Issue |
A&A
Volume 536, December 2011
Planck early results
|
|
---|---|---|
Article Number | A9 | |
Number of page(s) | 20 | |
Section | Cosmology (including clusters of galaxies) | |
DOI | https://doi.org/10.1051/0004-6361/201116460 | |
Published online | 01 December 2011 |
Planck early results. IX. XMM-Newton follow-up for validation of Planck cluster candidates⋆
1
Aalto University Metsähovi Radio Observatory,
Metsähovintie 114,
02540
Kylmälä,
Finland
2
Agenzia Spaziale Italiana Science Data Center,
c/o ESRIN, via Galileo
Galilei, Frascati, Italy
3
Astroparticule et Cosmologie, CNRS (UMR7164), Université
Denis Diderot Paris 7, Bâtiment Condorcet, 10 rue A. Domon et Léonie Duquet,
Paris,
France
4
Astrophysics Group, Cavendish Laboratory, University of
Cambridge, J J Thomson
Avenue, Cambridge
CB3 0HE,
UK
5
Atacama Large Millimeter/submillimeter Array, ALMA Santiago
Central Offices, Alonso de
Cordova 3107, Vitacura, Casilla
763 0355, Santiago,
Chile
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
e-mail: etienne.pointecouteau@cesr.fr
8
California Institute of Technology,
Pasadena, California,
USA
9
Centre of Mathematics for Applications, University of
Oslo, Blindern,
Oslo,
Norway
10
Centro de Astrofísica, Universidade do Porto,
Rua das Estrelas,
4150-762
Porto,
Portugal
11
DAMTP, University of Cambridge, Centre for Mathematical
Sciences, Wilberforce
Road, Cambridge
CB3 0WA,
UK
12
DSM/Irfu/SPP, CEA-Saclay, 91191
Gif-sur-Yvette Cedex,
France
13
DTU Space, National Space Institute,
Juliane Mariesvej 30,
Copenhagen,
Denmark
14
Departamento de Física, Universidad de Oviedo,
Avda. Calvo Sotelo s/n,
Oviedo,
Spain
15
Department of Astronomy and Astrophysics, University of
Toronto, 50 Saint George
Street, Toronto, Ontario, Canada
16
Department of Physics & Astronomy, University of
British Columbia, 6224
Agricultural Road, Vancouver,
British Columbia,
Canada
17
Department of Physics and Astronomy, University of Southern
California, Los
Angeles, California, USA
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, Purdue University,
525 Northwestern Avenue,
West Lafayette,
Indiana,
USA
21
Department of Physics, University of
California, Berkeley, California, USA
22
Department of Physics, University of
California, One Shields
Avenue, Davis, California, USA
23
Department of Physics, University of
California, Santa
Barbara, California, USA
24
Department of Physics, University of Illinois at
Urbana-Champaign, 1110 West
Green Street, Urbana, Illinois, USA
25
Dipartimento di Fisica G. Galilei, Università degli Studi di
Padova, via Marzolo
8, 35131
Padova,
Italy
26
Dipartimento di Fisica, Università La
Sapienza, P. le A. Moro
2, Roma,
Italy
27
Dipartimento di Fisica, Università degli Studi
diMilano, via Celoria,
16, Milano,
Italy
28
Dipartimento di Fisica, Università degli Studi di
Trieste, via A. Valerio
2, Trieste,
Italy
29
Dipartimento di Fisica, Università di Ferrara,
via Saragat 1,
44122
Ferrara,
Italy
30
Dipartimento di Fisica, Università di Roma Tor
Vergata, via della Ricerca
Scientifica, 1, Roma, Italy
31
Discovery Center, Niels Bohr Institute,
Blegdamsvej
17, Copenhagen, Denmark
32
Dpto. Astrofísica, Universidad de La Laguna
(ULL), 38206
La Laguna, Tenerife,
Spain
33
European Southern Observatory, ESO Vitacura, Alonso de Cordova 3107, Vitacura, Casilla
19001, Santiago,
Chile
34
European Space Agency, ESAC, Camino bajo del
Castillo, s/n, Urbanización
Villafranca del Castillo, Villanueva de la Cañada,
Madrid,
Spain
35
European Space Agency, ESAC, Planck Science Office, Camino
bajo del Castillo, s/n,
Urbanización Villafranca del Castillo, Villanueva de la Cañada,
Madrid,
Spain
36
European Space Agency, ESTEC, Keplerlaan 1, 2201 AZ
Noordwijk, The
Netherlands
37
Helsinki Institute of Physics, Gustaf Hällströmin katu 2,
University of Helsinki, Helsinki, Finland
38
INAF – Osservatorio Astronomico di Padova,
Vicolo dell’Osservatorio 5,
Padova,
Italy
39
INAF – Osservatorio Astronomico di Roma,
via di Frascati 33,
Monte Porzio Catone,
Italy
40
INAF – Osservatorio Astronomico di Trieste,
via G.B. Tiepolo 11,
Trieste,
Italy
41
INAF/IASF Bologna, via Gobetti
101, Bologna,
Italy
42
INAF/IASF Milano, via E. Bassini 15, Milano, Italy
43
INRIA, Laboratoire de Recherche en Informatique, Université
Paris-Sud 11, Bâtiment
490, 91405
Orsay Cedex,
France
44
IPAG: Institut de Planétologie et d’Astrophysique de
Grenoble, Université Joseph Fourier, Grenoble 1 / CNRS-INSU, UMR
5274, 38041
Grenoble,
France
45
Imperial College London, Astrophysics group, Blackett
Laboratory, Prince Consort
Road, London,
SW7 2AZ,
UK
46
Infrared Processing and Analysis Center, California
Institute of Technology, Pasadena, CA
91125,
USA
47
Institut Néel, CNRS, Université Joseph Fourier Grenoble
I, 25 rue des
Martyrs, Grenoble, France
48
Institut d’Astrophysique Spatiale, CNRS (UMR8617) Université
Paris-Sud 11, Bâtiment
121, Orsay,
France
49
Institut d’Astrophysique de Paris, CNRS UMR7095, Université
Pierre & Marie Curie, 98 bis boulevard Arago, Paris, France
50
Institute of Astronomy and Astrophysics, Academia
Sinica, Taipei,
Taiwan
51
Institute of Astronomy, University of
Cambridge, Madingley
Road, Cambridge
CB3 0HA,
UK
52
Institute of Theoretical Astrophysics, University of
Oslo, Blindern,
Oslo,
Norway
53
Instituto de Astrofísica de Canarias,
C/Vía Láctea s/n,
La Laguna, Tenerife,
Spain
54
Instituto de Física de Cantabria (CSIC-Universidad de
Cantabria), Avda. de los
Castros s/n, Santander, Spain
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 Cosmology Cambridge,
Madingley Road,
Cambridge, CB3 0HA,
UK
58
LERMA, CNRS, Observatoire de Paris,
61 Avenue de
l’Observatoire, Paris, France
59
Laboratoire AIM, IRFU/Service d’Astrophysique - CEA/DSM -
CNRS - Université Paris Diderot, Bât. 709, CEA-Saclay,
91191
Gif-sur-Yvette Cedex,
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 de Cosmologie,
CNRS/IN2P3, Université Joseph Fourier Grenoble I, Institut National
Polytechnique de Grenoble, 53
rue des Martyrs, 38026
Grenoble Cedex,
France
62
Laboratoire de l’Accélérateur Linéaire, Université Paris-Sud
11, CNRS/IN2P3, Orsay, France
63
Lawrence Berkeley National Laboratory,
Berkeley,
California,
USA
64
Max-Planck-Institut für Astrophysik,
Karl-Schwarzschild-Str. 1,
85741
Garching,
Germany
65
Max-Planck-Institut für Extraterrestrische
Physik, Giessenbachstraße, 85748
Garching,
Germany
66
MilliLab, VTT Technical Research Centre of
Finland, Tietotie
3, Espoo,
Finland
67
National University of Ireland, Department of Experimental
Physics, Maynooth, Co.
Kildare, Ireland
68
Niels Bohr Institute, Blegdamsvej 17, Copenhagen,
Denmark
69
Observational Cosmology, Mail Stop 367-17, California
Institute of Technology, Pasadena, CA
91125,
USA
70
SISSA, Astrophysics Sector, via Bonomea 265, 34136, Trieste,
Italy
71
SUPA, Institute for Astronomy, University of Edinburgh,
Royal Observatory, Blackford
Hill, Edinburgh
EH9 3HJ,
UK
72
School of Physics and Astronomy, Cardiff
University, Queens Buildings,
The Parade, Cardiff, CF24
3AA, UK
73
Space Research Institute (IKI), Russian Academy of
Sciences, Profsoyuznaya Str,
84/32, Moscow
117997,
Russia
74
Space Sciences Laboratory, University of
California, Berkeley, California, USA
75
Stanford University, Dept of Physics, Varian Physics
Bldg, 382 via Pueblo
Mall, Stanford, California, USA
76
Tartu Observatory, Toravere, Tartumaa 61602, Estonia
77
Tuorla Observatory, Department of Physics and Astronomy,
University of Turku, Väisäläntie 20, 21500
Piikkiö,
Finland
78
Universität Heidelberg, Institut für Theoretische
Astrophysik, Albert-Überle-Str. 2, 69120
Heidelberg,
Germany
79
Université de Toulouse, UPS-OMP, IRAP, 31028
Toulouse Cedex 4,
France
80
University of Granada, Departamento de Física Teórica y del
Cosmos, Facultad de Ciencias, Granada, Spain
81
University of Miami, Knight Physics Building, 1320 Campo Sano
Dr., Coral
Gables, Florida, USA
82
Warsaw University Observatory, Aleje Ujazdowskie 4, 00-478
Warszawa,
Poland
Received:
7
January
2011
Accepted:
2
July
2011
We present the XMM-Newton follow-up for confirmation of Planck cluster candidates. Twenty-five candidates have been observed to date using snapshot (~10ks) exposures, ten as part of a pilot programme to sample a low range of signal-to-noise ratios (4 < S/N < 6), and a further 15 in a programme to observe a sample of S/N > 5 candidates. The sensitivity and spatial resolution of XMM-Newton allows unambiguous discrimination between clusters and false candidates. The 4 false candidates have S/N ≤ 4.1. A total of 21 candidates are confirmed as extended X-ray sources. Seventeen are single clusters, the majority of which are found to have highly irregular and disturbed morphologies (about ~70%). The remaining four sources are multiple systems, including the unexpected discovery of a supercluster at z = 0.45. For 20 sources we are able to derive a redshift estimate from the X-ray Fe K line (albeit of variable quality). The new clusters span the redshift range 0.09 ≲ z ≲ 0.54, with a median redshift of z ~ 0.37. A first determination is made of their X-ray properties including the characteristic size, which is used to improve the estimate of the SZ Compton parameter, Y500. The follow-up validation programme has helped to optimise the Planck candidate selection process. It has also provided a preview of the X-ray properties of these newly-discovered clusters, allowing comparison with their SZ properties, and to the X-ray and SZ properties of known clusters observed in the Planck survey. Our results suggest that Planck may have started to reveal a non-negligible population of massive dynamically perturbed objects that is under-represented in X-ray surveys. However, despite their particular properties, these new clusters appear to follow the Y500–YX relation established for X-ray selected objects, where YX is the product of the gas mass and temperature.
Key words: cosmology: observations / galaxies: clusters: general / galaxies: clusters: intracluster medium / cosmic background radiation / X-rays: galaxies: clusters
© ESO, 2011
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