16.8 Megapixel back-illuminated CCDs (e2v).TE cooling to -100 ☌ - NO liquid nitrogen or cryo-cooling.18-bit Extended Dynamic Range technology Key Applications: Wide field spectroscopic survey, Deep space observation, Exoplanet detection & Radial velocimetry, Large sky surveys and NEO detection.26 - 515 full frames per second Key Applications: Wavefront sensors, High time resolution astrophysics, Speckle imaging and Transit surveys.ĮMCCDs for Fast Time Resolution Featuring single photon sensitivity, TE cooling to -100 ☌ and >95% QE, the iXon EMCCD range has been central to many demanding observing initiatives, such as the RAVEN ‘Multi-Object Adaptive Optics’ system at the Subaru Telescope (Hawaii), CHIMERA, the Caltech high speed multi-color camera for detecting transiting objects in the Kuiper Belt and SOFIA (pictured).We are currently developing a next-generation, very large area sCMOS camera – enquire for further details! SCMOS for Fast Time Resolution Scientific CMOS (sCMOS) technology is especially relevant for fast time resolution astronomy, combining high resolution / large field of view coverage of the sky with very fast time resolution, yet without sacrificing ultra-low noise performance. ![]() ![]() Rapid frame rates up to 100 fps (full frame).
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