Shack-Hartmann wavefront sensor for optimizing telescopes
A finely tuned telescope is the key to obtaining deep, highquality astronomical images.
Puntino, our Shack-Hartmann wavefront sensor specially developed for telescopes, is based on our extensive 10-year experience of use at observatories around the world.
It gives you complete analysis of the optics, mechanics, mirror supports, mirror and dome seeing.
Based on the analysis, the software suggests corrective action to be taken, enormously simplifying maintenance work, enabling you to achieve in hours what would normally take longer.
In keeping with our philosophy of providing you with a full set of tools, we also provide a CCD-based system for alignment telescopes and autocollimators.