Environmental dependence of AGN activity in the supercluster A901/2
R. Gilmour, M. E. Gray, O. Almaini, P. Best, C. Wolf, K. Meisenheimer,, C.Papovich, and E. Bell

TL;DR
This study investigates how the environment within a supercluster influences the activity of active galactic nuclei (AGN), revealing that AGN prevalence varies with local galaxy density and environment type.
Contribution
It provides the first detailed analysis of AGN distribution in the supercluster A901/2 using multi-wavelength data, highlighting environmental dependence of AGN activity.
Findings
AGN are predominantly found in moderate-density environments.
No AGN detected in the highest or lowest density regions.
AGN host galaxies are often in blue, less dense areas, except near cluster centers.
Abstract
We present XMM data for the supercluster A901/2, at z ~ 0.17, which is combined with deep imaging and 17-band photometric redshifts (from the COMBO-17 survey), 2dF spectra and Spitzer 24um data, to identify AGN in the supercluster. The 90ksec XMM image contains 139 point sources, of which 11 are identified as supercluster AGN with L_X(0.5-7.5keV) > 1.7x10^41 erg/cm2/s. The host galaxies have M_R < -20 and only 2 of 8 sources with spectra could have been identified as AGN by the detected optical emission lines. Using a large sample of 795 supercluster galaxies we define control samples of massive galaxies with no detected AGN. The local environments of the AGN and control samples differ at >98 per cent significance. The AGN host galaxies lie predominantly in areas of moderate projected galaxy density and with more local blue galaxies than the control sample, with the exception of one…
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