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dc.contributor.authorCroston, J. H.
dc.contributor.authorHardcastle, M. J.
dc.contributor.authorMingo, B.
dc.contributor.authorBest, P. N.
dc.contributor.authorSabater, J.
dc.contributor.authorShimwell, T. W.
dc.contributor.authorWilliams, W. L.
dc.contributor.authorDuncan, K. J.
dc.contributor.authorRöttgering, H. J. A.
dc.contributor.authorBrienza, M.
dc.contributor.authorGürkan, G.
dc.contributor.authorIneson, J.
dc.contributor.authorMorabito, L. M.
dc.contributor.authorMiley, G. K.
dc.contributor.authorO'Sullivan, S. P.
dc.contributor.authorPrandoni, I.
dc.date.accessioned2019-01-17T16:15:19Z
dc.date.available2019-01-17T16:15:19Z
dc.date.issued2018-10-10
dc.identifier.citationCroston , J H , Hardcastle , M J , Mingo , B , Best , P N , Sabater , J , Shimwell , T W , Williams , W L , Duncan , K J , Röttgering , H J A , Brienza , M , Gürkan , G , Ineson , J , Morabito , L M , Miley , G K , O'Sullivan , S P & Prandoni , I 2018 , ' The environments of radio-loud AGN from the LOFAR Two-Metre Sky Survey (LoTSS) ' , Astronomy & Astrophysics . https://doi.org/10.1051/0004-6361/201834019
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 15717771
dc.identifier.otherPURE UUID: bc095606-25d9-47eb-aad1-0b5deb4f5523
dc.identifier.otherArXiv: http://arxiv.org/abs/1811.07949v1
dc.identifier.otherScopus: 85062015616
dc.identifier.urihttp://hdl.handle.net/2299/20988
dc.description13 pages, 7 figures. This paper is part of the LOFAR surveys data release 1 and has been accepted for publication in a special edition of A&A that will appear in Feb 2019, volume 622. The catalogues and images from the data release will be publicly available on lofar-surveys.org upon publication of the journal. Reproduced with permission from Astronomy & Astrophysics. © 2018 ESO
dc.description.abstractAn understanding of the relationship between radio-loud active galaxies and their large-scale environments is essential for realistic modelling of radio-galaxy evolution and environmental impact, for understanding AGN triggering and life cycles, and for calibrating galaxy feedback in cosmological models. We use the LOFAR Two-Metre Sky Survey (LoTSS) Data Release 1 catalogues to investigate this relationship. We cross-matched 8,745 radio-loud AGN with 0.08en
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysics
dc.rightsOpen
dc.subjectastro-ph.GA
dc.titleThe environments of radio-loud AGN from the LOFAR Two-Metre Sky Survey (LoTSS)en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeFinal Accepted Version
dcterms.dateAccepted2018-10-10
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1051/0004-6361/201834019
rioxxterms.licenseref.uriOther
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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