The NYX series is a completely redesigned thermal imaging camera platform designed to deliver unsurpassed performance with state-of-the-art technology, which can always provide good thermal imaging in dark and bright areas without user adjustment. NyX technology enables you to experience improved situational awareness. • Detector type : Cooled InSb 15μm (1280 x 1024) • NETD : <25mk typical (without lens) • Continuous ZOOM LENS • Continuous Digital Zoom • Advanced image processing - Auto Gain Control (AGC) - Adaptive Histogram Equalization (Adaptive HEQ) - Local Area Enhancement (LAE) - Digital Detail Enhancement (DDE) - Denoise Reduction (DNR) - Sharpness • MTTF(Mean Time To Failure) 12,000 hours • Various color sets (WhiteHot / Rainbow / Twilight / TwilightShifted / Turbo / Iron / Plasma)

Ultra-High Accuracy MEMS Certus Evo features some of the highest accuracy MEMS accelerometers and gyroscopes currently available. Certus Evo’s inertial performance exceeds some FOG IMUs and is up to 100x smaller and 10x cheaper. Certus Evo is put through Advanced Navigation’s intensive calibration process to provide consistently accurate data over an extended temperature range of -40°C to 85°C. AI-Based Algorithm Certus Evo features Advanced Navigation’s revolutionary AI neural network sensor fusion algorithm. It was designed for control applications and has a high level of health monitoring and instability prevention to ensure stable and reliable data. Dual Antenna RTK GNSS Certus Evo contains a dual frequency RTK GNSS receiver that provides up to 1 cm accuracy positioning and supports all of the current and future satellite navigation systems, including GPS, GLONASS, GALILEO, BeiDou and QZSS. Dual antenna heading provides high accuracy heading that is not impacted by magnetic interference and has no motion requirements. Time Synchronization Certus Evo contains a GNSS disciplined oscillator that can act as the primary time source within a distributed time system, enabling access to ultra-accurate system time using PTP or NTP network time sync. Certus also has a high-accuracy 1PPS and frequency output. Multi Protocol Support Certus Evo features multiple interfaces including Ethernet, CAN, RS232, RS422 and GPIOs. Certus supports all the industry standard protocols including NMEA 0183, NMEA 2000, TSS, PASHR, Simrad as well as a wide variety of proprietary protocols. It features a rich web UI and 256GB of internal logging.

VERSAWAVE HIGHLIGHTS: -Real-time video surveillance -Smallest and lightest Inmarsat UAV/UGV solution -Highest performing SATCOM solution of its size, weight and price -Proven global SATCOM solution for air, land and sea -Proven reliability, dependability and security -Low power consumption -See farther with the world's smallest satellite communication solution: enabling real-time video streaming and beyond visual line-of-sight communication with consistent global high-speed broadband coverage.

Features ● Wideband Frequency Range of 2.0~18.0GHz ● Rigid Construction with AL Brazing ● Monotonic Beam Shape, No Beam Split ● Optimized Gain Ripple and VSWR Applications ● General Purpose TX/RX Antenna ● EMC Testing ● TX/RX Antenna for EW Testing ● Wideband TX Antenna for Anechoic Chamber

• Openable sleeves • Expandable sleeves • Convoluted conduits • Heat shrink tubing & sleeves • Heats shrink boots • Specific sleeves

◾ Drive Motor : Electric motor installed in the Explosive Ordnance Disposal (EOD) Robot to supply power for driving. ◾ Flipper Motor : Electric motor that supplies power for driving the flipper of the Explosive Ordnance Disposal (EOD) Robot.

- Fire response time: 0.004 seconds - Fire monitoring range: cone angle of 90° or greater - Equipped with self-diagnostic function - Capable of distinguishing between major fires and minor fires

The Crane stands as a state-of-the-art Mid-Wave Infrared (MWIR) detector. This device features a 5-megapixel resolution in a 2560×2048 format with a fine 5μm pitch. It is based on SCD's established XBn technology or Hot Full Midwave (HFM) and incorporates a digital readout circuit developed using an advanced CMOS process. The High Operating Temperature (HOT) Focal Plane Array (FPA) functions efficiently at 150K or 120K, enabling a large-format detector that excels in image quality while maintaining a relatively compact size, weight, and power consumption. SCD continues to lead in innovation.