Hostname: page-component-745bb68f8f-hvd4g Total loading time: 0 Render date: 2025-01-11T22:25:42.893Z Has data issue: false hasContentIssue false
  • English
  • Français

"Planet Finder" on the VLT: context, goals and critical specifications for adaptive optics

Published online by Cambridge University Press:  28 May 2003

Claude Aime ,
Rémi Soummer ,
D. Mouillet ,
T. Fusco ,
A.-M. Lagrange  and
J.-L. Beuzit
D. Mouillet
Affiliation:
Laboratoire d'Astrophysique, Observatoire Midi-Pyrénées, France
T. Fusco
Affiliation:
DOTA, Office National d' Études et Recherches Aérospatiales, France
A.-M. Lagrange
Affiliation:
Laboratoire d'Astrophysique, Observatoire de Grenoble, France
J.-L. Beuzit
Affiliation:
Laboratoire d'Astrophysique, Observatoire de Grenoble, France
Get access

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 contrastimager that will improve significantly or will complement current andforthcoming instruments. This project would benefit a interesting numberof astrophysical issues; it will also prepare later more ambitiousground-based imagers or space-based high contrast instruments.The limitations of the turbulence are severe and demand very performantadaptive optics. This critical question is addressed specifically.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 8: Astronomy with High Contrast Imaging , 2003 , pp. 193 - 199
Copyright
© EAS, EDP Sciences, 2003

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)