A quadratic parametrization of dust-scattered UV light, fitted to GALEX data at the North Galactic Pole, yields an isotropic background of 267 ± 7 photon units and is consistent with the Astrodust dust model.
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Modeling the Cosmic Ultraviolet Background at the North Galactic Pole
A quadratic parametrization of dust-scattered UV light, fitted to GALEX data at the North Galactic Pole, yields an isotropic background of 267 ± 7 photon units and is consistent with the Astrodust dust model.