Vega

    High‑performance LED illumination engineered for fast‑exposure imaging

    Vega

    Vega

    Vega

    High‑Stability DC‑Driven LED Illumination for Ultra‑Short‑Exposure Imaging

    The Vega light source is engineered for high‑precision camera measurements at extremely short exposure times, making it ideal for automotive‑grade imaging, HDR sensors, and contrast‑based performance testing. Its DC‑driven LED architecture delivers exceptionally stable illumination, ensuring repeatable CTA and CSNR results even under demanding fast‑exposure conditions.

    Vega’s direct‑current intensity regulation eliminates the instability commonly seen in PWM‑controlled systems. By carefully selecting the LEDs and maintaining a thermally consistent operating point, Vega prevents color shifting, intensity fluctuations, and other artifacts that compromise measurement accuracy. The thermal system maintains ±0.5 °C stability, supporting both heating and cooling without drift, even when switching light sources or adjusting intensity.

    To support real‑world testing scenarios, Vega provides advanced flicker generation across a wide frequency range, including sine, triangular, and square waveforms. This enables precise evaluation of camera behavior under modulated illumination, a critical requirement for modern automotive imaging systems.

    Why Vega?

    Unlike PWM‑controlled light sources, which modulate intensity by rapidly switching LEDs on and off, Vega regulates intensity through current control, enabling fine‑grained adjustment and high‑intensity output at ultra‑short exposure times. This makes Vega particularly effective for HDR automotive cameras, where illumination stability directly impacts safety‑critical performance metrics.

    For applications requiring even higher intensity and stability, explore the Arcturus light source.

    Key Benefits of Vega

    Vega is designed for high‑precision visible‑light measurements under extremely short exposure times, particularly for automotive HDR cameras.

    DC-driven LED Technology

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

    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.

    Multiple waveforms

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

    Flicker testing

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

    IEEE-2020:2024 measurements

    Measure most of the KPIs from the IEEE-2020:2024 standard, including CTA, CSNR, MMP, and dynamic range.

    Use Case

    IEEE-2020:2024 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-2020:2024 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 Specifications

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

    Vega
    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) VIS [K]
    4900 K (± 200 K)
    Color Rendering Index (CRI)
    > 95
    Minimum luminance
    0.1 – 0.5 cd/m2
    Maximum luminance [cd/m²]
    55,500 – 61,500 cd/m²
    Dim function
    Software based | 106 - 10 steps
    Flicker frequency range
    1 – 1000 Hz (Square) 10 – 1000 Hz (Sine) 10 – 1000 Hz (Triangle)
    Flicker frequency step width
    0.1 Hz (1 – 200 Hz) 0.2 Hz (200 – 500 Hz) 0.5 Hz (500 – 1000 Hz)

    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 TE294

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

    Vega IR Test charts

    Vega IR is used with grayscale test charts selected for defined behavior in the near-infrared range. Please contact our sales team to confirm the chart configuration for your wavelengths.

    Note:

    As with the Vega light sources, you can purchase charts in one-, three-, or seven-piece sets.

    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 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

    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)

    Compatible Illumination Systems

    Arcturus

    Arcturus

    Arcturus provides extreme illumination levels for challenging HDR sensors, enabling accurate CTA, CNR, and MMP testing in realistic high‑brightness scenes.

    Vega IR cube

    Vega IR (940 nm Near‑Infrared)

    Vega IR extends the Vega platform into the near‑infrared band, enabling contrast‑based KPIs for cameras operating under 940 nm illumination (DMS, OMS, RGB‑IR sensors).

    Lightcube-Controller

    Lightcube-Controller

    The Lightcube‑Controller delivers reliable power management and seamless control for all Vega and Arcturus illumination devices.