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Distant galaxy clusters in the XMM Large Scale Structure survey

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 28 Jan 2013Embargo end date: 01 Jan 2012 English Publisher:Oxford University Press (OUP)Journal:Monthly Notices of the Royal Astronomical Society, volume 430, pages 134-156 (issn: 0035-8711, eissn: 1365-2966, Copyright policy )Funded by:NSERC | unidentified
Authors: Karun Thanjavur; C. Adami; Sophie Maurogordato; Stephen Gwyn; Jon Willis; Nicolas Clerc; Malcolm N. Bremer; +9 Authors

doi: 10.1093/mnras/sts540 , 10.48550/arxiv.1212.4185

arXiv: http://arxiv.org/abs/1212.4185

handle: 1983/fed0bb07-d298-4f07-831c-71e88a5d5ad5

Distant galaxy clusters in the XMM Large Scale Structure survey

Abstract

(Abridged) Distant galaxy clusters provide important tests of the growth of large scale structure in addition to highlighting the process of galaxy evolution in a consistently defined environment at large look back time. We present a sample of 22 distant (z>0.8) galaxy clusters and cluster candidates selected from the 9 deg2 footprint of the overlapping X-ray Multi Mirror (XMM) Large Scale Structure (LSS), CFHTLS Wide and Spitzer SWIRE surveys. Clusters are selected as extended X-ray sources with an accompanying overdensity of galaxies displaying optical to mid-infrared photometry consistent with z>0.8. Nine clusters have confirmed spectroscopic redshifts in the interval 0.80.8 clusters.

Accepted by MNRAS, 25 pages, 15 figures

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Keywords

Cosmology and Nongalactic Astrophysics (astro-ph.CO), astro-ph.CO, 500, FOS: Physical sciences, [SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph], 520, Astrophysics - Cosmology and Nongalactic Astrophysics

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    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
51
Top 10%
Top 10%
Top 10%
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gold
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