A structure in the early Universe at z similar to 1.3 that exceeds the homogeneity scale of the R-W concordance cosmology
Author
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Clowes, Roger G.
Author
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Harris, Kathryn A.
es_CL
Author
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Raghunathan, Srinivasan
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Author
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Campusano Brown, Luis
es_CL
Author
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Söchting, Ilona K.
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Author
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Graham, Matthew J.
es_CL
Admission date
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2014-01-24T14:06:08Z
Available date
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2014-01-24T14:06:08Z
Publication date
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2013-03
Cita de ítem
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MNRAS 429, 2910–2916 (2013)
en_US
Identifier
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doi:10.1093/mnras/sts497
Identifier
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https://repositorio.uchile.cl/handle/2250/126275
General note
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Artículo de publicación ISI.
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Abstract
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A 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.
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Patrocinador
dc.description.sponsorship
Center 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 England
en_US
Lenguage
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en
en_US
Publisher
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Oxford University Press on behalf of the Royal Astronomical Society