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dc.contributor.authorVillforth, C.
dc.contributor.authorHamann, F.
dc.contributor.authorRosario, D.~J.
dc.contributor.authorSantini, P.
dc.contributor.authorMcGrath, E.~J.
dc.contributor.authorvan der Wel, A.
dc.contributor.authorChang, Y.-Y.
dc.contributor.authorGuo, Y.
dc.contributor.authorDahlen, T.
dc.contributor.authorBell, E.~F.
dc.contributor.authorConselice, C.~J.
dc.contributor.authorCroton, D.
dc.contributor.authorDekel, A.
dc.contributor.authorFaber, S.~M.
dc.contributor.authorGrogin, N.
dc.contributor.authorHamilton, T.
dc.contributor.authorHopkins, P.~F.
dc.contributor.authorJuneau, S.
dc.contributor.authorKartaltepe, J.
dc.contributor.authorKocevski, D.
dc.contributor.authorKoekemoer, A.
dc.contributor.authorKoo, D.~C.
dc.contributor.authorLotz, J.
dc.contributor.authorMcIntosh, D.
dc.contributor.authorMozena, M.
dc.contributor.authorSomerville, R.
dc.contributor.authorWild, V.
dc.identifier.citationVillforth , C , Hamann , F , Rosario , D J , Santini , P , McGrath , E J , van der Wel , A , Chang , Y-Y , Guo , Y , Dahlen , T , Bell , E F , Conselice , C J , Croton , D , Dekel , A , Faber , S M , Grogin , N , Hamilton , T , Hopkins , P F , Juneau , S , Kartaltepe , J , Kocevski , D , Koekemoer , A , Koo , D C , Lotz , J , McIntosh , D , Mozena , M , Somerville , R & Wild , V 2014 , ' Morphologies of z~0.7 AGN host galaxies in CANDELS : no trend of merger incidence with AGN luminosity ' , Monthly Notices of the Royal Astronomical Society , vol. 439 , no. 4 , pp. 3342-3356 .
dc.identifier.otherPURE: 95242588
dc.identifier.otherPURE UUID: ffa83b5a-01a1-4e56-aba9-34f8ec2356b6
dc.identifier.otherBibtex: urn:f3f6c117d2587dea96d806b54fc0041d
dc.identifier.otherScopus: 84897065707
dc.identifier.otherWOS: 000334115400012
dc.descriptionPS would like to acknowledge funding through grant ASI I/005/11/0. DKoo would like to acknowledge funding through grant NSF AST-0808133. SJ acknowledges financial support from the EC through an ERC grant StG-257720.en
dc.description.abstractThe processes that trigger active galactic nuclei (AGN) remain poorly understood. While lower luminosity AGN may be triggered by minor disturbances to the host galaxy, stronger disturbances are likely required to trigger luminous AGN. Major wet mergers of galaxies are ideal environments for AGN triggering since they provide large gas supplies and galaxy scale torques. There is however little observational evidence for a strong connection between AGN and major mergers. We analyse the morphological properties of AGN host galaxies as a function of AGN and host galaxy luminosity and compare them to a carefully matched sample of control galaxies. AGN are X-ray selected in the redshift range 0.5 < z < 0.8 and have luminosities 41 ≲ log (LX [erg s−1]) ≲ 44.5. ‘Fake AGN’ are simulated in the control galaxies by adding point sources with the magnitude of the matched AGN. We find that AGN host and control galaxies have comparable asymmetries, Sérsic indices and ellipticities at rest frame ∼950 nm. AGN host galaxies show neither higher average asymmetries nor higher fractions of very disturbed objects. There is no increase in the prevalence of merger signatures with AGN luminosity. At 95 per cent confidence we find that major mergers are responsible for <6 per cent of all AGN in our sample as well as <40 per cent of the highest luminosity AGN (log  (LX [erg s−1]) ∼ 43.5). Major mergers therefore either play only a very minor role in the triggering of AGN in the luminosity range studied or time delays are too long for merger features to remain visible.
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rightsThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. © 2014 The Authors, Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.en
dc.subjectGalaxies: activeen
dc.subjectGalaxies: evolutionen
dc.subjectGalaxies: interactionsen
dc.subjectGalaxies: irregularen
dc.subjectQuasars: generalen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.titleMorphologies of z~0.7 AGN host galaxies in CANDELS : no trend of merger incidence with AGN luminosityen
dc.typeJournal articleen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.description.statusPeer revieweden

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