Ultra Deep Catalogue of Galaxy Structures in the Cosmic Evolution Survey field
Author
dc.contributor.author
Söchting, Ilona K.
Author
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Coldwell, Georgina V.
es_CL
Author
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Clowes, Roger G.
es_CL
Author
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Campusano Brown, Luis
es_CL
Author
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Graham, Matthew J.
es_CL
Admission date
dc.date.accessioned
2014-01-10T15:28:14Z
Available date
dc.date.available
2014-01-10T15:28:14Z
Publication date
dc.date.issued
2012-04-03
Cita de ítem
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Mon. Not. R. Astron. Soc. 423, 2436–2450 (2012)
en_US
Identifier
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doi:10.1111/j.1365-2966.2012.21050.x
Identifier
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https://repositorio.uchile.cl/handle/2250/126182
General note
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Artículo de publicación ISI.
en_US
Abstract
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detected using a fully automated search in the Cosmic Evolution Survey field. The detection
algorithm is based on density peak extraction from a density distribution sampled usingVoronoi
tessellation within overlapping slices in the photometric redshift space. The cluster catalogue
contains 1780 structures covering the redshift range 0.2 < z < 3.0, spanning three orders of
magnitude in luminosity (108 < L4 < 5 × 1011 L ) and richness from eight to hundreds of
galaxies. All clusters at z > 0.4 and many even below this threshold show very prominent
substructure indicating that z∼0.4marks the slow emergence of virialized clusters in this field
in agreement with published findings for other regions of the sky. The redshift distribution of
detected structures shows strong variations with prominent peaks suggesting the presence of
large-scale structures across the whole range covered by this catalogue. Supercluster candidates
have been identified at redshifts z = 0.35, 0.72, 0.94, 1.12, 1.27, 1.45, 2.0 and 2.52. At z = 2.9
we identified a compact agglomeration of galaxy groups and clusters suggesting the presence
of another supercluster-like structure which has been the highest redshift candidate so far. Out
of the nine supercluster candidates found in this study, six are new detections.