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dc.contributor.authorKalfountzou, E.
dc.contributor.authorStevens, J. A.
dc.contributor.authorJarvis, M. J.
dc.contributor.authorHardcastle, M. J.
dc.contributor.authorWilner, D.
dc.contributor.authorElvis, M.
dc.contributor.authorPage, M. J.
dc.contributor.authorTrichas, M.
dc.contributor.authorSmith, D. J. B.
dc.date.accessioned2017-10-16T14:32:54Z
dc.date.available2017-10-16T14:32:54Z
dc.date.issued2017-10-11
dc.identifier.citationKalfountzou , E , Stevens , J A , Jarvis , M J , Hardcastle , M J , Wilner , D , Elvis , M , Page , M J , Trichas , M & Smith , D J B 2017 , ' Observational evidence that positive and negative AGN feedback depends on galaxy mass and jet power ' , Monthly Notices of the Royal Astronomical Society , vol. 471 , no. 1 . https://doi.org/10.1093/mnras/stx1333
dc.identifier.issn0035-8711
dc.identifier.otherArXiv: http://arxiv.org/abs/1706.02334v1
dc.identifier.otherORCID: /0000-0002-4010-8310/work/62747554
dc.identifier.otherORCID: /0000-0001-9708-253X/work/69424294
dc.identifier.urihttp://hdl.handle.net/2299/19463
dc.descriptionThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. ©: 2017 The Author (s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
dc.description.abstractSeveral studies support the existence of a link between the AGN and star formation activity. Radio jets have been argued to be an ideal mechanism for direct interaction between the AGN and the host galaxy. A drawback of previous surveys of AGN is that they are fundamentally limited by the degeneracy between redshift and luminosity in flux-density limited samples. To overcome this limitation, we present far-infrared Herschel observations of 74 radio-loud quasars (RLQs), 72 radio-quiet quasars (RQQs) and 27 radio galaxies (RGs), selected at 0.9zen
dc.format.extent5889327
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectastro-ph.GA
dc.titleObservational evidence that positive and negative AGN feedback depends on galaxy mass and jet poweren
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.versionofrecord10.1093/mnras/stx1333
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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