberg, Germany
35 Helsinki Instituteof Physics, Gustaf Hällströmin katu 2, University of Helsinki, 00014 Helsinki, Finland
36 INAF–Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, 35122 Padova, Italy
37 INAF–Osservatorio Astronomico di Roma, via di Frascati 33, 00040 Monte Porzio Catone, Italy
38 INAF–Osservatorio Astronomico di Trieste, via G.B. Tiepolo 11, 40127 Trieste, Italy
39 INAF/IASF Bologna, via Gobetti 101, 40129 Bologna, Italy
40 INAF/IASF Milano, via E. Bassini 15, 20133 Milano, Italy
41 INFN – CNAF, viale Berti Pichat 6/2, 40127 Bologna, Italy
42 INFN, Sezione di Bologna, viale Berti Pichat 6/2, 40127 Bologna, Italy
43 INFN, Sezione di Ferrara, via Saragat 1, 44122 Ferrara, 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, 00185 Roma, Italy
46 Imperial College London, Astrophysics group, Blackett Laboratory, Prince Consort Road, London, SW7 2AZ, UK
47 Institut d’Astrophysique Spatiale, CNRS, Univ. Paris-Sud, Université Paris-Saclay, Bât. 121, 91405 Orsay Cedex, France
48 Institut d’Astrophysique de Paris, CNRS (UMR 7095), 98 bis Boulevard Arago, 75014 Paris, France
49 Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
50 Institute of Theoretical Astrophysics, University of Oslo, Blindern, 0371 Oslo, Norway
51 Instituto de Astrofísica de Canarias, C/Vía Láctea s/n, La Laguna, 38205 Tenerife, Spain
52 Instituto de Física de Cantabria (CSIC-Universidad de Cantabria), Avda. de los Castros s/n, 39005 Santander, Spain
53 Istituto Nazionale di Fisica Nucleare, Sezione di Padova, via Marzolo 8, 35131 Padova, Italy
54 Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, CA 31109, USA
55 Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester, M13 9PL, UK
56 Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA
57 Kavli Institute for Cosmology Cambridge, Madingley Road, Cambridge, CB3 0HA, UK
58 LAL, Université Paris-Sud, CNRS/IN2P3, 91898 Orsay, France
59 LERMA, CNRS, Observatoire de Paris, 61 Avenue de l’Observatoire, 75014 Paris, France
60 Laboratoire Traitement et Communication de l’Information, CNRS (UMR 5141) and Télécom ParisTech, 46 rue Barrault, 75634 Paris Cedex 13, 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, California, USA
64 Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741 Garching, Germany
65 Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
66 Nicolaus Copernicus Astronomical Center, Bartycka 18, 00-716 Warsaw, Poland
67 Nordita (Nordic Institute for Theoretical Physics), Roslagstullsbacken 23, 106 91 Stockholm, Sweden
68 SISSA, Astrophysics Sector, via Bonomea 265, 34136 Trieste, Italy
69 School of Chemistry and Physics, University of KwaZulu-Natal, Westville Campus, Private Bag X54001, Durban 4000, South Africa
70 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
71 School of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RD, UK
72 Simon Fraser University, Department of Physics, 8888 University Drive, Burnaby BC, Canada
73 Sorbonne Université-UPMC, UMR 7095, Institut d’Astrophysique de Paris, 98 bis Boulevard Arago, 75014 Paris, France
74 Space Sciences Laboratory, University of California, Berkeley, California, CA 94720, USA
75 Sub-Department of Astrophysics, University of Oxford, Keble Road, Oxford OX1 3RH, UK
76 The Oskar Klein Centre for Cosmoparticle Physics, Department of Physics, Stockholm University, AlbaNova, 106 91 Stockholm, Sweden
77 UPMC Univ Paris 06, UMR 7095, 98 bis Boulevard Arago, 75014 Paris, France
78 Université de Toulouse, UPS-OMP, IRAP, 31028 Toulouse Cedex 4, France
79 University of Granada, Departamento de Física Teórica y del Cosmos, Facultad de Ciencias, 18071 Granada, Spain
80 Warsaw University Observatory, Aleje Ujazdowskie 4, 00-478 Warszawa, Poland
⋆
Corresponding author: M. Remazeilles, e-mail: mathieu.remazeilles@manchester.ac.uk
Received: 27 May 2016
Accepted: 9 August 2016
Using the Planck 2015 data release (PR2) temperature maps, we separate Galactic thermal dust emission from cosmic infrared background (CIB) anisotropies. For this purpose, we implement a specifically tailored component-separation method, the so-called generalized needlet internal linear combination (GNILC) method, which uses spatial information (the angular powerspectra) to disentangle the Galactic dust emission and CIB anisotropies. We produce significantly improved all-sky maps of Planck thermal dust emission, with reduced CIB contamination, at 353, 545, and 857 GHz. By reducing the CIB contamination of the thermal dust maps, we provide more accurate estimates of the local dust temperature and dust spectral index over the sky with reduced dispersion, especially at high Galactic latitudes above b = ±20°. We find that the dust temperature is T = (19.4 ± 1.3) K and the dust spectral index is β = 1.6 ± 0.1 averaged over the whole sky, while T = (19.4 ± 1.5) K and β = 1.6 ± 0.2 on 21% of the sky at high latitudes. Moreover, subtracting the new CIB-removed thermal dust maps from the CMB-removed Planck maps gives access to the CIB anisotropies over 60% of the sky at Galactic latitudes |b| > 20°. Because they are a significant improvement over previous Planck products, the GNILC maps are recommended for thermal dust science. The new CIB maps can be regarded as indirect tracers of the dark matter and they are recommended for exploring cross-correlations with lensing and large-scale structure optical surveys. The reconstructed GNILC thermal dust and CIB maps are delivered as Planck products.
Key words: cosmology: observations / methods: data analysis / ISM: general / dust, extinction / infrared: diffuse background / large-scale structure of Universe
© ESO, 2016
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