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dc.contributor.authorElbaz, D.
dc.contributor.authorHwang, H. S.
dc.contributor.authorMagnelli, B.
dc.contributor.authorDaddi, E.
dc.contributor.authorAussel, H.
dc.contributor.authorAltieri, B.
dc.contributor.authorAmblard, A.
dc.contributor.authorAndreani, P.
dc.contributor.authorArumugam, V.
dc.contributor.authorAuld, R.
dc.contributor.authorBabbedge, T.
dc.contributor.authorBerta, S.
dc.contributor.authorBlain, A.
dc.contributor.authorBock, J.
dc.contributor.authorBongiovanni, A.
dc.contributor.authorBoselli, A.
dc.contributor.authorBuat, V.
dc.contributor.authorBurgarella, D.
dc.contributor.authorCastro-Rodriguez, N.
dc.contributor.authorCava, A.
dc.contributor.authorCepa, J.
dc.contributor.authorChanial, P.
dc.contributor.authorChary, R.-R.
dc.contributor.authorCimatti, A.
dc.contributor.authorClements, D. L.
dc.contributor.authorConley, A.
dc.contributor.authorConversi, L.
dc.contributor.authorCooray, A.
dc.contributor.authorDickinson, M.
dc.contributor.authorDominguez, H.
dc.contributor.authorDowell, C.D.
dc.contributor.authorDunlop, James S.
dc.contributor.authorDwek, E.
dc.contributor.authorEales, S.
dc.contributor.authorFarrah, D.
dc.contributor.authorFörster Schreiber, N.
dc.contributor.authorFox, M.
dc.contributor.authorFranceschini, A.
dc.contributor.authorGear, W.
dc.contributor.authorGenzel, R.
dc.contributor.authorGlenn, J.
dc.contributor.authorGriffin, M.
dc.contributor.authorGruppioni, C.
dc.contributor.authorHalpern, M.
dc.contributor.authorHatziminaoglou, E.
dc.contributor.authorIbar, E.
dc.contributor.authorIsaak, K.
dc.contributor.authorIvison, R.J.
dc.contributor.authorLagache, G.
dc.contributor.authorLe Borgne, D.
dc.contributor.authorLe Floc'h, E.
dc.contributor.authorLevenson, L.
dc.contributor.authorLu, N.
dc.contributor.authorLutz, D.
dc.contributor.authorMadden, S.
dc.contributor.authorMaffei, B.
dc.contributor.authorMagdis, G.
dc.contributor.authorMainetti, G.
dc.contributor.authorMaiolino, R.
dc.contributor.authorMarchetti, L.
dc.contributor.authorMortier, A. M. J.
dc.contributor.authorNguyen, H.T.
dc.contributor.authorNordon, R.
dc.contributor.authorO'Halloran, B.
dc.contributor.authorOkumura, K.
dc.contributor.authorOliver, S. J.
dc.contributor.authorOmont, A.
dc.contributor.authorPage, M.J.
dc.contributor.authorPanuzzo, P.
dc.contributor.authorPapageorgiou, A.
dc.contributor.authorPearson, C.P.
dc.contributor.authorPerez Fournon, I.
dc.contributor.authorGarcia Perez, Ana
dc.contributor.authorPoglitsch, A.
dc.contributor.authorPohlen, M.
dc.contributor.authorPopesso, P.
dc.contributor.authorPozzi, F.
dc.contributor.authorRawlings, J.I.
dc.contributor.authorRigopoulou, D.
dc.contributor.authorRiguccini, L.
dc.contributor.authorRizzo, D.
dc.contributor.authorRodighiero, G.
dc.contributor.authorRoseboom, I.G.
dc.contributor.authorRowan-Robinson, M.
dc.contributor.authorSaintonge, A.
dc.contributor.authorSanchez Portal, M.
dc.contributor.authorSantini, P.
dc.contributor.authorSauvage, M.
dc.contributor.authorSchulz, B.
dc.contributor.authorScott, D.
dc.contributor.authorSeymour, N.
dc.contributor.authorShao, L.
dc.contributor.authorShupe, D. L.
dc.contributor.authorSmith, A. J.
dc.contributor.authorStevens, Jason
dc.contributor.authorSturm, E.
dc.contributor.authorSymeonidis, M.
dc.contributor.authorTacconi, L.
dc.contributor.authorTrichas, M.
dc.contributor.authorTugwell, K.E.
dc.contributor.authorVaccari, M.
dc.contributor.authorValtchanov, I.
dc.contributor.authorVieira, J.
dc.contributor.authorVigroux, L.
dc.contributor.authorWang, L.
dc.contributor.authorWard, R.
dc.contributor.authorWright, G.
dc.contributor.authorXu, C.K.
dc.contributor.authorZemcov, M.
dc.date.accessioned2012-03-21T10:01:30Z
dc.date.available2012-03-21T10:01:30Z
dc.date.issued2010-07-01
dc.identifier.citationElbaz , D , Hwang , H S , Magnelli , B , Daddi , E , Aussel , H , Altieri , B , Amblard , A , Andreani , P , Arumugam , V , Auld , R , Babbedge , T , Berta , S , Blain , A , Bock , J , Bongiovanni , A , Boselli , A , Buat , V , Burgarella , D , Castro-Rodriguez , N , Cava , A , Cepa , J , Chanial , P , Chary , R-R , Cimatti , A , Clements , D L , Conley , A , Conversi , L , Cooray , A , Dickinson , M , Dominguez , H , Dowell , C D , Dunlop , J S , Dwek , E , Eales , S , Farrah , D , Förster Schreiber , N , Fox , M , Franceschini , A , Gear , W , Genzel , R , Glenn , J , Griffin , M , Gruppioni , C , Halpern , M , Hatziminaoglou , E , Ibar , E , Isaak , K , Ivison , R J , Lagache , G , Le Borgne , D , Le Floc'h , E , Levenson , L , Lu , N , Lutz , D , Madden , S , Maffei , B , Magdis , G , Mainetti , G , Maiolino , R , Marchetti , L , Mortier , A M J , Nguyen , H T , Nordon , R , O'Halloran , B , Okumura , K , Oliver , S J , Omont , A , Page , M J , Panuzzo , P , Papageorgiou , A , Pearson , C P , Perez Fournon , I , Garcia Perez , A , Poglitsch , A , Pohlen , M , Popesso , P , Pozzi , F , Rawlings , J I , Rigopoulou , D , Riguccini , L , Rizzo , D , Rodighiero , G , Roseboom , I G , Rowan-Robinson , M , Saintonge , A , Sanchez Portal , M , Santini , P , Sauvage , M , Schulz , B , Scott , D , Seymour , N , Shao , L , Shupe , D L , Smith , A J , Stevens , J , Sturm , E , Symeonidis , M , Tacconi , L , Trichas , M , Tugwell , K E , Vaccari , M , Valtchanov , I , Vieira , J , Vigroux , L , Wang , L , Ward , R , Wright , G , Xu , C K & Zemcov , M 2010 , ' Herschel unveils a puzzling uniformity of distant dusty galaxies ' , Astronomy & Astrophysics , vol. 518 , pp. L29 . https://doi.org/10.1051/0004-6361/201014687
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 519271
dc.identifier.otherPURE UUID: ff44be90-654e-4168-a625-3428ddb1c95d
dc.identifier.otherBibtex: urn:98f90fbca143f125fc281082890bcc3c
dc.identifier.otherScopus: 77957851369
dc.identifier.urihttp://hdl.handle.net/2299/8014
dc.description.abstractThe Herschel Space Observatory enables us to accurately measure the bolometric output of starburst galaxies and active galactic nuclei (AGN) by directly sampling the peak of their far-infrared (IR) emission. Here we examine whether the spectral energy distribution (SED) and dust temperature of galaxies have strongly evolved over the last 80% of the age of the Universe. We discuss possible consequences for the determination of star-formation rates (SFR) and any evidence for a major change in their star-formation properties. We use Herschel deep extragalactic surveys from 100 to 500 μm to compute total IR luminosities in galaxies down to the faintest levels, using PACS and SPIRE in the GOODS-North field (PEP and HerMES key programs). An extension to fainter luminosities is done by stacking images on 24 μm prior positions. We show that measurements in the SPIRE bands can be used below the statistical confusion limit if information at higher spatial resolution is used, e.g. at 24 μm, to identify “isolated” galaxies whose flux is not boosted by bright neighbors.en
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysics
dc.rightsOpen
dc.subjectgalaxies: evolution, galaxies: active, galaxies: starburst, infrared: galaxies
dc.titleHerschel unveils a puzzling uniformity of distant dusty galaxiesen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeFinal Accepted Version
dcterms.dateAccepted2010-07-01
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1051/0004-6361/201014687
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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