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<ri:Resource created="2023-11-06T08:19:24Z" status="active" updated="2026-03-03T20:03:43Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>X-ray active galactic nucleus at z~0.4</title><shortName>J/MNRAS/498/4095</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/498/4095</identifier><altIdentifier>doi:10.26093/cds/vizier.74984095</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Noordeh E.</name></creator><creator><name>Canning R.E.A.</name></creator><creator><name>King A.</name></creator><creator><name>Allen S.W.</name></creator><creator><name>Mantz A.</name></creator><creator><name>Morris R.G.,Ehlert S.</name></creator><creator><name>von der Linden A.</name></creator><creator><name>Brandt W.N.</name></creator><creator><name>Luo B.</name></creator><creator><name>Xue Y.Q.</name></creator><creator><name>Kelly P.</name></creator><date role="Updated">2026-03-03T20:03:43Z</date><date role="Created">2023-11-06T08:19:24Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>galaxy-clusters</subject><subject>active-galactic-nuclei</subject><subject>x-ray-sources</subject><subject>redshifted</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><description>We present an analysis of the X-ray active galactic nucleus (AGN) population in a sample of seven massive galaxy clusters in the redshift range 0.35&lt;z&lt;0.45. We utilize high-quality Chandra X-ray imaging to robustly identify AGN and precisely determine cluster masses and centroids. Follow-up VIsible Multi-Object Spectrograph optical spectroscopy allows us to determine which AGN are cluster members. Studying the subset of AGN with 0.5-8keV luminosities &gt;6.8x10^42^erg/s, within r~&lt;2r_500_ (approximately the virial radius), we find that the cluster AGN space density scales with cluster mass as ~M^(-2.0+0.8-0.9)^. This result rules out zero mass dependence of the cluster X-ray AGN space density at the 2.5{sigma} level. We compare our cluster X-ray AGN sample to a control field with identical selection and find that the cluster AGN fraction is significantly suppressed relative to the field when considering the brightest galaxies with V&lt;21.5. For fainter galaxies, this difference is not present. Comparing the X-ray hardness ratios of cluster member AGN to those in the control field, we find no evidence for enhanced X-ray obscuration of cluster member AGN. 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