High angular resolution coronography for adaptive optics
| dc.creator | Malbet, Fabien | |
| dc.date | 1995-09-14 | |
| dc.date.accessioned | 2026-07-07T02:20:11Z | |
| dc.date.available | 2026-07-07T02:20:11Z | |
| dc.description | Recent adaptive optics systems in astronomy achieve high-angular resolution. With the extreme stability of the images, detection at very low fluxes can be reached using a coronograph at the diffraction limit of the telescopes. This paper is an overview of the issues of stellar coronography used at the diffraction limit. Image formation through such a system is illustrated by numerical simulations. The description of a coronograph implemented on the VLT adaptive optics prototype, COME-ON, is presented as well as the first observations. | |
| dc.description | 23 pages including figures and tables, uuencoded gz-compressed postscript | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9509072 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9509072 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/10130 | |
| dc.subject | Astrophysics | |
| dc.title | High angular resolution coronography for adaptive optics | |
| dc.type | text |