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Authordc.contributor.authorHigh, F. W. 
Authordc.contributor.authorStalder, B. 
Authordc.contributor.authorSong, J. 
Authordc.contributor.authorAde, P. A.R. 
Authordc.contributor.authorAird, K. A. 
Authordc.contributor.authorAllam, S. S. 
Authordc.contributor.authorArmstrong, R. 
Authordc.contributor.authorBarkhouse, W. A. 
Authordc.contributor.authorBenson, B. A. 
Authordc.contributor.authorBertin, E. 
Authordc.contributor.authorBhattacharya, S. 
Authordc.contributor.authorBleem, L. E. 
Authordc.contributor.authorBrodwin, M. 
Authordc.contributor.authorBuckley-Geer, E. J. 
Authordc.contributor.authorCarlstrom, J. E. 
Authordc.contributor.authorChallis, P. 
Authordc.contributor.authorChang, C. L. 
Authordc.contributor.authorCrawford, T. M. 
Authordc.contributor.authorCrites, 
Admission datedc.date.accessioned2018-12-20T14:12:46Z
Available datedc.date.available2018-12-20T14:12:46Z
Publication datedc.date.issued2010
Cita de ítemdc.identifier.citationAstrophysical Journal, Volumen 723, Issue 2, 2018, Pages 1736-1747
Identifierdc.identifier.issn15384357
Identifierdc.identifier.issn0004637X
Identifierdc.identifier.other10.1088/0004-637X/723/2/1736
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/154799
Abstractdc.description.abstractWe present redshifts and optical richness properties of 21 galaxy clusters uniformly selected by their Sunyaev-Zel'dovich (SZ) signature. These clusters, plus an additional, unconfirmed candidate, were detected in a 178 deg 2 area surveyed by the South Pole Telescope (SPT) in 2008. Using griz imaging from the Blanco Cosmology Survey and from pointed Magellan telescope observations, as well as spectroscopy using Magellan facilities, we confirm the existence of clustered red-sequence galaxies, report red-sequence photometric redshifts, present spectroscopic redshifts for a subsample, and derive R 200 radii and M200 masses from optical richness. The clusters span redshifts from 0.15 to greater than 1, with a median redshift of 0.74; three clusters are estimated to be at z > 1. Redshifts inferred from mean red-sequence colors exhibit 2% rms scatter in σz/(1 + z) with respect to the spectroscopic subsample for z > 1. We show that the M200 cluster masses derived from optical richness correla
Lenguagedc.language.isoen
Publisherdc.publisherInstitute of Physics Publishing
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
Sourcedc.sourceAstrophysical Journal
Keywordsdc.subjectCosmology: observations
Keywordsdc.subjectGalaxies: clusters: general
Títulodc.titleOptical redshift and richness estimates for galaxy clusters selected with the Sunyaev-Zel'dovich effect from 2008 South Pole Telescope observations
Document typedc.typeArtículo de revista
Catalogueruchile.catalogadorSCOPUS
Indexationuchile.indexArtículo de publicación SCOPUS
uchile.cosechauchile.cosechaSI


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Attribution-NonCommercial-NoDerivs 3.0 Chile
Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 Chile