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dc.contributor.authorJarvis, M.J.
dc.contributor.authorMcLure, R.J.
dc.contributor.editorRichards, G. T.
dc.contributor.editorHall, P. B.
dc.date.accessioned2011-10-20T11:01:16Z
dc.date.available2011-10-20T11:01:16Z
dc.date.issued2004
dc.identifier.citationJarvis , M J & McLure , R J 2004 , Using MgII to investigate quasars and their black-hole masses . in G T Richards & P B Hall (eds) , AGN Physics with the Sloan Digital Sky Survey . ASP Conference Series , vol. 311 , Astronomical Society of the Pacific , pp. 79-82 .
dc.identifier.otherPURE: 425418
dc.identifier.otherPURE UUID: b109cdfe-a039-4a29-871f-5a37920dbf03
dc.identifier.otherdspace: 2299/1516
dc.identifier.urihttp://hdl.handle.net/2299/6737
dc.description.abstractWe highlight the importance of the Mg II λ2800 emission-line doublet in probing high-redshift quasars and their supermassive black holes. In the SDSS era, where large scale investigations of quasars across the age of the Universe are possible, this emission-line has the ability to provide accurate systemic redshifts which are important for a variety of follow-up studies, as well as probe the masses of the supermassive black holes that power these phenomena.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofAGN Physics with the Sloan Digital Sky Survey
dc.relation.ispartofseriesASP Conference Series
dc.rights/dk/atira/pure/core/openaccesspermission/open
dc.titleUsing MgII to investigate quasars and their black-hole massesen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeFinal Published version
rioxxterms.versionVoR
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeopenAccess


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