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<ri:Resource created="2020-09-14T10:55:32Z" 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>X-ray sources in the USS 1558-003 protocluster</title><shortName>J/ApJ/874/54</shortName><identifier>ivo://CDS.VizieR/J/ApJ/874/54</identifier><altIdentifier>doi:10.26093/cds/vizier.18740054</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Macuga M.</name></creator><creator><name>Martini P.</name></creator><creator><name>Miller E.D.</name></creator><creator><name>Brodwin M.</name></creator><creator><name>Hayashi M.</name></creator><creator><name>Kodama T.,Koyama Y.</name></creator><creator><name>Overzier R.A.</name></creator><creator><name>Shimakawa R.</name></creator><creator><name>Tadaki K.-I.</name></creator><creator><name>Tanaka I.</name></creator><date role="Updated">2021-03-23T12:33:03Z</date><date role="Created">2020-09-14T10:55:32Z</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>active-galactic-nuclei</subject><description>The incidence of active galactic nuclei (AGNs) within the local environment is a potentially valuable probe of the mechanisms that trigger and provide fuel for accretion onto supermassive black holes. While the correlation between AGN fraction and environment has been well-studied in the local universe, AGN fractions have been measured for relatively few dense environments at high redshift. In this paper, we present a measurement of the X-ray AGN fraction in the USS 1558-003 protocluster associated with the z=2.53 radio galaxy 4C-00.62. Our measurement is based on a 100-ks Chandra observation, follow-up spectroscopy from the Multi-Object Double Spectrograph on the Large Binocular Telescope, and broad and narrowband photometry. These data are sensitive to AGNs more luminous than L_X_&gt;2x10^43^erg/s in the rest-frame hard X-ray band (2-10keV). We have identified two X-ray AGNs at the redshift of USS 1558-003, one of which is the radio galaxy. We have determined that 2.0_-1.3_^+2.6^% of the H{alpha} emitters in the protocluster are X-ray AGNs. Unlike most other high-redshift cluster progenitors studied with similar techniques, USS1558-003 does not have a significantly higher fraction of AGNs than field galaxies at similar redshifts. This lower AGN fraction is inconsistent with the expectation that the higher gas fractions at high redshift, combined with the high galaxy densities and modest relative velocities in protoclusters, should produce higher AGN fractions.</description><source format="bibcode">2019ApJ...874...54M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/874/54</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/J/ApJ/592/728">J/ApJ/592/728 : Lyman break galaxies at redshift z~3 (Steidel+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/184/158">J/ApJS/184/158 : Chandra COSMOS survey I. (Elvis+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/701/587">J/ApJ/701/587 : Deep HST H-band survey. II. QUEST QSOs (Veilleux+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/761/114">J/ApJ/761/114 : Multi-wavelength study of clusters of gal. II. (Atlee+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/765/87">J/ApJ/765/87 : Chandra obs. of the 2QZ Cluster 1004+00 (Lehmer+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/428/1128">J/MNRAS/428/1128 : UDS/COSMOS HiZELS galaxies (Sobral+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/825/72">J/ApJ/825/72 : Follow-up study of AGNs in z&gt;1 clusters (Alberts+, 2016)</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/874/54</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/874/54</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/874/54</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/874/54</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/874/54</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/874/54</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/874/54/table1 (X-ray sources)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/874/54/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/874/54/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/874/54/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>240.322</ra><dec>-0.479</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/31332</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/874/54?format=ascii</footprint><waveband>X-ray</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/874/54/table1</name><description>X-ray sources</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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