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| 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
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.
| 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 |
| 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 |
| 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. |