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Herschel-ATLAS: Evolution of the 250 µm luminosity function out to z = 0.5

dc.contributor.authorDye, S.
dc.contributor.authorDunne, L.
dc.contributor.authorEales, S.
dc.contributor.authorSmith, Daniel
dc.contributor.authorAmblard, A.
dc.contributor.authorAuld, R.
dc.contributor.authorBaes, M.
dc.contributor.authorBaldry, I.K.
dc.contributor.authorBamford, S.
dc.contributor.authorBlain, A.W.
dc.contributor.authorBonfield, D.
dc.contributor.authorBremer, M.
dc.contributor.authorBurgarella, D.
dc.contributor.authorButtiglione, S.
dc.contributor.authorCameron, E.
dc.contributor.authorCava, A.
dc.contributor.authorClements, D.
dc.contributor.authorCooray, A.
dc.contributor.authorCroom, S.
dc.contributor.authorDariush, A.
dc.contributor.authorde Zotti, G.
dc.contributor.authorDriver, S.
dc.contributor.authorDunlop, J.S.
dc.contributor.authorFrayer, D.
dc.contributor.authorFritz, J.
dc.contributor.authorGardner, J.P.
dc.contributor.authorGomez, H.L.
dc.contributor.authorGonzalez-Nuevo, J.
dc.contributor.authorHerranz, D.
dc.contributor.authorHill, D.
dc.contributor.authorHopkins, A.
dc.contributor.authorIbar, E.
dc.contributor.authorIvison, R.J.
dc.contributor.authorJarvis, M.J.
dc.contributor.authorJones, D.H.
dc.contributor.authorKelvin, L.
dc.contributor.authorLagache, G.
dc.contributor.authorLeeuw, L.
dc.contributor.authorLiske, J.
dc.contributor.authorLopez-Caniego, M.
dc.contributor.authorLoveday, J.
dc.contributor.authorMaddox, S.
dc.contributor.authorMichalowski, M.
dc.contributor.authorNegrello, M.
dc.contributor.authorNorberg, P.
dc.contributor.authorPage, M.J.
dc.contributor.authorParkinson, H.
dc.contributor.authorPascale, E.
dc.contributor.authorPeacock, J.A.
dc.contributor.authorPohlen, M.
dc.contributor.authorPopescu, C.
dc.contributor.authorPrescott, M.
dc.contributor.authorRigopoulou, D.
dc.contributor.authorRobotham, A.
dc.contributor.authorRigby, E.
dc.contributor.authorRodighiero, G.
dc.contributor.authorSamui, S.
dc.contributor.authorScott, D.
dc.contributor.authorSerjeant, S.
dc.contributor.authorSharp, R.G.
dc.contributor.authorSibthorpe, B.
dc.contributor.authorTemi, P.
dc.contributor.authorThompson, M.A.
dc.contributor.authorTuffs, R.
dc.contributor.authorValtchanov, I.
dc.contributor.authorvan der Werf, P.
dc.contributor.authorvan Kampen, E.
dc.contributor.authorVerma, A.
dc.date.accessioned2012-03-07T11:00:06Z
dc.date.available2012-03-07T11:00:06Z
dc.date.issued2010
dc.identifier.citationDye , S , Dunne , L , Eales , S , Smith , D , Amblard , A , Auld , R , Baes , M , Baldry , I K , Bamford , S , Blain , A W , Bonfield , D , Bremer , M , Burgarella , D , Buttiglione , S , Cameron , E , Cava , A , Clements , D , Cooray , A , Croom , S , Dariush , A , de Zotti , G , Driver , S , Dunlop , J S , Frayer , D , Fritz , J , Gardner , J P , Gomez , H L , Gonzalez-Nuevo , J , Herranz , D , Hill , D , Hopkins , A , Ibar , E , Ivison , R J , Jarvis , M J , Jones , D H , Kelvin , L , Lagache , G , Leeuw , L , Liske , J , Lopez-Caniego , M , Loveday , J , Maddox , S , Michalowski , M , Negrello , M , Norberg , P , Page , M J , Parkinson , H , Pascale , E , Peacock , J A , Pohlen , M , Popescu , C , Prescott , M , Rigopoulou , D , Robotham , A , Rigby , E , Rodighiero , G , Samui , S , Scott , D , Serjeant , S , Sharp , R G , Sibthorpe , B , Temi , P , Thompson , M A , Tuffs , R , Valtchanov , I , van der Werf , P , van Kampen , E & Verma , A 2010 , ' Herschel-ATLAS: Evolution of the 250 µm luminosity function out to z = 0.5 ' , Astronomy and Astrophysics , vol. 518 , L10 . https://doi.org/10.1051/0004-6361/201014614
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 158064
dc.identifier.otherPURE UUID: 1acfad5b-0c25-4a31-baf4-f413475e59c3
dc.identifier.otherdspace: 2299/4995
dc.identifier.otherScopus: 77954767657
dc.identifier.otherORCID: /0000-0001-5392-909X/work/30970847
dc.identifier.otherORCID: /0000-0001-9708-253X/work/69424325
dc.identifier.urihttp://hdl.handle.net/2299/7906
dc.descriptionOriginal article can be found at: http://www.aanda.org/ Copyright The European Southern Observatory
dc.description.abstractWe have determined the luminosity function of 250 μm-selected galaxies detected in the ~14 deg2 science demonstration region of the Herschel-ATLAS project out to a redshift of z = 0.5. Our findings very clearly show that the luminosity function evolves steadily out to this redshift. By selecting a sub-group of sources within a fixed luminosity interval where incompleteness effects are minimal, we have measured a smooth increase in the comoving 250 μm luminosity density out to z = 0.2 where it is 3.6+1.4-0.9 times higher than the local value.en
dc.language.isoeng
dc.relation.ispartofAstronomy and Astrophysics
dc.titleHerschel-ATLAS: Evolution of the 250 µm luminosity function out to z = 0.5en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1051/0004-6361/201014614
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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