The XXL Survey: XXV. Cosmological analysis of the C1 cluster number counts
Reviewartikel, 2018

Context. We present an estimation of cosmological parameters with clusters of galaxies. Aims. We constrain the Ωm, σ8, and w parameters from a stand-alone sample of X-ray clusters detected in the 50 deg2 XMM-XXL survey with a well-defined selection function. Methods. We analyse the redshift distribution of a sample comprising 178 high signal-to-noise ratio clusters out to a redshift of unity. The cluster sample scaling relations are determined in a self-consistent manner. Results. In a lambda cold dark matter (ΛCDM) model, the cosmology favoured by the XXL clusters compares well with results derived from the Planck Sunyaev-Zel'dovich clusters for a totally different sample (mass/redshift range, selection biases, and scaling relations). However, with this preliminary sample and current mass calibration uncertainty, we find no inconsistency with the Planck CMB cosmology. If we relax the w parameter, the Planck CMB uncertainties increase by a factor of ~10 and become comparable with those from XXL clusters. Combining the two probes allows us to put constraints on Ωm = 0.316 ± 0.060, σ8 = 0.814 ± 0.054, and w = -1.02 ± 0.20. Conclusions. This first self-consistent cosmological analysis of a sample of serendipitous XMM clusters already provides interesting insights into the constraining power of the XXL survey. Subsequent analysis will use a larger sample extending to lower confidence detections and include additional observable information, potentially improving posterior uncertainties by roughly a factor of 3.

Surveys

Large-scale structure of Universe

X-rays: galaxies: clusters

Galaxies: clusters: intracluster medium

Cosmological parameters

Författare

F. Pacaud

Universität Bonn

M. Pierre

Université Paris-Saclay

J. B. Melin

Université Paris-Saclay

C. Adami

Laboratoire d'Astrophysique de Marseille

A. E. Evrard

University of Michigan

S. Galli

Institut d 'Astrophysique de Paris

F. Gastaldello

INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan

B. Maughan

University of Bristol

M. Sereno

INAF OAS Bologna

Universita di Bologna

S. Alis

Istanbul Universitesi

B. Altiéri

European Space Astronomy Centre (ESAC)

M. Birkinshaw

University of Bristol

L. Chiappetti

INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan

L. Faccioli

Université Paris-Saclay

P. Giles

University of Bristol

Cathy Horellou

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik, Extragalaktisk astrofysik

A. Iovino

Osservatorio Astronomico di Brera

E. Koulouridis

Université Paris-Saclay

J. P. Le Fevre

Institut de Recherche sur les Lois Fondamentales de l'Univers

C. Lidman

Australian National University

M. Lieu

European Space Astronomy Centre (ESAC)

S. Maurogordato

Université Nice Sophia Antipolis (UNS)

L. Moscardini

INAF OAS Bologna

Universita di Bologna

Istituto Nazionale Di Fisica Nucleare, Frascati

M. Plionis

National Observatory of Athens

Aristotelio Panepistimio Thessalonikis

B. M. Poggianti

Osservatorio Astronomico di Padova

E. Pompei

European Southern Observatory Santiago

T. Sadibekova

Université Paris-Saclay

I. Valtchanov

European Space Astronomy Centre (ESAC)

J. Willis

University of Victoria

Astronomy and Astrophysics

0004-6361 (ISSN) 1432-0746 (eISSN)

Vol. 620 A10

Ämneskategorier

Analytisk kemi

Astronomi, astrofysik och kosmologi

Sannolikhetsteori och statistik

DOI

10.1051/0004-6361/201834022

Mer information

Senast uppdaterat

2019-04-04