May 25, 2017 | Detectors, Glossary of Spectroscopy Terms
Shot noise is a type of electronic noise that happens because electrons and photons are discrete particles. It arises in situations where the measurement involves counting events. In spectroscopy experiments, the event is a photon generating an electron. This process...
May 25, 2017 | Glossary of Spectroscopy Terms, Spectroscopy
The signal to noise ratio, often abbreviated S/N, is exactly what it sounds like; it’s the ratio of the magnitude of the signal to the magnitude of the noise. Experiments need a large S/N to be able to distinguish features in the signal from the noise. If the S/N is...
May 25, 2017 | Detectors, Glossary of Spectroscopy Terms
Dark noise is the noise associated with the dark current. It is a type of shot noise where the event is a thermally generated electron. If the dark current generates N counts on the detector, the dark noise is √N. Dark noise is indirectly dependent on temperature...
May 25, 2017 | Detectors, Glossary of Spectroscopy Terms
Noise is a collective term for sources of unwanted signal. Some noise sources introduce systematic error, and can be corrected for, such as with a dark spectrum. Other noise sources introduce random error, and can be averaged out over several acquisitions. The...
May 25, 2017 | Detectors, Glossary of Spectroscopy Terms
Spectrometer Quantum efficiency describes how many photons that hit a detector actually generate electrons. It is usually expressed as a percentage of photons. It is also wavelength dependent. StellarNet provides detector efficiency curves that display this...
May 25, 2017 | Glossary of Spectroscopy Terms, StellarNet Definition
For clarity, “Dark” will be used to indicate a SpectraWiz dark spectrum and “dark spectrum” will refer to the concept. When you acquire a Dark, the SpectraWiz software saves the spectrum and subtracts it from all subsequent spectra that are acquired. Because of this...