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HerMES: The submillimeter spectral energy distributions of Herschel/SPIRE-detected galaxies

dc.contributor.authorSchulz, B.
dc.contributor.authorPearson, C.P.
dc.contributor.authorClements, D. L.
dc.contributor.authorAltieri, B.
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.authorBuat, V.
dc.contributor.authorBurgarella, D.
dc.contributor.authorCastro-Rodríguez, N.
dc.contributor.authorCava, A.
dc.contributor.authorChanial, P.
dc.contributor.authorConley, A.
dc.contributor.authorConversi, L.
dc.contributor.authorCooray, A.
dc.contributor.authorDowell, C.D.
dc.contributor.authorDwek, E.
dc.contributor.authorEales, S.
dc.contributor.authorElbaz, D.
dc.contributor.authorFox, M.
dc.contributor.authorFranceschini, A.
dc.contributor.authorGear, W.
dc.contributor.authorGiovannoli, E.
dc.contributor.authorGlenn, J.
dc.contributor.authorGriffin, M.
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.authorLevenson, L.
dc.contributor.authorLu, N.
dc.contributor.authorMadden, S.
dc.contributor.authorMaffei, B.
dc.contributor.authorMainetti, G.
dc.contributor.authorMarchetti, L.
dc.contributor.authorMarsden, G.
dc.contributor.authorMortier, A.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.authorPérez-Fournon, I.
dc.contributor.authorPohlen, M.
dc.contributor.authorRangwala, N.
dc.contributor.authorRawlings, J.I.
dc.contributor.authorRaymond, G.
dc.contributor.authorRigopoulou, D.
dc.contributor.authorRizzo, D.
dc.contributor.authorRoseboom, I.G.
dc.contributor.authorRowan-Robinson, M.
dc.contributor.authorSánchez Portal, M.
dc.contributor.authorScott, D.
dc.contributor.authorSeymour, N.
dc.contributor.authorShupe, D. L.
dc.contributor.authorStevens, Jason
dc.contributor.authorSymeonidis, M.
dc.contributor.authorTrichas, M.
dc.contributor.authorTugwell, K.E.
dc.contributor.authorVaccari, M.
dc.contributor.authorValiante, 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.accessioned2012-02-23T13:00:55Z
dc.date.available2012-02-23T13:00:55Z
dc.date.issued2010-07-01
dc.identifier.citationSchulz , B , Pearson , C P , Clements , D L , Altieri , B , Amblard , A , Arumugam , V , Auld , R , Aussel , H , Babbedge , T , Blain , A , Bock , J , Boselli , A , Buat , V , Burgarella , D , Castro-Rodríguez , N , Cava , A , Chanial , P , Conley , A , Conversi , L , Cooray , A , Dowell , C D , Dwek , E , Eales , S , Elbaz , D , Fox , M , Franceschini , A , Gear , W , Giovannoli , E , Glenn , J , Griffin , M , Halpern , M , Hatziminaoglou , E , Ibar , E , Isaak , K , Ivison , R J , Lagache , G , Levenson , L , Lu , N , Madden , S , Maffei , B , Mainetti , G , Marchetti , L , Marsden , G , Mortier , A M J , Nguyen , H T , O'Halloran , B , Oliver , S J , Omont , A , Page , M J , Panuzzo , P , Papageorgiou , A , Pérez-Fournon , I , Pohlen , M , Rangwala , N , Rawlings , J I , Raymond , G , Rigopoulou , D , Rizzo , D , Roseboom , I G , Rowan-Robinson , M , Sánchez Portal , M , Scott , D , Seymour , N , Shupe , D L , Stevens , J , Symeonidis , M , Trichas , M , Tugwell , K E , Vaccari , M , Valiante , E , Valtchanov , I , Vigroux , L , Wang , L , Ward , R , Wright , G , Xu , C K & Zemcov , M 2010 , ' HerMES: The submillimeter spectral energy distributions of Herschel/SPIRE-detected galaxies ' , Astronomy and Astrophysics , vol. 518 , L32 . https://doi.org/10.1051/0004-6361/201014673
dc.identifier.issn0004-6361
dc.identifier.otherBibtex: urn:7b42ef2eb056be3fa4a782290442ae2a
dc.identifier.otherORCID: /0000-0002-4010-8310/work/62747595
dc.identifier.urihttp://hdl.handle.net/2299/7895
dc.description.abstractWe present colours of sources detected with the Herschel/SPIRE instrument in deep extragalactic surveys of the Lockman Hole, Spitzer-FLS, and GOODS-N fields in three photometric bands at 250, 350 and 500 μm. We compare these with expectations from the literature and discuss associated uncertainties and biases in the SPIRE data. We identify a 500 μm flux limited selection of sources from the HerMES point source catalogue that appears free from neighbouring/blended sources in all three SPIRE bands. We compare the colours with redshift tracks of various contemporary models. Based on these spectral templates we show that regions corresponding to specific population types and redshifts can be identified better in colour-flux space. The redshift tracks as well as the colour-flux plots imply a majority of detected objects with redshifts at 1 < z < 3.5, somewhat depending on the group of model SEDs used.en
dc.format.extent512172
dc.language.isoeng
dc.relation.ispartofAstronomy and Astrophysics
dc.subjectsubmillimeter: galaxies, galaxies: evolution, galaxies: high-redshift
dc.titleHerMES: The submillimeter spectral energy distributions of Herschel/SPIRE-detected 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
rioxxterms.versionofrecord10.1051/0004-6361/201014673
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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