Quadro expands the capabilities of Exolaunch's microsatellite separation systems with a four-point offering tailored to match the Arrow 150 satellite with masses up to 250 kg. It is currently the only separation system which is qualified to fly the Arrow 150 platform on the SpaceX Transporter missions. Quadro was crowned the most innovative separation system in Europe by winning the Innovation in Space Award 2023 at the European Space Summit, celebrating its unique blend of flight-proven technology and cutting edge four-point design securing access to orbit for the next generation of microsatellite buses.

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 CLR-30 amplifies and transmits Camera Link signals in Base/Medium/Full configurations (up to 10 Taps supported) from a camera to a PC frame grabber. Key Features  Fully supports the Camera Link interface (Area/Line Scan).  Supports Base/Medium/Full setups (CC1~4, RS232, LVAL, DVAL, FVAL).  Supports pixel frequency from 20 to 85 MHz.  Supports 10 Taps cameras.  Enables lossless transmission.  Provides additional full-duplex RS232 communication at up to 256 Kbps.  Supports PoCL signal bypass (patented).  Features a locking DC power jack (Molex) and SDR connectors.  Compact size compared to previous models.

The Nebula connector employs the renowned Hypertac hyperboloid contacts as the bedrock of its high reliability providing immunity to shock and vibration fretting and over 100,000 mating cycles. These features combine with current carrying capacity up to 1.5 Amps per contact and low insertion / extraction forces to provide significantly enhanced quality and reliability performance compared with other more commodity connector solutions. Available for direct mounting to PCB, the Nebula Series supports independent function for all its 22 contacts. It also offers optional quarter-turn locking hardware for faster connector securing and to prevent unintentional separation.

The Monitor meets the military environmental specifications. COTS technology's design, manufacturing and technical support is committed to continuously providing a total solution to your display needs. The Monitor uses a full array of LED backlights which employ a local dimming technology for precise picture control and smooth motion for a more natural picture.

Portable Real time USB signal analyzer, 9 kHz-7.5 GHz

Our XR-based aircraft maintenance simulator is officially certified by the Ministry of Land, Infrastructure and Transport (MOLIT) of South Korea for training and education. It provides specialized training environments for the A321, B737-MAX, and B737-800NG aircraft, featuring over 80 detailed modules—including procedures for engine removal, main landing gear installation, and more. This subscription-based simulator is fully compatible with smartphones, tablets, and wearable XR devices, enabling seamless access through a cloud-based web service. Users can train anytime, anywhere—perfect for both remote learning and remote maintenance scenarios. Compared to traditional classroom learning, the XR platform is 4 times more effective and requires only one-third the training time. It also improves user confidence in real-world technical applications by up to 275%. By transforming traditional paper manuals into immersive, interactive training environments, the simulator delivers the next generation of aircraft MRO education for both civil and defense sectors.

CATIS™ is an ultra-high-resolution, small satellite imaging radar device independently developed by Lumir. It consists of three components: the radar signal transmission/reception device SCEU, an active phased array antenna SATA, and a data downlink antenna KaPA. This X-band imaging radar device is designed for small satellites weighing 150 kg, offering an ultra-high resolution of 0.3 m. It transmits wideband RF signals to the observation area while orbiting at an altitude of 500 km and receives the reflected signals to acquire Earth observation data.