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<ri:Resource created="2012-05-21T10:11:24Z" status="active" updated="2025-05-19T09:50:00Z" 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>AMUSE-Virgo survey. II.</title><shortName>J/ApJ/714/25</shortName><identifier>ivo://CDS.VizieR/J/ApJ/714/25</identifier><altIdentifier>doi:10.26093/cds/vizier.17140025</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gallo E.</name></creator><creator><name>Treu T.</name></creator><creator><name>Marshall P.J.</name></creator><creator><name>Woo J.-H.</name></creator><creator><name>Leipski C.</name></creator><creator><name>Antonucci R.</name></creator><date role="Updated">2017-12-15T10:56:05Z</date><date role="Created">2012-05-21T10:11:24Z</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>x-ray-sources</subject><subject>galaxy-clusters</subject><subject>galaxies</subject><subject>surveys</subject><subject>galaxy-kinematics</subject><description>We complete the census of nuclear X-ray activity in 100 early-type Virgo galaxies observed by the Chandra X-ray Telescope as part of the AMUSE-Virgo survey, down to a (3{sigma}) limiting luminosity of 3.7x10^38^erg/s over 0.5-7keV. The stellar mass distribution of the targeted sample, which is mostly composed of formally "inactive" galaxies, peaks below 10^10^M_{sun}_, a regime where the very existence of nuclear supermassive black holes (SMBHs) is debated. Out of 100 objects, 32 show a nuclear X-ray source, including 6 hybrid nuclei which also host a massive nuclear cluster as visible from archival Hubble Space Telescope images. After carefully accounting for contamination from nuclear low-mass X-ray binaries based on the shape and normalization of their X-ray luminosity function (XLF), we conclude that between 24% and 34% of the galaxies in our sample host an X-ray active SMBH (at the 95% confidence level). This sets a firm lower limit to the black hole (BH) occupation fraction in nearby bulges within a cluster environment.</description><source format="bibcode">2010ApJ...714...25G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/714/25</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/164/334">J/ApJS/164/334 : ACS Virgo Cluster Survey. VI (Ferrarese+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/600/729">J/ApJ/600/729 : Chandra LMXB in NGC 4649 (Randall+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/153/223">J/ApJS/153/223 : ACS Virgo Cluster Survey. I. (Cote+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/599/218">J/ApJ/599/218 : Chandra LMXB in NGC 4365 and NGC 4382 (Sivakoff+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/586/814">J/ApJ/586/814 : NGC 4472 Chandra/HST study (Maccarone+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/142/65">J/A+AS/142/65 : Galaxies morphology and IR photometry III. 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