YSL FEMTOYL™-100

YSL Photonics’ FemtoYL-100 is the latest 100W high power femtosecond fiber laser. It can deliver a ~400fs-6ps variable pulse width and over 100uJ pulse power, making it an ideal laser for micromachining application.

Applications:

• OLED Dicing
• Full Screen Dicing
• Sapphire Drilling
• Silicon Dicing
• SiC Dicing
• Metal Cutting and Drilling
• FPC Cutting

Features:
• Average Power 100W
• Pulse Duration ~400fs-6ps
• Peak Power 250MW
• Repetition Rate 25-5000kHz
• Pulse Energy 100uJ
• M2<1.3
• Burst Mode Function

Digital Microscope and Scanner O8

The unique solution for oil immersion, whole slide scanning and complete solution for digital microscopy.

 

See for yourself: scanned with 100 times oil

The image is hosted on PreciCloud, our web-based platform for centralizing
and digitization of your workflow.

Whole Slide Scanning

Scan entire slides and selected regions of interest with objectives from 20x to 100x in oil or air. For the first time, users are offered the ability to create the highest quality scanned whole slide images with oil lenses. The resulting images are stunning. The O8 is a great working tool for various applications, that enable completely new use cases. The availability of digital whole-slide images helps users simplify and standardize their work, increasing efficiency and quality.

Precipoint Digital Microscope and Scanner M8

Simplicity ~ The M8 from PreciPoint is as intuitive and ergonomic as your smart phone.

The M8 from PreciPoint is a microscope and a scanner at the same time, but as easy to handle as your smart phone. Don‘t get lost in the set up and operation of your work tool, we want you to be able to dedicate yourself
fully to your work.

You may operate the M8 from PreciPoint with a touchscreen computer, a tablet or a smart phone. The intuitive navigation makes you feel as if you could examine the sample with your own hands.

 Contact us today for free demo.

 

Andor iKon-XL 230 & 231

Andor’s iKon-XL is a thermoelectrically (TE) cooled, very large area CCD camera platform, accommodating large field of view sensors that are ideally suited to long exposure astronomy applications. Using the unique, patent-pending ColdSpace™ technology, the ultrasensitive iKon-XL is capable of TE cooling a 16.8 Megapixel sensor (e2v back-illuminated) down to -100 °C, avoiding the requirement for liquid nitrogen or unreliable cryo coolers. The iKon-XL also uses an exclusive Extended Dynamic Range technology, facilitating lowest noise and maximum well depth within one scan, complemented by up to 18-bit digitization capability. Flexible connectivity is standard through either USB 3.0 or a long distance direct fibre optic interface.

 

 

Andor iKon-M PV Inspector

Andor’s PV Inspector NIR Camera is designed to offer ultimate speed and sensitivity performance for in-line Electro- and Photoluminescence Inspection, delivering > 90% QE beyond 800 nm and incorporating Fringe Suppression Technology™ to minimize fringing effects in the NIR

  • QE > 90% beyond 800 nm
  • 5 MHz and 3 MHz readout speeds
  • Dual Exposure Ring Mode
  • Fringe Suppression Technology ™
  • UltraVac™

Andor Balor sCMOS

Balor is Andor’s game-changing, very large area sCMOS camera platform for Astronomy. It launches with the Balor 17-12 model, featuring an enhanced FoV 16.9 Megapixel, 70mm diagonal sensor, coupled with fast, low noise readout capability. Balor is ideal for measuring photometric and astrometric variability from milliseconds to tens of seconds timescales.

Balor is the largest commercially available sCMOS camera, designed for ‘dynamic astronomy’ applications such as Orbital Debris tracking, Solar Astronomy, Solar System Object detection, Exoplanet Discovery, Atmospheric Studies and Fast Time Resolution Astrophysics. Balor lends itself particularly well to the ‘atmospheric freezing’ techniques of Speckle/Lucky Imaging, enabling resolution enhancement of ground-based astronomy over a much larger field of view than is readily achievable through use of adaptive optics.

Key Applications

  • Orbital debris & asteroid tracking
  • Large sky surveys
  • Solar studies
  • Exoplanet discovery
  • Supernovae detection
  • Atmospheric studies
  • Speckle/lucky imaging

LUNA Phase Only Spatial Light Modulator (Reflective)

The LUNA phase only Spatial Light Modulator (SLM) consists of a driver unit with standard digital video interface (DisplayPort) and a phase only LCOS (Liquid Crystal on Silicon) microdisplay with full HD resolution (1920 x 1080 pixel) and 4.5 µm pixel pitch leading to an active area diagonal of 0.39” with an aspect ratio of 16:9.

The LUNA Spatial Light Modulator is our most compact SLM platform for integration into small sized or even portable solutions.

The LUNA phase only Spatial Light Modulator (SLM) consists of a driver unit with standard digital video interface (DisplayPort) and a phase only LCOS (Liquid Crystal on Silicon) microdisplay with full HD resolution (1920 x 1080 pixel) and 4.5 µm pixel pitch leading to an active area diagonal of 0.39” with an aspect ratio of 16:9.

The driver ASIC is embedded in the LCOS microdisplay itself. This saves board space which enables a very compact driver and makes integration more convenient. The standard driver box has a size of only 84.4 x 47 x 28.8 mm. The display can even accept video data input via a 4-lane MIPI DSI. This brings phase only Spatial Light Modulator technology to a new level of potential for industrial implementations.

The LUNA SLM usees fast full digital addressing which assures high reliability and a compact driver unit. A certain gray level represents a defined average voltage across the LC cell. This voltage leads to a variable tilt of the LC molecules due to their electrical anisotropy. As LC molecules also show optical anisotropy this tilt changes the refractive index of the LC molecules (for incident polarization along the long display axis) which causes a modified optical path length within the LC cell. The addressed gray level is converted into a phase level.

The LUNA driver unit is equipped with an USB interface for changing the voltage vs. phase level distribution (gamma control) and dynamic range (voltage across the LC cell) in order to calibrate the SLM for different wavelengths.

The LUNA SLM is a plug & play phase modulator and can be addressed with phase functions via standard graphics cards as extended monitor device. Addressing can be done using the supplied Pattern Generator software, the HOLOEYE Slideshow Player software or standard image viewer software. HOLOEYE also provides an SLM Display Software Development Kit (SDK) which provides APIs (Application Programming Interface) for different programming languages.

LUNA Spatial Light Modulator – Microdisplay Features
Display Type: Reflective LCOS (Phase Only)
Resolution: 1920 x 1080
Pixel Pitch: 4.5 µm
Fill Factor: 91 %
Active Area 8.64 x 4.86 mm (0.39″ Diagonal)
Addressing 8 Bit (256 Phase Levels)
Signal Formats DisplayPort – HDTV Resolution
Input Frame Rate 60 Hz

LUNA Phase Only Spatial Light Modulator Versions

LUNA LCOS SLM Wavelengths Ranges

HOLOEYE offers different phase display versions which can be driven with the LUNA driver unit. The different display versions are optimized for the use at different wavelength ranges. Currently we offer a VIS version (420 – 650 nm) and a version for the telecommunication waveband around 1550 nm (1400-1700 nm).

Version Wavelength Range Reflectivity Max. Phase Shift
LUNA-VIS-111 420 – 650 nm 61-67% 4.3 π @ 450 nm
3.2 π @ 520 nm
2.4 π @ 635 nm
LUNA-TELCO-112 1400 – 1700 nm 70 % 2.3 π @ 1550 nm

LUNA Spatial Light Modulator Kit – Contents:

 

LUNA Spatial Light Modulator – Scope of Supply
LUNA phase display (1920 x 1080 pixel) incl. flex cable
LUNA driver unit
USB Cable
DisplayPort / Mini DisplayPort cable
Magnetic display mount & display adaptor
Screw adaptor M4 to ½”
Safety instructions & quick-start guide
USB flash drive with documentations, detailed manual, Configuration Manager and SLM software

LUNA Phase Modulator – Software Features:

he LUNA phase only spatial light modulator devices can simply be addressed like an external monitor using the standard DisplayPort interface of the graphics card. No additional software or dedicated hardware is needed to operate the SLM.

The device is delivered with a Configuration Manager software. The Configuration Manager can be used to change geometrical settings, brightness, contrast and the electrooptical response by applying a new gamma curve or another digital drive scheme. For these advanced calibrations the device uses an USB connection to a virtual COM port of the computer.

In addition a HOLOEYE SLM Pattern Generator software is provided with the SLM:

  • Computation of computer generated holograms (CGH) from user defined images
  • generation of SLM signals representing basic optical functions such as lenses, gratings, axicon and vortex functions
  • superposition of CGH’s with basic optical functions to combine functionalities

Besides that a special SLM Slideshow Player Software comes with the device. Also an SLM Display SDK is available for download which provides APIs (Application Programming Interface) for different programming languages to show images and data/ phase arrays directly on a HOLOEYE Spatial Light Modulator:

  • National Instruments LabVIEW™ 8.6 and later
  • MathWorks MATLAB® R2009b and later
  • Octave 5.2
  • Python™ 2.7 and 3.x
  • C or C++ compiler (e. g. Microsoft Visual C++ Compiler)

Driver Dimensions (Unit: mm):

LUNA LCOS Spatial Light Modulator Driver Dimensions

Display Dimensions (Unit: mm):

The current LUNA microdisplay package has a size of only 25.7 x 12.6 x 3.4 mm. For more convienient mounting we deliver it with a display mounting adaptor.

LUNA LCOS Spatial Light Modulator Display Adaptor

 

LETO-3 Phase Only Spatial Light Modulator

The LETO-3 phase only Spatial Light Modulator is based on a reflective LCOS microdisplay with full HD (1920 x 1080 pixel ) resolution. With a pixel pitch of 6.4 µm and a small interpixel gap of 0.2 µm the LETO-3 SLM provides a high fill factor of 93%.

The LETO-3 Spatial Light Modulator offers a reflectivity between 62% up to 75% (dependent on wavelength and version). The device offers diffraction efficiencies of more than 80% (16 level blazed grating) which leads to a total light efficiency of ~ 60%.

The LETO-3 SLM driver is prepared to work in color-field-sequential (CFS) mode e.g. with color-switchable LASER or LED lighting and the device features an LED-connector which can be used to synchronize the light source with the device. The driver features 4 slots with preconfigured CFS configurations for different environments which can be slected using the Configuration Manager Software.

 

 

Versions

HOLOEYE offers three different LETO-3 Spatial Light Modulator versions which are optimized for the use at different wavelength ranges / for different applications. One SLM version is optimized for the visible range, one version for the near IR range up to 1100 nm and a third version is optimized for fast response (180 Hz) and use for color-field-sequential (CFS) operation in the visible range with color-switchable RGB Laser.

LETO-3 Spatial Light Modulator Wavelength Ranges

QNW – Temperature-Controlled Cuvette Holder for UV/Vis Spectrophotometers

The t2 Sport™ is a Peltier-Temperature controlled cuvette holder with two optical ports for absorbance. It has a short, compact structure that will fit into nearly any UV/Vis spectrophotometer.

t2 Sport™: Temperature Controlled Cuvette Holder for UV/Vis Spectrophotometers

The device is mounted on a post to allow adjustment of the cuvette to the optimal height. On ordering, the user selects the cuvette holder z-height of 8.5 or 15 mm. With variable-speed magnetic stirring, the t2 Sport™ is built to maintain uniform temperature within the cuvette. A dry gas purge system directs dry gas to the surfaces of the cuvette to minimize condensation when working below the dew point temperature.

The t2 Sport™ package includes a matched and calibrated TC 1 Temperature Controller, and provides rapid, precise temperatures in the range of -15 °C to +110 °C with a precision of ±0.02 °C. While lower temperatures may be readily achieved, it is important to avoid the risk of condensation on cuvette surfaces. The TC 1 controller has a probe input that accepts a Series 400 or Series 500 thermistor probe for independent measurement of the sample temperature.

Versions of the t2 Sport™ are available for mounting in a variety of different spectrophotometers. The device can be easily adapted to others as needed. For more information on an individual adaptation, click on a version below.