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Authordc.contributor.authorClowes, Roger G. 
Authordc.contributor.authorHarris, Kathryn A. es_CL
Authordc.contributor.authorRaghunathan, Srinivasan es_CL
Authordc.contributor.authorCampusano Brown, Luis es_CL
Authordc.contributor.authorSöchting, Ilona K. es_CL
Authordc.contributor.authorGraham, Matthew J. es_CL
Admission datedc.date.accessioned2014-01-24T14:06:08Z
Available datedc.date.available2014-01-24T14:06:08Z
Publication datedc.date.issued2013-03
Cita de ítemdc.identifier.citationMNRAS 429, 2910–2916 (2013)en_US
Identifierdc.identifier.otherdoi:10.1093/mnras/sts497
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/126275
General notedc.descriptionArtículo de publicación ISI.en_US
Abstractdc.description.abstractA large quasar group (LQG) of particularly large size and high membership has been identified in the DR7QSO catalogue of the Sloan Digital Sky Survey. It has characteristic size (volume(1/3)) similar to 500 Mpc (proper size, present epoch), longest dimension similar to 1240 Mpc, membership of 73 quasars and mean redshift (z) over bar = 1.27. In terms of both size and membership, it is the most extreme LQG found in the DR7QSO catalogue for the redshift range 1.0 <= z <= 1.8 of our current investigation. Its location on the sky is similar to 8 degrees.8 north (degrees 615 Mpc projected) of the Clowes & Campusano LQG at the same redshift, (z) over bar = 1.28, which is itself one of the more extreme examples. Their boundaries approach to within similar to 2 degrees (similar to 140 Mpc projected). This new, Huge-LQG appears to be the largest structure currently known in the early Universe. Its size suggests incompatibility with the Yadav et al. scale of homogeneity for the concordance cosmology, and thus challenges the assumption of the cosmological principle.en_US
Patrocinadordc.description.sponsorshipCenter of Excellence in Astrophysics and Associated Technologies (PFB 06), and from a CONICYT Anillo project (ACT 1122). SR is in receipt of a CONICYT PhD studentship. The referee, Maret Einasto, is thanked for helpful comments. This research has used the SDSS DR7QSO catalogue (Schneider et al. 2010). Funding for the SDSS and SDSSII has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the U.S. Department of Energy, the National Aeronautics and Space Administration, the Japanese Monbukagakusho, the Max Planck Society and the Higher Education Funding Council for Englanden_US
Lenguagedc.language.isoenen_US
Publisherdc.publisherOxford University Press on behalf of the Royal Astronomical Societyen_US
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile*
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/*
Keywordsdc.subjectgalaxies: clusters: generalen_US
Títulodc.titleA structure in the early Universe at z similar to 1.3 that exceeds the homogeneity scale of the R-W concordance cosmologyen_US
Document typedc.typeArtículo de revista


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