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Deep UV
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LED Phosphorescence Light Sources
SpectraLED
Innovative and affordable pulsed light source for phosphorescence measurements from deep UV to NIRThe SpectraLED is a novel light source designed specifically for the measurement of phosphorescence lifetimes. These phosphorescence sources are based on LED technology and the emission wavelengths range from the deep UV to the NIR.
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Photodiodes
Opto Diode manufactures high quality standard and custom photodiodes. Our wide range of standard device feature low dark current and low capacitance. The silicon detectors are ideal for general purpose applications, laser monitoring, position sensing, measuring photons, electrons, or X-rays, or for detecting sun and rain applications. The devices operate from the deep UV to the near-infrared wavelengths.
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Ambient Pressure Photoemission Spectroscopy With Nitrogen Environment
The APS04-N2-RH incorporates a tuneable deep ultra-violet (UV) source outputting 3.4 - 7.0 eV, for absolute work function and highest occupied molecular orbital (HOMO) measurements, a surface photovoltage spectroscopy (SPS) module outputting 400 - 1000 nm for Voc and Eg measurements, together with a 50 x 50 mm scanning area for planar relative work function measurements (Fermi level).
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DUV Lithography Systems
ASML's deep ultraviolet (DUV) lithography systems dive deep into the UV spectrum to print the tiny features that form the basis of the microchip.
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Deep Cooled UV/Vis/NIR and VUV Scientific Cameras
Syncerity Scientific Cameras
HORIBA Scientific offers a complete line of spectroscopic multi-channel detectors for scientific research. For spectral detection from UV to near-IR, two dimensional CCDs offering a faster acquisition option over single point detectors with relatively high sensitivity. Coupled with HORIBA’s range of aberration corrected flat field imaging spectrographs, OEM packages can be assembled for a variety of applications.
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UV SHG Cavity Compact Frequency Quadrupling Module
SolsTiS ECD-X-Q
SolsTiS ECD-X Q extends the range of the SolsTiS platform into the deep UV providing unrivalled power and tuning. SolsTiS ECD-X-Q is used in combination with the ECD X doubling cavity (wavelength ranges between 210–250 nm) or the EMM mixing module (wavelength ranges between 250–300 nm).
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photonSPECTRAL
Photonfocus has developed outstanding solutions for numerous fields of application in order to meet the growing demand for imaging applications in invisible light spectra. The photonSPECTRAL platform offers highly sensitive cameras with wavelengths ranging from deep UV to short-wavelength infrared light (SWIR), as well as innovative systems for the hyperspectral range. Our vast expertise in this area is also reflected in our leading market position: Photonfocus launched a UV-suitable CMOS camera with global shutter for machine vision applications.
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Fluorometers
Our Fluorometers can accommodate any size work-area, and are available as compact or benchtop models, or as large modular systems, to suit your requirements. In addition, our Fluorometers can be coupled to become modular Fluorometer systems, or supercontinuum white-light laser-powered lifetime Fluorometers!HORIBA’s Fluorometers offer incredibly fast lifetime determinations down to picoseconds, deep UV absorbance and fluorescence excitation from as short as 200 nm in the UV, all the way to near-IR wavelengths of 1000 nm.
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Laser Power Sensors
Make accurate laser power measurements, from the deep UV to the infrared, with these calibrated, traceable sensors.
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Deep Cooled UV-VIS/NIR Scientific Cameras
TE and cryogenically cooled CCD and EMCCD scientific cameras for ultra sensitivity from 200 nm to 1100 nmHORIBA Scientific offers a complete line of spectroscopic multi-channel detectors for scientific research. For spectral detection from UV to near-IR, two dimensional CCDs and indium gallium arsenide linear arrays offer a faster acquisition option over single point detectors with relatively high sensitivity. Coupled with HORIBA’s range of aberration corrected, flat field imaging spectrographs, custom spectroscopy packages can be assembled for a variety of applications.
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Intensified Cameras - Ultra-Sensitive CMOS Cameras from Deep UV to NIR Spectrum
iCameras
The cameras are equipped with a high-resolution sensor with high frame rate for excellent quality of image production, which is well‐suited to detect high speed moving objects or ultra-fast phenomenon.The mechanical architecture of the iCamera is small, compact and light-weight, especially designed for easy integration into any system.The iCamera features an exceptional sensitivity based on high QE image intensifier - ultra-fast gating technology down to a few nanoseconds, which allows it to be coupled with a laser source to perform high fidelity active imaging.
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M2 & BPP Systems
The M2 factor wil define the beam propagation characteristics compared to ideal Gaussian beam propagation. According to ISO Standard 11146 rightfully offers the laser beam characterization as "M2 times diffraction limited beam", as such, a perfect beam will have an M2 of 1. 1 will be the best achievable value and no beam could have an M2 less than 1. Our conceptual design is based on sub-assemblies allowing to change the sensing head in the M2 device, offering multiple wavelengths heads up to 2.7 microns from deep UV (knife-edge technology) and camera based technology with built-in automatic filter wheel for adjustment. For focused beams, the same measuring head could be attached to a device for meauring highly divergent or highly convergent beams - FocusGage-BA, wherein the Laser Analyzing Electronic Autocollimator offers the capability of divergence measurement with Coming Soon M2 definition. M2Beam is the cornerstone of those measuring devices.
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UV Analyzer
AF45
The AF45 is a high precision UV light absorption analyzer designed for inline operation to provide accurate concentration measurements with remarkable repeatability, linearity and resolution. Wavelength and optical path length are individually configurable for extremely high accuracy to meet process control requirements.
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UV Meters
USHIO developed a UV meter series to measure intensities of UV radiation. As an add-on, the temperature is also registered. You can decide between the high-end UV meter UIT-250, and UIT-201. The former has a wider measurement range, allows the measurement of energy doses and has the capability to transfer the data via a serial communication protocol to a PC. Various sensors are available. The most popular sensors have center wavelengths at 254 nm, 365 nm or 410 nm.
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UV Calibration
Determination of the angle dependent sensitivity of sensors in use with different UV lamps
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Deep Ultraviolet Spectrophotometer System
VUVAS-10X
A new ultraviolet spectrophotometer system for optical metrology just arrived at NASA Goddard! The VUVAS-10X spectrophotometer works best in the 90 to 160 nanometer wavelength range, also known as deep or vacuum ultraviolet (VUV) region. It uses a windowless hydrogen plasma light source and differential pump section to reach many wavelengths beyond those of conventional deuterium lamps. The source also works with other gases, or gas mixtures, for atomic spectral line emission from about 30 nanometers (double ionized Helium gas) up to the Visible light range. The new spectrophotometer system, McPherson VUVAS-10X, uses a one-meter focal length high-resolution monochromator with the special light source, scintillated detector and Model 121 goniometric sample chamber. The system is ideal for optical transmission, absorbance and specular reflectance at incident angles up to 60 degrees. This McPherson spectrophotometer system will help develop, inspect and qualify optical materials and coatings used for very high altitude and extraterrestrial space flight missions.
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UV Light Meters
* Long wave 365 nm ultra-violetirradiance measurement.* Professional, high quality UVA meter.* Wide measurement range,199.9 uW/cm^2, 1.999 mW/cm^2 and19.99 mW/cm^2.* Microprocessor circuit assuresmaximum possible accuracy,provided special functions andfeatures.* Exclusive UVA sensor withcorrection filter.
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UV Analyzer
AF46
The AF46 is a dual wavelength, high precision UV light absorption analyzer designed for inline operation to provide accurate concentration measurements with remarkable repeatability, linearity and resolution. Wavelength and optical path length can be individually configured to specific requirements for the highest accuracy.
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On-Camera Deep Learning
Firefly DL
Deep learning is a powerful tool for system designers to quickly automate complex and subjective decision making and deliver higher quality products and improved productivity. Deploy your trained neural network to the FLIR Firefly DL with Neuro technology and reduce system cost and complexity by making decisions on-camera without host PC. With its very small size, low weight and power consumption, the Firefly DL camera is ideal for embedding into mobile, desktop, and handheld systems.
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Deep Ultraviolet Observation System for Microscope
U-UVF248
Model Capable of High-magnification/High-contrast Deep Ultraviolet (DUV) Observation. A Semiconductor / FPD Inspection Microscopes.
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UV Cameras
Solar blind UV cameras are imaging devices optimized to detect ultraviolet light of wavelengths below about 280nm. Such cameras are insensitive against sunlight due to negligible sensitivity to visible and long wavelength UV light. Solar blind UV cameras are used in a series of applications like corona detection, fire detection, combustion analysis, plasma research, testing UV lamps, etc. However, highly sensitive corona detection is the main mass application and these devices are of crucial importance in electric power industry. These imaging devices enable easy detection of degraded insulators of high voltage transmission lines, distributions and substations. They can see the emission of UV light when discharges occur at defect insulators. From design point of view solar blind UV cameras are actually bispectral imaging systems built by combining true UV camera with typical visible camera. These bispectral imaging system generate output image as overlay of typical visible image with UV image of analyzed UV source.
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Pocket UV Radiometer
UV-365
Shenzhen Chuangxin Instruments Co., Ltd.
Detector of many bands optional UV365(λP=365nm)UV310(λP=310nm) UV297(λP=297nm) UV254(λP=254nm)Measure range: 0.1-1.99×105μw/cm2 Measure accuracy: ±5%Automatic switch rangeLow power consumption, automatic shutdownZero stable and high accuracy
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Deep Learning Bundle
Set of Deep Learning inspection libraries optimized for machine vision applicationsPerforms image classification, supervised or unsupervised segmentation and object localizationIncludes EasyClassify, EasySegment and EasyLocateSimple APIIncludes the free Deep Learning Studio application for dataset creation, training and evaluationSupports data augmentation and masksCompatible with CPU and GPU processing
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UV & Visible SHG Cavity
SolsTiS ECD-X
The external cavity doubler SolsTiS ECD-X is an extension for SolsTiS. It extends the range of output wavelengths via frequency doubling in a resonant cavity with optimised conversion efficiency to generate high power output from 350-525 nm with a suite of crystals and a single optics set. Automatic, stable lock to SolsTiS is achieved with Hansch-Couillard locking. ECD-X automatically follows SolsTiS frequency scans to deliver >40 GHz of mode hope free tuning across the doubled wavelengths.
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Deep Submersible Particle Size Analyzer
LISST-Deep
The LISST-DEEP instrument obtains in-situmeasurements of particle size distribution,optical transmission, and the opticalvolume scattering function (VSF). Using ared 670nm diode laser and a customsilicon detector, small-angle scatteringfrom suspended particles is sensed at 32specific log-spaced angle ranges. Thismeasurement is post-processed to obtainsediment size distribution, volumeconcentration, optical transmission, andVSF. The electronics and opticalconfiguration in the LISST-DEEP are verysimilar to Sequoia’s workhorse, the LISST-100X. However, because of the extremedifficulty associated with keepingalignment under high pressure, the LISSTDEEPhardware design is radically differentfrom the LISST-100X. This allows theLISST-DEEP to be deployed down to 3000m and obtain reliable measurements ofthe in situ particle size distribution andvolume concentration in waters withoptical transmission up to 98.5%.
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Deep Water Multibeam Echosounders
Deep Water Multibeam Echosounders by Teledyne Marine RESON
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UV Meters
OAI’s UV Measurement Instrumentation are the standard for Semiconductor Lithography, MEMS, Sensors, Microfluidics, UV Curing, 3-D Printing, Sterilization, Water Purification and Solar/PVC industries. For over 45 years our meters have earned a reputation for accuracy, repeatability and dependability. We offer full calibration and support services worldwide.
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UV Sensors
With analog (4-20mA, 0-5V, 0-10V) or digital (USB, Modbus) output, also available with Android device (incl. app). SiC photodiode chip based Broadband UV sensitivity or filtered for UVA, UVB, UVC or UV-Index spectral sensitivity. Our sensors are also available with logarithmic signal transduction, linearity from 0 … 1500 mV. Calibration services available at our Berlin facility prior to delivery and after use
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Multibeam Echosounder - Deep Water
SeaBat 7160
The SeaBat 7160 transducer array is comprised of linear receive and transmit arrays mounted together on a support base. The T-shaped array geometry provides the basis for a compact, high-resolution sonar which is easily installed for portable or hull mounts – a first for a high-resolution system in this frequency range. The system features a pitch-stabilized transmitter and an active roll compensated receiver.
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Rack Extender Kit, G12, 2.5" Deep
310113548
The Rack Mount Extender Block Kit is used for mounting to racks with recessed mounting rails recessed more than 1”. It is made of aluminum with a black anodized finish. NOTE: Used only with slide mounted G12 Receivers.