The Discover-It-Yourself UV-Visible platform provides a range of wavelengths and performance to get measurements up and running quickly. No matter where you start, DIY will help you find answers fast.
Find the right configuration with our pre-optimized tiers of spectrometers for UV-Vis measurements. The spectrometers are all designed with important parameters, such as Stray Light and Quantum Efficiency, to ensure value from entry-level visible-only systems to high-performance UV-visible systems.
| Spectrometer Options | Quest® | Glacier® | Exemplar® |
| Application | VIS/NIR | UV/VIS | UV/VIS/NIR |
| Slit Size / Resolution | 25um / ~1.5 nm FWHM | 25um / ~1.2 nm FWHM | 25um / ~1.8 nm FWHM |
| Coverage Range | 350 nm to 1050 nm | 200 nm to 800 nm | 190 nm to 1100 nm |
| Detector Type | 2048-element Front Illuminated Linear CCD Array | 2048-element TE Cooled Front Illuminated Linear CCD Array | 2048-element High Quantum Efficiency Back-Thinned CCD Array |
| Thermoelectric Cooling | n/a | 14° C | 0 °C |
| Lamp + Lifetime | Tungsten-Halogen > 10,000 hrs | Deterium > 1,000 hrs Tungsten > 2,000 hrs |
Deterium > 1,000 hrs Tungsten > 2,000 hrs |
| Light Source Coverage | 350 to 1100 nm | 200 to 1100 nm | 200 to 1100 nm |
| Lamp Shutter | n/a | Built-In | Built-In |
