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Rapid Coeval Black Hole and Host Galaxy Growth in MRCnbsp1138-262 : The Hungry Spider

dc.contributor.authorSeymour, N.
dc.contributor.authorAltieri, B.
dc.contributor.authorDe Breuck, C.
dc.contributor.authorBarthel, P.
dc.contributor.authorCoia, D.
dc.contributor.authorConversi, L.
dc.contributor.authorDannerbauer, H.
dc.contributor.authorDey, A.
dc.contributor.authorDickinson, M.
dc.contributor.authorDrouart, G.
dc.contributor.authorGalametz, A.
dc.contributor.authorGreve, T.R.
dc.contributor.authorHaas, M.
dc.contributor.authorHatch, N.
dc.contributor.authorIbar, E.
dc.contributor.authorIvison, R.
dc.contributor.authorJarvis, M.J.
dc.contributor.authorKovács, A.
dc.contributor.authorKurk, J.
dc.contributor.authorLehnert, M.
dc.contributor.authorMiley, G.
dc.contributor.authorNesvadba, N.
dc.contributor.authorRawlings, J.I.
dc.contributor.authorRettura, A.
dc.contributor.authorRöttgering, H.
dc.contributor.authorRocca-Volmerange, B.
dc.contributor.authorSánchez-Portal, M.
dc.contributor.authorSantos, J. S.
dc.contributor.authorStern, D.
dc.contributor.authorStevens, J.
dc.contributor.authorValtchanov, I.
dc.contributor.authorVernet, J.
dc.contributor.authorWylezalek, D.
dc.date.accessioned2013-02-13T17:00:01Z
dc.date.available2013-02-13T17:00:01Z
dc.date.issued2012-08-01
dc.identifier.citationSeymour , N , Altieri , B , De Breuck , C , Barthel , P , Coia , D , Conversi , L , Dannerbauer , H , Dey , A , Dickinson , M , Drouart , G , Galametz , A , Greve , T R , Haas , M , Hatch , N , Ibar , E , Ivison , R , Jarvis , M J , Kovács , A , Kurk , J , Lehnert , M , Miley , G , Nesvadba , N , Rawlings , J I , Rettura , A , Röttgering , H , Rocca-Volmerange , B , Sánchez-Portal , M , Santos , J S , Stern , D , Stevens , J , Valtchanov , I , Vernet , J & Wylezalek , D 2012 , ' Rapid Coeval Black Hole and Host Galaxy Growth in MRCnbsp1138-262 : The Hungry Spider ' , The Astrophysical Journal , vol. 755 , no. 2 , 146 . https://doi.org/10.1088/0004-637X/755/2/146
dc.identifier.issn0004-637X
dc.identifier.otherBibtex: urn:4e62d3db8d3c3b9507f728a7a0b0b893
dc.identifier.otherORCID: /0000-0002-4010-8310/work/62747575
dc.identifier.urihttp://hdl.handle.net/2299/9998
dc.descriptionCopyright American Astronomical Society
dc.description.abstractWe present a detailed study of the infrared spectral energy distribution of the high-redshift radio galaxy MRC1138-26 at z = 2.156, also known as the Spiderweb Galaxy. By combining photometry from Spitzer, Herschel and LABOCA we fit the rest-frame 5−300 μm emission using a two component, starburst and active galactic nucleus (AGN), model.en
dc.format.extent8
dc.format.extent328832
dc.language.isoeng
dc.relation.ispartofThe Astrophysical Journal
dc.titleRapid Coeval Black Hole and Host Galaxy Growth in MRCnbsp1138-262 : The Hungry Spideren
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1088/0004-637X/755/2/146
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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