Massive galaxies at redshifts 5 release

R. J. McLure, M. Cirasuolo, J. S. Dunlop

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

In this proceedings we report the findings of a search for bright Lyman-break galaxies (LBGs) at z > 5 using the UKIDSS Ultra Deep Survey (UDS) and Subaru/XMM-Newton Deep Survey (SXDS). Within the 0.6 square degree region covered by the SXDS and UDS early data release (EDR) we identify nine 5 < z < 6 LBG candidates brighter than z'(AB) = 25, corresponding to a surface density of 0.005 +/- 0.002 per square arcmin. Modelling of the optical+near-infrared photometry suggests that the typical stellar mass of the LBG candidates is greater than or similar to 5 x 10(10) M-circle dot, placing them amongst the most massive galaxies currently known at z >= 5. It is found that ACDM structure formation can produce sufficient numbers of dark matter halos at z >= 5 to accommodate our estimated number density of massive LBGs for plausible values Of sigma(8) and the ratio of stellar to dark matter. Moreover, it is found that recent galaxy formation models can also account for the existence of such massive galaxies at z >= 5.

Original languageEnglish
Title of host publicationAT THE EDGE OF THE UNIVERSE: LATEST RESULTS FROM THE DEEPEST ASTRONOMICAL SURVEYS
EditorsJ Afonso, HC Ferguson, B Mobasher, R Norris
Place of PublicationSAN FRANCISCO
PublisherASTRONOMICAL SOC PACIFIC
Pages321-326
Number of pages6
ISBN (Print)978-1-58381-323-2
Publication statusPublished - 2007
EventMeeting on At the Edge of the Universe - Sintra
Duration: 9 Oct 200613 Oct 2006

Conference

ConferenceMeeting on At the Edge of the Universe
CitySintra
Period9/10/0613/10/06

Fingerprint

Dive into the research topics of 'Massive galaxies at redshifts 5 release'. Together they form a unique fingerprint.

Cite this