It is also ideal for dense multi-fiber hyperspectral applications. Marana 4.2B-11: This large field of view option utilizes a unique Anti-Glow Technology approach that enables one to usefully access the entire 2048 x 2048 array, offering an impressive 32mm sensor diagonal, which in combination with fast frame rates up to 24 fps (16-bit) and 48 fps (12-bit), renders the camera ideal for large sky scanning astronomy applications such as orbital debris tracking and Near Earth Asteroid detection. Furthermore, to achieve best-in-class quantification accuracy, Andor have implemented enhanced on-head intelligence to deliver market-leading linearity of > 99.7% across the whole dynamic range, ideal for accurate photometry. The innovative ‘dual-amplifier’ approach to extended dynamic range is ideal for accurately visualizing and quantifying challenging scenes that have both extremely weak and bright regions, such as solar measurements and spectroscopic materials characterisations. Higher sensitivity also means that exposure times can be shortened, facilitating faster frame rate measurements of dynamic processes.Ĭrucially, Marana sCMOS reads out 4.2 Megapixel high resolution arrays in less than 50 milliseconds, while maintaining very low read noise hundreds of times faster than a similar resolution CCD detector.
Andor’s unique capability to deliver the ultimate in sCMOS sensitivity means Signal to Noise can be optimized under light starved conditions, ideal for tracking smaller orbital objects, spectroscopic detection of trace concentrations and BEC fluorescence detection of discrete numbers of atoms/ions. Both Marana models feature 4.2 Megapixel sensors, 95% Quantum Efficiency (QE) and market-leading vacuum cooling to -45 ☌, making Marana the most sensitive back-illuminated sCMOS platform available. Marana is Andor’s latest high performance sCMOS camera platform, ideal for diverse applications within the physical sciences such as astronomy, Bose Einstein Condensation, quantum optics, hyperspectral imaging, neutron tomography and fast spectroscopy.
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