Covering ultraviolet, visible, and near-infrared spectral ranges

Low dark noise, high signal-to-noise ratio, high dynamic range

High frame rate, multiple integration methods

Hamamatsu cooling-type Detectors, with peak quantum efficiency of 95%

Low noise, high signal-to-noise ratio, high resolution

Long integration time, adapted for weak optical signal detection

Covers UV, visible, and near-infrared spectral ranges

Area-array back-illuminated CCD detectors, with UV Quantum Efficiency peak >70%

High signal-to-noise ratio, high dynamic range, suitable for weak-light detection scenarios such as fluorescence/Raman

Resolution up to 0.15nm

Multiple detection channels available

High linearity correction

Cooled linear array InGaAs detectors

900~2500 nm wide spectral coverage, multiple band options available

Millisecond-level spectral acquisition, significantly improving testing efficiency