UV and Visible Spectrometers - High-sensitivity Fiber-optic Spectrometer -- AvaSpec-HS1024x122TEC-USB2Supplier: Avantes
Description: 1392 µm high and for the AvaSpec-HS1024x12TEC2 they measure 2928 µm high. The instrument’s optical bench design is based on a revolutionary concept with high numerical (0.22) aperture and throughput. TE-cooled backthinned CCD detectors are used as a linear array of 1024 pixels
- Photometric System Design: Non-Scanning Array-Detector
- Detector Type: Other Detector
- Wavelength Range: 200 to 1100 nm
- Spectral Resolution: 1.2 nm
Description: (see table) Stray light 0.04-0.1%, depending on the grating Sensitivity 160,000 counts/µW per ms integration time Detector CCD linear array, 3648 pixels Signal/Noise 350:1 AD converter 16 bit, 1 MHz Integration time 10 µs - 10 minutes Interface USB 2.0 high speed, 480 Mbps RS-232
- Photometric System Design: Scanning Single Beam
- Detector Type: Charge Coupled Device (CCD)
- Wavelength Range: 200 to 1100 nm
- Display Options: None
Supplier: HORIBA Scientific
Description: HORIBA Scientific supplies a complete range of OEM imaging miniature spectrographs optimized for use with CCD and Photodiode array detectors to operate from the UV through to the IR. These mini spectrometer units are available in a variety of focal lengths and resolutions and incorporate aberration
Supplier: Excelitas Technologies Corp.
Description: Excelitas’ P-series linear imager combines the best features of high-sensitivity photodiode array detection and high speed, charge-coupled scanning to ofer an uncompromising solution to the increasing demands of advanced imaging applications. Tese high-performance imagers feature low noise
- Array Type: Linear Array
- Horizontal Pixels: 4096
- Pixel Size: 14 µm
- Spectral Response: 200 to 1000 nm
Supplier: HORIBA Scientific
Description: Type IV aberration corrected flat field & imaging gratings are designed to focus a spectrum onto a plane surface, making them ideal for use with linear or 2-D array detectors. These gratings are produced with grooves that are neither equispaced nor parallel, and are computer optimized to form
- Grating Type: Ruled Grating
- Grating Design: Spherical Reflection
- Ion Etched: Yes
- Wavelength Range: UV, Visible, IR
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Spectroscopic Diagnostics of an Atmospheric Microwave Plasma
StellarNet 1024 and 2048 uv enhanced ccd linear arrays Pixel width .
Development and characterization of a broad-bandwidth polarization-insensitive
subwavelength optical device
There are a few defects in this array. . a 2048-element linear array UV –visible CCD spectrometer (BWTek, BRC111A) at far field.
All�?epitaxial fabrication of a nanowire plasmon laser structure
The uncorrected photoluminescence spectra were acquired with a fiber optical spectrometer, which is fitted with an UV -extended linear CCD array and a grating blazed at 350 nm, coupled to a near-UV transmitting optical microscope.
Determination of silver in geological samples using high-resolution continuum source electrothermal atomic absorption spectrometry and direct solid sampling
The system is equipped with a high pressure Xe short-arc lamp operating in hot spot mode, with a nominal power of 300 W, and a UV -sensitive linear CCD array detector with 512 pixels.
High-resolution continuum-source atomic absorption spectrometry: what can we expect?. J. Braz. Chem. Soc., Apr 2003, vol.14, no.2, p.220-229. ISSN 0103-5053
An L 172 UV -sensitive linear CCD array detector with 512 pixels, 23 mm x 480 mm (WF, Berlin, Germany) was used, resulting in an instrumental bandwidth of 1.8 pm / pixel at 200 nm (with a slit width of 23...
CYCLOPE remote sensing: a multipurpose optronic payload and the associated subsystem
silicon CCD linear array Spectral band : UV : 0.35 to 0.45 p.m - Visible : 0.4 to 0.7 p.m Typical sensitivity : detection ofa 14 mW/m2/sr source Angular resolution : 3 mid .
Low Stray Light CCD Spectrometer: Quest™ U
The Quest™ U is a linear CCD array spectrometer optimized for UV performance using a low straylight optical bench.
Hybrid native phosphorescence and fluorescence spectroscopy for cancer detection
The collection fiber was coupled to a UV sensitive spectrophotometer with a linear CCD array (Ocean Optics model USB2000, Dunedin, FL).
Study on the test of transient ultraviolet spectrum for remote extended area sources with spectrometer
CCD detector adopts high-sensitivity UV -enhanced linear CCD photosensitive element arrays , of which pixel number is 1024 and pixel size is 25μm.
Authentication and Discrimination of Whiskies of High Commercial Value by Pattern Recognition
UV–Vis spectral measurements were taken using an Ocean Optics Model CHEMUSB4000 UV –Vis spectrophotometer with a linear CCD array detector (Duiven, The Netherlands).
Solar Occultation Measurements of the Martian Atmosphere on the Phobos Spacecraft: Water Vapor Profile, Aerosol Parameters, and Other Results
The corresponding signals were fiber-fed to the Fabry–Perot interferometer with the resolving pwer of λ/∆λ ≈ 1.5 × 105.A Reticon CCD lin- ear array , identical to that employed in the UV channel, was used as a detector, but only...
A TL/OSL emission spectrometer extension of the Risø reader.
The light is measured with a high sensitivity 2048-element CCD - linear array detector (Avantes PC2000) sensitive in the UV -VIS region.
High Speed Back-thinned CCD Spectrometer With Excellent UV/NIR Sensitivity
The detector has superior response over standard CCDs in the UV and NIR ranges and the linear array of 2048 pixels is suitable for higher speed triggering.
Visible�?to�?UV/Violet Upconversion Dynamics in Er 3+ �?Doped Oxyfluoride Nanoscale Glass Ceramics
These spectra were collected by a spectrometer (ANDOR Shamrock) equipped with an UV –visible CCD camera (Newton CCD) and a NIR linear array (Idus InGaAs).
The Cabauw Intercomparison campaign for Nitrogen Dioxide measuring Instruments (CINDI): design, execution, and early results
The CCD detector is a Sony 2048 linear array with a Deep- UV coating for signal enhancement below 350 nm, 40 pho- tons per count sensitivity at 600 nm and a signal-to-noise ra- tio of 200.