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3D-HST+CANDELS : the evolution of the galaxy size-mass distribution since z=3

dc.contributor.authorvan der Wel, A.
dc.contributor.authorFranx, M.
dc.contributor.authorvan Dokkum, P.G.
dc.contributor.authorSkelton, R.E.
dc.contributor.authorMomcheva, I.G.
dc.contributor.authorWhitaker, K.E.
dc.contributor.authorBrammer, G.B.
dc.contributor.authorBell, Eric F.
dc.contributor.authorRix, H-W.
dc.contributor.authorWuyts, Stijn
dc.contributor.authorFerguson, H. C.
dc.contributor.authorHolden, B.P.
dc.contributor.authorBarro, G.
dc.contributor.authorKoekemoer, A. M.
dc.contributor.authorChang, Yu-Yen
dc.contributor.authorMcGrath, E.J.
dc.contributor.authorHaussler, B.
dc.contributor.authorDekel, A.
dc.contributor.authorBehroozi, P.
dc.contributor.authorFumagalli, M.
dc.contributor.authorLeja, J.
dc.contributor.authorLundgren, B.F.
dc.contributor.authorMaseda, M.V.
dc.contributor.authorNelson, E.J.
dc.contributor.authorWake, D.A.
dc.contributor.authorPatel, S.G.
dc.contributor.authorLabbe, I.
dc.contributor.authorFaber, Sandra M.
dc.contributor.authorGrogin, N. A.
dc.contributor.authorKocevski, D.D.
dc.date.accessioned2015-09-10T10:58:43Z
dc.date.available2015-09-10T10:58:43Z
dc.date.issued2014-06-10
dc.identifier.citationvan der Wel , A , Franx , M , van Dokkum , P G , Skelton , R E , Momcheva , I G , Whitaker , K E , Brammer , G B , Bell , E F , Rix , H-W , Wuyts , S , Ferguson , H C , Holden , B P , Barro , G , Koekemoer , A M , Chang , Y-Y , McGrath , E J , Haussler , B , Dekel , A , Behroozi , P , Fumagalli , M , Leja , J , Lundgren , B F , Maseda , M V , Nelson , E J , Wake , D A , Patel , S G , Labbe , I , Faber , S M , Grogin , N A & Kocevski , D D 2014 , ' 3D-HST+CANDELS : the evolution of the galaxy size-mass distribution since z=3 ' , The Astrophysical Journal , vol. 788 , no. 1 , 28 . https://doi.org/10.1088/0004-637X/788/1/28
dc.identifier.issn0004-637X
dc.identifier.otherPURE: 9202049
dc.identifier.otherPURE UUID: 15c4d21c-21f8-4c26-b04d-2f506874628d
dc.identifier.otherScopus: 84901810801
dc.identifier.urihttp://hdl.handle.net/2299/16425
dc.description.abstractSpectroscopic+photometric redshifts, stellar mass estimates, and rest-frame colors from the 3D-HST survey are combined with structural parameter measurements from CANDELS imaging to determine the galaxy size-mass distribution over the redshift range 0 < z < 3. Separating early- and late-type galaxies on the basis of star-formation activity, we confirm that early-type galaxies are on average smaller than late-type galaxies at all redshifts, and we find a significantly different rate of average size evolution at fixed galaxy mass, with fast evolution for the early-type population, R eff∝(1 + z)–1.48, and moderate evolution for the late-type population, R eff∝(1 + z)-0.75en
dc.format.extent19
dc.language.isoeng
dc.relation.ispartofThe Astrophysical Journal
dc.title3D-HST+CANDELS : the evolution of the galaxy size-mass distribution since z=3en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1088/0004-637X/788/1/28
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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