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QHYCCD QHY533C Color

by QHYCCD
SKU QHY-110101
Original price CA$1,343.00 - Original price CA$1,343.00
Original price
CA$1,343.00
CA$1,343.00 - CA$1,343.00
Current price CA$1,343.00
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  • 9 Megapixel Sony IMX533 Back-Side Illuminated (BSI) Color Sensor
  • 1-inch square format with 3.76µm pixels
  • 14-bit A/D conversion for deep dynamic range
  • High 58ke- full well capacity
  • Ultra-low 1.3e- read noise
  • Regulated two-stage cooling to -35°C below ambient
  • 1GB DDR3 image buffer to prevent dropped frames
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  • Description
  • FAQ
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  • QHYCCD QHY533C Color CMOS Camera

    The QHYCCD QHY533C combines the 9 Megapixel Sony IMX533 square sensor with a 14-bit A/D converter to capture deep-sky objects with exceptional dynamic range. Its 3.76µm back-illuminated pixels and extremely low 1.3e- read noise resolve fine detail in galaxies and nebulae. A deep full well capacity of 58ke- prevents stars from saturating, while the two-stage TEC cooler reaches -35°C below ambient to reduce thermal noise to just 0.0005e-/pixel/sec.

    Sony IMX533 BSI Sensor: 9MP at 3.76µm

    At the core of the QHY533C is Sony's 1-inch format IMX533 sensor, a popular choice for its square aspect ratio that eliminates the need for image rotation when framing targets. With 9 Megapixels and a pixel size of 3.76µm, this camera achieves excellent resolution with short-to-medium focal length refractors and astrographs. The back-side illuminated (BSI) architecture maximizes quantum efficiency for capturing faint signal with every exposure.

    14-bit ADC and a 58ke- Full Well

    The QHY533C digitizes images with a 14-bit Analog-to-Digital converter, providing over 16,000 levels of gray to distinguish subtle tonal variations in nebulosity. This is paired with a very large full well capacity of 58,000 electrons (58ke-), allowing you to take longer sub-exposures without clipping the bright cores of objects like the Orion Nebula (M42) or the Andromeda Galaxy (M31). This combination ensures you retain color and detail in both the brightest and dimmest parts of your target.

    1.3e- Read Noise and Zero Amp Glow

    For deep-sky imagers, low noise is critical. The QHY533C delivers exceptionally clean data with read noise as low as 1.3 electrons at high gain settings. Furthermore, QHY's implementation provides nearly zero amplifier glow, a common source of noise on long exposures that can be difficult to remove with calibration frames. This clean signal foundation means your final stacked image has a smoother background and reveals more faint detail.

    -35°C Cooling and 1GB DDR3 Buffer

    A regulated, two-stage thermoelectric cooler aggressively combats thermal noise by chilling the sensor to a stable -35°C below the ambient temperature. This consistency is vital for creating an accurate dark frame library. For high-speed planetary or lunar imaging, the camera can capture full-resolution 16-bit frames at 20 FPS, with an onboard 1GB DDR3 buffer that ensures no frames are dropped during transfer over its USB 3.0 interface.

    QHY533C vs. QHY533M: Color Simplicity and 17mm Back Focus

    The QHY533 series comes in both color (QHY533C) and monochrome (QHY533M) versions. The primary difference is the imaging workflow and mechanical interface.

    • QHY533C (Color): Ideal for users who want a streamlined imaging process. You capture full-color images in a single shot, without the need for filters or a filter wheel. It features a standard 17mm back focal distance.
    • QHY533M (Monochrome): Offers higher sensitivity and the flexibility to shoot through LRGB and narrowband filters for advanced imaging. It is designed with a shorter 14mm back focal distance for direct, rigid integration with QHY's filter wheels.

    The QHY533C is the clear choice for astronomers seeking deep-sky imaging capability without the added complexity and cost of a monochrome filter-based system.

  • What is the advantage of the QHY533C's 1-inch square sensor?

    The 1-inch square sensor (3008 x 3028 pixels) is a significant benefit for framing. Unlike rectangular sensors, you never have to rotate the camera to fit a target like the Hercules Cluster (M13) or a round galaxy. The field of view is consistent regardless of orientation, simplifying your setup.

    How does the QHY533C's 58ke- full well help with my images?

    A high full well capacity of 58,000 electrons (58ke-) allows the pixels to collect more light before becoming saturated (turning pure white). This gives you greater dynamic range, allowing you to capture faint nebulosity around bright stars without blowing out the star cores. It's especially useful for targets with a high contrast range, like the Trapezium region within the Orion Nebula (M42).

    Is the QHY533C a good camera for imaging Jupiter with a Celestron 8" SCT?

    Yes, the QHY533C is an excellent planetary camera. When used with an 8" f/10 SCT, you can use a region of interest (ROI) to achieve very high frame rates. For example, at a 480-line resolution, it can capture up to 152 FPS in 8-bit mode. This high speed allows you to "freeze" atmospheric seeing and produce sharp, detailed images of Jupiter's cloud bands and the Great Red Spot.

    What does "zero amplifier glow" mean for long exposures with the QHY533C?

    Amplifier glow is a faint illumination, usually in the corners of an image, caused by the sensor's electronics during readout. The QHY533C is engineered to have nearly zero amplifier glow, which means your raw long-exposure images have a much cleaner, more uniform background. This makes calibration with dark frames more accurate and simplifies your processing workflow.

    With a 17mm back focus, how do I connect a filter drawer to the QHY533C?

    The 17mm back focus is a standard distance that works well with most imaging accessories. To add a filter drawer (typically 20mm thick) and an off-axis guider (typically 10-12mm thick), you will use a combination of M42 or M48 extension rings to achieve the standard 55mm back focus required by most flatteners and correctors.

    Can the QHY533C capture the entire Andromeda Galaxy (M31) with a RedCat 51 telescope?

    A RedCat 51 has a 250mm focal length. The QHY533C's 1-inch sensor (11.31mm x 11.38mm) on this telescope would yield a field of view of approximately 2.59° x 2.61°. Since the Andromeda Galaxy (M31) is about 3° wide, you would capture the bright core and a significant portion of the spiral arms, but you would likely clip the very faint outer edges. It's a great match for framing the core and prominent dust lanes in high resolution.

  • Sensor SONY IMX533 BSI CMOS (Color)
    Effective Pixels 9 Megapixels
    Sensor Size 1-inch Format
    Pixel Size 3.76µm x 3.76µm
    Full Well Capacity 58,000 e-
    A/D Converter 14-bit
    Readout Noise 1.3e- to 3.4e-
    Dark Current 0.0005 e-/pixel/sec @ -20°C
    Exposure Range 30µs to 3600s
    Frame Rate (Full Res) 20 FPS @ 16bit / 26.5 FPS @ 8bit
    Frame Rate (Max ROI) 215 FPS @ 16bit / 280 FPS @ 8bit (240 lines)
    Image Buffer 1GB DDR3 Memory
    Shutter Type Electronic Rolling Shutter
    Amp Glow Control Nearly Zero Amplifier Glow
    Cooling System 2-Stage TEC, -35°C below ambient
    Anti-Dew Heater Yes
    Optical Window AR+AR Coated
    Computer Interface USB 3.0
    Telescope Interface M42 x 0.75 (female)
    Back Focal Length 17mm (±0.2mm)
    Weight 845g
  • QHYCCD Warranty