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dc.contributor.authorRowan-Robinson, M.
dc.contributor.authorRoseboom, I.G.
dc.contributor.authorVaccari, M.
dc.contributor.authorAmblard, A.
dc.contributor.authorArumugam, V.
dc.contributor.authorAuld, R.
dc.contributor.authorAussel, H.
dc.contributor.authorBabbedge, T.
dc.contributor.authorBlain, A.
dc.contributor.authorBock, J.
dc.contributor.authorBoselli, A.
dc.contributor.authorBrisbin, D.
dc.contributor.authorBuat, V.
dc.contributor.authorBurgarella, D.
dc.contributor.authorCastro-Rodriguez, N.
dc.contributor.authorCava, A.
dc.contributor.authorChanial, P.
dc.contributor.authorClements, D. L.
dc.contributor.authorConley, A.
dc.contributor.authorConversi, L.
dc.contributor.authorCooray, A.
dc.contributor.authorDowell, C.D.
dc.contributor.authorDwek, E.
dc.contributor.authorDye, S.
dc.contributor.authorEales, S.
dc.contributor.authorElbaz, D.
dc.contributor.authorFarrah, D.
dc.contributor.authorFox, M.
dc.contributor.authorFranceschini, A.
dc.contributor.authorGear, W.
dc.contributor.authorGlenn, J.
dc.contributor.authorGonzález Solares, E.A.
dc.contributor.authorGriffin, M.
dc.contributor.authorHalpern, M.
dc.contributor.authorHatziminaoglou, E.
dc.contributor.authorHuang, J.
dc.contributor.authorIbar, E.
dc.contributor.authorIsaak, K.
dc.contributor.authorIvison, Rob J.
dc.contributor.authorLagache, G.
dc.contributor.authorLevenson, L.
dc.contributor.authorLu, N.
dc.contributor.authorMadden, S.
dc.contributor.authorMaffei, B.
dc.contributor.authorMainetti, G.
dc.contributor.authorMarchetti, L.
dc.contributor.authorMortier, Angela M. J.
dc.contributor.authorNguyen, H.T.
dc.contributor.authorO'Halloran, B.
dc.contributor.authorOliver, S.J.
dc.contributor.authorOmont, A.
dc.contributor.authorPage, M. J.
dc.contributor.authorPanuzzo, P.
dc.contributor.authorPapageorgiou, A.
dc.contributor.authorPatel, H.
dc.contributor.authorPearson, C.P.
dc.contributor.authorPerez Fournon, I.
dc.contributor.authorPohlen, M.
dc.contributor.authorRawlings, J.I.
dc.contributor.authorRaymond, G.
dc.contributor.authorRigopoulou, D.
dc.contributor.authorRizzo, D.
dc.contributor.authorSchulz, B.
dc.contributor.authorScott, D.
dc.contributor.authorSeymour, N.
dc.contributor.authorShupe, D. L.
dc.contributor.authorSmith, A. J.
dc.contributor.authorStevens, Jason
dc.contributor.authorSymeonidis, M.
dc.contributor.authorTrichas, M.
dc.contributor.authorTugwell, K.E.
dc.contributor.authorValtchanov, I.
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.accessioned2012-01-16T10:01:28Z
dc.date.available2012-01-16T10:01:28Z
dc.date.issued2010-11-01
dc.identifier.citationRowan-Robinson , M , Roseboom , I G , Vaccari , M , Amblard , A , Arumugam , V , Auld , R , Aussel , H , Babbedge , T , Blain , A , Bock , J , Boselli , A , Brisbin , D , Buat , V , Burgarella , D , Castro-Rodriguez , N , Cava , A , Chanial , P , Clements , D L , Conley , A , Conversi , L , Cooray , A , Dowell , C D , Dwek , E , Dye , S , Eales , S , Elbaz , D , Farrah , D , Fox , M , Franceschini , A , Gear , W , Glenn , J , González Solares , E A , Griffin , M , Halpern , M , Hatziminaoglou , E , Huang , J , Ibar , E , Isaak , K , Ivison , R J , Lagache , G , Levenson , L , Lu , N , Madden , S , Maffei , B , Mainetti , G , Marchetti , L , Mortier , A M J , Nguyen , H T , O'Halloran , B , Oliver , S J , Omont , A , Page , M J , Panuzzo , P , Papageorgiou , A , Patel , H , Pearson , C P , Perez Fournon , I , Pohlen , M , Rawlings , J I , Raymond , G , Rigopoulou , D , Rizzo , D , Schulz , B , Scott , D , Seymour , N , Shupe , D L , Smith , A J , Stevens , J , Symeonidis , M , Trichas , M , Tugwell , K E , Valtchanov , I , Vigroux , L , Wang , L , Ward , R , Wright , G , Xu , C K & Zemcov , M 2010 , ' Cold dust and young starbursts : spectral energy distributions of Herschel SPIRE sources from the HerMES survey ' , Monthly Notices of the Royal Astronomical Society , vol. 409 , pp. 2-11 . https://doi.org/10.1111/j.1365-2966.2010.17041.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 516990
dc.identifier.otherPURE UUID: dcd46993-f871-4888-a779-49b8fdbe7342
dc.identifier.otherBibtex: urn:3169a1370942f3ecb7fd0be10cf809ea
dc.identifier.otherScopus: 78149366397
dc.identifier.otherORCID: /0000-0002-4010-8310/work/62747624
dc.identifier.urihttp://hdl.handle.net/2299/7648
dc.descriptionnot available in arXiv
dc.description.abstractWe present spectral energy distributions (SEDs) for 68 Herschel sources detected at 5σ at 250, 350 and 500 μm in the HerMES SWIRE-Lockman field. We explore whether existing models for starbursts, quiescent star-forming galaxies and active galactic nucleus dust tori are able to model the full range of SEDs measured with Herschel. We find that while many galaxies (∼56 per cent) are well fitted with the templates used to fit IRAS, Infrared Space Observatory (ISO) and Spitzer sources, for about half the galaxies two new templates are required: quiescent (‘cirrus’) models with colder (10–20 K) dust and a young starburst model with higher optical depth than Arp 220. Predictions of submillimetre fluxes based on model fits to 4.5–24 μm data agree rather poorly with the observed fluxes, but the agreement is better for fits to 4.5–70 μm data. Herschel galaxies detected at 500 μm tend to be those with the highest dust masses.en
dc.format.extent10
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectgalaxies: evolution, galaxies: starburst, galaxies: star formation, cosmology: observations, infrared: galaxies
dc.titleCold dust and young starbursts : spectral energy distributions of Herschel SPIRE sources from the HerMES surveyen
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.school
dcterms.dateAccepted2010-11-01
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2010.17041.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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