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A trusted technology for telescope alignment and characterization

A trusted technology for telescope alignment and characterization

For the past 25 years, Imagine Optic's HASO family of wavefront sensors and optical metreology systems has relied on Shack-Hartman wavefront measurement. This technology was originaly developed for the metrology of primary mirrors, and subsequently used in adaptive...

Optics Characterization with R-Flex2 and R-Flex LA – webinar

Optics Characterization with R-Flex2 and R-Flex LA – webinar

Optics Characterization" ran 3 succesful sessions, and inaugurates a series of wavefront metrology. The 100+ attendees saw live demos by our CTO Guillaume Dovillaire to demonstrate the outstanding capabilities of our newly released R-Flex2 and R-Flex LA, and notably...

10 reasons to use Shack-Hartmann wavefront sensors

10 reasons to use Shack-Hartmann wavefront sensors

Wavefront sensors have various perceived benefits but here are 10 objective reasons that have made Shack-Hartmann a trusted standard in the field.  Real time measurement (up to several kHz) Achromatic Absolute measurement (typ. lambda/100, lambda/1000 achievable)...

Make the Most of UHIL Systems with Adaptive Optics

Make the Most of UHIL Systems with Adaptive Optics

Adaptive Optics (AO) dramatically improve the performance of optical systems by mastering wavefront distortions to deliver optimal focus and quality imaging for both scientific and industrial applications. The principle of an AO optimization for UHIL is that a...