Vega
    Illumination

    Vega illumination

    Vega illumination

    Vega Overview

    The Vega light source provides a solution for high-precision measurements at very short exposure times, as seen in automotive-grade cameras. Vega uses LEDs driven by DC (direct current) technology, making it one of our most sophisticated and unique light sources ever developed.

    Cameras with very short exposure times often experience stability problems due to inadequate testing devices. Vega's extremely high stability provides a previously unattainable consistency for measuring these types of cameras.

    Looking for even higher intensity and stability? Check out our Arcturus light source.

    While we use DC technology for this device, we can eliminate color shifting by carefully selecting the LEDs. The DC driver does not affect temperature regulation, and we can achieve temperature stability within 0.5 degrees. The temperature system works both ways (i.e., heating and cooling) and will remain consistent even when turning on/off different light sources or changing the intensities.

    Vega also has advanced flicker capabilities and can be generated from a wider frequency range. We have also further developed the low-frequency functionality to include sine, triangular, and square waveforms, which allows us to cover nearly all real-world scenarios.

    Why Vega?

    Unlike PWM-controlled light sources, where intensity is regulated by the high frequency of switching LEDs on/off, Vega regulates intensity by the amount of current and offers very fine adjustment. These features allow the Vega to measure high intensities with extremely short exposure times. HDR cameras from the automotive sector benefit greatly from this technology as they require the highest level of performance to ensure safety.

    Key Benefits of Vega

    DC-driven LED Technology

    DC (direct current) technology does not affect temperature regulation and can achieve temperature stability within 0.5 degee.

    IEEE-2020 measurements

    Measure most of the KPIs from the IEEE-2020 standard, including CTA, CSNR, MMP, and dynamic range.

    Extremely high stability

    Vega's extremely high stability provides a very strong consistency for testing cameras with very short exposure times.

    Eliminate color shifiting

    Vega can eliminate color shifting through the meticulous selection of the LEDs.

    Flicker testing

    Vega has advanced flicker capabilities that can be generated from a wider frequency range.

    Multiple waveforms

    Advanced low-frequency functionality to include sine, triangular, and square waveforms to cover nearly all real-world scenarios.

    Technical Specifications

    SpecificationValue
    Light Source 36 Temperature controlled LEDs based on iQ-DC technology
    Uniformity (active area)> 95% at 100% output intensity | > 94% at 10% output intensity | > 90% at 1% output intensity | > 90% at 0.1% output intensity
    Illumination stability± 0,5%
    Correlated Color Temperature (CCT)4900 K (± 200 K)
    Color Rendering Index (CRI)> 95
    Minimum luminance0.1 – 0.5 cd/m2
    Maximum luminance55,500 – 61,500 cd/m²
    Dim function Software based | 106 - 10 steps
    Flicker frequency range1 – 1000 Hz (Square) | 10 – 1000 Hz (Sine) | 10 – 1000 Hz (Triangle)
    Flicker frequency step width0.1 Hz (1 – 200 Hz) | 0.2 Hz (200 – 500 Hz) | 0.5 Hz (500 – 1000 Hz)

    Documentation

    Vega Datasheet (EN)

    Technical specifications and product details

    Vega User Manual (EN)

    Complete operating instructions

    Vega Datenblatt (DE)

    Technische Spezifikationen und Produktdetails

    Vega Betriebsanleitung (DE)

    Vollständige Betriebsanleitung

    Vega Product Flyer

    A basic product overview

    Vega C API documentation (web)

    Vega C++ API documentation (web)

    Vega Python API documentation (web)

    Vega Product Video

    Use Case

    IEEE-2020 Measurements

    Vega is an ideal solution for measuring Contrast Transfer Accuracy (CTA), Modulated Light Mitigation Probability (MMP), Contrast Signal-to-Noise Ratio (CSNR), or other high-intensity measurements outlined in the IEEE-2020 standard. These factors are relevant to almost all automotive camera applications, which require test solutions capable of creating dynamic test scenes for cameras with very short exposure times.

    Product Options and Software

    We offer multiple setup options and control software
    Vega C++ API

    Vega software and APIs

    Vega is sold with control software that lets you manage up to seven devices simultaneously. APIs are also available (sold separately) to enable seamless integration into individual designs. We offer APIs in C, C++, and Python.


    VLS-Evaluation

    The evaluation software analyzes the camera's performance using the defined KPIs, including CTA, MMP, and CSNR. CTA evaluations are based on pixel-value distributions. Results are exported as XML files. This software is sold separately.

    Vega grayscale test chart

    Vega charts (TE294)

    The TE294 chart is optimized for Vega. It is a unique series of grayscale test charts for high-precision measurements, including Contrast Transfer Accuracy (CTA) and other contrast-based performance indicators. Charts are available individually or in sets. As with the Vega light source, you can purchase charts in one-, three-, or seven-piece sets.


    Please note that the TE294 charts are always sold separately from the Vega light source.

    Vega Hardware Sets

    The Vega is available in two separate hardware sets. Each set comes with a controller and control software. The controller can connect and control up to seven different Vega light sources. All of which can be programmed with the control software.

    The Vega 1+1* is sold with one Vega light source and is perfect for those looking for a simple solution for testing HDR cameras with very short exposure times.

    The Vega 3 + 1 Set* includes three Vega light sources and is a great solution for testing camera performance at varying flicker frequencies or for contrast transfer accuracy (CTA) measurements.

    In addition to the two sets listed above, we also offer individual Vega light sources as an “add-on” option for your project (an “add-on” does not come with a controller or control software).

    Please contact our sales department for a consultation if you have questions or inquiries.

    *Evaluation software not included.

    Software Downloads

    Download the latest software package for Vega.

    Vega Software (Version 1.0.0)

    Vega software (Windows 64bit installer)

    Vega APIs

    Contact our sales teams for API access

    VLS-Evaluation

    Contact our sales team for download access