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dc.contributor.authorWilkinson, A.
dc.contributor.authorAlmaini, O.
dc.contributor.authorChen, C.-C.
dc.contributor.authorSmail, I.
dc.contributor.authorArumugam, V.
dc.contributor.authorBlain, A.
dc.contributor.authorChapin, E.~L.
dc.contributor.authorChapman, S.~C.
dc.contributor.authorConselice, C.~J.
dc.contributor.authorCowley, W.~I.
dc.contributor.authorDunlop, J.~S.
dc.contributor.authorFarrah, D.
dc.contributor.authorGeach, J.
dc.contributor.authorHartley, W.~G.
dc.contributor.authorIvison, R.~J.
dc.contributor.authorMaltby, D.~T.
dc.contributor.authorMichalowski, M.~J.
dc.contributor.authorMortlock, A.
dc.contributor.authorScott, D.
dc.contributor.authorSimpson, C.
dc.contributor.authorSimpson, J.~M.
dc.contributor.authorvan der Werf, P.
dc.contributor.authorWild, V.
dc.date.accessioned2019-02-13T00:09:08Z
dc.date.available2019-02-13T00:09:08Z
dc.date.issued2017-01-11
dc.identifier.citationWilkinson , A , Almaini , O , Chen , C-C , Smail , I , Arumugam , V , Blain , A , Chapin , E L , Chapman , S C , Conselice , C J , Cowley , W I , Dunlop , J S , Farrah , D , Geach , J , Hartley , W G , Ivison , R J , Maltby , D T , Michalowski , M J , Mortlock , A , Scott , D , Simpson , C , Simpson , J M , van der Werf , P & Wild , V 2017 , ' The SCUBA-2 Cosmology Legacy Survey: the clustering of submillimetre galaxies in the UKIDSS UDS field ' Monthly Notices of the Royal Astronomical Society , vol. 464 , no. 2 , pp. 1380-1392 . https://doi.org/10.1093/mnras/stw2405
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 16294740
dc.identifier.otherPURE UUID: 02903558-57f2-4179-b236-4d7ff094baae
dc.identifier.otherBibtex: urn:6e22216c1350d75c100ab0f7a026b846
dc.identifier.otherScopus: 85014711756
dc.identifier.urihttp://hdl.handle.net/2299/21064
dc.description© 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society.
dc.description.abstractSubmillimetre galaxies (SMGs) are among the most luminous dusty galaxies in the Universe, but their true nature remains unclear; are SMGs the progenitors of the massive elliptical galaxies we see in the local Universe, or are they just a short-lived phase among more typical star-forming galaxies? To explore this problem further, we investigate the clustering of SMGs identified in the SCUBA-2 Cosmology Legacy Survey. We use a catalogue of submillimetre (850 μm) source identifications derived using a combination of radio counterparts and colour/infrared selection to analyse a sample of 610 SMG counterparts in the United Kingdom Infrared Telescope (UKIRT) Infrared Deep Survey (UKIDSS) Ultra Deep Survey (UDS), making this the largest high-redshift sample of these galaxies to date. Using angular cross-correlation techniques, we estimate the halo masses for this large sample of SMGs and compare them with passive and star-forming galaxies selected in the same field. We find that SMGs, on average, occupy high-mass dark matter haloes (Mhalo > 1013 M⊙) at redshifts z > 2.5, consistent with being the progenitors of massive quiescent galaxies in present-day galaxy clusters. We also find evidence of downsizing, in which SMG activity shifts to lower mass haloes at lower redshifts. In terms of their clustering and halo masses, SMGs appear to be consistent with other star-forming galaxies at a given redshift.en
dc.format.extent13
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectgalaxies: evolution, galaxies: formation, galaxies: high-redshift, galaxies: starburst, large-scale structure of Universe
dc.titleThe SCUBA-2 Cosmology Legacy Survey: the clustering of submillimetre galaxies in the UKIDSS UDS fielden
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted2016-09-21
rioxxterms.versionofrecordhttps://doi.org/10.1093/mnras/stw2405
rioxxterms.typeJournal Article/Review
herts.rights.accesstypeclosedAccess


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