The SQM is equipped with a silicon
photodiode functioning as detector which is partially covered by a rejection filter for the near-infrared wavelength. The system has a high response to wavelengths up to the near-infrared (from 350 nm to 2500 nm), thanks to a converter from light to frequency. This structure tries to mimic the
human eye spectral response under the photopic regime. A final spectral response is provided by the combination of the photodiode and the transmission near-infrared cut-off filter. This response overlaps the Johnson B and V bands, well known in astronomical photometry, in the wavelength range between 320 nm and 720 nm, which includes visible light spectrum. Beyond amateur astronomers, the SQM photometers have become very popular among researchers from different fields of study, including associations involved in fighting light pollution. The instrument has a systematic uncertainty which is quoted of 10% (0.1 mag arcsec−2). The aspect of uncertainty is also related to the stability of these radiometers: the variation of the instrument behaviour (mainly due to sensor ageing, the influence of the air temperature and atmospheric conditions and internal temperature) could be confused with changes of the sky brightness, especially when NSB tracking is performed over a long time interval. ==Models and Production==