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<ri:Resource created="2020-08-26T13:53:36Z" 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>The COS CGM Compendium (CCC). II. Lyman limit syst.</title><shortName>J/ApJ/872/81</shortName><identifier>ivo://CDS.VizieR/J/ApJ/872/81</identifier><altIdentifier>doi:10.26093/cds/vizier.18720081</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wotta C.B.</name></creator><creator><name>Lehner N.</name></creator><creator><name>Howk J.C.</name></creator><creator><name>O'Meara J.M.</name></creator><creator><name>Oppenheimer B.D.,Cooksey K.L.</name></creator><date role="Updated">2022-10-14T13:10:27Z</date><date role="Created">2020-08-26T13:53:36Z</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>spectroscopy</subject><subject>ultraviolet-astronomy</subject><subject>intergalactic-medium</subject><subject>chemical-abundances</subject><subject>redshifted</subject><subject>h-i-line-emission</subject><description>We present the results from our COS circumgalactic medium (CGM) compendium (CCC), a survey of the CGM at z&lt;~1 using HI-selected absorbers with 15&lt;logN_HI_&lt;19. We focus here on 82 partial Lyman limit systems (pLLSs, 16.2&lt;=logN_HI_&lt;17.2) and 29 LLSs (17.2&lt;=logN_HI_&lt;19). Using Bayesian techniques and Markov Chain Monte Carlo sampling of a grid of photoionization models, we derive the posterior probability distribution functions (PDFs) for the metallicity of each absorber in CCC. We show that the combined pLLS metallicity PDF at z&lt;~1 has two main peaks at [X/H]~-1.7 and -0.4, with a strong dip at [X/H]~-1. The metallicity PDF of the LLSs might be more complicated than a unimodal or bimodal distribution. The pLLSs and LLSs probe a similar range of metallicities -3&lt;~[X/H]&lt;~+0.4, but the fraction of very metal-poor absorbers with [X/H]&lt;~-1.4 is much larger for the pLLSs than the LLSs. In contrast, absorbers with logN_HI_&gt;=19 have mostly -1&lt;~[X/H]&lt;~0 at z&lt;~1. The metal-enriched gas probed by pLLSs and LLSs confirms that galaxies that have been enriching their CGM over billions of years. Surprisingly, despite this enrichment, there is also abundant metal-poor CGM gas (41%-59% of the pLLSs have [X/H]&lt;~-1.4), representing a reservoir of near-pristine gas around z&lt;~1 galaxies. We compare our empirical results to recent cosmological zoom simulations, finding some discrepancies, including an overabundance of metal- enriched CGM gas in simulations.</description><source format="bibcode">2019ApJ...872...81W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/872/81</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/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/164/1">J/ApJS/164/1 : IGM absorbers toward HE 0226-4110 (Lehner+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/636/610">J/ApJ/636/610 : Damped Ly{alpha} systems at z&lt;1.65 (Rao+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/168/213">J/ApJS/168/213 : Ionization states and cooling efficiencies (Gnat+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/676/262">J/ApJ/676/262 : PKS1302-102 intergalactic absorption system (Cooksey+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/177/39">J/ApJS/177/39 : Survey of low-redshift OVI absorbers (Tripp+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/700/1299">J/ApJ/700/1299 : Gas-phase element depletions in the ISM (Jenkins, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/193/28">J/ApJS/193/28 : Galaxy survey around 20 UV-bright quasars (Prochaska+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/736/42">J/ApJ/736/42 : HST QSO Catalog (Ribaudo+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/740/91">J/ApJ/740/91 : Ly{alpha} &amp; OVI in galaxies around QSOs (Prochaska+, 2011)</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/770/138">J/ApJ/770/138 : Metallicities of Lyman limit systems and DLA (Lehner+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/765/137">J/ApJ/765/137 : HST survey for Lyman limit systems. 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