QHYCCD 992 Short Wavelength infrared (SWIR) Scientific Camera
The QHY990, QHY991, and QHY992 models are advanced short-wavelength infrared (SWIR) cameras that utilize Sony’s InGaAs sensors: IMX990, IMX991, and IMX992. These scientific imaging devices offer a high quantum efficiency, reaching up to 77% at 1200 nm, and cover a broad spectral range from 0.4 μm to 1.7 μm with excellent sensitivity.
The QHY990 series provides both air and liquid cooling options. Air cooling allows a temperature drop of -35℃ below ambient, while liquid cooling achieves -45℃ using regular water, and even lower–between -60℃ and -80℃–with a chilled coolant. Since InGaAs sensors typically produce more dark current than silicon-based ones, effective cooling systems are essential.
Applications include:
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Infrared astronomy and photometry
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Daylight star detection
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Optical communication and laser experiments
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Scientific research and optical laboratory setups
Overview
The QHY990/QHY991/QHY992 series are cutting-edge SWIR imaging solutions featuring Sony’s IMX990, IMX991, and IMX992 InGaAs sensors. These cameras deliver exceptional quantum efficiency–up to 77% at 1200 nm–and operate over a wide spectral range of 0.4 μm to 1.7 μm. Utilizing Cu-Cu bonding technology, the sensors minimize fixed pattern noise (FPN) and maintain a low rate of defective pixels.
Cooling flexibility is a key strength of the QHY990 series. With air cooling, the cameras can drop temperatures to 35℃ below ambient. When using standard water for liquid cooling, they can reach -45℃, and with chilled fluid, they are capable of going as low as -60℃ to -80℃. This strong thermal management is vital due to the relatively high dark current characteristics of InGaAs detectors.
Additionally, QHY990 series cameras are equipped with 25mm filter holders–an industry-standard size widely used in laboratory settings. Installing SWIR filters is simple, and the cameras offer a 17.5mm back focal length (B.F.L.) using a standard C-mount interface.
TECHNICAL SPECIFICATION
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Image Sensor
Sony IMX992 InGaAs
Pixel Size
3.45 μm × 3.45 μm
Effective Pixels
5.32 Megapixels
Effective Image Area
1/4 inch
Effective Pixel Area
2592 × 2056
Total Pixel Area
2688 × 2080
A/D Conversion
12-bit A/D
Full Well Capacity
30ke⁻ (LG AllPixel Mode)
23ke⁻ (HG AllPixel Mode)
Read Noise
The measured data is after Bias Frame FPN calibration.
83e⁻ (LG AllPixel Mode)
63e⁻ (HG AllPixel Mode)
Exposure Time Range
30μs – 300 sec
Shutter Type
Electronic Global Shutter
Computer Interface
USB 3.0
Filter Wheel Interface
4PIN QHYCCD CFW Port
Trigger Port
One Hardware Trig-In Socket (RCA type), Opto-isolated
Full Frame Rates
USB 3.0:
48 FPS @ 8bit
32 FPS @ 16bit
ROI Frame Rates
USB 3.0:
1080 lines – 83 FPS @ 8bit, 56 FPS @ 16bit
768 lines – 110 FPS @ 8bit, 75 FPS @ 16bit
480 lines – 158 FPS @ 8bit, 110 FPS @ 16bit
Built-in Image Buffer
128MB DDR2 Memory Buffer
Cooling System
Dual Stage TEC Cooler: –35℃ below ambient (Test temperature 20℃)
Anti-Dew Heater
Available
Firmware / FPGA Upgrade
Available via Camera USB Port
Optic Window Type
AR + AR High-Quality Multi-Layer Anti-Reflection Coating
Back Focal Length
12.5 mm
Adapters
Supports C-Mount, 1.25″ (with adapter)
Supports D=25mm and D=25.4mm filters
Power Consumption
25W (100%)
10W (50%)
2W (0%)
Curves 











Mechanical Dimensions

Sample Images
QHY990 Sample Image in daytime. With 16mmF1.4 SWIR lens @F2.8 , 1200-1800nm filter. Gain=0, exposure time = 1.3ms. Download 16bit FITs QHY990_DAYTIMEQHY990_DAYTIME

QHY990 Sample image under sky (at night). . With 16mmF1.4 SWIR lens @F1.4 , 1200-1800nm filter. Exposure = 2sec stack 29frames . -11C sensor temperature. Dark frame calibrated.

Here are the stars in the daytime with QHY991 camera by Martin Miller:



The Orion Nebula, First Light Captured with the QHY992 Camera and a 1200-1700 nm Bandpass Filter. The shortwave infrared image reveals details in the nebula’s center that differ significantly from those seen in visible light.
Accessories
