Issue |
A&A
Volume 550, February 2013
|
|
---|---|---|
Article Number | A133 | |
Number of page(s) | 19 | |
Section | Cosmology (including clusters of galaxies) | |
DOI | https://doi.org/10.1051/0004-6361/201220053 | |
Published online | 07 February 2013 |
Planck intermediate results
VII. Statistical properties of infrared and radio extragalactic sources from the Planck Early Release Compact Source Catalogue at frequencies between 100 and 857 GHz ⋆,⋆⋆
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,
Cape Town, South
Africa
4
Agenzia Spaziale Italiana Science Data Center, c/o ESRIN, via
Galileo Galilei, Frascati, Italy
5
Agenzia Spaziale Italiana, viale Liegi 26, Roma, Italy
6
Astrophysics Group, Cavendish Laboratory, University of
Cambridge, J J Thomson
Avenue, Cambridge
CB3 0HE,
UK
7
Atacama Large Millimeter/submillimeter Array, ALMA Santiago
Central Offices, Alonso de Cordova
3107, Vitacura, Casilla 763 0355, Santiago, Chile
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 of Mathematics for Applications, University of Oslo,
Blindern, Oslo,
Norway
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), 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,
Oviedo,
Spain
20
Departamento de Matemáticas, Universidad de Oviedo,
Avda. Calvo Sotelo s/n,
Oviedo,
Spain
21
Department of Astrophysics/IMAPP, Radboud University
Nijmegen, PO Box
9010, 6500 GL
Nijmegen, The
Netherlands
22
Department of Physics & Astronomy, University of British
Columbia, 6224 Agricultural Road,
Vancouver, British
Columbia, Canada
23
Department of Physics and Astronomy, Dana and David Dornsife
College of Letter, Arts and Sciences, University of Southern California,
Los Angeles, CA
90089,
USA
24
Department of Physics and Astronomy, Tufts
University, Medford,
MA
02155,
USA
25
Department of Physics, Gustaf Hällströmin katu 2a, University of
Helsinki, Helsinki,
Finland
26
Department of Physics, Princeton University,
Princeton, New Jersey, USA
27
Department of Physics, University of California,
Berkeley, California, USA
28
Department of Physics, University of California,
One Shields Avenue,
Davis, California, USA
29
Department of Physics, University of California,
Santa Barbara, California, USA
30
Department of Physics, University of Illinois at
Urbana-Champaign, 1110 West Green
Street, Urbana,
Illinois,
USA
31
Department of Statistics, Purdue University, 250 N. University
Street, West
Lafayette, Indiana, USA
32
Dipartimento di Fisica e Astronomia G. Galilei, Università degli
Studi di Padova, via Marzolo
8, 35131
Padova,
Italy
33
Dipartimento di Fisica e Scienze della Terra, Università di
Ferrara, via Saragat
1, 44122
Ferrara,
Italy
34
Dipartimento di Fisica, Università La Sapienza,
P. le A. Moro 2, Roma, Italy
35
Dipartimento di Fisica, Università degli Studi di
Milano, via Celoria
16, Milano,
Italy
36
Dipartimento di Fisica, Università degli Studi di
Trieste, via A. Valerio
2, Trieste,
Italy
37
Dipartimento di Fisica, Università di Roma Tor
Vergata, via della Ricerca
Scientifica, 1, Roma, Italy
38
Dipartimento di Matematica, Università di Roma Tor
Vergata, via della Ricerca
Scientifica, 1, Roma, Italy
39
Discovery Center, Niels Bohr Institute,
Blegdamsvej 17, Copenhagen, Denmark
40
Dpto. Astrofísica, Universidad de La Laguna (ULL),
38206
La Laguna, Tenerife,
Spain
41
European Southern Observatory, ESO Vitacura,
Alonso de Cordova 3107, Vitacura, Casilla
19001, Santiago,
Chile
42
European Space Agency, ESAC, Planck Science Office, Camino bajo
del Castillo, s/n, Urbanización
Villafranca del Castillo, 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, Helsinki, Finland
46
INAF – Osservatorio Astronomico di Padova,
Vicolo dell’Osservatorio 5,
Padova,
Italy
47
INAF – Osservatorio Astronomico di Roma,
via di Frascati 33,
Monte Porzio Catone,
Italy
48
INAF – Osservatorio Astronomico di Trieste,
via G.B. Tiepolo 11,
Trieste,
Italy
49
INAF Istituto di Radioastronomia, via P. Gobetti 101, 40129
Bologna,
Italy
50
INAF/IASF Bologna, via Gobetti 101, Bologna, Italy
51
INAF/IASF Milano, via E. Bassini 15, Milano, Italy
52
INFN, Sezione di Roma 1, Universit‘a di Roma
Sapienza, Piazzale Aldo Moro
2, 00185
Roma,
Italy
53
IPAG: Institut de Planétologie et d’Astrophysique de Grenoble,
Université Joseph Fourier, Grenoble 1/CNRS-INSU, UMR 5274,
38041
Grenoble,
France
54
ISDC Data Centre for Astrophysics, University of
Geneva, Ch. d’Ecogia
16, Versoix,
Switzerland
55
IUCAA, Post Bag 4, Ganeshkhind, Pune University
Campus, 411007
Pune,
India
56
Imperial College London, Astrophysics group, Blackett
Laboratory, Prince Consort
Road, London,
SW7 2AZ,
UK
57
Infrared Processing and Analysis Center, California Institute of
Technology, Pasadena,
CA
91125,
USA
58
Institut Néel, CNRS, Université Joseph Fourier Grenoble
I, 25 rue des
Martyrs, 38041
Grenoble,
France
59
Institut Universitaire de France, 103 bd Saint-Michel, 75005
Paris,
France
60
Institut d’Astrophysique Spatiale, CNRS (UMR 8617) Université
Paris-Sud 11, Bâtiment
121, Orsay,
France
61
Institut d’Astrophysique de Paris, CNRS (UMR 7095),
98bis boulevard Arago,
75014
Paris,
France
62
Institut de Ciències de l’Espai, CSIC/IEEC, Facultat de
Ciències, Campus UAB, Torre C5
par-2, Bellaterra
08193,
Spain
63
Institute for Space Sciences, Bucharest-Magurale,
Romania
64
Institute of Astronomy and Astrophysics, Academia
Sinica, Taipei,
Taiwan
65
Institute of Astronomy, University of Cambridge,
Madingley Road, Cambridge
CB3 0HA,
UK
66
Institute of Theoretical Astrophysics, University of
Oslo, Blindern,
Oslo,
Norway
67
Instituto de Astrofísica de Canarias, C/vía Láctea s/n, La Laguna, Tenerife, Spain
68
Instituto de Física de Cantabria (CSIC-Universidad de
Cantabria), Avda. de los Castros
s/n, Santander,
Spain
69
Jet Propulsion Laboratory, California Institute of
Technology, 4800 Oak Grove
Drive, Pasadena,
California,
USA
70
Jodrell Bank Centre for Astrophysics, Alan Turing Building, School
of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester, M13
9PL, UK
71
Kavli Institute for Cosmology Cambridge,
Madingley Road, Cambridge, CB3 0HA, UK
72
LAL, Université Paris-Sud, CNRS/IN2P3,
Orsay,
France
73
LERMA, CNRS, Observatoire de Paris, 61 avenue de
l’Observatoire, Paris, France
74
Laboratoire AIM, IRFU/Service d’Astrophysique – CEA/DSM – CNRS –
Université Paris Diderot, Bât. 709,
CEA-Saclay, 91191
Gif-sur-Yvette Cedex,
France
75
Laboratoire Traitement et Communication de l’Information, CNRS
(UMR 5141) and Télécom ParisTech, 46 rue Barrault, 75634
Paris Cedex 13,
France
76
Laboratoire de Physique Subatomique et deCosmologie, Université
Joseph Fourier Grenoble I, CNRS/IN2P3, Institut National Polytechnique de
Grenoble, 53 rue des
Martyrs, 38026
Grenoble Cedex,
France
77
Laboratoire de Physique Théorique, Université Paris-Sud 11 &
CNRS, Bâtiment 210,
91405
Orsay,
France
78
Lawrence Berkeley National Laboratory,
Berkeley, California, USA
79
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741
Garching,
Germany
80
National University of Ireland, Department of Experimental
Physics, Maynooth,
Co. Kildare,
Ireland
81
Niels Bohr Institute, Blegdamsvej 17, Copenhagen, Denmark
82
Observational Cosmology, Mail Stop 367-17, California Institute of
Technology, Pasadena,
CA, 91125, USA
83
Optical Science Laboratory, University College
London, Gower
Street, London,
UK
84
SISSA, Astrophysics Sector, via Bonomea 265, 34136, Trieste, Italy
85
School of Physics and Astronomy, Cardiff University,
Queens Buildings, The Parade,
Cardiff, CF24 3AA, UK
86
Space Sciences Laboratory, University of California,
Berkeley, California, USA
87
Stanford University, Dept of Physics, Varian Physics
Bldg, 382 via Pueblo
Mall, Stanford,
California,
USA
88
UPMC Univ Paris 06, UMR7095, 98bis boulevard Arago, 75014
Paris,
France
89
Université de Toulouse, UPS-OMP, IRAP,
31028
Toulouse Cedex 4,
France
90
Universities Space Research Association, Stratospheric Observatory
for Infrared Astronomy, MS
211-3, Moffett
Field, CA
94035,
USA
91
University of Granada, Departamento de Física Teórica y del
Cosmos, Facultad de Ciencias, Granada, Spain
92
Warsaw University Observatory, Aleje Ujazdowskie 4, 00-478
Warszawa,
Poland
Received:
19
July
2012
Accepted:
27
November
2012
We make use of the Planck all-sky survey to derive number counts and spectral indices of extragalactic sources – infrared and radio sources – from the Planck Early Release Compact Source Catalogue (ERCSC) at 100 to 857 GHz (3mm to 350 μm). Three zones (deep, medium and shallow) of approximately homogeneous coverage are used to permit a clean and controlled correction for incompleteness, which was explicitly not done for the ERCSC, as it was aimed at providing lists of sources to be followed up. Our sample, prior to the 80% completeness cut, contains between 217 sources at 100 GHz and 1058 sources at 857 GHz over about 12800 to 16550 deg2 (31 to 40% of the sky). After the 80% completeness cut, between 122 and 452 and sources remain, with flux densities above 0.3 and 1.9 Jy at 100 and 857 GHz. The sample so defined can be used for statistical analysis. Using the multi-frequency coverage of the Planck High Frequency Instrument, all the sources have been classified as either dust-dominated (infrared galaxies) or synchrotron-dominated (radio galaxies) on the basis of their spectral energy distributions (SED). Our sample is thus complete, flux-limited and color-selected to differentiate between the two populations. We find an approximately equal number of synchrotron and dusty sources between 217 and 353 GHz; at 353 GHz or higher (or 217 GHz and lower) frequencies, the number is dominated by dusty (synchrotron) sources, as expected. For most of the sources, the spectral indices are also derived. We provide for the first time counts of bright sources from 353 to 857 GHz and the contributions from dusty and synchrotron sources at all HFI frequencies in the key spectral range where these spectra are crossing. The observed counts are in the Euclidean regime. The number counts are compared to previously published data (from earlier Planck results, Herschel, BLAST, SCUBA, LABOCA, SPT, and ACT) and models taking into account both radio or infrared galaxies, and covering a large range of flux densities. We derive the multi-frequency Euclidean level – the plateau in the normalised differential counts at high flux-density – and compare it to WMAP, Spitzer and IRAS results. The submillimetre number counts are not well reproduced by current evolution models of dusty galaxies, whereas the millimetre part appears reasonably well fitted by the most recent model for synchrotron-dominated sources. Finally we provide estimates of the local luminosity density of dusty galaxies, providing the first such measurements at 545 and 857 GHz.
Key words: cosmology: observations / surveys / galaxies: statistics / galaxies: evolution / galaxies: star formation / galaxies: active
Appendices are available in electronic form at http://www.aanda.org
© ESO, 2013
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