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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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QHYCCD QHY367CPRO-C Color

by QHYCCD
SKU QHY-110059
Original price $4,399.00 - Original price $4,399.00
Original price
$4,399.00
$4,399.00 - $4,399.00
Current price $4,399.00
Price Match Policy!
  • Effective Pixels: 36MP
  • Sensor Size: Full Frame (36mm x 24mm)
  • Readout Noise: 2.4e- to 3.2e-
  • Cooling System: -45℃ below ambient
  • Built-in Image Buffer: 128MB DDR2
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  • Description
  • FAQ
  • Specifications
  • In the Box
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  • Warranty
  • QHYCCD QHY367CPRO-C Color Cooled CMOS Camera

    The QHYCCD QHY367CPRO-C brings the full-frame 36MP Sony IMX094 sensor to dedicated astrophotography, using its 4.88μm pixels to capture massive fields of view with high resolution. It delivers a true 14-bit output with a deep 56ke- full well capacity, while keeping read noise as low as 2.4e- for clean images. A 128MB DDR2 buffer ensures stable, drop-free data transfer even at the camera's full resolution frame rate of 3.2 FPS.

    Sony IMX094 Sensor: 36MP Full-Frame Imaging at 4.88μm

    At the core of the QHY367CPRO-C is the 36mm x 24mm full-frame Sony IMX094 sensor, renowned for its use in high-end DSLR cameras. With a resolution of 36 megapixels (7376x4938), you can frame enormous celestial targets like the Andromeda Galaxy (M31) or the entire Veil Nebula complex in a single shot with a wide-field refractor. The 4.88µm pixels provide an excellent balance of image scale and sensitivity for a wide range of focal lengths, from short refractors to larger Ritchey-Chrétien telescopes.

    Advanced Noise Control: -45°C Cooling & 2.4e- Read Noise

    QHYCCD's design masters thermal and electronic noise. The dual-stage TEC cooling system achieves a delta of -45°C below ambient, dramatically reducing thermal signal for pristine long exposures. This results in an exceptionally low dark current of just 0.0015e-/pixel/sec at -15°C. The camera's read noise floor of 2.4e- to 3.2e- preserves the faintest wisps of nebulosity, while proprietary hardware control virtually eliminates amplifier glow, a common artifact in uncooled cameras during long exposures.

    Stable Data Transfer: 128MB DDR2 Buffer at 3.2 FPS

    To handle the massive amount of data generated by the 36MP sensor, the QHY367CPRO-C incorporates a 128MB DDR2 image buffer. This onboard memory is critical for preventing dropped frames during high-speed captures, ensuring data integrity from the camera to your computer over the USB3.0 interface. This feature provides a stable imaging platform, which is essential for advanced techniques like lucky imaging or creating large-scale mosaics.

    Mechanical Design: M54 Interface, 17.5mm Back Focus, and Full Dew Control

    Weighing 680g, the QHY367CPRO-C is built for reliable integration into your imaging train. It features a secure M54x0.75 female thread for connection to large-format correctors and filter wheels. The standard 17.5mm back focus distance simplifies spacing calculations. To combat moisture, the camera employs a complete anti-dew solution, including a built-in heater for the AR-coated optical window and a sealed sensor chamber with a desiccant plug to prevent internal condensation on even the most humid nights.

    QHY367C Pro vs. DSLR: Why True RAW Output Matters

    While the Sony IMX094 sensor is famous for its use in Nikon DSLRs, the QHY367CPRO-C offers critical advantages for astrophotography. A DSLR is a self-contained unit, but its firmware often applies non-defeatable noise reduction and filtering to the RAW file, which can clip faint stars and alter subtle details—an effect known as "star eating."

    • True RAW Signal: The QHY367C Pro provides a TRUE RAW image output, delivering the original, unprocessed signal from the sensor. This maintains maximum flexibility for advanced processing techniques in software like PixInsight.
    • Regulated Cooling: Unlike a DSLR's passive cooling, the QHY367C's regulated TEC system provides consistent, low-noise performance regardless of ambient temperature, making calibration with dark frames far more accurate.
    • Zero Amp Glow: The camera's hardware design specifically targets and eliminates the amplifier glow that often plagues long-exposure DSLR images, resulting in cleaner, more uniform backgrounds.
  • What is the main advantage of the QHY367CPRO-C over a DSLR using the same IMX094 sensor?

    The primary advantages are regulated two-stage cooling and True RAW data output. Cooling reduces thermal noise to 0.0015e-/pixel/sec (@-15℃), far below what a DSLR can achieve. True RAW output ensures no in-camera filtering or "star-eater" algorithms are applied, preserving the faintest details for post-processing.

    How does the 128MB DDR2 buffer on the QHY367CPRO-C help my imaging sessions?

    The 128MB buffer acts as a temporary storage for image frames before they are transferred to the computer. This prevents data loss and dropped frames, which can occur if the USB connection is momentarily slow or the computer's resources are taxed. It ensures every frame you capture is saved reliably, especially when running sequences at the maximum 3.2 FPS.

    Is the 4.88µm pixel size of the QHY367CPRO-C a good match for my telescope?

    The 4.88µm pixels are very versatile. For optimal sampling (between 1.0 and 2.0 arcseconds/pixel), this camera pairs well with telescopes in the 500mm to 1000mm focal length range under typical seeing conditions. However, its high 36MP resolution still delivers excellent results on longer focal length instruments, especially with good seeing.

    How effective is the anti-dew system on the QHY367CPRO-C for imaging in humid conditions?

    The anti-dew system is highly effective. It uses two methods: a built-in heater on the optical window to prevent external dew formation, and a sealed sensor chamber with a desiccant system to absorb any internal moisture. This dual approach provides robust protection against dew, allowing for uninterrupted imaging sessions even on nights with high humidity.

    What field of view can I expect with the QHY367CPRO-C on a 1000mm refractor imaging the Andromeda Galaxy (M31)?

    On a 1000mm telescope, the QHY367CPRO-C's full-frame (36mm x 24mm) sensor will yield a field of view of approximately 2.06° x 1.37°. This is large enough to comfortably frame the entire Andromeda Galaxy (M31), including its faint outer extensions and satellite galaxies M32 and M110, in a single shot.

    With a read noise of 2.4e-, is the QHY367CPRO-C suitable for narrowband imaging of the Cygnus Loop (NGC 6960)?

    Yes, absolutely. A low read noise of 2.4e- is excellent for narrowband imaging where signals are often very faint. It allows you to stack many shorter sub-exposures to build up signal-to-noise without being overwhelmed by camera noise. This makes the QHY367CPRO-C a capable performer for capturing detailed structures in emission nebulae like the Cygnus Loop (NGC 6960) or the Heart Nebula (IC 1805).

  • Sensor Sony IMX094 Full Frame (36mm x 24mm) Color FSI CMOS
    Resolution 36MP (7376 x 4938)
    Pixel Size 4.88μm
    A/D Conversion 14-bit
    Full Well Capacity 56,000e-
    Readout Noise 2.4e- to 3.2e-
    Max Frame Rate 3.2 FPS (at full resolution)
    Dark Current 0.0015e-/pixel/sec @ -15℃
    Exposure Range 60μs - 3600s
    Recommended Gain 2800
    Amp Glow Control Nearly Zero Amplifier Glow
    Shutter Type Electronic Rolling Shutter
    Cooling System Dual Stage TEC, -45℃ below ambient
    Image Buffer 128MB DDR2 Memory
    Anti-Dew System Yes, built-in optical window heater
    Computer Interface USB3.0
    Telescope Interface M54 x 0.75
    Back Focus 17.5mm + 6mm (with CAA)
    Optical Window AR+AR Coated
    Weight 680g
  • QHYCCD Warranty