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Marana is Andor’s high performance sCMOS camera platform for Astronomy and Physical Sciences, featuring 95% Quantum Efficiency (QE) and market-leading vacuum cooling to -45 °C. The platform offers solutions for large field of view and high-speed imaging/spectroscopy.
Resources:
Features & Benefits:
Up to 95% QE & lowest noise
Maximum signal to noise for light starved measurements. Detect smaller orbital debris; BEC fluorescence.
Vacuum cooled to -45°C
Very weak signals require lowest noise floor and longer exposures: Don’t be restricted by camera thermal noise!
4.2 Megapixel
High pixel resolution, maintaining image clarity over an extended field of view
The ONLY vacuum back-illuminated sCMOS
Andor’s proprietary UltraVac™ technology protects the sensor from (a) QE degradation, and (b) moisture condensation
Extended Dynamic Range (EDR) Mode
‘One snap quantification’ across the full dynamic range – perfect for Photometry.
> 99.7% linearity
Market leading quantitative accuracy over the whole signal range.
Fan and liquid cooling as standard
Liquid cooling for maximum sensitivity.
Adaptive Optics Ready
Minimize lag after data collection – transfer of row data immediately after exposing.
Technical Specifications:
High resolution: 4.2 Megapixel.
High sensitivity: Up to 95% QE .
Fast speeds: Up to 74 fps.
Large field of view: Up to 32 mm.
Deep cooled: -45°C cooling.
Protected: UltraVac.
TM sensor enclosure.
Flexible: 11 μm & 6.5 μm pixel sensors.
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Our team is here to help you! Call us or leave us a message and an Apel Laser consultant will be happy to answer your questions and find personalized solutions for you.
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