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dc.contributor.authorBleem, L. E.
dc.contributor.authorStalder, Brian A
dc.contributor.authorde Haan, T.
dc.contributor.authorAird, K. A.
dc.contributor.authorAllen, S. W.
dc.contributor.authorApplegate, D. E.
dc.contributor.authorAshby, Matthew L N
dc.contributor.authorBautz, M.
dc.contributor.authorBayliss, Matthew
dc.contributor.authorBenson, B. A.
dc.contributor.authorBocquet, S.
dc.contributor.authorBrodwin, M.
dc.contributor.authorCarlstrom, J. E.
dc.contributor.authorChang, C. L.
dc.contributor.authorChiu, I.
dc.contributor.authorCho, H. M.
dc.contributor.authorClocchiatti, A.
dc.contributor.authorCrawford, T. M.
dc.contributor.authorCrites, A. T.
dc.contributor.authorDesai, S.
dc.contributor.authorDietrich, J. P.
dc.contributor.authorDobbs, M. A.
dc.contributor.authorFoley, R. J.
dc.contributor.authorForman, William R.
dc.contributor.authorGeorge, E. M.
dc.contributor.authorGladders, M. D.
dc.contributor.authorGonzalez, A. H.
dc.contributor.authorHalverson, N. W.
dc.contributor.authorHennig, C.
dc.contributor.authorHoekstra, H.
dc.contributor.authorHolder, G. P.
dc.contributor.authorHolzapfel, W. L.
dc.contributor.authorHrubes, J. D.
dc.contributor.authorJones, C.
dc.contributor.authorKeisler, R.
dc.contributor.authorKnox, L.
dc.contributor.authorLee, A. T.
dc.contributor.authorLeitch, E. M.
dc.contributor.authorLiu, J.
dc.contributor.authorLueker, M.
dc.contributor.authorLuong-Van, D.
dc.contributor.authorMantz, A.
dc.contributor.authorMarrone, D. P.
dc.contributor.authorMcDonald, M.
dc.contributor.authorMcMahon, J. J.
dc.contributor.authorMeyer, S. S.
dc.contributor.authorMocanu, L.
dc.contributor.authorMohr, J. J.
dc.contributor.authorMurray, S. S.
dc.contributor.authorPadin, S.
dc.contributor.authorPryke, C.
dc.contributor.authorReichardt, C. L.
dc.contributor.authorRest, Armin Wolfgang
dc.contributor.authorRuel, J.
dc.contributor.authorRuhl, J. E.
dc.contributor.authorSaliwanchik, B. R.
dc.contributor.authorSaro, A.
dc.contributor.authorSayre, J. T.
dc.contributor.authorSchaffer, K. K.
dc.contributor.authorSchrabback, T.
dc.contributor.authorShirokoff, E.
dc.contributor.authorSong, J.
dc.contributor.authorSpieler, H. G.
dc.contributor.authorStanford, S. A.
dc.contributor.authorStaniszewski, Z.
dc.contributor.authorStark, Antony A.
dc.contributor.authorStory, K. T.
dc.contributor.authorStubbs, Christopher William
dc.contributor.authorVanderlinde, K.
dc.contributor.authorVieira, J. D.
dc.contributor.authorVikhlinin, Alexey A.
dc.contributor.authorWilliamson, R.
dc.contributor.authorZahn, O.
dc.contributor.authorZenteno, A.
dc.date.accessioned2015-06-12T18:39:29Z
dc.date.issued2015
dc.identifier.citationBleem, L. E., B. Stalder, T. de Haan, K. A. Aird, S. W. Allen, D. E. Applegate, M. L. N. Ashby, et al. 2015. “Galaxy Clusters Discovered via the Sunyaev-Zel'dovich Effect in the 2500-square-degree SPT-SZ survey.” The Astrophysical Journal Supplement Series 216, no. 2: 27. doi:10.1088/0067-0049/216/2/27en_US
dc.identifier.issn1538-4365en_US
dc.identifier.urihttp://nrs.harvard.edu/urn-3:HUL.InstRepos:16310008
dc.description.abstractWe present a catalog of galaxy clusters selected via their Sunyaev-Zel'dovich (SZ) effect signature from 2500 deg2 of South Pole Telescope (SPT) data. This work represents the complete sample of clusters detected at high significance in the 2500 deg2 SPT-SZ survey, which was completed in 2011. A total of 677 (409) cluster candidates are identified above a signal-to-noise threshold of ξ = 4.5 (5.0). Ground- and space-based optical and near-infrared (NIR) imaging confirms overdensities of similarly colored galaxies in the direction of 516 (or 76%) of the ξ > 4.5 candidates and 387 (or 95%) of the ξ > 5 candidates; the measured purity is consistent with expectations from simulations. Of these confirmed clusters, 415 were first identified in SPT data, including 251 new discoveries reported in this work. We estimate photometric redshifts for all candidates with identified optical and/or NIR counterparts; we additionally report redshifts derived from spectroscopic observations for 141 of these systems. The mass threshold of the catalog is roughly independent of redshift above z ~ 0.25 leading to a sample of massive clusters that extends to high redshift. The median mass of the sample is M 500c(ρcrit) $\sim 3.5\times 10^{14}\,M_\odot \,h_{70}^{-1}$, the median redshift is z med = 0.55, and the highest-redshift systems are at z > 1.4. The combination of large redshift extent, clean selection, and high typical mass makes this cluster sample of particular interest for cosmological analyses and studies of cluster formation and evolution.en_US
dc.description.sponsorshipPhysicsen_US
dc.language.isoen_USen_US
dc.publisherIOP Publishingen_US
dc.relation.isversionofdoi:10.1088/0067-0049/216/2/27en_US
dash.licenseOAP
dc.subjectcosmology: observationsen_US
dc.subjectgalaxies: clusters: individualen_US
dc.subjectlarge-scale structure of universeen_US
dc.titleGalaxy Clusters Discovered via the Sunyaev-Zel'dovich Effect in the 2500-square-degree SPT-SZ surveyen_US
dc.typeJournal Articleen_US
dc.description.versionAccepted Manuscripten_US
dc.relation.journalThe Astrophysical Journal Supplement Seriesen_US
dash.depositing.authorStubbs, Christopher William
dc.date.available2015-06-12T18:39:29Z
dc.identifier.doi10.1088/0067-0049/216/2/27*
dash.authorsorderedfalse
dash.contributor.affiliatedAshby, Matthew
dash.contributor.affiliatedStalder, Brian
dash.contributor.affiliatedBayliss, Matthew
dash.contributor.affiliatedForman, William
dash.contributor.affiliatedRest, Armin
dash.contributor.affiliatedViklinin, Alexey
dash.contributor.affiliatedStark, Antony
dash.contributor.affiliatedStubbs, Christopher


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