• Ultra-Low SWaP: Very compact and high stability
• Swatch Width: 9.7 km @ 500 km
• Wide Aperture: 230 mm
• GSD: 1.03 @ 500 km; special mode at 0.7m
• Zerodur® Telescope: High resolution

• Wire-speed traffic generation and analysis
• High precision solution for chassis time synchronization
• Used for OWL measurements, synchronized traffic start and timestamping
• Can use any combination of NTP, PTP or RFC 868 TIME
• Legacy Xena testers can be retro-fitted with XenaTimeSynch (GPS requires factory refit)
• Compatible with Xena1564 (ITU-T Y.1564) test methodology

LUMIMAX® High Power LED Spot Lights are particularly compact, but at the same time extremely powerful and versatile. 

Adjustable precision optics of the LED Spot Lights allow adjustment of the radiation characteristic to the required working distances and image fields, enabling a focused or very homogeneous illumination of the object to be inspected.

LED Spot Light's filter thread allows mounting of components such as polarisation filters or bandpass filters for fluorescence applications. With the C-Mount connector, either integrated or available as an accessory, lenses for focusing can be used.

Despite their compact design, the LUMIMAX® LED Spot Lights feature an integrated lighting controller for continuous or strobe mode.

• PowerFlex design provides higher currents at lower voltages enabling one model to meet many different voltage/current requirements. 
• Compact design for bench use or rack mounting (1/2 or 1/4 rack width) 
• True analog controls with digital settings locking (S-Lock) 
• Mixed-mode regulation with linear final regulation for low noise 
• Dual models have isolated voltage tracking and synchronous on/off. 
• P models have RS-232, USB, and LXI-compliant LAN interfaces plus duplicate rear terminals. GPIB Optional.

The all new Linea HS™ delivers line rates up to an incredible 400 kHz at 32k resolution — over 13 Gpixels/sec via CLHS interface. With up to 128 TDI stages (plus an extra 64 in HDR mode) for unmatched sensitivity and incredibly low noise, Linea HS excels in the highest speed, lowest light applications.

• Reduced dark noise levels and improved dark offset 
• Improved sensitivity, including NIR response 
• In-camera image pre-processing (lens shading correction, pixel correction) 
• Large full well when using in-sensor binning >142Ke 
• Thousands of frames per second in Partial Scan Mode (ROI) 
• Multi-ROI support (up to 32 ROI) and Cycling Mode 
• Advanced Sequencer functions of different features

• 32 bit 3U CPCI module
• IRIG B, 1 PPS sync inputs
• GPS sync option (maintains single-slot)
• Have Quick sync input option
• Propagation delay correction
• Zero latency time reads
• Match Time output
• IRIG-B or IRIG-G time code output (Option)
• External Event time tags
• Three user programmable rates
• +3.3V or +5V PCI signaling levels

• Complete bias circuits
• Requires no external components
• Extremely flat output power versus frequency characteristics

The NC500 (through-hole) and NC500SM (surface mount) Series noise modules are an economical solution for built-in test requirements. They contain complete bias circuits and require no external components. Some models contain additional gain stages for high power ENR output (51 dB). The surface mount package is suitable for mounting on micro strip. The modules have extremely flat output power versus frequency characteristics that are insensitive to temperature and voltage variations.

• Designed for Harsh Environment: High Shocks, High Vibration, EMI/EMC, -50/+105 Celsius, Waterproof, Lightning
• Ultra Compact and Generic: Generic Analog Module, 2x3" / 51x76 mm, from 1 to 16 modules per stack
• Best data Ever: 1000 ppm in extreme temperature range
• Easy to Configure: eZ software Suite
• Process & Command: Preprocess Data and Program Commands to External Systems
• Multi Format Output Stream: PCM Chapter 4, PCM Chapter 7, Low latency video, UDP output