QHYCCD QHY367CPRO-C Color
- 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
Simulate the exact field of view of the QHYCCD QHY367CPRO-C Color with your specific telescope.
Launch Imaging AssistantThe 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.
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.
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.
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.
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.
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."
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.
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.
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.
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.
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.
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 |