Adaptive Optics System
The Adaptive optics package is based on a 4 sub-aperture Shack Hartmann Wave Front Sensor (SHWFS) and a bimorph wave front corrector. The system is intended to correct atmospheric fluxuations seen by the telescope.
Rear view of the Bimorph
View from the science camera position
Top view of the optical bench
Front view of SH Wave front sensor
