Using MgII to investigate quasars and their black-hole masses

dc.contributor.author	Jarvis, M.J.
dc.contributor.author	McLure, R.J.
dc.contributor.editor	Richards, G. T.
dc.contributor.editor	Hall, P. B.
dc.date.accessioned	2011-10-20T11:01:16Z
dc.date.available	2011-10-20T11:01:16Z
dc.date.issued	2004
dc.identifier.citation	Jarvis , 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.other	dspace: 2299/1516
dc.identifier.uri	http://hdl.handle.net/2299/6737
dc.description.abstract	We 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.format.extent	195490
dc.language.iso	eng
dc.publisher	Astronomical Society of the Pacific
dc.relation.ispartof	AGN Physics with the Sloan Digital Sky Survey
dc.relation.ispartofseries	ASP Conference Series
dc.title	Using MgII to investigate quasars and their black-hole masses	en
dc.contributor.institution	School of Physics, Astronomy and Mathematics
rioxxterms.type	Other
herts.preservation.rarelyaccessed	true