Dataciencia

Colección SciELO Chile

The XXL Survey XVI. The clustering of X-ray selected galaxy clusters at z ∼ 0.3

Indexado

WoS	WOS:000450930100001
Scopus	SCOPUS_ID:85057329819

DOI

10.1051/0004-6361/201833238

Año

2018

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

Results. Modelling the redshift-space clustering in the scale range 10 < r [h(-1) Mpc] < 40, we obtain Omega(M) = 0.27(0.04)(+0.06) and b(eff) = 2.73(0.20)(+0.18). This is the first time the two-point correlation function of an X-ray selected cluster catalogue at such relatively high redshifts and low masses has been measured. The XXL cluster clustering appears fully consistent with standard cosmological predictions. The analysis presented in this work demonstrates the feasibility of a cosmological exploitation of the XXL cluster clustering, paving the way for a combined analysis of XXL cluster number counts and clustering.

Revista

Revista	ISSN
Astronomy & Astrophysics	0004-6361

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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	Marulli, F.	Hombre	UNIV BOLOGNA - Italia INAF Osservatorio Astrofis & Sci Spazio Bologna - Italia INFN Sez Bologna - Italia Alma Mater Studiorum Università di Bologna - Italia INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia Istituto Nazionale di Fisica Nucleare, Sezione di Bologna - Italia
2	Veropalumbo, A.	-	Univ Roma Tre - Italia Università degli Studi Roma Tre - Italia
3	Sereno, M.	Hombre	UNIV BOLOGNA - Italia INAF Osservatorio Astrofis & Sci Spazio Bologna - Italia Alma Mater Studiorum Università di Bologna - Italia INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia
4	Moscardini, L.	-	UNIV BOLOGNA - Italia INAF Osservatorio Astrofis & Sci Spazio Bologna - Italia INFN Sez Bologna - Italia Alma Mater Studiorum Università di Bologna - Italia INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia Istituto Nazionale di Fisica Nucleare, Sezione di Bologna - Italia
5	Pacaud, F.	-	UNIV BONN - Alemania Universität Bonn - Alemania
6	Pierre, M.	-	Univ Paris Diderot - Francia Universite Paris-Saclay - Francia Astrophysique, Instrumentation et Modélisation de Paris-Saclay - Francia
7	Plionis, Manolis	Hombre	Lofos Nymphon - Grecia Aristotle Univ Thessaloniki - Grecia National Observatory of Athens - Grecia Aristotle University of Thessaloniki - Grecia
8	Cappi, A.	-	INAF Osservatorio Astrofis & Sci Spazio Bologna - Italia Univ Nice Sophia Antipolis - Francia INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia Université Nice Sophia Antipolis - Francia Laboratoire Joseph-Louis Lagrange - Francia
9	Adami, Christophe	Hombre	Aix Marseille Univ - Francia Laboratoire d'Astrophysique de Marseille - Francia
10	Alis, S.	-	Istanbul Univ - Turquía Istanbul Üniversitesi - Turquía
11	Altieri, B.	Hombre	European Space Astron Ctr - España European Space Astronomy Centre - España
12	Birkinshaw, Mark	Hombre	Univ Bristol - Reino Unido University of Bristol - Reino Unido
13	Ettori, S.	Hombre	INAF Osservatorio Astrofis & Sci Spazio Bologna - Italia INFN Sez Bologna - Italia INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia Istituto Nazionale di Fisica Nucleare, Sezione di Bologna - Italia
14	Faccioli, L.	-	Univ Paris Diderot - Francia Universite Paris-Saclay - Francia Astrophysique, Instrumentation et Modélisation de Paris-Saclay - Francia
15	Gastaldello, Fabio	Hombre	Ist Astrofis Spaziale & Fis Cosm Milano - Italia INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan - Italia
16	Koulouridis, E.	-	Univ Paris Diderot - Francia Universite Paris-Saclay - Francia Astrophysique, Instrumentation et Modélisation de Paris-Saclay - Francia
17	Lidman, Chris	Hombre	Australian Astron Observ - Australia Australian Natl Univ - Australia Australian Astronomical Observatory - Australia Australian National University - Australia The Australian National University - Australia
18	Le Fevre, J. P.	-	CEA Saclay - Francia
18	Le Fèvre, J. P.	-	CEA Saclay - Francia
19	Maurogordato, S.	-	Univ Nice Sophia Antipolis - Francia Université Nice Sophia Antipolis - Francia Laboratoire Joseph-Louis Lagrange - Francia
20	Poggianti, B.	Mujer	Istituto Nazionale di Astrofisica - Italia Osservatorio Astronomico di Padova - Italia INAF - Italia
21	Ségransan, Damien	Hombre	ESO - Chile European Southern Observatory Santiago - Chile
22	Sadibekova, T.	-	Univ Paris Diderot - Francia Uzbek Acad Sci - Uzbekistán Universite Paris-Saclay - Francia Ulugh Beg Astronomical Institute Uzbekistan Academy of Sciences - Uzbekistán Astrophysique, Instrumentation et Modélisation de Paris-Saclay - Francia
23	Valtchanov, I.	Hombre	European Space Astron Ctr - España European Space Astronomy Centre - España

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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: 6.06 %
Citas No-identificadas: 93.94 %

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

Citas Identificadas: 6.06 %
Citas No-identificadas: 93.94 %

Financiamiento

Fuente
Istanbul University
CNRS
STFC
ASI-INAF
CNES
Ministero dell’Istruzione, dell’Università e della Ricerca
Centre National de la Recherche Scientifique
Centre national d'etudes spatiales (CNES)
Ministero dellâIstruzione, dellâUniversitÃ e della Ricerca
College of Natural Resources and Sciences, Humboldt State University
Centre National d’Etudes Spatiales
Istanbul Üniversitesi
Centre National dâEtudes Spatiales
MIUR PRIN 2015
Istanbul Ãniversitesi

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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 6 x 10<SUP>-15</SUP> erg cm<SUP>-2</SUP> s<SUP>-1</SUP> in the [0.5-2] keV band for point-like sources. The XXL website is http://irfu.cea.fr/xxl. Multi-band information and spectroscopic follow-ups of the X-ray sources are obtained through a number of survey programmes, summarised at http://xxlmultiwave.pbworks.com/. We thank L. Chiappetti and M. Roncarelli for helpful comments. F.M. acknowledges support from the grant MIUR PRIN 2015 "Cosmology and Fundamental Physics: Illuminating the Dark Universe with Euclid". The Saclay group acknowledges long-term support from the Centre National d'Etudes Spatiales (CNES). S.E. acknowledges financial contribution from the contracts NARO15 ASI-INAF I/037/12/0, ASI 2015-046-R.0, and ASI-INAF n. 2017-14-H.0. S.A. acknowledges support from Istanbul University with the project number BEK-54547. E.K. thanks CNES and CNRS for support of post-doctoral research.
XXL is an international project based around an XMM Very Large Programme surveying two 25 deg2 extragalactic fields at a depth of ∼6 × 10-15 erg cm-2 s-1 in the [0.5-2] keV band for point-like sources. The XXL website is http://irfu.cea.fr/xxl. Multi-band information and spectroscopic follow-ups of the X-ray sources are obtained through a number of survey programmes, summarised at http://xxlmultiwave.pbworks.com/. We thank L. Chiappetti and M. Roncarelli for helpful comments. F.M. acknowledges support from the grant MIUR PRIN 2015 "Cosmology and Fundamental Physics: Illuminating the Dark Universe with Euclid". The Saclay group acknowledges long-term support from the Centre National d'Études Spatiales (CNES). S.E. acknowledges financial contribution from the contracts NARO15 ASI-INAF I/037/12/0, ASI 2015-046-R.0, and ASI-INAF n.2017-14-H.0. S.A. acknowledges support from Istanbul University with the project number BEK-54547. E.K. thanks CNES and CNRS for support of post-doctoral research.

Agradecimiento

XXL is an international project based around an XMM Very Large Programme surveying two 25 deg2 extragalactic fields at a depth of similar to 6 x 10-15 erg cm-2 s-1 in the [0.5-2] keV band for point-like sources. The XXL website is http://irfu.cea.fr/xxl. Multi-band information and spectroscopic follow-ups of the X-ray sources are obtained through a number of survey programmes, summarised at http://xxlmultiwave.pbworks.com/. We thank L. Chiappetti and M. Roncarelli for helpful comments. F.M. acknowledges support from the grant MIUR PRIN 2015 "Cosmology and Fundamental Physics: Illuminating the Dark Universe with Euclid". The Saclay group acknowledges long-term support from the Centre National d'Etudes Spatiales (CNES). S.E. acknowledges financial contribution from the contracts NARO15 ASI-INAF I/037/12/0, ASI 2015-046-R.0, and ASI-INAF n. 2017-14-H.0. S.A. acknowledges support from Istanbul University with the project number BEK-54547. E.K. thanks CNES and CNRS for support of post-doctoral research.

XXL is an international project based around an XMM Very Large Programme surveying two 25 deg2 extragalactic fields at a depth of ∼6 × 10-15 erg cm-2 s-1 in the [0.5-2] keV band for point-like sources. The XXL website is http://irfu.cea.fr/xxl. Multi-band information and spectroscopic follow-ups of the X-ray sources are obtained through a number of survey programmes, summarised at http://xxlmultiwave.pbworks.com/. We thank L. Chiappetti and M. Roncarelli for helpful comments. F.M. acknowledges support from the grant MIUR PRIN 2015 "Cosmology and Fundamental Physics: Illuminating the Dark Universe with Euclid". The Saclay group acknowledges long-term support from the Centre National d'Études Spatiales (CNES). S.E. acknowledges financial contribution from the contracts NARO15 ASI-INAF I/037/12/0, ASI 2015-046-R.0, and ASI-INAF n.2017-14-H.0. S.A. acknowledges support from Istanbul University with the project number BEK-54547. E.K. thanks CNES and CNRS for support of post-doctoral research.

Muestra la fuente de financiamiento declarada en la publicación.

Abstract

Revista

Métricas Externas

Disciplinas de Investigación

Colaboración Institucional

Autores - Afiliación

Origen de Citas Identificadas

Financiamiento

Agradecimientos

Departamento Gestión de Conocimiento, Monitoreo y Prospección