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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 QHY183M Mono

by QHYCCD
SKU QHY-100105
Original price $999.00 - Original price $999.00
Original price
$999.00
$999.00 - $999.00
Current price $999.00
Price Match Policy!
  • 20 Megapixel back-illuminated Sony IMX183 mono sensor
  • 2.4µm pixels for high-resolution imaging
  • Dual-stage TEC cooling to -40°C below ambient
  • Extremely low 1.0e- read noise at high gain
  • 128MB DDR2 image buffer to prevent dropped frames
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  • Description
  • FAQ
  • Specifications
  • In the Box
  • Downloads
  • Warranty
  • QHYCCD QHY183M Monochrome CMOS Camera

    The QHYCCD QHY183M combines a high-resolution 20 Megapixel Sony IMX183 sensor with an efficient, low-noise architecture designed for both deep-sky and planetary astrophotography. Its 2.4µm pixels are ideally matched to short-focal-length refractors, while the dual-stage TEC cooler achieves a -40°C delta to minimize thermal noise during long exposures. With a read noise as low as 1.0e- and a 128MB DDR2 buffer ensuring stable data transfer over USB 3.0, the QHY183M captures clean, detailed data from faint nebulae and fast-moving planets alike.

    Sony IMX183 Sensor: 20 Megapixels at 2.4µm

    At the heart of the QHY183M is Sony's 1-inch back-illuminated IMX183 sensor, which delivers a massive 5544x3684 image array. The small 2.4µm pixels achieve fine image sampling, resolving intricate details in galaxies and planetary nebulae even with telescopes under 1000mm in focal length. This high resolution makes the camera a powerful tool for capturing smaller targets without requiring extreme focal lengths or barlow lenses.

    Deep-Sky Imaging: -40°C Cooling and 1.0e- Read Noise

    For long-exposure astrophotography, thermal noise is the primary challenge. The QHY183M's dual-stage TEC cooling system aggressively drops the sensor temperature to -40°C below ambient, reducing dark current to a negligible 0.0024e-/pixel/sec at -15°C. This deep cooling, combined with an exceptionally low read noise of 1.0e- in high-gain mode, ensures that faint, wispy details in nebulae are captured with excellent contrast and signal-to-noise ratio.

    Planetary Performance: 19 FPS and 128MB DDR2 Buffer

    While excelling at deep-sky work, the QHY183M is also a capable high-speed planetary imager. It can stream full-resolution 20 Megapixel frames at 19 FPS in 8-bit mode, with rates climbing to 130 FPS at 640x480 resolution for capturing moments of steady seeing. A built-in 128MB DDR2 image buffer is critical for this task, preventing data loss and dropped frames during high-speed captures over its USB 3.0 interface.

    Field-Ready Design: Anti-Glow and Anti-Dew Systems

    QHYCCD has engineered the QHY183M for reliability during all-night imaging sessions. The camera incorporates active Anti-Glow Control, which significantly reduces the amplifier glow common in CMOS sensors, resulting in cleaner calibration. A built-in anti-dew heater on the optical window prevents condensation from forming, ensuring a clear light path even on nights with high humidity. The camera connects to your optical train via a standard M42/0.75 interface with a 17.5mm back focal length.

    QHY183M vs. QHY163M: Resolution vs. Field of View

    Choosing between the QHY183M and its sibling, the QHY163M, comes down to a trade-off between image scale and sky coverage. The decision depends on your primary targets and telescope.

    • QHY163M Advantage: With its larger 4/3" sensor and 3.8µm pixels, the QHY163M captures a wider field of view. This makes it a better choice for large targets like the Andromeda Galaxy (M31) or the North American Nebula (NGC 7000), especially on longer focal length telescopes.
    • QHY183M Advantage: The QHY183M's smaller 2.4µm pixels and higher 20 Megapixel resolution provide a more detailed image scale. It excels at framing smaller galaxies, planetary nebulae, and globular clusters, or when used with wide-field refractors where it can capture stunning detail across a broad patch of sky.
  • What kind of telescope is a good match for the QHY183M's 2.4µm pixels?

    The QHY183M is ideally suited for short-focal-length telescopes like apochromatic refractors and fast astrographs (f/4 to f/6). The small 2.4µm pixels achieve excellent image sampling without needing a Barlow lens, capturing high-resolution, wide-field views of large nebulae and star clusters.

    How does the QHY183M's 128MB DDR2 buffer help with planetary imaging of Jupiter?

    When imaging Jupiter, you need to capture thousands of frames as quickly as possible to "freeze" atmospheric seeing. The 128MB DDR2 buffer acts as a temporary storage space, ensuring that data from the sensor is captured without interruption, even if the computer's USB bus is momentarily busy. This prevents dropped frames, which is critical for creating a smooth, high-quality final image from the best data.

    What is the benefit of the QHY183M's low 1.0e- read noise?

    Read noise is the electronic noise introduced when the sensor's signal is read out. A very low read noise of 1.0e- (at high gain) means the camera can detect extremely faint signals before they are lost in the noise floor. This is crucial for both narrowband deep-sky imaging and "lucky imaging" of planets, where you use very short exposures.

    Can I use the QHY183M for narrowband imaging?

    Yes, the QHY183M is an excellent camera for narrowband imaging. Its monochrome sensor is highly sensitive to the specific wavelengths of H-alpha, OIII, and SII filters. The combination of low read noise and efficient cooling allows you to take the long exposures necessary to capture faint emission nebulae with high contrast.

    How does the Anti-Glow Control on the QHY183M work?

    Many CMOS sensors exhibit "amp glow," a faint illumination from the sensor's electronics that can be seen in long exposures. The QHY183M features Anti-Glow Control, a hardware-level function that significantly suppresses this glow. This results in much cleaner raw frames that are easier to calibrate with standard dark frame subtraction.

    What is the difference between the QHY183M and QHY183C models?

    Both cameras use the same Sony IMX183 sensor. The key difference is:

    • QHY183M: This is a monochrome camera. It is more sensitive and produces sharper images but requires separate filters (L, R, G, B, or narrowband) to create a color image.
    • QHY183C: This is a one-shot-color (OSC) camera. It has a built-in Bayer filter matrix to capture color images in a single exposure and includes an IR-Cut filter window. It is more convenient but less sensitive than the monochrome version.
  • CMOS Sensor Sony IMX183, Back-Side Illuminated (BSI)
    Sensor Size 1-inch (13.3mm x 8.87mm)
    Effective Pixels 20 Megapixels
    Resolution 5544 x 3684
    Pixel Size 2.4µm
    Full Well Capacity 15,500 e-
    Readout Noise 1.0e- (High Gain) to 2.7e- (Lowest Gain)
    AD Sample Depth 12-bit (output as 16-bit and 8-bit)
    Shutter Type Electric Rolling Shutter
    Max Frame Rate (Full Res) 19 FPS @ 8-bit / 7.5 FPS @ 12-bit
    Frame Rate (ROI) 4K Video (4096x2160): 31 FPS @ 8-bit
    HD Video (1920x1080): 60 FPS @ 8-bit
    VGA (640x480): 130 FPS @ 8-bit
    Exposure Time Range 50µs to 3600s
    Unity Gain 10
    Dark Current 0.0024 e-/pixel/sec @ -15°C
    Cooling System Dual-Stage TEC
    Cooling Delta -40°C below ambient
    Image Buffer 128MB DDR2
    Computer Interface USB 3.0
    Telescope Interface M42x0.75
    Back Focal Length 17.5mm (±0.2mm)
    Optical Window AR+AR Coated
    Anti-Glow Control Yes, Amplifier Glow Reduction
    Anti-Dew Heater Yes
    Weight 650g
  • QHYCCD Warranty