On the Relation between the Astronomical and Visual Photometric Systems in Specifying the Brightness of the Night Sky for Mesopically Adapted Observers

References

• Alamús R, Bará S, Corbera J, Escofet J, Palà V, Pipia L, Tardà A. 2017. Ground-based hyperspectral analysis of the urban nightscape. ISPRS J Photogramm Remote Sens. 124:16–26.
   Web of Science ®Google Scholar
• Allen CW. 1973. Astrophysical quantities. 3rd ed. London (UK): Athlone Press.
   Google Scholar
• Aubé M. 2008. Light pollution modelling and detection in a heterogeneous environment. In: Marín C, Jafari J, editors. StarLight: a common heritage; StarLight Initiative La Palma Biosphere Reserve, Instituto De Astrofísica De Canarias, Government of The Canary Islands, Spanish Ministry of The Environment. Canary Islands (Spain): UNESCO-MaB; p. 351–358.
   Google Scholar
• Bará S. 2017. Variations on a classical theme: on the formal relationship between magnitudes per square arcsecond and luminance. Int J Sustainable Light IJSL. 19(2):104–111.
   Google Scholar
• Bará S. 2019. Black-body luminance and magnitudes per square arcsecond in the Johnson-Cousins BVR photometric bands. Photonics Lett Pol. 11(3):63–65.
   Web of Science ®Google Scholar
• Bará S, Aubé M, Barentine J, Zamorano J. 2020. Magnitude to luminance conversions and visual brightness of the night sky. Mon Not R Astron Soc. 493:2429–2437.
   Web of Science ®Google Scholar
• Bará S, Rigueiro I, Lima RC. 2019. Monitoring transition: expected night sky brightness trends in different photometric bands. J Quant Spectrosc Radiat Transf. 239:106644.
   Web of Science ®Google Scholar
• Bessell MS. 1990. UBVRI passbands. Publ Astron Soc Pac. 102:1181–1199.
   Web of Science ®Google Scholar
• Bessell MS. 2005. Standard photometric systems. Annu Rev Astron Astrophys. 43:293–336.
   Web of Science ®Google Scholar
• Blundell E, Schaffer V, Moyle BD. 2020. Dark sky tourism and the sustainability of regional tourism destinations. Tourism Recreation Res. 45(4):549–556.
   Web of Science ®Google Scholar
• Brown P. 1998. Recent visual observations of the leonid meteor shower. In: Andersen J, editor. Highlights of astronomy. Vol. I IB. Germany, Heidelberg: Springer; p. 1013–1014.
   Google Scholar
• Brown P. 1999. The leonid meteor shower: historical visual observations. Icarus. 138:287–308.
   Web of Science ®Google Scholar
• [CIE] Commision Internationale de l’Éclairage. 1990. CIE 1988 2° spectral luminous efficiency function for photopic vision. CIE. 86:1990.
   Google Scholar
• [CIE] Commission Internationale de l’Éclairage. 2010. Recommended system for mesopic photometry based on visual performance. CIE. 191:2010.
   Google Scholar
• Cinzano P, Falchi F, Elvidge CD. 2001. Naked-eye star visibility and limiting magnitude mapped from DMSP-OLS satellite data. Mon Not R Astron Soc. 323:34–46.
   Web of Science ®Google Scholar
• Cinzano P, Falchi F. 2020. Toward an atlas of the number of visible stars. J Quant Spectrosc Radiat Transf. 253:107059.
   Web of Science ®Google Scholar
• Evans DW, Riello M, De Angeli F, Carrasco JM, (+ 42 coauthors). 2018. Gaia data release 2 - photometric content and validation. A&A. 616:A4. doi:10.1051/0004-6361/201832756.
   Web of Science ®Google Scholar
• Falchi F, Cinzano P, Duriscoe D, Kyba CCM, Elvidge CD, Baugh K, Portnov BA, Rybnikova NA, Furgoni R. 2016. The new world atlas of artificial night sky brightness. Sci Adv. 2:e1600377.
   PubMed Web of Science ®Google Scholar
• Fryc I, Bisegna F, Tabaka P. 2017. Lighting of recreation grounds as a source of sky glow-the influence of luminaire type on this phenomenon. 2017 IEEE International Conference on Environment and Electrical Engineering and 2017 IEEE Industrial and Commercial Power Systems Europe (EEEIC/I&CPS Europe); Milan. doi: 10.1109/EEEIC.2017.7977724.
   Google Scholar
• Fukugita M, Ichikawa T, Gunn JE, Doi M, Shimasaku K, Schneider DP. 1996. The sloan digital sky survey photometric system. Astron J. 111(4):1748–1756.
   Web of Science ®Google Scholar
• Gălăţanu CD, Gherasim I, Beu D, Lucache DD. 2018. Luminance Field of the Façades: from aggressive to attractive lighting. 2018 IEEE International Conference on Environment and Electrical Engineering and 2018 IEEE Industrial and Commercial Power Systems Europe (EEEIC/I&CPS Europe); Palermo. p. 1–5. doi: 10.1109/EEEIC.2018.8494624.
   Google Scholar
• Gronkowski P, Tralle I, Wesołowski M. 2017. Visibility of comets during their outbursts and the night sky light pollution—use the bortle scale. Astron Nachr /AN. doi:10.1002/asna.201713387
   Google Scholar
• Hayakawa H, Mitsuma Y, Ebihara Y, Miyake F. 2019. The earliest candidates of auroral observations in Assyrian astrological reports: insights on solar activity around 660 BCE. Astrophys J Lett. 884:L18.
   Web of Science ®Google Scholar
• Hayakawa H, Tamazawa H, Ebihara Y, Miyahara H, Kawamura AD, Aoyama T, Isobe H. 2017. Records of sunspots and aurora candidates in the Chinese official histories of the Yuán and Míng dynasties during 1261–1644. Publ Astron Soc Japan. 69(4):65.
   Google Scholar
• [IDA] International Dark-Sky Association. 2020. International dark sky places conservation program. https://www.darksky.org/our-work/conservation/idsp/.
   Google Scholar
• Johnson HL. 1965. The absolute calibration of the Arizona photometry. Commun Lunar Planet Lab. 3(1):73–77.
   Google Scholar
• Jordi C, Gebran M, Carrasco JM, de Bruijne J, Voss H, Fabricius C, Knude J, Vallenari A, Kohley R, Mora A. 2010. Gaia broad band photometry. A&A. 523:A48.
   Web of Science ®Google Scholar
• Kyba CCM, Wagner JM, Kuechly HU, Walker CE, Elvidge CD, Falchi F, Ruhtz T, Fischer J, Hölker F. 2013. Citizen science provides valuable data for monitoring global night sky luminance. Sci Rep. 31835. doi:10.1038/srep01835
   Google Scholar
• Lee JS, Sul SH. 2017. Media Façade and the design identity of buildings based on visual density. Int J Asia Digital Art Design Assoc. 21(1):49–55.
   Google Scholar
• Maksimainen M, Kurkela M, Bhusa P, Hyyppä H. 2019. Calculation of mesopic luminance using per pixel S/P ratios measured with digital imaging. Leukos. 15(4):309–317.
   Web of Science ®Google Scholar
• Marín C, Jafari J. 2008. StarLight: a common heritage; StarLight Initiative La Palma Biosphere Reserve, Instituto De Astrofísica De Canarias, Government of The Canary Islands. Canary Islands (Spain): Spanish Ministry of The Environment, UNESCO-MaB.
   Google Scholar
• Masana E, Carrasco JM, Bará S, Ribas SJ. 2021. A multi-band map of the natural night sky brightness including Gaia and Hipparcos integrated starlight. Mon Not R Astron Soc. 501:5443–5456.
   Web of Science ®Google Scholar
• Mitchell D, Gallaway T. 2019. Dark sky tourism: economic impacts on the Colorado Plateau Economy, USA. Tourism Rev. 74(4):930–942.
   Web of Science ®Google Scholar
• Oke JB. 1974. Absolute spectral energy distributions for white dwarfs. Astron J Suppl Ser. 236(27):21–35.
   Google Scholar
• Pogson N. 1856. Magnitude of 36 of the minor planets. Mon Not R Astron Soc. 17:12.
   Google Scholar
• Rendtel J, Brown P. 1997. Visual observations of the Perseid meteor shower 1988-1994. Planet Space Sci. 45(5):585–593.
   Web of Science ®Google Scholar
• Rieke GH, Blaylock M, Decin L, Engelbracht C, Ogle P, Avrett E, Carpenter J, Cutri RM, Armus L, Gordon K, et al. 2008. Absolute physical calibration in the infrared. Astron J. 135(6):2245–2263.
   Web of Science ®Google Scholar
• Sánchez de Miguel A, Kyba CCM, Aubé M, Zamorano J, Cardiel N, Tapia C, Bennie J, Gaston KJ. 2019. Colour remote sensing of the impact of artificial light at night (I): the potential of the international space station and other DSLR-based platforms. Remote Sens Environ. 224:92–103.
   Web of Science ®Google Scholar
• Schaefer BE. 1990. Telescopic limiting magnitudes. Publ Astron Soc Pac. 102:212–229.
   Web of Science ®Google Scholar
• Schaefer BE. 1991. Glare and Celestial Visibility. Publ Astron Soc Pac. 103:645–660.
   Web of Science ®Google Scholar
• Schaefer BE. 1993. Astronomy and the Limits of Vision. Vistas in Astronomy 36:311–361. http://dx.doi.org/10.1016/0083-6656(93)90113-X
   Google Scholar
• Starlight Foundation. 2015. List of starlight tourist destinations. [accessed 2018 Sept 10]. https://fundacionstarlight.org/en/section/list-of-starlight-tourist-destinations/293.html.
   Google Scholar
• Tapia C, Sánchez de Miguel A, Zamorano J. 2017. LICA-UCM lamps spectral database 2.6. [accessed 2019 Apr 15]. http://guaix.fis.ucm.es/lamps_spectra.
   Google Scholar
• Upgren AR. 1991. Night-sky brightness from the visibility of stars near the horizon. Publ Astron Soc Pac. 103:1292–1295. http://articles.adsabs.harvard.edu//full/1991PASP.103.1292U/0001292.000.html
   Web of Science ®Google Scholar
• Weaver D. 2011. Celestial ecotourism: new horizons in nature-based tourism. J Ecotourism. 10(1):38–45.
   Google Scholar
• Yendell PS. 1905. On the observation of variable stars. I. The argelander method. Popular Astron. 13:453–460.
   Google Scholar