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The XXL Survey: II. the bright cluster sample: Catalogue and luminosity function
Indexado
WoS WOS:000384722600020
Scopus SCOPUS_ID:84975514127
DOI 10.1051/0004-6361/201526891
Año 2016
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



Results. The bright cluster sample consists of systems with masses between M-500 = 7 x 10(13) and 3 x 10(14) M-circle dot, mostly located between z = 0.1 and 0.5. The observed sky density of clusters is slightly below the predictions from the WMAP9 model, and significantly below the prediction from the Planck 2015 cosmology. In general, within the current uncertainties of the cluster mass calibration, models with higher values of sigma(8) and/or Omega(M) appear more difficult to accommodate. We provide tight constraints on the cluster differential luminosity function and find no hint of evolution out to z similar to 1. We also find strong evidence for the presence of large-scale structures in the XXL bright cluster sample and identify five new superclusters.

Revista



Revista ISSN
Astronomy & Astrophysics 0004-6361

Métricas Externas



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Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Scopus
Sin Disciplinas
SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 Pacaud, F. - UNIV BONN - Alemania
Universität Bonn - Alemania
2 Clerc, Nicolas Hombre Max Planck Inst Extraterr Phys - Alemania
Max Planck Institute for Extraterrestrial Physics - Alemania
3 Giles, P. A. - Univ Bristol - Reino Unido
University of Bristol - Reino Unido
4 Adami, Christophe Hombre Aix Marseille Univ - Francia
Laboratoire d'Astrophysique de Marseille - Francia
5 Sadibekova, T. - CEA Saclay - Francia
6 Pierre, M. - CEA Saclay - Francia
7 Maughan, B. J. - Univ Bristol - Reino Unido
University of Bristol - Reino Unido
8 Lieu, M. - Univ Birmingham - Reino Unido
University of Birmingham - Reino Unido
9 Le Fevre, J. P. - CEA Saclay - Francia
10 Alis, S. - Istanbul Univ - Turquía
Univ Nice Sophia Antipolis - Francia
Istanbul Üniversitesi - Turquía
Laboratoire Joseph-Louis Lagrange - Francia
11 Altieri, B. Hombre European Space Astronomy Centre - España
12 Ardila, F. - UNIV FLORIDA - Estados Unidos
University of Florida - Estados Unidos
13 Baran, Andrzej S. Hombre Liverpool John Moores Univ - Reino Unido
Liverpool John Moores University - Reino Unido
14 Benoist, C. Hombre Univ Nice Sophia Antipolis - Francia
Laboratoire Joseph-Louis Lagrange - Francia
15 Birkinshaw, Mark Hombre Univ Bristol - Reino Unido
University of Bristol - Reino Unido
16 Chiappetti, L. - Istituto Nazionale di Astrofisica - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan - Italia
17 Democles, J. - Univ Birmingham - Reino Unido
University of Birmingham - Reino Unido
18 Eckert, D. - Univ Geneva - Suiza
Université de Genève - Suiza
19 Evrard, A. E. Hombre UNIV MICHIGAN - Estados Unidos
University of Michigan, Ann Arbor - Estados Unidos
20 Faccioli, L. - CEA Saclay - Francia
21 Gastaldello, Fabio Hombre Istituto Nazionale di Astrofisica - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan - Italia
22 Guennou, Loic - Univ KwaZulu Natal - República de Sudáfrica
University of KwaZulu-Natal - República de Sudáfrica
23 Horellou, C. - Chalmers - Suecia
24 Iovino, A. - Istituto Nazionale di Astrofisica - Italia
Osservatorio Astronomico di Brera - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan - Italia
25 Koulouridis, E. - Natl Observ Athens - Grecia
CEA Saclay - Francia
National Observatory of Athens - Grecia
26 Le Brun, V. Hombre Laboratoire d'Astrophysique de Marseille - Francia
27 Lidman, Chris Hombre Australian Astronomical Observatory - Australia
28 Liske, J. Hombre ESO - Alemania
29 Maurogordato, S. - Laboratoire Joseph-Louis Lagrange - Francia
30 Menanteau, F. Hombre UNIV ILLINOIS - Estados Unidos
University of Illinois at Urbana-Champaign - Estados Unidos
University of Illinois Urbana-Champaign - Estados Unidos
31 Owers, Matt Hombre Australian Astron Observ - Australia
Macquarie Univ - Australia
Australian Astronomical Observatory - Australia
Macquarie University - Australia
32 Poggianti, B. Mujer Istituto Nazionale di Astrofisica - Italia
Osservatorio Astronomico di Padova - Italia
33 Pomarede, D. - CEA Saclay - Francia
34 Ségransan, Damien Hombre ESO - Chile
European Southern Observatory Santiago - Chile
ESO - Alemania
35 Ponman, T. - Univ Birmingham - Reino Unido
University of Birmingham - Reino Unido
36 Rapetti, D. Hombre Univ Copenhagen - Dinamarca
UNIV MUNICH - Alemania
Niels Bohr Institute - Dinamarca
Ludwig-Maximilians-Universität München - Alemania
Niels Bohr Institutet - Dinamarca
37 Reiprich, T. H. - UNIV BONN - Alemania
Universität Bonn - Alemania
38 Smith, G. P. Hombre Univ Birmingham - Reino Unido
University of Birmingham - Reino Unido
39 Steenkamp, R. Hombre Max Planck Inst Kernphys - Alemania
Max Planck Institute for Nuclear Physics - Alemania
Max-Planck-Institut für Kernphysik - Alemania
40 Valageas, P. - CEA DSM IPhT - Francia
CNRS - Francia
Institut de Physique Théorique, Gif-sur-Yvette - Francia
Commissariat a l'Energie Atomique et aux Energies Alternatives - Francia
41 Valtchanov, I. Hombre ESA - España
European Space Astronomy Centre - España
42 Willis, Jon P. Hombre Univ Victoria - Canadá
University of Victoria - Canadá
43 Ziparo, F. Mujer Univ Birmingham - Reino Unido
University of Birmingham - Reino Unido

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Origen de Citas Identificadas



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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 12.61 %
Citas No-identificadas: 87.39 %

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 12.61 %
Citas No-identificadas: 87.39 %

Financiamiento



Fuente
Deutsche Forschungsgemeinschaft
DFG
STFC
Science and Technology Facilities Council
National Aeronautics and Space Administration
Danish National Research Foundation
Danmarks Grundforskningsfond
European Space Agency
Ecological Society of America
Bundesministerium fur Wirtschaft und Energie
NASA/IPAC
Centre National d’Etudes Spatiales
Deutsches Zentrum für Luft- und Raumfahrt
Centre National d’Etudes Spatiales
IPAC
BMWi/DLR grant
DFG Heisenberg grant
BMWi/DLR
Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung

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Agradecimientos



Agradecimiento
XXL is an international project based around an XMM Very Large Programme surveying two 25 deg<SUP>2</SUP> extragalactic fields at a depth of similar to 5 x 10<SUP>-15</SUP> erg s<SUP>-1</SUP> cm<SUP>-2</SUP> in [0.5-2] keV. The XXL website is http://irfu.cea.fr/xxl. Multiband information and spectroscopic follow-up of the X-ray sources are obtained through a number of survey programmes, summarised at http://xxlmultiwave.pbworks.com/. This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This research has made use of ALADIN SKY ATLAS and SIMBAD database, both developed at CDS, Strasbourg Observatory, France. In particular, we would like to thank Thomas Boch for his help with ALADIN LITE. F.P. acknowledges support from the BMWi/DLR grant 50 OR 1117, the DFG grant RE 1462-6 and the DfG Transregio Programme TR33. T.R. acknowledges support from the DFG Heisenberg grant RE 1462-5. The Saclay group acknowledges long-term support by the Centre National d'Etudes Spatiales (CNES). The XXL team would also like to thank the VLT support astronomers C. Hummel and N. Neumayer for their dedicated help in the implementation of the XXL ESO Large Program and with the data reduction. The Dark Cosmology Centre is funded by the Danish National Research Foundation. B.J.M., P.A.G. and M.B. acknowledge support from STFC grants ST/J001414/1 and ST/M000907/1.
Based on observations obtained with XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA. Based on observations made with ESO Telescopes at the La Silla and Paranal Observatories under programme ID 089.A-0666 and LP191.A-0268. XXL is an international project based around an XMM Very Large Programme surveying two 25 deg2 extragalactic fields at a depth of ~5 × 10-15 erg s-1 cm-2 in [0.5-2] keV. The XXL website is http://irfu. cea.fr/xxl. Multiband information and spectroscopic follow-up of the X-ray sources are obtained through a number of survey programmes, summarised at http://xxlmultiwave.pbworks.com/. This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This research has made use of Aladin sky atlas and simbad database, both developed at CDS, Strasbourg Observatory, France. In particular, we would like to thank Thomas Boch for his help with Aladin Lite. F.P. acknowledges support from the BMWi/DLR grant 50 OR 1117, the DFG grant RE 1462-6 and the DfG Transregio Programme TR33. T.R. acknowledges support from the DFG Heisenberg grant RE 1462- 5. The Saclay group acknowledges long-term support by the Centre National d'Études Spatiales (CNES). The XXL team would also like to thank the VLT support astronomers C. Hummel and N. Neumayer for their dedicated help in the implementation of the XXL ESO Large Program and with the data reduction. The Dark Cosmology Centre is funded by the Danish National Research Foundation. B.J.M., P.A.G. and M.B. acknowledge support from STFC grants ST/J001414/1 and ST/M000907/1.

Muestra la fuente de financiamiento declarada en la publicación.