Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
ONERA
ONERA, France and Groupement d'Intéret Scientifique PHASE, France
ONERA / DOTA, France and Groupement d'Interet Scientifique PHASE, France
Office National d'Études et de Recherches Aerospatiales, France
Office National d'Estudes et de Recherches Aerospatiales, France
Office National d'Études et de Recherches Aérospatiales, Département d'Optique Théorique et Appliquée, BP 72, 92322 Châtillon Cedex, France
ONERA, Chatillon, France
ONERA, BP 72, 92322 Chatillon, France
Office National d'Études et de Rechereches Aérospatiales, Chatillon, France
ONERA, France
ONERA, BP. 72, 92322 Chatillon Cedex, France; Departement d'Astrophysique, URA 709 du CNRS, UFR Faculte des Sciences, Universite de Nice-Sophia Antipolis, Parc Valrose, 06034 Nice Cedex, France
ONERA, DOTA-E, BP 72, F-92322 Chatillon, France
ONERA, Châtillon, France
Onera - France
Onera, France
ONERA, France and Groupement d'Intérêt Scientifique PHASE, France
Laboratoire D'Études Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris, Bât. 16, 5 Place J. Jansen, 92195 Meudon, France
ONERA -- DOTA, 92322 Châtillon, France
ONERA, BP72 - 29 Avenue de la Division Leclerc, F-92322 Chatillon Cedex, France
ONERA, BP. 72, F-92322 Chatillon Cedex, France
ESO
Office National d'Études et de Recherches Aérospatiales, France
ONERA, DOTA-E, BP 72, 92322 Châtillon, France
ONERA, BP 52, 29 avenue de la Division Leclerc, 92320 Châtillon Cedex, France
DOTA-ONERA, Av. de la division Leclerc, Châtillon, France
ONERA, Departement d'Optique Theorique et Appliquée, France
ONERA / Département d'Optique Théorique et Appliquée, BP 72, F-92322 Châtillon Cedex, France
ONERA, Optics Department BP 72, Chatillon cedex, 92322 France, Metropolitan
ONERA / France
A "Planet Finder" instrument for the VLT
A probable giant planet imaged in the Beta Pictoris disk
A simple and efficient model for polychromatic focal plane wave-front sensor
A strong volcanic outburst on Io as observed with the Keck AO system
Actual and future monitoring of Io's hot spots by used of Adaptive Optics systems
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