Abstract:
We have modeled the diffuse background at the Galactic Poles in the far-ultraviolet (FUV: 1536 Å)
and the near-ultraviolet (NUV: 2316 Å). The background is well-fit using a single-scattering dustmodel with an
offset representing the extragalactic light plus any other contribution to the diffuse background.We have found
a dust albedo of 0.35–0.40 (FUV) and 0.11–0.19 in the NGP (b > 70◦) and 0.46–0.56 (FUV) and 0.31–0.33
(NUV) in the SGP (b < 70◦
). The differences in the albedo may reflect changes in the dust-to-gas ratio over
the sky or in the dust distribution. We find offsets at zero-reddening of 273–286 and 553–581 photons cm−2
s−1 sr−1 Å−1 in the FUV and NUV, respectively, in the NGP with similar values in the SGP.
