SVBONY SV605CC IMX533 Cooled Colour Astronomy Camera
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The SVBONY SV605CC colour astronomy camera, powered by the Sony IMX533 sensor, delivers outstanding performance for deep-sky astrophotography. With low read noise, high quantum efficiency, and a square sensor format, it is ideal for capturing detailed images of nebulae, galaxies, and star clusters.
Sony IMX533 Sensor Performance
The IMX533 sensor provides excellent sensitivity with low noise characteristics, making it highly effective for long-exposure imaging. Its square format ensures balanced framing and efficient use of the image circle.
Low Read Noise with HCG Mode
The SV605CC features High Conversion Gain (HCG) mode, significantly reducing read noise while maintaining dynamic range. This results in cleaner images with improved signal-to-noise ratio.
2-Stage TEC Cooling System
The advanced two-stage TEC cooling system can reduce the sensor temperature by up to 30°C below ambient, dramatically lowering thermal noise and enabling long exposure imaging sessions.
DDR3 256MB Buffer
The integrated DDR3 buffer ensures stable data transmission and reduces the risk of dropped frames during long imaging sessions.
Broad Software Compatibility
Compatible with major astrophotography software platforms, the SV605CC integrates easily into existing imaging workflows on Windows systems.
Flexible ROI & BIN Functions
The ROI (Region of Interest) and binning functions allow for flexible resolution control, improving frame rates and optimising data capture for different targets.
Optimised Mechanical & Optical Design
Featuring a robust CNC-machined aluminium body with AR-coated protective glass, the SV605CC is designed for durability and optimal light transmission.
55mm Back Focus Compatibility
Designed to integrate seamlessly into standard astrophotography setups, the SV605CC supports the common 55mm back focus spacing used with flatteners and reducers.
AR Coating & Build Quality
The AR-coated window improves light transmission, while the anodised aluminium body ensures durability and thermal stability.
Astrophotography Results