Showing results: 91 - 98 of 98 items found.
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Sidewinder - TE cooled -
OtO Photonics Inc.
Sidewinder - TE cooled Series spectrometer ,built with the InGaAs type sensor and high performance 32bits RISC controller in, is specially designed for long wavelengths range. The optical engine is very simple and optimized for the spectrometer. The optical bench is very rigid and stable for measurement system, especially SW series has outstanding stability of thermo-hygro variation, vibration and shock on resolution and wavelength shift performance. The compact size is very flexible for system integration.
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InfraScan™ 400TDM -
Checkpoint Technologies, LLC.
The InfraScanTM 400TDM is the newest evolution of Checkpoint's pioneering top-down laser scanning and emission tools. This tool is specifically designed to accommodate any commercially available probe station, up to 300 mm wafers. The combination of Checkpoint Technologies, world leading laser scanning microscope and its best in class emission system into a single tool, gives users the most sensitive and easy to use system on the market. The TDM can be configured with up to 3 lasers and a choice of InGaAs, MCT or Si CCD emission cameras.
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OWL 1280 -
Raptor Photonics
Using a 1280 x 1024 InGaAs sensor from SCD, the OwL 1280 offers visible extension from 0.6µm to 1.7µm to enable high sensitivity imaging. The 10µm x 10µm pixel pitch enables the highest resolution imaging. It will offer less than 28 electrons readout noise (rms) and with a high intra-scene dynamic range of 51dB, this enables simultaneous capture of bright & dark portions of a scene. Available with a 12 bit medium Camera Link digital output, the Owl 1280 will run from 10 to 60Hz. The camera features an on-board Automated Gain Control (AGC) which enables the best contrast image from low to bright light. The camera also has an on-board intelligent 3 point Non Uniform Correction (NUC) providing the highest quality images. As with all Raptor cameras, the Owl 1280 is ultra compact and rugged. The camera sensor temperature is stabilised to 15°C and the camera does not have a fan.
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CA92001B -
UC Instruments, Corp.
UCINSTRUMENTS CA92001B C band optical spectrum analyzer module is a spectral engine for Process Analytical Technology applications. The OSA module acts as a stand-alone spectral engine, imaging and measuring a wide range of vapors, liquids and solids through transmission and diffuse reflection in a rapid non-destructive process. Leveraging our proprietary Micro-Optic technology, UC INSTRUMENTS’ C band OSA module features the following characteristics: (1) compact; (2) light-weight; (3) low power consumption; and (4) wide wavelength coverage. These characteristics of UC INSTRUMENTS’ compact OSA engines are suitable for a variety of handheld, portable or bench-top OSA/spectrometer applications. Equipped with a state-of-the-art internal wavelength reference, the OSA module is capable of precisely measuring optical spectrum. Because it does not require an expensive InGaAs detector array, the compact OSA module is a cost-effective alternative to other grating-based OSA/spectrometer engines. The OSA communicates with a PC or an instrument motherboard via an USB interface. UCINSTRUMENTS’ OSA module platform can be installed or co-packaged into existing NIR OSA/spectrometers as a cost-efficient alternative to other scanning optical engines.
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Wildcat+ 1280 Series -
Xenics
The Wildcat+ 1280 series is based upon a state-of-the-art InGaAs photodiode array with 1280×1024 pixels and 5 μm pixel pitch. The camera offers superior, high-resolution SWIR imaging capabilities, comes in a versatile and industry-proven Wildcat camera package (GenICam compliant) and offers advanced on-board image processing.The Wildcat+ 1280 camera outputs full frame images at 120 Hz via either a CameraLink or USB3 Vision interface.The Wildcat+ 1280 is suitable for semiconductor inspection, display inspection (mobile phone and TV), microscopy and laser beam analysis.Benefits & Features• Compact and industry-proven camera design• High-resolution SWIR imaging• Advanced on-board image processing performance• GenlCam compliant• Flexible optical mount and lens options
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MPA-100 -
Santec Corporation
MPA-100 is a highly integrated rack mountable model of pigtailed photo-detectors. Multi-channel optical power from MPO or MTP connectors are measured. Photo-detectors of Silicon type for 850 nm range and InGaAs type for 1260 - 1610 nm are available. The detected photo-current is converted into a voltage output using a 16-bit multi-channel DAQ interface. The dimensions are (W) 482.6 x (D) 430 x (H) 44 mm. The highly integrated MPA-100 is available up to 80 channels with an excellent cost performance and small footprint. The MPA-100 is useful for many 40 GbE / 100 GbE applications, such as testing and monitoring of transceivers (SR4, SR10, LR4, and ER4) for data communications, broadband / CATV, and telecommunications. Tap-PD model (Eg. a partial 5 % tapped power detection) is also available with customization.
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mks Ophir
Pulse Characterization Sensors provide the ability to see and measure the temporal characteristics of pulsed and CW laser beams. Ophir Fast Photodiode Detectors are designed to convert optical signals into electrical signals which are then measured with third-party instrumentation such as oscilloscopes and spectrum analyzers. Accessories are available to connect to IS6 integrating spheres or fiber optic cables. Attenuating filter accessories are also available to increase their dynamic range. Different models offer silicon, UV enhanced silicon and InGaAs PIN photodiodes, covering a combined spectral range of 193 nm to 1700 nm. Rise times range from 25 picoseconds to 3 nanoseconds. The fast rise times are achieved by an internal reverse bias voltage circuit. Power is supplied by internal batteries and/or an external power supply depending on the model. Detectors should be connected to a 50Ω impedance in order to maintain their nominal rise times. They can be connected to higher impedance loads, but this will result in a significant increase in the rise time. If higher output voltage is required, it is recommended to connect the detector to a trans-impedance amplifier with an Input impedance of 50Ω
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1024L1 -
Princeton Infrared Technologies, Inc.
The 1024L1 is a 1024x1 state of the art InGaAs linear array imager on 12.5 µm pitch that was built for both spectroscopy and machine vision in the short wave infrared band. The 1024L1-12.5-T is an advanced digital array with the lowest read noise available <110e- for a 250 μm tall pixel. Our new advanced SWIR On-chip Noise Suppression Circuit will enable some spectroscopic applications to see read noise levels <80e-. A single ROIC chip is used thus minimizing variation from output to output found on linear arrays with multiple ROICs. The chips have built in 14bit A/Ds that are designed for the system thus maximizing dynamic range and minimizing the noise while enabling 34k lines/s at 1024 elements. Multiple full well capacities from 75ke- to 100Me- with 128 steps are available to optimize the array for the signal levels. On chip optical pixel binning (where every other detector is disconnected from the ROIC thus signal is captured by neighboring pixels) is available by command to trade spectral resolution for increased signal level. Pixel skipping or binning is also available allowing for 48k lines/s at 512 resolution on the same imager.
