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dc.contributor.authorSmith, Daniel
dc.contributor.authorJarvis, M.J.
dc.contributor.authorSimpson, C.
dc.contributor.authorMartinez-Sansigre, A.
dc.date.accessioned2009-06-30T07:15:57Z
dc.date.available2009-06-30T07:15:57Z
dc.date.issued2009
dc.identifier.citationSmith , D , Jarvis , M J , Simpson , C & Martinez-Sansigre , A 2009 , ' An 80-kpc Ly alpha halo around a high-redshift type-2 quasi-stellar object ' , Monthly Notices of the Royal Astronomical Society , vol. 393 , no. 1 , pp. 309-316 . https://doi.org/10.1111/j.1365-2966.2008.14232.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 172345
dc.identifier.otherPURE UUID: bf93e25f-6af7-4673-bb17-46c6756782fc
dc.identifier.otherdspace: 2299/3630
dc.identifier.otherWOS: 000262782500039
dc.identifier.otherScopus: 58749086719
dc.identifier.otherORCID: /0000-0001-9708-253X/work/69424343
dc.identifier.urihttp://hdl.handle.net/2299/3630
dc.description‘The definitive version is available at: www3.interscience.wiley.com '. Copyright Blackwell Publishing / Royal Astronomical Society. DOI: 10.1111/j.1365-2966.2008.14232.x
dc.description.abstractWe announce the discovery of an extended emission line region associated with a high redshift type-2 QSO. The halo, which was discovered in our new wide-field narrow-band survey, resides at z = 2.85 in the Spitzer First Look Survey region and is extended over 80 kpc. Deep VLBI observations imply that approximately 50 per cent of the radio emission is extended on scales > 200pc. The inferred AGN luminosity is sufficient to ionize the extended halo, and the optical emission is consistent with being triggered coevally with the radio source. The Lyman- α halo is as luminous as those found around high redshift radio galaxies, however the active nucleus is several orders of magnitude less luminous at radio wavelengths than those FRIIs more commonly associated with extended emission line regions. AMS05 appears to be a highredshift analogue to the radio-quiet quasar E1821+643which is core dominated but which also exhibits extended FRI-like structure and contains an optically powerfulAGN.en
dc.format.extent8
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectgalaxies: haloes
dc.subjectgalaxies: high-redshift
dc.subjectgalaxies: jets
dc.subjectaccretion
dc.subjectquasars: emission lines
dc.subjectSPITZER-SPACE-TELESCOPE
dc.subjectACTIVE GALACTIC NUCLEI
dc.subjectSPECTRUM RADIO-SOURCES
dc.subjectCOMPACT STEEP-SPECTRUM
dc.subjectEXTRAGALACTIC 1ST
dc.subjectUNIFIED SCHEMES
dc.subject1ST-LOOK SURVEY
dc.subjectCOLLAPSING PROTOGALAXIES
dc.subjectENERGY-DISTRIBUTIONS
dc.subjectLUMINOSITY FUNCTION
dc.titleAn 80-kpc Ly alpha halo around a high-redshift type-2 quasi-stellar objecten
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=58749086719&partnerID=8YFLogxK
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2008.14232.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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