Cluster Reconstruction from Combined Strong and Weak Lensing
| dc.creator | Saha, Prasenjit | |
| dc.creator | Williams, Liliya L. R. | |
| dc.creator | AbdelSalam, Hanadi | |
| dc.date | 1999-09-14 | |
| dc.date.accessioned | 2026-07-07T02:33:16Z | |
| dc.date.available | 2026-07-07T02:33:16Z | |
| dc.description | The lensing information provided by multiple images, arclets, and statistical distortions can all be formulated as linear constraints on the arrival-time surface, and hence on the mass distribution. This reduces cluster lens reconstruction from combined strong and weak lensing to a standard type of inversion problem. Moreover, the mass sheet degeneracy is broken if there are sources at different redshifts. | |
| dc.description | 8 pages incl 6 figures. Invited talk at "Gravitational Lensing: Recent Progress and Future Goals", Boston University, MA, July 1999, eds. T.G. Brainerd and C.S. Kochanek | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9909249 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9909249 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/14779 | |
| dc.subject | Astrophysics | |
| dc.title | Cluster Reconstruction from Combined Strong and Weak Lensing | |
| dc.type | text |