The extreme-ultraviolet excess emission of the Virgo and A1795 clusters: Reobservation with in situ background measurements

The Virgo and A1795 clusters of galaxies were reobserved by the Extreme Ult raviolet Explorer with in situ background measurements by pointing at small offsets. Earlier, a similar reobservational strategy applied to the cluste r A2199 revealed that the background radial profile was consistent with a f lat distribution, and therefore the original method of extracting cluster E UV signals by the subtraction of an asymptotically determined background wa s valid. It is shown here that the same conclusions hold for the current sa mple. A model of the background was obtained from its known properties and the in situ measurements, and the subtracted cluster fluxes remain in agree ment with those reported in our discovery papers. They are also consistent with results from the most conservative procedure of direct point-to-point subtraction of the in situ background and proper error propagation, which s till preserves the existence of the EUV excess and its rising radial trend. We present evidence that argues against the soft excess as due to peculiar ities in the line-of-sight Galactic absorption. The data appear to favor a thermal origin of the emission.