2020
DOI: 10.1016/j.jqsrt.2020.107162
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Introducing the dark sky unit for multi-spectral measurement of the night sky quality with commercial digital cameras

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Cited by 35 publications
(51 citation statements)
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“…The SQM is designed to measure at the zenith and should be used with care in the context of biological studies (Longcore et al ., 2020). There are attempts to establish more intuitive units for the night sky brightness like the ‘natural sky unit’ and the ‘dark sky unit’ (see Kolláth et al ., 2020), but so far none of them has been standardised.…”
Section: Brief Overview Of Light Measurement Basicsmentioning
confidence: 99%
“…The SQM is designed to measure at the zenith and should be used with care in the context of biological studies (Longcore et al ., 2020). There are attempts to establish more intuitive units for the night sky brightness like the ‘natural sky unit’ and the ‘dark sky unit’ (see Kolláth et al ., 2020), but so far none of them has been standardised.…”
Section: Brief Overview Of Light Measurement Basicsmentioning
confidence: 99%
“…Unfortunately, some of these metrics were not well defined, and most of them did not follow the requirements of SI traceability. To eliminate these problems, Kolláth et al (2020) provided a recommendation for a new unit. The definition is based on spectroradiometry, and it can be directly applied for digital camera measurements.…”
Section: Evaluation Of the Measurementsmentioning
confidence: 99%
“…This drawback can be solved without changing our device if we rotate the camera by 90 degrees and take two or multiple fish-eye images in the vertical plane [ 22 ]. The best way to achieve the highest precision and resolution at dark locations and under clear sky conditions is to use a robotic panorama head with a 24 mm or 35 mm rectilinear lens on a full-frame digital camera [ 23 ]. With this set-up, 28 individual images are enough to cover the whole sky and some of the ground and environment with high spatial resolution.…”
Section: Introductionmentioning
confidence: 99%
“…Because of the short exposure time, the movement artefacts (like star trails) caused by the apparent rotation of the sky do not disturb the measurement. Astrometry-based corrections of the images can also be made during post-processing [ 23 ].…”
Section: Introductionmentioning
confidence: 99%
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