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<ri:Resource created="2025-07-23T13:25:33Z" status="active" updated="2026-07-02T11:59:17Z" 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>Opt. selected close galaxy pairs with Chandra obs.</title><shortName>J/ApJ/949/49</shortName><identifier>ivo://CDS.VizieR/J/ApJ/949/49</identifier><altIdentifier>doi:10.26093/cds/vizier/ba-xn-1h</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>He L.</name></creator><creator><name>Hou M.</name></creator><creator><name>Li Z.</name></creator><creator><name>Feng S.</name></creator><creator><name>Liu X.</name></creator><date role="Updated">2026-07-02T11:59:17Z</date><date role="Created">2025-07-23T13:25:33Z</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>interacting-galaxies</subject><subject>active-galactic-nuclei</subject><subject>redshifted</subject><subject>visible-astronomy</subject><subject>x-ray-sources</subject><subject>black-holes</subject><description>High-resolution X-ray observations offer a unique tool for probing the still-elusive connection between galaxy mergers and active galactic nuclei (AGNs). We present an analysis of nuclear X-ray emission in an optically selected sample of 92 close galaxy pairs (with projected separations &lt;~20kpc and line-of-sight velocity offsets &lt;500km/s) at low redshift (\bar{z}~0.07), based on archival Chandra observations. The parent sample of galaxy pairs is constructed without imposing an optical classification of nuclear activity, thus it is largely free of selection effect for or against the presence of an AGN. Nor is this sample biased for or against gas-rich mergers. An X-ray source is detected in 70 of the 184 nuclei, giving a detection rate of 38%_-5%_^+5%^, down to a 0.5-8keV limiting luminosity of &lt;~10^40^erg/s. The detected and undetected nuclei show no systematic difference in their host galaxy properties such as galaxy morphology, stellar mass, and stellar velocity dispersion. When potential contamination from star formation is avoided (i.e., L_2-10keV_&gt;10^41^erg/s), the detection rate becomes 18%_-3%_^+3%^ (32/184), which shows no excess compared to the X-ray detection rate of a comparison sample of optically classified single AGNs. The fraction of pairs containing dual AGN is only 2%_-2%_^+2%^. Moreover, most nuclei at the smallest projected separations probed by our sample (a few kiloparsecs) have an unexpectedly low apparent X-ray luminosity and Eddington ratio, which cannot be solely explained by circumnuclear obscuration. These findings suggest that close galaxy interaction is not a sufficient condition for triggering a high level of AGN activity.</description><source format="bibcode">2023ApJ...949...49H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/949/49</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/B/chandra">B/chandra : The Chandra Archive Log (CXC, 1999-2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/294">II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/156">V/156 : LAMOST DR7 catalogs (Luo+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/705/L76">J/ApJ/705/L76 : AGNs with double-peaked [OIII] lines (Wang+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/737/101">J/ApJ/737/101 : AGN pairs from SDSS-DR7. 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(Liu+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/746/L22">J/ApJ/746/L22 : Dual AGNs in the nearby Universe (Koss+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/419/2095">J/MNRAS/419/2095 : HMXBs in nearby galaxies (Mineo+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/764/41">J/ApJ/764/41 : X-ray binary evolution across cosmic time (Fragos+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/799/72">J/ApJ/799/72 : Binary AGNs from the VLA Stripe 82 survey (Fu+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/RAA/16.C7">J/other/RAA/16.C7 : LAMOST-SDSS galaxy pairs (Shen+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/836/99">J/ApJ/836/99 : NuSTAR serendipitous survey: 40-month cat (Lansbury+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/869/171">J/ApJ/869/171 : Chandra observations of NuSTAR sources (Tomsick+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/474/3875">J/MNRAS/474/3875 : Galaxy And Mass Assembly (GAMA): DR3 (Baldry+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/900/79">J/ApJ/900/79 : Chandra obs. of SDSS AGN pairs at z_med_~0.1 (Hou+, 2020)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/949/49</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/949/49</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/949/49</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/949/49</accessURL><mirrorURL 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