QHYCCD QHY991 Class 1 SWIR Camera
- Class 1 Scientific SWIR Camera
- Sony InGaAs Sensor Technology
- Broad Spectral Response (400-1700 nm)
- Active Air and Liquid Cooling Support
- Standard C-Mount Interface
Simulate the exact field of view of the QHYCCD QHY991 Class 1 SWIR Camera with your specific telescope.
Launch Imaging AssistantThe QHY991 is a Class 1 scientific short-wave infrared (SWIR) camera built around a high-sensitivity Sony InGaAs sensor, designed for applications requiring a broad spectral response from visible light into the SWIR spectrum.
At the core of the QHY991 is a Sony InGaAs sensor, which provides high sensitivity across an exceptionally broad spectral range. This allows for detailed imaging in wavelengths beyond the reach of typical silicon-based sensors. The sensor's architecture, which utilizes Cu-Cu interconnect technology, is engineered to minimize fixed-pattern noise and reduce the pixel defect ratio, ensuring clean data for scientific analysis.
InGaAs sensors inherently produce a higher dark current than their silicon counterparts, making active cooling a critical requirement for long-exposure or high-precision measurements. The QHY991 addresses this with a powerful cooling system that supports both air and liquid cooling methods. This thermal management is essential for stabilizing the sensor and reducing thermal noise to achieve the highest possible signal-to-noise ratio in demanding conditions.
Designed for straightforward integration into scientific and industrial setups, the QHY991 features a standard C-mount thread. The camera body also includes an integrated filter holder designed for common filter sizes used in laboratory applications. This allows you to easily install SWIR-pass or other specialized filters required for your specific imaging or measurement task without complex adapters.
The QHY991 is a scientific camera ideal for applications that benefit from imaging in the short-wave infrared spectrum. This includes semiconductor inspection, material sorting, anti-counterfeiting, biological imaging, and specialized astronomical imaging where SWIR can reveal details obscured in visible light.
InGaAs sensors, by nature, generate more thermal noise (dark current) than silicon CMOS or CCD sensors. The QHY991's robust air and liquid cooling support is essential to lower the sensor's operating temperature, which significantly reduces this noise. Lower noise is critical for achieving clear, high-contrast images, especially during longer exposures.
Jupiter's atmosphere has distinct absorption and reflection bands in the SWIR spectrum, particularly for methane. Using the QHY991 with an appropriate methane filter would allow you to capture high-contrast images of Jupiter's cloud structures, revealing details about storm systems and atmospheric layers that are invisible to standard RGB cameras.
The Cu-Cu (copper-to-copper) interconnect technology used in the QHY991's Sony sensor allows for a more direct and efficient connection between pixel layers. This advanced manufacturing technique results in significantly lower fixed-pattern noise (FPN) and a lower defect pixel ratio, leading to cleaner and more uniform images.
The QHY991 includes an integrated filter holder designed to accept common filter sizes used in laboratory and industrial settings. This allows for the direct installation of SWIR-pass, bandpass, or other analytical filters into the optical path in front of the sensor.
Class 1 typically refers to the grade of the sensor, indicating it meets the manufacturer's highest standards for quality. For scientific cameras, this usually means the sensor has a very low number of pixel defects and provides the most uniform response, making it suitable for quantitative measurement and analysis.
| Product | Scientific Cameras - QHY991 |
| Sensor Class | Class 1 |
| Spectrum | SWIR (Short-Wave Infrared) |
| Sensor Technology | InGaAs |
| Cooling | Air Cooling (Liquid Supported) |