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QHYCCD QHY600C PRO SBFL Scientific Color CMOS Camera

by QHYCCD
SKU QHY-110067
Original price CA$11,199.00 - Original price CA$11,199.00
Original price
CA$11,199.00
CA$11,199.00 - CA$11,199.00
Current price CA$11,199.00
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  • 61.17 Megapixel Full-Frame (36mm x 24mm) Sony IMX455 BSI CMOS Sensor
  • Native 16-bit A/D Conversion for 65,535 grayscale levels
  • Read Noise as low as 1.1e- in High Gain Mode
  • 2GB DDR3 Image Buffer for drop-free transfer
  • Dual 10Gigabit Fiber and USB3.0 computer interfaces
  • Short Back Focus (SBFL) design with 14.5mm spacing
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  • QHY600C PRO SBFL Scientific Color CMOS Camera

    The QHY600C PRO SBFL combines a full-frame 61.17 megapixel Sony IMX455 BSI sensor with a native 16-bit A/D converter, delivering an unprecedented level of resolution and dynamic range for scientific imaging. With multiple readout modes offering noise as low as 1.1e- and a full well capacity exceeding 80ke-, this camera captures both the faintest nebulosity and brightest stellar cores in a single exposure. Data integrity is ensured by a 2GB DDR3 buffer and dual 2x10Gigabit Fiber interfaces, enabling a full-resolution 16-bit frame rate of up to 3.5 FPS for demanding research applications.

    Full-Frame 61.17MP Sony IMX455 Sensor: Native 16-Bit Depth

    At the heart of the QHY600C Pro is the 36mm x 24mm Sony IMX455 sensor, which provides an enormous 9576 x 6388 pixel array. The 3.76µm pixels are an ideal match for high-resolution refractors and corrected reflectors, sampling the sky with immense detail. Unlike cameras that use 12-bit or 14-bit conversion, the QHY600 Pro employs a true, native 16-bit A/D converter, rendering 65,535 distinct grayscale levels for exceptionally smooth tonal gradations in deep-sky objects.

    Multi-Mode Readout: 1.1e- Read Noise and >80ke- Full Well

    The QHY600C Pro offers several selectable readout modes to optimize the camera for any target. In High Gain Mode, read noise plummets to a mere 1.1e-, allowing you to extract faint signal from photon-starved regions with minimal noise penalty. For bright targets or long-exposure narrowband imaging, the Extended Full Well Mode expands pixel capacity to over 80ke-, preventing saturated stars and preserving highlight detail. This flexibility, combined with a dark current of just 0.0022e-/pixel/sec at -20°C and zero amplifier glow, ensures a clean, data-rich foundation for your images.

    Professional I/O: 2x10Gbit Fiber, USB3.0, and a 2GB DDR3 Buffer

    Designed for applications where speed and reliability are critical, the QHY600C Pro includes both a standard USB3.0 port and a dual 10Gigabit Fiber Optic interface. The fiber connection allows for high-speed data transfer over long distances, delivering up to 3.5 FPS at full 16-bit resolution. To handle this massive data stream without dropped frames, the camera incorporates a 2GB DDR3 memory buffer, a feature essential for remote observatories and automated scientific surveys.

    Regulated Cooling to -35°C Below Ambient

    Thermal noise is suppressed by a powerful dual-stage thermoelectric cooling system, capable of achieving a regulated temperature typically -35°C below ambient for long exposures. This aggressive cooling dramatically reduces dark current, a critical factor for clean, multi-hour integrations. To combat condensation in humid environments, the camera is equipped with a built-in anti-dew heater for the optical window and an internal humidity sensor to monitor conditions within the sealed sensor chamber.

    Short Back Focus (SBFL) Design: 14.5mm for Complex Imaging Trains

    This SBFL (Short Back Focus) version of the QHY600 Pro is engineered with a reduced back focus distance of just 14.5mm. This minimal spacing is a critical advantage for imagers using complex optical trains that include filter wheels, off-axis guiders, and adaptive optics. The reduced profile provides the extra room needed to accommodate these accessories while still reaching the precise 55mm back focus required by most coma correctors and field flatteners.

    QHY600 Pro SBFL vs. Standard: Which Version is Right?

    The primary difference between the QHY600 Pro models is the back focal length. This SBFL model has 14.5mm of back focus, while the standard version has 17.5mm. While a 3mm difference seems small, it can be the deciding factor in a complex imaging train.

    • Choose the SBFL (14.5mm) version if: You use a filter wheel (typically 20mm thick) and an off-axis guider (typically 10-15mm thick). The shorter back focus of the camera itself provides the necessary space to fit these components within the standard 55mm spacing of your corrector.
    • Choose the Standard (17.5mm) version if: Your imaging train is simpler, perhaps using only a filter drawer or no accessories between the camera and corrector. The standard version allows for more straightforward connections with fewer thin, specialized adapters.
  • What are the main benefits of the QHY600C Pro's 16-bit A/D converter?

    A native 16-bit A/D converter allows the QHY600C Pro to distinguish between 65,535 different levels of brightness. Compared to 12-bit (4,096 levels) or 14-bit (16,384 levels) cameras, this provides significantly smoother tonal transitions and greater dynamic range, especially in bright objects with subtle details like the core of the Orion Nebula (M42) or bright globular clusters.

    How does the 2GB DDR3 buffer on the QHY600C Pro prevent dropped frames?

    The 2GB DDR3 buffer acts as a high-speed temporary storage for image frames before they are transferred to the computer. When the host computer or USB bus is temporarily busy, the buffer holds the incoming data from the 61.17MP sensor, preventing data loss. This is crucial for maintaining a stable frame rate, especially during high-speed ROI imaging or when running multiple applications on the control PC.

    How does the QHY600C Pro's 3.76µm pixel size perform with a 500mm f/5 refractor for imaging the North American Nebula (NGC 7000)?

    With a 500mm focal length telescope, the QHY600C Pro's 3.76µm pixels yield an image scale of 1.55 arcseconds per pixel. This is an excellent match for typical seeing conditions (1.5-3.0 arcseconds), ensuring you capture sharp, well-sampled stellar detail across the vast expanse of the North American Nebula (NGC 7000). The full-frame sensor will easily frame the entire nebula and the neighboring Pelican Nebula (IC 5070) in a single shot.

    What readout mode on the QHY600C Pro is best for imaging faint galactic details in M51 with an 11" SCT at f/7?

    For capturing the faint tidal tails and dust lanes of the Whirlpool Galaxy (M51) with an SCT, the High Gain Mode is the ideal choice. This mode reduces the read noise to as low as 1.1e-, which allows you to stack many shorter exposures to build up signal-to-noise on faint structures without being dominated by camera noise. This strategy also helps mitigate the impact of tracking errors or seeing fluctuations during a long imaging session.

    What is the purpose of the 2x10Gigabit Fiber interface on the QHY600C Pro?

    The 2x10Gigabit Fiber interface is a professional feature for applications requiring very high data rates over long distances, such as remote observatories or scientific surveys. It allows the camera to stream data at its maximum frame rate (e.g., 3.5 FPS @ 16-bit) without the bandwidth limitations or distance constraints of USB3.0, ensuring perfect data integrity.

    Why is the Short Back Focus (14.5mm) version of the QHY600C Pro necessary?

    The Short Back Focus (SBFL) version (14.5mm) is specifically designed for imagers who use multiple accessories like filter wheels, off-axis guiders, or adaptive optics. These components add significant length to the optical path. The SBFL's shorter body provides the critical extra millimeters needed to fit all accessories into the light path and still achieve the standard 55mm back focus distance required by most field flatteners and coma correctors.

    Does the QHY600C Pro suffer from amplifier glow?

    No. The QHY600C Pro is designed to produce zero amplifier glow, regardless of exposure length or gain setting. This simplifies calibration by eliminating the need for complex dark frame libraries that must perfectly match the exposure time and temperature of your light frames.

  • Sensor Sony IMX455 Color BSI CMOS
    Optical Format Full Frame (36mm x 24mm)
    Resolution 9576 x 6388 (61.17 Megapixels)
    Pixel Size 3.76µm
    A/D Conversion Native 16-bit
    Full Well Capacity >51ke- (Photographic Mode) / >80ke- (Extended Mode)
    Read Noise 1.1e- to 7.8e- (Mode Dependent)
    Dark Current 0.0022e-/pixel/sec @ -20°C
    Image Buffer 2GB DDR3 Memory
    Max Frame Rate (16-bit) 2.5 FPS (USB3.0) / 3.5 FPS (PCIE Mode)
    Cooling System Dual-Stage TEC, -35°C below ambient (typical)
    Anti-Dew / Humidity Yes, built-in heater and humidity sensor
    Shutter Type Electronic Rolling Shutter
    Exposure Range 40µs - 3600s
    Computer Interface USB3.0, 2x10Gigabit Fiber
    Accessory Ports 4PIN QHYCCD CFW Port, Trigger/GPS Port
    Back Focal Length 14.5mm (SBFL Version)
    Optical Window AR+AR Coated
    Weight Approx. 1kg
    Power Consumption Up to 40W (100% cooling)
  • QHYCCD Warranty