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H-ATLAS/GAMA : Quantifying the morphological evolution of the galaxy population using cosmic calorimetry

dc.contributor.authorEales, Stephen
dc.contributor.authorFullard, Andrew
dc.contributor.authorAllen, Matthew
dc.contributor.authorSmith, M. W. L.
dc.contributor.authorBaldry, Ivan
dc.contributor.authorBourne, Nathan
dc.contributor.authorClark, C. J. R.
dc.contributor.authorDriver, Simon
dc.contributor.authorDunne, Loretta
dc.contributor.authorDye, Simon
dc.contributor.authorGraham, Alister W.
dc.contributor.authorIbar, Edo
dc.contributor.authorHopkins, Andrew
dc.contributor.authorIvison, Rob
dc.contributor.authorKelvin, Lee S.
dc.contributor.authorMaddox, Steve
dc.contributor.authorMaraston, Claudia
dc.contributor.authorRobotham, Aaron S. G.
dc.contributor.authorSmith, Daniel
dc.contributor.authorTaylor, Edward N.
dc.contributor.authorValiante, Elisabetta
dc.contributor.authorWerf, Paul van der
dc.contributor.authorBaes, Maarten
dc.contributor.authorBrough, Sarah
dc.contributor.authorClements, David
dc.contributor.authorCooray, Asantha
dc.contributor.authorGomez, Haley
dc.contributor.authorLoveday, Jon
dc.contributor.authorPhillipps, Steven
dc.contributor.authorScott, Douglas
dc.contributor.authorSerjeant, Steve
dc.date.accessioned2016-03-16T10:14:41Z
dc.date.available2016-03-16T10:14:41Z
dc.date.issued2015-10-01
dc.identifier.citationEales , S , Fullard , A , Allen , M , Smith , M W L , Baldry , I , Bourne , N , Clark , C J R , Driver , S , Dunne , L , Dye , S , Graham , A W , Ibar , E , Hopkins , A , Ivison , R , Kelvin , L S , Maddox , S , Maraston , C , Robotham , A S G , Smith , D , Taylor , E N , Valiante , E , Werf , P V D , Baes , M , Brough , S , Clements , D , Cooray , A , Gomez , H , Loveday , J , Phillipps , S , Scott , D & Serjeant , S 2015 , ' H-ATLAS/GAMA : Quantifying the morphological evolution of the galaxy population using cosmic calorimetry ' , Monthly Notices of the Royal Astronomical Society , vol. 452 , no. 4 , pp. 3489-3507 . https://doi.org/10.1093/mnras/stv1300
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 9717979
dc.identifier.otherPURE UUID: 9d63b646-3a23-4d11-83b5-dc8e7c739179
dc.identifier.otherArXiv: http://arxiv.org/abs/1506.05466v2
dc.identifier.otherScopus: 84940118233
dc.identifier.otherORCID: /0000-0001-9708-253X/work/69424333
dc.identifier.urihttp://hdl.handle.net/2299/16794
dc.description.abstractUsing results from the Herschel Astrophysical Terrahertz Large-Area Survey and the Galaxy and Mass Assembly project, we show that, for galaxy masses above approximately 1.0e8 solar masses, 51% of the stellar mass-density in the local Universe is in early-type galaxies (ETGs: Sersic n > 2.5) while 89% of the rate of production of stellar mass-density is occurring in late-type galaxies (LTGs: Sersic nen
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectastro-ph.GA
dc.subjectastro-ph.CO
dc.titleH-ATLAS/GAMA : Quantifying the morphological evolution of the galaxy population using cosmic calorimetryen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1093/mnras/stv1300
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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