There are 15 “optically black” pixels on StellarNet detectors that are not hit by light during an acquisition. They provide a continuous measurement of the average dark spectrum and can be used to adjust for baseline drift during an experiment. In other words, this feature compensates for changes in the baseline due to temperature.
Introducing our new Applied Spectroscopy Division
New Handheld Raman!
New! ChemWiz-ADK Handheld NIR Spectrophotometer with on board chemometrics and spectral matching!
Read More
Check out our SpectroChemistry Systems for UV-VIS and Fluorescence Applications
Learn More
New Spectrometer Python Application Driver
for Windows, Linux, RasPi, Mac
Check it out!
HYPER-Nova Highest Performance Raman Spectrometer
Learn More
