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dc.contributor.authorHardcastle, M.J.
dc.contributor.authorVirdee, J.S.
dc.contributor.authorJarvis, M.J.
dc.contributor.authorBonfield, D.
dc.contributor.authorDunne, L.
dc.contributor.authorRawlings, S.
dc.contributor.authorStevens, J. A.
dc.contributor.authorChristopher, N. M.
dc.contributor.authorHeywood, I.
dc.contributor.authorMauch, Tom
dc.contributor.authorRigopoulou, D.
dc.contributor.authorVerma, A.
dc.contributor.authorBaldry, Ivan K.
dc.contributor.authorBamford, S. P.
dc.contributor.authorButtiglione, S.
dc.contributor.authorCava, A.
dc.contributor.authorClements, D. L.
dc.contributor.authorCooray, A.
dc.contributor.authorCroom, S. M.
dc.contributor.authorDariush, A.
dc.contributor.authorde Zotti, G.
dc.contributor.authorEales, S.
dc.contributor.authorFritz, J.
dc.contributor.authorHill, D. T.
dc.contributor.authorHughes, D.
dc.contributor.authorHopwood, R.
dc.contributor.authorIbar, E.
dc.contributor.authorIvison, Rob J.
dc.contributor.authorJones, D.H.
dc.contributor.authorLoveday, J.
dc.contributor.authorMaddox, S. J.
dc.contributor.authorMichalowski, M. J.
dc.contributor.authorNegrello, M.
dc.contributor.authorNorberg, P.
dc.contributor.authorPohlen, M.
dc.contributor.authorPrescott, M.
dc.contributor.authorRigby, E. E.
dc.contributor.authorRobotham, A. S. G.
dc.contributor.authorRodighiero, G.
dc.contributor.authorScott, D.
dc.contributor.authorSharp, R.
dc.contributor.authorSmith, Daniel
dc.contributor.authorTemi, P.
dc.contributor.authorvan Kampen, E.
dc.date.accessioned2011-05-09T08:53:10Z
dc.date.available2011-05-09T08:53:10Z
dc.date.issued2010
dc.identifier.citationHardcastle , M J , Virdee , J S , Jarvis , M J , Bonfield , D , Dunne , L , Rawlings , S , Stevens , J A , Christopher , N M , Heywood , I , Mauch , T , Rigopoulou , D , Verma , A , Baldry , I K , Bamford , S P , Buttiglione , S , Cava , A , Clements , D L , Cooray , A , Croom , S M , Dariush , A , de Zotti , G , Eales , S , Fritz , J , Hill , D T , Hughes , D , Hopwood , R , Ibar , E , Ivison , R J , Jones , D H , Loveday , J , Maddox , S J , Michalowski , M J , Negrello , M , Norberg , P , Pohlen , M , Prescott , M , Rigby , E E , Robotham , A S G , Rodighiero , G , Scott , D , Sharp , R , Smith , D , Temi , P & van Kampen , E 2010 , ' Herschel-ATLAS: far-infrared properties of radio-selected galaxies ' , Monthly Notices of the Royal Astronomical Society , vol. 409 , no. 1 , pp. 122-131 . https://doi.org/10.1111/j.1365-2966.2010.17791.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 161720
dc.identifier.otherPURE UUID: 0d43c65f-894b-40a2-8f33-68fa6e907d7d
dc.identifier.otherdspace: 2299/5754
dc.identifier.otherScopus: 78149372887
dc.identifier.otherORCID: /0000-0002-4010-8310/work/62747572
dc.identifier.urihttp://hdl.handle.net/2299/5754
dc.description.abstractWe use the Herschel-Astrophysical Terahertz Large Area Survey (ATLAS) science demonstration data to investigate the star formation properties of radio-selected galaxies in the GAMA-9h field as a function of radio luminosity and redshift. Radio selection at the lowest radio luminosities, as expected, selects mostly starburst galaxies. At higher radio luminosities, where the population is dominated by active galactic nuclei (AGN), we find that some individual objects are associated with high far-infrared luminosities. However, the far-infrared properties of the radio-loud population are statistically indistinguishable from those of a comparison population of radio-quiet galaxies matched in redshift and K-band absolute magnitude. There is thus no evidence that the host galaxies of these largely low-luminosity (Fanaroff–Riley class I), and presumably low-excitation, AGN, as a population, have particularly unusual star formation histories. Models in which the AGN activity in higher luminosity, high-excitation radio galaxies is triggered by major mergers would predict a luminosity-dependent effect that is not seen in our data (which only span a limited range in radio luminosity) but which may well be detectable with the full Herschel-ATLAS data set.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectgalaxies : active
dc.subjectradio continuum : galaxies
dc.subjectinfrared : galaxies
dc.titleHerschel-ATLAS: far-infrared properties of radio-selected galaxiesen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2010.17791.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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