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http://hdl.handle.net/20.500.12386/28299
Titolo: | The XXL Survey. XXV. Cosmological analysis of the C1 cluster number counts | Autori: | Pacaud, F. Pierre, M. Melin, J. -B. Adami, C. Evrard, A. E. Galli, S. GASTALDELLO, FABIO Maughan, B. J. Sereno, Mauro Alis, S. Altieri, B. Birkinshaw, M. CHIAPPETTI, LUCIO Faccioli, L. Giles, P. A. Horellou, C. IOVINO, Angela Koulouridis, E. Le Fèvre, J. -P. Lidman, C. Lieu, M. Maurogordato, S. Moscardini, L. Plionis, M. POGGIANTI, Bianca Maria Pompei, E. Sadibekova, T. Valtchanov, I. Willis, J. P. |
Data pubblicazione: | 2018 | Rivista: | ASTRONOMY & ASTROPHYSICS | Numero: | 620 | Da pagina:: | A10 | Abstract: | Context. We present an estimation of cosmological parameters with clusters of galaxies. <BR /> Aims: We constrain the Ω<SUB>m</SUB>, σ<SUB>8</SUB>, and w parameters from a stand-alone sample of X-ray clusters detected in the 50 deg<SUP>2</SUP> XMM-XXL survey with a well-defined selection function. <BR /> 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. <BR /> 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 Ω<SUB>m</SUB> = 0.316 ± 0.060, σ<SUB>8</SUB> = 0.814 ± 0.054, and w = -1.02 ± 0.20. <BR /> 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. Based on observations obtained with XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA. | URI: | http://hdl.handle.net/20.500.12386/28299 | URL: | https://www.aanda.org/articles/aa/abs/2018/12/aa34022-18/aa34022-18.html | ISSN: | 0004-6361 | DOI: | 10.1051/0004-6361/201834022 | Bibcode ADS: | 2018A&A...620A..10P | Fulltext: | open |
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