| Our product line combines ease of use with the wide-ranging functionality that scientific users depend on for aligning and characterizing optical systems including telescope mirrors and other imaging instruments used in astronomy. HASO™ wavefront sensors enable you to perform complete characterizations of laser beams including phase, intensity, M², and Strehl ratio. When used in conjunction with adaptive optics systems, they allow you to optimize the beam's shape and focal spot.
If you would like more information on our products, please call +33 (0)1 64 86 15 60 or e-mail us by clicking here.
Wavefront measurement and analysis
Software
- HASOv3 - the latest release of our flagship wavefront measurement
and analysis software offers a wide array of standard features
to make working with your HASO wavefront sensors easy. HASO
v3 provides wide-ranging diagnostic features, offers traceability
and security to fulfill the needs of the most demanding
scientists.
- Software Development
KIt - the solution to develop your own applications
with our sensors to perfectly fit your process or human
resources requirements.
Solutions
- LIP™ - the ideal accessory to your HASO sensor for easy and efficient
characterization of large mirrors. The LIP is the perfect
adjustment tool for your collimators and telescopes.
Adaptive optics and wavefront correction
- Wavefront sensors - HASO3 32 wavefront sensors offer the best combination of quality and price for control of active components.
- Wavefront correction - Our systems are ready to work with many of available wavefront correction
technologies: spatial light modulators (SLM),
Monomorph, Bimorph, Stack array, electrostatic... and the patented mirao™ 52-e Electromagnetic Deformable Mirror.
- Closed loop Software - Our latest proprietary CASAO™ software offers performances and security and large diagnostic
capability.
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