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We use data from the All Wavelength Extended Groth Strip International Surveyto construct stacked X-ray maps of optically bright active galaxies (AGN) andan associated control sample of galaxies at high redshift (z less than 0.6).From our analysis of the surface brightness profiles obtained from these X-raymaps, we find evidence of feedback from the active nuclei. We find thatexcluding galaxies and AGN, residing in group environments, from our samplesenhances the significance of our detection. Our results support the tentativefindings of Chatterjee et al. who use X-ray selected AGN for their analysis. Wediscuss the implications of these results in the context of quantifying AGNfeedback and show that the current method can be used to extract X-ray sourcepopulation in high redshift galaxies.

X-ray Surface Brightness Profiles of Optically Selected Active Galactic Nuclei: Comparison with X-ray AGN