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QHYCCD QHY174M-GPS

by QHYCCD
SKU QHY-100117
Original price CA$1,735.00 - Original price CA$1,735.00
Original price
CA$1,735.00
CA$1,735.00 - CA$1,735.00
Current price CA$1,735.00
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  • 2 Megapixel Sony IMX174 Mono Sensor
  • Electronic Global Shutter Eliminates Motion Artifacts
  • Integrated GPS Module with 1 Microsecond UTC Time-Stamp Precision
  • Captures up to 138 FPS at Full 1920x1200 Resolution
  • Dual-Stage TEC Cooling to -40°C Below Ambient
  • 5.86μm Pixels and >32ke- Full Well Capacity
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  • Description
  • FAQ
  • Specifications
  • In the Box
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  • Warranty
  • QHYCCD QHY174M-GPS Mono CMOS Camera

    The QHYCCD QHY174M-GPS is engineered for scientific applications where precision timing is non-negotiable, integrating a hardware GPS module that stamps each frame with a 1-microsecond UTC timestamp. Its 2 Megapixel Sony IMX174 sensor combines 5.86μm pixels with an electronic global shutter to capture fast-moving objects at up to 138 FPS without distortion. A dual-stage TEC cools the sensor to -40°C below ambient, reducing dark current to just 0.224e-/pixel/sec for clean, low-noise data acquisition critical for occultations and exoplanet transit analysis.

    Sony IMX174 Global Shutter: 138 FPS with Zero Artifacts

    Unlike rolling shutters that expose different parts of the sensor sequentially, the Sony IMX174's electronic global shutter exposes all 2 million pixels simultaneously. This completely eliminates motion artifacts, which is critical when imaging rapidly rotating planets like Jupiter, turbulent solar prominences, or fast-moving asteroids. At a full resolution of 1920x1200, the camera streams data over USB 3.0 at 138 FPS in 8-bit mode or 75.1 FPS in 16-bit mode, ensuring you can freeze moments of perfect seeing.

    GPS-Enabled Precision: 1 Microsecond UTC Time Stamping

    The defining feature of the QHY174M-GPS is its integrated GPS receiver, which provides hardware-level time stamping on every captured frame with a precision of 1 microsecond. This capability is essential for scientific work such as timing asteroid occultations to map their size and shape, or recording exoplanet transits to refine orbital data. For pro-am collaborations and time-critical event capture, this removes all timing ambiguity introduced by software or computer clock drift.

    Scientific-Grade Cooling: -40°C Delta for Low-Noise Data

    To ensure clean data, the QHY174M-GPS employs a powerful dual-stage TEC cooler capable of reaching -40°C below the ambient temperature. This aggressive cooling drastically reduces thermal noise, lowering the dark current to an exceptionally low 0.224e-/pixel/sec when cooled to -20°C. Combined with a read noise as low as 1.6e-, the camera produces clean frames even during longer exposures, pushing its capabilities beyond planetary imaging into more demanding scientific applications.

    • Deep Cooling: The -40°C delta T ensures stable, low-noise performance even on warm nights.
    • Anti-Dew Heater: An integrated heater for the optical window prevents dew or frost formation during cooling cycles, maintaining a clear optical path.

    On-Camera Analysis: 100KB Buffer for Occultations and Seeing

    A unique feature for field research is the camera's 512KB built-in memory, with 100KB of user-accessible space. This allows the camera to store hundreds or even thousands of small region-of-interest (ROI) frames directly in its memory, independent of a connected computer. This is ideal for creating a remote seeing monitor, an automated occultation recording system, or for performing on-the-fly optical analysis without the overhead of continuous data transfer.

    QHY174M-GPS vs. Standard QHY174M: When Precision Timing Matters

    Both cameras share the same excellent Sony IMX174 global shutter sensor, high frame rates, and powerful cooling system. The choice between them comes down to a single question: do you need verifiable, microsecond-accurate time data?

    • Choose the Standard QHY174M if: Your primary targets are general solar, lunar, and planetary imaging. The global shutter and high frame rate are the key features you need, and software-based timing is sufficient.
    • Choose the QHY174M-GPS if: You are involved in scientific research like asteroid occultations, satellite tracking, exoplanet transit timing, or any other field where your data's temporal accuracy is as important as its image quality. The hardware-based UTC timestamp is the reason this model exists.
  • What is the main advantage of the QHY174M-GPS for scientific work?

    The primary advantage is its integrated GPS module, which provides hardware-level timestamps on every frame with 1-microsecond precision to the Coordinated Universal Time (UTC) standard. This eliminates timing errors from software or computer clocks, which is critical for applications like asteroid occultation and exoplanet transit timing.

    How would I use the QHY174M-GPS to time an asteroid occultation?

    During an occultation, you record a high-speed video of the target star. The GPS module on the QHY174M-GPS embeds a highly accurate UTC timestamp into each frame's metadata. By analyzing when the star disappears and reappears, you can determine the precise start and end times of the event, which helps scientists create a detailed profile of the asteroid's shape and size.

    Does the Global Shutter on the QHY174M-GPS help when imaging Jupiter?

    Yes, absolutely. Jupiter rotates in under 10 hours, and this rapid motion can cause distortion or "smear" with a common rolling shutter camera, especially during longer video captures. The Electronic Global Shutter on the QHY174M-GPS exposes the entire sensor at once, freezing the planet's motion and atmospheric turbulence on every frame, resulting in significantly sharper and more detailed final images.

    Is the QHY174M-GPS a good choice for solar imaging in an H-alpha telescope?

    It is an excellent choice. The same benefit of the global shutter applies to solar imaging. Fast-moving solar features like prominences, flares, and turbulent filaments can be easily distorted by a rolling shutter. The QHY174M-GPS's global shutter ensures these dynamic events are captured without any motion artifacts, producing sharp, clean images of the solar surface and chromosphere.

    What does the built-in 100KB image buffer on the QHY174M-GPS allow me to do?

    The 100KB user-accessible buffer allows you to store small Region of Interest (ROI) frames directly on the camera. This is useful for creating a standalone, automated system like a remote seeing monitor or an occultation detector that can capture and analyze data without being actively managed by a connected PC.

    Do I need the QHY174M-GPS for casual planetary imaging?

    For casual lunar, solar, and planetary imaging, the GPS functionality is likely unnecessary. The standard QHY174M offers the same superb IMX174 sensor with its global shutter. You should only invest in the QHY174M-GPS model if your work specifically requires the verifiable, high-precision UTC time stamping for scientific purposes.

  • Sensor Sony IMX174 Mono FSI CMOS
    Resolution 2 Megapixels (1920 x 1200)
    Pixel Size 5.86μm
    Sensor Size 11.25mm x 7.03mm (1/1.2-inch)
    A/D Conversion 12-bit (output as 16-bit or 8-bit)
    Shutter Type Electronic Global Shutter
    Full Well Capacity >32,000e-
    Read Noise 1.6e- to 5.3e-
    Exposure Range 5μs to 900s
    Dark Current 0.224e-/pixel/sec @ -20℃
    Max Frame Rate (Full) 138 FPS @ 8-bit / 75.1 FPS @ 16-bit
    Max Frame Rate (ROI) Up to 305 FPS @ 8-bit (480 lines)
    Computer Interface USB 3.0
    GPS Time Stamping 1 micro-second precision to GPS UTC clock
    Cooling System Dual-Stage TEC, -40°C below ambient
    Anti-Dew Heater Yes
    Built-in Buffer 512KB Flash (100KB user-accessible)
    Optical Window AR+AR Coated
    Back Focus 17.5mm
    Filter Wheel Port 4-PIN QHYCCD CFW Port
    Weight 450g
    Power Consumption 3W (0%) to 27W (100% TEC)
  • QHYCCD Warranty