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arXiv · 1001.2246

Light pollution at high zenith angles, as measured at Cerro Tololo Inter-American Observatory

Kevin Krisciunas·Hector Bogglio·Pedro Sanhueza·Malcolm G. Smith
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Abstract

On the basis of measurements of the V-band sky brightness obtained at Cerro Tololo Inter-American Observatory in December 2006 and December 2008 we confirm the functional form of the basic model of Garstang (1989, 1991). At high zenith angles we measure an enhancement of a factor of two over Garstang's later model when there is no marine cloud layer over La Serena/Coquimbo. No corresponding enhancement is found in the B-band.

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Kevin Krisciunas, Hector Bogglio, Pedro Sanhueza, Malcolm G. Smith. 2010-01-13. Light pollution at high zenith angles, as measured at Cerro Tololo Inter-American Observatory. https://doi.org/10.1086/651246

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