[en] Adaptive optics (AO), by compensating in real time the blurring due to atmospheric turbulence, improves the angular resolution and the sensitivity of ground-based telescopes. AO represents an opportunity for medium size telescopes to be competitive with respect to large and very large observatories. AO can be beneficial for most scientific cases and – we think – reachable with a reasonable effort. In this contribution, we review the current state of adaptive optics in medium size telescopes, discuss promising avenues and present a possible science case for the DOT. In the second part, we present the relevant expertise we are currently building up in Lie`ge in the framework of the SALTO project, a 1-m telescope demonstrator with laser guided adaptive optics.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Orban De Xivry, Gilles ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > PSILab
Absil, Olivier ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > PSILab
Moreau, V.; Advanced Mechanical and Optical System
Language :
English
Title :
A sharp future for the 3.6-m DOT? The power of adaptive optics for medium size telescopes
Publication date :
2019
Journal title :
Bulletin de la Société Royale des Sciences de Liège
ISSN :
0037-9565
eISSN :
1783-5720
Publisher :
Société Royale des Sciences de Liege, Liège, Belgium