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dc.contributor.authorDrake, Alyssa B.
dc.contributor.authorSimpson, Chris
dc.contributor.authorBaldry, Ivan K.
dc.contributor.authorJames, Phil A.
dc.contributor.authorCollins, Chris A.
dc.contributor.authorOuchi, Masami
dc.contributor.authorYuma, Suraphong
dc.contributor.authorDunlop, James S.
dc.contributor.authorSmith, Daniel
dc.date.accessioned2016-03-16T10:14:36Z
dc.date.available2016-03-16T10:14:36Z
dc.date.issued2015-12-01
dc.identifier.citationDrake , A B , Simpson , C , Baldry , I K , James , P A , Collins , C A , Ouchi , M , Yuma , S , Dunlop , J S & Smith , D 2015 , ' Evolution of star formation in the UKIDSS Ultra Deep Survey Field - II : Star formation as a function of stellar mass between z=1.46 and z=0.63 ' , Monthly Notices of the Royal Astronomical Society , vol. 454 , no. 2 , pp. 2015-2025 . https://doi.org/10.1093/mnras/stv2027
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 9717791
dc.identifier.otherPURE UUID: 79cabdf7-8d68-4b59-aaa6-229acc75de2a
dc.identifier.otherArXiv: http://arxiv.org/abs/1509.06900v1
dc.identifier.otherScopus: 84963559841
dc.identifier.urihttp://hdl.handle.net/2299/16792
dc.description.abstractWe present new results on the evolution of the cosmic star formation rate as a function of stellar mass in the SXDS-UDS field. We make use of narrow-band selected emission line galaxies in four redshift slices between z = 1.46 and z = 0.63, and compute stellar masses by fitting a series of templates to recreate each galaxy's star formation history. We determine mass-binned luminosity functions in each redshift slice, and derive the star formation rate density (rhoSFR) as a function of mass using the [OIII] or [OII] emission lines. We calculate dust extinction and metallicity as a function of stellar mass, and investigate the effect of these corrections on the shape of the overall rhoSFR(M). We find that both these corrections are crucial for determining the shape of the rhoSFR(M), and its evolution with redshift. The fully corrected rhoSFR(M) is a relatively flat distribution, with the normalisation moving towards lower values of rhoSFR with increasing cosmic time/decreasing redshift, and requiring star formation to be truncated across all masses studied here. The peak of rhoSFR(M) is found in the 10^10.5Msun10^7.0Msunen
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.rights/dk/atira/pure/core/openaccesspermission/open
dc.subjectastro-ph.GA
dc.subjectastro-ph.CO
dc.titleEvolution of star formation in the UKIDSS Ultra Deep Survey Field - II : Star formation as a function of stellar mass between z=1.46 and z=0.63en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeFinal Accepted Version
dcterms.dateAccepted2015-09-01
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1093/mnras/stv2027
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeopenAccess


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