Services
-
Articles citing this article
- Same authors
- Recommend this article
- Download citation
- Alert me when this article is cited
- Alert me when this article is corrected
|
Astronomy with High Contrast Imaging
C. Aime and R. Soummer (eds)
EAS Publications Series, Vol. 8, 2003
DOI: 10.1051/eas:2003061
"Planet Finder" on the VLT: context, goals and critical specifications for adaptive optics
D. Mouillet1, T. Fusco2, A.-M. Lagrange3 and J.-L. Beuzit31 Laboratoire d'Astrophysique, Observatoire Midi-Pyénées, France
2 DOTA, Office National d'Études et Recherches Aérospatiales, France
3 Laboratoire d'Astrophysique, Observatoire de Grenoble, France
Abstract
ESO offers the opportunity to install a new (second generation)
instrumentation on 8-m telescopes before 2010, for a wide community.
We, as a consortium, argue that it is possible to develop a high contrast
imager that will improve significantly or will complement current and
forthcoming instruments. This project would benefit a interesting number
of astrophysical issues; it will also prepare later more ambitious
ground-based imagers or space-based high contrast instruments.
The limitations of the turbulence are severe and demand very performant
adaptive optics. This critical question is addressed specifically.
© EAS, EDP Sciences 2003
| What is OpenURL? |

Document
BibSonomy
CiteUlike
Connotea
Del.icio.us
Digg
Facebook