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<ri:Resource created="2017-08-22T14:56:49Z" 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>Circumgalactic medium surrounding z~2 quasars</title><shortName>J/ApJ/796/140</shortName><identifier>ivo://CDS.VizieR/J/ApJ/796/140</identifier><altIdentifier>doi:10.26093/cds/vizier.17960140</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Prochaska J.X.</name></creator><creator><name>Lau M.W.</name></creator><creator><name>Hennawi J.F.</name></creator><date role="Updated">2017-09-18T13:01:36Z</date><date role="Created">2017-08-22T14:56:49Z</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>galaxy-clusters</subject><subject>redshifted</subject><subject>line-intensities</subject><description>We survey the incidence and absorption strength of the metal-line transitions C II 1334 and C IV 1548 from the circumgalactic medium (CGM) surrounding z~2 quasars, which act as signposts for massive dark matter halos M_halo_~10^12.5^ M_{sun}_. On scales of the virial radius (r_vir_~160 kpc), we measure a high covering fraction f_C_=0.73+/-0.10 to strong C II 1334 absorption (rest equivalent width W_1334_&gt;=0.2 {AA}), implying a massive reservoir of cool (T~10^4^ K) metal enriched gas. We conservatively estimate a metal mass exceeding 10^8^ M_{sun}_. We propose that these metals trace enrichment of the incipient intragroup/intracluster medium that these halos eventually inhabit. This cool CGM around quasars is the pinnacle among galaxies observed at all epochs, as regards covering the fraction and average equivalent width of H I Ly{alpha} and low-ion metal absorption. We argue that the properties of this cool CGM primarily reflect the halo mass, and that other factors such as feedback, star-formation rate, and accretion from the intergalactic medium are secondary. We further estimate that the CGM of massive, z~2 galaxies accounts for the majority of strong Mg II absorption along random quasar sightlines. Last, we detect an excess of strong C IV 1548 absorption (W_1548_&gt;=0.3 {AA}) over random incidence to the 1 Mpc physical impact parameter and measure the quasar-C IV cross-correlation function: {zeta}_CIV_-Q(r)=(r/r_0_)^-{gamma}^ with r_0_=7.5_-1.4_^+2.8^ h^-1^ Mpc and {gamma}=1.7_-0.2_^+0.1^. Consistent with previous work on larger scales, we infer that this highly ionized C IV gas traces massive (10^12^ M_{sun}_) halos.</description><source format="bibcode">2014ApJ...796..140P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/796/140</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/VII/69">VII/69 : Asiago Catalogue of QSOs (Barbieri+ 1983)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/241">VII/241 : The 2dF QSO Redshift Survey (Croom+ 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/1">J/AJ/131/1 : Binary quasars in the SDSS (Hennawi+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/2222">J/AJ/133/2222 : Clustering of high-redshift QSOs from SDSS (Shen+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/401/2715">J/MNRAS/401/2715 : CIV column densities in z&lt;2.5 QSOs (D'odorico+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/762/L19">J/ApJ/762/L19 : Quasar pairs spectroscopy (Prochaska+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/776/136">J/ApJ/776/136 : QPQ VI. 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