Galaxy Cluster Contribution to the Diffuse Extragalactic Ultraviolet Background
Abstract
The diffuse ultraviolet background radiation has been mapped over most of the sky with 2 \ resolution using data from the GALEX survey. We utilize this map to study the correlation between the UV background and clusters of galaxies discovered via the Sunyaev-Zeldovich effect in the Planck survey. We use only high Galactic latitude (|b| > 60 ) galaxy clusters to avoid contamination by Galactic foregrounds, and we only analyze clusters with a measured redshift. This leaves us with a sample of 142 clusters over the redshift range 0.02 ≤ z ≤ 0.72, which we further subdivide into four redshift bins. In analysing our stacked samples binned by redshift, we find evidence for a central excess of UV background light compared to local backgrounds for clusters with z<0.3. We then stacked these z<0.3 clusters to find a statistically significant excess of 12 2.3 photon cm-2 s-1 sr-1 -1 \ over the median of 380 photon cm-2 s-1 sr-1 -1 \ measured around random blank fields. We measure the stacked radial profile of these clusters, and find that the excess UV radiation decays to the level of the background at a radius of 1 Mpc, roughly consistent with the maximum radial extent of the clusters. Analysis of possible physical processes contributing to the excess UV brightness indicates that non-thermal emission from relativistic electrons in the intracluster medium and faint, unresolved UV emission from cluster member galaxies and intracluster light are likely the dominant contributors.