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<ri:Resource created="2023-02-28T07:59:56Z" status="active" updated="2025-06-13T15:25:00Z" 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>Galaxy Environment of Extremely Massive Quasars. I.</title><shortName>J/ApJ/920/74</shortName><identifier>ivo://CDS.VizieR/J/ApJ/920/74</identifier><altIdentifier>doi:10.26093/cds/vizier.19200074</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Jun H.D.</name></creator><creator><name>Im M.</name></creator><creator><name>Hyun M.</name></creator><creator><name>Yoon Y.</name></creator><creator><name>Eisenhardt P.R.M.</name></creator><creator><name>Hong J.</name></creator><creator><name>Jeon Y.,Kim D.,Kim J.-W.,Kim Ji H.,Park C.</name></creator><date role="Updated">2023-05-26T09:10:58Z</date><date role="Created">2023-02-28T07:59:56Z</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>quasars</subject><subject>black-holes</subject><subject>infrared-photometry</subject><description>We measure a strong excess in the galaxy number density around PG1630+377, an extremely massive (MBH~109.7M{sun}) quasar at z=1.475, using near-infrared narrowband imaging. We identify 79 narrow H-band excess objects in a 525arcmin^2^ area including the vicinity and surroundings of the quasar. These sources are likely H{alpha} line emitting, star-forming galaxies at z~1.47. We detect a {delta}=6.6{+/-}2.7 overdensity of narrow H-band excess objects located at a projected distance ~2.1Mpc northeast of the quasar, which is the densest region in the target area. The overdensity is present in BzK color-selected galaxies, while a previously reported overdensity in the immediate vicinity of PG1630+377 is not, and yet appears as a group-like structure. These megaparsec-scale environments are estimated to merge into a ~1014.7M{sun} cluster at present. Our results support the view that extremely massive black holes form and grow in group-scale environments and later incorporate into a galaxy cluster.</description><source format="bibcode">2021ApJ...920...74J</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/920/74</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/II/207">II/207 : Palomar-Green catalog UV-excess stellar objects (Green+ 1986)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/289">VII/289 : SDSS quasar catalog, sixteenth data release (DR16Q) (Lyke+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/162/1">J/ApJS/162/1 : MUSYC; optical source catalog (Gawiser+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/1275">J/AJ/132/1275 : CIRS (Cluster Infall Regions in the SDSS). 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