Mapping the Diffuse Ultraviolet Sky with GALEX

TL;DR

This paper presents a detailed map of the diffuse ultraviolet sky using GALEX data, revealing dust-scattered starlight distribution, its correlation with infrared emission, and notable features around hot stars.

Contribution

First comprehensive UV diffuse background map covering 75% of the sky using GALEX archival data, highlighting dust scattering and specific bright features.

Findings

Diffuse UV flux follows a cosecant law with specific slopes.

Strong correlation between UV background and IRAS 100 μm flux.

Identification of bright spots around hot stars like Spica and Achernar.

Abstract

We present a map of the diffuse ultraviolet cosmic background in two wavelength bands (FUV: 1530 {\AA}; NUV: 2310 {\AA}) over almost 75% of the sky using archival data from the GALEX mission. Most of the diffuse flux is due to dust-scattered starlight and follows a cosecant law with slopes of 545 photons cm-2 s-1 sr-1 {\AA}-1 and 433 photons cm-2 s-1 sr-1 {\AA}-1 in the FUV and NUV bands, respectively. There is a strong correlation with the 100 {\mu}m IRAS flux with an average UV/IR ratio of 300 photons cm-2 s-1 sr-1 {\AA}-1 (MJy sr-1)-1 in the FUV band and 220 photons cm-2 s-1 sr-1 {\AA}-1 (MJy sr-1)-1 in the NUV but with significant variations over the sky. In addition to the large scale distribution of the diffuse light, we note a number of individual features including bright spots around the hot stars Spica and Achernar.