Modeling the Cosmic Ultraviolet Background at the North Galactic Pole

I explore models of the dust-scattered component of the Cosmic Ultraviolet Background (CUVB) at the North Galactic Pole (NGP) in order to develop a framework for calculating the dust-scattered light as a function of the optical depths. As expected, I find that the dust-scattered emission scales linearly with reddening up to $E(B-V)\approx 0.1$\ mag and derive a parametric model for this dependence. I have applied these models to fit the far-ultraviolet (1350–1800 Å) observations from the $\mathit{\text{Galaxy}}\mathit{\text{Evolution}}\mathit{\text{Explorer}}\mathit{\text{(GALEX)}}$ finding that the optical constants of the interstellar dust grains – albedo ($a$) and phase function asymmetry factor ($g$) – are consistent with predictions from the Astrodust model ($a=0.33$, $g=0.68$). I detect an isotropic offset of $267\pm 7$ ph cm${}^{-2}$ s${}^{-1}$ sr${}^{-1}$ Å${}^{-1}$, half of which remains unaccounted for by known Galactic or extragalactic sources. I will now extend my analysis to wider sky regions with the goal of generating high-resolution extinction maps.