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.
X-rays: galaxies: clusters
Large-scale structure of Universe
Galaxies: clusters: intracluster medium
Cosmological parameters
Surveys
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
Universita di Bologna
INAF OAS 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
Istituto Nazionale di Fisica Nucleare
Universita di Bologna
INAF OAS Bologna
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 A10Ämneskategorier
Analytisk kemi
Astronomi, astrofysik och kosmologi
Sannolikhetsteori och statistik
DOI
10.1051/0004-6361/201834022