The statistics of wide-separation lenses
| dc.creator | Mortlock, Daniel J. | |
| dc.date | 2000-11-08 | |
| dc.date.accessioned | 2026-07-07T01:56:28Z | |
| dc.date.available | 2026-07-07T01:56:28Z | |
| dc.description | The probability that high-redshift sources are gravitationally-lensed with large image separations (i.e., greater than can be produced by galactic deflectors) is determined by the cosmological population of group- and cluster-sized halos. Thus the observed frequency of wide-separation lensed quasars can be used to constrain not only the halo distribution, but also a number of cosmological parameters. A calculation of the optical depth due to collapsed, isothermal halos is a useful guide to the lens statistics, and illustrates that the number of wide-separation lenses is a sensitive probe of the mean density of the universe and the present day density variance whilst being nearly independent of the cosmological constant. | |
| dc.description | Cosmological Physics with Gravitational Lensing, J.-P. Kneib, Y. Mellier, M. Moniez & J. Tran Thanh Van, eds., in press; 4 pages; 7 figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0011174 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0011174 | |
| dc.identifier | 2001, in Cosmological Physics with Gravitational Lensing (Proceedings of the XXth Moriond Meeting), Tran Thanh Van, J., Mellier, Y. & Moniez, M., eds., EDP Sciences, Les Ulis, 283 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/2010 | |
| dc.subject | Astrophysics | |
| dc.title | The statistics of wide-separation lenses | |
| dc.type | text |