MODULAR SPECTROMETRY
Compare AstroLite Models.
Compare AstroLite models by wavelength range, detector type, optical resolution, sensitivity, and integration-time requirements.
Compare AstroLite models by wavelength range, detector type, optical resolution, sensitivity, and integration-time requirements.
Compare the available wavelength coverage of each AstroLite model at a glance.
The actual configured wavelength range and optical resolution depend on the selected grating, slit width, and optical configuration.
Compare the wavelength range, detector, and key specifications of each AstroLite model.
Compact spectrometer for VIS / VIS-NIR measurement and system integration.
Compact UV–VIS platform with higher signal handling and dynamic range.
Designed for narrow spectral features, laser measurement, and LIBS analysis.
Back-thinned CCD area sensor model for weak spectral signals, fluorescence emission, and Raman scattering.
TE-cooled back-thinned CCD area sensor model for low-noise and long-integration measurements.
Compact InGaAs spectrometer for extended near-infrared measurement.
Select the light source, fiber, probe, optical path, and spectrometer together for the required wavelength range and sample geometry.