Abstract
We present simulations of a GLAO system in Dome C. The number of guide stars, the temporal frequency or the number of sub-apertures in the wave front sensor have to be optimized. Performances are presented.
© 2007 OSA
PDF ArticleWe present simulations of a GLAO system in Dome C. The number of guide stars, the temporal frequency or the number of sub-apertures in the wave front sensor have to be optimized. Performances are presented.
© 2007 OSA
PDF Article