ECOC Exhibition 2026: Meet us in Málaga
Discover optical solutions for faster, more efficient and scalable data communication.
FYCMA, Málaga, Spain
Booth #1289
Empowering next-generation data communication
At ECOC 2026, discover our solutions for optical communication – from microoptics and PIC testing to telecommunications gratings and free-space optical communication. Discover our Highlights:Microlens Arrays for fiber coupling and collimation
Opto-electronic probe card for PIC wafer testing
Telcom-Gratings for WSS and ROADM applications
Leightweight mirrors and subassemblies for FSOC
Want to make the most of your visit? Book your slot with our team!
Enabling high data rates in free space
We deliver:
- Highest performance and reliability
- Empowering next-gen Laser Communication Terminals
- Full space-qualified compliance
Products:
- Built to print
- Built to print + (partly development)
- Built to specification (development)
Lightweight and spectral mirrors for space applications
Lightweighting technology ensures mechanical stiffness and high form accuracy at greatly reduced mass. Discover our products:- Primary Mirror for Space Telescope
- Secondary Mirror for Space Telescope
- Spectral Mirror for Spectrometer
Primary Mirror for Space Telescope
Lightweighted high-precision mirrors are critical for Earth Observation satellites, enabling larger apertures without excessive launch mass. Their optical accuracy ensures crisp, detailed imagery essential for monitoring climate change, urban expansion, and disaster response. By minimizing structural weight while maintaining stability, these mirrors allow satellites to carry more instruments, significantly enhancing our ability to observe and protect our planet effectively from space.
| Category | Value |
| Type of mirror | Asphere |
| Material | Zerodur class 0 |
| Diameter | 277 mm |
| Height | 40 mm |
| Weight | 2 kg |
| Surface Quality | <15nm RMSi |
| Coating | 1500 - 1610 nm |
| Grounding points | 6x |
| Tracking balls | ---- |
| Category | Value |
| Type of mirror | Asphere |
| Material | Zerodur class 0 |
| Diameter | 200 mm |
| Height | 37 mm |
| Weight | 1,6 kg |
| Surface Quality | <13nm RMSi |
| Coating | 430 – 950 nm |
| Grounding points | ---- |
| Tracking balls | 3x |
Secondary Mirror for Space Telescope
Unlike terrestrial telescopes, which can support massive, heavy glass mirrors, space-based instruments must launch into orbit where every kilogram of payload drastically increases launch costs and complexity. This necessity has driven the development of lightweight mirror technologies that redefine the limits of optical engineering.
| Category | Value |
| Type of mirror | Asphere |
| Material | Zerodur class 0 |
| Diameter | 204x113mm |
| Height | 43mm |
| Weight | 1.2 kg |
| Surface Quality | <28nm RMSi |
| Coating | 430 – 950nm |
| Grounding points | ---- |
| Tracking balls | 3x |
| Category | Value |
| Type of mirror | Prisma |
| Material | F2 (Schott) |
| Diameter | 80x9mm |
| Height | 7mm |
| Weight | <1 kg |
| Surface Quality | <15nm RMSi |
| Coating | 1300 – 1410nm |
| Anti reflec | Actar Foil |
