The Zyla is available with two front-illuminated sensor formats: 5,5 Megapixel and 4,2 Megapixel with pixel sizes of 6,5 µm.
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The Zyla sCMOS cameras, with read noise of only 0,9 electrons, can provide 100 fps (via CameraLink connectivity) at full frame (higher frame rates possible by using ROIs). Furthermore, it offers rolling as well as global shutter mode (“snapshot mode”) and frame rates of up to 100 fps at full frame. The Neo 5.5 low-noise sCMOS camera is based on a front-illuminated sensor with 5,5 MP and a pixel size of 6,5 µm.The Neo is a unique –40☌ vacuum cooled platform, which allows to reach extremely low dark noise levels of ~0,007 e-/pix/s. One of the sensor options also features UV opimization with high sensitivities in the wavelength range between 250-400 nm. This camera model is available with sensors of 11 µm and 6,5 µm pixel size. The Marana utilizes back-illuminated sCMOS sensors with 4,2 Megapixels and a quantum efficiency of up to 95%. The Balor sCMOS has a read out rate of 18.5ms, offering 54 fps at full frame and read noise of <3 electrons. Balor - Andor’s game-changing, very large area sCMOS camera for Astronomyīalor features an enhanced FoV 16.9 Megapixel, 70mm diagonal front-illuminated sensor, coupled with high speed and low read noise capability. In addition, the sensors of the Balor, Marana and Neo can be cooled down to -30☌, -45☌ or -40☌, thanks to the vacuum sensor enclosure technology.įurthermore, Andor’s Balor, Zyla 5.5 and Neo 5.5 cameras allow to select rolling as well as global shutter modes, whereas global shutter is similar to a ‘snapshot mode’. In contrast to previous CMOS or CCD technologies, these cameras offer maximum sensitivity, resolution, speed, and field of view at the same time. The Balor, Marana, Neo and Zyla sCMOS cameras are specifically designed to provide the highest level of sensitivity (i.e., front and back-illuminated sensors). Because of their special characteristics - extremely low read noise and fast frame rates - they are ideal camera solutions for various applications in physics and astronomy.
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