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The XMM Cluster Survey: X‐ray analysis methodology
dc.contributor.authorLloyd‐davies, E. J.en_US
dc.contributor.authorRomer, A. Kathyen_US
dc.contributor.authorMehrtens, Nicolaen_US
dc.contributor.authorHosmer, Marken_US
dc.contributor.authorDavidson, Michaelen_US
dc.contributor.authorSabirli, Kivancen_US
dc.contributor.authorMann, Robert G.en_US
dc.contributor.authorHilton, Matten_US
dc.contributor.authorLiddle, Andrew R.en_US
dc.contributor.authorViana, Pedro T. P.en_US
dc.contributor.authorCampbell, Heather C.en_US
dc.contributor.authorCollins, Chris A.en_US
dc.contributor.authorDubois, E. Naomien_US
dc.contributor.authorFreeman, Peteren_US
dc.contributor.authorHarrison, Craig D.en_US
dc.contributor.authorHoyle, Benen_US
dc.contributor.authorKay, Scott T.en_US
dc.contributor.authorKuwertz, Emmaen_US
dc.contributor.authorMiller, Christopher J.en_US
dc.contributor.authorNichol, Robert C.en_US
dc.contributor.authorSahlén, Martinen_US
dc.contributor.authorStanford, S. A.en_US
dc.contributor.authorStott, John P.en_US
dc.date.accessioned2011-12-05T18:32:40Z
dc.date.available2013-01-02T16:32:48Zen_US
dc.date.issued2011-11-21en_US
dc.identifier.citationLloyd‐davies, E. J. ; Romer, A. Kathy; Mehrtens, Nicola; Hosmer, Mark; Davidson, Michael; Sabirli, Kivanc; Mann, Robert G.; Hilton, Matt; Liddle, Andrew R.; Viana, Pedro T. P.; Campbell, Heather C.; Collins, Chris A.; Dubois, E. Naomi; Freeman, Peter; Harrison, Craig D.; Hoyle, Ben; Kay, Scott T.; Kuwertz, Emma; Miller, Christopher J.; Nichol, Robert C.; Sahlén, Martin ; Stanford, S. A.; Stott, John P. (2011). "The XMM Cluster Survey: Xâ ray analysis methodology." Monthly Notices of the Royal Astronomical Society 418(1). <http://hdl.handle.net/2027.42/88033>en_US
dc.identifier.issn0035-8711en_US
dc.identifier.issn1365-2966en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/88033
dc.description.abstractThe XMM Cluster Survey (XCS) is a serendipitous search for galaxy clusters using all publicly available data in the XMM–Newton Science Archive. Its main aims are to measure cosmological parameters and trace the evolution of X‐ray scaling relations. In this paper we describe the data processing methodology applied to the 5776  XMM observations used to construct the current XCS source catalogue. A total of 3675 > 4σ cluster candidates with >50 background‐subtracted X‐ray counts are extracted from a total non‐overlapping area suitable for cluster searching of 410 deg 2 . Of these, 993  candidates are detected with >300 background‐subtracted X‐ray photon counts, and we demonstrate that robust temperature measurements can be obtained down to this count limit. We describe in detail the automated pipelines used to perform the spectral and surface brightness fitting for these candidates, as well as to estimate redshifts from the X‐ray data alone. A total of 587  (122) X‐ray temperatures to a typical accuracy of <40 (<10) per cent have been measured to date. We also present the methodology adopted for determining the selection function of the survey, and show that the extended source detection algorithm is robust to a range of cluster morphologies by inserting mock clusters derived from hydrodynamical simulations into real XMM images. These tests show that the simple isothermal β‐profiles is sufficient to capture the essential details of the cluster population detected in the archival XMM observations. The redshift follow‐up of the XCS cluster sample is presented in a companion paper, together with a first data release of 503  optically confirmed clusters.en_US
dc.publisherBlackwell Publishing Ltden_US
dc.publisherWiley Periodicals, Inc.en_US
dc.subject.otherSurveysen_US
dc.subject.otherGalaxies: Clusters: Intracluster Mediumen_US
dc.subject.otherCosmology: Observationsen_US
dc.subject.otherX‐Rays: Galaxies: Clustersen_US
dc.titleThe XMM Cluster Survey: X‐ray analysis methodologyen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelAstronomyen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Astronomy, University of Michigan, Ann Arbor, MI 48109, USAen_US
dc.contributor.affiliationotherAstronomy Centre, University of Sussex, Falmer, Brighton BN1 9QHen_US
dc.contributor.affiliationotherSUPA, Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh EH9 3HJen_US
dc.contributor.affiliationotherDepartment of Physics, Carnegie Mellon University, 5000 Forbes Avenue, Pittsburgh, PA 15213, USAen_US
dc.contributor.affiliationotherSchool of Mathematical Sciences, University of KwaZulu‐Natal, Private Bag X54001, Durban 4000, South Africaen_US
dc.contributor.affiliationotherSchool of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RDen_US
dc.contributor.affiliationotherCentro de Astrofísica da Universidade do Porto, Rua das Estrelas, 4150‐762 Porto, Portugalen_US
dc.contributor.affiliationotherDepartamento de Física e Astronomia, Faculdade de Ciências, Universidade do Porto, 4169‐007 Porto, Portugalen_US
dc.contributor.affiliationotherInstitute of Cosmology and Gravitation, Dennis Sciama Building, Burnaby Road, Portsmouth PO1 3FXen_US
dc.contributor.affiliationotherAstrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead CH41 1LDen_US
dc.contributor.affiliationotherDepartment of Statistics, Carnegie Mellon University, 5000 Forbes Avenue, Pittsburgh, PA 15213, USAen_US
dc.contributor.affiliationotherInstitute of Sciences of the Cosmos (ICCUB‐IEEC), Department of Physics, University of Barcelona, Barcelona 08024, Spainen_US
dc.contributor.affiliationotherCSIC, Consejo Superior de Investigaciones Cientiþcas, Serrano 117, Madrid 28006, Spainen_US
dc.contributor.affiliationotherHelsinki Institute of Physics, University of Helsinki, PO Box 64, FIN‐00014 Helsinki, Finlanden_US
dc.contributor.affiliationotherJodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PLen_US
dc.contributor.affiliationotherThe Oskar Klein Centre for Cosmoparticle Physics, Department of Physics, Stockholm University, SE‐106 91 Stockholm, Swedenen_US
dc.contributor.affiliationotherDepartment of Physics, University of California, Davis, CA 95616, USAen_US
dc.contributor.affiliationotherInstitute of Geophysics and Planetary Physics, Lawrence Livermore National Laboratory, Livermore, CA 94551, USAen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/88033/1/j.1365-2966.2011.19117.x.pdf
dc.identifier.doi10.1111/j.1365-2966.2011.19117.xen_US
dc.identifier.sourceMonthly Notices of the Royal Astronomical Societyen_US
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