I will still need to change this.īut still! This camera is a monster. The result is a proof that the mechanical backfocus of my setup is an ever so tiny bit too long (maybe 0.2/0.3 mm). UHC-L subframes are balanced between Blue/Green and Red. Countless subframes needed to be inspected/measured individually for best selection.įWHM weighting of Green and Blue are very similar, w. Fast changing air transparency really was my problem during these nights. This is true "Lucky-imaging"Įach subframe is just signal - no noise at all. RGB and an impeccable camera - what a dream come true. An ideal number of UHC-L frames, balanced w. Such kind of data set rested in my dreams since long.time. Protoplanets made visible in the heart of Orion (Andor Marana w. In case you have further questions, please contact us via kontakt (at) Please note that additional information and spec sheets are available in the “downloads” section. This is in response to requests from companies, institutes and amateur astronomers to integrate these high-quality special cameras into telescope systems and observing stations. Please note: We offer ANDOR cameras exclusively for astronomical applications and satellite tracking. High-Speed Spectroscopy (e.g., Marana and Zyla for Multi-Track and Hyperspectral Imaging)įurther information about Andor’s sCMOS camera solutionss can be found on Andor Technology's website.The Zyla 5.5 offers rolling and true global shutter functionality, whereas the Zyla 4.2+ has rolling shutter only, but provides a higher quantum efficiency of 82% peak QE. 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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#ANDOR SOLIS SPOOL FILE TYOPE FULL#
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.
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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.
#ANDOR SOLIS SPOOL FILE TYOPE SERIES#
View All Adapters & Imaging AccessoriesĪndor Technology’s sCMOS camera series (Balor, Marana, Neo, Zyla)Īndor’s scientific CMOS (sCMOS) cameras represent a breakthrough technology based on next-generation CMOS Image Sensor (CIS) design and fabrication techniques.
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