Untitled - Laboratoire d'Astrophysique de l'Observatoire de Grenoble
Untitled - Laboratoire d'Astrophysique de l'Observatoire de Grenoble
Untitled - Laboratoire d'Astrophysique de l'Observatoire de Grenoble
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Figure 12.1: All the GRIL projects for the next 5 years. Those yet to be <strong>de</strong>ci<strong>de</strong>d are indicated as ”un<strong>de</strong>r<br />
discussion”. Note that GRIL will not get involved in all of them (see text). See also caption of Figure 10.1<br />
OPTIONAL PROJECTS<br />
Following the opportunities that will appear in the next years, the LAOG could participate in the projects<br />
presented below <strong>de</strong>pending on the conditions and possibilities.<br />
Interferometric telescopes AO equipment Equipping with AO systems the small telescopes used, for<br />
instance, in large interferometers is in discussion. Observations with the VLTI AT would benefit from it and a<br />
similar need is invoqued for CHARA. These needs may be covered by low-cost AO systems that are still to be<br />
<strong>de</strong>signed. In the event where the LAOG would start a full AO system <strong>de</strong>velopment, we would establish a link<br />
with these partners in or<strong>de</strong>r to try collaborating on this matter.<br />
AO equipment for ELT Another direction in the longer range is a participation to the AO equipment<br />
of ELT by providing micro-mirrors components and possibly other sub-systems of these probably large and<br />
complex systems. AO might be employed here not only for turbulence-<strong>de</strong>gra<strong>de</strong>d PSF correction but also for<br />
instrumental phase errors correction. Our involvement will largely <strong>de</strong>pend on the success of R&D planned in<br />
the JRA1 and on the conceptual view emerging from the starting studies.<br />
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