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dc.contributor.authorSeymour, N.
dc.contributor.authorSymeonidis, M.
dc.contributor.authorPage, M. J.
dc.contributor.authorAmblard, A.
dc.contributor.authorArumugam, V.
dc.contributor.authorAussel, H.
dc.contributor.authorBlain, A.
dc.contributor.authorBock, J.
dc.contributor.authorBoselli, A.
dc.contributor.authorBuat, V.
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.authorEales, S.
dc.contributor.authorElbaz, D.
dc.contributor.authorFranceschini, A.
dc.contributor.authorGlenn, J.
dc.contributor.authorSolares, E. A. Gonzalez
dc.contributor.authorGriffin, 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.authorNguyen, H. T.
dc.contributor.authorO'Halloran, B.
dc.contributor.authorOliver, S. J.
dc.contributor.authorOmont, A.
dc.contributor.authorPanuzzo, P.
dc.contributor.authorPapageorgiou, A.
dc.contributor.authorPearson, C. P.
dc.contributor.authorPerez-Fournon, I.
dc.contributor.authorPohlen, M.
dc.contributor.authorRawlings, J. I.
dc.contributor.authorRizzo, D.
dc.contributor.authorRoseboom, I. G.
dc.contributor.authorRowan-Robinson, M.
dc.contributor.authorSchulz, B.
dc.contributor.authorScott, Douglas
dc.contributor.authorShupe, D. L.
dc.contributor.authorSmith, A. J.
dc.contributor.authorStevens, J. A.
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.authorWright, G.
dc.contributor.authorXu, C. K.
dc.contributor.authorZemcov, M.
dc.date.accessioned2011-09-15T11:01:12Z
dc.date.available2011-09-15T11:01:12Z
dc.date.issued2011-05
dc.identifier.citationSeymour , N , Symeonidis , M , Page , M J , Amblard , A , Arumugam , V , Aussel , H , Blain , A , Bock , J , Boselli , A , Buat , V , Castro-Rodriguez , N , Cava , A , Chanial , P , Clements , D L , Conley , A , Conversi , L , Cooray , A , Dowell , C D , Dwek , E , Eales , S , Elbaz , D , Franceschini , A , Glenn , J , Solares , E A G , Griffin , M , Hatziminaoglou , E , Ibar , E , Isaak , K , Ivison , R J , Lagache , G , Levenson , L , Lu , N , Madden , S , Maffei , B , Mainetti , G , Marchetti , L , Nguyen , H T , O'Halloran , B , Oliver , S J , Omont , A , Panuzzo , P , Papageorgiou , A , Pearson , C P , Perez-Fournon , I , Pohlen , M , Rawlings , J I , Rizzo , D , Roseboom , I G , Rowan-Robinson , M , Schulz , B , Scott , D , Shupe , D L , Smith , A J , Stevens , J A , Trichas , M , Tugwell , K E , Vaccari , M , Valtchanov , I , Vigroux , L , Wang , L , Wright , G , Xu , C K & Zemcov , M 2011 , ' HerMES: SPIRE emission from radio-selected active galactic nuclei ' , Monthly Notices of the Royal Astronomical Society , vol. 413 , no. 3 , pp. 1777-1786 . https://doi.org/10.1111/j.1365-2966.2011.18253.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 357980
dc.identifier.otherPURE UUID: 12613da9-6ca6-4142-be30-49402be8fc66
dc.identifier.otherWOS: 000290487700024
dc.identifier.otherScopus: 79955750899
dc.identifier.otherORCID: /0000-0002-4010-8310/work/62747604
dc.identifier.urihttp://hdl.handle.net/2299/6442
dc.descriptionThe definitive version can be found at: http://onlinelibrary.wiley.com/ Copyright Royal Astronomical Society
dc.description.abstractWe examine the rest-frame far-infrared emission from powerful radio sources with 1.4-GHz luminosity densities of 25 < log(L-1.4/W Hz-1) < 26.5 in the extragalactic Spitzer First Look Survey field. We combine Herschel/SPIRE flux densities with Spitzer/Infrared Array Camera and Multiband Imaging Photometer for Spitzer infrared data to obtain total (<file name="mnr_18253_mu1.gif" type="gif"/>m) infrared luminosities for these radio sources. We separate our sources into a moderate, 0.4 < z < 0.9, and a high, 1.2 < z < 3.0, redshift sub-sample and we use Spitzer observations of a z < 0.1 3CRR sample as a local comparison. By comparison to numbers from the Square Kilometre Array (SKA) Simulated Skies, we find that our moderate-redshift sample is complete and our high-redshift sample is 14 per cent complete. We constrain the ranges of mean star formation rates (SFRs) to be 3.4-4.2, 18-41 and 80-581 M-circle dot yr-1 for the local, moderate- and high-redshift samples, respectively. Hence, we observe an increase in the mean SFR with increasing redshift which we can parametrize as similar to(1 + z)Q, where Q = 4.2 +/- 0.8. However, we observe no trends of mean SFR with radio luminosity within the moderate- or high-redshift bins. We estimate that radio-loud active galactic nuclei (AGN) in the high-redshift sample contribute 0.1-0.5 per cent to the total SFR density at that epoch. Hence, if all luminous starbursts host radio-loud AGN we infer a radio-loud phase duty cycle of 0.001-0.005.en
dc.format.extent10
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectgalaxies: active
dc.subjectinfrared: galaxies
dc.subjectradio continuum: galaxies
dc.titleHerMES: SPIRE emission from radio-selected active galactic nucleien
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.embargoedUntil2011-11-01
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2011.18253.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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