The COX640AV embodies COX’s cutting-edge cooled MWIR imaging technology, delivering unparalleled performance for the most demanding applications. Its 640x512 resolution and 15μm pixel pitch InSb sensor achieve thermal sensitivity of less than 20mK, ensuring crystal-clear imaging for precise analysis. Capable of operating across a wide temperature range, the COX640AV supports multiple imaging modes and advanced processing functions including AGC, NUC, and customizable color palettes. This ensures adaptability to a variety of mission-critical environments such as defense, aerospace, scientific research, and industrial inspection. In addition to superior imaging quality, the COX640AV is designed for reliability and operational readiness. With rapid image stabilization after startup and robust construction, it performs consistently in harsh environments where stability is non-negotiable. Its combination of cooled MWIR precision, advanced processing features, and rugged design positions the COX640AV as a trusted solution for customers who require accuracy, speed, and durability. By integrating COX’s proprietary calibration expertise, it not only provides outstanding real-time imaging but also guarantees long-term reliability and service continuity.

[LEO GNSS-R] Satellite : LEO RF Characteristics : GPS L1/L5, Galileo E1/E5a(option) Accuracy : Position ≤ 10m(3DRMS), Velocity : ≤ 1m/s Raw Data Accuracy : Pseudo-Range : 1m(RMS) Carrier-Phase : 10mm(RMS) Data Output Rate : 1Hz 1PPS Accuracy : Sync to GPS Time Data < 1us (1PPS Accuracy < 1.5us) TTFF : Cold Start ≤ 20min / Warm Start ≤ 10min Dara Interface : MIL-STD-1553B, RS-422(Data Interface) [GEO GNSS-R] Satellite : GEO RF Characteristics : GPS L1/L2C/L5, Galileo E1 Accuracy : Position :: ≤ 30m(3DRMS), Velocity : ≤ 1m/s Raw Data Accuracy : Pseudo-Range : 1m(RMS) Carrier-Phase : 10mm(RMS) Data Output Rate : 1Hz 1PPS Accuracy : 2us(RMS)/Sync to GPS Time Data TTFF : Cold Start ≤ 45min / Warm Start ≤ 20min Dara Interface : MIL-STD-1553B EEE Parts : ITAR Free Parts

The maximum transmission distance varies based on the following frequency-related specifications. Camera Frequency Max Cable Length ================ =============== 20 ~ 60 MHz 10 m 60 ~ 80 MHz 7 m 80 ~ 85 MHz 5 m The PoCL Bypass function supports Power over Camera Link (PoCL) operation from the Frame Grabber to the selected camera. However, the power supply to unselected cameras is automatically disabled. To prevent power cutoff, separate power must be provided to the cameras. Configurations are available as follows, including image signal amplification. [Features of CLM-30C4]  Fully supports the Camera Link interface (Area/Line Scan).  Provides manual (switch) or remote (RS232) camera selection.  Allows selection from one of four cameras configured for Base (Layer 1) or Medium/Full (Layer 2) levels.  Supports Base/Medium/Full setups (CC1~4, RS232, LVAL, DVAL, FVAL)  PoCL bypass function: Automatically powers only the selected camera when PoCL-compatible cameras, frame grabbers, and cables are used.  Supports pixel frequency from 20 to 85 MHz.  Supports PoCL signal bypass (patented).  Enables lossless transmission.  Provides additional full-duplex RS232 communication at up to 256 Kbps.  Features a locking DC power jack (Molex).

APA-110 is designed to eliminate CO2 emissions with its unique technical characteristics. It can perform the complete service of aircraft at remote parking places with diesel engine and it is also capable to operate from the 50/60Hz, 400V, 3 phase main power supply grid as any electrical GPU, without fuel consumption and with zero operating emissions. The range of different APA configurations with no emissions allow for safer, cleaner and more practical operational conditions for operators and personnel at the location.

The EXOpod is the most advanced cubesat deployment system on the market. It is available in 6U/8U, 12U and 16U sizes which can be broken down into smaller slots to accommodate cubesats of any size. EXOpod Nova, the latest generation of the EXOpod line, is rapidly expanding what the cubesat design standard (CDS) is capable of – cubesats launching with Nova can now increase the volume of their lateral protrusions by 400% and their mass by 30%, enabling a wider and more powerful array of satellite designs and use cases.

ㅇKey Features - Null Steering / Beam Forming - 4 Channel RF Input (changeable, 3/5/7 channel) - Anti Jamming Performance : ≥ JSR 00 dB - RAIM Detect and Isolation - RS-422 (SDLC Protocols) - High temperature resistance radome can be applied on the externally mounted antenna environment ㅇQuality and Certification - MIL-STD-810G - MIL-STD-461F - Certicicates of Defense Quality (Anti-jamming Receiver System)

The Ophir® SupIR 80-1200mm MWIR f/5.5 and SupIR 60-1200mm MWIR f/4 lenses are designed for 15 µm 640x512 and SXGA 10 µm pitch FPA (focal plan arrays) cooled MWIR detectors, respectively, providing detection ranges exceeding 28 km. Key Features: - High performance IR continuous zoom lens - Compatibility with 10 µm SXGA/HD and 15 µm 640x512 cameras - Maintains accurate LOS & focus through the full zoom range - Designed for extended range observation & C-UAS systems - Detection range exceeds 26 km