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<ri:Resource created="2014-10-22T09:15:24Z" 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>Quasar pairs spectroscopy</title><shortName>J/ApJ/762/L19</shortName><identifier>ivo://CDS.VizieR/J/ApJ/762/L19</identifier><altIdentifier>doi:10.26093/cds/vizier.17629019</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Prochaska J.X.</name></creator><creator><name>Hennawi J.F.</name></creator><creator><name>Simcoe R.A.</name></creator><date role="Updated">2017-12-15T10:56:06Z</date><date role="Created">2014-10-22T09:15:24Z</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>quasars</subject><subject>redshifted</subject><subject>line-intensities</subject><description>The hosts of luminous z~2 quasars evolve into today's massive elliptical galaxies. Current theories predict that the circumgalactic medium (CGM) of these massive, dark matter halos (M_DM_~10^12.5^M_{sun}_) should be dominated by a T~10^7^K virialized plasma. We test this hypothesis with observations of 74 close-projected quasar pairs, using spectra of the background QSO to characterize the CGM of the foreground one. Surprisingly, our measurements reveal a cool (T~10^4^K), massive (M_CGM_&gt;10^10^M_{sun}_), and metal-enriched (Z&gt;~0.1Z_{sun}_) medium extending to at least the expected virial radius (r_vir_=160kpc). Furthermore, we conservatively estimate that the quasar CGM has a 64^+6^_-7_% covering fraction of optically thick gas (N_HI_&gt;10^17.2^/cm^2^) within r_vir_; this covering factor is twice that of the contemporaneous Lyman break galaxy population. This unexpected reservoir of cool gas is rarely detected "down-the-barrel" to quasars, and hence it is likely that our background sight lines intercept gas that is shadowed from the quasar ionizing radiation by the same obscuring medium often invoked in models of active galactic nucleus unification. Because the high-z halos inhabited by quasars predate modern groups and clusters, these observations are also relevant to the formation and enrichment history of the intragroup/intracluster medium.</description><source format="bibcode">2013ApJ...762L..19P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/762/L19</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/V/139">V/139 : The SDSS Photometric Catalog, Release 9 (Adelman-McCarthy+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/755/89">J/ApJ/755/89 : Metallicities of damped Ly{alpha} systems (Rafelski+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/740/91">J/ApJ/740/91 : Ly{alpha} &amp; OVI in galaxies around quasars (Prochaska+, 2011)</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/ApJ/727/47">J/ApJ/727/47 : The MgII cross-section of red galaxies (Bowen+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/719/1672">J/ApJ/719/1672 : SDSS binary quasars at high redshift. I. (Hennawi+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/699/782">J/ApJ/699/782 : High-redshift SDSS-DR5 QSOs (Diamond-Stanic+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/182/378">J/ApJS/182/378 : HI and OVI absorbers in nearby Universe (Wakker+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/679/1144">J/ApJ/679/1144 : Galaxy clusters in LOS to background QSOs. I. 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