The CORTEX RTR-X1 (formerly RX-1) is a compact, dual-channel telemetry receiver with a pre-D combiner, designed to span all IRIG frequency bands and conform to IRIG-specified modulations. 

This off-the-shelf (COTS) product leverages the rock-solid CORTEX RTR technology components, inheriting their renowned RF performance and signal processing prowess. 

The RX-1 excels in test range scenarios, offering cutting-edge features to ensure maximum data accessibility. Trust the RX-1 for top-tier telemetry reception in challenging conditions.

Configuring, managing, and integrating the system are crucial steps for ensuring the success of flight testing and achieving precise telemetry. eZ Software is your go-to solution. 

• eZ SetUp software allows to configure from a single acquisition unit to a complete acquisition system within a network architecture. 
• eZ Operation software is an advanced tool for centralized supervision and control of complex test systems from an onboard operator station. 
• eZ Processing / Advantys software offers advanced functions for data display and processing.

The SPARTE 300 series antenna is a battle-tested product that has consistently delivered top-tier performance for mission-critical applications where reliable telemetry reception is paramount. This rugged antenna guarantees our customers the utmost precision, a long operational life, and straightforward maintenance.

The SPARTE 300 series opens up a world of possibilities for users, ranging from aircraft tracking and high-speed target monitoring to duplex datalinks with both receiving and transmitting capabilities.

Furthermore, the extensive and customizable input/output options empower users to operate multiple antennas in a coordinated, multi-site tracking setup. With all antennas, regardless of size, being effortlessly monitored, managed and controlled by using our TM Maestro software.

Acquire high quality images with accurate radiometry for LEO (Low Earth Observation) earth observation applications with 65 MP focal plane and control electronics. From a 500 km orbit, SEEING™ 230 Ident has 9 x 6 km2 swath, offering a 1.03m native Ground Sample Distance (GSD), and features a super-resolution optional mode providing 70cm GSD. Thanks to its unique design, SEEING™ 230 Ident has an ultra-low SWaP factor. It is made of advanced ceramic material for strength during launch and stability during operation in space. It is athermalized and gradient insensitive between -10°C to +50°C. It has a low mass, below 8kg, saving both platform and launch costs.

With its small and high ruggedized design, XMA is the best fit for remote data acquisitions in harsh and small space areas. 

It is the perfect candidate for network telemetry applications and remote acquisitions, to reduce the wire intrusiveness, and acquire the data closer to the sensors. 

XMA also allows data recording, data processing, GPS localization and data transmission. XMA has the smallest size/channel types ratio, and proposes optimized module set for a large number of data type acquisitions, with state-of-the-art accuracy. 

A complete set of status and health information of the unit is remotely available for live monitoring and accurate data qualifiers.

TM MAESTRO provides a comprehensive and centralized solution for monitoring and controlling telemetry infrastructure worldwide.

Designed to meet the critical needs of telemetry operators, this software offers a user-configurable GUI that adapts to various user profiles and mission phases, from preparation to live flight tests and station maintenance. TM MAESTRO is scalable and easily accommodates new telemetry equipment, allowing for the addition of an unlimited number of components, from antennas to decommutators, making it a highly flexible system.

The D19-GT/-GTS Download Station ensures a secure and high-speed data download (via 40 Gbit Ethernet) from MDR or MDR-GT/-GTS storage media. Specifically designed for flight testing applications with demanding data rates and storage needs, the D19-GTS, when paired with MDR-GTS, incorporates advanced cybersecurity features like Data-At-Rest (DAR) protection and firmware updates. Configuration changes are facilitated through a Removable Secure Operational Disk (RSOD).

Safran’s SEEING™ 130 Wide includes a unique medium focal length catadioptric optics, limited by diffraction only and with ultra-low distortion, offering perfect imaging over 35 mm full-frame image format. It is fitted with a 10megapixel sensor. 

SEEING™ 130 Wide enables high Signal to Noise Ratio for multispectral (MS), hyperspectral (HS) and low light level imaging. SEEING™ 130 Wide includes a spectral filter with 23 bands covering Blue, Green, Red, Near InfraRed and Red Edge MS, for a broad spectral range between 475 and 900nm. SEEING™ 130 Wide has a large Field of View of 6.3° x 4.3° / 54 x 36 km2 from a 500km/310 miles orbit.

In addition to its a thermal design within a robust structure, SEEING™ 130 Wide has a low SWaP, saving launch and operational costs.

The PPS®1350 Hall Effet plasma thruster draws on Safran’s long experience with electric propulsion. It is designed for orbital transfer, station keeping and deorbiting satellites and other spacecraft. In particular, the PPS 1350 was the primary engine on ESA’s lunar probe, Smart-1, launched in 2003 by an Ariane 5 rocket. This mission was completed in September 2006.