Collect more light. Keep more light.


Detect more light. This may sound simple, but it’s the driving force behind all we do – because it makes for good spectroscopy. Starting with our own proprietary volume holographic phase (VPH) grating, we design low f-number spectrometers and systems that maximize efficiency at every step.


> Higher sensitivity > Faster acquisition rates > Lower limit of detection


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KEYNOTE SPEAKER: Prof Lene Broeng Oddershede, University of Copenhagen


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