An objective classification scheme for QSO spectra
| dc.contributor.author | Francis, Paul | |
| dc.contributor.author | Hewett, Paul C. | |
| dc.contributor.author | Foltz, Craig B. | |
| dc.contributor.author | Chaffee, Frederic H. | |
| dc.date.accessioned | 2018-09-11T04:01:09Z | |
| dc.date.available | 2018-09-11T04:01:09Z | |
| dc.date.issued | 1992 | |
| dc.description.abstract | The 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.mimetype | application/pdf | en_AU |
| dc.identifier.issn | 0004-637X | en_AU |
| dc.identifier.uri | http://hdl.handle.net/1885/147320 | |
| dc.publisher | American Astronomical Society | en_AU |
| dc.rights | http://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.source | The Astrophysical Journal | en_AU |
| dc.title | An objective classification scheme for QSO spectra | en_AU |
| dc.type | Journal article | en_AU |
| dcterms.accessRights | Open Access | en_AU |
| local.bibliographicCitation.issue | 2 | en_AU |
| local.bibliographicCitation.lastpage | 490 | en_AU |
| local.bibliographicCitation.startpage | 476 | en_AU |
| local.contributor.affiliation | Francis, P., Mount Stromlo Observatory, Research School of Astronomy and Astrophysics, The Australian National University | en_AU |
| local.contributor.authoruid | u9710753 | en_AU |
| local.description.notes | The author was affiliated with University of Institute of Astronomy, Cambridge, England when the paper was published. | en_AU |
| local.identifier.citationvolume | 398 | en_AU |
| local.identifier.doi | 10.1086/171870 | en_AU |
| local.publisher.url | https://aas.org/ | en_AU |
| local.type.status | Published Version | en_AU |