GALAXY CLUSTERS IN THESWIFT/BAT ERA. II. 10 MORE CLUSTERS DETECTED ABOVE 15 keV

We report on the discovery of 10 additional galaxy clusters detected in the ongoing Swift /Burst Alert Telescope (BAT) all-sky survey. Among the newly BAT-discovered clusters there are Bullet, A85, Norma, and PKS 0745-19. Norma is the only cluster, among those presented here, which is resolved by BAT. For all the clusters, we perform a detailed spectral analysis using XMM-Newton and Swift /BAT data to investigate the presence of a hard (non-thermal) X-ray excess. We find that in most cases the clusters' emission in the 0.3–200 keV band can be explained by a multi-temperature thermal model confirming our previous results. For two clusters (Bullet and A3667), we find evidence for the presence of a hard X-ray excess. In the case of the Bullet cluster, our analysis confirms the presence of a non-thermal, power-law-like, component with a 20–100 keV flux of 3.4 × 10 −12 erg cm −2 s −1 as detected in previous studies. For A3667, the excess emission can be successfully modeled as a hot component ( kT ∼ 13 keV). We thus conclude that the hard X-ray emission from galaxy clusters (except the Bullet) has most likely a thermal origin.