An objective classification scheme for QSO spectra

dc.contributor.authorFrancis, Paul
dc.contributor.authorHewett, Paul C.
dc.contributor.authorFoltz, Craig B.
dc.contributor.authorChaffee, Frederic H.
dc.date.accessioned2018-09-11T04:01:09Z
dc.date.available2018-09-11T04:01:09Z
dc.date.issued1992
dc.description.abstractThe classification of QSO rest-frame optical and UV spectra is undertaken by means of a statistical principal component analysis (PCA) emphasizing the relation between QSO properties. The PCA is applied directly to a sample of QSO UV spectra from the Large Bright QSO Survey, and relations are studied between continuum, emission-line, and broad-absorption-line properties. Quantitative classifications are derived based on a limited number of principal components, and three components account for approximately 75 percent of the sample and describe: emission-line core strength, continuum slope, and broad absorption features. Broad-absorption-line QSOs appear as a natural subclass of the population with characteristic excess emissions, and continuum hardness correlates with the equivalent widths of C IV and Lyman-alpha emission lines. Quantitative properties are derived from the study that serve to classify QSO emissions ranging from broad low-equivalent-width lines to narrow high-equivalent-width lines.en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0004-637Xen_AU
dc.identifier.urihttp://hdl.handle.net/1885/147320
dc.publisherAmerican Astronomical Societyen_AU
dc.rightshttp://www.sherpa.ac.uk/romeo/issn/0004-637X/..."Publisher's version/PDF may be used on any website or authors' institutional repository" from SHERPA/RoMEO site (as at 11/09/18).en_AU
dc.sourceThe Astrophysical Journalen_AU
dc.titleAn objective classification scheme for QSO spectraen_AU
dc.typeJournal articleen_AU
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue2en_AU
local.bibliographicCitation.lastpage490en_AU
local.bibliographicCitation.startpage476en_AU
local.contributor.affiliationFrancis, P., Mount Stromlo Observatory, Research School of Astronomy and Astrophysics, The Australian National Universityen_AU
local.contributor.authoruidu9710753en_AU
local.description.notesThe author was affiliated with University of Institute of Astronomy, Cambridge, England when the paper was published.en_AU
local.identifier.citationvolume398en_AU
local.identifier.doi10.1086/171870en_AU
local.publisher.urlhttps://aas.org/en_AU
local.type.statusPublished Versionen_AU

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