High-resolution APS-C sensor: SC571CC CMOS Telescope Camera features the IMX571 APS-C BSI sensor with a 23.4×15.7mm area and 26MP resolution; Its 3.76 µm pixels and efficient BSI design capture sharp stars and faint nebulae with clean deep-sky data
Heat the Glass, Clear imaging: Safeguard your imaging sessions from dew and moisture with SC571CC's front-window heater; the heater is seamlessly integrated for software control; with theoption to activate Heating/Defog' directly; safeguard image quality and maximize your productive imaging time
Dual-stage TEC cooling: APS-C Format Camera lowers the sensor temperature by 35°C below ambient (ΔT = -35°C); reducing dark current and noise. Its all-metal heat-dissipation design ensures stability for long deep-sky exposure
Wide telescope compatibility: SVBONY SC571CC Cooled Camera is compatible with APO; Newtonian; RC; and catadioptric scopes; offering image circle and sharp detail at medium-to-long focal lengths
16-bit wide dynamic range: APS-C Camera features a 16-bit ADC; delivering up to 14 stops of dynamic range; It produces smoother tonal transitions; preserves faint details; ensuring ideal deep-sky images
Zero Amp-Glow: Astro Camera features a Zero Amp-Glow sensor for clean dark frames during long exposures; Optimized circuits reduce noise stripes; ensuring pure image quality; Ideal for capturing faint nebulae; Ha regions; and molecular clouds
Stable USB 3.0 connection: equipped with USB 3.0; SC571CC astronomical camera ensures fast and reliable data transfer without frame drops or interruptions; even when connecting multiple devices or running long deep-sky imaging sessions
High QE (>80%) for faint targets: SVBONY SC571CC features a back-illuminated sensor with large pixels to enhance photon efficiency; capturing faint nebulae and Ha regions with clean; detailed deep-sky images—even under light-polluted skies
512 MB DDR3 buffer for stable transfer: the IMX571 Camera's USB 3.0 interface with 512 MB DDR3 memory reduces frame drops and interruptions when multiple devices are connected; ensuring smooth all-night imaging sequences
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