H-ATLAS/GAMA : Quantifying the morphological evolution of the galaxy population using cosmic calorimetry
dc.contributor.author | Eales, Stephen | |
dc.contributor.author | Fullard, Andrew | |
dc.contributor.author | Allen, Matthew | |
dc.contributor.author | Smith, M. W. L. | |
dc.contributor.author | Baldry, Ivan | |
dc.contributor.author | Bourne, Nathan | |
dc.contributor.author | Clark, C. J. R. | |
dc.contributor.author | Driver, Simon | |
dc.contributor.author | Dunne, Loretta | |
dc.contributor.author | Dye, Simon | |
dc.contributor.author | Graham, Alister W. | |
dc.contributor.author | Ibar, Edo | |
dc.contributor.author | Hopkins, Andrew | |
dc.contributor.author | Ivison, Rob | |
dc.contributor.author | Kelvin, Lee S. | |
dc.contributor.author | Maddox, Steve | |
dc.contributor.author | Maraston, Claudia | |
dc.contributor.author | Robotham, Aaron S. G. | |
dc.contributor.author | Smith, Daniel | |
dc.contributor.author | Taylor, Edward N. | |
dc.contributor.author | Valiante, Elisabetta | |
dc.contributor.author | Werf, Paul van der | |
dc.contributor.author | Baes, Maarten | |
dc.contributor.author | Brough, Sarah | |
dc.contributor.author | Clements, David | |
dc.contributor.author | Cooray, Asantha | |
dc.contributor.author | Gomez, Haley | |
dc.contributor.author | Loveday, Jon | |
dc.contributor.author | Phillipps, Steven | |
dc.contributor.author | Scott, Douglas | |
dc.contributor.author | Serjeant, Steve | |
dc.date.accessioned | 2016-03-16T10:14:41Z | |
dc.date.available | 2016-03-16T10:14:41Z | |
dc.date.issued | 2015-10-01 | |
dc.identifier.citation | Eales , 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.issn | 0035-8711 | |
dc.identifier.other | ArXiv: http://arxiv.org/abs/1506.05466v2 | |
dc.identifier.other | ORCID: /0000-0001-9708-253X/work/69424333 | |
dc.identifier.uri | http://hdl.handle.net/2299/16794 | |
dc.description.abstract | Using 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 n | en |
dc.format.extent | 4618446 | |
dc.language.iso | eng | |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
dc.subject | astro-ph.GA | |
dc.subject | astro-ph.CO | |
dc.title | H-ATLAS/GAMA : Quantifying the morphological evolution of the galaxy population using cosmic calorimetry | en |
dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
dc.description.status | Peer reviewed | |
rioxxterms.versionofrecord | 10.1093/mnras/stv1300 | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true |