The HASO DUV Shack Hartmann wavefront sensor combines all the unique features developed by Imagine Optic during 30+ years of innovation and customers feedback: ease of use (absolute measurement thanks to the embedded factory calibration), high performance (high accuracy of lambda/100 RMS, very large dynamic range), robustness (phase measurement independent of beam intensity variation, achromaticity over calibrated spectral range, insensitivity to vibrations).

Software

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The R-Flex Kit comprises 3 features essential for customer Quality Assurance and easier Quality Control:

1/ Verify periodically the calibration of Imagine Optic’s R-FLEX2 VIS and R-FLEX2 SWIR metrology systems
2/ Inspect and clean them if necessary
3/ In the case of the R-FLEX2 SWIR metrology systems, facilitate its optical alignment on the optic to be tested by the use of visible light source

Box Content

+ Instructions for R-FLEX2 calibration check
+ Calibration check accessory with retroreflector and autocollimation flat reference mirror
+ Source for prealignment of the system at a visible wavelength
+ Fiber visual fault locator
+ Lamp, telescopic inspection mirror, Air blower and soft lens brush for dust inspection and cleaning
+ Optional R-FLEX50 adapter

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Easy to use and reliable, these mount stages provide perfect alignment for your family of wavefront sensors and R-FLEX2. They have been designed and assembled in such a way that their center of rotation corresponds to the sensor analysis pupil: so you can perform pure alignment without having to compensate for unwanted translation of the analysis pupil. A must-for quick and easy installation of you instrument. You’re welcome!

Mount Stages for wavefront sensing

The mount stages are ready-to-use solutions for quick and easy alignment of your instrument. HASO and LIFT wavefront sensors need Tip-Tilt degrees of freedom while OEC R-FLEX metrology systems need X, Y, Z translations in addition.

Features

Mounts and wavefront sensors compatibility

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MESO SWIR metrology system is a one-stop solution to many challenges in optical metrology. Shop floor measurements ensure quality control testing and in situ process control of your flat optics right next to the manufacturing line. A unique instrument allows to measure at several different wavelengths with no chromatic abberations and to characterize the whole range of your optics with no loss of resolution.

MESO™ is packed with innovation:

+ LIFT-enhanced high wavefront sensing resolution
+ POP patented  procedure for the testing of (thin) plane parallel optics
+ Spot Tracker™ proprietary technology provides absolute measurement of tilt and wavefront.

KEY FEATURES​

+ Insensitive to vibrations​
+ At-design wavelength testing​
+ Insensitive to reflections from sample back surface​​

APPLICATIONS​

MESO is the perfect testing tool for the control of:

KEY SPECS of MESO SWIR metrology system

WAVESURF supportive Software for MESO metrology system​

​Wavesurf allows operators and engineers in manufacturing environments to perform wavefront and surface characterization of flat optics and large lenses with just a few clicks. Scripted testing procedures guide users through all the steps. It makes control easy, automated and error-proof.

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The LIFT LP 512 phase retrieval wavefront sensor combines all the unique features developed by Imagine Optic during 30+ years of innovation and customers feedback: ease of use (absolute measurement thanks to the embedded factory calibration), high performance (high accuracy of lambda/100 RMS, very large dynamic range), robustness (phase measurement independent of beam intensity variation, achromaticity over calibrated spectral range, insensitivity to vibrations) together with ultra high resolution (spatial resolution x16 compared with Shack Hartmann).

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With its very high frame rate, the HASO SWIR FAST Wavefront sensor is used in most demanding applications where measurement accuracy in Soft Wave InfraRed bandwidth and high temporal resolution are needed. Thanks to its large wavefront measurement dynamic and its internal calibration, its implementation in an optical bench is simplified.

Software

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The HASO LP Shack Hartmann wavefront sensor combines all the unique features developed by Imagine Optic during 30+ years of innovation and customers feedback: ease of use (absolute measurement thanks to the embedded factory calibration), high performance (high accuracy of lambda/100 RMS, very large dynamic range), robustness (phase measurement independent of beam intensity variation, achromaticity over calibrated spectral range, insensitivity to vibrations)

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WAVESQUARED M2 factor analysis software has been designed specifically to pair with CAMSQUARED M and CAM SQUARED L laser quality testing solutions for the lab or the production.

Key features M2 factor analysis software

+ 3 clicks acquisition set up
+ Live M2 measurement (µs to ms acquisition cycle)
+ ISO 11146 standard (astigmatic, circular, general astig or auto detection)
+ Automatic pdf report generation for laser testing traceability
+ Compatible Windows 10 and Windows 11

Laser beam parameters and displays

+ M-Squared factor (M2)
+ Width at waist
+ Divergence angle
+ Beam Propagation Parameter (BPP)
+ Waist location
+ Astigmatism
+ Asymmetry ratio and more. All parameters acquired in live can be displayed in time plots

Options in WAVESQUARED M2 factor analysis SOFTWARE

Full wavefront analysis is available in option. It is best for:
+ Live alignment thanks to the knowledge of aberrations
+ Collimation
+ Beam pointing stability

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MS-LAMBDA is a compact electronic driver embedding laser diode or SLED at any wavelength you need for your optical setup.
Its monomode fiber output generates a spherical wavefront that makes optical engineer life easy to create high quality illumination paths.

+ WAVELAMBDA dedicated SW for remote control
+ Optional SDK for interfacing

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Connecting directly to the telescope eyepiece, CIAO is inserted between the telescope’s focal plane and the user plane (sensor or fiber holder) without modifying the optical path. Set up is facilitated by the embedded tip-tilt alignment interface and autocalibration tools. After pointing on the target, the user can close the Adaptive Optics loop with a simple click, to activate the aberrations correction or to lock in very fine pointing.   

Software 

+ Dedicated software for fast AO loop control
+ Many parameters are available to optimize the loop and adapt the configuration to the telescope, the seeing condition, the target and the application.

CIAO is a compact innovative adaptive optics add-on that enhances your telescope’s performance. We customize for our users: please contact us to discuss how it benefits your application 

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