The adaptive optics system Naco

Recipe against atmospheric turbulence: the adaptive optics system Naco at the  Very Large Telescope.  

NACO is a first generation VLT instrument, developed in a joint effort between French and German research institutes and ESO. NACO is short for NAOS-CONICA, which acronyms in turn stand for the instrument's two sub-systems:

The Nasmyth Adaptive Optics System (NAOS) has been developed, with the support of Institut National des Sciences de lUnivers/Centre National de la Recherche Scientifique (INSU/CNRS) by a French Consortium in collaboration with ESO. The French consortium consists of Office National d'Etudes et de Recherches Aèrospatiales (ONERA), Institut de Planetologie et d'Astrophysique de Grenoble (IPAG, formerly called Laboratoire d'Astrophysique de Grenoble) and Observatoire de Paris: Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA, formerly called DESPA) and DASGAL (which does not exist anymore). The Project Manager is Gérard Rousset (ONERA), the Instrument Scientist responsible is François Lacombe (Observatoire de Paris) and the Project Scientist is Anne-Marie Lagrange (Institut de Planetologie et d'Astrophysique de Grenoble, OSUG, Université Joseph Fourier/CNRS).

The CONICA Near-Infrared CAmera has been developed by a German Consortium, with an extensive ESO collaboration. The Consortium consists of the Max Planck Institute for Astronomy (MPIA) (Heidelberg) and the Max Planck Institute for Extraterrestrial Physics (MPE) (Garching). The Principal Investigator (PI) is Rainer Lenzen (MPIA), with Reiner Hofmann (MPE) as Co-Investigator.

MP/HOR

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