Hostname: page-component-78c5997874-dh8gc Total loading time: 0 Render date: 2024-11-04T19:48:23.598Z Has data issue: false hasContentIssue false

High order Adaptive Optics Requirements and feasibility for high contrast imaging

Published online by Cambridge University Press:  02 May 2006

T. Fusco
Affiliation:
ONERA, B.P.72, 92322 Chatillon, France
G. Rousset
Affiliation:
ONERA, B.P.72, 92322 Chatillon, France
J.-L. Beuzit
Affiliation:
Observatoire de Grenoble, B.P. 53, 38041 Grenoble, France
D. Mouillet
Affiliation:
Observatoire Midi-Pyrénées, B.P. 826, 65008 Tarbes, France
K. Dohlen
Affiliation:
Observatoire de Marseille, B.P. 8, 13376 Marseille, France
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

In the frame of the VLT Planet-Finder project, the phase A system study has demonstrated the feasibility of an extreme adaptive optics system aimed at the direct detection of extrasolar giant planets. The main results of this study are presented in this paper.

Type
Contributed Papers
Copyright
© 2006 International Astronomical Union