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The stellar masses of ~40 000 UV selected galaxies from the WiggleZ survey at 0.3 < z < 1.0: analogues of Lyman break galaxies?

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dc.contributor.authorBanerji, Manda
dc.contributor.authorGlazebrook, Karl
dc.contributor.authorBlake, Chris
dc.contributor.authorBrough, Sarah
dc.contributor.authorColless, Matthew
dc.contributor.authorContreras, Carlos
dc.contributor.authorCouch, Warrick
dc.contributor.authorCroton, Darren
dc.contributor.authorCroom, Scott M
dc.contributor.authorDavis, Tamara
dc.contributor.authorDrinkwater, Michael John
dc.contributor.authorSharp, Robert
dc.contributor.authorForster, Karl
dc.contributor.authorGilbank, David
dc.contributor.authorMadore, Barry
dc.contributor.authorWyder, Ted
dc.date.accessioned2015-12-13T22:28:51Z
dc.date.issued2013
dc.date.updated2016-02-24T09:21:21Z
dc.description.abstractWe characterize the stellar masses and star formation rates in a sample of ̃40 000 spectroscopically confirmed UV-luminous galaxies at 0.3<z<1.0 selected from within theWiggleZ Dark Energy Survey. In particular, we match this UV bright population t
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/74403
dc.publisherBlackwell Publishing Ltd
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Galaxies:Evolution; Galaxies:Formation; Galaxies:Stellar content.
dc.titleThe stellar masses of ~40 000 UV selected galaxies from the WiggleZ survey at 0.3 < z < 1.0: analogues of Lyman break galaxies?
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue3
local.bibliographicCitation.lastpage2229
local.bibliographicCitation.startpage2209
local.contributor.affiliationBanerji, Manda, University of Cambridge
local.contributor.affiliationGlazebrook, Karl, Swinburne University of Technology
local.contributor.affiliationBlake, Chris, Swinburne University of Technology
local.contributor.affiliationBrough, Sarah, Australian Astronomical Observatory
local.contributor.affiliationColless, Matthew, Australian Astronomical Observatory
local.contributor.affiliationContreras, Carlos, Swinburne University of Technology
local.contributor.affiliationCouch, Warrick, Swinburne University of Technology
local.contributor.affiliationCroton, Darren, Swinburne University of Technology
local.contributor.affiliationCroom, Scott M, University of Sydney
local.contributor.affiliationDavis, Tamara, University of Queensland
local.contributor.affiliationDrinkwater, Michael John, University of Queensland
local.contributor.affiliationSharp, Robert, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationForster, Karl, California Institute of Technology
local.contributor.affiliationGilbank, David, South African Astronomical Observatory
local.contributor.affiliationMadore, Barry, Observatories of the Carnegie Institution of Washington
local.contributor.affiliationWyder, Ted, California Institute of Technology
local.contributor.authoruidSharp, Robert, u4954956
local.description.notesImported from ARIES
local.identifier.absfor020103 - Cosmology and Extragalactic Astronomy
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
local.identifier.ariespublicationf5625xPUB4106
local.identifier.ariespublicationu4630950xPUB75
local.identifier.citationvolume431
local.identifier.doi10.1093/mnras/stt320
local.identifier.scopusID2-s2.0-84877077325
local.identifier.thomsonID000318347500015
local.type.statusPublished Version

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