GS-SW6401715-40-G is an independently developed domestic scientific deep-cooled short-wave infrared camera covering 0.9–1.7μm spectral band, targeted at high-standard laboratory and astronomical research scenarios. Equipped with 640×512 high-sensitivity InGaAs FPA featuring 15μm pixel, it adopts advanced deep TEC cooling architecture that stabilizes detector temperature at -40℃ without extra water cooling, effectively suppressing thermal dark noise and significantly improving signal-to-noise ratio during long-time integration imaging. It takes GigE digital as standard output; PAL/NTSC analog video can be customized on demand. Compatible with TTL/LVDS dual external trigger signals, and reserves interface for onboard laser spot centroid tracking algorithm integration. Global shutter with 1μs adjustable minimum exposure, arbitrary ROI window function, and full set of built-in image correction algorithms fully meet hyperspectral, fluorescence, quantum dot and astronomical observation demands. Customizable C lens mount, matched dedicated multi-algorithm imaging software and complete cross-platform SDK are supplied for user secondary development, breaking import deep-cooled camera monopoly for domestic scientific research.

1. High-performance InGaAs sensor, quantum efficiency over 70% between 1.0μm–1.6μm, pixel operability higher than 99.5%
2. Core deep cooling advantage: TEC structure, stable -40℃ sensor temperature, ultra-low dark current for hours-long exposure
3. 640×512@50Hz full frame, freely configurable arbitrary ROI to raise frame rate for fast small scientific targets
4. Global shutter with ultra-wide 1μs–1/frame exposure range, compatible with both microsecond transient and long weak light accumulation
5. Standard GigE digital transmission; PAL/NTSC analog video is optional customized function
6. Dual TTL/LVDS external trigger, perfectly matched with spectrometers, microscopy and synchronous optical test platforms
7. Integratable onboard centroid tracking for high-precision laser spot measurement and beam profiling
8. Independent air-cooled structure, no water cooling system required, simpler laboratory deployment and maintenance
9. Oversized 90×90mm reinforced heat dissipation housing, 3-side M3 multi-angle mounting holes for large optical systems
10. Fully domestic independent R&D, wide adaptability for astronomy, life science, EMMI and semiconductor precision inspection

Note: Specifications are for reference only and subject to change without prior notice.

Low-light imaging, Medical & life science imaging, Hyperspectral analysis, Laser spot tracking, High-temperature thermal detection, Astronomical observation, EMMI system, Quantum dot & fluorescence imaging, Camouflage identification, Semiconductor precision inspection, Garbage sorting