Showing results: 1 - 15 of 20 items found.
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Thales SESO, SAS
For more than 40 years, Thales has delivered high accuracy optics for ground-based Astronomy all around the world. These optics range from single, but challenging, unmounted optical components up to fully integrated opto-mechanical systems. Our design heritage and past experience in this field cover the design, manufacture and AIT activities of many optics and sub-assemblies used in Telescope instrumentation, such as focal plane assemblies as well as the direct production of telescope mirrors themselves. Several major achievements of Thales ground-based Astronomy products were the Optical wide field corrector for the Dark Energy Survey (lien), the Reference Body for future Deformable Secondary Mirror of the VLT (lien) and different challenging spectrograph optics (Collimator and Cameras) for different Observatories (lien). One advantage Thales has with this activity is that most part of the manufacturing steps involved (i.e. opto-mechanical design, milling/grinding, lightening, polishing and coating) are directly under our control in our own facility. Our current capabilities for the production of optics for ground-based Astronomy are from a few centimeters size up to 2 meters. Thanks to the continuous efforts in R& D and investments into new production machines, Thales is now ready for future industrial challenges including the optical production of some key elements of the E-ELT, GMT and TMT programs.
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HORIBA, Ltd.
HORIBA Scientific proposes large size Transmission Holographic Fused Silica Etched (FSE) gratings or Ruled blazed reflection gratings for Astronomy.Both technologies offer a very high efficiency, low polarization dependence and low angular sensitivity.
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COSMOS™ -
Teledyne Princeton Instruments
The COSMOS™ is the only large format, high performance CMOS camera designed and manufactured entirely within a single source. With LACera™ technology, the COSMOS offers superior sensitivity, large imaging area, low noise and fast frame rate.
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Teledyne e2v
EM (Electron Multiplication) is a technology that uses on-chip gain in the charge domain to effectively eliminate read noise from an image sensor. This enables advanced ultra-low light applications that require extreme sensitivity at fast frame rates such as adaptive optics and lucky imaging™.The combination of Teledyne e2v’s back-thinning technology and anti-reflection coatings enables industry leading quantum efficiency that can be optimised for applications in the visible, UV or NIR wavelength ranges.
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Teledyne e2v
(CCDs) for Space science, Ground-based Astronomy, and Earth observation applications with an impressive record of successful deliveries to a wide range of customers over 40 years.All Teledyne e2v devices can be supplied partially or fully customised to fit the application and achieve the best possible system performance. CCD image sensor design, manufacture, test and characterisation are carried out in-house enabling control from start to finish. Multi-polysilicon, multi-metal and back-illumination options are available for high resolution, high sensitivity and very low noise.
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PI-3105 -
Pulse Instruments
This highly flexible system is designed to test a wide variety of imaging devices, from low-noise astronomy and medical devices, to military and machine-vision devices with GB/sec data rates.
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KURO® -
Teledyne Princeton Instruments
The KURO® is the first back-illuminated scientific CMOS camera. With high sensitivity and fast frame rates the KURO is optimal for applications such as hyperspectral imaging, astronomy, cold-atom imaging, quantum imaging, fluorescence spectroscopy, and high-speed spectroscopy
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Teledyne Lincoln Microwave
Teledyne Lincoln Microwave designs our own proprietary microwave diodes, which underpin many of our performance advantages.Our Semiconductor Technology Centre is located at the School of Physics and Astronomy within the University of Nottingham, UK. Facilities include a 90m2 ISO class 6 process cleanroom with ISO class 5 laminar flow.
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HORIBA, Ltd.
HORIBA Scientific’s diffraction gratings are found in cutting-edge scientific applications including ultrafast and highenergy lasers, space flight instruments, astronomy, and synchrotron spectrometers.HORIBA’s scientific gratings are either masters or replicas, depending on the application. HORIBA Scientific also produces custom diffraction gratings, which can be specified according to our customers’ unique technical requirements.
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Teledyne e2v
Our front and backside illuminated (BSI) and backthinned Charge Coupled Devices (CCDs) are seen as the gold standard for scientific and quantum imaging in applications in spectroscopy, microscopy, In vivo, x-ray and astronomy. We understand that every imaging application is unique and requires our engineers and scientists to work closely with our customers providing highly tailored imaging solutions.
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2100 -
Valon Technology, LLC
1440MHz inputLow noise figure LNA 0.3dB 20 KHigh gain >40dB8-pole ceramic dielectric input filterHigh dynamic range, low-spurious responses Rugged milled aluminum housingRFI shielded constructionDesigned for use with Valon 5009 as LOSuitable for hydrogen line observation and general radio astronomy in the 21cm band.6Vdc @ 400mAIncludes 20” dc power supply cable
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Teledyne e2v
Our backside illuminated (BSI) and backthinned Charge Coupled Devices (CCDs) and front and back illuminated CMOS image sensors (CIS) are seen as the gold standard for scientific and quantum imaging in applications in spectroscopy, microscopy, in vivo, x-ray and astronomy. We understand that every imaging application is unique and requires our engineers and scientists to work closely with our customers providing highly tailored imaging solutions.
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CryoTel® -
Sunpower Inc.
With Sunpower’s reputation for quality and performance, the CryoTel® family of cryocoolers is increasingly used in the medical, instrumentation, security, astronomy, telecommunications, and pharmaceuticals markets. Sunpower’s cryocoolers integrate with and support technologies such as high-temperature superconductivity, radiation detection, optics, CCD, LNA, gas liquefaction, and more. The CryoTel® cryocoolers provide cost advantages during product development and during volume production. Our customers also benefit from the unsurpassed reliability, efficiency, and power density of our superior cryocooler technology.
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Teledyne e2v
Teledyne e2v has been trusted to design and deliver CCD and CMOS imaging sensors and sub-systems for over 150 space missions by the world's largest space agencies, including NASA, ESA, JAXA, CNSA and most recently for the Russian-led World Space Observatory.We offer space imaging solutions, including space qualified imaging sensors, arrays and sub-systems for space science, ground astronomy and Earth observation; helping solve the mysteries of the Universe and understand climate change on Earth.
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CH1-1007 -
VREMYA-CH JS Company
Hydrogen frequency and time standard Ch1-1007 is designed to generate and reproduce precision, highly stable, spectrally pure frequency and time signals. Main areas of application: – in metrology when transferring the sizes of units of frequency and time, including as part of mobile measuring complexes; – in radio astronomy when conducting scientific research; - in radio navigation when working as part of automated measuring systems and complexes.
