2dF QSO Redshift Survey
| dc.creator | Shanks, T. | |
| dc.creator | Boyle, B. J. | |
| dc.creator | Croom, S. M. | |
| dc.creator | Loaring, N. | |
| dc.creator | Miller, L. | |
| dc.creator | Smith, R. J. | |
| dc.date | 2000-03-14 | |
| dc.date.accessioned | 2026-07-07T01:52:44Z | |
| dc.date.available | 2026-07-07T01:52:44Z | |
| dc.description | With approximately 6000 QSO redshifts,the 2dF QSO redshift survey is already the biggest complete QSO survey. The aim for the survey is to have 25000 QSO redshifts, providing an order of magnitude increase in QSO clustering statistics. We first describe the observational parameters of the 2dF QSO survey. We then describe several highlights of the survey so far, including new estimates of the QSO luminosity function and its evolution. We also review the current status of QSO clustering analyses from the 2dF data. Finally, we discuss how the complete QSO survey will be able to constrain the value of Omega_o by measuring the evolution of QSO clustering, place limits on the cosmological constant via a direct geometrical test and determine the form of the fluctuation power-spectrum out to the approximately 1000 Mpc scales only previously probed by COBE. | |
| dc.description | 6 pages; to be published in Clustering at High Redshift, Marseille, June 1999, eds. A. Mazure, O. LeFevre, V. Lebrun | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0003206 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0003206 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/722 | |
| dc.subject | Astrophysics | |
| dc.title | 2dF QSO Redshift Survey | |
| dc.type | text |