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<ri:Resource created="2020-08-10T09:19:52Z" 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>SDSS &amp; MMT obs. of extremely massive QSOs &amp; gal.</title><shortName>J/ApJ/871/57</shortName><identifier>ivo://CDS.VizieR/J/ApJ/871/57</identifier><altIdentifier>doi:10.26093/cds/vizier.18710057</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Yoon Y.</name></creator><creator><name>Im M.</name></creator><creator><name>Hyun M.</name></creator><creator><name>David Jun H.</name></creator><creator><name>Hwang N.</name></creator><creator><name>Kim M.</name></creator><creator><name>Park B.-G.</name></creator><date role="Updated">2021-07-09T07:52:49Z</date><date role="Created">2020-08-10T09:19:52Z</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>quasars</subject><subject>galaxies</subject><subject>spectroscopy</subject><subject>redshifted</subject><subject>visible-astronomy</subject><subject>sloan-photometry</subject><subject>black-holes</subject><description>Black hole mass scaling relations suggest that extremely massive black holes (EMBHs) with M_BH_&gt;~10^9.4^M_{sun}_ are found in the most massive galaxies with M_star_&gt;~10^11.6^M_{sun}_, which are commonly found in dense environments, like galaxy clusters. Therefore, one can expect that there is a close connection between active EMBHs and dense environments. Here, we study the environments of 9461 galaxies and 2943 quasars at 0.24&lt;~z&lt;~0.40, among which 52 are extremely massive quasars with log(M_BH_/M_{sun}_)&gt;=~9.4, using Sloan Digital Sky Survey and MMT Hectospec data. We find that, on average, both massive quasars and massive galaxies reside in environments more than ~2 times as dense as those of their less massive counterparts with log(M_BH_/M_{sun}_)&lt;~9.0. However, massive quasars reside in environments about ~2 times less dense than inactive galaxies with log(M_BH_/M_{sun}_)&gt;=9.4, and only about one third of massive quasars are found in galaxy clusters, while about two thirds of massive galaxies reside in such clusters. This indicates that massive galaxies are a much better signpost for galaxy clusters than massive quasars. The prevalence of massive quasars in moderate to low density environments is puzzling, considering that several simulation results show that these quasars appear to prefer dense environments. Several possible reasons for this discrepancy are discussed, although further investigation is needed to obtain a definite explanation.</description><source format="bibcode">2019ApJ...871...57Y</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/871/57</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/294">II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/147">V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/1720">J/AJ/126/1720 : ugriz and H{alpha} of double-peaked AGN (Strateva+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/654/115">J/ApJ/654/115 : DEEP2 Galaxy Redshift Survey: SDSS QSOs (Coil+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/662/808">J/ApJ/662/808 : Cusp radius in luminous elliptical galaxies (Lauer+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/678/635">J/ApJ/678/635 : Spectroscopy of quasar binary candidates (Myers+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/690/20">J/ApJ/690/20 : Models of the AGN &amp; black hole populations (Shankar+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/708/137">J/ApJ/708/137 : Broad-line AGNs in zCOSMOS survey (Merloni+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/194/45">J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/196/11">J/ApJS/196/11 : Bulge+disk decompositions of SDSS galaxies (Simard+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/734/68">J/ApJ/734/68 : High redshift galaxy clusters in deep fields (Wen+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/200/8">J/ApJS/200/8 : AGES: the AGN and Galaxy Evolution Survey (Kochanek+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/753/125">J/ApJ/753/125 : NIR spectrosc. follow-up of 60 SDSS-DR7 QSOs (Shen+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/199/34">J/ApJS/199/34 : Clusters of galaxies in SDSS-III (Wen+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/436/34">J/MNRAS/436/34 : GALEX Arecibo SDSS survey. 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