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IMPORTANT: Our store is located in Canada. All orders that include products manufactured outside of Canada or USA will be subject to tariffs and duties, regardless of the order value. US customers are responsible for all applicable duties and tariffs, and those will be billed by the carrier, except for the Lacerta upgrade kit, for which we collect them at checkout.

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SVBONY SV605CC Cooled Color OSC Camera IMX533

by SVBONY
SKU SV-F9198K
Original price $471.03 - Original price $471.03
Original price
$471.03
$471.03 - $471.03
Current price $471.03
Price Match Policy!
  • Features a 9.0 Megapixel, 1-inch square format IMX533 color CMOS sensor
  • High-sensitivity 3.76μm pixels with a peak Quantum Efficiency of 91%
  • 2-stage TEC cooling system reduces sensor noise for long-exposure imaging
  • Ultra-low readout noise ranging from 1.0e- to 3.3e-
  • Onboard 256MB DDR3 buffer ensures stable data transfer up to 20 FPS
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  • Description
  • FAQ
  • Specifications
  • In the Box
  • Warranty
  • SVBONY Cooled Color Astronomical Camera SV605CC

    The SVBONY Cooled Color Astronomical Camera SV605CC combines the celebrated 9.0 Megapixel Sony IMX533 square sensor with a powerful 2-stage TEC cooling system. With 3.76μm pixels, a peak QE of 91%, and ultra-low read noise down to 1.0e-, this camera captures deep-sky objects with exceptional detail and dynamic range. A 256MB DDR3 buffer ensures stable, drop-free data transfer at a maximum frame rate of 20 FPS over its USB 3.0 connection, while the 14-bit ADC renders smooth tonal gradations from the brightest stellar cores to the faintest nebulosity.

    IMX533 Sensor: A 9.0MP Square Format with 91% QE

    At the heart of the SV605CC is the 1-inch Sony IMX533 sensor, renowned for its complete absence of amp glow. Its 3008x3008 pixel square format simplifies framing and mosaic planning, eliminating the need to rotate the camera to fit targets like the Hercules Cluster (M13). The 3.76μm pixels offer a high-resolution sampling for a wide range of telescopes, while the back-illuminated architecture delivers a peak Quantum Efficiency of 91%, capturing faint signal with remarkable speed.

    2-Stage TEC Cooling for Ultra-Low Noise Imaging

    Deep-sky astrophotography relies on minimizing thermal noise during long exposures. The SV605CC's 2-stage thermoelectric cooling system actively reduces the sensor's temperature by up to 30°C below ambient. This dramatic cooling drastically cuts dark current, resulting in cleaner, higher-contrast images. Paired with a readout noise as low as 1.0e- and a deep 50ke- full well capacity, the camera preserves faint details in nebulae and galaxies without being overwhelmed by noise.

    256MB DDR3 Buffer and Broad OS Support

    To prevent dropped frames and data corruption during transfer, the SV605CC includes a 256MB DDR3 memory buffer. This cache ensures stable communication between the camera and your computer, even on less powerful systems, providing a reliable imaging experience at the maximum 20 FPS frame rate. The camera offers extensive compatibility, with stable drivers for Windows, Linux, Mac OS, and even Raspberry Pi, working seamlessly with popular acquisition software like SharpCap and N.I.N.A.

    SVBONY SV605CC vs. ZWO ASI533MC Pro: A Head-to-Head Comparison

    Both the SV605CC and the ZWO ASI533MC Pro are built around the same exceptional 9.0MP IMX533 sensor, offering identical resolution, pixel size, and 14-bit ADC.

    • Cooling: The ASI533MC Pro often specifies a slightly greater cooling delta of 35°C below ambient, compared to the SV605CC's 30°C. In practice, both provide the crucial noise reduction needed for serious deep-sky imaging.
    • Core Hardware: Both cameras feature a 256MB DDR3 buffer for stable data transfer and produce images with zero amp glow, making them functionally very similar for capturing raw data.
    • Ecosystem & Compatibility: The SV605CC stands out with its explicitly broad OS support, including Chrome OS and Raspberry Pi, making it a flexible choice for various setups. ZWO has a deeply established ASCOM and INDI driver ecosystem. Your choice may depend on existing software preferences and budget.
  • What is the advantage of the SVBONY SV605CC's 9.0MP square sensor?

    The 3008x3008 pixel square format of the SV605CC simplifies framing for many deep-sky objects, which are often round or irregular. It eliminates the need to perfectly orient a rectangular sensor, saving time and making it easier to create mosaics. The 9.0 Megapixel resolution provides ample detail for large prints and cropping.

    How does the TEC cooling on the SV605CC improve my deep-sky images?

    The 2-stage TEC cooling system chills the IMX533 sensor, significantly reducing thermal noise (dark current) that builds up during long exposures. This results in much cleaner, higher signal-to-noise ratio images, allowing the faint details of galaxies and nebulae to stand out against a dark background.

    What do the 6.5mm and 17.5mm back focus options on the SV605CC let me do?

    The dual back focus distances provide flexibility for connecting different accessories. The 17.5mm distance is standard for configurations that include a filter wheel or off-axis guider. The shorter 6.5mm distance is useful for setups with coma correctors or reducers that have very specific spacing requirements, allowing you to place the sensor at the optimal focal plane without extra adapters.

    Can I use the SVBONY SV605CC to image the Orion Nebula (M42) with an 8" SCT at f/10?

    Yes, the SV605CC is an excellent choice. The camera's 3.76μm pixels provide good resolution at the long focal length of an f/10 SCT. The high 91% QE will capture the faint outer nebulosity of M42 efficiently, while its 14-bit ADC and 50ke- full well depth will help preserve detail in the bright Trapezium core without saturation, especially when using a series of short exposures.

    Is the SVBONY SV605CC suitable for planetary imaging of Jupiter?

    While the SV605CC is primarily designed for deep-sky imaging, it can be used for planetary work. Its maximum frame rate of 20 FPS is modest compared to dedicated planetary cameras, but using the Region of Interest (ROI) feature to capture a smaller portion of the sensor will increase this rate significantly. This allows you to "freeze" atmospheric seeing and capture detailed images of Jupiter's cloud bands and Saturn's rings.

    What software is compatible with the SVBONY SV605CC?

    The SVBONY SV605CC has broad software compatibility. It works with most popular astrophotography acquisition software, including SharpCap, N.I.N.A., TheSkyX, and AstroDMx Capture. It is supported on multiple operating systems, including Windows, Linux, Mac OS, Raspberry Pi, and Chrome OS.

  • Sensor 1" Color Sony IMX533 CMOS
    Resolution 3008 x 3008 (9.0 MP)
    Pixel Size 3.76μm
    Sensor Diagonal 15.968mm
    Quantum Efficiency (Peak) 91%
    Readout Noise 1.0e- to 3.3e-
    Full Well Capacity 50ke-
    ADC 14-bit
    Shutter Type Rolling Shutter
    Max Frame Rate 20 FPS
    Exposure Range 0.05ms to 2000s
    Onboard Cache 256MB DDR3
    Cooling System 2-Stage TEC, Semiconductor
    Back Focus 6.5mm / 17.5mm
    Data Port USB 3.0 Type-B
    Mechanical Interface 2", 1.25", M42x0.75
    Protective Window AR Coated Optical Glass
    ROI Support Yes
    Pixel Binning 1x1, 2x2, 3x3, 4x4
    Digital Noise Reduction Yes
    Supported OS Windows, Linux, Mac OS, Raspberry Pi, Chrome OS
    Working Current < 300mA
    Stand-by Current < 30mA
  • SVBONY 1-Year Warranty