Using MgII to investigate quasars and their black-hole masses
| dc.creator | Jarvis, Matt J. | |
| dc.creator | McLure, Ross J. | |
| dc.date | 2003-10-30 | |
| dc.date.accessioned | 2026-07-07T02:10:57Z | |
| dc.date.available | 2026-07-07T02:10:57Z | |
| dc.description | We highlight the importance of the MgII 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. | |
| dc.description | 4 pages, 4 figures. To appear in "AGN Physics with the Sloan Digital Sky Survey, ed. G. T. Richards and P. B. Hall (San Francisco: ASP)" | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0310880 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0310880 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6914 | |
| dc.subject | Astrophysics | |
| dc.title | Using MgII to investigate quasars and their black-hole masses | |
| dc.type | text |