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The XMM Cluster Survey: predicted overlap with the Planck Cluster Catalogue

dc.contributor.authorViana, Pedro T. P.en_US
dc.contributor.authorDa Silva, Antónioen_US
dc.contributor.authorRamos, Elsa P. R. G.en_US
dc.contributor.authorLiddle, Andrew R.en_US
dc.contributor.authorLloyd‐davies, E. J.en_US
dc.contributor.authorRomer, A. Kathyen_US
dc.contributor.authorKay, Scott T.en_US
dc.contributor.authorCollins, Chris A.en_US
dc.contributor.authorHilton, Matten_US
dc.contributor.authorHosmer, Marken_US
dc.contributor.authorHoyle, Benen_US
dc.contributor.authorMayers, Julian A.en_US
dc.contributor.authorMehrtens, Nicolaen_US
dc.contributor.authorMiller, Christopher J.en_US
dc.contributor.authorSahlén, Martinen_US
dc.contributor.authorStanford, S. Adamen_US
dc.contributor.authorStott, John P.en_US
dc.date.accessioned2012-05-21T15:49:08Z
dc.date.available2013-07-01T14:33:05Zen_US
dc.date.issued2012-05-11en_US
dc.identifier.citationViana, Pedro T. P.; Da Silva, António ; Ramos, Elsa P. R. G.; Liddle, Andrew R.; Lloyd‐davies, E. J. ; Romer, A. Kathy; Kay, Scott T.; Collins, Chris A.; Hilton, Matt; Hosmer, Mark; Hoyle, Ben; Mayers, Julian A.; Mehrtens, Nicola; Miller, Christopher J.; Sahlén, Martin ; Stanford, S. Adam; Stott, John P. (2012). "The XMM Cluster Survey: predicted overlap with the Planck Cluster Catalogue." Monthly Notices of the Royal Astronomical Society 422(2). <http://hdl.handle.net/2027.42/91194>en_US
dc.identifier.issn0035-8711en_US
dc.identifier.issn1365-2966en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/91194
dc.description.abstractWe present a list of 15 clusters of galaxies, serendipitously detected by the XMM Cluster Survey (XCS), that have a high probability of detection by the Planck satellite. Three of them already appear in the Planck Early Sunyaev–Zel’dovich (ESZ) catalogue. The estimation of the Planck detection probability assumes the flat Lambda cold dark matter (ΛCDM) cosmology most compatible with 7‐year Wilkinson Microwave Anisotropy Probe ( WMAP 7) data. It takes into account the XCS selection function and Planck sensitivity, as well as the covariance of the cluster X‐ray luminosity, temperature and integrated Comptonization parameter, as a function of cluster mass and redshift, determined by the Millennium gas simulations. We also characterize the properties of the galaxy clusters in the final data release of the XCS that we expect Planck will have detected by the end of its extended mission. Finally, we briefly discuss possible joint applications of the XCS and Planck data.en_US
dc.publisherBlackwell Publishing Ltden_US
dc.publisherWiley Periodicals, Inc.en_US
dc.subject.otherGalaxies: Clusters: Generalen_US
dc.titleThe XMM Cluster Survey: predicted overlap with the Planck Cluster Catalogueen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelAstronomyen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumAstronomy Department, University of Michigan, Ann Arbor, MI 48109, USAen_US
dc.contributor.affiliationotherInstitute of Geophysics and Planetary Physics, Lawrence Livermore National Laboratory, Livermore, CA 94551, USAen_US
dc.contributor.affiliationotherCentro de Astrofísica, Universidade do Porto, Rua das Estrelas, 4150‐762 Porto, Portugalen_US
dc.contributor.affiliationotherDepartamento de Física e Astronomia, Faculdade de Ciências, Universidade do Porto, Rua do Campo Alegre, 687, 4169‐007 Porto, Portugalen_US
dc.contributor.affiliationotherAstronomy Centre, University of Sussex, Falmer, Brighton BN1 9QHen_US
dc.contributor.affiliationotherJodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PLen_US
dc.contributor.affiliationotherAstrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead CH41 1LDen_US
dc.contributor.affiliationotherSchool of Physics & Astronomy, University of Nottingham, Nottingham NG7 2RDen_US
dc.contributor.affiliationotherInstitut de Ciéncies del Cosmos (ICCUB‐IEEC), Departmento de Física, Martí i Franqués 1, 08034 Barcelona, Spainen_US
dc.contributor.affiliationotherInstitute of Cosmology and Gravitation, Dennis Sciama Building, Burnaby Road, Portsmouth PO1 3FXen_US
dc.contributor.affiliationotherHelsinki Institute of Physics, P.O. Box 64, University of Helsinki, FIN‐00014 Helsinki, Finlanden_US
dc.contributor.affiliationotherThe Oskar Klein Centre for Cosmoparticle Physics, Department of Physics, Stockholm University, SE‐106 91 Stockholm, Swedenen_US
dc.contributor.affiliationotherPhysics Department, University of California, Davis, CA 95616, USAen_US
dc.contributor.affiliationotherDepartment of Physics, Institute for Computational Cosmology, Durham University, South Road, Durham DH1 3LEen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/91194/1/j.1365-2966.2012.20673.x.pdf
dc.identifier.doi10.1111/j.1365-2966.2012.20673.xen_US
dc.identifier.sourceMonthly Notices of the Royal Astronomical Societyen_US
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dc.owningcollnameInterdisciplinary and Peer-Reviewed


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