The ultraviolet UV spectrum encompasses wavelengths from 10nm to 400nm, known as extreme UV, vacuum UV, far, middle and near UV.
Teledyne Imaging offers extensive detector technology to serve applications in the UV spectrum. With our combined expertise and technical capabilities, Teledyne Imaging can offer solutions for even the most challenging applications combining single detector packages to sense in both UV and visible wavelengths through superior optimisation techniques including specialist coatings and spectral filters.
Notable space missions that have been enabled by Teledyne Imaging that operate in the UV or include UV wavelength sensing include the World Space Observatory – Ultraviolet (Roscosmos), GOES-16 (NASA), Meteosat Third Generation (EUMETSAT) and Sentinel-5 (ESA / Copernicus).
Resolution: 1024 × 1024 Pixel size: 13 µm Back illumination technology and extremely low noise amplifiers
Resolution: 720 × 1152 Pixel size: 22.5 µm Full-frame imaging device with two image area sections that can be clocked separately
Resolution: 16 × 16 Pixel size: 16 µm
Resolution: 4096 × 4112 Pixel size: 15 µm Exceptional sensitivity with minimum readout times
Resolution: 4096 × 4112 Pixel size: 15 µm SiC-Flexi or ceramic-PGA
Resolution: 6144 × 6160 Pixel size: 15 µm Four separately connected image area sections to allow full-frame, frame transfer, split full-frame or split frame-transfer modes
Resolution: 6144 × 6160 Pixel size: 10 µm Back-illuminated spectral response and very low read-out noise give exceptional sensitivity.
Resolution: 80 × 80 Pixel size: 24 µm
Resolution: 80 × 80 Pixel size: 24 µm Optimised for use at high frame rates
Resolution: 1024 × 127 Pixel size: 26 µm
Resolution: 2048 × 2048 Pixel size: 13.5 µm Well suited to the most demanding applications requiring a high dynamic range.
Resolution: 2048 × 4612 Pixel size: 13.5 µm Well suited to the most demanding astronomical and scientific imaging applications.
Resolution: 512 × 512 Pixel size: 16 µm Well suited for scientific imaging where the illumination is limited.
Resolution: 1056 × 1027 Pixel size: 13 µm Full-frame architecture well suited to the most demanding scientific applications.
Resolution: 2048 × 2048 Pixel size: 13.5 µm
Resolution: 2048 × 2064 Pixel size: 15 µm Back Illuminated Scientific CCD Sensor
Resolution: 2048 × 1024 Pixel size: 13.5 µm CCD Sensor with full frame architecture, back illumination technology, and an extremely low noise amplifier. Well suited to the most demanding applications such as astronomy.
Resolution: 2051 × 4096 Pixel size: 15 µm Full frame imaging CCD designed to operate in Inverted Mode for low dark signal.
Resolution: 4096 × 4096 Pixel size: 12 µm Large image area with back-illuminated spectral response and very low read-out noise. Designed for demanding astronomical applications.
Resolution: 512 × 580 Pixel size: 16 µm
Resolution: 4096 × 3112 Pixel size: 12 µm Designed for the World Space Observatory Ultraviolet Spectrographs (WUVS) instrument, Teledyne e2v is supplying the CCD and the assembled cryo-cooled UV detector subsystems.
Resolution: 1404 × 1350 Pixel size: 20 × 30 µm CCD sensor with a graded anti-reflective coating unique to Teledyne e2v
Resolution: 1404 × 1350 Pixel size: 20 × 30 µm CCD image senor optimized for ultraviolet and visible wavelengths
Resolution: 384 × 288 Pixel size: 22 µm Inverted mode X-Ray to NIR sensor primarily intended to suit the requirements of astronomy and scientific measuring instruments.
Resolution: 264 × 2048 Pixel size: 15 µm Full frame spectroscopic format sensor
Resolution: 16000 × 4 Pixel size: 5 µm Very high resolution CMOS time delay integration (TDI) image sensors with CCD on CMOS architecture designed for space satellite Earth observation (EO) applications.
Resolution: 1280 × 1024 Pixel size: 5.3 µm 1.3 Mpixels B&W and Color CMOS Image Sensor
Resolution: 1280 × 1024 Pixel size: 5.3 µm 1.3 Mpixels B&W and Color CMOS Image Sensor
Resolution: 244 × 488 Pixel size: 70 µm space qualified CMOS image sensors, with unparalleled performance in terms of sensitivity, radiation tolerance and low power consumption.
