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HerMES: Far infrared properties of known AGN in the HerMES fields

dc.contributor.authorHatziminaoglou, E.
dc.contributor.authorOmont, A.
dc.contributor.authorStevens, Jason
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.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.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.authorMortier, A.M.J.
dc.contributor.authorNguyen, H.T.
dc.contributor.authorO'Halloran, B.
dc.contributor.authorOliver, S. J.
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.authorRigopoulou, D.
dc.contributor.authorRizzo, D.
dc.contributor.authorRoseboom, I.G.
dc.contributor.authorRowan-Robinson, M.
dc.contributor.authorSanchez Portal, M.
dc.contributor.authorSchulz, B.
dc.contributor.authorScott, D.
dc.contributor.authorSeymour, N.
dc.contributor.authorShupe, D. L.
dc.contributor.authorSymeonidis, M.
dc.contributor.authorTrichas, M.
dc.contributor.authorTugwell, K.E.
dc.contributor.authorVaccari, M.
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.accessioned2012-02-23T13:00:52Z
dc.date.available2012-02-23T13:00:52Z
dc.date.issued2010-07-01
dc.identifier.citationHatziminaoglou , E , Omont , A , Stevens , J , 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 , 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 , 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 , Page , M J , Panuzzo , P , Papageorgiou , A , Pearson , C P , Pérez-Fournon , I , Pohlen , M , Rawlings , J I , Rigopoulou , D , Rizzo , D , Roseboom , I G , Rowan-Robinson , M , Sanchez Portal , M , Schulz , B , Scott , D , Seymour , N , Shupe , D L , Symeonidis , M , Trichas , M , Tugwell , K E , Vaccari , M , Valtchanov , I , Vigroux , L , Wang , L , Ward , R , Wright , G , Xu , C K & Zemcov , M 2010 , ' HerMES: Far infrared properties of known AGN in the HerMES fields ' , Astronomy and Astrophysics , vol. 518 , L33 . https://doi.org/10.1051/0004-6361/201014679
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 518696
dc.identifier.otherPURE UUID: 18f1c114-0a31-443e-8d6a-c636e0aff76e
dc.identifier.otherBibtex: urn:9e443e4dcb91e9714806a7c9e8436955
dc.identifier.otherScopus: 77954785966
dc.identifier.otherORCID: /0000-0002-4010-8310/work/62747541
dc.identifier.urihttp://hdl.handle.net/2299/7894
dc.description.abstractNuclear and starburst activity are known to often occur concomitantly. Herschel-SPIRE provides sampling of the far-infrared (FIR) spectral energy distributions (SEDs) of type 1 and type 2 AGN, allowing for the separation between the hot dust (torus) and cold dust (starburst) emission. We study large samples of spectroscopically confirmed type 1 and type 2 AGN lying within the Herschel Multi-tiered Extragalactic Survey (HerMES) fields observed during the science demonstration phase, aiming to understand their FIR colour distributions and constrain their starburst contributions.en
dc.language.isoeng
dc.relation.ispartofAstronomy and Astrophysics
dc.subjectgalaxies: active, galaxies: Seyfert, galaxies: star formation, infrared: general, quasars: general
dc.titleHerMES: Far infrared properties of known AGN in the HerMES fieldsen
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.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1051/0004-6361/201014679
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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