2018
DOI: 10.1016/j.jqsrt.2018.05.012
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The effect of the spectral response of measurement instruments in the assessment of night sky brightness

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Cited by 8 publications
(4 citation statements)
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“…Due to the transition towards solid-state lighting with LEDs, it is difficult to judge whether a site has become brighter or not 50 when devices are used that are not matching photometric visual band such as the SQM (see the comprehensive discussion on this topic by Sanchez de Miguel et al . 51 or recent work by Bouroussis 52 ) or even nighttime satellites, as the DMSP and VIIRS sensors lack sensitivity at short visible wavelengths 5,53 .…”
Section: Summary and Discussionmentioning
confidence: 99%
“…Due to the transition towards solid-state lighting with LEDs, it is difficult to judge whether a site has become brighter or not 50 when devices are used that are not matching photometric visual band such as the SQM (see the comprehensive discussion on this topic by Sanchez de Miguel et al . 51 or recent work by Bouroussis 52 ) or even nighttime satellites, as the DMSP and VIIRS sensors lack sensitivity at short visible wavelengths 5,53 .…”
Section: Summary and Discussionmentioning
confidence: 99%
“…A further source of error is the different spectral sensitivity of the instruments [41]. The VIIRS/DNB sensor lacks sensitivity for short wavelength radiation, and the SQM and the DSLR spectral bands have also a mismatch to each other and to the photometric band.…”
Section: Deviation Between Measurements and Modeled Nsb From Nwamentioning
confidence: 99%
“…A.20) during the overcast night would have been difficult to interpret with SQM measurements. Furthermore, the SQM itself has several drawbacks that have been discussed in earlier work [41,24].…”
Section: Comparison With Existing Workmentioning
confidence: 99%
“…Such measurements are not easily obtained in the field with single-channel devices, much less those intended to operate autonomously. Furthermore, panchromatic imagery is preferable to luminance measurements in restricted passbands, presuming that the spectrum of the night sky will continue to change in the future [ 122 ]. In order to make future comparisons of like with like, the spectral response characteristics of detectors should be standardized to the greatest extent possible.…”
Section: Future Prospectsmentioning
confidence: 99%