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dc.contributor.authorBrodwin, M.
dc.contributor.authorGreer, C. H.
dc.contributor.authorLeitch, E. M.
dc.contributor.authorStanford, S. A.
dc.contributor.authorGonzalez, A. H.
dc.contributor.authorGettings, D. P.
dc.contributor.authorAbdulla, Z.
dc.contributor.authorCarlstrom, J. E.
dc.contributor.authorDecker, B.
dc.contributor.authorEisenhardt, P. R.
dc.contributor.authorLin, H.-W.
dc.contributor.authorMantz, Adam B.
dc.contributor.authorMarrone, Daniel P.
dc.contributor.authorStalder, B.
dc.contributor.authorStern, D.
dc.contributor.authorWylezalek, D.
dc.contributor.authorMcDonald, Michael A.
dc.date.accessioned2015-09-01T20:36:34Z
dc.date.available2015-09-01T20:36:34Z
dc.date.issued2015-06
dc.date.submitted2014-10
dc.identifier.issn1538-4357
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1721.1/98312
dc.description.abstractWe present CARMA 30 GHz Sunyaev–Zel'dovich (SZ) observations of five high-redshift (z [> over ~] 1), infrared-selected galaxy clusters discovered as part of the all-sky Massive and Distant Clusters of WISE Survey (MaDCoWS). The SZ decrements measured toward these clusters demonstrate that the MaDCoWS selection is discovering evolved, massive galaxy clusters with hot intracluster gas. Using the SZ scaling relation calibrated with South Pole Telescope clusters at similar masses and redshifts, we find these MaDCoWS clusters have masses in the range M[subscript 200] ≈ 2-6 X 10[superscript 14] M[subscript ʘ. Three of these are among the most massive clusters found to date at z [> over ~] 1, demonstrating that MaDCoWS is sensitive to the most massive clusters to at least z = 1.3. The added depth of the AllWISE data release will allow all-sky infrared cluster detection to z ≈ 1.5 and beyond.en_US
dc.language.isoen_US
dc.publisherIOP Publishingen_US
dc.relation.isversionofhttp://dx.doi.org/10.1088/0004-637x/806/1/26en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceIOP Publishingen_US
dc.titleTHE MASSIVE AND DISTANT CLUSTERS OF WISE SURVEY. III. SUNYAEV-ZEL'DOVICH MASSES OF GALAXY CLUSTERS AT z ~ 1en_US
dc.typeArticleen_US
dc.identifier.citationBrodwin, M., C. H. Greer, E. M. Leitch, S. A. Stanford, A. H. Gonzalez, D. P. Gettings, Z. Abdulla, et al. “THE MASSIVE AND DISTANT CLUSTERS OF WISE SURVEY. III. SUNYAEV–ZEL’DOVICH MASSES OF GALAXY CLUSTERS AT z ~ 1.” The Astrophysical Journal 806, no. 1 (June 5, 2015): 26. © 2015 The American Astronomical Societyen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.mitauthorMcDonald, Michael A.en_US
dc.relation.journalThe Astrophysical Journalen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsBrodwin, M.; Greer, C. H.; Leitch, E. M.; Stanford, S. A.; Gonzalez, A. H.; Gettings, D. P.; Abdulla, Z.; Carlstrom, J. E.; Decker, B.; Eisenhardt, P. R.; Lin, H. W.; Mantz, A. B.; Marrone, D. P.; McDonald, M.; Stalder, B.; Stern, D.; Wylezalek, D.en_US
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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