The Large Adaptive Reflector concept
| dc.creator | Dougherty, S. M. | |
| dc.creator | Dewdney, P. E. | |
| dc.creator | Gray, A. | |
| dc.creator | Taylor, A. R. | |
| dc.date | 2005-10-18 | |
| dc.date.accessioned | 2026-07-07T06:43:57Z | |
| dc.date.available | 2026-07-07T06:43:57Z | |
| dc.description | Cost effective, new antenna technology is required to build the large collecting area being planned for the next generation of radio telescopes. The Large Adaptive Reflector (LAR) is a novel concept being developed in Canada to meet this challenge. A prototype with a 200-350m diameter reflector, operating up to 2 GHz with a bandwidth of 750 MHz is planned. With a collecting area up to ~10% of the planned SKA, and an array feed capable of imaging a 0.3 deg^2 field-of-view, the prototype would address a number of the most compelling questions in modern astrophysics. | |
| dc.description | 2 pages, 4 figures, to appear in Proceeding of the 9th Asian-Pacific Regional IAU Meeting, 2005 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0510541 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0510541 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/102611 | |
| dc.subject | Astrophysics | |
| dc.title | The Large Adaptive Reflector concept | |
| dc.type | text |