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 | |