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dc.contributor.authorRoseboom, I.G.
dc.contributor.authorIvison, Rob J.
dc.contributor.authorGreve, T.R.
dc.contributor.authorAmblard, A.
dc.contributor.authorArumugam, V.
dc.contributor.authorAuld, R.
dc.contributor.authorAussel, H.
dc.contributor.authorBethermin, M.
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-Rodríguez, N.
dc.contributor.authorCava, A.
dc.contributor.authorChanial, P.
dc.contributor.authorChapin, E.
dc.contributor.authorChapman, S.
dc.contributor.authorClements, D. L.
dc.contributor.authorConley, A.
dc.contributor.authorConversi, L.
dc.contributor.authorCooray, A.
dc.contributor.authorDowell, C.D.
dc.contributor.authorDunlop, James S.
dc.contributor.authorDwek, E.
dc.contributor.authorEales, S.
dc.contributor.authorElbaz, D.
dc.contributor.authorFarrah, D.
dc.contributor.authorFranceschini, A.
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.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.authorMorrison, G.
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.authorPearson, C.P.
dc.contributor.authorPérez-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.authorRodighiero, G.
dc.contributor.authorRowan-Robinson, M.
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.authorVaccari, M.
dc.contributor.authorValtchanov, I.
dc.contributor.authorVieira, J. D.
dc.contributor.authorViero, M.P.
dc.contributor.authorVigroux, L.
dc.contributor.authorWardlow, J.
dc.contributor.authorWang, L.
dc.contributor.authorWright, G.
dc.contributor.authorXu, C.K.
dc.contributor.authorZemcov, M.
dc.date.accessioned2012-01-17T10:01:13Z
dc.date.available2012-01-17T10:01:13Z
dc.date.issued2012-02-01
dc.identifier.citationRoseboom , I G , Ivison , R J , Greve , T R , Amblard , A , Arumugam , V , Auld , R , Aussel , H , Bethermin , M , Blain , A , Bock , J , Boselli , A , Brisbin , D , Buat , V , Burgarella , D , Castro-Rodríguez , N , Cava , A , Chanial , P , Chapin , E , Chapman , S , Clements , D L , Conley , A , Conversi , L , Cooray , A , Dowell , C D , Dunlop , J S , Dwek , E , Eales , S , Elbaz , D , Farrah , D , Franceschini , A , Glenn , J , Griffin , M , Halpern , M , Hatziminaoglou , E , Ibar , E , Isaak , K , Lagache , G , Levenson , L , Lu , N , Madden , S , Maffei , B , Mainetti , G , Marchetti , L , Marsden , G , Morrison , G , Mortier , A M J , Nguyen , H T , O'Halloran , B , Oliver , S J , Omont , A , Page , M J , Panuzzo , P , Papageorgiou , A , Pearson , C P , Pérez-Fournon , I , Pohlen , M , Rawlings , J I , Raymond , G , Rigopoulou , D , Rizzo , D , Rodighiero , G , Rowan-Robinson , M , Schulz , B , Scott , D , Seymour , N , Shupe , D L , Smith , A J , Stevens , J , Symeonidis , M , Trichas , M , Tugwell , K E , Vaccari , M , Valtchanov , I , Vieira , J D , Viero , M P , Vigroux , L , Wardlow , J , Wang , L , Wright , G , Xu , C K & Zemcov , M 2012 , ' The Herschel Multi-tiered Extragalactic Survey : SPIRE-mm photometric redshifts ' , Monthly Notices of the Royal Astronomical Society , vol. 419 , no. 4 , pp. 2758-2773 . https://doi.org/10.1111/j.1365-2966.2011.19827.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 525367
dc.identifier.otherPURE UUID: b513e620-cc7d-49ee-af57-98a814f81a6f
dc.identifier.otherBibtex: urn:a6091674a56e70468ae5816f84612277
dc.identifier.otherScopus: 84855593284
dc.identifier.otherORCID: /0000-0002-4010-8310/work/62747599
dc.identifier.urihttp://hdl.handle.net/2299/7666
dc.description.abstractWe investigate the potential of submm–mm and submm–mm–radio photometric redshifts using a sample of mm-selected sources as seen at 250, 350 and 500μm by the SPIRE instrument on Herschel. From a sample of 63 previously identified mm sources with reliable radio identifications in the Great Observatories Origins Deep Survey North and Lockman Hole North fields, 46 (73 per cent) are found to have detections in at least one SPIRE band. We explore the observed submm/mm colour evolution with redshift, finding that the colours of mm sources are adequately described by a modified blackbody with constant optical depth τ= (ν/nu0)β, where β=+1.8 and ν0=c/100 μm. We find a tight correlation between dust temperature and IR luminosity. Using a single model of the dust temperature and IR luminosity relation, we derive photometric redshift estimates for the 46 SPIRE-detected mm sources. Testing against the 22 sources with known spectroscopic or good quality optical/near-IR photometric redshifts, we find submm/mm photometric redshifts offer a redshift accuracy of |Δz|/(1 +z) = 0.16 (〈|Δz|〉= 0.51). Including constraints from the radio–far-IR correlation, the accuracy is improved to |Δz|/(1 +z) = 0.15 (〈|Δz|〉= 0.45). We estimate the redshift distribution of mm-selected sources finding a significant excess at z > 3 when compared to ∼ 850 μm selected samples.en
dc.format.extent16
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.rightsEmbargoed
dc.subjectgalaxies: high-redshift - galaxies: statistics - submillimetre: galaxies
dc.titleThe Herschel Multi-tiered Extragalactic Survey : SPIRE-mm photometric redshiftsen
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.date.embargoedUntil2012-08-01
dc.description.versiontypeFinal Accepted Version
dcterms.dateAccepted2012-02-01
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2011.19827.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeEmbargoed


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