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Mars with adaptive optics

Mars with adaptive optics

Imagine Optic is proud to share this image of the planet Mars (high resolution) acquired at Pic Du Midi with the 1 meter diameter telescope "T1M." We used an adaptive optic system "CIAO" to get rid of the telescope's static aberrations and some of the turbulence...

Adaptive Optics opens gates for Nobel prizes

Adaptive Optics opens gates for Nobel prizes

In the past six years, adaptive optics (AO) has contributed to 8 Nobel Prizes. Unseen but essential, adaptive optics allows significant improvements in optical performance for imaging and laser systems... and Nobels. The 2014 chemistry laureates, Stefan Hell, Eric...

Adaptive Optics boost Lattice Light Sheet Microscope in Premiere

Adaptive Optics boost Lattice Light Sheet Microscope in Premiere

A flavor of the now trending light sheet microscopy, the Lattice Light Sheet Microscopy (LLSM) developed by Eric Betzig at Janelia Research Campus, recently revolutionized the field of in vivo microscopy. Despite the superb imaging performance provided by LLSM, this...

10 PetaWatts peak power at ELI-NP

10 PetaWatts peak power at ELI-NP

The most powerful laser in the world has reached 10 PetaWatts with a 0.9 Strehl ratio, and the help of Imagine Optic's AO Laser solutions. In the last two decades, adaptive optics (AO) has dramatically improved the performance of Ultra-High Intensity Laser (UHIL) by...

(Re)watch A Practical Tour of Adaptive Optics

(Re)watch A Practical Tour of Adaptive Optics

Our third webinar and live demo completes our on ongoing series on wavefront metrology and correction. You can (re)watch our 3rd webinar, a practical tour of adaptive optics, wavefront sensing and correction. Our CSO Xavier Levecq, and our CTO Guillaume Dovillaire...

Can you trust your wavefront sensor ? (Re)watch our live demo webinar

Can you trust your wavefront sensor ? (Re)watch our live demo webinar

 Putting trust in your wavefront sensor is a necessity at some point. It is precisely the reason why our CSO Xavier Levecq addressed fundamental topics on wavefront analysis, and best practices/tips and tricks to evaluate the accuracy and trustworthiness of any...

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...

Maximize EUV-XUV photons through adaptive optics for HHG

Maximize EUV-XUV photons through adaptive optics for HHG

The use of adaptive optics (AO) for IR wavefront control is essential to optimize the phase-matching conditions and therefore enhance the signal of the HHG. Furthermore, the vortex IR driver results in up-converted EUV with a wide range of orbital angular momentum...

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)...