摘要：We present a study of the distribution of X-ray detected active galactic nuclei (AGN) in the five most massive,M500SZ> 1014M⊙, and distant,z ∼ 1, galaxy clusters in thePlanckand South Pole Telescope (SPT) surveys. The spatial and thermodynamic individual properties of each cluster have been defined with unprecedented accuracy at this redshift using deep X-ray observations. This is an essential property of our sample in order to precisely determine theR500Yxradius of the clusters. For our purposes, we computed the X-ray point-like source surface density in 0.5R500Yxwide annuli up to a clustercentric distance of 4R500Yx, statistically subtracting the background and accounting for the respective average density of optical galaxies. We found a significant excess of X-ray point sources between 2 and 2.5R500Yxat the 99.9% confidence level. The results clearly display for the first time strong observational evidence of AGN triggering in the outskirts of high-redshift massive clusters with such a high statistical significance. We argue that the particular conditions at this distance from the cluster centre increase the galaxy merging rate, which is probably the dominant mechanism of AGN triggering in the outskirts of massive clusters.
